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Images of Ames Research Center (ARC) and California
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Earth Resources Project
Ames Earth Resources project
3/23/09
| Description |
Ames Earth Resources project U-2 aircraft shot this oblique image off the coast of California, USA in 1972. The Golden Gate is in the foreground. As the image looks out across California the blue spot at the top enter is Lake Tahoe in the Sierra Nevada. Photo Credit: NASA Ames Research Center |
| Date |
3/23/09 |
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California Governor Visits N
Gov. Arnold Schwarzenegger v
7/17/08
| Title |
California Governor Visits NASA Ames Research Center |
| Date |
7/17/08 |
| Description |
Gov. Arnold Schwarzenegger visited NASA's Ames Research Center July 17 to see first-hand how the agency is helping firefighters battle the widespread wildfires raging throughout the state. |
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Ikhana
NASA Aircraft Aiding Souther
7/9/08
| Description |
NASA Aircraft Aiding Southern California Firefighting EffortRelease: 07-57 In response to a request from the California Office of Emergency Services and the National Interagency Fire Center, NASA is flying an aircraft equipped with sophisticated infrared imaging equipment today to assist firefighters battling several of the Southern California wildfires. The Ikhana unmanned aircraft system, a Predator B modified for civil science and research missions, was launched about 8:45 a.m. PDT from its base at NASA's Dryden Flight Research Center at Edwards Air Force Base. It is expected to fly over the major blazes burning in the Lake Arrowhead and Running Springs areas and possibly down into San Diego County to image wildfires raging in that area. The aircraft is controlled remotely by pilots in a ground control station at NASA Dryden. The Ikhana is carrying the Autonomous Modular Scanner, a thermal-infrared imaging system developed at NASA's Ames Research Center in Northern California. The system is capable of peering through heavy smoke and darkness to see hot spots, flames and temperature differences, processing the imagery on-board, and then transmitting that information in near real time so it can aid fire incident commanders in allocating their firefighting resources...Read more Photo Description: With smoke from the Lake Arrowhead, CA area fires streaming in the background, NASA's Ikhana unmanned aircraft heads out on a wildfire imaging mission. October 24, 2007 NASA Photo / Jim Ross ED07-0243-37 |
| Date |
7/9/08 |
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Our Chaotic Neighbor
| Title |
Our Chaotic Neighbor |
| Description |
This vibrant image from NASA's Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. The infrared image, a mosaic of more than 100,000 individual tiles, offers astronomers a unique chance to study the lifecycle of stars and dust in a single galaxy. Nearly one million objects are revealed for the first time in this Spitzer view, which represents about a 1,000-fold improvement in sensitivity over previous space-based missions. Most of the new objects are dusty stars of various ages populating the Large Magellanic Cloud, the rest are thought to be background galaxies. The blue color in the picture, seen most prominently in the central bar, represents starlight from older stars. The chaotic, bright regions outside this bar are filled with hot, massive stars buried in thick blankets of dust. The red clouds contain cooler interstellar gas and molecular-sized dust grains illuminated by ambient starlight. The Large Magellanic Cloud, located 160,000 light-years from Earth, is one of a handful of dwarf galaxies that orbit our own Milky Way. It is approximately one-third as wide as the Milky Way, and, if it could be seen in its entirety, would cover the same amount of sky as a grid of about 480 full moons. About one-third of the whole galaxy can be seen in the Spitzer image. This picture is a composite of infrared light captured by Spitzer's infrared array camera. Light with wavelengths of 8 and 5.8 microns is red and orange: 4.5-micron light is green, and 3.6-micron light is blue. |
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Our Chaotic Neighbor
| Title |
Our Chaotic Neighbor |
| Description |
