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It looks like the 6961 lost the fight and took one in the nose. It's the single unit on a rare daylight move coming up Track 9 approaching the Rock Island main headed to Rockdale, just west of UD Tower and start of Chessie System's New Rock Sub. This is early on in the operation of the old Rock Island and the work was being handled by GP30's and GP35's. The arrival of the GP15T's was still over a year away.

It's a gorgeous day in the city today. There was a buzz in the air the Outdoor Warning System's weekly test sounded the arrival of the lunch hour.

 

I was fortunate enough to have some free time on this trip and got out to walk around and to enjoy the warm sunshine and flow of pedestrian traffic in the Financial District.

 

I've been taking fewer street shots lately as I experiment and play with landscape photography (not terribly well, I admit). Today's lunch hour showed me and reminded me of everything I love about street photography: being out in the world, seeing what's happening for the thousands of people I pass by, identifying something fun, different or pleasing to the eye and capturing it just as the players in my imagined scene are in the correct position, looking the correct direction, on their marks as I envision them.

 

This image might have worked in color, but I was concerned that the reds of the planted flowers and of the Wells Fargo sign and the bright greens of the shrubs would distract the viewer from the people in the shot.

A United Launch Alliance Atlas V rocket with Boeing’s CST-100 Starliner spacecraft aboard launches from Space Launch Complex 41, Thursday, May 19, 2022, at Cape Canaveral Space Force Station in Florida. Boeing’s Orbital Flight Test-2 (OFT-2) is Starliner’s second uncrewed flight test and will dock to the International Space Station as part of NASA's Commercial Crew Program. OFT-2 launched at 6:54 p.m. ET, and will serve as an end-to-end test of the system's capabilities. Photo Credit: (NASA/Joel Kowsky)

When this uniquely beautiful meteorite surfaced in the Sahara last year, I jumped on it, buying the 1,857g stone before the isotope analyses confirmed that it was a meteorite at all. It was an enigmatic mystery, looking unlike any meteorite I had ever seen. Michael Farmer agreed, and when we sliced it in half, we found a treasure trove of green crystals (some 4cm long!) that must have formed in a planetary-sized body with very slow cooling of the crust over 100,000+ years. But which? Given the Earth-like preponderance of silicon dioxide crystals (58% by volume), some speculated that it might be the first meteorite knocked loose from the Earth itself, an emissary from its early formation.

 

MORE INSIDE VIEWS BELOW

 

But we now know it’s older still. It is an ancient survivor from the crust of a lost cousin planet that formed 23 million years before Earth itself! EC 002 was all over the science news this week, with some of the articles featuring photos of my stones. What a beautiful birthday-week surprise! (and here are all of my photos)

 

From New Scientist: 4.6-billion-year-old meteorite is the oldest volcanic rock ever found

 

"The oldest volcanic rock we have ever discovered may help us understand the building blocks of planets. The meteorite, which was discovered in the Sahara desert in 2020, dates from just 2 million years after the formation of the solar system – making it more than a million years older than the previous record-holder.

 

“I have been working on meteorites for more than 20 years now, and this is possibly the most fantastic new meteorite I have ever seen,” says Jean-Alix Barrat at the University of Western Brittany in France. When he and his colleagues analysed the meteorite, called Erg Chech 002 or EC 002, they found that it was unlike any other meteorite we have ever located.

 

It is a type of rock called andesite that, on Earth, is found mostly in subduction zones – areas where tectonic plates have collided and one has been pushed beneath the other – and rarely in meteorites. Most of the meteorites discovered on Earth are made of another kind of volcanic rock called basalt. Analysis of the chemical make-up of the new meteorite showed that it was once molten, and solidified nearly 4.6 billion years ago.

 

This means it was probably part of the crust of an ancient protoplanet that broke up early in the solar system’s past. No known asteroid looks like EC 002, which indicates that almost none of these relics still exist: nearly all of them have either crashed together to form planets or been smashed to bits.

 

“When you go close to the beginning of the solar system, it’s more and more complicated to get samples,” says Barrat. “We probably will not find another sample older than this one.”

 

The researchers’ analysis showed that it took the magma that makes up EC 002 at least 100,000 years to cool and solidify after it melted, which may indicate that it was unusually viscous. Further study of this artefact from the early solar system could help us understand how the planets, including Earth, formed."

 

LiveScience added: 4.6-billion-year-old meteorite belongs to Earth’s long-lost baby cousin

 

"When the scientists peered at distant cosmic objects' spectral "fingerprints" — wavelength patterns in the light they emit or reflect — and compared them to EC 002, they found no matches. Even after comparison with 10,000 objects in the Sloan Digital Sky Survey database, EC 002 was "clearly distinguishable from all asteroid groups," the scientists reported. "No object with spectral characteristics similar to EC 002 has been identified to date."

 

Where are all the protoplanets with andesite crusts today? During our solar system's volatile period of planetary birth, most of these protoplanets likely didn't make it past infancy, according to the study. Either they were smashed to bits in collisions with other rocky bodies, or they were absorbed by bigger and more successful rocky planets, such as Earth, Mars, Venus and Mercury, leaving few traces behind to spawn meteorites such as EC 002.

 

"Remains of primordial andesitic crust are therefore not only rare in the meteorite record, but they are also rare today in the asteroid belt," the scientists wrote."

 

And here is the original paper in the Proceedings of the National Academy of Sciences: A 4,565-My-old andesite from an extinct chondritic protoplanet

A United Launch Alliance Atlas V rocket with Boeing’s CST-100 Starliner spacecraft aboard launches from Space Launch Complex 41, Thursday, May 19, 2022, at Cape Canaveral Space Force Station in Florida. Boeing’s Orbital Flight Test-2 (OFT-2) is Starliner’s second uncrewed flight test and will dock to the International Space Station as part of NASA's Commercial Crew Program. OFT-2 launched at 6:54 p.m. ET, and will serve as an end-to-end test of the system's capabilities. Photo Credit: (NASA/Joel Kowsky)

Overseas from the conflict in Europe, America has been designing its own VCS units to support both its own military and to hopefully sell to the URE. The ALDIS (Armored Long-Distance Infantry Support) is the first system to go into full production. It is designed to support regular tanks and infantry from a distance, and can utilize its legs to reach previously treacherous strategic positions. Each ALDIS system is equipped with a light railgun, and a short-range missile launcher. Although not designed for close combat, the ALDIS has two light machine guns affixed to the underside of its "head." The head does not serve any purpose other than carrying the guns, as it is a residual relic from the system's initial design phase. Most of the ALDIS's sensors are built into the main body, and it uses a back mounted non-combustible high-capacity battery pack for power. Each ALDIS system has one human pilot, but similar to the URE's Hornet, have a basic AI system which puts them into an "overwatch" mode. ALDIS systems have been deployed to great success, and currently have a very low pilot death count.

 

This started out as a Power-Miners inspired humanoid mech, but I didn't like how the legs clashed with the rest of it so I made something new out of them. This was a pretty fun build, I might do more like this in the future.

Available @ Fable5 on 8/8!

 

Taxi: maps.secondlife.com/secondlife/Brewery/45/81/21

 

Particle Texture Appliers are designed to go with ELEMENTAL Magic Aura Systems! Each Particle Applier comes with 12 effects that can be added to the system's effects.

 

Examples of Elemental particle Systems are:

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Boeing’s CST-100 Starliner spacecraft lands at White Sands Missile Range’s Space Harbor, Wednesday, May 25, 2022, in New Mexico. Boeing’s Orbital Flight Test-2 (OFT-2) is Starliner’s second uncrewed flight test to the International Space Station as part of NASA's Commercial Crew Program. OFT-2 serves as an end-to-end test of the system's capabilities. Photo Credit: (NASA/Bill Ingalls)

A United Launch Alliance Atlas V rocket with Boeing’s CST-100 Starliner spacecraft aboard launches from Space Launch Complex 41, Thursday, May 19, 2022, at Cape Canaveral Space Force Station in Florida. Boeing’s Orbital Flight Test-2 (OFT-2) is Starliner’s second uncrewed flight test and will dock to the International Space Station as part of NASA's Commercial Crew Program. OFT-2 launched at 6:54 p.m. ET, and will serve as an end-to-end test of the system's capabilities. Photo Credit: (NASA/Joel Kowsky)

A SpaceX Falcon 9 rocket with the company's Crew Dragon spacecraft onboard is seen as it is rolled out of the horizontal integration facility at Launch Complex 39A as preparations continue for the Demo-1 mission, Feb. 28, 2019 at the Kennedy Space Center in Florida. The Demo-1 mission will be the first launch of a commercially built and operated American spacecraft and space system designed for humans as part of NASA's Commercial Crew Program. The mission, currently targeted for a 2:49am launch on March 2, will serve as an end-to-end test of the system's capabilities. Photo Credit: NASA/Joel Kowsky

NASA image use policy.

A Bradford trolleybus slowly turns at 'Thackley Corner' during an enthusiast’s tour, one of the many tours that took place during the final months of the system’s life. Sometime prior to the end, the City Council had agreed that the last day of trolleybus operation was to be on Sunday 26th March1972, when the trolleys would be seen off in spectacular style.

 

Following the closure of the much smaller Teesside trolleybus system in 1971, Bradford was now the last place in Britain to operate trolleybuses in normal public service, so it was important that all went ahead smoothly, as Bradford’s last trolleybus would also be Britain’s last trolleybus.

 

During January 1972, the National Union of Mineworkers (NUM) went on strike over pay. The NUM's aim was to freeze domestic and industrial coal supplies to force the Coal Board to the negotiating table. At that time, three-quarters of the country’s electricity was generated by coal-burning power stations, not surprisingly coal stocks quickly ran down as a result of the strike action. The situation became so bad that the government declared a state of emergency on the 9th February; many people will remember the power cuts and having to use candles for lighting during evening time outages. From 11th February The Yorkshire Electricity Board introduced selective power cuts to preserve coal stocks. This action forced the decision to withdraw trolleybuses until a normal power supply was resumed, but enthusiasts and council officials feared that the trolleybuses might never return to the City’s streets.

 

On 26th February, the Country breathed a sigh of relief, as the seven-week strike ended; Power supplies began to return to normal allowing Bradford to reinstate its trolleybuses for the last few weeks of operation, during which time, the City was almost besieged by enthusiasts who came to witness their last days.

 

The biggest crowds arrived from Friday 24th March to Sunday 26th March, when many hundreds of people converged on Bradford to say farewell to the trolleybus. Enthusiasts crowded onto every available service trolleybus, some chased ahead of them in cars, waiting on almost every street corner to get their last glimpses and photographs of the remaining trolleybuses at work.

 

As planned, the end came on Sunday 26th March, when civic dignitaries and special guests boarded trolleybus 844 on the last trolleybus journey to Thornton. On 844’s return to Thornbury Depot, the civic party alighted the vehicle and several speeches were made to the crowds, before the Lord Mayor threw the switch, killing the power to the system and ending 60 years of trolleybus operation in Bradford and ending Britain’s trolleybus era.

 

The scene of the photograph as it is today:

maps.google.co.uk/maps?f=q&source=s_q&hl=en&g...

A United Launch Alliance Atlas V rocket with Boeing’s CST-100 Starliner spacecraft onboard is seen as it is rolled out of the Vertical Integration Facility to the launch pad at Space Launch Complex 41 ahead of the Orbital Flight Test-2 (OFT-2) mission, Thursday, July 29, 2021 at Cape Canaveral Space Force Station in Florida. Boeing’s Orbital Flight Test-2 will be Starliner’s second uncrewed flight test and will dock to the International Space Station as part of NASA's Commercial Crew Program. The mission, currently targeted for launch at 2:53 p.m. EDT Friday, July 30, will serve as an end-to-end test of the system's capabilities. Photo Credit: (NASA/Joel Kowsky)

A SpaceX Falcon 9 rocket with the company's Crew Dragon spacecraft onboard is seen illuminated on the launch pad by spotlights at Launch Complex 39A as preparations continue for the Demo-1 mission, Friday, March 1, 2019 at the Kennedy Space Center in Florida. The Demo-1 mission will be the first launch of a commercially built and operated American spacecraft and space system designed for humans as part of NASA's Commercial Crew Program. The mission, currently targeted for a 2:49am launch on March 2, will serve as an end-to-end test of the system's capabilities. Photo Credit: (NASA/Joel Kowsky)

The geothermal areas of Yellowstone include several geyser basins in Yellowstone National Park as well as other geothermal features such as hot springs, mud pots, and fumaroles. The number of thermal features in Yellowstone is estimated at 10,000. A study that was completed in 2011 found that a total of 1,283 geysers have erupted in Yellowstone, 465 of which are active during an average year. These are distributed among nine geyser basins, with a few geysers found in smaller thermal areas throughout the Park. The number of geysers in each geyser basin are as follows: Upper Geyser Basin (410), Midway Geyser Basin (59), Lower Geyser Basin (283), Norris Geyser Basin (193), West Thumb Geyser Basin (84), Gibbon Geyser Basin (24), Lone Star Geyser Basin (21), Shoshone Geyser Basin (107), Heart Lake Geyser Basin (69), other areas (33). Although famous large geysers like Old Faithful are part of the total, most of Yellowstone's geysers are small, erupting to only a foot or two. The hydrothermal system that supplies the geysers with hot water sits within an ancient active caldera. Many of the thermal features in Yellowstone build up sinter, geyserite, or travertine deposits around and within them.

 

The various geyser basins are located where rainwater and snowmelt can percolate into the ground, get indirectly superheated by the underlying Yellowstone hotspot, and then erupt at the surface as geysers, hot springs, and fumaroles. Thus flat-bottomed valleys between ancient lava flows and glacial moraines are where most of the large geothermal areas are located. Smaller geothermal areas can be found where fault lines reach the surface, in places along the circular fracture zone around the caldera, and at the base of slopes that collect excess groundwater. Due to the Yellowstone Plateau's high elevation the average boiling temperature at Yellowstone's geyser basins is 199 °F (93 °C). When properly confined and close to the surface it can periodically release some of the built-up pressure in eruptions of hot water and steam that can reach up to 390 feet (120 m) into the air (see Steamboat Geyser, the world's tallest geyser). Water erupting from Yellowstone's geysers is superheated above that boiling point to an average of 204 °F (95.5 °C) as it leaves the vent. The water cools significantly while airborne and is no longer scalding hot by the time it strikes the ground, nearby boardwalks, or even spectators. Because of the high temperatures of the water in the features it is important that spectators remain on the boardwalks and designated trails. Several deaths have occurred in the park as a result of falls into hot springs.

 

Prehistoric Native American artifacts have been found at Mammoth Hot Springs and other geothermal areas in Yellowstone. Some accounts state that the early people used hot water from the geothermal features for bathing and cooking. In the 19th century Father Pierre-Jean De Smet reported that natives he interviewed thought that geyser eruptions were "the result of combat between the infernal spirits". The Lewis and Clark Expedition traveled north of the Yellowstone area in 1806. Local natives that they came upon seldom dared to enter what we now know is the caldera because of frequent loud noises that sounded like thunder and the belief that the spirits that possessed the area did not like human intrusion into their realm. The first white man known to travel into the caldera and see the geothermal features was John Colter, who had left the Lewis and Clark Expedition. He described what he saw as "hot spring brimstone". Beaver trapper Joseph Meek recounted in 1830 that the steam rising from the various geyser basins reminded him of smoke coming from industrial smokestacks on a cold winter morning in Pittsburgh, Pennsylvania. In the 1850s famed trapper Jim Bridger called it "the place where Hell bubbled up".

 

The heat that drives geothermal activity in the Yellowstone area comes from brine (salty water) that is 1.5–3 miles (7,900–15,800 ft; 2,400–4,800 m) below the surface. This is actually below the solid volcanic rock and sediment that extends to a depth of 3,000 to 6,000 feet (900 to 1,800 m) and is inside the hot but mostly solid part of the pluton that contains Yellowstone's magma chamber. At that depth the brine is superheated to temperatures that exceed 400 °F (204 °C) but is able to remain a liquid because it is under great pressure (like a huge pressure cooker).

 

Convection of the churning brine and conduction from surrounding rock transfers heat to an overlaying layer of fresh groundwater. Movement of the two liquids is facilitated by the highly fractured and porous nature of the rocks under the Yellowstone Plateau. Some silica is dissolved from the fractured rhyolite into the hot water as it travels through the fractured rock. Part of this hard mineral is later redeposited on the walls of the cracks and fissures to make a nearly pressure-tight system. Silica precipitates at the surface to form either geyserite or sinter, creating the massive geyser cones, the scalloped edges of hot springs, and the seemingly barren landscape of geyser basins.

