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Whole Earth
This image from Apollo 17, a
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4/2/09
| Description |
This image from Apollo 17, and others like it, captured whole hemispheres of water, land and weather. This photo was the first view of the south polar ice cap. Almost the entire coastline of Africa is visible, along with the Arabian Peninsula. |
| Date |
4/2/09 |
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On a Roll
The NOAA-N Prime spacecraft
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1/6/09
| Description |
The NOAA-N Prime spacecraft arrives at NASA's Hazardous Processing Facility on Vandenberg Air Force Base in California. It is the latest polar-orbiting operational environmental weather satellite developed by NASA for the National Oceanic and Atmospheric Administration. Image credit: NASA/Jerry Nagy, VAFB Nov. 4, 2008 |
| Date |
1/6/09 |
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Readied for Flight
The NOAA-N Prime satellite s
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1/28/09
| Description |
The NOAA-N Prime satellite stands in the payload processing facility at Vandenberg Air Force Base in California. NOAA-N Prime is the latest polar-orbiting operational environmental weather satellite developed by NASA for the National Oceanic and Atmospheric Administration. Image credit: NASA Nov. 11, 2008 |
| Date |
1/28/09 |
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Processing Under Way
The NOAA-N Prime satellite i
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1/28/09
| Description |
The NOAA-N Prime satellite is displayed in the payload processing facility at Vandenberg Air Force Base in California. NOAA-N Prime is the latest polar-orbiting operational environmental weather satellite developed by NASA for the National Oceanic and Atmospheric Administration. Image credit: NASA Nov. 11, 2008 |
| Date |
1/28/09 |
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NOAA-N Prime Processing
Inside the payload processin
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1/28/09
| Description |
Inside the payload processing facility at Vandenberg Air Force Base in California, the NOAA-N Prime satellite is rotated toward a vertical position. NOAA-N Prime is the latest polar-orbiting operational environmental weather satellite developed by NASA for the National Oceanic and Atmospheric Administration. Image credit: NASA Nov. 6, 2008 |
| Date |
1/28/09 |
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Spacecraft Testing
At Space Launch Complex 2 at
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2/6/09
| Description |
At Space Launch Complex 2 at Vandenberg Air Force Base in California, the NOAA-N Prime spacecraft is set up for testing. NOAA-N Prime is the latest polar-orbiting operational environmental weather satellite developed by NASA for the National Oceanic and Atmospheric Administration. Image Credit: NASA/Daniel Liberotti, VAFB Jan. 20, 2009 |
| Date |
2/6/09 |
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Liftoff!
A Delta II rocket climbs int
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2/6/09
| Description |
A Delta II rocket climbs into the dark, pre-dawn sky at Vandenberg Air Force Base in California. The rocket successfully propelled the NOAA-N Prime spacecraft toward its polar orbit around Earth. Image credit: Carleton Bailie/United Launch Alliance Feb. 6, 2009 |
| Date |
2/6/09 |
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Studying Auroras
NASA's THEMIS mission launch
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| Description |
NASA's THEMIS mission launches on Feb. 15 to study the fiery skies over the Earth's northern and southern polar regions. |
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LRO 50km Up
The Lunar Reconnaissance Orb
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2/24/09
| Description |
The Lunar Reconnaissance Orbiter will circle the moon approximately 50km above the surface in a polar orbit. Credit: Chris Meaney, NASA Conceptual Image Lab |
| Date |
2/24/09 |
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NASA's Lunar Reconnaissance
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NASA's Lunar Reconnaissance
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2/13/09
| Description |
NASA's Lunar Reconnaissance Orbiter, or LRO, spacecraft arrived in Florida on Feb. 13 and was transported to a payload processing facility at the Astrotech Space Operations facility in Titusville to being preparations for launch. The spacecraft's solar arrays were deployed and checked out for flight on Feb. 15. The satellite's mission is one of the first steps in NASA's plan to return astronauts to the moon. LRO will spend at least one year in a low polar orbit on its primary exploration mission, with the possibility of three more years to collect additional detailed scientific information about the moon and its environment. |
| Date |
2/13/09 |
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NOAA-N Prime Soars into Pola
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NASA launches a new satellit
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2/6/09
| Title |
NOAA-N Prime Soars into Polar Orbit! |
| Date |
2/6/09 |
| Description |
NASA launches a new satellite to improve weather forecasting around the world. |
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Successful Flight Through En
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The Cassini spacecraft has w
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11/6/09
| Description |
The Cassini spacecraft has weathered the Monday, Nov. 2, 2009, flyby of SaturnÎÿ_Îÿ_Îÿ__Îÿ__Îÿ_s moon Enceladus in good health and has been sending images and data of the encounter back to Earth. Cassini had approached Enceladus more closely before, but this passage took the spacecraft on its deepest plunge yet through the heart of the plume shooting out from the south polar region. Scientists are eagerly sifting through the results. In this unprocessed image, sunlight brightens a crescent curve along the edge of Saturn's moon Enceladus and highlights its misty plume. The image was captured by Cassini's narrow-angle camera as the spacecraft passed about 190,000 kilometers (120,000 miles) over the moon. This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2010. At its closest point on Nov. 2, Cassini flew about 100 kilometers (60 miles) above the surface of Enceladus. Since the discovery of the plume in 2005, scientists have been captivated by the enigmatic jets. Previous flybys detected water vapor, sodium and organic molecules, but scientists need to know more about the plumeÎÿ_Îÿ_Îÿ__Îÿ__Îÿ_s composition and density to characterize the source, possibly a liquid ocean under the moonÎÿ_Îÿ_Îÿ__Îÿ__Îÿ_s icy surface. It would also help them determine whether Enceladus has the conditions necessary for life. Mission managers did extensive studies to make sure the spacecraft could fly safely through the plumes and not use an excessive amount of propellant. Image Credit: NASA/JPL/Space Science Institute |