This vibrant image from NASA's Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. The infrared image, a mosaic of more than 100,000 individual tiles, offers astronomers a unique chance to study the lifecycle of stars and dust in a single galaxy. Nearly one million objects are revealed for the first time in this Spitzer view, which represents about a 1,000-fold improvement in sensitivity over previous space-based missions. Most of the new objects are dusty stars of various ages populating the Large Magellanic Cloud, the rest are thought to be background galaxies. The blue color in the picture, seen most prominently in the central bar, represents starlight from older stars. The chaotic, bright regions outside this bar are filled with hot, massive stars buried in thick blankets of dust. The red clouds contain cooler interstellar gas and molecular-sized dust grains illuminated by ambient starlight. The Large Magellanic Cloud, located 160,000 light-years from Earth, is one of a handful of dwarf galaxies that orbit our own Milky Way. It is approximately one-third as wide as the Milky Way, and, if it could be seen in its entirety, would cover the same amount of sky as a grid of about 480 full moons. About one-third of the whole galaxy can be seen in the Spitzer image. This picture is a composite of infrared light captured by Spitzer's infrared array camera. Light with wavelengths of 8 and 5.8 microns is red and orange: 4.5-micron light is green, and 3.6-micron light is blue. |
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Our Chaotic Neighbor
| Title |
Our Chaotic Neighbor |
| Description |
This vibrant image from NASA's Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. The infrared image, a mosaic of more than 100,000 individual tiles, offers astronomers a unique chance to study the lifecycle of stars and dust in a single galaxy. Nearly one million objects are revealed for the first time in this Spitzer view, which represents about a 1,000-fold improvement in sensitivity over previous space-based missions. Most of the new objects are dusty stars of various ages populating the Large Magellanic Cloud, the rest are thought to be background galaxies. The blue color in the picture, seen most prominently in the central bar, represents starlight from older stars. The chaotic, bright regions outside this bar are filled with hot, massive stars buried in thick blankets of dust. The red clouds contain cooler interstellar gas and molecular-sized dust grains illuminated by ambient starlight. The Large Magellanic Cloud, located 160,000 light-years from Earth, is one of a handful of dwarf galaxies that orbit our own Milky Way. It is approximately one-third as wide as the Milky Way, and, if it could be seen in its entirety, would cover the same amount of sky as a grid of about 480 full moons. About one-third of the whole galaxy can be seen in the Spitzer image. This picture is a composite of infrared light captured by Spitzer's infrared array camera. Light with wavelengths of 8 and 5.8 microns is red and orange: 4.5-micron light is green, and 3.6-micron light is blue. |
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What's Old Is New in the Lar
| Title |
What's Old Is New in the Large Magellanic Cloud |
| Description |
This vibrant image from NASA's Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. The infrared image, a mosaic of 300,000 individual tiles, offers astronomers a unique chance to study the lifecycle of stars and dust in a single galaxy. Nearly one million objects are revealed for the first time in this Spitzer view, which represents about a 1,000-fold improvement in sensitivity over previous space-based missions. Most of the new objects are dusty stars of various ages populating the Large Magellanic Cloud, the rest are thought to be background galaxies. The blue color in the picture, seen most prominently in the central bar, represents starlight from older stars. The chaotic, bright regions outside this bar are filled with hot, massive stars buried in thick blankets of dust. The red color around these bright regions is from dust heated by stars, while the red dots scattered throughout the picture are either dusty, old stars or more distant galaxies. The greenish clouds contain cooler interstellar gas and molecular-sized dust grains illuminated by ambient starlight. Astronomers say this image allows them to quantify the process by which space dust ? the same stuff that makes up planets and even people ? is recycled in a galaxy. The picture shows dust at its three main cosmic hangouts: around the young stars, where it is being consumed (red-tinted, bright clouds), scattered about in the space between stars (greenish clouds), and in expelled shells of material from old stars (randomly-spaced red dots). The Large Magellanic Cloud, located 160,000 light-years from Earth, is one of a handful of dwarf galaxies that orbit our own Milky Way. It is approximately one-third as wide as the Milky Way, and, if it could be seen in its entirety, would cover the same amount of sky as a grid of about 480 full moons. About one-third of the entire galaxy can be seen in the Spitzer image. This picture is a composite of infrared light captured by Spitzer. Light with wavelengths of 3.6 (blue) and 8 (green) microns was captured by the telescope's infrared array camera, 24-micron light (red) was detected by the multiband imaging photometer. |
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What's Old Is New in the Lar
| Title |
What's Old Is New in the Large Magellanic Cloud |
| Description |
