|
|
International Teams
The 2008 race was the second
6/16/08
| Description |
The 2008 race was the second year that a team representing the German Space Education Institute entered the moonbuggy race. Other countries represented in 2008 were Canada and India. |
| Date |
6/16/08 |
|
Fires in Yukon Territory, Ca
Sixty-eight fires were affec
8/3/09
| Description |
Sixty-eight fires were affecting an estimated 94,107 hectares (232,543 acres) in Canada's Yukon Territory on July 30, 2009, according to the daily situation report from the Canadian Interagency Forest Fire Centre. Several large blazes were pouring out thick smoke plumes when the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Terra satellite passed overhead and captured this natural-color image. Places where MODIS detected active fire are outlined in red. This image is cropped (at left) along the border with Alaska (visible in large image), where even smokier fires are burning. The smoke from these fires and others in Russia's Far East are veiling the entire Arctic with haze. NASA image by Jeff Schmaltz, MODIS Rapid Response Team. Caption by Rebecca Lindsey. |
| Date |
8/3/09 |
|
Wildfires in Alaska's Yukon
Large fires in eastern Alask
8/3/09
| Description |
Large fires in eastern Alaska's Yukon Flats National Wildlife Refuge were billowing out thick plumes of yellowish smoke when the Moderate Resolution Imaging Spectroradiometer (MODIS) on NASA's Terra satellite captured this natural-color image on July 30, 2009. The smoke appears to be relatively close to the ground, in many places, brighter clouds lie over top of the smoke. The large version of the image shows that the smoke covers a wide area of Alaska and western Canada. NASA image by Jeff Schmaltz, MODIS Rapid Response Team. Caption by Rebecca Lindsey. |
| Date |
8/3/09 |
|
Prince Albert, Canada Season
This is a comparison of imag
10/5/94
| Date |
10/5/94 |
| Description |
This is a comparison of images over Prince Albert, produced by the Spaceborne Imaging Radar-C and X-band Synthetic Aperture Radar aboard the space shuttle Endeavour on its 20th orbit on April 10, 1994, and again on orbit 20 of the second flight of Endeavour on October 1, 1994. The area is centered at 53.91 degrees north latitude and 104.69 degrees west longitude and is located 40 kilometers (25 miles) north and 30 kilometers (18.5 miles) east of the town of Prince Albert in the Saskatchewan province of Canada. The image covers the area east of Candle Lake, between the gravel highway of 120 and west of highway 106. The area imaged is near the southern limit of the boreal forest. The boreal forest of North America is a continuous vegetation belt at high latitudes stretching across the continent from the Atlantic shoreline of central Labrador and then westward across Canada to the interior mountains and central coastal plains of Alaska. The forest is also part of a larger northern hemisphere circumpolar boreal forest belt. Coniferous trees dominate the entire forest but deciduous trees are also present. During the month of April, the forest experiences seasonal changes from a frozen condition to a thawed condition. The trees are completely frozen over the winter season and the forest floor is covered by snow. As the average temperature rises in the spring, the trees are thawed and the snow melts. This transition has an impact on the rate of moisture evaporation and release of carbon dioxide into the atmosphere. In late September and early October, the boreal forest experiences a relatively different seasonal change. At this time, the leaves on deciduous trees start changing color and dropping off. The soil and trees are quite often moist due to frequent rainfall and cloud cover. The evaporation of moisture and carbon dioxide into the atmosphere also diminshes at this time. SIR-C/X-SAR is sensitive to the moisture of soil and vegetation and can sense this freeze-thaw cycle and the summer- fall seasonal transition over forested areas in particular. Optical sensors, by contrast, are blind to these regions, which are perpetually obscured by thick cloud cover. These changes were detected by comparing the April and October color composite images of L-band data in red, C- band data in green and X-band (vertically received and transmitted) in blue. The changes in intensity of each color over lakes, various forest stands and clear cuts in the two images is striking. Lakes such as Lake Heiberg, Crabtree Lake and Williams Lake, in the right middle part of the image, are frozen in April (appearing in bright blue) and melted (appearing in black) in October. The higher intensity of blue over lakes in April is due to low penetration of the X-band (vertically received and transmitted) and the radar's high sensitivity to surface features. Forest stands also exhibit major changes between the two images. The red areas in the October image are old jack pine canopies that cause higher return at L-band because of their moist condition in late summer compared to their partially frozen condition in April (in purple). Similarly, in the areas