 

There are at least five types of geothermal features found at Yellowstone:

 

Fumaroles: Fumaroles, or steam vents, are the hottest hydrothermal features in the park. They have so little water that it all flashes into steam before reaching the surface. At places like Roaring Mountain, the result is loud hissing of steam and gases.

Geysers: Geysers such as Old Faithful are a type of geothermal feature that periodically erupt scalding hot water. Increased pressure exerted by the enormous weight of the overlying rock and water prevents deeper water from boiling. As the hot water rises it is under less pressure and steam bubbles form. They, in turn, expand on their ascent until the bubbles are too big and numerous to pass freely through constrictions. At a critical point the confined bubbles actually lift the water above, causing the geyser to splash or overflow. This decreases the pressure of the system and violent boiling results. Large quantities of water flash into tremendous amounts of steam that force a jet of water out of the vent: an eruption begins. Water (and heat) is expelled faster than the geyser's recharge rate, gradually decreasing the system's pressure and eventually ending the eruption.

Hot springs: Hot springs such as Grand Prismatic Spring are the most common hydrothermal features in the park. Their plumbing has no constrictions. Superheated water cools as it reaches the surface, sinks, and is replaced by hotter water from below. This circulation, called convection, prevents water from reaching the temperature needed to set off an eruption. Many hot springs give rise to streams of heated water.

Mudpots: Mudpots such as Fountain Paint Pots are acidic hot springs with a limited water supply. Some microorganisms use hydrogen sulfide (rotten egg smell), which rises from deep within the earth, as an energy source. They convert the gas into sulfuric acid, which breaks down rock into clay.

Travertine terraces: Travertine terraces, found at Mammoth Hot Springs, are formed from limestone (a rock type made of calcium carbonate). Thermal waters rise through the limestone, carrying high amounts of dissolved carbonate. Carbon dioxide is released at the surface and calcium carbonate deposited as travertine, the chalky white rock of the terraces. These features constantly and quickly change due to the rapid rate of deposition.

Geyser basins

 

The Norris Geyser Basin 44°43′43″N 110°42′16″W is the hottest geyser basin in the park and is located near the northwest edge of Yellowstone Caldera near Norris Junction and on the intersection of three major faults. The Norris-Mammoth Corridor is a fault that runs from Norris north through Mammoth to the Gardiner, Montana, area. The Hebgen Lake fault runs from northwest of West Yellowstone, Montana, to Norris. This fault experienced an earthquake in 1959 that measured 7.4 on the Richter scale (sources vary on exact magnitude between 7.1 and 7.8; see 1959 Hebgen Lake earthquake). Norris Geyser Basin is so hot and dynamic because these two faults intersect with the ring fracture zone that resulted from the creation of the Yellowstone Caldera of 640,000 years ago.

 

The Basin consists of three main areas: Porcelain Basin, Back Basin, and One Hundred Springs Plain. Unlike most of other geyser basins in the park, the waters from Norris are acidic rather than alkaline (for example, Echinus Geyser has a pH of ~3.5). The difference in pH allows for a different class of bacterial thermophiles to live at Norris, creating different color patterns in and around the Norris Basin waters.

 

The Ragged Hills that lie between Back Basin and One Hundred Springs Plain are thermally altered glacial kames. As glaciers receded the underlying thermal features began to express themselves once again, melting remnants of the ice and causing masses of debris to be dumped. These debris piles were then altered by steam and hot water flowing through them. Madison lies within the eroded stream channels cut through lava flows formed after the caldera eruption. The Gibbon Falls lies on the caldera boundary as does Virginia Cascades.

 

Algae on left bacteria on right at the intersection of flows from the Constant & Whirlgig Geysers at Norris Geyser Basin

The tallest active geyser in the world, Steamboat Geyser,[11] is located in Norris Basin. Unlike the slightly smaller but much more famous Old Faithful Geyser located in Upper Geyser Basin, Steamboat has an erratic and lengthy timetable between major eruptions. During major eruptions, which may be separated by intervals of more than a year (the longest recorded span between major eruptions was 50 years), Steamboat erupts over 300 feet (90 m) into the air. Steamboat does not lie dormant between eruptions, instead displaying minor eruptions of approximately 40 feet (12 m).

 

Norris Geyser Basin periodically undergoes a large-scale, basin-wide thermal disturbance lasting a few weeks. Water levels fluctuate, and temperatures, pH, colors, and eruptive patterns change throughout the basin. During a disturbance in 1985, Porkchop Geyser continually jetted steam and water; in 1989, the same geyser apparently clogged with silica and blew up, throwing rocks more than 200 feet (61 m). In 2003 a park ranger observed it bubbling heavily, the first such activity seen since 1991. Activity increased dramatically in mid-2003. Because of high ground temperatures and new features beside the trail much of Back Basin was closed until October. In 2004 the boardwalk was routed around the dangerous area and now leads behind Porkchop Geyser.

 

North of Norris, Roaring Mountain is a large, acidic hydrothermal area (solfatara) with many fumaroles. In the late 19th and early 20th centuries, the number, size, and power of the fumaroles were much greater than today. The fumaroles are most easily seen in the cooler, low-light conditions of morning and evening.

 

The Gibbon Geyser Basin 44°41′58″N 110°44′34″W includes several thermal areas in the vicinity of the Gibbon River between Gibbon Falls and Norris. The most accessible feature in the basin is Beryl Spring, with a small boardwalk right along the Grand Loop Road. Artists' Paintpots is a small hydrothermal area south of Norris Junction that includes colorful hot springs and two large mudpots.

 

The Monument Geyser Basin 44°41′03″N 110°45′14″W has no active geysers, but its 'monuments' are siliceous sinter deposits similar to the siliceous spires discovered on the floor of Yellowstone Lake. Scientists hypothesize that this basin's structures formed from a hot water system in a glacially dammed lake during the waning stages of the Pinedale Glaciation. The basin is on a ridge reached by a very steep one-mile (1.6 km) trail south of Artists' Paint Pots. Other areas of thermal activity in Gibbon Geyser Basin lie off-trail.

 

South of Norris along the rim of the caldera is the Upper Geyser Basin 44°27′52″N 110°49′45″W, which has the highest concentration of geothermal features in the park. This complement of features includes the most famous geyser in the park, Old Faithful Geyser, as well as four other predictable large geysers. One of these large geysers in the area is Castle Geyser which is about 1,400 feet (430 m) northwest of Old Faithful. Castle Geyser has an interval of approximately 13 hours between major eruptions, but is unpredictable after minor eruptions. The other three predictable geysers are Grand Geyser, Daisy Geyser, and Riverside Geyser. Biscuit Basin and Black Sand Basin are also within the boundaries of Upper Geyser Basin.

 

The hills surrounding Old Faithful and the Upper Geyser Basin are reminders of Quaternary rhyolitic lava flows. These flows, occurring long after the catastrophic eruption of 640,000 years ago, flowed across the landscape like stiff mounds of bread dough due to their high silica content.

 

Evidence of glacial activity is common, and it is one of the keys that allows geysers to exist. Glacier till deposits underlie the geyser basins providing storage areas for the water used in eruptions. Many landforms, such as Porcupine Hills north of Fountain Flats, are made up of glacial gravel and are reminders that 70,000 to 14,000 years ago, this area was buried under ice.

 

Signs of the forces of erosion can be seen everywhere, from runoff channels carved across the sinter in the geyser basins to the drainage created by the Firehole River. Mountain building is evident on the drive south of Old Faithful, toward Craig Pass. Here the Rocky Mountains reach a height of 8,262 feet (2,518 m), dividing the country into two distinct watersheds.

 

Midway Geyser Basin 44°31′04″N 110°49′56″W is much smaller than the other basins found alongside the Firehole River. Despite its small size, it contains two large features, the 200-by-300-foot-wide (60 by 90 m) Excelsior Geyser which pours over 4,000 U.S. gallons (15,000 L; 3,300 imp gal) per minute into the Firehole River. The largest hot spring in Yellowstone, the 370-foot-wide (110 m) and 121-foot-deep (37 m) Grand Prismatic Spring is found here. Also in the basin is Turquoise Pool and Opal Pool.

 

Lower Geyser Basin

Blue spring with steam rising from it; irregular blotches of red and orange residue are on the banks, along with dead tree trunks.

Silex Spring at Fountain Paint Pot

 

Farther north is the Lower Geyser Basin 44°32′58″N 110°50′09″W, which is the largest geyser basin in area, covering approximately 11 square miles. Due to its large size, it has a much less concentrated set of geothermal features, including Fountain Paint Pots. Fountain Paint Pots are mud pots, that is, a hot spring that contains boiling mud instead of water. The mud is produced by a higher acidity in the water which enables the spring to dissolve surrounding minerals to create an opaque, usually grey, mud. Also there is Firehole Spring, Celestine Pool, Leather Pool, Red Spouter, Jelly spring, and a number of fumaroles.

 

Geysers in Lower Geyser Basin include Great Fountain Geyser, whose eruptions reach 100 to 200 feet (30–61 m) in the air, while waves of water cascade down its sinter terraces., the Fountain group of Geysers (Clepsydra Geyser which erupts nearly continuously to heights of 45 feet (14 m), Fountain Geyser, Jelly Geyser, Jet Geyser, Morning Geyser, and Spasm Geyser), the Pink Cone group of geysers (Dilemma Geyser, Labial Geyser, Narcissus Geyser, Pink Geyser, and Pink Cone Geyser), the White Dome group of geysers (Crack Geyser, Gemini Geyser, Pebble Geyser, Rejuvenated Geyser, and White Dome Geyser), as well as Sizzler Geyser.

 

Clepsydra Geyser erupting. July 2019

Fountain Paint Pots

White Dome Geyser

West Thumb Geyser Basin

Several pools of blue water in ashen rock basin.

West Thumb Geyser Basin

Blackened basin with orange streaks; steam is rising from it with fir trees in the background.

Overflow areas of Silex springs

 

The West Thumb Geyser Basin 44°25′07″N 110°34′23″W, including Potts Basin to the north, is the largest geyser basin on the shores of Yellowstone Lake. The heat source of the thermal features in this location is thought to be relatively close to the surface, only 10,000 feet (3,000 m) down. West Thumb is about the same size as another famous volcanic caldera, Crater Lake in Oregon, but much smaller than the great Yellowstone Caldera which last erupted about 640,000 years ago. West Thumb is a caldera within a caldera.

 

West Thumb was created approximately 162,000 years ago when a magma chamber bulged up under the surface of the earth and subsequently cracked it along ring fracture zones. This in turn released the enclosed magma as lava and caused the surface above the emptied magma chamber to collapse. Water later filled the collapsed area of the caldera, forming an extension of Yellowstone Lake. This created the source of heat and water that feed the West Thumb Geyser Basin today.

 

The thermal features at West Thumb are not only found on the lake shore, but extend under the surface of the lake as well. Several underwater hydrothermal features were discovered in the early 1990s and can be seen as slick spots or slight bulges in the summer. During the winter, the underwater thermal features are visible as melt holes in the icy surface of the lake. The surrounding ice can reach three feet (one yard) in thickness.

 

Perhaps the most famous hydrothermal feature at West Thumb is a geyser on the lake shore known as Fishing Cone. Walter Trumbull of the 1870 Washburn-Langford-Doane Expedition described a unique event while a man was fishing adjacent to the cone: "...in swinging a trout ashore, it accidentally got off the hook and fell into the spring. For a moment it darted about with wonderful rapidity, as if seeking an outlet. Then it came to the top, dead, and literally boiled." Fishing Cone erupted frequently to the height of 40 feet (12 m) in 1919 and to lesser heights in 1939. One fisherman was badly burned in Fishing Cone in 1921. Fishing at the geyser is now prohibited.

 

Early visitors would arrive at West Thumb via stagecoach from the Old Faithful area. They had a choice of continuing on the stagecoach or boarding the steamship Zillah to continue the journey by water to Lake Hotel. The boat dock was located near the south end of the geyser basin near Lakeside Spring.

 

Backcountry Geyser Basins

The Heart Lake 44°18′00″N 110°30′56″W, Lone Star 44°24′50″N 110°49′04″W, and Shoshone Geyser Basins 44°21′16″N 110°47′57″W are located away from the road and require at least several miles of hiking to reach. These areas lack the boardwalks and other safety features of the developed areas. As falling into geothermal features can be fatal, it is usually advisable to visit these areas with an experienced guide or at the very least, travelers need to ensure they remain on well-marked trails.

 

The Heart Lake Geyser Basin contains several groups of geysers and deep blue hot springs near Heart Lake in the south-central portion of Yellowstone, southeast of most of the main geyser basins. Lying in the Snake River watershed east of Lewis Lake and south of Yellowstone Lake, Heart Lake was named sometime before 1871 for Hart Hunney, a hunter. Other explorers in the region incorrectly assumed that the lake's name was spelled 'heart' because of its shape. The Heart Lake Geyser Basin begins a couple miles from the lake and descends along Witch Creek to the lakeshore. Five groups of hydrothermal features comprise the basin, and all of them contain geysers, although some are dormant.

 

Between Shoshone Lake and Old Faithful is the Lone Star Geyser Basin, of which the primary feature is Lone Star Geyser, named for its isolation from the nearby geysers of the Upper Geyser Basin. The basin is reachable on foot or bicycle via a 3 mile road that is closed to vehicles.

 

The Shoshone Geyser Basin, reached by hiking or by boat, contains one of the highest concentrations of geysers in the world – more than 80 in an area 1,600 by 800 feet (490 by 240 m). Hot springs and mudpots dot the landscape between the geyser basin and Shoshone Lake.

 

Hot Spring Basin is located 15 miles (24 km) north-northeast of Fishing Bridge and has one of Yellowstone's largest collections of hot springs and fumaroles. The geothermal features there release large amounts of sulfur. This makes water from the springs so acidic that it has dissolved holes in the pants of people who sit on wet ground and causes mounds of sulfur three feet (1 m) high to develop around fumaroles. The very hot acidic water and steam have also created voids in the ground that are only covered by a thin crust.

 

Mammoth Hot Springs is a large complex of hot springs on a hill of travertine in Yellowstone National Park adjacent to Fort Yellowstone and the Mammoth Hot Springs Historic District. It was created over thousands of years as hot water from the spring cooled and deposited calcium carbonate (over two tons flow into Mammoth each day in a solution). Because of the huge amount of geothermal vents, travertine flourishes. Although these springs lie outside the caldera boundary, their energy has been attributed to the same magmatic system that fuels other Yellowstone geothermal areas.

 

The thermal features at Mud Volcano and Sulphur Caldron are primarily mud pots and fumaroles because the area is situated on a perched water system with little water available. Fumaroles or "steam vents" occur when the ground water boils away faster than it can be recharged. Also, the vapors are rich in sulfuric acid that leaches the rock, breaking it down into clay. Because no water washes away the acid or leached rock, it remains as sticky clay to form a mud pot. Hydrogen sulfide gas is present deep in the earth at Mud Volcano and is oxidized to sulfuric acid by microbial activity, which dissolves the surface soils to create pools and cones of clay and mud. Along with hydrogen sulfide, steam, carbon dioxide, and other gases explode through the layers of mud.

 

A series of shallow earthquakes associated with the volcanic activity in Yellowstone struck this area in 1978. Soil temperatures increased to nearly 200 °F (93 °C). The slope between Sizzling Basin and Mud Geyser, once covered with green grass and trees, became a barren landscape of fallen trees known as "the cooking hillside".

 

Yellowstone National Park is a national park located in the western United States, largely in the northwest corner of Wyoming and extending into Montana and Idaho. It was established by the 42nd U.S. Congress with the Yellowstone National Park Protection Act and signed into law by President Ulysses S. Grant on March 1, 1872. Yellowstone was the first national park in the U.S. and is also widely held to be the first national park in the world. The park is known for its wildlife and its many geothermal features, especially the Old Faithful geyser, one of its most popular. While it represents many types of biomes, the subalpine forest is the most abundant. It is part of the South Central Rockies forests ecoregion.

 

While Native Americans have lived in the Yellowstone region for at least 11,000 years, aside from visits by mountain men during the early-to-mid-19th century, organized exploration did not begin until the late 1860s. Management and control of the park originally fell under the jurisdiction of the U.S. Department of the Interior, the first Secretary of the Interior to supervise the park being Columbus Delano. However, the U.S. Army was eventually commissioned to oversee the management of Yellowstone for 30 years between 1886 and 1916. In 1917, the administration of the park was transferred to the National Park Service, which had been created the previous year. Hundreds of structures have been built and are protected for their architectural and historical significance, and researchers have examined more than a thousand archaeological sites.