This vibrant image from NASA's Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. The infrared image, a mosaic of 300,000 individual tiles, offers astronomers a unique chance to study the lifecycle of stars and dust in a single galaxy. Nearly one million objects are revealed for the first time in this Spitzer view, which represents about a 1,000-fold improvement in sensitivity over previous space-based missions. Most of the new objects are dusty stars of various ages populating the Large Magellanic Cloud, the rest are thought to be background galaxies. The blue color in the picture, seen most prominently in the central bar, represents starlight from older stars. The chaotic, bright regions outside this bar are filled with hot, massive stars buried in thick blankets of dust. The red color around these bright regions is from dust heated by stars, while the red dots scattered throughout the picture are either dusty, old stars or more distant galaxies. The greenish clouds contain cooler interstellar gas and molecular-sized dust grains illuminated by ambient starlight. Astronomers say this image allows them to quantify the process by which space dust ? the same stuff that makes up planets and even people ? is recycled in a galaxy. The picture shows dust at its three main cosmic hangouts: around the young stars, where it is being consumed (red-tinted, bright clouds), scattered about in the space between stars (greenish clouds), and in expelled shells of material from old stars (randomly-spaced red dots). The Large Magellanic Cloud, located 160,000 light-years from Earth, is one of a handful of dwarf galaxies that orbit our own Milky Way. It is approximately one-third as wide as the Milky Way, and, if it could be seen in its entirety, would cover the same amount of sky as a grid of about 480 full moons. About one-third of the entire galaxy can be seen in the Spitzer image. This picture is a composite of infrared light captured by Spitzer. Light with wavelengths of 3.6 (blue) and 8 (green) microns was captured by the telescope's infrared array camera, 24-micron light (red) was detected by the multiband imaging photometer. |
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What's Old Is New in the Lar
| Title |
What's Old Is New in the Large Magellanic Cloud |
| Description |
This vibrant image from NASA's Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. The infrared image, a mosaic of 300,000 individual tiles, offers astronomers a unique chance to study the lifecycle of stars and dust in a single galaxy. Nearly one million objects are revealed for the first time in this Spitzer view, which represents about a 1,000-fold improvement in sensitivity over previous space-based missions. Most of the new objects are dusty stars of various ages populating the Large Magellanic Cloud, the rest are thought to be background galaxies. The blue color in the picture, seen most prominently in the central bar, represents starlight from older stars. The chaotic, bright regions outside this bar are filled with hot, massive stars buried in thick blankets of dust. The red color around these bright regions is from dust heated by stars, while the red dots scattered throughout the picture are either dusty, old stars or more distant galaxies. The greenish clouds contain cooler interstellar gas and molecular-sized dust grains illuminated by ambient starlight. Astronomers say this image allows them to quantify the process by which space dust ? the same stuff that makes up planets and even people ? is recycled in a galaxy. The picture shows dust at its three main cosmic hangouts: around the young stars, where it is being consumed (red-tinted, bright clouds), scattered about in the space between stars (greenish clouds), and in expelled shells of material from old stars (randomly-spaced red dots). The Large Magellanic Cloud, located 160,000 light-years from Earth, is one of a handful of dwarf galaxies that orbit our own Milky Way. It is approximately one-third as wide as the Milky Way, and, if it could be seen in its entirety, would cover the same amount of sky as a grid of about 480 full moons. About one-third of the entire galaxy can be seen in the Spitzer image. This picture is a composite of infrared light captured by Spitzer. Light with wavelengths of 3.6 (blue) and 8 (green) microns was captured by the telescope's infrared array camera, 24-micron light (red) was detected by the multiband imaging photometer. |
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NASA TV's This Week @NASA, J
More than 250 students joine
06/11/10
| Description |
More than 250 students joined with astronaut Leland Melvin and Administrator Charles Bolden at the Jet Propulsion Laboratory to help kickoff NASA's Summer of Innovation.* The launch nears for Expedition 24's three new members. Cosmonaut Fyodor Yurchikhin, and NASA astronauts Dough Wheelock and Shannon Walker are slated to liftoff on a Soyuz rocket for the International Space Station on Tuesday, June 15.* The Langley Research Center has broken ground on a new facility dedicated to bringing astronauts home safely from space. * The Marshall Space Flight Center honored the ''best of the best'' during its Honor Awards ceremony. *NASA's second Global Hawk Earth sciences aircraft has completed its first checkout flight. * The California School for the Blind is among six schools in the San Francisco Bay Area that've hosted “Space Dayâ€ activities including a Traveling Space Museum from the Ames Research Center. * The Ames Research Center turned the spotlight on NASA's collaborative “Smart Skiesâ€ project by showcasing the curriculum's software at a kick-off media event.* |
