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NASA's green aviation project is one step closer to developing technology that could make future airliners quieter and more fuel-efficient with the successful flight test of a wing surface that can change shape in flight. This past summer, researchers replaced an airplane’s conventional aluminum flaps with advanced, shape-changing assemblies that form seamless bendable and twistable surfaces. Flight testing will determine whether flexible trailing-edge wing flaps are a viable approach to improve aerodynamic efficiency and reduce noise generated during takeoffs and landings. For the initial Adaptive Compliant Trailing Edge (ACTE) flight, shown in this image, the experimental control surfaces were locked at a specified setting. Varied flap settings on subsequent tests will demonstrate the capability of the flexible surfaces under actual flight conditions. ACTE technology is expected to have far-reaching effects on future aviation. Advanced lightweight materials will reduce wing structural weight and give engineers the ability to aerodynamically tailor the wings to promote improved fuel economy and more efficient operations, while reducing environmental impacts. > More: NASA Tests Revolutionary Shape Changing Aircraft Flap for the First Time Image Credit: NASA/Ken Ulbrich via NASA ift.tt/1u6aVU8

via NASA Earth Observatory Image of the Day ift.tt/2HF8gAg

NASA trip STEM students, March 24, 2018

can the shuttle take off without the pilot??

laughingsquid.com/nasa-launch-of-space-shuttle-sts-129/

 

photo by Scott Beale / Laughing Squid

 

This photo is licensed under a Creative Commons license. If you use this photo within the terms of the license or make special arrangements to use the photo, please list the photo credit as "Scott Beale / Laughing Squid" and link the credit to laughingsquid.com.

Shots from Iceland Airwaves 2011 festival in october. Damn this was fun!

  

Canon 1Ds Mark III / Canon 16-35mm F/2.8L

  

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What are those colorful rings around the Moon? A corona. Rings like this will sometimes appear when the Moon is seen through thin clouds. The effect is created by the quantum mechanical diffraction of light around individual, similarly-sized water droplets in an intervening but mostly-transparent cloud. Since light of different colors has different wavelengths, each color diffracts differently. Lunar Coronae are one of the few quantum mechanical color effects that can be easily seen with the unaided eye. The featured lunar corona was captured around a Strawberry Moon on June 2 from La Plata, Argentina. Similar coronae that form around the Sun are typically harder to see because of the Sun's great brightness. via NASA ift.tt/1IF9Pt1

What I believe was the Communications or Telemetry Room

On June 21, 2020, as the International Space Station orbited over Kazakhstan and into China, an external high-definition camera captures this picture of the solar eclipse shadowing a portion of the Asian continent. via NASA June 24, 2020

Took at NASA JPL, Pasadena, California, June 2010

Wandering around Google Mars! Everyone should try it,

Families lined up to play the R2 game and learn about NASA

Looking Westward, across one modern-era (my guess: 1980s) antenna tower foundation at the large, modern-era antenna tower.

'NASA 926' is one of two highly modified WB-57F Canberras usually operated by NASA for high altitude sampling and testing. One of the aircraft has infrequently deployed to RAF Miidenhall in previous years for this task. This is the first time I have seen 926, most recent visits have been conducted by 928.

Flag flown at Half-Mast above the Mission Control Center in Houston, Texas.

(image: NASA/CXC/UC Berkeley/N.Smith et al.)

News Top Stories: May 7, 2007 -- A massive exploding faraway star -- Shield Your Eyes: A Wild Orbit -- This artist's illustration gives life to observations made by NASA's Chandra X-ray Observatory and ground-based optical telescopes. Supernova SN 2006gy is the brightest and most energetic stellar explosion ever recorded, and may be a long-sought new type of explosion.

Taking part in the Safari 2000 project in Pietersburg, South Africa

 

SAFARI 2000 – Pietersberg, 2000

 

The Southern African Regional Science Initiative (SAFARI 2000) project was an international science initiative to study the linkages between land and atmosphere processes conducted from 1999-2001 in the southern African region. In addition, SAFARI 2000 examined the relationship of biogenic, pyrogenic, and anthropogenic emissions and the consequences of their deposition to the functioning of the biogeophysical and biogeochemical systems of southern Africa.

 

During September 2000 NASA flew an ER-2 out of Polokwane, also known as Pietersburg. The ER2 carried a number of imaging instruments and was accompanied by low level in situ measurements conducted from a University of Washington C-580. Flying took place over South Africa, Namibia, Botswana, Mozambique and Zambia. The project was supported and supplied by a USAF C-141 and K -135 from March AFB. The single seater ER-2 flew across the Atlantic from Recife Brazil.

   

daac.ornl.gov/cgi-bin/dataset_lister.pl?p=18

  

All Photos: Courtesy of Frank Eckardt

Stairs leading up to the RADAR antenna platform. Now exposed to the elements, the RADAR antenna & this area would have been enclosed by the 51' diameter radome.

September 7-9 Nasa GRAIL launch Tweetup

A few pix from our third Science Live show focused on Earth Science and Earth Day.