 

Yellowstone National Park spans an area of 3,468.4 sq mi (8,983 km2), comprising lakes, canyons, rivers, and mountain ranges. Yellowstone Lake is one of the largest high-elevation lakes in North America and is centered over the Yellowstone Caldera, the largest super volcano on the continent. The caldera is considered a dormant volcano. It has erupted with tremendous force several times in the last two million years. Well over half of the world's geysers and hydrothermal features are in Yellowstone, fueled by this ongoing volcanism. Lava flows and rocks from volcanic eruptions cover most of the land area of Yellowstone. The park is the centerpiece of the Greater Yellowstone Ecosystem, the largest remaining nearly intact ecosystem in the Earth's northern temperate zone. In 1978, Yellowstone was named a UNESCO World Heritage Site.

 

Hundreds of species of mammals, birds, fish, reptiles, and amphibians have been documented, including several that are either endangered or threatened. The vast forests and grasslands also include unique species of plants. Yellowstone Park is the largest and most famous megafauna location in the contiguous United States. Grizzly bears, cougars, wolves, and free-ranging herds of bison and elk live in this park. The Yellowstone Park bison herd is the oldest and largest public bison herd in the United States. Forest fires occur in the park each year; in the large forest fires of 1988, nearly one-third of the park was burnt. Yellowstone has numerous recreational opportunities, including hiking, camping, boating, fishing, and sightseeing. Paved roads provide close access to the major geothermal areas as well as some of the lakes and waterfalls. During the winter, visitors often access the park by way of guided tours that use either snow coaches or snowmobiles.

 

Teton County is a county in the U.S. state of Wyoming. As of the 2020 United States Census, the population was 23,331. Its county seat is Jackson. Its west boundary line is also the Wyoming state boundary shared with Idaho and the southern tip of Montana. Teton County is part of the Jackson, WY-ID Micropolitan Statistical Area.

 

Teton County contains the Jackson Hole ski area, all of Grand Teton National Park, and 40.4% of Yellowstone National Park's total area, including over 96.6% of its water area (largely in Yellowstone Lake).

 

Wyoming is a state in the Mountain West subregion of the Western United States. It borders Montana to the north and northwest, South Dakota and Nebraska to the east, Idaho to the west, Utah to the southwest, and Colorado to the south. With a population of 576,851 in 2020, Wyoming is the least populous state despite being the 10th largest by area, with the second-lowest population density after Alaska. The state capital and most populous city is Cheyenne, which had an estimated population of 63,957 in 2018.

 

Wyoming's western half consists mostly of the ranges and rangelands of the Rocky Mountains; its eastern half consists of high-elevation prairie, and is referred to as the High Plains. Wyoming's climate is semi-arid in some parts and continental in others, making it drier and windier overall than other states, with greater temperature extremes. The federal government owns just under half of Wyoming's land, generally protecting it for public uses. The state ranks sixth in the amount of land—-and fifth in the proportion of its land—-that is owned by the federal government. Its federal lands include two national parks (Grand Teton and Yellowstone), two national recreation areas, two national monuments, and several national forests, as well as historic sites, fish hatcheries, and wildlife refuges.

 

Indigenous peoples inhabited the region for thousands of years. Historic and currently federally recognized tribes include the Arapaho, Crow, Lakota, and Shoshone. Part of the land that is now Wyoming came under American sovereignty via the Louisiana Purchase, part via the Oregon Treaty, and, lastly, via the Mexican Cession. With the opening of the Oregon Trail, the Mormon Trail, and the California Trail, vast numbers of pioneers travelled through parts of the state that had once been traversed mainly by fur trappers, and this spurred the establishment of forts, such as Fort Laramie, that today serve as population centers. The Transcontinental Railroad supplanted the wagon trails in 1867 with a route through southern Wyoming, bringing new settlers and the establishment of founding towns, including the state capital of Cheyenne. On March 27, 1890, Wyoming became the union's 44th state.

 

Farming and ranching, and the attendant range wars, feature prominently in the state's history. Today, Wyoming's economy is largely based on tourism and the extraction of minerals such as coal, natural gas, oil, and trona. Its agricultural commodities include barley, hay, livestock, sugar beets, wheat, and wool.

 

Wyoming was the first state to allow women the right to vote (not counting New Jersey, which had allowed it until 1807), and the right to assume elected office, as well as the first state to elect a female governor. In honor of this part of its history, its most common nickname is "The Equality State" and its official state motto is "Equal Rights". It is among the least religious states in the country, and is known for having a political culture that leans towards libertarian conservatism. The Republican presidential nominee has carried the state in every election since 1968.

At the height of Lothian's craze for branding buses it was possible to regularly see branded buses on routes they ought not to have been on. Whilst the concept of branding generally helped the passenger, it hindered them when their branded bus wasn't quite what it seemed !

 

The colours for service 26 were an attractive red gold and white, gold had been prominent in Edinburgh's colour schemes since 1922 so it was particularly welcome to see it continued on these buses.

 

Here at Tranent in 2007, Trident 690 suitably dressed for the 26 appears on service 15, which to further confuse the passenger had run for some years in a rather rusty red branding thought to resemble the Mactours livery and dubbed 'macred' by drivers. Service 15, which derives from old tram route 15, was at one time one of the system's busiest, running 7 days from 5am till midnight. However attempts to change it over the years, in particular recent changes to 'express' running have succeeded only in losing custom to the extent it now runs just half hourly and not at all on Sundays.

Boeing and NASA teams work around Boeing’s CST-100 Starliner spacecraft after it landed at White Sands Missile Range’s Space Harbor, Wednesday, May 25, 2022, in New Mexico. Boeing’s Orbital Flight Test-2 (OFT-2) is Starliner’s second uncrewed flight test to the International Space Station as part of NASA's Commercial Crew Program. OFT-2 serves as an end-to-end test of the system's capabilities. Photo Credit: (NASA/Bill Ingalls)

With the decline of the Greco-Roman Federation and the decreasing need for large quantities of VCS, the URE commissioned a new design, based around the Grouse II, that would be able to hold their own against multiple enemy VCS. Thus, the Grouse III (commonly known as the "Crusader") was born.

 

The Grouse III shares almost no physical elements with its predecessor, except for some parts of its inner structural design. It is a much heavier VCS, due mostly in part to its thicker armor and considerably more extensive array of equipment. In addition, the Grouse III has a much more comfortable and complex cockpit, alloying the pilot greater control over the system.

 

The Grouse III's primary weapon is a elite-issue 09R-Gunbow, a weapon that can convert between a machine gun (higher firing rate) and an energy crossbow (more accuracy). It also carries a hefty vibrotech sword, and a carbon-based shield. The shield can fire multiple small rockets. In addition, there are to small machine guns in the cranial unit, and a small semi-automated turret on the system's left shoulder. Two small rockets can be fired from each shoulder as well.

 

Here's the inevitable follow-up to the Grouse II. I started with the cockpit, since I wanted it to be as detailed a possible. The original design for it was even larger than the current one, which is already too bulky. Because of the bulk, I opted for a more medieval knight-inspired mech, an idea which suited it quite well.

A United Launch Alliance Atlas V rocket with Boeing’s CST-100 Starliner spacecraft onboard is seen as it is rolled out of the Vertical Integration Facility to the launch pad at Space Launch Complex 41 ahead of the Orbital Flight Test-2 (OFT-2) mission, Thursday, July 29, 2021 at Cape Canaveral Space Force Station in Florida. Boeing’s Orbital Flight Test-2 will be Starliner’s second uncrewed flight test and will dock to the International Space Station as part of NASA's Commercial Crew Program. The mission, currently targeted for launch at 2:53 p.m. EDT on Friday, July 30, will serve as an end-to-end test of the system's capabilities. Photo Credit: (NASA/Aubrey Gemignani)

The Faeth site just went live, and the scientific founders' groundbreaking work was just featured in Science:

"Special diets might boost the power of drugs to vanquish cancers

 

"Scientists including Vousden, who cofounded a company with Cantley to test diet-drug combinations in cancer trials, are unraveling the molecular pathways by which slashing calories or removing a dietary component can bolster the effects of drugs. In mice with cancer, “the effects are oftentimes on the same order of magnitude as those from the drugs that we give patients. That’s a powerful thing to think about"

 

In one trial, participants will shop for and prepare meals according to instructions. In the other, the company Faeth Therapeutics that Cantley co-founded will ship meals to patients to help them stay on track.

 

If those trials show the ketogenic diet helps curb tumor growth for a year or two longer than the PI3K inhibitor otherwise would, the diet “could become the standard of care,” Cantley says. “That will be what physicians will tell patients to do.”

 

A ketogenic diet may enhance other cancer treatments, too. Immunologist Laurence Zitvogel of the Gustave Roussy Institute in France recently studied mice with skin, kidney, or lung cancers receiving a drug known as a checkpoint inhibitor that helps the immune system’s T cells kill tumors. In animals on a ketogenic diet, the ketone bodies they produced boosted the T cells’ power, her team reported in January. Rabinowitz and collaborators have begun enrollment for a 40-person trial to see whether the diet can enhance the impact on pancreatic cancer of a chemotherapy cocktail.

 

OTHER RESEARCHERS ARE exploring an even more precise dietary limitation: cutting out specific amino acids, best known as the building blocks of proteins but also key to many other metabolic processes. Vousden unexpectedly veered into that line of research while studying a cancer-preventing gene called p53. The protein it encodes can trigger cells that have DNA damage to self-destruct, stopping them from turning cancerous. The gene is mutated in many tumors, allowing unrestrained growth.

 

But in 2005, a U.S. lab reported a surprising finding: The intact p53 protein helps healthy cells survive when glucose is scarce, suggesting p53-mutated cancer cells are especially vulnerable to glucose limitation. Vousden wondered whether the protein also helps cells survive a shortage of other, less explored nutrients, such as amino acids—and whether the mutated p53 in cancer would make the cells less resilient.

 

To find out, her postdoc Oliver Maddocks [and Faeth Head of Research] methodically removed various amino acids from cancer cells’ culture medium. Many types of cancer cells grew more slowly when deprived of two related amino acids, serine and glycine, and deleting p53 ramped up that effect. The scientists then tested the effects of a serine- and glycine-free diet in mice. Maddocks and Vousden reported in 2013 and 2017 that the special diet slowed cancer growth and extended the lives of mice implanted with colon cancer cells lacking p53 as well as in mice engineered to develop lymphoma or colon tumors. Cells need serine or glycine to make a compound that sops up DNA-damaging free radicals, and the deprivation made tumor cells more sensitive to that oxidative stress. Radiation and some chemotherapies kill cells by generating free radicals, so the results suggested the diet could prime tumors for those treatments.

 

Similar findings have emerged for other amino acids. Limiting the essential amino acid methionine appears to amplify the effects of radiation and chemotherapy in mice with colon cancer and sarcomas. And removing asparagine, an amino acid abundant in asparagus, from mouse diets curbed the spread of metastatic breast cancer, suggesting the diet could enhance drug treatments.

 

As with serine, depriving mice of one of those amino acids apparently disrupts metabolic cycles by which cancer cells respond to oxidative stress, synthesize DNA, and turn genes off and on.

 

The company Vousden and Cantley founded, Faeth (Welsh for nutrition), is gearing up to test amino acid–depleted diets in two clinical trials this year. Faeth, also cofounded by Maddocks, will combine chemotherapy with a shake lacking specific amino acids, delivered to participants’ homes alongside other meal components, such as salads. The researchers got support from private investors after failing to win research grants for their idea, says Maddocks, now at the University of Glasgow. “It’s quite out of the box.”

 

Maddocks expects the cancer-diet field will take years to move from “piecemeal forays” to a clear understanding of each diet’s pros and cons. Establishing that a specific diet works well enough to become part of routine clinical care also will take time. But Zitvogel says fighting cancer with diet is no longer a fringe idea. The field is at the start of “a new era where people will really take diet seriously into account,” she says. “The time is ripe.”

A United Launch Alliance Atlas V rocket with Boeing’s CST-100 Starliner spacecraft onboard is seen before being rollout out of the Vertical Integration Facility to the launch pad at Space Launch Complex 41 ahead of the Orbital Flight Test mission, Wednesday, Dec. 18, 2019 at Cape Canaveral Air Force Station in Florida. The Orbital Flight Test with be Starliner’s maiden mission to the International Space Station for NASA's Commercial Crew Program. The mission, currently targeted for a 6:36 a.m. EST launch on Dec. 20, will serve as an end-to-end test of the system's capabilities. Photo Credit: (NASA/Joel Kowsky)

Loch Tummel is a long, narrow loch, seven kilometres (4+1⁄2 miles) northwest of Pitlochry in the council area of Perth and Kinross, Scotland. It is fed and drained by the River Tummel, which flows into the River Tay about 13 km (8 mi) south-east of the Clunie Dam at the loch's eastern end.

 

The loch is traversed by roads to both north and south. Along the northern side the road is numbered as the B8019, and runs from the Pass of Killiecrankie on the A9 in the east to Tummel Bridge at the head of the loch. The road on the southern side is unclassified, and meets the A9 further south, near to Pitlochry.

 

The loch gives its name to the Loch Tummel National Scenic Area (NSA), one of 40 such areas in Scotland, which are defined so as to identify areas of exceptional scenery and to ensure its protection by restricting certain forms of development. The Loch Tummel Lyon NSA covers 9,013 hectares (22,272 acres), all of which lies within Perth and Kinross. The NSA covers the hills surrounding the loch, and extends along the River Tummel to also take in the area surrounding the Pass of Killiecrankie on the River Garry.

 

Loch Tummel is popular with anglers who fish for brown trout and pike. Fishing is managed by the Loch Rannoch Conservation Association, who issue permits and control catches. Loch Tummel Sailing Club is based at Foss on the south west shore of the loch. The loch is also very popular with campers during the spring and summer. The roads on either side of the loch both offer splendid views of the surrounding countryside, especially from the well-known 'Queen's View' from the north shore, which was made famous by Queen Victoria in 1866. This viewpoint offers a magnificent vista over the loch with Schiehallion in the background. It is also claimed that the view was originally named after Queen Isabel, wife of Robert the Bruce, who is said to have hidden in the nearby woods after the Bruce's defeat at the Battle of Methven in 1306.

 

Areas of forestry around Loch Tummel owned by Forestry and Land Scotland (FLS) form part of the Tay Forest Park, a network of FLS forests spread across the Highland parts of Perthshire that are managed to provide walks and amenities for visitors.

 

The River Tummel is a tributary of the River Tay, and Loch Tummel is included as part of the River Tay Special Area of Conservation. The designation notes the river system's importance for salmon, otters, brook lampreys, river lampreys and sea lampreys. Brown trout and pike are also present in the loch.

 

The woods to the north of the loch are home to a number of protected species, including capercaillie, black grouse, red squirrel, pearl-bordered fritillary and juniper.

 

Loch Tummel from the Queen's View in about 1895. Note the lower water level when compared to the modern image.

Loch Tummel became part of the Tummel Hydro-Electric Power Scheme when the Clunie Dam was constructed by Wimpey Construction at its eastern end in 1950, raising the water level by 4.5 m (15 ft). Prior to this the loch, which is now approximately 11 km (7 mi) long and just under 0 km (1 mi) wide was much smaller, being 4.4 km (2+3⁄4 mi) long and 0.8 km (1⁄2 mi) wide.

 

Water from Loch Tummel is diverted to Loch Faskally, running via Clunie power station, which has a vertical head of 53 m (174 ft) and a total generating capacity of 61 MW. There is also a power station at Tummel Bridge at the western end of the loch that takes water from Dunalastair reservoir below Loch Rannoch, and discharges into Loch Tummel: this station has a vertical head of 53 m (174 ft) and a total generating capacity of 34 MW.

 

The northern side of the loch has many archeological sites, including an Iron Age ring fort, abandoned townships, and the remains of Pictish fortified villages. This area also includes the standing stones of Clachan Aoraidh, located at the head of Glen Fincastle in the Allean Forest. Fincastle House, a 17th-century Category A listed building, sits at the eastern end of the strath.

 

The raising of the loch for hydroelectricity led to the drowning of an artificial island of a type known as a crannog lying off Port an Eilean on the northern side of the loch. The island is now 3 m underwater, and was investigated by the Scottish Trust for Underwater Archaeology and Perth & Kinross Heritage Trust in 2004. A well-made flagstone floor and a flight of steps that led down a distance of 2 m to the loch bed were found. Analysis of one of the timbers found on the site revealed that it dated from around 1840.