| Date |
06/11/10 |
|
NASA TV's This Week at NASA,
The new members of the Exped
04/02/10
| Description |
The new members of the Expedition 23 crew began their journey to the International Space Station with a successful launch from the Baikonur Cosmodrome in Kazakhstan. Soyuz Commander Alexander Skvortsov, Flight Engineers Mikhail Kornienko and Tracy Caldwell Dyson will spend the next six months aboard the orbiting complex. * The new members of the Expedition 23 crew began their journey to the International Space Station with a successful launch from the Baikonur Cosmodrome in Kazakhstan. Soyuz Commander Alexander Skvortsov, Flight Engineers Mikhail Kornienko and Tracy Caldwell Dyson will spend the next six months aboard the orbiting complex. * Soon on their way to the ISS are the members of the STS-131 crew, they√¢re scheduled to liftoff with space shuttle Discovery from the Kennedy Space Center on Monday at 6:21 a.m. EDT. * Students, educators, scientists and the public came together at the Pasadena Convention Center for Climate Day 2010 -- a fun-filled educational event about Earth√¢s changing climate. * Dozens of teachers are conducting real science in an extreme environment. Through Ames Research Center's Spaceward Bound project, NASA has sent teachers to California State University's Desert Study Center in Zzyzx. |
| Date |
04/02/10 |
|
Pioneer 10 Construction
| title |
Pioneer 10 Construction |
| date |
12.20.1971 |
| description |
Pioneer 10 in the final stage of construction in at the TRW plant in Southern California. *Image Credit*: NASA Ames Research Center |
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Impact Studies
| title |
Impact Studies |
| description |
The photo shows the "energy flash" when a projectile launched at speeds up to 17,000 mph impacts a solid surface at the Hypervelocity Ballistic Range at NASA's Ames Research Center, Mountain View, California. This test is used to simulate what happens when a piece of orbital debris hits a spacecraft in orbit. *Image Credit*: NASA |
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High-Speed Impact
| title |
High-Speed Impact |
| date |
01.01.1963 |
| description |
The photo shows the "energy flash" when a projectile launched at speeds up to 17,000 mph impacts a solid surface at the Hypervelocity Ballistic Range at NASA's Ames Research Center, Mountain View, California. This test is used to simulate what happens when a piece of orbital debris hits a spacecraft in orbit. *Image Credit*: NASA |
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Leonid Meteor Train
| title |
Leonid Meteor Train |
| date |
11.18.1995 |
| description |
This gradually changing persistent train of a bright Leonid was photographed over California by Peter Jenniskens at the San Luis Reservoir on November 18, 1995. The meteor appeared at 11:45:22 Universal Time (UT). A persistent train was visible with the naked eye for six minutes. The train was photographed in a series of one-minute exposures starting at 11:45:59, 11:46:59, 11:47:59, 11:49:06, 11:50:05, and 11:51:06 UT. The inset shows the same meteor from a different observing site in an image by Mike Koop at Henry Coe State Park. *Image Credit*: Mike Koop (California Meteor Society), Peter Jenniskens (NASA Ames Research Center) |
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40 x 80 Foot Data Acquisitio
| Title |
40 x 80 Foot Data Acquisition System |
| Full Description |
The 40 x 80 Foot Data Acquisition System at the Ames Research Center, Mountain View, California. |
| Date |
02/16/1990 |
| NASA Center |
Ames Research Center |
|
M-1 Model in Hypersonic Tunn
| Title |
M-1 Model in Hypersonic Tunnel |
| Full Description |
An engineer mounts a model of the M-1 Lifting Body in the throat of the 3.5 Foot Hypersonic Tunnel at the Nasa Ames Research Center, Mountain View, California. |
| Date |
01/01/1964 |
| NASA Center |
Ames Research Center |
|
Aerial View of Ames Wind Tun
| Title |
Aerial View of Ames Wind Tunnels |
| Full Description |
An aerial view of the NACA Ames Aeronautical Laboratory, Moffett Field, California. |
| Date |
02/11/1947 |
| NASA Center |
Ames Research Center |
|
Mapping out the Neural Netwo
| Title |
Mapping out the Neural Networks |
| Full Description |
Mapping out the neural networks of the inner ear as part of Dr. Murial Ross's study of the effects of space travel at the NASA Ames Research Center, Mountain View, California. |
| Date |
02/23/1990 |
| NASA Center |
Ames Research Center |
|
Aerial View of NASA Ames Res
