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Inflated pressure suit of the type used by U-2 and SR-71 pilots. It was also used for the first three shuttle missions. There was a very nice lady from NASA who explained the purpose of the golf ball retrofitted to the suit. If cockpit lost pressure and the suit inflated the lower part of the helmet would block the pilot's field of view. By yanking down on the golf ball (and strap) the pilot would lower the helmet.
And yes, that's a MiG in the background.
Telling NASA's Tales With Hollywood's Tools
Space Center Uses Pixar's Palette To Artfully Explain Scientific Data
By Michael S. Rosenwald
Washington Post Staff Writer
Monday, August 21, 2006; D01
[We are lucky to be working with world class data visualizers and animators. This article in the Washington Post is one of the best print stories I've seen on the folks who are on the front lines of translating our science and making it accessible to our many audiences.]
www.washingtonpost.com/wp-dyn/content/article/2006/08/20/... ( www.washingtonpost.com/wp-dyn/content/article/2006/08/20/... )
Every once in a while when a new movie with mind-blowing special effects or oh-my-gosh-it-looked-so-real animation opens, a nondescript office at NASA Goddard Space Center in Greenbelt will mysteriously empty of employees during matinee hours.
Before an investigation is launched into the whereabouts of these workers -- particularly, say, around last year's opening of "Star Wars: Episode III -- Revenge of the Sith" -- understand that they are not blowing off work. The absentee employees are animators, NASA staffers and contractors who use the same software Pixar Animation Studios uses to tell stories about talking cars to instead tell stories about the Earth. They just want to see what their counterparts in Hollywood have been up to.
There is the occasional did-you-see-that elbow nudge, but in their case it's about craft, not cinematic delight, said Horace Mitchell, project manager at the space center's scientific visualization studio. Mitchell is a NASA employee, but the studio is staffed primarily by animators working for Global Science & Technology Inc., a government contractor in Greenbelt. The company uses the Hollywood software, including Pixar's RenderMan and Autodesk Inc.'s Maya, to translate complicated data into animated movies that illustrate what is happening in and around Earth. The videos often end up on the evening news.
The crucial difference in NASA's use of the software is that Hollywood uses it to spin inspiring, happy-ending stories about love and courage and friendship and hope, while the animators in Greenbelt are often telling stories about bad things happening in the atmosphere, such as last year's hurricane season. In their chilling short film "27 Storms: Arlene to Zeta," set to Vincenzo Bellini's eerie music, viewers can watch the ocean heat up, helping fuel one storm after another -- thanks to the same Pixar software used in the upcoming version of "Charlotte's Web."
NASA oceanographer Gene Carl Feldman frequently collaborates with the Global Science studio. He studies the ocean from space.
"Visualization is that link between the flood of data coming down from space and the ability of the human mind to interpret it," Feldman said. "That's the crux of the story. Better than most other groups in the world, they are able to take this fire hose of data coming down and turn it into images -- visual animation -- that then allows the general public to see this data in ways their brains can interpret and study."
The Hollywoodization of NASA data is in part the result of Pixar's success in creating real-life worlds from fantasy stories. People have come to expect that even the most fantastical of ideas -- a talking, curmudgeonly Mr. Potato Head -- can look and feel exceedingly real. "They don't expect to see crudity," Mitchell said. "They expect to see sophistication because they see it everywhere. In order for us to tell the story, we have to be sophisticated about telling stories and we have to use sophisticated technology to tell them."
Pixar was spun off from George Lucas's film company, and its early days were spent selling animation software and hardware -- a way to pay the bills until computer technology caught up with the firm's vision of making the incredibly life-like films that it produces today.
Today, anyone can purchase versions of RenderMan online, for $995 to $3,500.
Global Science, a private company that employs about 250 people, is definitely not a movie studio. It was founded in 1991 by Chieh-san Cheng, a former employee of an aerospace and technology company with advanced degrees in technical management and meteorology. Global Science provides services in applied science and research, geospatial standards, engineering services, and information technology. The firm's contract with NASA is a small part of its business, contributing about $650,000 a year to about $45 million in revenue.