 

Above the head of the loch, there are two bridges over the River Tummel at Tummel Bridge. The original humpbacked bridge was built by General Wade in about 1734 as part of his construction of some 240 miles (390 km) of roads and 30 bridges in Scotland between 1725 and 1737. A modern replacement alongside Wade's bridge carries the traffic from Aberfeldy on the B846 road. The historic drove road of the Road to the Isles leaves Wade's military road at Tummel Bridge, from where it heads west into Lochaber, and Tummel is one of the places mentioned in the Scottish folk song named after the road.

 

The Highlands is a historical region of Scotland. Culturally, the Highlands and the Lowlands diverged from the Late Middle Ages into the modern period, when Lowland Scots language replaced Scottish Gaelic throughout most of the Lowlands. The term is also used for the area north and west of the Highland Boundary Fault, although the exact boundaries are not clearly defined, particularly to the east. The Great Glen divides the Grampian Mountains to the southeast from the Northwest Highlands. The Scottish Gaelic name of A' Ghàidhealtachd literally means "the place of the Gaels" and traditionally, from a Gaelic-speaking point of view, includes both the Western Isles and the Highlands.

 

The area is very sparsely populated, with many mountain ranges dominating the region, and includes the highest mountain in the British Isles, Ben Nevis. During the 18th and early 19th centuries the population of the Highlands rose to around 300,000, but from c. 1841 and for the next 160 years, the natural increase in population was exceeded by emigration (mostly to Canada, the United States, Australia and New Zealand, and migration to the industrial cities of Scotland and England.) and passim  The area is now one of the most sparsely populated in Europe. At 9.1/km2 (24/sq mi) in 2012, the population density in the Highlands and Islands is less than one seventh of Scotland's as a whole.

 

The Highland Council is the administrative body for much of the Highlands, with its administrative centre at Inverness. However, the Highlands also includes parts of the council areas of Aberdeenshire, Angus, Argyll and Bute, Moray, North Ayrshire, Perth and Kinross, Stirling and West Dunbartonshire.

 

The Scottish Highlands is the only area in the British Isles to have the taiga biome as it features concentrated populations of Scots pine forest: see Caledonian Forest. It is the most mountainous part of the United Kingdom.

 

Between the 15th century and the mid-20th century, the area differed from most of the Lowlands in terms of language. In Scottish Gaelic, the region is known as the Gàidhealtachd, because it was traditionally the Gaelic-speaking part of Scotland, although the language is now largely confined to The Hebrides. The terms are sometimes used interchangeably but have different meanings in their respective languages. Scottish English (in its Highland form) is the predominant language of the area today, though Highland English has been influenced by Gaelic speech to a significant extent. Historically, the "Highland line" distinguished the two Scottish cultures. While the Highland line broadly followed the geography of the Grampians in the south, it continued in the north, cutting off the north-eastern areas, that is Eastern Caithness, Orkney and Shetland, from the more Gaelic Highlands and Hebrides.

 

Historically, the major social unit of the Highlands was the clan. Scottish kings, particularly James VI, saw clans as a challenge to their authority; the Highlands was seen by many as a lawless region. The Scots of the Lowlands viewed the Highlanders as backward and more "Irish". The Highlands were seen as the overspill of Gaelic Ireland. They made this distinction by separating Germanic "Scots" English and the Gaelic by renaming it "Erse" a play on Eire. Following the Union of the Crowns, James VI had the military strength to back up any attempts to impose some control. The result was, in 1609, the Statutes of Iona which started the process of integrating clan leaders into Scottish society. The gradual changes continued into the 19th century, as clan chiefs thought of themselves less as patriarchal leaders of their people and more as commercial landlords. The first effect on the clansmen who were their tenants was the change to rents being payable in money rather than in kind. Later, rents were increased as Highland landowners sought to increase their income. This was followed, mostly in the period 1760–1850, by agricultural improvement that often (particularly in the Western Highlands) involved clearance of the population to make way for large scale sheep farms. Displaced tenants were set up in crofting communities in the process. The crofts were intended not to provide all the needs of their occupiers; they were expected to work in other industries such as kelping and fishing. Crofters came to rely substantially on seasonal migrant work, particularly in the Lowlands. This gave impetus to the learning of English, which was seen by many rural Gaelic speakers to be the essential "language of work".

 

Older historiography attributes the collapse of the clan system to the aftermath of the Jacobite risings. This is now thought less influential by historians. Following the Jacobite rising of 1745 the British government enacted a series of laws to try to suppress the clan system, including bans on the bearing of arms and the wearing of tartan, and limitations on the activities of the Scottish Episcopal Church. Most of this legislation was repealed by the end of the 18th century as the Jacobite threat subsided. There was soon a rehabilitation of Highland culture. Tartan was adopted for Highland regiments in the British Army, which poor Highlanders joined in large numbers in the era of the Revolutionary and Napoleonic Wars (1790–1815). Tartan had largely been abandoned by the ordinary people of the region, but in the 1820s, tartan and the kilt were adopted by members of the social elite, not just in Scotland, but across Europe. The international craze for tartan, and for idealising a romanticised Highlands, was set off by the Ossian cycle, and further popularised by the works of Walter Scott. His "staging" of the visit of King George IV to Scotland in 1822 and the king's wearing of tartan resulted in a massive upsurge in demand for kilts and tartans that could not be met by the Scottish woollen industry. Individual clan tartans were largely designated in this period and they became a major symbol of Scottish identity. This "Highlandism", by which all of Scotland was identified with the culture of the Highlands, was cemented by Queen Victoria's interest in the country, her adoption of Balmoral as a major royal retreat, and her interest in "tartenry".

 

Recurrent famine affected the Highlands for much of its history, with significant instances as late as 1817 in the Eastern Highlands and the early 1850s in the West.  Over the 18th century, the region had developed a trade of black cattle into Lowland markets, and this was balanced by imports of meal into the area. There was a critical reliance on this trade to provide sufficient food, and it is seen as an essential prerequisite for the population growth that started in the 18th century. Most of the Highlands, particularly in the North and West was short of the arable land that was essential for the mixed, run rig based, communal farming that existed before agricultural improvement was introduced into the region.[a] Between the 1760s and the 1830s there was a substantial trade in unlicensed whisky that had been distilled in the Highlands. Lowland distillers (who were not able to avoid the heavy taxation of this product) complained that Highland whisky made up more than half the market. The development of the cattle trade is taken as evidence that the pre-improvement Highlands was not an immutable system, but did exploit the economic opportunities that came its way.  The illicit whisky trade demonstrates the entrepreneurial ability of the peasant classes. 

 

Agricultural improvement reached the Highlands mostly over the period 1760 to 1850. Agricultural advisors, factors, land surveyors and others educated in the thinking of Adam Smith were keen to put into practice the new ideas taught in Scottish universities.  Highland landowners, many of whom were burdened with chronic debts, were generally receptive to the advice they offered and keen to increase the income from their land.  In the East and South the resulting change was similar to that in the Lowlands, with the creation of larger farms with single tenants, enclosure of the old run rig fields, introduction of new crops (such as turnips), land drainage and, as a consequence of all this, eviction, as part of the Highland clearances, of many tenants and cottars. Some of those cleared found employment on the new, larger farms, others moved to the accessible towns of the Lowlands.

 

In the West and North, evicted tenants were usually given tenancies in newly created crofting communities, while their former holdings were converted into large sheep farms. Sheep farmers could pay substantially higher rents than the run rig farmers and were much less prone to falling into arrears. Each croft was limited in size so that the tenants would have to find work elsewhere. The major alternatives were fishing and the kelp industry. Landlords took control of the kelp shores, deducting the wages earned by their tenants from the rent due and retaining the large profits that could be earned at the high prices paid for the processed product during the Napoleonic wars.

 

When the Napoleonic wars finished in 1815, the Highland industries were affected by the return to a peacetime economy. The price of black cattle fell, nearly halving between 1810 and the 1830s. Kelp prices had peaked in 1810, but reduced from £9 a ton in 1823 to £3 13s 4d a ton in 1828. Wool prices were also badly affected.  This worsened the financial problems of debt-encumbered landlords. Then, in 1846, potato blight arrived in the Highlands, wiping out the essential subsistence crop for the overcrowded crofting communities. As the famine struck, the government made clear to landlords that it was their responsibility to provide famine relief for their tenants. The result of the economic downturn had been that a large proportion of Highland estates were sold in the first half of the 19th century. T M Devine points out that in the region most affected by the potato famine, by 1846, 70 per cent of the landowners were new purchasers who had not owned Highland property before 1800. More landlords were obliged to sell due to the cost of famine relief. Those who were protected from the worst of the crisis were those with extensive rental income from sheep farms.  Government loans were made available for drainage works, road building and other improvements and many crofters became temporary migrants – taking work in the Lowlands. When the potato famine ceased in 1856, this established a pattern of more extensive working away from the Highlands.

 

The unequal concentration of land ownership remained an emotional and controversial subject, of enormous importance to the Highland economy, and eventually became a cornerstone of liberal radicalism. The poor crofters were politically powerless, and many of them turned to religion. They embraced the popularly oriented, fervently evangelical Presbyterian revival after 1800. Most joined the breakaway "Free Church" after 1843. This evangelical movement was led by lay preachers who themselves came from the lower strata, and whose preaching was implicitly critical of the established order. The religious change energised the crofters and separated them from the landlords; it helped prepare them for their successful and violent challenge to the landlords in the 1880s through the Highland Land League. Violence erupted, starting on the Isle of Skye, when Highland landlords cleared their lands for sheep and deer parks. It was quietened when the government stepped in, passing the Crofters' Holdings (Scotland) Act, 1886 to reduce rents, guarantee fixity of tenure, and break up large estates to provide crofts for the homeless. This contrasted with the Irish Land War underway at the same time, where the Irish were intensely politicised through roots in Irish nationalism, while political dimensions were limited. In 1885 three Independent Crofter candidates were elected to Parliament, which listened to their pleas. The results included explicit security for the Scottish smallholders in the "crofting counties"; the legal right to bequeath tenancies to descendants; and the creation of a Crofting Commission. The Crofters as a political movement faded away by 1892, and the Liberal Party gained their votes.

 

Today, the Highlands are the largest of Scotland's whisky producing regions; the relevant area runs from Orkney to the Isle of Arran in the south and includes the northern isles and much of Inner and Outer Hebrides, Argyll, Stirlingshire, Arran, as well as sections of Perthshire and Aberdeenshire. (Other sources treat The Islands, except Islay, as a separate whisky producing region.) This massive area has over 30 distilleries, or 47 when the Islands sub-region is included in the count. According to one source, the top five are The Macallan, Glenfiddich, Aberlour, Glenfarclas and Balvenie. While Speyside is geographically within the Highlands, that region is specified as distinct in terms of whisky productions. Speyside single malt whiskies are produced by about 50 distilleries.

 

According to Visit Scotland, Highlands whisky is "fruity, sweet, spicy, malty". Another review states that Northern Highlands single malt is "sweet and full-bodied", the Eastern Highlands and Southern Highlands whiskies tend to be "lighter in texture" while the distilleries in the Western Highlands produce single malts with a "much peatier influence".

 

The Scottish Reformation achieved partial success in the Highlands. Roman Catholicism remained strong in some areas, owing to remote locations and the efforts of Franciscan missionaries from Ireland, who regularly came to celebrate Mass. There remain significant Catholic strongholds within the Highlands and Islands such as Moidart and Morar on the mainland and South Uist and Barra in the southern Outer Hebrides. The remoteness of the region and the lack of a Gaelic-speaking clergy undermined the missionary efforts of the established church. The later 18th century saw somewhat greater success, owing to the efforts of the SSPCK missionaries and to the disruption of traditional society after the Battle of Culloden in 1746. In the 19th century, the evangelical Free Churches, which were more accepting of Gaelic language and culture, grew rapidly, appealing much more strongly than did the established church.

 

For the most part, however, the Highlands are considered predominantly Protestant, belonging to the Church of Scotland. In contrast to the Catholic southern islands, the northern Outer Hebrides islands (Lewis, Harris and North Uist) have an exceptionally high proportion of their population belonging to the Protestant Free Church of Scotland or the Free Presbyterian Church of Scotland. The Outer Hebrides have been described as the last bastion of Calvinism in Britain and the Sabbath remains widely observed. Inverness and the surrounding area has a majority Protestant population, with most locals belonging to either The Kirk or the Free Church of Scotland. The church maintains a noticeable presence within the area, with church attendance notably higher than in other parts of Scotland. Religion continues to play an important role in Highland culture, with Sabbath observance still widely practised, particularly in the Hebrides.

 

In traditional Scottish geography, the Highlands refers to that part of Scotland north-west of the Highland Boundary Fault, which crosses mainland Scotland in a near-straight line from Helensburgh to Stonehaven. However the flat coastal lands that occupy parts of the counties of Nairnshire, Morayshire, Banffshire and Aberdeenshire are often excluded as they do not share the distinctive geographical and cultural features of the rest of the Highlands. The north-east of Caithness, as well as Orkney and Shetland, are also often excluded from the Highlands, although the Hebrides are usually included. The Highland area, as so defined, differed from the Lowlands in language and tradition, having preserved Gaelic speech and customs centuries after the anglicisation of the latter; this led to a growing perception of a divide, with the cultural distinction between Highlander and Lowlander first noted towards the end of the 14th century. In Aberdeenshire, the boundary between the Highlands and the Lowlands is not well defined. There is a stone beside the A93 road near the village of Dinnet on Royal Deeside which states 'You are now in the Highlands', although there are areas of Highland character to the east of this point.

 

A much wider definition of the Highlands is that used by the Scotch whisky industry. Highland single malts are produced at distilleries north of an imaginary line between Dundee and Greenock, thus including all of Aberdeenshire and Angus.

 

Inverness is regarded as the Capital of the Highlands, although less so in the Highland parts of Aberdeenshire, Angus, Perthshire and Stirlingshire which look more to Aberdeen, Dundee, Perth, and Stirling as their commercial centres.

 

The Highland Council area, created as one of the local government regions of Scotland, has been a unitary council area since 1996. The council area excludes a large area of the southern and eastern Highlands, and the Western Isles, but includes Caithness. Highlands is sometimes used, however, as a name for the council area, as in the former Highlands and Islands Fire and Rescue Service. Northern is also used to refer to the area, as in the former Northern Constabulary. These former bodies both covered the Highland council area and the island council areas of Orkney, Shetland and the Western Isles.

 

Much of the Highlands area overlaps the Highlands and Islands area. An electoral region called Highlands and Islands is used in elections to the Scottish Parliament: this area includes Orkney and Shetland, as well as the Highland Council local government area, the Western Isles and most of the Argyll and Bute and Moray local government areas. Highlands and Islands has, however, different meanings in different contexts. It means Highland (the local government area), Orkney, Shetland, and the Western Isles in Highlands and Islands Fire and Rescue Service. Northern, as in Northern Constabulary, refers to the same area as that covered by the fire and rescue service.

 

There have been trackways from the Lowlands to the Highlands since prehistoric times. Many traverse the Mounth, a spur of mountainous land that extends from the higher inland range to the North Sea slightly north of Stonehaven. The most well-known and historically important trackways are the Causey Mounth, Elsick Mounth, Cryne Corse Mounth and Cairnamounth.

 

Although most of the Highlands is geographically on the British mainland, it is somewhat less accessible than the rest of Britain; thus most UK couriers categorise it separately, alongside Northern Ireland, the Isle of Man, and other offshore islands. They thus charge additional fees for delivery to the Highlands, or exclude the area entirely. While the physical remoteness from the largest population centres inevitably leads to higher transit cost, there is confusion and consternation over the scale of the fees charged and the effectiveness of their communication, and the use of the word Mainland in their justification. Since the charges are often based on postcode areas, many far less remote areas, including some which are traditionally considered part of the lowlands, are also subject to these charges. Royal Mail is the only delivery network bound by a Universal Service Obligation to charge a uniform tariff across the UK. This, however, applies only to mail items and not larger packages which are dealt with by its Parcelforce division.

 

The Highlands lie to the north and west of the Highland Boundary Fault, which runs from Arran to Stonehaven. This part of Scotland is largely composed of ancient rocks from the Cambrian and Precambrian periods which were uplifted during the later Caledonian Orogeny. Smaller formations of Lewisian gneiss in the northwest are up to 3 billion years old. The overlying rocks of the Torridon Sandstone form mountains in the Torridon Hills such as Liathach and Beinn Eighe in Wester Ross.