| Title |
Aerial View of NASA Ames Research Center |
| Full Description |
Aerial view of the NASA Ames Research Center, Mountain View, California. The large flaired rectangular structure in the center of the photo is the 80 x 120 Foot Full Scale Wind Tunnel. Adjacent to it is the 40 x 80 Foot Full Scale Wind Tunnel which has been designated a National Historic Landmark. |
| Date |
01/01/1987 |
| NASA Center |
Ames Research Center |
|
Aerial View of the NASA Ames
| Title |
Aerial View of the NASA Ames Research Center |
| Full Description |
Aerial view of the NASA Ames Research Center, Mountain View, California. |
| Date |
01/01/1982 |
| NASA Center |
Ames Research Center |
|
Ames Smoke Tunnel
| Title |
Ames Smoke Tunnel |
| Full Description |
The N-260 Fluid Mechanics Laboratory (FML) test facilities, Smoke Tunnel shown with Greg Zilliac at the NASA Ames Research Center, Mountain View, California. |
| Date |
03/02/1987 |
| NASA Center |
Ames Research Center |
|
Apache Helicopter Helmet & D
| Title |
Apache Helicopter Helmet & Display System |
| Full Description |
The AH-64 Apache helicopter simulator with Intergrated Helmet & Display Sighting System (IHADSS) at the Ames Research Center, Moffett Field, California. |
| Date |
12/14/1989 |
| NASA Center |
Ames Research Center |
|
Model in 6 x 6 Foot Superson
| Title |
Model in 6 x 6 Foot Supersonic Wind Tunnel at Ames |
| Full Description |
Testing advanced designs for high-speed aircraft, an engineer makes final calibrations to a model mounted in the 6 x 6 Foot Supersonic Wind Tunnel at the NACA Ames Aeronautical Laboratory, Moffett Field, California. |
| Date |
06/01/1948 |
| NASA Center |
Ames Research Center |
|
NACA Ames 16 Foot High Speed
| Title |
NACA Ames 16 Foot High Speed Wind Tunnel |
| Full Description |
View of the 16 Foot High Speed Wind Tunnel at the NACA Ames Aeronautical Laboratory, Moffett Field, California. |
| Date |
04/01/1948 |
| NASA Center |
Ames Research Center |
|
NASA New Virtual Airport
| Title |
NASA New Virtual Airport |
| Full Description |
NASA's Virtual Airport Tower is located at the Ames Research Center, Moffett Field, California. The Virtual Airport Tower's two-story structure is a full-scale, highly sophisticated simulation facility that will emulate Level 5 air traffic control towers and the busiest airports. It provides the platform to conduct in-depth human factors studies with quantifiable results using actual air traffic controllers, airline dispatchers and airport managers. |
| Date |
01/01/1995 |
| NASA Center |
Ames Research Center |
|
NASA Robot Brain Surgeon
| Title |
NASA Robot Brain Surgeon |
| Full Description |
Mechanical Engineer Michael Guerrero works on the Robot Brain Surgeon testbed in the NeuroEngineering Group at the Ames Research Center, Moffett Field, California. Principal investigator Dr. Robert W. Mah states that potentially the simple robot will be able to feel brain structures better than any human surgeon, making slow, very precise movements during an operation. The brain surgery robot that may give surgeons finer control of surgical instruments during delicate brain operations is still under development. |
| Date |
06/02/1997 |
| NASA Center |
Ames Research Center |
|
Apollo Launch Escape System
| Title |
Apollo Launch Escape System in Wind Tunnel |
| Full Description |
A technician mounts a model of the Apollo Launch Escape System (LES) in the Unitary Wind Tunnel at the NASA Ames Research Center, Moffett Field, California. The LES was a tower like structure consisting of four solid propellent motors mounted atop the Apollo Command Module. In the event of a contingency, (booster failure or some other imminent failure) the LES would be commanded to ignite, subsequently removing the Command Module from the Saturn launch vehicle. |
| Date |
01/01/1963 |
| NASA Center |
Ames Research Center |
|
Atmospheric Entry Simulator
| Title |
Atmospheric Entry Simulator at Ames |
| Full Description |
The Atmospheric Entry Simulator at NASA's Ames Research Center, Moffett Field, California. Visible in the foreground is a large tank containing air under high pressure. In the middle ground directly behind it is a special trumpet- shaped nozzle, contured so that air flowing through it gradually changes in density in the same way that the Earth's atmosphere changes in density with altitude. Not visible in this photograph is a high speed gun used to launch a test model at earth re-entry speed (17,000 mph) upstream through a special nozzle while air is flowing through it. Technicians are adjusting the spark shadowgraph station required to make accurate picture and time recording of the model in flight. When a gun-launched model flies at full re-entry velocity into the simulator nozzle, it experiences the decelerations, stresses, pressures and temperatures of actual re-entry during a few thousandths of a second. The simulator can quickly and economically determine in the laboratory whether a specific design can survive atmospheric re-entry. |