| Date |
11/6/09 |
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Successful Flight Through En
…
The Cassini spacecraft has w
…
11/9/09
| Description |
The Cassini spacecraft has weathered the Monday, Nov. 2, 2009, flyby of SaturnÎÿ_Îÿ_Îÿ__Îÿ__Îÿ_s moon Enceladus in good health and has been sending images and data of the encounter back to Earth. Cassini had approached Enceladus more closely before, but this passage took the spacecraft on its deepest plunge yet through the heart of the plume shooting out from the south polar region. Scientists are eagerly sifting through the results. In this unprocessed image, sunlight brightens a crescent curve along the edge of Saturn's moon Enceladus and highlights its misty plume. The image was captured by Cassini's narrow-angle camera as the spacecraft passed about 190,000 kilometers (120,000 miles) over the moon. This image has not been validated or calibrated. A validated/calibrated image will be archived with the NASA Planetary Data System in 2010. At its closest point on Nov. 2, Cassini flew about 100 kilometers (60 miles) above the surface of Enceladus. Since the discovery of the plume in 2005, scientists have been captivated by the enigmatic jets. Previous flybys detected water vapor, sodium and organic molecules, but scientists need to know more about the plumeÎÿ_Îÿ_Îÿ__Îÿ__Îÿ_s composition and density to characterize the source, possibly a liquid ocean under the moonÎÿ_Îÿ_Îÿ__Îÿ__Îÿ_s icy surface. It would also help them determine whether Enceladus has the conditions necessary for life. Mission managers did extensive studies to make sure the spacecraft could fly safely through the plumes and not use an excessive amount of propellant. Image Credit: NASA/JPL/Space Science Institute |
| Date |
11/9/09 |
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The 2001 Mars Odyssey Orbite
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| Description |
The 2001 Mars Odyssey Orbiter is scheduled for launch on April 7, 2001. It will arrive at Mars in October. After a propulsive maneuver into a 25-hour capture orbit, aerobraking will be used over the next 76 days to achieve the 2-hour science orbit. Aerobraking was utilized on the Mars Global Surveyor and Mars Polar Orbiter missions. The Orbiter will carry 3 science instruments, the Thermal Emission Imaging System (THEMIS), the Gamma Ray Spectrometer (GRS), and the Mars Radiation Environment Experiment (MARIE). THEMIS will map the mineralogy and morphology of the Martian surface using a high- resolution camera and a thermal infrared imaging spectrometer. The GRS will achieve global mapping of the elemental composition of the surface and determine the abundance of hydrogen in the shallow subsurface. The GRS is a rebuild of the instrument lost with the Mars Observer mission. The MARIE will characterize aspects of the near-space radiation environment as related to the radiation-related risk to human explorers. |
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Mars Polar Lander
A bottom view of the Mars Po
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| Description |
A bottom view of the Mars Polar Lander spacecraft. The spacecraft will travel 10 months from Earth to Mars to land near the southern polar cap in December 1999 and carry out a three- month mission to search for traces of subsurface water in this frozen, layered terrain. The lander carries three scientific packages: the Mars descent imager, furnished by Malin Space Science Systems, Inc., which will view the landing site at increasingly higher resolution, the atmospheric lidar experiment, provided by Russia's Space Research Institute, which will measure the presence and height of atmospheric hazes, along with a miniature microphone provided by The Planetary Society, to record the sounds of Mars, and the Mars Volatile and Climate Surveyor science package. The mission is part of NASA's Mars Surveyor program, a sustained program of robotic exploration of the red planet, managed by the Jet Propulsion Laboratory for NASA's Office of Space Science, Washington, DC. Lockheed Martin Astronautics is NASA's industrial partner in the mission. ##### |
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Mars Polar Lander
A top view of the Mars Polar
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| Description |
A top view of the Mars Polar Lander spacecraft. The spacecraft will travel 10 months from Earth to Mars to land near the southern polar cap in December 1999 and carry out a three- month mission to search for traces of subsurface water in this frozen, layered terrain. The lander carries three scientific packages: the Mars descent imager, furnished by Malin Space Science Systems, Inc., which will view the landing site at increasingly higher resolution, the atmospheric lidar experiment, provided by Russia's Space Research Institute, which will measure the presence and height of atmospheric hazes, along with a miniature microphone provided by The Planetary Society, to record the sounds of Mars, and the Mars Volatile and Climate Surveyor science package. The mission is part of NASA's Mars Surveyor program, a sustained program of robotic exploration of the red planet, managed by the Jet Propulsion Laboratory for NASA's Office of Space Science, Washington, DC. Lockheed Martin Astronautics is NASA's industrial partner in the mission. ##### |
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Mars '98 Camera
This photograph shows the Ma
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12/1/95
| Date |
12/1/95 |
| Description |
This photograph shows the Mars Surveyor '98 Orbiter Color Imager, a high resolution camera that will be flown aboard a NASA orbiter in 1998. The camera will be built by Dr. Michael Malin of Malin Space Science Systems, Inc., San Diego, and the California Institute of Technology in Pasadena, Calif. This tiny instrument consists of two cameras with unique optics and identical focal plane assemblies, data acquisition system electronics and power supplies. The wide-angle camera will acquire daily weather maps of Mars with a surface resolution of 0.8 kilometers up to 7.2 kilometers (0.5 mile to 4.5 miles). The camera produces these maps in five spectral bands, including two ultraviolet bands that will characterize atmospheric ozone and provide global maps of other atmospheric phenomena such as clouds, hazes, dust storms and the polar hood. The medium-angle camera will be used to study selected areas of Mars with a resolution of 40 meters (131 feet) and observe alterations in the planet's surface over time due to changing atmospheric conditions and winds. Ten spectral channels will provide the ability to discriminate both atmospheric and surface features on the basis of composition. The Mars '98 Orbiter mission is tentatively scheduled for launch aboard a Med- Lite expendable launch vehicle in December 1998. The mission will be managed by NASA's Jet Propulsion Laboratory for NASA's Office of Space Science, Washington, D.C. ##### |