Global Science and Pixar know about each other, but interaction between the staffs is generally limited to animation conferences and trade shows. But the Global Science staff does feel a strong bond with Pixar, particularly when watching one of its movies.
Jim Williams, a Global Science animator, said, "I'll go into it thinking I'm going to look at the technical stuff and then I'll get completely sucked into the story."
This happened during Pixar's recent hit, "Cars."
"I'm watching it, I'm totally into the story, and they get to the end and they go into that stadium, and there's tens of thousands of cars in there and I drop out of the story and think, 'Wow, that must have been a pain in the butt to get that right.' And then I'm back into the story," he said.
The difference between the storylines is that Pixar is trying to get laughing cars right and Global Science is trying to get the atmosphere right. The way in which Global Science uses RenderMan is not easy. Here's one way of looking at it: This article has been typed on a word processor. The computer received the data -- in this case, they looked like letters -- and displayed them on a screen. The lines were long, containing dozens of words. Those words needed to appear in the newspaper, and to do that a graphic designer used another program to render and squeeze the words into narrow columns of newsprint, with black type, a font, and italics , and so forth so the words appear in the paper as they do now. That's essentially what RenderMan does for data -- whether it be information about Buzz Lightyear's appearance or atmospheric models of hurricanes. RenderMan is the mechanism by which data are translated. Another program, Maya, acts as the word processor.
Global Science translates scientific data this way. Recently, one of its animators sat behind a computer monitor in a dark room with an image that could have appeared as a backdrop in a Van Gogh painting. But it was a depiction of aerosols moving across the atmosphere, a way of illustrating air quality. Yellow represented dust, the green was sulfates produced by humans, the blue was sea salt. Altogether, it was sort of beautiful but apparently not good news for the atmosphere.
Like their Hollywood counterparts, the Global Science animators typically refer to their finished products as releases, but the scripts are composed of data and the script writers are some of the world's most brilliant scientists. The creative process generally works like this: A scientist or a public affairs officer will ask the animators to illustrate a concept or data set. It can be as simple as ocean temperatures or as complicated as a collection of satellite images. A discussion with the scientific team and public affairs officer ensues over the best way to illustrate the data, and the animators get to work.
Feldman, the NASA oceanographer, studies oceans from space because, as he said: "Oceans are really, really, really big and they change very, very quickly. You can't track that from a ship. What a satellite sees in a minute would take a ship a decade." Feldman is particularly interested in the relationship between the changing environment and ocean life, which he pursues by studying the first level of life in the ocean, or microscopic plants, through ocean color.
The only problem is that satellites collect a very large amount of complicated data. The visualization studio helps him make sense of it. Feldman has made animations of what happened to the ocean during the transition between El Niño and La Niña -- "it was the biggest phytoplankton bloom in the world ever observed," he said. He has animated Lake Michigan's microscopic plant blooms and a dust storm the size of Spain that blew across the ocean in the past few years. He has animated autumn in Boston, which roughly translates into, as he put it, "how life follows the sun."
If Cheng, chief executive of Global Science, has his way, NASA scientists wouldn't be the only people relying on his firm's handling of Hollywood software to explain complicated subjects. Cheng would like to use the software to better explain the human body to doctors. He said the company is finalizing plans for a medical-imaging division and is exploring the possibility of a partnership with Maryland universities.
"What we could do is use movie techniques to give the doctor and medical staff more dynamic and accurate images to make a diagnosis," he said.