 

These foundations are interspersed with many igneous intrusions of a more recent age, the remnants of which have formed mountain massifs such as the Cairngorms and the Cuillin of Skye. A significant exception to the above are the fossil-bearing beds of Old Red Sandstone found principally along the Moray Firth coast and partially down the Highland Boundary Fault. The Jurassic beds found in isolated locations on Skye and Applecross reflect the complex underlying geology. They are the original source of much North Sea oil. The Great Glen is formed along a transform fault which divides the Grampian Mountains to the southeast from the Northwest Highlands.

 

The entire region was covered by ice sheets during the Pleistocene ice ages, save perhaps for a few nunataks. The complex geomorphology includes incised valleys and lochs carved by the action of mountain streams and ice, and a topography of irregularly distributed mountains whose summits have similar heights above sea-level, but whose bases depend upon the amount of denudation to which the plateau has been subjected in various places.

Climate

 

The region is much warmer than other areas at similar latitudes (such as Kamchatka in Russia, or Labrador in Canada) because of the Gulf Stream making it cool, damp and temperate. The Köppen climate classification is "Cfb" at low altitudes, then becoming "Cfc", "Dfc" and "ET" at higher altitudes.

 

Places of interest

An Teallach

Aonach Mòr (Nevis Range ski centre)

Arrochar Alps

Balmoral Castle

Balquhidder

Battlefield of Culloden

Beinn Alligin

Beinn Eighe

Ben Cruachan hydro-electric power station

Ben Lomond

Ben Macdui (second highest mountain in Scotland and UK)

Ben Nevis (highest mountain in Scotland and UK)

Cairngorms National Park

Cairngorm Ski centre near Aviemore

Cairngorm Mountains

Caledonian Canal

Cape Wrath

Carrick Castle

Castle Stalker

Castle Tioram

Chanonry Point

Conic Hill

Culloden Moor

Dunadd

Duart Castle

Durness

Eilean Donan

Fingal's Cave (Staffa)

Fort George

Glen Coe

Glen Etive

Glen Kinglas

Glen Lyon

Glen Orchy

Glenshee Ski Centre

Glen Shiel

Glen Spean

Glenfinnan (and its railway station and viaduct)

Grampian Mountains

Hebrides

Highland Folk Museum – The first open-air museum in the UK.

Highland Wildlife Park

Inveraray Castle

Inveraray Jail

Inverness Castle

Inverewe Garden

Iona Abbey

Isle of Staffa

Kilchurn Castle

Kilmartin Glen

Liathach

Lecht Ski Centre

Loch Alsh

Loch Ard

Loch Awe

Loch Assynt

Loch Earn

Loch Etive

Loch Fyne

Loch Goil

Loch Katrine

Loch Leven

Loch Linnhe

Loch Lochy

Loch Lomond

Loch Lomond and the Trossachs National Park

Loch Lubnaig

Loch Maree

Loch Morar

Loch Morlich

Loch Ness

Loch Nevis

Loch Rannoch

Loch Tay

Lochranza

Luss

Meall a' Bhuiridh (Glencoe Ski Centre)

Scottish Sea Life Sanctuary at Loch Creran

Rannoch Moor

Red Cuillin

Rest and Be Thankful stretch of A83

River Carron, Wester Ross

River Spey

River Tay

Ross and Cromarty

Smoo Cave

Stob Coire a' Chàirn

Stac Polly

Strathspey Railway

Sutherland

Tor Castle

Torridon Hills

Urquhart Castle

West Highland Line (scenic railway)

West Highland Way (Long-distance footpath)

Wester Ross

Boeing and NASA teams work around Boeing’s CST-100 Starliner spacecraft after it landed at White Sands Missile Range’s Space Harbor, Wednesday, May 25, 2022, in New Mexico. Boeing’s Orbital Flight Test-2 (OFT-2) is Starliner’s second uncrewed flight test to the International Space Station as part of NASA's Commercial Crew Program. OFT-2 serves as an end-to-end test of the system's capabilities. Photo Credit: (NASA/Bill Ingalls)

Thank you for 9.2 million views, and 17,500+ faves since 2017

 

The above image is a scan from an original Kodachrome™ slide. The default size is 2000 x 1250 pixels, so clicking on the photo will enlarge it for better viewing.

 

The original image comes from my slide collection, amassed over the past 40+ years. They are a combination of my own photographs and ones acquired through trades or purchases.

 

I created this Photostream in 2017 for the purpose of holding my slide collection as an archive, as otherwise they would just remain in binders and boxes, not being enjoyed by anyone, myself included.

 

Comments are welcome.

 

Aircraft MSN: 210

 

Type & Series: Grumman Gulfstream 2

 

Registration: HB-IEY

 

Operator: Petrolair Systems S.A.

 

Location (when available): Paris LBG Jul-1979

 

Remarks:

 

My websites:

www.TwinOtterWorld.com

www.TwinOtterWorldNews.com

www.Dash7World.com

www.Dash8World.com

  

Our solar system’s most massive planet, Jupiter, was slipping towards the western horizon when I captured this scene at around 12:30 am on July 14 of this year. There was a stiff breeze blowing across the top of this man-made pond, causing the water to be anything but smooth, and so diffusing the reflection of Jupiter’s light. That light had travelled across close to 737 million km (458 million mi) of space to reach the pond’s shimmering surface before bouncing the few metres up to my camera.

 

As well as being the most massive planet, Jupiter holds a few other records. At the time of writing, Jupiter is known to have 79 moons orbiting it. The magnetic field of this “gas giant” planet is the strongest of any of the Sun's satellites, at about 14 times that of the Earth’s. A day on Jupiter (the time it takes to rotate once on its axis) is only 10 hours long, and this high rotational speed causes Jupiter to bulge slightly at its equator.

 

Dwarfing Jupiter in size, magnetic field, brightness and every other aspect is the central band and galactic core of our Milky Way galaxy, owning the top 1/3 of my photo. The sky was exceptionally clear and dark on this night, enabling me to capture lots of fine details in the wisps and filigrees of the Milky Way’s “dust lanes”. Mars was part of the show, too, up at the top of the photo.

 

This photo is a cropped version of a much taller image created from nine overlapping frames. I shot each of those individual photos with a Canon EOS 6D camera, a Rokinon 24mm f/1.4 lens @ f/2.4, exposed for 15 seconds @ ISO 6400. I used a Nodal Ninja 3 panoramic head, tipped on its side, to take the nine photos with enough overlap between them to create a smoothly stitched vertical panorama.

Quiapo district is a primary city square of Manila. It derives its name from the water cabbage (Pistia stratiotes), which is named Quiapo or Kiapo in the Tagalog language. Referred to as the "Old Downtown of Manila", Quiapo is home to the Quiapo Church, where the feast of the Black Nazarene is held with millions of people attending annually. Quiapo has also made a name for itself as a place for marketplace bargain hunting.

Plaza Miranda, in the heart of the Quiapo district, is a town square named after Jose Sandino y Miranda, who served as secretary of the treasury of the Philippines from 1853 to 1863. It is located in front of the Quiapo Church, and has become a popular site of political rallies. On August 21, 1971, while the Liberal Party held their Miting de Avance in the plaza, a bomb exploded, killing nine and injuring almost 100 civilians.

The Quiapo district is also home to a sizable Muslim population in Manila. The Golden Mosque and Green Mosque are located there.

A veritable army of fortune tellers and stores offering herbal products surround the Quiapo church. Ongoing sales of pirated media[3][4] and thievery are prevalent in the district.

Since the American insular government and commonwealth periods through to the late 1970s, Quiapo shared its status as the center of the activities of Manila's social elites as well as trade, fashion, art and higher learning with its surrounding vicinities (Avenida Rizal, Binondo, Santa Cruz, Escolta and the Manila University Belt). However, with the construction of the Manila Light Rail Transit System's Yellow Line spanning over Rizal Avenue, the occlusion of light, the trapping of smog and vehicle emissions left the streets beneath dark, gloomy and with an increase in crime and transients. Consequently, many long-time establishments vacated the area. Following the People Power Revolution in 1986, the vibrancy of Quiapo further diminished, with the void filled by makeshift markets to accommodate visitors to the Quiapo Church.

IQuiapo is geographically located at the very center of the city of Manila. It is bounded by Estero de San Miguel to the South, San Miguel to the east, Recto Avenue to the north and Quezon Boulevard to the west.

  

source: wikipedia

This 2.7kg meteorite is an individual stone found in 2011 in the desert of Oman (find photo below in comments). And so, it has its own MetBull entry, and has been characterized by Berlin’s Museum für Naturkunde as an H6 chondrite.

 

As a member the iron-rich H-group, it is a deep reddish brown, and homogenous in color from a near-melting heating event that blended the early chondrules of our solar system’s formation.

Edited Hubble Space Telescope image of the group of three galaxies known by NGC 7764A. Color/processing variant.

 

Original caption: The subject of this image is a group of three galaxies, collectively known as NGC 7764A. They were imaged by the NASA/ESA Hubble Space Telescope, using both its Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3). The two galaxies in the upper right of the image appear to be interacting with one another — indeed, the long trails of stars and gas extending from them both give the impression that they have both just been struck at great speed, thrown into disarray by the bowling-ball-shaped galaxy to the lower left of the image. In reality, however, interactions between galaxies happen over very long time periods, and galaxies rarely collide head-on with one another. It is also unclear whether the galaxy to the lower left is actually interacting with the other two, although they are so relatively close in space that it seems possible that they are. By happy coincidence, the collective interaction between these galaxies have caused the two on the upper right to form a shape, which from our Solar System's perspective, ressembles the starship known as the USS Enterprise from Star Trek! NGC 7764A, which lies about 425 million light years from Earth in the constellation Phoenix, is a fascinating example of just how awkward astronomical nomenclature can be. The three galaxies are individually referred to as NGC 7764A1, NGC 7764A2 and NGC 7764A3, and just to be really difficult, an entirely separate galaxy, named NGC 7764, sits in the skies about a Moon’s distance (as seen from Earth) away. This rather haphazard naming makes more sense when we consider that many of the catalogues for keeping track of celestial bodies were compiled well over 100 years ago, long before modern technology made standardising scientific terminology much easier. As it is, many astronomical objects have several different names, or might have names that are so similar to other objects’ names that they cause confusion.

Central hall of metro station Baltiyskaya on the Kirovsko-Vyborgskaya Line (Line 1), Ploshchad' Baltiyskogo Vokzala, Saint Petersburg, Russia

 

Some background information:

 

The Saint Petersburg Metro is the underground railway system of the city of Saint Petersburg. It has been open since 15th November 1955. Formerly known as the V.I. Lenin Order of Lenin Leningrad Metropoliten, the system exhibits many typical Soviet designs and features exquisite decorations and artwork making it one of the most attractive and elegant metros in the world, maybe only excelled by the Moscow Metro. Due to the city's unique geology, the Saint Petersburg Metro is also one of the deepest metro systems in the world and the deepest by the average depth of all the stations. The system's deepest station, Admiralteyskaya, is located 86 metres below ground. Serving 2.1 million passengers daily (resp. 763.1 million passengers per year), the Saint Petersburg Metro is the 19th busiest metro system in the world.

 

Baltiyskaya is a station on the Kirovsko-Vyborgskaya Line of the Saint Petersburg Metro, located between Narvskaya and Tekhnologichesky Institut, close to the Balitc station. Baltiyskaya is an underground bore-tunnel tri-span station with one exit and middle tunnel of full length. It is situated 57 metres (187 feet) under surface level. The exit feeds into Baltiysky Rail Terminal building. A second exit, which will lead from the opposite side of the underground platform, is also planned. For the decoration of the station Ural marble was used, representing the silver colour of the sea. Baltiyskaya station was opened on 15th November 1955 as the first part of Saint Petersburg's metro system. The project name for the station had been Baltiyskiy Vokzal.

 

In Saint Petersburg’s history, the question of building an underground transport system arose several times, the first time in 1820, when the idea was hatched to build an underground road in a tunnel. By the end of the 19th century, certain interested parties began discussing the possibility of opening the Russian Empire's first metropolitan railway system. Almost all pre-revolutionary designs featured the concept of an elevated metro system, similar to the Paris or Vienna metros. However, as was later discovered through the experience of operating open (ground-level) metro lines in the city, such schemes would likely have resulted in a poor metro service. Unfortunately, at the time, Russian engineers did not have sufficient expertise or technical resources for the construction of deep underground tunnels through the bedrock located far beneath St Petersburg. Hence, it was finally Moscow that got the first underground railway system in the Soviet Union in 1935.

 

In 1938 the question of building a metro for Saint Petersburg (by then renamed to Leningrad), resurfaced again. The initial project was designed by the Moscow institute 'Metrogiprotrans', but on 21st January 1941, "Construction Directorate № 5 of the People's Commissariat" was founded as a body to specifically oversee the design and construction of the Leningrad Metro. By April 1941, 34 shafts for the initial phase of construction had been finished. During the Second World War construction works were frozen due to severe lack of available funding, manpower and equipment. At this time, many of the metro construction workers were employed in the construction and repair of railheads and other objects vital to the besieged city.

 

In 1946 Lenmetroproyekt was created, to finish the construction of the metro first phase. A new version of the metro project, devised by specialists, identified two new solutions to the problems to be encountered during the metro construction. Firstly, stations were to be built at a level slightly raised above that of normal track so as to prevent drainage directly into them, whilst the average tunnel width was to be reduced from the 6 metres (20 feet) standard of the Moscow Metro to 5.5 metres (18 feet).

 

On 3rd September 1947, construction in the Leningrad subway began again and eight years later, on 7 October 1955, the electricity was turned on in the metro l. On 15th November 1955, the subway grand opening was held, with the first seven stations being put into public use. These stations later became part of the Kirovsko-Vyborgskaya Line, connecting the Moscow Rail Terminal in the city centre with the Kirovsky industrial zone in the southwest. Subsequent development included lines under the Neva River in 1958, and the construction of the Vyborgsky Radius in the mid-1970s to reach the new housing developments in the north. In 1978, the line was extended past the city limits into the Leningrad Oblast.

 

By the time of the USSR's collapse, the Leningrad Metro comprised 54 stations and 94.2 kilometres (58.5 miles) of track. But development even continued in the modern, post-Soviet period. Today, the Saint Petersburg metro comprises five lines with altogether 69 stations and 118,6 kilometres (74 miles) of track. However, the present state is not meant to be the end of the story. Plans have been made to extend the Saint Petersburg Metro to nine lines with altogether 126 stations and 190 kilometres (118 miles) of track. But delays due to the difficult geology of the city's underground and to the insufficient funding have cut down these plans to 17 new stations and one new depot until 2025. At the same time, there are several short and mid-term projects on station upgrades, including escalator replacements and lighting upgrades.

 

On 3rd April 2017, a terrorist bombing caused an explosion on a train between Sennaya Ploshchad and Tekhnologicheski Institut stations, on the Line 2. 14 people died and over 50 sustained injuries, while Russian president Vladimir Putin was in the city, when the attack happened. On the same day, Russia's National anti-terrorist unit defused another explosive device at Ploshchad Vosstaniya station (which you can see on this picture).

 

Saint Petersburg (in Russian: Санкт-Петербу́рг) is Russia's second-largest city after Moscow, with currently 5.3 million inhabitants, part of the Saint Petersburg agglomeration with a population of 6.2 million (2015). An important Russian port on the Baltic Sea, it has a status of a federal city. Saint Petersburg is also the fourth-largest city in Europe, only excelled by Istanbul, London and Moscow. Other famous European cities like Paris, Berlin, Rome and Madrid are smaller. Furthermore, Saint Petersburg is the world’s northernmost megapolis and called "The Venice of the North", due to its many channels that traverse the city.

 

Situated on the Neva River, at the head of the Gulf of Finland on the Baltic Sea, it was founded by Tsar Peter the Great on 27th May 1703. On 1st September 1914, the name was changed from Saint Petersburg to Petrograd, on 26 January 1924 to Leningrad, and on 7 September 1991 back to Saint Petersburg. Between 1713 and 1728 and again between 1732 and 1918, Saint Petersburg was the capital of Imperial Russia. In 1918, the central government bodies moved to Moscow, which is located about 625 kilometres (388 miles) to the south-east.