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KENNEDY SPACE CENTER, FLA. -
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9/14/98
| Date |
9/14/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility-2 (SAEF-2), the Mars Climate Orbiter (background) is moved toward the workstand being readied by technicians (foreground). The Mars Climate Orbiter is heading for Mars where it will primarily support its companion Mars Polar Lander spacecraft, planned for launch on Jan. 3, 1999. After that, the Mars Climate Orbiter's instruments will monitor the Martian atmosphere and image the planet's surface on a daily basis for one Martian year (two Earth years). It will observe the appearance and movement of atmospheric dust and water vapor, as well as characterize seasonal changes on the surface. The detailed images of the surface features will provide important clues to the planet's early climate history and give scientists more information about possible liquid water reserves beneath the surface. The scheduled launch date for the Mars Climate Orbiter is Dec. 10, 1998, on a Boeing Delta II 7425 rocket. |
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KENNEDY SPACE CENTER, FLA. -
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9/14/98
| Date |
9/14/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- Technicians carefully maneuver the Mars Climate Orbiter toward its workstand in the Spacecraft Assembly and Encapsulation Facility-2 (SAEF-2). The Mars Climate Orbiter is heading for Mars where it will primarily support its companion Mars Polar Lander spacecraft, planned for launch on Jan. 3, 1999. After that, the Mars Climate Orbiter's instruments will monitor the Martian atmosphere and image the planet's surface on a daily basis for one Martian year (two Earth years). It will observe the appearance and movement of atmospheric dust and water vapor, as well as characterize seasonal changes on the surface. The detailed images of the surface features will provide important clues to the planet's early climate history and give scientists more information about possible liquid water reserves beneath the surface. The scheduled launch date for the Mars Climate Orbiter is Dec. 10, 1998, on a Boeing Delta II 7425 rocket. |
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KENNEDY SPACE CENTER, FLA. -
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9/14/98
| Date |
9/14/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- Technicians lower the Mars Climate Orbiter onto its workstand in the Spacecraft Assembly and Encapsulation Facility-2 (SAEF-2). The Mars Climate Orbiter is heading for Mars where it will primarily support its companion Mars Polar Lander spacecraft, planned for launch on Jan. 3, 1999. After that, the Mars Climate Orbiter's instruments will monitor the Martian atmosphere and image the planet's surface on a daily basis for one Martian year (two Earth years). It will observe the appearance and movement of atmospheric dust and water vapor, as well as characterize seasonal changes on the surface. The detailed images of the surface features will provide important clues to the planet's early climate history and give scientists more information about possible liquid water reserves beneath the surface. The scheduled launch date for the Mars Climate Orbiter is Dec. 10, 1998, on a Boeing Delta II 7425 rocket. |
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KENNEDY SPACE CENTER, FLA. -
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9/14/98
| Date |
9/14/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- Technicians check the connections on the workstand holding the Mars Climate Orbiter in the Spacecraft Assembly and Encapsulation Facility-2 (SAEF-2). The Mars Climate Orbiter is heading for Mars where it will primarily support its companion Mars Polar Lander spacecraft, planned for launch on Jan. 3, 1999. After that, the Mars Climate Orbiter's instruments will monitor the Martian atmosphere and image the planet's surface on a daily basis for one Martian year (two Earth years). It will observe the appearance and movement of atmospheric dust and water vapor, as well as characterize seasonal changes on the surface. The detailed images of the surface features will provide important clues to the planet's early climate history and give scientists more information about possible liquid water reserves beneath the surface. The scheduled launch date for the Mars Climate Orbiter is Dec. 10, 1998, on a Boeing Delta II 7425 rocket. |
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NASA Scatterometer
This is a photograph of the
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1/25/96
| Date |
1/25/96 |
| Description |
This is a photograph of the NASA Scatterometer (NSCAT) mated to Japan's Advanced Earth Observation Satellite (ADEOS) in a clean room at the Tsukuba Space Center, north of Tokyo. The NSCAT instrument is located on the forward end of the spacecraft and consists of six, 3-meter-long antennas that are shown at the top of the satellite in this photograph. Three electronic subsystems are located under the antennas. The instrument's mass is 280 kilograms and it uses 240 watts of power. NSCAT is a microwave radar that will measure both the speed and direction of winds over the global oceans. Scientists will use NSCAT's data to study ocean circulation, global climate change and regional weather patterns. The instrument will record data over 90 percent of the ice-free global oceans every two days during its three-year mission. The mission is the first major Earth resources collaboration between NASA and the Japanese Space Agency. The ADEOS spacecraft is the largest spacecraft Japan has developed. It is has a mass of 3,500 kilograms and generates 4.5 kilowatts of electrical power. The bus dimensions are 4 meters by 4 meters by 5 meters and, with the NSCAT antennas deployed, the spacecraft has a total height of 11 meters. It will be launched into a Sun- synchronous polar orbit at an altitude of 797 kilometers by the Japanese H-II rocket on July 31, 1996, at 6:15 pm Pacific Daylight Time. The Jet Propulsion Laboratory manages the NSCAT instrument for NASA's Office of Mission to Planet Earth. ##### |
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KENNEDY SPACE CENTER, FLA. -
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10/3/98
| Date |
10/3/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility-2 (SAEF-2), the Mars Polar Lander is secured on a workstand for testing, which includes a functional test of the science instruments and the basic spacecraft subsystems. The Mars Polar Lander is targeted for launch from Cape Canaveral Air Station aboard a Delta II rocket on Jan. 3, 1999. The solar-powered spacecraft is designed to touch down on the Martian surface near the northern-most boundary of the south pole in order to study the water cycle there. The lander also will help scientists learn more about climate change and current resources on Mars, studying such things as frost, dust, water vapor and condensates in the Martian atmosphere. |