© 2006 The Washington Post Company
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The first hint of what will become of our Sun was discovered inadvertently in 1764. At that time, Charles Messier was compiling a list of diffuse objects not to be confused with comets. The 27th object on Messier's list, now known as M27 or the Dumbbell Nebula, is a planetary nebula, the type of nebula our Sun will produce when nuclear fusion stops in its core. M27 is one of the brightest planetary nebulae on the sky, and can be seen toward the constellation of the Fox (Vulpecula) with binoculars. It takes light about 1000 years to reach us from M27, shown above in colors emitted by hydrogen and oxygen. Understanding the physics and significance of M27 was well beyond 18th century science. Even today, many things remain mysterious about bipolar planetary nebula like M27, including the physical mechanism that expels a low-mass star's gaseous outer-envelope, leaving an X-ray hot white dwarf. via NASA ift.tt/1tQjfJu
Spacecraft Rosetta continues to circle and map Comet Churyumov-Gerasimenko. Crossing the inner Solar System for ten years to reach the vicinity of the comet in 2014, the robotic spacecraft continues to image the unusual double-lobed comet nucleus. The featured image, taken one year ago, shows dust and gas escaping from the comet's nucleus. Although appearing bright here, the comet's surface reflects only about four percent of impinging visible light, making it as dark as coal. Comet 67P/Churyumov–Gerasimenko spans about four kilometers in length and has a surface gravity so low that an astronaut could jump off of it. With Rosetta in tow, Comet 67P passed its closest to the Sun last year and is now headed back to the furthest point -- just past the orbit of Jupiter. via NASA ift.tt/1RXUbjl
NASA astronauts Jessica Watkins, left, Kjell Lindgren, center, and Robert Hines, right, answer questions from students during an event at the Martin Luther King Jr Memorial Library, Thursday, March 30, 2023, in Washington. Lindgren, Hines, and Watkins spent 170 days in space as part of Expeditions 67 and 68 aboard the International Space Station. Photo Credit: (NASA/Keegan Barber)
NASA released a Blue Marble image of the earth using recent satelite images.
They explain how they create it here but the planet images that I'm used to usually have a description such as, "stereographic projection of this equirectangular panorama".
So I thought I would provide the accompanying source equirectangular image that their stereographic projection was made from.
Based on an idea from lrargerich.
This image of the northwest corner of Australia was snapped by a student on Earth after remotely controlling the Sally Ride EarthKAM aboard the International Space Station. The program allows students to request photographs of specific Earth features, which are taken by a special camera mounted on the station when it passes over these features. via NASA ift.tt/1S95YrK
On Nov. 2, 2000, the Expedition 1 crew - Commander William M. (Bill) Shepherd of NASA and Flight Engineer Sergei Krikalev and Soyuz Commander Yuri Gidzenko of Roscosmos - arrived at the International Space Station, marking the start of an uninterrupted human presence on the orbiting laboratory. via NASA ift.tt/1RpwUTP
Cartoonist and professor of creativity Lynda Barry presented the benefits of creativity in everyday life as part of Goddard's Office of Communications Story Lab seminar series.
Read more: www.nasa.gov/feature/goddard/2016/cartoonist-discusses-cr...
Credit: NASA/Goddard/Rebecca Roth
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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A look at NASA's Global Hawk unmanned aircraft from one of the wings. The Global Hawk is sitting at the aircraft hangar of NASA's Wallops Flight Facility in Wallops Island, Va on Sept. 7, 2012.