| Date |
01/01/1959 |
| NASA Center |
Ames Research Center |
|
Parafoil in 80 x 120 Foot Wi
| Title |
Parafoil in 80 x 120 Foot Wind Tunnel |
| Full Description |
The Pioneer Aerospace Parafoil (Advanced Recovery System II), undergoes testing in the world's largest wind tunnel, the 80 x 120 Foot Tunnel at NASA's Ames Research Center, Mountain View California. |
| Date |
04/10/1990 |
| NASA Center |
Ames Research Center |
|
Pioneer 10 Trajectory
| Title |
Pioneer 10 Trajectory |
| Full Description |
This image, drawn in 1970, is an artist's rendering of the Pioneer 10 spacecraft trajectory, with the planets labeled and a list of the instruments that were intended to be flown. Before the use of computer animation, artists were hired by JPL and NASA to depict a spacecraft in flight, for use as a visual aid to promote the project during development. Pioneer 10 was managed by NASA Ames Research Center in Moffett Field, California. The Pioneer F spacecraft, as it was known before launch, was designed and built by TRW Systems Group, Inc. JPL developed three instruments that flew on the spacecraft: Magnetic Fields, S-Band Occultation, and Celestial Mechanics, as well as running the Deep Space Network which provided tracking and data system support. Caltech was responsible for the Jovian Infrared Thermal Structure experiment. Pioneer was very successful, crossing the orbit of Mars and the asteroid belt beyond it, encountering, studying, and photographing Jupiter, then crossing the orbits of Saturn, Uranus, and Neptune. It left the solar system in 1983 and has been contacted several times in the past few years. As of July 2001, the spacecraft was still able to send a return signal to Earth. At Jupiter, the experiments of Pioneer were used to examine the environmental and atmospheric characteristics of the giant planet. Pioneer was also the vital precursor to all future flights to the outer solar system. It determined that a spacecraft could safely fly through the asteroid belt. It also measured the intensity of Jupiter's radiation belt so that NASA could design future Jupiter (and other outer planets) orbiters. |
| Date |
03/07/1972 |
| NASA Center |
Jet Propulsion Laboratory |
|
Cobra Helicopter at Sunrise
| Title |
Cobra Helicopter at Sunrise |
| Full Description |
A TH-1S (NASA-736) Cobra helicopter at sunrise on the ramp at the NASA Ames Research Center, Moffett Field, California. |
| Date |
12/01/1989 |
| NASA Center |
Ames Research Center |
|
Puma Robotic Arm
| Title |
Puma Robotic Arm |
| Full Description |
The Puma Robotic Sensor Arm for use in Virtual Reality development and studies at the NASA Ames Research Center, Mountain View, California |
| Date |
04/02/1990 |
| NASA Center |
Ames Research Center |
|
Republic F-84F on the Ramp a
| Title |
Republic F-84F on the Ramp at Moffett Field |
| Full Description |
The Republic F84F Thunderjet fighter-bomber used by the United States Air Force was one of several high speed aircraft involved in flight research at the NACA Ames Aeronautical Laboratory (now, Ames Research Center) at Moffett Field, California. Instruments inside the aircraft record large quantities of data on its aerodynamic performance as it is flown by a NACA scientist-pilot through a carefully planned research program. Later this data will be anyalyzed and interpreted by NACA scientists and reports based on their findings will provide valuable information for designers of future aircraft. NACA (now, NASA) is the independent federal government agency responsible for research into the problems associated with flight. |
| Date |
09/16/1954 |
| NASA Center |
Ames Research Center |
|
Cray 2 Supercomputer
| Title |
Cray 2 Supercomputer |
| Full Description |
Cray 2 Supercomputer for the Numerical Aerodynamic Simulator at the NASA Ames Research Center, Mountain View California. |
| Date |
01/01/1987 |
| NASA Center |
Ames Research Center |
|
Cray Y 190A Supercomputer
| Title |
Cray Y 190A Supercomputer |
| Full Description |
The Cray Y 190A Supercomputer at the NASA Ames Research Center, Mountain View, California. |
| Date |
03/01/1990 |
| NASA Center |
Ames Research Center |
|
ER-2 Airborne Science Aircra
| Title |
ER-2 Airborne Science Aircraft |
| Full Description |
First acquired in 1981, NASA has been using two ER-2 Airborne Science aircraft as flying laboratories. The aircraft once based at Ames Research Center now fly out of Dryden Flight Research Center in Edwards, California. They collect information about our surroundings, including Earth resources, celestial observations, atmospheric chemistry, and dynamics and oceanic processes. The aircraft are also used for electronic sensor research and development, satellite calibration, and satellite data validation. |
| Date |
1981 |
| NASA Center |
Dryden Flight Research Center |
|
EVA Exercise Device
| Title |
EVA Exercise Device |
| Full Description |
EVA (Extra Vehicular Activity) Exercise Device for evaluation and effectiveness of weightlessness on astronauts during long duration spaceflights at the NASA Ames Research Center, Mountain View, California. |