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KENNEDY SPACE CENTER, FLA. -
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10/3/98
| Date |
10/3/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility-2 (SAEF-2), the top of the Mars Polar Lander is swung out of the way before testing, which includes a functional test of the science instruments and the basic spacecraft subsystems. The Mars Polar Lander is targeted for launch from Cape Canaveral Air Station aboard a Delta II rocket on Jan. 3, 1999. The solar-powered spacecraft is designed to touch down on the Martian surface near the northern-most boundary of the south pole in order to study the water cycle there. The lander also will help scientists learn more about climate change and current resources on Mars, studying such things as frost, dust, water vapor and condensates in the Martian atmosphere. |
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KENNEDY SPACE CENTER, FLA. -
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10/3/98
| Date |
10/3/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility-2 (SAEF-2), the protective covering for the Mars Polar Lander is removed so technicians can prepare the Lander for testing, which includes a functional test of the science instruments and the basic spacecraft subsystems. The Mars Polar Lander is targeted for launch from Cape Canaveral Air Station aboard a Delta II rocket on Jan. 3, 1999. The solar- powered spacecraft is designed to touch down on the Martian surface near the northern-most boundary of the south pole in order to study the water cycle there. The lander also will help scientists learn more about climate change and current resources on Mars, studying such things as frost, dust, water vapor and condensates in the Martian atmosphere. |
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KENNEDY SPACE CENTER, FLA. -
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10/13/98
| Date |
10/13/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility-2 (SAEF-2), technicians test the science instruments and the basic spacecraft subsystems on the Mars Polar Lander. The solar-powered spacecraft is targeted for launch from Cape Canaveral Air Station aboard a Delta II rocket on Jan. 3, 1999. It is designed to touch down on the Martian surface near the northern-most boundary of the south pole in order to study the water cycle there. The lander also will help scientists learn more about climate change and current resources on Mars, studying such things as frost, dust, water vapor and condensates in the Martian atmosphere. |
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KENNEDY SPACE CENTER, FLA. -
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10/13/98
| Date |
10/13/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility-2 (SAEF-2), a technician tests the science instruments and the basic spacecraft subsystems on the Mars Polar Lander. The solar-powered spacecraft is targeted for launch from Cape Canaveral Air Station aboard a Delta II rocket on Jan. 3, 1999. It is designed to touch down on the Martian surface near the northern-most boundary of the south pole in order to study the water cycle there. The lander also will help scientists learn more about climate change and current resources on Mars, studying such things as frost, dust, water vapor and condensates in the Martian atmosphere. |
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KENNEDY SPACE CENTER, FLA. -
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10/13/98
| Date |
10/13/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility-2 (SAEF-2), technicians check underneath the Mars Polar Lander during the testing of science instruments. The solar-powered spacecraft is targeted for launch from Cape Canaveral Air Station aboard a Delta II rocket on Jan. 3, 1999. It is designed to touch down on the Martian surface near the northern-most boundary of the south pole in order to study the water cycle there. The lander also will help scientists learn more about climate change and current resources on Mars, studying such things as frost, dust, water vapor and condensates in the Martian atmosphere. |
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KENNEDY SPACE CENTER, FLA. -
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11/12/98
| Date |
11/12/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility -2 (SAEF-2), Chris Voorhees (left) and Satish Krishnan (right), from the Jet Propulsion Laboratory, remove the second Mars microprobe from a drum. Two microprobes will hitchhike on the Mars Polar Lander, scheduled to be launched Jan. 3, 1999, aboard a Delta II rocket. The solar-powered spacecraft is designed to touch down on the Martian surface near the northern-most boundary of the south pole in order to study the water cycle there. The lander also will help scientists learn more about climate change and current resources on Mars, studying such things as frost, dust, water vapor and condensates in the Martian atmosphere. The Mars microprobes, called Deep Space 2, are part of NASA's New Millennium Program. They will complement the climate-related scientific focus of the lander by demonstrating an advanced, rugged microlaser system for detecting subsurface water. Such data on polar subsurface water, in the form of ice, should help put limits on scientific projections for the global abundance of water on Mars. |
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KENNEDY SPACE CENTER, FLA. -
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11/12/98
| Date |
11/12/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility -2 (SAEF-2), a JPL worker checks the Mars microprobe. Two microprobes will hitchhike on the Mars Polar Lander, scheduled to be launched Jan. 3, 1999, aboard a Delta II rocket. The solar-powered spacecraft is designed to touch down on the Martian surface near the northern-most boundary of the south pole in order to study the water cycle there. The lander also will help scientists learn more about climate change and current resources on Mars, studying such things as frost, dust, water vapor and condensates in the Martian atmosphere. The Mars microprobes, called Deep Space 2, are part of NASA's New Millennium Program. They will complement the climate-related scientific focus of the lander by demonstrating an advanced, rugged microlaser system for detecting subsurface water. Such data on polar subsurface water, in the form of ice, should help put limits on scientific projections for the global abundance of water on Mars. |
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KENNEDY SPACE CENTER, FLA. -
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11/12/98
| Date |