Credit: NASA Wallops/Brea Reeves
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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Gravitational radiation has been directly detected. The first-ever detection was made by both facilities of the Laser Interferometer Gravitational-Wave Observatory (LIGO) in Washington and Louisiana simultaneously last September. After numerous consistency checks, the resulting 5-sigma discovery was published today. The measured gravitational waves match those expected from two large black holes merging after a death spiral in a distant galaxy, with the resulting new black hole momentarily vibrating in a rapid ringdown. A phenomenon predicted by Einstein, the historic discovery confirms a cornerstone of humanity's understanding of gravity and basic physics. It is also the most direct detection of black holes ever. The featured illustration depicts the two merging black holes with the signal strength of the two detectors over 0.3 seconds superimposed across the bottom. Expected future detections by Advanced LIGO and other gravitational wave detectors may not only confirm the spectacular nature of this measurement but hold tremendous promise of giving humanity a new way to see and explore our universe. via NASA ift.tt/20Xw6La
Eta Carinae may be about to explode. But no one knows when - it may be next year, it may be one million years from now. Eta Carinae's mass - about 100 times greater than our Sun - makes it an excellent candidate for a full blown supernova. Historical records do show that about 150 years ago Eta Carinae underwent an unusual outburst that made it one of the brightest stars in the southern sky. Eta Carinae, in the Keyhole Nebula, is the only star currently thought to emit natural LASER light. This featured image, taken in 1996, brought out new details in the unusual nebula that surrounds this rogue star. Now clearly visible are two distinct lobes, a hot central region, and strange radial streaks. The lobes are filled with lanes of gas and dust which absorb the blue and ultraviolet light emitted near the center. The streaks remain unexplained. via NASA ift.tt/1On0iH4
Sen. Barbara Mikulski participated in a ribbon cutting at NASA’s Goddard Space Flight Center on January 6th, 2016, to officially open the new Robotic Operations Center (ROC) developed by the Satellite Servicing Capabilities Office. Within the ROC's black walls, NASA is testing technologies and operational procedures for science and exploration missions, including the Restore-L satellite servicing mission and also the Asteroid Redirect Mission. During her tour of the ROC, Sen. Mikulski saw first-hand an early version of the NASA Servicing Arm, a 2-meter-class robot with the dexterity to grasp and refuel a satellite on orbit. She also heard a description of Raven, a payload launching to the International Space Station that will demonstrate real-time, relative space navigation technology. The robotic technologies that NASA is developing within the ROC also support the Journey to Mars.
Learn more about NASA’s satellite servicing technologies at ssco.gsfc.nasa.gov/.
Read more: www.nasa.gov/feature/goddard/2016/maryland-sen-barbara-mi...
Credit: NASA/Goddard/Chris Gunn
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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Sen. Barbara Mikulski participated in a ribbon cutting at NASA’s Goddard Space Flight Center on January 6th, 2016, to officially open the new Robotic Operations Center (ROC) developed by the Satellite Servicing Capabilities Office (SSCO). Within the ROC's black walls, NASA is testing technologies and operational procedures for science and exploration missions, including the Restore-L satellite servicing mission and also the Asteroid Redirect Mission.
During her tour of the ROC, Sen. Mikulski saw first-hand an early version of the NASA Servicing Arm (visible above, at right), a 2-meter-class robot with the dexterity to grasp and refuel a satellite on orbit. She also heard a description of Raven, a payload launching to the International Space Station that will demonstrate real-time, relative space navigation technology. The robotic technologies that NASA is developing within the ROC also support the Journey to Mars.
Learn more about NASA’s satellite servicing technologies at ssco.gsfc.nasa.gov/.
Image credit: NASA/Desiree Stover
Read more: www.nasa.gov/feature/goddard/2016/maryland-sen-barbara-mi...
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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A NASA Social participant asks a question to the astronauts onboard the International Space Station in a live downlink from the ISS at a NASA Social exploring science on the ISS at NASA Headquarters, Wednesday, Feb. 20, 2013 in Washington. Photo Credit: (NASA/Carla Cioffi)
Beautiful island universe Messier 94 lies a mere 15 million light-years distant in the northern constellation of the hunting dogs, Canes Venatici. A popular target for earth-based astronomers, the face-on spiral galaxy is about 30,000 light-years across, with spiral arms sweeping through the outskirts of its broad disk. But this Hubble Space Telescope field of view spans about 7,000 light-years or so across M94's central region. The sharp close-up examines the galaxy's compact, bright nucleus and prominent inner dust lanes, surrounded by a remarkable bluish ring of young, massive stars. The massive stars in the ring are all likely less than 10 million years old, indicating the galaxy experienced a well-defined era of rapid star formation. As a result, while the small, bright nucleus is typical of the Seyfert class of active galaxies, M94 is also known as a starburst galaxy. Because M94 is relatively nearby, astronomers can explore in detail reasons for the galaxy's burst of star formation. via NASA ift.tt/1PL9wS0
NASA's Earth observing satellite, Aqua, successfully launched at 2:55 a.m. PDT on ay 4, 2002. Aqua is dedicated to advancing our understanding of Earth's water cycle and our environment. Launching the Aqua spacecraft marks a major milestone in support of NASA's mission to help us better understand and protect our planet. The Aqua spacecraft lifted off from the Western Test Range of Vandenberg Air Force Base, Calif., aboard a Delta II rocket at 2:55 a.m. PDT. Spacecraft separation occurred at 3:54 a.m. PDT. inserting Aqua into a 438-mile (705-kilometer) orbit.