This self-portrait of NASA's Curiosity Mars rover shows the vehicle at the "Mojave" site, where its drill collected the mission's second taste of Mount Sharp. The scene combines dozens of images taken during January 2015 by the Mars Hand Lens Imager (MAHLI) camera at the end of the rover's robotic arm. The pale "Pahrump Hills" outcrop surrounds the rover, and the upper portion of Mount Sharp is visible on the horizon. Darker ground at upper right and lower left holds ripples of wind-blown sand and dust. An annotated version, Fig. A, labels several of the sites Curiosity has investigated during three passes up the Pahrump Hills outcrop examining the outcrop at increasing levels of detail. The rover used its sample-collecting drill at "Confidence Hills" as well as at Mojave, and in late February was assessing "Telegraph Peak" as a third drilling site. The view does not include the rover's robotic arm. Wrist motions and turret rotations on the arm allowed MAHLI to acquire the mosaic's component images. The arm was positioned out of the shot in the images, or portions of images, that were used in this mosaic. This process was used previously in acquiring and assembling Curiosity self-portraits taken at sample-collection sites "Rock Nest" (ift.tt/12SNjYb), "John Klein" (ift.tt/1iFLQAx) and "Windjana" (ift.tt/1vwpWGg). Curiosity used its drill to collect a sample of rock powder from target "Mojave 2" at this site on Jan. 31, 2015. The full-depth, sample-collection hole and the shallower preparation test hole beside it are visible in front of the rover in this self-portrait, and in more detail at ift.tt/1DDxW7C . The Mojave site is in the "Pink Cliffs" portion of the Pahrump Hills outcrop. The outcrop is an exposure of the Murray formation, which forms the basal geological layer of Mount Sharp. Views of Pahrump Hills from other angles are at ift.tt/13Erb9G and the inset at ift.tt/1EO3HMa . The frames showing the rover in this mosaic were taken during the 868th Martian day, or sol, of Curiosity's work on Mars (Jan. 14, 2015). Additional frames around the edges to extend the amount of terrain included in the scene were taken on Sol 882 (Jan. 29, 2015). The frames showing the drill holes were taken on Sol 884 (Jan. 31, 2015). For scale, the rover's wheels are 20 inches (50 centimeters) in diameter and about 16 inches (40 centimeters) wide. The drilled holes in the rock are 0.63 inch (1.6 centimeters) in diameter. MAHLI was built by Malin Space Science Systems, San Diego. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Science Laboratory Project for the NASA Science Mission Directorate, Washington. JPL designed and built the project's Curiosity rover. More information about Curiosity is online at www.nasa.gov/msl and ift.tt/wIaLrq. Credit: NASA/JPL-Caltech/MSSS via NASA ift.tt/1EO3EQg

"TELEPHONE TERMINAL BOARD"

Me and my boys saying "see ya!" to ye olde NASA sign.

 

c/w www.flickr.com/photos/found_drama/8560159897/

NASA image acquired November 9, 2012

 

In early November 2012, a wintery nor’easter followed on the heels of Hurricane Sandy. When that second storm cleared out of the region, it left behind snow stretching from New Jersey to Massachusetts. The Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA’s Aqua satellite captured this natural-color view of the region on November 9, 2012.

 

The National Weather Service’s Philadelphia / Mt. Holly (N.J.) forecast office reported that snowfall from the storm was “considerably worse than forecast for portions of northern and central New Jersey,” but less than forecast in other areas.

 

From the vantage point of MODIS, snowfall was the visible impact of the storm. But the areas blanketed in white were not the only ones affected by the storm. The National Weather Service also observed wind gusts up to 65 miles (105 kilometers) per hour; high waves and minor coastal flooding in New Jersey and Delaware; and 1.5 inches (4 centimeters) of rain along the New Jersey coast. Similar conditions were reported in coastal New England.

 

The nor’easter hit areas already struggling in the aftermath of Hurricane Sandy, including those suffering through ongoing power outages. The Associated Press reported that tens of thousands of customers in New York and New Jersey remained without electricity two weeks after Sandy’s landfall.

 

NASA image courtesy Jeff Schmaltz, LANCE MODIS Rapid Response Team at NASA GSFC. Caption by Michon Scott.

 

Instrument:

Aqua - MODIS

 

Credit: NASA Earth Observatory

 

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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Why does the Sombrero Galaxy look like a hat? Reasons include the Sombrero's unusually large and extended central bulge of stars, and dark prominent dust lanes that appear in a disk that we see nearly edge-on. Billions of old stars cause the diffuse glow of the extended central bulge. Close inspection of the bulge in the above photograph shows many points of light that are actually globular clusters. M104's spectacular dust rings harbor many younger and brighter stars, and show intricate details astronomers don't yet fully understand. The very center of the Sombrero glows across the electromagnetic spectrum, and is thought to house a large black hole. Fifty million-year-old light from the Sombrero Galaxy can be seen with a small telescope towards the constellation of Virgo. via NASA ift.tt/1GPP4Xq

Have you ever seen the Summer Triangle? The bright stars Vega, Deneb, and Altair form a large triangle on the sky that can be seen rising in the northern spring during the morning, and rising in the northern fall during the evening. During summer months, the triangle can be found nearly overhead near midnight as three of the brightest stars on the sky. Featured here, along with the arch of the central band of our Milky Way Galaxy, the Summer Triangle asterism was captured this spring over the Great Wall of China. This part of the Great Wall, a World Culture Heritage Site, was built during the 6th century on the Yan Mountains. At the summit is Wangjinglou Tower from which, on a clear night, the lights of Beijing are visible in the distance. via NASA ift.tt/2udOcP0

UPI Photog Bill Cantrell at STS 133 landing

On July 26, 2014, from 10:57 a.m. to 11:42 a.m. EDT, the moon crossed between NASA’s Solar Dynamics Observatory (SDO) and the sun, a phenomenon called a lunar transit. A lunar transit happens approximately twice a year, causing a partial solar eclipse that can only be seen from SDO's point of view. Images of the eclipse show a crisp lunar horizon, because the moon has no atmosphere that would distort light. This image shows the blended result of two SDO wavelengths - one in 304 wavelength and another in 171 wavelength. Image Credit: NASA/SDO via NASA 1.usa.gov/1yHsjaB

Part of the NASA Dryden facility.

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