11/12/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility -2 (SAEF-2), two JPL workers measure a Mars microprobe. Two microprobes will hitchhike on the Mars Polar Lander, scheduled to be launched Jan. 3, 1999, aboard a Delta II rocket. The solar-powered spacecraft is designed to touch down on the Martian surface near the northern-most boundary of the south pole in order to study the water cycle there. The lander also will help scientists learn more about climate change and current resources on Mars, studying such things as frost, dust, water vapor and condensates in the Martian atmosphere. The Mars microprobes, called Deep Space 2, are part of NASA's New Millennium Program. They will complement the climate-related scientific focus of the lander by demonstrating an advanced, rugged microlaser system for detecting subsurface water. Such data on polar subsurface water, in the form of ice, should help put limits on scientific projections for the global abundance of water on Mars. |
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KENNEDY SPACE CENTER, FLA. -
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11/12/98
| Date |
11/12/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility -2 (SAEF-2), JPL workers mount a Mars microprobe onto the Mars Polar Lander. Two microprobes will hitchhike on the lander, scheduled to be launched Jan. 3, 1999, aboard a Delta II rocket. The solar-powered spacecraft is designed to touch down on the Martian surface near the northern- most boundary of the south pole in order to study the water cycle there. The lander also will help scientists learn more about climate change and current resources on Mars, studying such things as frost, dust, water vapor and condensates in the Martian atmosphere. The Mars microprobes, called Deep Space 2, are part of NASA's New Millennium Program. They will complement the climate-related scientific focus of the lander by demonstrating an advanced, rugged microlaser system for detecting subsurface water. Such data on polar subsurface water, in the form of ice, should help put limits on scientific projections for the global abundance of water on Mars. |
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KENNEDY SPACE CENTER, FLA. -
…
11/12/98
| Date |
11/12/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility -2 (SAEF-2), a JPL worker carries a Mars microprobe to the Mars Polar Lander at left. Two microprobes will hitchhike on the lander, scheduled to be launched Jan. 3, 1999, aboard a Delta II rocket. The solar-powered spacecraft is designed to touch down on the Martian surface near the northern- most boundary of the south pole in order to study the water cycle there. The lander also will help scientists learn more about climate change and current resources on Mars, studying such things as frost, dust, water vapor and condensates in the Martian atmosphere. The Mars microprobes, called Deep Space 2, are part of NASA's New Millennium Program. They will complement the climate-related scientific focus of the lander by demonstrating an advanced, rugged microlaser system for detecting subsurface water. Such data on polar subsurface water, in the form of ice, should help put limits on scientific projections for the global abundance of water on Mars. |
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KENNEDY SPACE CENTER, FLA. -
…
11/12/98
| Date |
11/12/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility -2 (SAEF-2), JPL workers prepare to mount a Mars microprobe onto the Mars Polar Lander. Two microprobes will hitchhike on the lander, scheduled to be launched Jan. 3, 1999, aboard a Delta II rocket. The solar-powered spacecraft is designed to touch down on the Martian surface near the northern- most boundary of the south pole in order to study the water cycle there. The lander also will help scientists learn more about climate change and current resources on Mars, studying such things as frost, dust, water vapor and condensates in the Martian atmosphere. The Mars microprobes, called Deep Space 2, are part of NASA's New Millennium Program. They will complement the climate-related scientific focus of the lander by demonstrating an advanced, rugged microlaser system for detecting subsurface water. Such data on polar subsurface water, in the form of ice, should help put limits on scientific projections for the global abundance of water on Mars. |
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KENNEDY SPACE CENTER, FLA. -
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11/12/98
| Date |
11/12/98 |
| Description |
KENNEDY SPACE CENTER, FLA. -- In the Spacecraft Assembly and Encapsulation Facility -2 (SAEF-2), the two Mars microprobes are shown mounted on opposite sides of the Mars Polar Lander. The two microprobes and the lander are scheduled to be launched Jan. 3, 1999, aboard a Delta II rocket. The solar-powered spacecraft is designed to touch down on the Martian surface near the northern- most boundary of the south pole in order to study the water cycle there. The lander also will help scientists learn more about climate change and current resources on Mars, studying such things as frost, dust, water vapor and condensates in the Martian atmosphere. The Mars microprobes, called Deep Space 2, are part of NASA's New Millennium Program. They will complement the climate-related scientific focus of the lander by demonstrating an advanced, rugged microlaser system for detecting subsurface water. Such data on polar subsurface water, in the form of ice, should help put limits on scientific projections for the global abundance of water on Mars. |
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Europa's Broken Ice
Jupiter's moon Europa, as se
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| Description |
Jupiter's moon Europa, as seen in this image taken June 27, 1996 by NASA's Galileo spacecraft, displays features in some areas resembling ice floes seen in Earth's polar seas. Europa, about the size of Earth's moon, has an icy crust that has been severely fractured, as indicated by the dark linear, curved, and wedged- shaped bands seen here. These fractures have broken the crust into plates as large as 30 kilometers (18.5 miles) across. Areas between the plates are filled with material that was probably icy slush contaminated with rocky debris. Some individual plates were separated and rotated into new positions. Europa's density indicates that it has a shell of water ice as thick as 100 kilometers (about 60 miles), parts of which could be liquid. Currently, water ice could extend from the surface down to the rocky interior, but the features seen in this image suggest that motion of the disrupted icy plates was lubricated by soft ice or liquid water below the surface at the time of disruption. This image covers part of the equatorial zone of Europa and was taken from a distance of 156,000 kilometers (about 96,300 miles) by the solid-state imager camera on the Galileo spacecraft. North is to the right and the sun is nearly directly overhead. The area shown is about 360 by 770 kilometers (220-by-475 miles or about the size of Nebraska), and the smallest visible feature is about 1.6 kilometers (1 mile) across. |
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Sam Thurman is the Mars Pola
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| Description |
Sam Thurman is the Mars Polar Lander Flight Operations Manager. |