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About AIRS
The Atmospheric Infrared Sounder, AIRS, in conjunction with the Advanced Microwave Sounding Unit, AMSU, sense emitted infrared and microwave radiation from the Earth to provide a three-dimensional look at Earth's weather and climate. Working in tandem, the two instruments make simultaneous observations all the way down to the Earth's surface, even in the presence of heavy clouds. With more than 2,000 channels sensing different regions of the atmosphere, the system creates a global, 3-dimensional map of atmospheric temperature and humidity, cloud amounts and heights, greenhouse gas concentrations, and many other atmospheric phenomena. The AIRS and AMSU fly onboard NASA's Aqua spacecraft and are managed by the Jet Propulsion Laboratory, Pasadena, California, under contract to NASA. JPL is a division of the California Institute of Technology in Pasadena.
Credit
NASA
Download the image
Various sizes of the image are available, and there are two ways to download:
1) Right-click on the image. Click on a size next to "View all sizes".
2) Click on the "Actions" menu located above the image. Select "View all sizes".
Resources
Atmospheric Infrared Sounder web site ›
How to get the AIRS data
Do some surface features on Enceladus roll like a conveyor belt? A leading interpretation of images taken of Saturn's most explosive moon indicate that they do. This form of asymmetric tectonic activity, very unusual on Earth, likely holds clues to the internal structure of Enceladus, which may contain subsurface seas where life might be able to develop. Pictured above is a composite of 28 images taken by the robotic Cassini spacecraft in 2008 just after swooping by the ice-spewing orb. Inspection of these images show clear tectonic displacements where large portions of the surface all appear to move all in one direction. On the image right appears one of the most prominent tectonic divides: Labtayt Sulci, a canyon about one kilometer deep. The small magnitude of Enceladus' wobble as it orbits Saturn might indicate damping by a globally extending underground ocean layer. via NASA ift.tt/1iFN28I
NASA's New Horizons spacecraft captured this high-resolution enhanced color view of Charon just before closest approach on July 14, 2015. The image combines blue, red and infrared images taken by the spacecraft’s Ralph/Multispectral Visual Imaging Camera (MVIC); the colors are processed to best highlight the variation of surface properties. via NASA ift.tt/1JGKP1O
These are some images of Shuttle Atlantis as it was mated to the 747 at Edwards Air Force Base in California on May 31, 2009. This was prior to leaving Edwards on the morning of June 1 on the way to Biggs Army Air Field in El Paso, Texas.
Image credit: NASA
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NASA Armstrong Flight Research Center’s F-15D Eagle #897, flown by pilot Troy Asher with videographer Lori Losey in the back seat, serves as a chase vehicle for NASA's DC-8 flying laboratory on the Olympic Mountain Experiment (OLYMPEX) science mission, Nov. 10, 2015. via NASA ift.tt/1m8xewH
NASA's Earth observing satellite, Aqua, successfully launched at 2:55 a.m. PDT on ay 4, 2002. Aqua is dedicated to advancing our understanding of Earth's water cycle and our environment. Launching the Aqua spacecraft marks a major milestone in support of NASA's mission to help us better understand and protect our planet. The Aqua spacecraft lifted off from the Western Test Range of Vandenberg Air Force Base, Calif., aboard a Delta II rocket at 2:55 a.m. PDT. Spacecraft separation occurred at 3:54 a.m. PDT. inserting Aqua into a 438-mile (705-kilometer) orbit.
