View allAll Photos Tagged LargeMagellanicCloud
Edited Hubble Space Telescope image of a nebula in the Large Magellanic Cloud.
Original caption: Today’s NASA/ESA Hubble Space Telescope Picture of the Week features a sparkling cloudscape from one of the Milky Way’s galactic neighbours, a dwarf galaxy called the Large Magellanic Cloud. Located 160 000 light-years away in the constellations Dorado and Mensa, the Large Magellanic Cloud is the largest of the Milky Way’s many small satellite galaxies. This view of dusty gas clouds in the Large Magellanic Cloud is possible thanks to Hubble’s cameras, such as the Wide Field Camera 3 (WFC3) that was used to collect the observations for this image. WFC3 is equipped with a variety of filters, each of which lets through only specific wavelengths, or colours, of light. This image combines observations made with five different filters, including some that capture ultraviolet and infrared light that the human eye cannot see. The wispy gas clouds in this image resemble brightly coloured candyfloss. When viewing such a vividly coloured cosmic scene, it is natural to wonder whether the colours are ‘real’. After all, Hubble, with its 2.4 metre-wide mirror and advanced scientific instruments, doesn’t bear resemblance to a typical camera! When image-processing specialists combine raw filtered data into a multi-coloured image like this one, they assign a colour to each filter. Visible-light observations are typically matched to the colour that the filter allows through. Shorter wavelengths of light such as ultraviolet are usually coloured blue or purple, while longer wavelengths like infrared are typically coloured red. This colour scheme closely represents reality while adding new information from the portions of the electromagnetic spectrum that humans cannot see. However, there are endless possible colour combinations that can be employed to achieve an especially aesthetically pleasing or scientifically insightful image. [Image Description: A part of a nebula in space. It is made of layers of gas and dust clouds in different colours, from blue and green shades to pink, red and black, indicating light emitted by different molecules. The background cloud layers are thicker and puffier, though still translucent, and the upper layers are thin and bright at the edges. Behind the clouds are very many small, mostly orange and some blue, stars.]
EARTH & SKY Photo taken by David Weir - Location: Mt John University Observatory, Lake Tekapo, New Zealand
Edited European Southern Observatory image of a star-forming region in the Large Magellanic Cloud. Color/processing variant.
Original caption: This colourful new view shows the star-forming region LHA 120-N44 [1] in the Large Magellanic Cloud, a small satellite galaxy of the Milky Way. This picture combines the view in visible light from the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile with images in infrared light and X-rays from orbiting satellite observatories. At the centre of this very rich region of gas, dust and young stars lies the star cluster NGC 1929. Its massive stars produce intense radiation, expel matter at high speeds as stellar winds, and race through their short but brilliant lives to explode as supernovae. The winds and supernova shock waves have carved out a huge cavity, called a superbubble, in the surrounding gas. Observations with NASA's Chandra X-ray Observatory (shown here in blue) reveal hot regions created by these winds and shocks, while infrared data from NASA's Spitzer Space Telescope (shown in red) outline where the dust and cooler gas are found. The visible-light view from the MPG/ESO 2.2-metre telescope (in yellow) completes the picture and shows the hot young stars themselves as well as the glowing clouds of gas and dust that surround them. Combining these different views of this dramatic region has allowed astronomers to solve a mystery: why are N44, and similar superbubbles, giving off such strong X-rays? The answer seems to be that there are two extra sources of bright X-ray emission: supernova shock waves striking the walls of the cavities, and hot material evaporating from the cavity walls. This X-ray emission from the edge of the superbubble shows up clearly in the picture. Links NASA’s Chandra X-ray Observatory NASA’s Spitzer Space Telescope Notes [1] The designation of this object indicates that it was included in the Catalogue of H-alpha emission stars and nebulae in the Magellanic Clouds, compiled and published in 1956 by American astronomer–astronaut Karl Henize (1926–1993). The letter “N” indicates that it is a nebula. The object is often called simply N44.
EARTH & SKY Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
For some stunning Earth & Sky time-lapse animations, please refer to MakiTKP on You Tube.