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High Latitude Mottling on Ju
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The familiar banded appearan
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12/18/00
| Date |
12/18/00 |
| Description |
The familiar banded appearance of Jupiter at low and middle latitudes gradually gives way to a more mottled appearance at high latitudes in this striking true color image taken Dec. 13, 2000, by NASA's Cassini spacecraft. The intricate structures seen in the polar region are clouds of different chemical composition, height and thickness. Clouds are organized by winds, and the mottled appearance in the polar regions suggests more vortex-type motion and winds of less vigor at higher latitudes. The cause of this difference is not understood. One possible contributor is that the horizontal component of the Coriolis force, which arises from the planet's rotation and is responsible for curving the trajectories of ocean currents and winds on Earth, has its greatest effect at high latitudes and vanishes at the equator. This tends to create small, intense vortices at high latitudes on Jupiter. Another possibility may lie in that fact that Jupiter overall emits nearly as much of its own heat as it absorbs from the Sun, and this internal heat flux is very likely greater at the poles. This condition could lead to enhanced convection at the poles and more vortex-type structures. Further analysis of Cassini images, including analysis of sequences taken over a span of time, should help us understand the cause of equator-to-pole differences in cloud organization and evolution. By the time this picture was taken, Cassini had reached close enough to Jupiter to allow the spacecraft to return images with more detail than what's possible with the planetary camera on NASA's Earth-orbiting Hubble Space Telescope. The resolution here is 114 kilometers (71 miles) per pixel. This contrast- enhanced, edge-sharpened frame was composited from images take at different wavelengths with Cassini's narrow-angle camera, from a distance of 19 million kilometers (11.8 million miles). The spacecraft was in almost a direct line between the Sun and Jupiter, so the solar illumination on Jupiter is almost full phase. Cassini is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini mission for NASA's Office of Space Science, Washington, D.C. Credit: NASA/JPL/University of Arizona # # # # # |
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NSCAT/Antarctica
This image of Antarctica and
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11/18/96
| Date |
11/18/96 |
| Description |
This image of Antarctica and the surrounding sea-ice pack was constructed from six days of data taken by the NASA Scatterometer (NSCAT) onboard Japan's Advanced Earth Observing Satellite in September 1996. The scatterometer's primary function is to study winds over the oceans, but scientists have devised a way of studying changes in the instrument's radar backscatter to look at land and ice surfaces as well. The black circle in the center of the image is an area where no data were collected due to the orbit of the satellite. The dark band around the continent is the evolving sea-ice pack. The white, rectangular object in the ice pack on the lower left of the image is a 100-kilometer by 200- kilometer "super iceberg" that broke off the Thwaites ice tongue and is now circulating in the sea-ice pack. Other large icebergs are also visible in the image. Antarctica is covered with a thick ice sheet which appears very bright in the image because of the way the snow crust and refrozen ice reflect the scatterometer's radar signal. Details visible in the glacial ice cover show the locations of ice "hills" and "valleys" that give scientists new information about how the ice is flowing under the surface. Scientists are using images like this to understand the effects of the ice pack on the ocean and climate systems. The polar regions play a central role in regulating global climate, and it is important to accurately record and monitor the extent and surface conditions of the Earth's major ice masses. Such monitoring can only be done using spaceborne sensors, and the scatterometer radar remote sensors are uniquely suited for mapping the polar regions since the radar can image the surface through clouds, regardless of sunlight conditions. This instrument provides frequent, all weather, all year monitoring of these vital regions of the Earth. NSCAT was launched from Japan on August 16, 1996. The mission represents the first major collaboration between the two nations in Earth remote- sensing. JPL developed, built and manages the NSCAT instrument for NASA's Mission to Planet Earth program. ##### |
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Richard Zurek is the Mars Po
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| Description |
Richard Zurek is the Mars Polar Lander Project Scientist. |
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Europa Ice Rafts
This high resolution image s
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4/9/97
| Date |
4/9/97 |
| Description |
This high resolution image shows the ice-rich crust of Europa, one of the moons of Jupiter. Seen here are crustal plates ranging up to 13 kilometers (8 miles) across, which have been broken apart and "rafted" into new positions, superficially resembling the disruption of pack-ice on polar seas during spring thaws on Earth. The size and geometry of these features suggest that motion was enabled by ice-crusted water or soft ice close to the surface at the time of disruption. The area shown is about 34 kilometers by 42 kilometers (21 miles by 26 miles), centered at 9.4 degrees north latitude, 274 degrees west longitude, and the resolution is 54 meters (59 yards). This picture was taken by the Solid State Imaging system on board the Galileo spacecraft on February 20, 1997, from a distance of 5,340 kilometers (3,320 miles) during the spacecraft's close flyby of Europa. The Jet Propulsion Laboratory, Pasadena, CA, manages the mission for NASA's Office of Space Science, Washington D.C. This image and other images and data received from Galileo are posted on the World Wide Web Galileo mission home page at: http://www.jpl.nasa.gov/galileo. ##### |
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1998 Mars Polar Lander
The Mars Surveyor '98 Polar
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5/27/98
| Date |
5/27/98 |
| Description |