 

Saint Petersburg is also the cultural capital of Russia. Today, the city is inscribed on the UNESCO World Heritage list as an area with 36 historical architectural complexes and around 4000 outstanding individual monuments of architecture, history and culture. It has 221 museums, 2,000 libraries, more than 80 theaters, 100 concert organizations, 45 galleries and exhibition halls, 62 cinemas and around 80 other cultural establishments. Saint Petersburg is home to the Hermitage, one of the largest art museums in the world. Every year the city hosts around 100 festivals and various competitions of art and culture, including more than 50 international ones. In 2017, the city was visited by 7.2 million tourists and it is expected that in the years ahead the number of tourists will still be on the rise.

A United Launch Alliance Atlas V rocket with Boeing’s CST-100 Starliner spacecraft aboard is seen illuminated by spotlights on the launch pad at Space Launch Complex 41 ahead of the Orbital Flight Test-2 mission, Monday, Aug. 2, 2021 at Cape Canaveral Space Force Station in Florida. Boeing’s Orbital Flight Test-2 will be Starliner’s second uncrewed flight test and will dock to the International Space Station as part of NASA's Commercial Crew Program. The mission, currently targeted for launch on 1:20 p.m. EDT Tuesday, Aug. 3, will serve as an end-to-end test of the system's capabilities. Photo Credit: (NASA/Joel Kowsky)

D-197: "Transport TS-70721 this is Harbor Command Tower Delta-One-Nine-Seven, please alter your course. Your current vector will cause a structural collision."

 

D-197: "Transport TS-70721 I repeat, ALTER COURSE IMMEDIATELY!"

 

D-197: "M-Tron Transport TS-70721? Do you copy?"

 

Vahn: "Sorry about that. Guess when I jacked this shuttle the electrical system's a little funny."

 

D-197: "Shuttle TS-70721 we copy. Please alter your course."

 

Vahn: "Want to hear something else funny? Knock, Knock."

 

D-197: "Wh..who/s there?"

 

Vahn: "Justin"

 

D-197: "Justin who?"

 

Vahn: "Looks like I found the canopy release Justin time! HA! HA! HA!"

 

Carter: "Delta-One-Nine-Seven, I'm moving to intercept now!"

London Heathrow Airport Terminal 3 2007-09-22 departures schedules.

 

Many of the flights are listed under the code-sharing flight numbers.

 

All the flights to Canada (Toronto, Calgary, Ottawa, Vancouver, Montreal) are operated by Air Canada but are listed under Scandinavian Airlines System's SK flight numbers at this very moment.

 

The Air New Zealand flight NZ001 is particularly interesting. From London Heathrow to Los Angeles to Auckland, it's one of the very few routes in the world that flies over both the Atlantic and Pacific oceans!

La manevra de rebrusare a vagoanelor trenului EC Praha - Budapest Nyugati - Praha.

 

Reversing on the consist recently arrived from Prague to Budapest, to return back to Czech Republic.

 

Budapest Nyugati,

18.10.2024

Scanned Photo Postcard

Scan is presented for historical/archival purposes

No copyright is claimed or intended

 

From the back of the card:

 

"In the yard of subsidiary Northwestern Pacific at Willits, California, SOUTHERN PACIFIC 4302 is fresh from the system's main shop at Sacramento. Built as number 5430 in May, 1955, the 1750-horsepower Electro-Motive SD9 became the 3908 in the 1965 Espee renumbering, and in 1970 was reworked from the rail up and upgraded to an SD9E with this, its third number.

 

Pacific News photograph"

 

The post card was published by Chatham Publishing Co., Burlingame, CA. No date is given for the postcard.

 

SP SD9E 4302 (ex-SP SD9 3908, nee-SP 5430, to GWR 914)

Seen here as a static exhibit at Valley Heights Locomotive Depot Heritage Museum.

 

One of the system’s most outstanding locomotive classes, it was designed by W. Thow, the newly-appointed Locomotive Engineer in consultation with Beyer Peacock & Company. The firm delivered a batch of 50, which went into service between February, 1892, and July, 1893, and they at once became known as the "Manchester engines". The builders were rather diffident as to their success, as they had no previous experience of locomotives of "such heavy weight"!

 

At the request of the Railway Commissioners, the builders altered the last two of this batch to compounds, these having a single 21 in. (533 mm) high-pressure cylinder on the left-hand side and twin 22 in. (559 mm) low-pressure cylinders, driving a common crosshead, on the right-hand side. They had a von Borries' intercepting valve to permit high pressure steam being fed to all cylinders on starting. It may be noted that this cylinder arrangement for a compound locomotive was one never before or since employed in British locomotive practice.

 

Note: 98 tons (99.6 t) with bogie tender

101 tons 12 cwt (103.2 t) (Baldwin)

 

Recurrent difficulty associated with starting ended the experiment and the two locomotives were converted to two-cylinder simples in 1901 but, due to the unsatisfactory rearrangement of the blast pipe their record was not of the best.

The P(6)-class were the first on the system to be built new with Belpaire fireboxes, and Allan straight-link motion instead of the almost universal Stephenson valve gear. Their neat appearance, when compared with the earlier and comparable O(440)-class, was most marked and a noticeable and rather unusual feature, almost unique among locomotives generally, was the sandbox placed centrally atop the leading driving wheel splashier.

 

These locomotives became one of the most successful and versatile locomotives on the system and their numbers were added to repeatedly over the next 19 years, until their total rose to no less than 191. After the first 50, all others were fitted with a bogie tender when built, and the original batch had bogie tenders fitted later, except for a few, which still retained the six -wheel tender for turning on a 50-feet diameter turntable, at the end of 1965.

Their construction was shared by four builders, distributed as follows:-

 

Beyer Peacock & Company106

Baldwin Locomotive Works.20

Clyde Engineering Company NSW45

Eveleigh Workshop N.S.W.G.R.20

In 1911, No. 937 was obtained from Beyer Peacock with a Schmidt· superheater, as an experiment, having cylinders of 21 in. diameter and 150 lbs. boiler pressure. As a result of experience with this locomotive, the saturated engines were fitted with superheaters of various designs as they came in for re-boilering between 1914 and 1939, the cylinder diameters being increased to 21 inches and inside admission piston valves were substitute for the old, flat D-type.

From 1933, new and stronger frames were fitted, to prevent fractures that had been occurring. The alteration raised the boiler four inches, which actually improved their riding quality. With this alteration and the superheating, the old engines were given a new lease of life. They have been known to attain speeds of up to 73 m.p.h. (117 km/h), in spite of their small driving wheels.

It is interesting to note that the first passenger-type locomotives used on the Trans-Australian line, the G-class, followed the design of the P(6) class, their tenders, however, being of greater capacity.

Info source:

infobluemountains.net.au/locodepot/exhibits-large-3214.shtml

This NASA Hubble Space Telescope image of Comet (C/2012 S1) ISON was photographed on April 10, 2013, when the comet was slightly closer than Jupiter's orbit at a distance of 394 million miles from Earth.

 

Even at that great distance the comet is already active as sunlight warms the surface and causes frozen volatiles to boil off. Astronomers used such early images to try to measure the size of the nucleus, in order to predict whether the comet would stay intact when it slingshots around the sun -- at 700,000 miles above the sun's surface -- on Nov. 28, 2013.

 

The comet's dusty coma, or head of the comet, is approximately 3,100 miles across, or 1.2 times the width of Australia. A dust tail extends more than 57,000 miles, far beyond Hubble's field of view.

 

This image was taken in visible light. The blue false color was added to bring out details in the comet structure.

Credit: NASA/ ESA/STScI/AURA

 

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More details on Comet ISON:

 

Comet ISON began its trip from the Oort cloud region of our solar system and is now travelling toward the sun. The comet will reach its closest approach to the sun on Thanksgiving Day -- 28 Nov 2013 -- skimming just 730,000 miles above the sun's surface. If it comes around the sun without breaking up, the comet will be visible in the Northern Hemisphere with the naked eye, and from what we see now, ISON is predicted to be a particularly bright and beautiful comet.

 

Catalogued as C/2012 S1, Comet ISON was first spotted 585 million miles away in September 2012. This is ISON's very first trip around the sun, which means it is still made of pristine matter from the earliest days of the solar system’s formation, its top layers never having been lost by a trip near the sun. Comet ISON is, like all comets, a dirty snowball made up of dust and frozen gases like water, ammonia, methane and carbon dioxide -- some of the fundamental building blocks that scientists believe led to the formation of the planets 4.5 billion years ago.

 

NASA has been using a vast fleet of spacecraft, instruments, and space- and Earth-based telescope, in order to learn more about this time capsule from when the solar system first formed.

 

The journey along the way for such a sun-grazing comet can be dangerous. A giant ejection of solar material from the sun could rip its tail off. Before it reaches Mars -- at some 230 million miles away from the sun -- the radiation of the sun begins to boil its water, the first step toward breaking apart. And, if it survives all this, the intense radiation and pressure as it flies near the surface of the sun could destroy it altogether.

 

This collection of images show ISON throughout that journey, as scientists watched to see whether the comet would break up or remain intact.

 

The comet reaches its closest approach to the sun on Thanksgiving Day -- Nov. 28, 2013 -- skimming just 730,000 miles above the sun’s surface. If it comes around the sun without breaking up, the comet will be visible in the Northern Hemisphere with the naked eye, and from what we see now, ISON is predicted to be a particularly bright and beautiful comet.

 

ISON stands for International Scientific Optical Network, a group of observatories in ten countries who have organized to detect, monitor, and track objects in space. ISON is managed by the Keldysh Institute of Applied Mathematics, part of the Russian Academy of Sciences.

 

NASA image use policy.

 

NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission.

 

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Using original Lego set, modify it with system's bricks. Adding claws and tail to increase the "scary" feeling.

 

This is harder than I thought it would be.

The geothermal areas of Yellowstone include several geyser basins in Yellowstone National Park as well as other geothermal features such as hot springs, mud pots, and fumaroles. The number of thermal features in Yellowstone is estimated at 10,000. A study that was completed in 2011 found that a total of 1,283 geysers have erupted in Yellowstone, 465 of which are active during an average year. These are distributed among nine geyser basins, with a few geysers found in smaller thermal areas throughout the Park. The number of geysers in each geyser basin are as follows: Upper Geyser Basin (410), Midway Geyser Basin (59), Lower Geyser Basin (283), Norris Geyser Basin (193), West Thumb Geyser Basin (84), Gibbon Geyser Basin (24), Lone Star Geyser Basin (21), Shoshone Geyser Basin (107), Heart Lake Geyser Basin (69), other areas (33). Although famous large geysers like Old Faithful are part of the total, most of Yellowstone's geysers are small, erupting to only a foot or two. The hydrothermal system that supplies the geysers with hot water sits within an ancient active caldera. Many of the thermal features in Yellowstone build up sinter, geyserite, or travertine deposits around and within them.

 

The various geyser basins are located where rainwater and snowmelt can percolate into the ground, get indirectly superheated by the underlying Yellowstone hotspot, and then erupt at the surface as geysers, hot springs, and fumaroles. Thus flat-bottomed valleys between ancient lava flows and glacial moraines are where most of the large geothermal areas are located. Smaller geothermal areas can be found where fault lines reach the surface, in places along the circular fracture zone around the caldera, and at the base of slopes that collect excess groundwater. Due to the Yellowstone Plateau's high elevation the average boiling temperature at Yellowstone's geyser basins is 199 °F (93 °C). When properly confined and close to the surface it can periodically release some of the built-up pressure in eruptions of hot water and steam that can reach up to 390 feet (120 m) into the air (see Steamboat Geyser, the world's tallest geyser). Water erupting from Yellowstone's geysers is superheated above that boiling point to an average of 204 °F (95.5 °C) as it leaves the vent. The water cools significantly while airborne and is no longer scalding hot by the time it strikes the ground, nearby boardwalks, or even spectators. Because of the high temperatures of the water in the features it is important that spectators remain on the boardwalks and designated trails. Several deaths have occurred in the park as a result of falls into hot springs.

 

Prehistoric Native American artifacts have been found at Mammoth Hot Springs and other geothermal areas in Yellowstone. Some accounts state that the early people used hot water from the geothermal features for bathing and cooking. In the 19th century Father Pierre-Jean De Smet reported that natives he interviewed thought that geyser eruptions were "the result of combat between the infernal spirits". The Lewis and Clark Expedition traveled north of the Yellowstone area in 1806. Local natives that they came upon seldom dared to enter what we now know is the caldera because of frequent loud noises that sounded like thunder and the belief that the spirits that possessed the area did not like human intrusion into their realm. The first white man known to travel into the caldera and see the geothermal features was John Colter, who had left the Lewis and Clark Expedition. He described what he saw as "hot spring brimstone". Beaver trapper Joseph Meek recounted in 1830 that the steam rising from the various geyser basins reminded him of smoke coming from industrial smokestacks on a cold winter morning in Pittsburgh, Pennsylvania. In the 1850s famed trapper Jim Bridger called it "the place where Hell bubbled up".

 

The heat that drives geothermal activity in the Yellowstone area comes from brine (salty water) that is 1.5–3 miles (7,900–15,800 ft; 2,400–4,800 m) below the surface. This is actually below the solid volcanic rock and sediment that extends to a depth of 3,000 to 6,000 feet (900 to 1,800 m) and is inside the hot but mostly solid part of the pluton that contains Yellowstone's magma chamber. At that depth the brine is superheated to temperatures that exceed 400 °F (204 °C) but is able to remain a liquid because it is under great pressure (like a huge pressure cooker).

 

Convection of the churning brine and conduction from surrounding rock transfers heat to an overlaying layer of fresh groundwater. Movement of the two liquids is facilitated by the highly fractured and porous nature of the rocks under the Yellowstone Plateau. Some silica is dissolved from the fractured rhyolite into the hot water as it travels through the fractured rock. Part of this hard mineral is later redeposited on the walls of the cracks and fissures to make a nearly pressure-tight system. Silica precipitates at the surface to form either geyserite or sinter, creating the massive geyser cones, the scalloped edges of hot springs, and the seemingly barren landscape of geyser basins.

 

There are at least five types of geothermal features found at Yellowstone:

 

Fumaroles: Fumaroles, or steam vents, are the hottest hydrothermal features in the park. They have so little water that it all flashes into steam before reaching the surface. At places like Roaring Mountain, the result is loud hissing of steam and gases.

Geysers: Geysers such as Old Faithful are a type of geothermal feature that periodically erupt scalding hot water. Increased pressure exerted by the enormous weight of the overlying rock and water prevents deeper water from boiling. As the hot water rises it is under less pressure and steam bubbles form. They, in turn, expand on their ascent until the bubbles are too big and numerous to pass freely through constrictions. At a critical point the confined bubbles actually lift the water above, causing the geyser to splash or overflow. This decreases the pressure of the system and violent boiling results. Large quantities of water flash into tremendous amounts of steam that force a jet of water out of the vent: an eruption begins. Water (and heat) is expelled faster than the geyser's recharge rate, gradually decreasing the system's pressure and eventually ending the eruption.

Hot springs: Hot springs such as Grand Prismatic Spring are the most common hydrothermal features in the park. Their plumbing has no constrictions. Superheated water cools as it reaches the surface, sinks, and is replaced by hotter water from below. This circulation, called convection, prevents water from reaching the temperature needed to set off an eruption. Many hot springs give rise to streams of heated water.

Mudpots: Mudpots such as Fountain Paint Pots are acidic hot springs with a limited water supply. Some microorganisms use hydrogen sulfide (rotten egg smell), which rises from deep within the earth, as an energy source. They convert the gas into sulfuric acid, which breaks down rock into clay.

Travertine terraces: Travertine terraces, found at Mammoth Hot Springs, are formed from limestone (a rock type made of calcium carbonate). Thermal waters rise through the limestone, carrying high amounts of dissolved carbonate. Carbon dioxide is released at the surface and calcium carbonate deposited as travertine, the chalky white rock of the terraces. These features constantly and quickly change due to the rapid rate of deposition.

Geyser basins

 

The Norris Geyser Basin 44°43′43″N 110°42′16″W is the hottest geyser basin in the park and is located near the northwest edge of Yellowstone Caldera near Norris Junction and on the intersection of three major faults. The Norris-Mammoth Corridor is a fault that runs from Norris north through Mammoth to the Gardiner, Montana, area. The Hebgen Lake fault runs from northwest of West Yellowstone, Montana, to Norris. This fault experienced an earthquake in 1959 that measured 7.4 on the Richter scale (sources vary on exact magnitude between 7.1 and 7.8; see 1959 Hebgen Lake earthquake). Norris Geyser Basin is so hot and dynamic because these two faults intersect with the ring fracture zone that resulted from the creation of the Yellowstone Caldera of 640,000 years ago.