EARTH & SKY Photo taken by Igor Hoogerwerf - Location: Mt John University Observatory, Lake Tekapo, New Zealand
For tips on capturing your own images of the night sky www.earthandskynz.com/window-to-the-universe/en/astrophot....
For some stunning Earth & Sky time-lapse animations, please refer to MakiTKP on You Tube.
Attention: Due to the overwhelmingly positive response we've had to our photo stream we’re having to pare down the amount of archived material we leave open to the public to make it easier for our valued guests to locate new images… As the “group photos” garner the most attention and appear most popular we’ll endeavor to keep access to these priceless pictures open for at least two months. Many kind thanks, Earth & Sky team.
Edited European Southern Observatory image of a star forming region in the Large Magellanic Cloud.
Original caption: This dazzling region of newly-forming stars in the Large Magellanic Cloud (LMC) was captured by the Multi Unit Spectroscopic Explorer instrument on ESO’s Very Large Telescope. The relatively small amount of dust in the LMC and MUSE’s acute vision allowed intricate details of the region to be picked out in visible light.
EARTH & SKY Photo taken by Maki Yanagimachi- Location: Mt John University Observatory, Lake Tekapo, New Zealand
For tips on capturing your own images of the night sky click here.
For some stunning Earth & Sky time-lapse animations, please refer to MakiTKP on You Tube.
Attention: Due to the overwhelmingly positive response we've had to our photo stream we’re having to pare down the amount of archived material we leave open to the public to make it easier for our valued guests to locate new images… As the “group photos” garner the most attention and appear most popular we’ll endeavor to keep access to these priceless pictures open for at least two months. Many kind thanks, Earth & Sky team.
EARTH & SKY Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
For some stunning Earth & Sky time-lapse animations, please refer to MakiTKP on You Tube.
Edited TESS PR image of first light (or, more accurately, first released images) view. TESS is a satellite designed to search for planets. This is a set of strips of images showing what the camera saw (mainly stars and the Large and Small Magellanic Clouds (satellite galaxies of the Milky Way)). Color/processing variant.
Image source: www.nasa.gov/feature/goddard/2018/nasa-s-tess-shares-firs...
and
Image source: svs.gsfc.nasa.gov/13069
Original caption: NASA’s newest planet hunter, the Transiting Exoplanet Survey Satellite (TESS), is now providing valuable data to help scientists discover and study exciting new exoplanets, or planets beyond our solar system. Part of the data from TESS’ initial science orbit includes a detailed picture of the southern sky taken with all four of the spacecraft’s wide-field cameras. This “first light” science image captures a wealth of stars and other objects, including systems previously known to have exoplanets.
“In a sea of stars brimming with new worlds, TESS is casting a wide net and will haul in a bounty of promising planets for further study,” said Paul Hertz, astrophysics division director at NASA Headquarters in Washington. “This first light science image shows the capabilities of TESS’ cameras, and shows that the mission will realize its incredible potential in our search for another Earth.”
TESS acquired the image using all four cameras during a 30-minute period on Tuesday, Aug. 7. The black lines in the image are gaps between the camera detectors. The images include parts of a dozen constellations, from Capricornus to Pictor, and both the Large and Small Magellanic Clouds, the galaxies nearest to our own. The small bright dot above the Small Magellanic Cloud is a globular cluster — a spherical collection of hundreds of thousands of stars — called NGC 104, also known as 47 Tucanae because of its location in the southern constellation Tucana, the Toucan. Two stars, Beta Gruis and R Doradus, are so bright they saturate an entire column of pixels on the detectors of TESS’s second and fourth cameras, creating long spikes of light.
“This swath of the sky’s southern hemisphere includes more than a dozen stars we know have transiting planets based on previous studies from ground observatories,” said George Ricker, TESS principal investigator at the Massachusetts Institute of Technology’s (MIT) Kavli Institute for Astrophysics and Space Research in Cambridge.
EARTH & SKY Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
For tips on capturing your own images of the night sky www.earthandskynz.com/window-to-the-universe/en/astrophot....
For some stunning Earth & Sky time-lapse animations, please refer to MakiTKP on You Tube.
Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
Please refer to MakiTKP on You Tube for some stunning time-lapse animations.
Edited European Southern Observatory image of the Tarantula Nebula in the Large Magellanic Cloud. Color/processing variant.
Original caption: Glowing brightly about 160 000 light-years away, the Tarantula Nebula is the most spectacular feature of the Large Magellanic Cloud, a satellite galaxy to our Milky Way. This image from VLT Survey Telescope at ESO’s Paranal Observatory in Chile shows the region and its rich surroundings in great detail. It reveals a cosmic landscape of star clusters, glowing gas clouds and the scattered remains of supernova explosions.
Edited Hubble Space Telescope image (released as part of Hubble's 30th anniversary celebrations) of two nebulae in the Large Magellanic Cloud. Color/processing variant.
Original caption: This Hubble image shows how young, energetic, massive stars illuminate and sculpt their birthplace with powerful winds and searing ultraviolet radiation.
In this Hubble portrait, the giant red nebula (NGC 2014) and its smaller blue neighbor (NGC 2020) are part of a vast star-forming region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way, located 163,000 light-years away. The image is nicknamed the âCosmic Reef,â because it resembles an undersea world.
The sparkling centerpiece of NGC 2014 is a grouping of bright, hefty stars, each 10 to 20 times more massive than our Sun. The starsâ ultraviolet radiation heats the surrounding dense gas. The massive stars also unleash fierce winds of charged particles that blast away lower-density gas, forming the bubble-like structures seen on the right. The starsâ powerful stellar winds are pushing gas and dust to the denserÂ
left side of the nebula, where it is piling up, creating a series of dark ridges bathed in starlight. The blue areas in NGC 2014 reveal the glow of oxygen, heated to nearly 20,000 degrees Fahrenheit by the blast of ultraviolet light. The cooler, red gas indicates the presence of hydrogen and nitrogen.
By contrast, the seemingly isolated blue nebula at lower left (NGC 2020) has been created by a solitary mammoth star 200,000 times brighter than our Sun. The blue gasÂ
was ejected by the star through a series of eruptive events during which it lost part of its outer envelope of material.
The image, taken by Hubbleâs Wide Field Camera 3, commemorates the Earth-orbiting observatoryâs 30 years in space.
European Southern Observatory and NASA image of the supernova remnant from SN1987A, in the Tarantula Nebula in the Large Magellanic Cloud.
Edited United States Navy image of the Milky Way, Large and Small Magellanic Cloud galaxies (along with a bright planet - either Jupiter or Mars) while in the Red Sea. Seen from the deck of the USS Jason Dunham. Processing variant.
Original caption: RED SEA (Aug. 1, 2018) The guided-missile destroyer USS Jason Dunham (DDG 109) transits the Red Sea at night during exercise Eagle Salute 18. Eagle Salute 18 is a surface exercise with the Egyptian Naval Force (ENF) conducted to enhance interoperability and war-fighting readiness, fortify military-to-military relationships and advance operational capabilities of all participating units. Jason Dunham is deployed to the U.S. 5th Fleet area of operations in support of naval operations to ensure maritime stability and security in the Central region, connecting the Mediterranean and the Pacific through the western Indian Ocean and three strategic choke points. (U.S. Navy photo by Senior Chief Intelligence Specialist Matt Bodenner/Released) 180801-N-PY230-4224
Las Cañas, Uruguay . Un bosquet d’arbres sur fond de Voie Lactée et Grand Nuage de Magellan
Las Cañas, Uruguay . Some trees with a background composed of the Milky Way and the Large Magellanic Cloud Grand Nuage de Magellan
EARTH & SKY Photo taken by Igor Hoogerwerf - Location: University of Canterbury Mt John Observatory, Lake Tekapo, New Zealand. For some stunning Earth & Sky time-lapse animations, please refer to Earth & Sky Limited Partnership on You Tube.
All group photos will be available to view and download for two months, after this time frame you may contact Earth & Sky with your photo request.
Edited European Southern Observatory image of a star-forming region in the Large Magellanic Cloud. Color/processing variant.