| Date |
02/23/1990 |
| NASA Center |
Ames Research Center |
|
EVA Exercise Device
| Title |
EVA Exercise Device |
| Full Description |
The EVA (Extra Vehicular Activity) Exercise Device for evaluation and effectiveness of weightlessness on astronauts during long duration spaceflights, at the NASA Ames Research Center, Mountain View, California |
| Date |
02/23/1990 |
| NASA Center |
Ames Research Center |
|
Space Station Centrifuge
| Title |
Space Station Centrifuge |
| Full Description |
The 1.8 meter Space Station Centrifuge in Building N-244 at the NASA Ames Research Center, Mountain View, California. |
| Date |
01/01/1987 |
| NASA Center |
Ames Research Center |
|
F-86 in Full Scale Wind Tunn
| Title |
F-86 in Full Scale Wind Tunnel at Ames |
| Full Description |
This F-86 aircraft is mounted in the 40 x 80 Foot Full Scale Wind Tunnel at the NACA Ames Aeronautical Laboratory, Moffett Field California. |
| Date |
01/01/1954 |
| NASA Center |
Ames Research Center |
|
F-86 Lowered into Full Scale
| Title |
F-86 Lowered into Full Scale Tunnel at Ames |
| Full Description |
This F-86 aircraft is being lowered into the 40 x 80 Foot Full Scale Wind Tunnel at the NACA Ames Aeronautical Laboratory, Moffett Field California. Behind the aircraft and out of view, a crane operator lowers the jet as a mechanic holds a guide rope aligning the F-86 with supporting struts located down in the tunnel. Once the jet is mounted on the struts, tunnel doors visible on either side of the aircraft's wings will close to form an air tight seal. |
| Date |
01/01/1954 |
| NASA Center |
Ames Research Center |
|
First Meeting of the NACA 19
| Title |
First Meeting of the NACA 1915 |
| Full Description |
The first meeting of the National Advisory Committee for Aeronautics (NACA.) in the Office of The Secretary Of War April 23, 1915. Brig. Gen. George P. Scriven was elected as the temporary Chairman of the NACA and Dr. Charles D. Walcott (not pictured), Secretary of the Smithsonian, was elected Chairman of the NACA Executive Committee. After the Wright Brothers historic first flight in 1903, the United States began to fall behind in aeronautical research. With the beginning of World War I the nation realized it needed a center for aeronautical research as a means of catching up technologically with Europe. On March 3, 1915 the legislation creating the NACA passed and the NACA was born. For 43 years the NACA worked to advance aviation research until it was eventually absorbed into the new space agency, NASA, in 1958. Seated from Left to Right: Dr. William Durand, Stanford University, California. Dr. S.W. Stratton, Director, Bureau of Standards. Brig.Gen. George P. Scriven, Chief Signal Officer, War Dept. Dr. C.F. Marvin, Chief, United States Weather Bureau Dr. Michael I Pupin, Columbia University, New York. Standing: Holden C. Richardson, Naval Instructor. Dr. John F. Hayford, Northwestern University, Illinois. Capt. Mark L. Bristol, Director of Naval Aeronautics. Lt. Col. Samuel Reber, Signal Corps. Charge, Aviation Section Also present at the First Meeting: Dr. Joseph S. Ames, Johns Hopkins University, Baltimore, MD. Hon. B. R. Newton, Asst. Secretary of Treasury. |
| Date |
04/23/1915 |
| NASA Center |
Ames Research Center |
|
Free-Falling Body Nose Dives
| Title |
Free-Falling Body Nose Dives in Desert |
| Full Description |
This missile-like free-falling body was dropped from an altitude of seven miles. The purpose of this drop was to investigate the efficiency of air inlets of a type suitable for high speed jet aircraft. Its descent rate is checked first by automatic dive brakes (seen partially open) and then by parachute. The body has buried its nose in the California desert. The delicate onboard instruments which recorded performance data were recovered intact. |
| Date |
01/01/1955 |
| NASA Center |
Ames Research Center |
|
Fullerene Nanogears
| Title |
Fullerene Nanogears |
| Full Description |
The Numerical Aerospace Simulation Systems Division (NAS) of the NASA Ames Research Center, Moffett Field, California is conducting research into molecular-sized devices known as Nanotechnology. This photograph depicts two "Fullerene Nano-gears" with multiple teeth. The hope is that one day, products can be constructed made of thousands of tiny machines that could self-repair and adapt to the environment in which they exist. Researchers have simulated attaching benzyne molecules to the outside of a nanotube to form gear teeth. Nanotubes are molecular-sized pipes made of carbon atoms. To "drive" the gears, the supercomputer simulated a laser that served as a motor. The laser creates an electric field around the nanotube. A positively charged atom is placed on one side of the nanotube, and a negatively charged atom on the other side. The electric field drags the nanotube around like a shaft turning. Jie Han, Al Globus, Richard Jaffe and Glenn Deardorff are the authors of a technical paper detailing this technology which appears in The Journal of Nanotechnology. |