 

The Basin consists of three main areas: Porcelain Basin, Back Basin, and One Hundred Springs Plain. Unlike most of other geyser basins in the park, the waters from Norris are acidic rather than alkaline (for example, Echinus Geyser has a pH of ~3.5). The difference in pH allows for a different class of bacterial thermophiles to live at Norris, creating different color patterns in and around the Norris Basin waters.

 

The Ragged Hills that lie between Back Basin and One Hundred Springs Plain are thermally altered glacial kames. As glaciers receded the underlying thermal features began to express themselves once again, melting remnants of the ice and causing masses of debris to be dumped. These debris piles were then altered by steam and hot water flowing through them. Madison lies within the eroded stream channels cut through lava flows formed after the caldera eruption. The Gibbon Falls lies on the caldera boundary as does Virginia Cascades.

 

Algae on left bacteria on right at the intersection of flows from the Constant & Whirlgig Geysers at Norris Geyser Basin

The tallest active geyser in the world, Steamboat Geyser,[11] is located in Norris Basin. Unlike the slightly smaller but much more famous Old Faithful Geyser located in Upper Geyser Basin, Steamboat has an erratic and lengthy timetable between major eruptions. During major eruptions, which may be separated by intervals of more than a year (the longest recorded span between major eruptions was 50 years), Steamboat erupts over 300 feet (90 m) into the air. Steamboat does not lie dormant between eruptions, instead displaying minor eruptions of approximately 40 feet (12 m).

 

Norris Geyser Basin periodically undergoes a large-scale, basin-wide thermal disturbance lasting a few weeks. Water levels fluctuate, and temperatures, pH, colors, and eruptive patterns change throughout the basin. During a disturbance in 1985, Porkchop Geyser continually jetted steam and water; in 1989, the same geyser apparently clogged with silica and blew up, throwing rocks more than 200 feet (61 m). In 2003 a park ranger observed it bubbling heavily, the first such activity seen since 1991. Activity increased dramatically in mid-2003. Because of high ground temperatures and new features beside the trail much of Back Basin was closed until October. In 2004 the boardwalk was routed around the dangerous area and now leads behind Porkchop Geyser.

 

North of Norris, Roaring Mountain is a large, acidic hydrothermal area (solfatara) with many fumaroles. In the late 19th and early 20th centuries, the number, size, and power of the fumaroles were much greater than today. The fumaroles are most easily seen in the cooler, low-light conditions of morning and evening.

 

The Gibbon Geyser Basin 44°41′58″N 110°44′34″W includes several thermal areas in the vicinity of the Gibbon River between Gibbon Falls and Norris. The most accessible feature in the basin is Beryl Spring, with a small boardwalk right along the Grand Loop Road. Artists' Paintpots is a small hydrothermal area south of Norris Junction that includes colorful hot springs and two large mudpots.

 

The Monument Geyser Basin 44°41′03″N 110°45′14″W has no active geysers, but its 'monuments' are siliceous sinter deposits similar to the siliceous spires discovered on the floor of Yellowstone Lake. Scientists hypothesize that this basin's structures formed from a hot water system in a glacially dammed lake during the waning stages of the Pinedale Glaciation. The basin is on a ridge reached by a very steep one-mile (1.6 km) trail south of Artists' Paint Pots. Other areas of thermal activity in Gibbon Geyser Basin lie off-trail.

 

South of Norris along the rim of the caldera is the Upper Geyser Basin 44°27′52″N 110°49′45″W, which has the highest concentration of geothermal features in the park. This complement of features includes the most famous geyser in the park, Old Faithful Geyser, as well as four other predictable large geysers. One of these large geysers in the area is Castle Geyser which is about 1,400 feet (430 m) northwest of Old Faithful. Castle Geyser has an interval of approximately 13 hours between major eruptions, but is unpredictable after minor eruptions. The other three predictable geysers are Grand Geyser, Daisy Geyser, and Riverside Geyser. Biscuit Basin and Black Sand Basin are also within the boundaries of Upper Geyser Basin.

 

The hills surrounding Old Faithful and the Upper Geyser Basin are reminders of Quaternary rhyolitic lava flows. These flows, occurring long after the catastrophic eruption of 640,000 years ago, flowed across the landscape like stiff mounds of bread dough due to their high silica content.

 

Evidence of glacial activity is common, and it is one of the keys that allows geysers to exist. Glacier till deposits underlie the geyser basins providing storage areas for the water used in eruptions. Many landforms, such as Porcupine Hills north of Fountain Flats, are made up of glacial gravel and are reminders that 70,000 to 14,000 years ago, this area was buried under ice.

 

Signs of the forces of erosion can be seen everywhere, from runoff channels carved across the sinter in the geyser basins to the drainage created by the Firehole River. Mountain building is evident on the drive south of Old Faithful, toward Craig Pass. Here the Rocky Mountains reach a height of 8,262 feet (2,518 m), dividing the country into two distinct watersheds.

 

Midway Geyser Basin 44°31′04″N 110°49′56″W is much smaller than the other basins found alongside the Firehole River. Despite its small size, it contains two large features, the 200-by-300-foot-wide (60 by 90 m) Excelsior Geyser which pours over 4,000 U.S. gallons (15,000 L; 3,300 imp gal) per minute into the Firehole River. The largest hot spring in Yellowstone, the 370-foot-wide (110 m) and 121-foot-deep (37 m) Grand Prismatic Spring is found here. Also in the basin is Turquoise Pool and Opal Pool.

 

Lower Geyser Basin

Blue spring with steam rising from it; irregular blotches of red and orange residue are on the banks, along with dead tree trunks.

Silex Spring at Fountain Paint Pot

 

Farther north is the Lower Geyser Basin 44°32′58″N 110°50′09″W, which is the largest geyser basin in area, covering approximately 11 square miles. Due to its large size, it has a much less concentrated set of geothermal features, including Fountain Paint Pots. Fountain Paint Pots are mud pots, that is, a hot spring that contains boiling mud instead of water. The mud is produced by a higher acidity in the water which enables the spring to dissolve surrounding minerals to create an opaque, usually grey, mud. Also there is Firehole Spring, Celestine Pool, Leather Pool, Red Spouter, Jelly spring, and a number of fumaroles.

 

Geysers in Lower Geyser Basin include Great Fountain Geyser, whose eruptions reach 100 to 200 feet (30–61 m) in the air, while waves of water cascade down its sinter terraces., the Fountain group of Geysers (Clepsydra Geyser which erupts nearly continuously to heights of 45 feet (14 m), Fountain Geyser, Jelly Geyser, Jet Geyser, Morning Geyser, and Spasm Geyser), the Pink Cone group of geysers (Dilemma Geyser, Labial Geyser, Narcissus Geyser, Pink Geyser, and Pink Cone Geyser), the White Dome group of geysers (Crack Geyser, Gemini Geyser, Pebble Geyser, Rejuvenated Geyser, and White Dome Geyser), as well as Sizzler Geyser.

 

Clepsydra Geyser erupting. July 2019

Fountain Paint Pots

White Dome Geyser

West Thumb Geyser Basin

Several pools of blue water in ashen rock basin.

West Thumb Geyser Basin

Blackened basin with orange streaks; steam is rising from it with fir trees in the background.

Overflow areas of Silex springs

 

The West Thumb Geyser Basin 44°25′07″N 110°34′23″W, including Potts Basin to the north, is the largest geyser basin on the shores of Yellowstone Lake. The heat source of the thermal features in this location is thought to be relatively close to the surface, only 10,000 feet (3,000 m) down. West Thumb is about the same size as another famous volcanic caldera, Crater Lake in Oregon, but much smaller than the great Yellowstone Caldera which last erupted about 640,000 years ago. West Thumb is a caldera within a caldera.

 

West Thumb was created approximately 162,000 years ago when a magma chamber bulged up under the surface of the earth and subsequently cracked it along ring fracture zones. This in turn released the enclosed magma as lava and caused the surface above the emptied magma chamber to collapse. Water later filled the collapsed area of the caldera, forming an extension of Yellowstone Lake. This created the source of heat and water that feed the West Thumb Geyser Basin today.

 

The thermal features at West Thumb are not only found on the lake shore, but extend under the surface of the lake as well. Several underwater hydrothermal features were discovered in the early 1990s and can be seen as slick spots or slight bulges in the summer. During the winter, the underwater thermal features are visible as melt holes in the icy surface of the lake. The surrounding ice can reach three feet (one yard) in thickness.

 

Perhaps the most famous hydrothermal feature at West Thumb is a geyser on the lake shore known as Fishing Cone. Walter Trumbull of the 1870 Washburn-Langford-Doane Expedition described a unique event while a man was fishing adjacent to the cone: "...in swinging a trout ashore, it accidentally got off the hook and fell into the spring. For a moment it darted about with wonderful rapidity, as if seeking an outlet. Then it came to the top, dead, and literally boiled." Fishing Cone erupted frequently to the height of 40 feet (12 m) in 1919 and to lesser heights in 1939. One fisherman was badly burned in Fishing Cone in 1921. Fishing at the geyser is now prohibited.

 

Early visitors would arrive at West Thumb via stagecoach from the Old Faithful area. They had a choice of continuing on the stagecoach or boarding the steamship Zillah to continue the journey by water to Lake Hotel. The boat dock was located near the south end of the geyser basin near Lakeside Spring.

 

Backcountry Geyser Basins

The Heart Lake 44°18′00″N 110°30′56″W, Lone Star 44°24′50″N 110°49′04″W, and Shoshone Geyser Basins 44°21′16″N 110°47′57″W are located away from the road and require at least several miles of hiking to reach. These areas lack the boardwalks and other safety features of the developed areas. As falling into geothermal features can be fatal, it is usually advisable to visit these areas with an experienced guide or at the very least, travelers need to ensure they remain on well-marked trails.

 

The Heart Lake Geyser Basin contains several groups of geysers and deep blue hot springs near Heart Lake in the south-central portion of Yellowstone, southeast of most of the main geyser basins. Lying in the Snake River watershed east of Lewis Lake and south of Yellowstone Lake, Heart Lake was named sometime before 1871 for Hart Hunney, a hunter. Other explorers in the region incorrectly assumed that the lake's name was spelled 'heart' because of its shape. The Heart Lake Geyser Basin begins a couple miles from the lake and descends along Witch Creek to the lakeshore. Five groups of hydrothermal features comprise the basin, and all of them contain geysers, although some are dormant.

 

Between Shoshone Lake and Old Faithful is the Lone Star Geyser Basin, of which the primary feature is Lone Star Geyser, named for its isolation from the nearby geysers of the Upper Geyser Basin. The basin is reachable on foot or bicycle via a 3 mile road that is closed to vehicles.

 

The Shoshone Geyser Basin, reached by hiking or by boat, contains one of the highest concentrations of geysers in the world – more than 80 in an area 1,600 by 800 feet (490 by 240 m). Hot springs and mudpots dot the landscape between the geyser basin and Shoshone Lake.

 

Hot Spring Basin is located 15 miles (24 km) north-northeast of Fishing Bridge and has one of Yellowstone's largest collections of hot springs and fumaroles. The geothermal features there release large amounts of sulfur. This makes water from the springs so acidic that it has dissolved holes in the pants of people who sit on wet ground and causes mounds of sulfur three feet (1 m) high to develop around fumaroles. The very hot acidic water and steam have also created voids in the ground that are only covered by a thin crust.

 

Mammoth Hot Springs is a large complex of hot springs on a hill of travertine in Yellowstone National Park adjacent to Fort Yellowstone and the Mammoth Hot Springs Historic District. It was created over thousands of years as hot water from the spring cooled and deposited calcium carbonate (over two tons flow into Mammoth each day in a solution). Because of the huge amount of geothermal vents, travertine flourishes. Although these springs lie outside the caldera boundary, their energy has been attributed to the same magmatic system that fuels other Yellowstone geothermal areas.

 

The thermal features at Mud Volcano and Sulphur Caldron are primarily mud pots and fumaroles because the area is situated on a perched water system with little water available. Fumaroles or "steam vents" occur when the ground water boils away faster than it can be recharged. Also, the vapors are rich in sulfuric acid that leaches the rock, breaking it down into clay. Because no water washes away the acid or leached rock, it remains as sticky clay to form a mud pot. Hydrogen sulfide gas is present deep in the earth at Mud Volcano and is oxidized to sulfuric acid by microbial activity, which dissolves the surface soils to create pools and cones of clay and mud. Along with hydrogen sulfide, steam, carbon dioxide, and other gases explode through the layers of mud.

 

A series of shallow earthquakes associated with the volcanic activity in Yellowstone struck this area in 1978. Soil temperatures increased to nearly 200 °F (93 °C). The slope between Sizzling Basin and Mud Geyser, once covered with green grass and trees, became a barren landscape of fallen trees known as "the cooking hillside".

 

Yellowstone National Park is a national park located in the western United States, largely in the northwest corner of Wyoming and extending into Montana and Idaho. It was established by the 42nd U.S. Congress with the Yellowstone National Park Protection Act and signed into law by President Ulysses S. Grant on March 1, 1872. Yellowstone was the first national park in the U.S. and is also widely held to be the first national park in the world. The park is known for its wildlife and its many geothermal features, especially the Old Faithful geyser, one of its most popular. While it represents many types of biomes, the subalpine forest is the most abundant. It is part of the South Central Rockies forests ecoregion.

 

While Native Americans have lived in the Yellowstone region for at least 11,000 years, aside from visits by mountain men during the early-to-mid-19th century, organized exploration did not begin until the late 1860s. Management and control of the park originally fell under the jurisdiction of the U.S. Department of the Interior, the first Secretary of the Interior to supervise the park being Columbus Delano. However, the U.S. Army was eventually commissioned to oversee the management of Yellowstone for 30 years between 1886 and 1916. In 1917, the administration of the park was transferred to the National Park Service, which had been created the previous year. Hundreds of structures have been built and are protected for their architectural and historical significance, and researchers have examined more than a thousand archaeological sites.

 

Yellowstone National Park spans an area of 3,468.4 sq mi (8,983 km2), comprising lakes, canyons, rivers, and mountain ranges. Yellowstone Lake is one of the largest high-elevation lakes in North America and is centered over the Yellowstone Caldera, the largest super volcano on the continent. The caldera is considered a dormant volcano. It has erupted with tremendous force several times in the last two million years. Well over half of the world's geysers and hydrothermal features are in Yellowstone, fueled by this ongoing volcanism. Lava flows and rocks from volcanic eruptions cover most of the land area of Yellowstone. The park is the centerpiece of the Greater Yellowstone Ecosystem, the largest remaining nearly intact ecosystem in the Earth's northern temperate zone. In 1978, Yellowstone was named a UNESCO World Heritage Site.

 

Hundreds of species of mammals, birds, fish, reptiles, and amphibians have been documented, including several that are either endangered or threatened. The vast forests and grasslands also include unique species of plants. Yellowstone Park is the largest and most famous megafauna location in the contiguous United States. Grizzly bears, cougars, wolves, and free-ranging herds of bison and elk live in this park. The Yellowstone Park bison herd is the oldest and largest public bison herd in the United States. Forest fires occur in the park each year; in the large forest fires of 1988, nearly one-third of the park was burnt. Yellowstone has numerous recreational opportunities, including hiking, camping, boating, fishing, and sightseeing. Paved roads provide close access to the major geothermal areas as well as some of the lakes and waterfalls. During the winter, visitors often access the park by way of guided tours that use either snow coaches or snowmobiles.

 

Teton County is a county in the U.S. state of Wyoming. As of the 2020 United States Census, the population was 23,331. Its county seat is Jackson. Its west boundary line is also the Wyoming state boundary shared with Idaho and the southern tip of Montana. Teton County is part of the Jackson, WY-ID Micropolitan Statistical Area.

 

Teton County contains the Jackson Hole ski area, all of Grand Teton National Park, and 40.4% of Yellowstone National Park's total area, including over 96.6% of its water area (largely in Yellowstone Lake).

 

Wyoming is a state in the Mountain West subregion of the Western United States. It borders Montana to the north and northwest, South Dakota and Nebraska to the east, Idaho to the west, Utah to the southwest, and Colorado to the south. With a population of 576,851 in 2020, Wyoming is the least populous state despite being the 10th largest by area, with the second-lowest population density after Alaska. The state capital and most populous city is Cheyenne, which had an estimated population of 63,957 in 2018.