Original caption: This colourful new view shows the star-forming region LHA 120-N44 [1] in the Large Magellanic Cloud, a small satellite galaxy of the Milky Way. This picture combines the view in visible light from the MPG/ESO 2.2-metre telescope at ESO’s La Silla Observatory in Chile with images in infrared light and X-rays from orbiting satellite observatories. At the centre of this very rich region of gas, dust and young stars lies the star cluster NGC 1929. Its massive stars produce intense radiation, expel matter at high speeds as stellar winds, and race through their short but brilliant lives to explode as supernovae. The winds and supernova shock waves have carved out a huge cavity, called a superbubble, in the surrounding gas. Observations with NASA's Chandra X-ray Observatory (shown here in blue) reveal hot regions created by these winds and shocks, while infrared data from NASA's Spitzer Space Telescope (shown in red) outline where the dust and cooler gas are found. The visible-light view from the MPG/ESO 2.2-metre telescope (in yellow) completes the picture and shows the hot young stars themselves as well as the glowing clouds of gas and dust that surround them. Combining these different views of this dramatic region has allowed astronomers to solve a mystery: why are N44, and similar superbubbles, giving off such strong X-rays? The answer seems to be that there are two extra sources of bright X-ray emission: supernova shock waves striking the walls of the cavities, and hot material evaporating from the cavity walls. This X-ray emission from the edge of the superbubble shows up clearly in the picture. Links NASA’s Chandra X-ray Observatory NASA’s Spitzer Space Telescope Notes [1] The designation of this object indicates that it was included in the Catalogue of H-alpha emission stars and nebulae in the Magellanic Clouds, compiled and published in 1956 by American astronomer–astronaut Karl Henize (1926–1993). The letter “N” indicates that it is a nebula. The object is often called simply N44.
Edited European Southern Observatory image of a star forming region in the Large Magellanic Cloud. Color/processing variant.
Original caption: This dazzling region of newly-forming stars in the Large Magellanic Cloud (LMC) was captured by the Multi Unit Spectroscopic Explorer instrument on ESO’s Very Large Telescope. The relatively small amount of dust in the LMC and MUSE’s acute vision allowed intricate details of the region to be picked out in visible light.
EARTH & SKY Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
For tips on capturing your own images of the night sky click here.
For some stunning Earth & Sky time-lapse animations, please refer to MakiTKP on You Tube.
Spitzer Space Telescope image of the Tarantula Nebula in the Large Magellanic Cloud (a satellite galaxy to our own Milky Way Galaxy).
EARTH & SKY Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
For some stunning Earth & Sky time-lapse animations, please refer to MakiTKP on You Tube.
EARTH & SKY Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
Please refer to MakiTKP on You Tube for some stunning time-lapse animations.
EARTH & SKY Photo taken by Igor Hoogerwerf - Location: Mt John University Observatory, Lake Tekapo, New Zealand
For tips on capturing your own images of the night sky www.earthandskynz.com/window-to-the-universe/en/astrophot....
For some stunning Earth & Sky time-lapse animations, please refer to MakiTKP on You Tube.
Attention: Due to the overwhelmingly positive response we've had to our photo stream we’re having to pare down the amount of archived material we leave open to the public to make it easier for our valued guests to locate new images… As the “group photos” garner the most attention and appear most popular we’ll endeavor to keep access to these priceless pictures open for at least two months. Many kind thanks, Earth & Sky team.
EARTH & SKY Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
For some stunning Earth & Sky time-lapse animations, please refer to MakiTKP on You Tube.
Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
Please refer to MakiTKP on You Tube for some stunning time-lapse animations.
EARTH & SKY Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
For some stunning Earth & Sky time-lapse animations, please refer to MakiTKP on You Tube.
Hubble Space Telescope image of the Tarantula Nebula (30 Doradus) in the Large Magellanic Cloud. This is the infrared version of the image.
Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
Please refer to MakiTKP on You Tube for some stunning time-lapse animations.
Edited multi-observatory image (Hubble Space Telescope, Chandra Space Telescope, and ALMA) of the ring around the remnants of Supernova 1987A.