The Mars Surveyor '98 Polar Lander is shown during recent deployment and testing of its surface solar panels. The spacecraft will travel 10 months from Earth to Mars to land near the southern polar cap in December 1999 and carry out a three- month mission to search for traces of subsurface water in this frozen, layered terrain. The lander carries three scientific packages: the Mars descent imager, furnished by Malin Space Science Systems, Inc., which will view the landing site at increasingly higher resolution, the atmospheric lidar experiment, provided by Russia's Space Research Institute, which will measure the presence and height of atmospheric hazes, along with a miniature microphone provided by The Planetary Society, to record the sounds of Mars, and the Mars Volatile and Climate Surveyor science package. The mission is part of NASA's Mars Surveyor program, a sustained program of robotic exploration of the red planet, managed by the Jet Propulsion Laboratory for NASA's Office of Space Science, Washington, DC. Lockheed Martin Astronautics is NASA's industrial partner in the mission. Photo copyright 1998, Lockheed Martin ##### |
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Mars Polar Lander
The Mars Polar Lander is sho
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| Description |
The Mars Polar Lander is shown on the surface of Mars. The spacecraft will travel 10 months from Earth to Mars to land near the southern polar cap in December 1999 and carry out a three- month mission to search for traces of subsurface water in this frozen, layered terrain. The lander carries three scientific packages: the Mars descent imager, furnished by Malin Space Science Systems, Inc., which will view the landing site at increasingly higher resolution, the atmospheric lidar experiment, provided by Russia's Space Research Institute, which will measure the presence and height of atmospheric hazes, along with a miniature microphone provided by The Planetary Society, to record the sounds of Mars, and the Mars Volatile and Climate Surveyor science package. The mission is part of NASA's Mars Surveyor program, a sustained program of robotic exploration of the red planet, managed by the Jet Propulsion Laboratory for NASA's Office of Space Science, Washington, DC. Lockheed Martin Astronautics is NASA's industrial partner in the mission. ##### |
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POLAR STRATOSPHERIC CLOUDS
Polar stratospheric clouds o
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4/5/00
| Date |
4/5/00 |
| Description |
Polar stratospheric clouds over Kiruna, Sweden, on Jan. 27, 2000. The colorful appearance of these clouds is due to the small size of their droplets and their high altitude, approximately 21,300 meters (70,000 ft). The small droplets in the clouds result in separation of light of different colors due to refraction of sunlight. Their high altitude allows for full solar illumination for up to 20 minutes following sunset at the ground. These clouds, which have long been called "Mother of Pearl" by Scandinavians, participate in a chain of events that leads to ozone depletion by human-produced chlorine. Between November 1999 and March 2000, the SAGE III Ozone Loss and Validation Experiment (SOLVE) provided scientists with measurements of ozone using a variety of satellite-, airplane-, balloon- and ground-based instruments. Scientists also obtained a comprehensive inventory of numerous other atmospheric gases and information on the physical and chemical properties of polar stratospheric clouds. The SOLVE mission was co-sponsored by the Upper Atmosphere Research Program, Atmospheric Effects of Aviation Project, Atmospheric Chemistry Modeling and Analysis Program, and Earth Observing System of NASA's Earth Science Enterprise as part of the validation program for the SAGE III instrument. Based primarily in Kiruna, Sweden, the campaign included scientists from the United States, Europe, Canada, Russia and Japan. A key aspect to the success of this mission was the permission to fly both NASA research aircraft over Russia. SOLVE was managed by the Ames Research Center, Moffett Field, CA, with extensive participation by science teams from Goddard Space Flight Center, Greenbelt, MD, Langley Research Center, Hampton, VA, and the Jet Propulsion Laboratory, Pasadena, CA, as well as a number of other government laboratories and universities. The ER-2 and DC-8 aircraft are based at Dryden Flight Research Center, Edwards, CA, and the U.S. balloon operations in Sweden were conducted by a team from the National Scientific Balloon Facility, Palestine, TX. |
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HIGH ALTITUDE BALLOON/ARCTIC
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A NASA high-altitude researc
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4/5/00
| Date |
4/5/00 |
| Description |
A NASA high-altitude research balloon climbing to study the composition of the Arctic stratosphere from the Esrange Balloon Launch Facility near Kiruna, Sweden. With its helium bubble expanding to the size of a large building while in the stratosphere, the balloon carried a payload of about 450 Kg. (1000 lbs) to an altitude of about 30,500 meters (100,000 ft.). Following flight, the instrument payload lands by parachute and is recovered for subsequent flights. Between November 1999 and March 2000, the SAGE III Ozone Loss and Validation Experiment (SOLVE) provided scientists with measurements of ozone using a variety of satellite-, airplane-, balloon- and ground-based instruments. Scientists also obtained a comprehensive inventory of numerous other atmospheric gases and information on the physical and chemical properties of polar stratospheric clouds. The SOLVE mission was co-sponsored by the Upper Atmosphere Research Program, Atmospheric Effects of Aviation Project, Atmospheric Chemistry Modeling and Analysis Program, and Earth Observing System of NASA's Earth Science Enterprise as part of the validation program for the SAGE III instrument. Based primarily in Kiruna, Sweden, the campaign included scientists from the United States, Europe, Canada, Russia and Japan. A key aspect to the success of this mission was the permission to fly both NASA research aircraft over Russia. SOLVE was managed by the Ames Research Center, Moffett Field, CA, with extensive participation by science teams from Goddard Space Flight Center, Greenbelt, MD, Langley Research Center, Hampton, VA, and the Jet Propulsion Laboratory, Pasadena, CA, as well as a number of other government laboratories and universities. The ER-2 and DC-8 aircraft are based at Dryden Flight Research Center, Edwards, CA, and the U.S. balloon operations in Sweden were conducted by a team from the National Scientific Balloon Facility, Palestine, TX. |
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OZONE INSTRUMENTS LOADED ON
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Scientists preparing their i
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4/5/00
| Date |
4/5/00 |
| Description |