| Date |
04/01/1997 |
| NASA Center |
Ames Research Center |
|
Future Flight Central
| Title |
Future Flight Central |
| Full Description |
NASA "Future Flight Central," the world's first full-scale virtual airport control tower, opened December 13, 1999 at NASA Ames Research Center, Moffett Field, California. Constructed at a cost of $10 million, the two story facility was jointly funded by NASA and the Federal Aviation Administration (FAA). The facility is designed to test ways to solve potential air and ground traffic problems at commercial airports under realistic airport conditions and configurations. The facility provides an opportunity for airlines and airports to mitigate passenger delays by fine tuning airport hub operations, gate management, ramp movement procedures, and various other airport improvements. Twelve rear projection screens provide a seamless 360 degree high- resolution view of the airport or other screens being depicted. The imaging system, powered by supercomputers, provides a realistic view of weather conditions, enviromental and seasonal effects and the movement of up to 200 active aircraft and ground vehicles. |
| Date |
12/13/1999 |
| NASA Center |
Ames Research Center |
|
Godfrey, Cooper and DeFrance
| Title |
Godfrey, Cooper and DeFrance on the Ramp |
| Full Description |
Radio and early television personality Auther Godfrey, (left) has a discussion with NACA civilian pilot George Cooper, (center) and Smith DeFrance, (right) former director of the Ames Aeronautical Laboratory now NASA Ames Research Center, on the ramp at Moffett Field, California. |
| Date |
01/01/1948 |
| NASA Center |
Ames Research Center |
|
The 80 x 40 Foot Wind Tunnel
| Title |
The 80 x 40 Foot Wind Tunnel at Ames |
| Full Description |
Looking down the throat of the world's larget tunnel. The scene is NACA's 40 x 80 foot wind tunnel at Ames Aeronautical Laboratory, Moffett Field, California. The camera is stationed in the tunnel's largest section, 173 feet wide by 132 feet high. Here at top speed the air, driven by six 40 foot fans, is moving about 35 to 40 miles per hour. The rapid contraction of the throat (or nozzle) speeds up this air flow to more than 250 miles per hour in the oval test section, which is 80 feet wide and 40 feet high. The tunnel encloses 900 tons of air, 40 tons of which rush through the throat per second at maxium speed. Dwarfed by the immensity of the tunnel structure, the experimental model seen here is actually almost 50 feet long. Embodying a sharply swept-back wing suitable for supersonic flight, it is undergoing tests designed to improve the landing characteristics of this type of airfoil. Mounted on struts connected to scales under the test section, it is "flown standing still" while each element such as lift and drag is measured and air pressures occuring across the wing are recorded. Information gathered from such tests were made available to the nation's aircraft manufacturers by the NACA, an independent agency of the U.S. Government. |
| Date |
01/01/1947 |
| NASA Center |
Ames Research Center |
|
The Dirigible Hanger at Moff
| Title |
The Dirigible Hanger at Moffett Field |
| Full Description |
This is a view of the huge dirigible hangar with doors open at both ends at the NASA Ames Reserach Center, Moffett Field, California. Lockheed Missiles and Space Company under contract to the NASA-Marshall Space Flight Center was to use the hangar for construction and assembly of the nation's first nuclear stage rocket engine. Airplanes are on the ground at right, and in the background is San Francisco Bay. The ready-made "factory" structure was erected in 1931- 1933, to house the dirigible Macon, which crashed off the California coast in 1935. It has been used by the Navy for blimps and aircraft. The floor area 1,138 feet by 308 feet, covers over eight acres or enough to hold seven football fields. The height of the hangar is 198 feet, ample for the company to erect the RIET (Reactor-In-Flight Test) stage in an upright position. The program was eventually canceled. |
| Date |
01/01/1963 |
| NASA Center |
Ames Research Center |
|
The NASA Ames 40x80 Foot Win
| Title |
The NASA Ames 40x80 Foot Wind Tunnel |
| Full Description |
As tall as a 10 story building, this towering bank of vanes turns the air smoothly around one of the four corners of the world's largest wind tunnel. This tunnel which has a test section 40 feet high and 80 feet wide, is operated by the NACA's Ames Aeronautical Laboratory at Moffett Field, California. With a maxium air speed of 250 miles per hour, the 40 by 80 foot tunnel is proving very valuable in studying the low speed problems arising from new aircraft wing shapes designed for flight near or above the speed of sound. The tunnel structure covers eight acres and at the point shown in this photo is 172 feet wide and 123 feet high. |
| Date |
01/01/1945 |
| NASA Center |
Ames Research Center |
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