Original caption: Astronomers combined observations from three different observatories to produce this multiwavelength image of the remnants of SN 1987A. The red colour shows newly formed dust in the centre of the supernova remnant, taken at submillimeter wavelengths by the Atacama Large Millimeter/submillimeter Array (ALMA) telescope in Chile. The green represents the glow of visible light, captured by the NASA/ESA Hubble Space Telescope. The blue color reveals the hottest gas and is based on data from NASA’s Chandra X-Ray observatory. The green and blue hues reveal where the expanding shock wave from the explosion is colliding with a ring of material around the supernova. This ring was initially illuminated by the ultraviolet flash from the explosion, but over the past few years the ring material has brightened considerably as it collides with the expanding shock wave.
EARTH & SKY Photo taken by Maki Yanagimachi - Location: Lake Tekapo, New Zealand
For some stunning Earth & Sky time-lapse animations, please refer to MakiTKP on You Tube.
EARTH & SKY Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
For some stunning Earth & Sky time-lapse animations, please refer to MakiTKP on You Tube.
EARTH & SKY Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
Please refer to MakiTKP on You Tube for some stunning time-lapse animations.
EARTH & SKY Photo taken by David Weir - Location: Mt John University Observatory, Lake Tekapo, New Zealand
EARTH & SKY Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
For some stunning Earth & Sky time-lapse animations, please refer to MakiTKP on You Tube.
Edited Hubble Space Telescope image (released as part of Hubble's 30th anniversary celebrations) of two nebulae in the Large Magellanic Cloud. Inverted grayscale variant.
Original caption: This Hubble image shows how young, energetic, massive stars illuminate and sculpt their birthplace with powerful winds and searing ultraviolet radiation.
In this Hubble portrait, the giant red nebula (NGC 2014) and its smaller blue neighbor (NGC 2020) are part of a vast star-forming region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way, located 163,000 light-years away. The image is nicknamed the âCosmic Reef,â because it resembles an undersea world.
The sparkling centerpiece of NGC 2014 is a grouping of bright, hefty stars, each 10 to 20 times more massive than our Sun. The starsâ ultraviolet radiation heats the surrounding dense gas. The massive stars also unleash fierce winds of charged particles that blast away lower-density gas, forming the bubble-like structures seen on the right. The starsâ powerful stellar winds are pushing gas and dust to the denserÂ
left side of the nebula, where it is piling up, creating a series of dark ridges bathed in starlight. The blue areas in NGC 2014 reveal the glow of oxygen, heated to nearly 20,000 degrees Fahrenheit by the blast of ultraviolet light. The cooler, red gas indicates the presence of hydrogen and nitrogen.
By contrast, the seemingly isolated blue nebula at lower left (NGC 2020) has been created by a solitary mammoth star 200,000 times brighter than our Sun. The blue gasÂ
was ejected by the star through a series of eruptive events during which it lost part of its outer envelope of material.
The image, taken by Hubbleâs Wide Field Camera 3, commemorates the Earth-orbiting observatoryâs 30 years in space.
Edited United States Navy image of the Milky Way, Large and Small Magellanic Cloud galaxies (along with a bright planet - either Jupiter or Mars) while in the Red Sea. Seen from the deck of the USS Jason Dunham. Color/processing variant.