______________________________________________________________________
About AIRS
The Atmospheric Infrared Sounder, AIRS, in conjunction with the Advanced Microwave Sounding Unit, AMSU, sense emitted infrared and microwave radiation from the Earth to provide a three-dimensional look at Earth's weather and climate. Working in tandem, the two instruments make simultaneous observations all the way down to the Earth's surface, even in the presence of heavy clouds. With more than 2,000 channels sensing different regions of the atmosphere, the system creates a global, 3-dimensional map of atmospheric temperature and humidity, cloud amounts and heights, greenhouse gas concentrations, and many other atmospheric phenomena. The AIRS and AMSU fly onboard NASA's Aqua spacecraft and are managed by the Jet Propulsion Laboratory, Pasadena, California, under contract to NASA. JPL is a division of the California Institute of Technology in Pasadena.
Credit
NASA
Download the image
Various sizes of the image are available, and there are two ways to download:
1) Right-click on the image. Click on a size next to "View all sizes".
2) Click on the "Actions" menu located above the image. Select "View all sizes".
Resources
Atmospheric Infrared Sounder web site ›
How to get the AIRS data
Expedition 46 flight engineer Tim Peake of ESA captured this photo on Jan. 29, 2016 from the International Space Station, as the robotic arm in Japan's Kibo laboratory successfully deployed two combined satellites: AggieSat4 built by Texas A&M University students, and BEVO-2 built by University of Texas students. via NASA ift.tt/1PdBVNe
NASA's New Horizons spacecraft captured this high-resolution enhanced color view of Charon just before closest approach on July 14, 2015. The image combines blue, red and infrared images taken by the spacecraft’s Ralph/Multispectral Visual Imaging Camera (MVIC); the colors are processed to best highlight the variation of surface properties. via NASA ift.tt/1JGKP1O
NASA's Hubble Space Telescope presents a festive holiday greeting that's out of this world. The bipolar star-forming region, called Sharpless 2-106, looks like a soaring, celestial snow angel. The outstretched "wings" of the nebula record the contrasting imprint of heat and motion against the backdrop of a colder medium.
Sharpless 2-106, Sh2-106 or S106 for short, lies nearly 2,000 light-years from us. The nebula measures several light-years in length. It appears in a relatively isolated region of the Milky Way galaxy.
A massive, young star, IRS 4 (Infrared Source 4), is responsible for the furious activity we see in the nebula. Twin lobes of super-hot gas, glowing blue in this image, stretch outward from the central star. This hot gas creates the "wings" of our angel.
Credit: NASA, ESA, the Hubble Heritage Team, (STScI/AURA)
Engineers and technicians moved the Orion service module test article into the Reverberant Acoustic Test Facility at NASA Glenn Research Center’s Plum Brook Station in Sandusky, Ohio on Friday, April 8. Acoustic testing is scheduled to begin April 18. The blue structure sitting on top of the test article is a mass simulator that represents the Orion crew module.
The test article will be blasted with at least 152 decibels and 20-10,000 hertz of sound pressure and vibration to simulate the intense sounds the Orion service module will be subjected to during launch and ascent into space atop the agency’s Space Launch System (SLS) rocket. This is part of a series of tests to verify the structural integrity of Orion’s service module for Exploration Mission-1, the spacecraft’s first flight atop SLS.
Provided by ESA (European Space Agency) and built by Airbus Defence and Space, the service module will power, propel and cool the vehicle and also supply it with air and water.
Photo credit: NASA
Rami Daud (Alcyon Technical Services JV, LLC)