Scientists preparing their instruments for flight on the NASA ER-2 research aircraft inside the Arena Arctica hangar, Kiruna, Sweden. The plane carries dozens of instruments in two pods attached to the wings, in the Q-bay area below the cockpit and in the nose. These pieces of the plane can be detached allowing access to the instruments prior to take-off. Between November 1999 and March 2000, the SAGE III Ozone Loss and Validation Experiment (SOLVE) provided scientists with measurements of ozone using a variety of satellite-, airplane-, balloon- and ground-based instruments. Scientists also obtained a comprehensive inventory of numerous other atmospheric gases and information on the physical and chemical properties of polar stratospheric clouds. The SOLVE mission was co-sponsored by the Upper Atmosphere Research Program, Atmospheric Effects of Aviation Project, Atmospheric Chemistry Modeling and Analysis Program, and Earth Observing System of NASA's Earth Science Enterprise as part of the validation program for the SAGE III instrument. Based primarily in Kiruna, Sweden, the campaign included scientists from the United States, Europe, Canada, Russia and Japan. A key aspect to the success of this mission was the permission to fly both NASA research aircraft over Russia. SOLVE was managed by the Ames Research Center, Moffett Field, CA, with extensive participation by science teams from Goddard Space Flight Center, Greenbelt, MD, Langley Research Center, Hampton, VA, and the Jet Propulsion Laboratory, Pasadena, CA, as well as a number of other government laboratories and universities. The ER-2 and DC-8 aircraft are based at Dryden Flight Research Center, Edwards, CA, and the U.S. balloon operations in Sweden were conducted by a team from the National Scientific Balloon Facility, Palestine, TX. |
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ER-2 USED IN ARCTIC OZONE RE
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The NASA ER-2 high-altitude
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4/5/00
| Date |
4/5/00 |
| Description |
The NASA ER-2 high-altitude research plane on the runway of Kiruna, Sweden. The airplane -- a civilian variant of the U-2 reconnaissance plane capable of reaching altitudes as high as 21,330 meters (70,000 feet) -- carried into the stratosphere dozens of scientific instruments that measure the composition of Earth's ozone layer. The only person on board is the pilot, who must wear a pressurized spacesuit to guard against the dangers of high-altitude flight. Between November 1999 and March 2000, the SAGE III Ozone Loss and Validation Experiment (SOLVE) provided scientists with measurements of ozone using a variety of satellite-, airplane-, balloon- and ground-based instruments. Scientists also obtained a comprehensive inventory of numerous other atmospheric gases and information on the physical and chemical properties of polar stratospheric clouds. The SOLVE mission was co-sponsored by the Upper Atmosphere Research Program, Atmospheric Effects of Aviation Project, Atmospheric Chemistry Modeling and Analysis Program, and Earth Observing System of NASA's Earth Science Enterprise as part of the validation program for the SAGE III instrument. Based primarily in Kiruna, Sweden, the campaign included scientists from the United States, Europe, Canada, Russia and Japan. A key aspect to the success of this mission was the permission to fly both NASA research aircraft over Russia. SOLVE was managed by the Ames Research Center, Moffett Field, CA, with extensive participation by science teams from Goddard Space Flight Center, Greenbelt, MD, Langley Research Center, Hampton, VA, and the Jet Propulsion Laboratory, Pasadena, CA, as well as a number of other government laboratories and universities. The ER-2 and DC-8 aircraft are based at Dryden Flight Research Center, Edwards, CA, and the U.S. balloon operations in Sweden were conducted by a team from the National Scientific Balloon Facility, Palestine, TX. |
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Voyager 2-N77
Voyager 2 obtained this high
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8/29/89
| Date |
8/29/89 |
| Description |
Voyager 2 obtained this high-resolution color image of Neptune's large satellite Triton during its close flyby on Aug. 25, 1989. Approximately a dozen individual images were combined to produce this comprehensive view of the Neptune-facing hemisphere of Triton. Fine detail is provided by high-resolution, clear-filter images, with color information added from lower-resolution frames. The large south polar cap at the bottom of the image is highly reflective and slightly pink in color, it may consist of a slowly evaporating layer of nitrogen ice deposited during the previous winter. From the ragged edge of the polar cap northward the satellite's face is generally darker and redder in color. This coloring may be produced by the action of ultraviolet light and magnetospheric radiation upon methane in the atmosphere and surface. Running across this darker region, approximately parallel to the edge of the polar cap, is a band of brighter white material that is almost bluish in color. The underlying topography in this bright band is similar, however to that in the darker, redder regions surrounding it. The Voyager Mission is conducted by JPL for NASA's Office of Space Science and Applications. ##### |
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Voyager 2
This picture of Neptune was
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4/2/90
| Date |
4/2/90 |
| Description |
This picture of Neptune was produced from the last whole planet images taken through the green and orange filters on the Voyager 2 narrow angle camera. The images were taken at a range of 4.4 million miles from the planet, 4 days and 20 hours before closest approach. The picture shows the Great Dark Spot and its companion bright smudge, on the west limb the fast moving bright feature called Scooter and the little dark spot are visible. These clouds were seen to persist for as long as Voyager's cameras could resolve them. North of these, a bright cloud band similar to the south polar streak may be seen. The Voyager Mission is conducted by JPL for NASA's Office of Space Science and Applications. |
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GLL/EM15
This mosaic picture of the M
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12/22/92
| Date |
12/22/92 |
| Description |
This mosaic picture of the Moon was compiled from 18 images taken with a green filter by Galileo's imaging system during the spacecraft's flyby on December 7, 1992, some 11 hours before its Earth flyby at 1509 UTC (7:09 a.m. Pacific Standard Time) December 8. The north polar region is near the top part of the mosaic, which also shows Mare Imbrium, the dark area on the left, Mare Serenitatis at center, and Mare Crisium, the circular dark area to the right. Bright crater rim and ray deposits are from Copernicus, an impact crater 96 kilometers (60 miles) in diameter. Computer processing has exaggerated the brightness of poorly illuminated features near the day/night terminator in the polar regions, giving a false impression of high reflectivity there. The digital image processing was done by DLR the German aerospace research establishment near Munich, an international collaborator in the Galileo mission. The Galileo project, whose primary mission is the exploration of the Jupiter system in 1995-97, is managed for NASA's Office of Space Science and Applications by the Jet Propulsion Laboratory. ##### |
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