Original caption: RED SEA (Aug. 1, 2018) The guided-missile destroyer USS Jason Dunham (DDG 109) transits the Red Sea at night during exercise Eagle Salute 18. Eagle Salute 18 is a surface exercise with the Egyptian Naval Force (ENF) conducted to enhance interoperability and war-fighting readiness, fortify military-to-military relationships and advance operational capabilities of all participating units. Jason Dunham is deployed to the U.S. 5th Fleet area of operations in support of naval operations to ensure maritime stability and security in the Central region, connecting the Mediterranean and the Pacific through the western Indian Ocean and three strategic choke points. (U.S. Navy photo by Senior Chief Intelligence Specialist Matt Bodenner/Released) 180801-N-PY230-4224
Nikon D7100
Focal Length: 300mm
Optimize Image: Custom
Color Mode: Mode III (aRGB)
Long Exposure NR: Off
High ISO NR: On (Low)
2015/01/22 00:22:30.7
Exposure Mode: Manual
Latitude: S 33°37.01'(33°37'0.5")
White Balance: Auto
RAW (14-bit)
Metering Mode: Multi-Pattern
AF Mode: Manual
15 sec - F/4
Flash Sync Mode: Not Attached
Longitude: W 69°58.16'(69°58'9.8")
Azimuth: 205º (SSW)
Sharpening: Normal
Altitude: 2697 m
Lens: 100-300mm F/4D Sigma
Sensitivity: ISO 6400
Image Comment: (c) Gerard Prins (+56) 22758 7209
Edited United States Navy image of the Milky Way, Large and Small Magellanic Cloud galaxies (along with a bright planet - either Jupiter or Mars) while in the Red Sea. Seen from the deck of the USS Jason Dunham.
Original caption: RED SEA (Aug. 1, 2018) The guided-missile destroyer USS Jason Dunham (DDG 109) transits the Red Sea at night during exercise Eagle Salute 18. Eagle Salute 18 is a surface exercise with the Egyptian Naval Force (ENF) conducted to enhance interoperability and war-fighting readiness, fortify military-to-military relationships and advance operational capabilities of all participating units. Jason Dunham is deployed to the U.S. 5th Fleet area of operations in support of naval operations to ensure maritime stability and security in the Central region, connecting the Mediterranean and the Pacific through the western Indian Ocean and three strategic choke points. (U.S. Navy photo by Senior Chief Intelligence Specialist Matt Bodenner/Released) 180801-N-PY230-4224
The brightly glowing plumes seen in this image are reminiscent of an underwater scene, with turquoise-tinted currents and nebulous strands reaching out into the surroundings. However, this is no ocean. This image actually shows part of the Large Magellanic Cloud (LMC), a small nearby galaxy that orbits our galaxy, the Milky Way, and appears as a blurred blob in our skies. The NASA/ESA Hubble Space Telescope has peeked many times into this galaxy, releasing stunning images of the whirling clouds of gas and sparkling stars (opo9944a, heic1301, potw1408a). This image shows part of the Tarantula Nebula's outskirts. This famously beautiful nebula, located within the LMC, is a frequent target for Hubble (heic1206, heic1402). In most images of the LMC the colour is completely different to that seen here. This is because, in this new image, a different set of filters was used. The customary R filter, which selects the red light, was replaced by a filter letting through the near-infrared light. In traditional images, the hydrogen gas appears pink because it shines most brightly in the red. Here however, other less prominent emission lines dominate in the blue and green filters. This data is part of the Archival Pure Parallel Project (APPP), a project that gathered together and processed over 1000 images taken using Hubble’s Wide Field Planetary Camera 2, obtained in parallel with other Hubble instruments. Much of the data in the project could be used to study a wide range of astronomical topics, including gravitational lensing and cosmic shear, exploring distant star-forming galaxies, supplementing observations in other wavelength ranges with optical data, and examining star populations from stellar heavyweights all the way down to solar-mass stars. A version of this image was entered into the Hubble’s Hidden Treasures image processing competition by contestant Josh Barrington.
Photo taken by Maki Yanagimachi - Location: Mt John University Observatory, Lake Tekapo, New Zealand
Please refer to MakiTKP on You Tube for some stunning time-lapse animations.
EARTH & SKY Photo taken by Igor Hoogerwerf - Location: University of Canterbury Mt John Observatory, Lake Tekapo, New Zealand
For tips on capturing your own images of the night sky www.earthandskynz.com/window-to-the-universe/en/astrophot....
For some stunning Earth & Sky time-lapse animations, please refer to Earth&Sky Ltd on You Tube.
Attention: Due to the overwhelmingly positive response we've had to our photo stream we’re having to pare down the amount of archived material we leave open to the public to make it easier for our valued guests to locate new images… As the “group photos” garner the most attention and appear most popular we’ll endeavor to keep access to these priceless pictures open for at least two months. Many kind thanks, Earth & Sky team.