 

Wyoming's western half consists mostly of the ranges and rangelands of the Rocky Mountains; its eastern half consists of high-elevation prairie, and is referred to as the High Plains. Wyoming's climate is semi-arid in some parts and continental in others, making it drier and windier overall than other states, with greater temperature extremes. The federal government owns just under half of Wyoming's land, generally protecting it for public uses. The state ranks sixth in the amount of land—-and fifth in the proportion of its land—-that is owned by the federal government. Its federal lands include two national parks (Grand Teton and Yellowstone), two national recreation areas, two national monuments, and several national forests, as well as historic sites, fish hatcheries, and wildlife refuges.

 

Indigenous peoples inhabited the region for thousands of years. Historic and currently federally recognized tribes include the Arapaho, Crow, Lakota, and Shoshone. Part of the land that is now Wyoming came under American sovereignty via the Louisiana Purchase, part via the Oregon Treaty, and, lastly, via the Mexican Cession. With the opening of the Oregon Trail, the Mormon Trail, and the California Trail, vast numbers of pioneers travelled through parts of the state that had once been traversed mainly by fur trappers, and this spurred the establishment of forts, such as Fort Laramie, that today serve as population centers. The Transcontinental Railroad supplanted the wagon trails in 1867 with a route through southern Wyoming, bringing new settlers and the establishment of founding towns, including the state capital of Cheyenne. On March 27, 1890, Wyoming became the union's 44th state.

 

Farming and ranching, and the attendant range wars, feature prominently in the state's history. Today, Wyoming's economy is largely based on tourism and the extraction of minerals such as coal, natural gas, oil, and trona. Its agricultural commodities include barley, hay, livestock, sugar beets, wheat, and wool.

 

Wyoming was the first state to allow women the right to vote (not counting New Jersey, which had allowed it until 1807), and the right to assume elected office, as well as the first state to elect a female governor. In honor of this part of its history, its most common nickname is "The Equality State" and its official state motto is "Equal Rights". It is among the least religious states in the country, and is known for having a political culture that leans towards libertarian conservatism. The Republican presidential nominee has carried the state in every election since 1968.

Bangkok Railway Station (Thai: สถานีรถไฟกรุงเทพ), unofficially known as Hua Lamphong Station (หัวลำโพง), is the main railway station in Bangkok, Thailand. It is in the center of the city in the Pathum Wan District, and is operated by the State Railway of Thailand.

 

The station is officially referred to by the State Railway of Thailand as Krungthep Station in Thai ('Krungthep' is the transliteration of the common Thai language name of Bangkok) and Bangkok Station in English. Hua Lamphong is the informal name of the station, used by both foreign travellers and locals. The station is often named as Hua Lamphong in travel guide books and in the public press.

 

In other areas of Thailand the station is commonly referred to as Krungthep Station, and the name Hua Lamphong is not well-known.

 

In all documents published by the State Railway of Thailand (such as train tickets, timetables, and tour pamphlets) the station is uniformly transcribed as Krungthep (กรุงเทพฯ) in Thai.

 

The station was opened on June 25, 1916 after six years' construction. The site of the railway station was previously occupied by the national railway's maintenance centre, which moved to Makkasan in June 1910. At the nearby site of the previous railway station a pillar commemorates the inauguration of the Thai railway network in 1897.

 

The station was built in an Italian Neo-Renaissance-style, with decorated wooden roofs and stained glass windows. The architecture is attributed to Turin-born Mario Tamagno, who with countryman Annibale Rigotti (1870–1968) was also responsible for the design of several other early 20th century public buildings in Bangkok. The pair designed Bang Khun Prom Palace (1906), Ananta Samakhom Throne Hall in the Royal Plaza (1907–15) and Suan Kularb Residential Hall and Throne Hall in Dusit Garden, among other buildings.

 

There are 14 platforms, 26 ticket booths, and two electric display boards. Hua Lamphong serves over 130 trains and approximately 60,000 passengers each day. Since 2004 the station has been connected by an underground passage to the MRT (Metropolitan Rapid Transit) subway system's Hua Lamphong Station.

 

The station is also a terminus of the Eastern and Oriental Express luxury trains.

 

From Wikipedia

 

The Hispasat AG1 communications satellite completes the integration phase of testing in OHB System's cleanroom in Bremen, Germany. Hispasat AG1 will provide Spain, Portugal, the Canary Islands and the Americas with faster multimedia services through its reconfigurable Redsat payload.

 

AG1 is now at the IABG (Industrieanlagen-Betriebsgesellschaft) in Ottobrunn, Germany, undergoing environmental impact testing. There it will be placed in the thermal-vacuum chamber and its systems tested under ultra-high and low temperatures to simulate the conditions in space.

 

AG1 is the first satellite to use Europe’s new SmallGEO platform, developed through a public–private partnership between ESA and OHB. SmallGEO will strengthen the position of European industry in the commercial telecommunications market, expanding the current range of available products.

 

Credit:OHB

A United Launch Alliance Atlas V rocket with Boeing’s CST-100 Starliner spacecraft aboard is seen after being rolled out of the Vertical Integration Facility to the launch pad at Space Launch Complex 41 ahead of the Orbital Flight Test-2 (OFT-2) mission, Wednesday, May 18, 2022 at Cape Canaveral Space Force Station in Florida. Boeing’s Orbital Flight Test-2 will be Starliner’s second uncrewed flight test and will dock to the International Space Station as part of NASA's Commercial Crew Program. The mission, currently targeted for launch at 6:54 p.m. ET on May 19, will serve as an end-to-end test of the system's capabilities. Photo Credit: (NASA/Joel Kowsky)

A United Launch Alliance Atlas V rocket with Boeing’s CST-100 Starliner spacecraft aboard is seen at sunrise on the launch pad at Space Launch Complex 41 ahead of the Orbital Flight Test-2 mission, Tuesday, Aug. 3, 2021 at Cape Canaveral Space Force Station in Florida. Boeing’s Orbital Flight Test-2 will be Starliner’s second uncrewed flight test and will dock to the International Space Station as part of NASA's Commercial Crew Program. The mission, currently targeted for launch at 1:20 p.m. EDT, will serve as an end-to-end test of the system's capabilities. Photo Credit: (NASA/Aubrey Gemignani)

This cow statue in South Station has the Boston rapid transit system painted all over its body. (The blue areas are water.) I guess the circle-T on its forehead is the brand for the MBTA, the transit system's name, and the one red teat is the southern end of the Red Line (but which end -- Ashmont or Braintree?)

 

The words across its horns are a lyric from a local political song that the Kingston Trio made into a national hit in the Fifties. They called it "M.T.A." (the old name for the system), but most people know it as "Charlie on the MTA" -- "He may ride forever 'neath the streets of Boston / He's the man who never returned."

 

June 2006 [6 months later]: Click here to see one of the first of the outdoor cows in the Boston Cow Parade -- www.flickr.com/photos/antydiluvian/162067356/?#comment721....

 

Our solar system’s most massive planet, Jupiter, was about 739 million kilometres (460 million miles) from the Earth when I captured this photo at Seven Mile Beach, Australia. Saturn, the planet known for its beautiful system of encircling rings, was orbiting further out in space at a distance of 1.48 billion kilometres (920 million miles) at that time. These two “gas giant” planets are the two bright spots visible in my image, appearing to hover over the Tasman Sea. The light coming from Jupiter was intense enough for it to be reflected off the water’s surface, visible to human eyes and the camera, as you can see here. Saturn is the less-bright spot below and to the right of Jupiter, and its usually yellow-white light reddened by atmospheric refraction.

 

The background sky colour has a green hue, created by the atmospheric phenomenon known as “airglow”, and this is also reflected in the shallow foreground wash along with some of the stars. Giving the blue colour to the more distant waves is the glow of bioluminescent marine organisms. The agitation from each breaking wave stirred up the little critters, causing them to glow in the dark. The whole scene was beautiful beyond belief, once more leaving me open-mouthed, humbled and in awe of the Creator.

 

The photo is a single-frame image that I shot using my Canon EOS 6D Mk II camera, a Yongnuo 50mm f/1.4 lens @ f/1.8, with an exposure time of 10 seconds @ ISO 6400.

The Porsche 959 is a sports car manufactured by Porsche from 1986 to 1989, first as a Group B rally car and later as a legal production car designed to satisfy FIA homologation regulations requiring that a minimum number of 200 street legal units be built.

 

During its production run, it was hailed as being the most technologically advanced road-going sports car ever built and the harbinger of the future of sports cars: it was one of the first high-performance vehicles to use an all-wheel drive system; it provided the basis for Porsche's first all-wheel drive Carrera 4 model; and it convinced Porsche executives of the system's viability so well that they chose to make all-wheel drive standard on all versions of the 911 Turbo starting with the 993 variant. During its lifetime, the vehicle had only one other street legal peer with comparable performance, the Ferrari F40. The 959's short production run and performance have kept values high. In 2004, Sports Car International named this car number one on the list of Top Sports Cars of the 1980s.

  

In reality, the sign is part of a traffic education program intended to help drivers visualize a safe following distance at highway speeds. The sign, by itself, just seems incongruous and, well, funny as you pass by.

“Views of the STS-7 shuttle Challenger taken from the Shuttle pallet satellite (SPAS-01) include: Close-up view of shuttle Challenger payload bay with the Remote Manipulator System (RMS) arm bent in the shape of a seven.”

 

Above per the National Archives and Records Administration (NARA) description/caption linked to below.

 

A great rarely seen closeup image. I was hoping to see an Astronaut’s face in one of the overhead windows but there only seems to be an external reflection of the Remote Manipulator System’s end effector/wrist area visible in the left window.

 

20/20 hindsight: The tiles, especially on the bottom of the orbiter, were of concern since day 1. This would’ve been an excellent opportunity – early on – to take a good look. It seems it would’ve been a simple matter to do a flip/pirouette of the spacecraft to allow the venerable Hasselblad camera system aboard SPAS-01 to capture some detailed images. Surely someone must’ve proposed it? Was it considered to be a risky move…due to losing line-of-sight? Isn’t that what the Ku-band radar, seen at the upper right corner of the payload bay, is for?

If brought up/considered, who knows what questionable, convoluted & egregious factors precluded such. Or was it an unconscionable 'head in the sand' mentality/culture? Since, if the tiles were severely damaged or missing, nothing could've been done anyhow?

 

Note the fondly nostalgic fiducial marks within the image…Long Live Apollo, and to lesser extent, Hasselblad. 😉

 

catalog.archives.gov/id/22489930

Credit: National Archives and Records Administration (NARA) website

A SpaceX Falcon 9 rocket with the company's Crew Dragon spacecraft onboard is seen as it is rolled to the launch pad at Launch Complex 39A as preparations continue for the Demo-1 mission, Feb. 28, 2019 at the Kennedy Space Center in Florida. The Demo-1 mission will be the first launch of a commercially built and operated American spacecraft and space system designed for humans as part of NASA's Commercial Crew Program. The mission, currently targeted for a 2:49am launch on March 2, will serve as an end-to-end test of the system's capabilities Photo Credit: (NASA/Joel Kowsky)

Use this image without my permission is illegal. All Rights Reserved ste.t.©

 

Although ya try to iscredit

Ya still never edit

The needle, I'll thread it

Radically poetic

Standin' with the fury that they had in '66

And like E-Double, I'm mad

Still knee-deep in the system's shit

Hoover, he was a body remover

I'll give ya a dose

But it'll never come close

To the rage built up inside of me

Fist in the air, in the land of hypocrisy

 

Movements come and movements go

Leaders speak, movements cease

When theirheads are flown

'Cause all these punks

Got bullets in their heads

Department of police, the judge, the feds

Networks at work, keepin' people calm

 

You know they went after King

When he spoke out on Vietnam

He turned the power to the have-nots

And then came the shot

 

Wit' poetry, my mind I flex

Flip like Wilson, vocals never lackin' dat fitnesse

Whadda I have to do to wake you up

To shake you up, to break the structure up

'Cause this blood still floods in the gutter

I'm like talkin' photos

Mad boy kicks open the shutter

Set the groove

Then I stick and move like I was Cassius

Rep the stutter step

Then bomb a left upon the facists

Yea, the several federal men

Who pulled schemes on the dream

And put it to an end

 

Ya better beware

Of retribution with mind war

20/20 visions and murals with metaphors

 

The networks at work, keepin' people calm

Ya know they murdered X

And tried to blame it on Islam

He turned the power to the have-nots

And then came the shot

 

What was the price on his head

 

Rage Against The Machine

wake up

 

NASA image acquired: June 03, 2012

 

This scene is to the northwest of the recently named crater Magritte, in Mercury's south. The image is not map projected; the larger crater actually sits to the north of the two smaller ones. The shadowing helps define the striking "Mickey Mouse" resemblance, created by the accumulation of craters over Mercury's long geologic history.

 

This image was acquired as part of MDIS's high-incidence-angle base map. The high-incidence-angle base map is a major mapping activity in MESSENGER's extended mission and complements the surface morphology base map of MESSENGER's primary mission that was acquired under generally more moderate incidence angles. High incidence angles, achieved when the Sun is near the horizon, result in long shadows that accentuate the small-scale topography of geologic features. The high-incidence-angle base map is being acquired with an average resolution of 200 meters/pixel.

 

The MESSENGER spacecraft is the first ever to orbit the planet Mercury, and the spacecraft's seven scientific instruments and radio science investigation are unraveling the history and evolution of the Solar System's innermost planet. Visit the Why Mercury? section of this website to learn more about the key science questions that the MESSENGER mission is addressing. During the one-year primary mission, MESSENGER acquired 88,746 images and extensive other data sets. MESSENGER is now in a yearlong extended mission, during which plans call for the acquisition of more than 80,000 additional images to support MESSENGER's science goals.

 

Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

 

NASA image use policy.

 

NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission.

 

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Alcatraz

 

Early Years as a Military Prison

 

In 1775, Spanish explorer Juan Manuel de Ayala (1745-97) mapped and named rugged Alcatraz Island, christening it La Isla de los Alcatraces, or Island of the Pelicans, due to its large population of sea birds. Seventy-five years later, in 1850, President Millard Fillmore (1800-74) signed an order reserving the island for military use. During the 1850s, a fortress was constructed on Alcatraz and some 100 cannons were installed around the island to protect San Francisco Bay. Also during this time, Alcatraz became home to the West Coast’s first operational lighthouse.

By the late 1850s, the U.S. Army had begun holding military prisoners at Alcatraz. Isolated from the mainland by the cold, strong waters of San Francisco Bay, the island was deemed an ideal location for a prison. It was assumed no Alcatraz inmate could attempt to escape by swimming and survive.

 

During its years as a military prison, the inmates at Alcatraz included Confederate sympathizers and citizens accused of treason during the American Civil War (1861-65). Alcatraz also housed a number of “rebellious” American Indians, including 19 Hopis from the Arizona Territory who were sent to the prison in 1895 following land disagreements with the federal government. The inmate population at Alcatraz continued to rise during the Spanish-American War (1898).

 

During the early 20th century, inmate labor fueled the construction of a new cellhouse (the 600-cell structure still stands today) on Alcatraz, along with a hospital, mess hall and other prison buildings. According to the National Park Service, when this new complex was finished in 1912 it was the world’s largest reinforced concrete building.

Doing Time as a Federal Prison: 1934-63

 

In 1933, the Army relinquished Alcatraz to the U.S. Justice Department, which wanted a federal prison that could house a criminal population too difficult or dangerous to be handled by other U.S. penitentiaries. Following construction to make the existing complex at Alcatraz more secure, the maximum-security facility officially opened on July 1, 1934. The first warden, James A. Johnston (1874-1954), hired approximately one guard for every three prisoners. Each prisoner had his own cell.

 

The Federal Bureau of Prisons (BOP) viewed Alcatraz as “the prison system’s prison,” a place where the most disruptive inmates could be sent to live under sparse conditions with few privileges in order to learn how to follow rules (at which point, they could be transferred to other federal prisons to complete their sentences). According to the BOP, Alcatraz typically held some 260 to 275 prisoners, which represented less than 1 percent of the entire federal inmate population.

 

The federal prison on Alcatraz Island in the chilly waters of California’s San Francisco Bay housed some of America’s most difficult and dangerous felons during its years of operation from 1934 to 1963. Among those who served time at the maximum-security facility were the notorious gangster Al “Scarface” Capone (1899-1947) and murderer Robert “Birdman of Alcatraz” Stroud (1890-1963). No inmate ever successfully escaped The Rock, as the prison was nicknamed, although more than a dozen known attempts were made over the years. After the prison was shut down due to high operating costs, the island was occupied for almost two years, starting in 1969, by a group of Native-American activists. Today, historic Alcatraz Island, which was also the site of a U.S. military prison from the late 1850s to 1933, is a popular tourist destination.

 

Source: www.history.com/topics/alcatraz

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