near the middle of the image, where black spruce and mixed aspen and jack pine trees dominate, the contrast between blue in October and red and green in April is an indication that the top of the canopy (needles and branches) were frozen in April and moist in October. The changes due to deforestation by logging companies or natural fires can also be detected by comparing the images. For example, the small blue area near the intersection of Harding Road and Highway 120 is the result of logging which occurred after the April data was acquired. The surface area of clear cut is approximately 4 hectares, which is calculated from the high-resolution capability of the radar images and verified by scientists participating in fieldwork during the mission. ----- Spaceborne Imaging Radar-C and X-band Synthetic Aperture Radar (SIR-C/X- SAR) is part of NASA's Mission to Planet Earth. The radars illuminate Earth with microwaves, allowing detailed observations at any time, regardless of weather or sunlight conditions. SIR-C/X-SAR uses three microwave wavelengths: L-band (24 cm), C-band (6 cm) and X-band (3 cm). The multi-frequency data will be used by the international scientific community to better understand the global environment and how it is changing. The SIR-C/X-SAR data, complemented by aircraft and ground studies, will give scientists clearer insights into those environmental changes which are caused by nature and those changes which are induced by human activity. SIR-C w as developed by NASA's Jet Propulsion Laboratory. X-SAR was developed by the Dornier and Alenia Spazio companies for the German space agency, Deutsche Agentur fuer Raumfahrtangelegenheiten (DARA), and the Italian space agency, Agenzia Spaziale Italiana (ASI), with the Deutsche Forschungsanstalt fuer Luft und Raumfahrt e.V.(DLR), the major partner in science, operations and data processing of X-SAR. |
|
Dark Globule in IC 1396
| Title |
Dark Globule in IC 1396 |
| Description |
NASA's Spitzer Space Telescope image of a glowing stellar nursery provides a spectacular contrast to the opaque cloud seen in visible light. The Elephant's Trunk Nebula is an elongated dark globule within the emission nebula IC 1396 in the constellation of Cepheus. Located at a distance of 2,450 light-years, the globule is a condensation of dense gas that is barely surviving the strong ionizing radiation from a nearby massive star. The globule is being compressed by the surrounding ionized gas. The dark globule is seen in silhouette at visible-light wavelengths, backlit by the illumination of a bright star located to the left of the field of view. The Spitzer Space Telescope pierces through the obscuration to reveal the birth of new protostars, or embryonic stars, and previously unseen young stars. The infrared image, which transforms the dark cloud into a 'flying dragon,' was obtained by Spitzer's infrared array camera. The image is a four-color composite of invisible light, showing emissions from wavelengths of 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange) and 8.0 microns (red). The filamentary appearance of the globule results from the sculpting effects of competing physical processes. The winds from a massive star, located to the left of the image, produce a dense circular rim comprising the 'head' of the globule and a swept-back tail of gas. A pair of young stars (LkHa 349 and LkHa 349c) that formed from the dense gas has cleared a spherical cavity within the globule head. While one of these stars is significantly fainter than the other in the visible-light image, they are of comparable brightness in the infrared Spitzer image. This implies the presence of a thick and dusty disc around LkHa 349c. Such circumstellar discs are the precursors of planetary systems. They are much thicker in the early stages of stellar formation when the placental planet-forming material (gas and dust) is still present. |
|
Dark Globule in IC 1396
| Title |
Dark Globule in IC 1396 |
| Description |
NASA's Spitzer Space Telescope image of a glowing stellar nursery provides a spectacular contrast to the opaque cloud seen in visible light. The Elephant's Trunk Nebula is an elongated dark globule within the emission nebula IC 1396 in the constellation of Cepheus. Located at a distance of 2,450 light-years, the globule is a condensation of dense gas that is barely surviving the strong ionizing radiation from a nearby massive star. The globule is being compressed by the surrounding ionized gas. The dark globule is seen in silhouette at visible-light wavelengths, backlit by the illumination of a bright star located to the left of the field of view. The Spitzer Space Telescope pierces through the obscuration to reveal the birth of new protostars, or embryonic stars, and previously unseen young stars. The infrared image, which transforms the dark cloud into a 'flying dragon,' was obtained by Spitzer's infrared array camera. The image is a four-color composite of invisible light, showing emissions from wavelengths of 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange) and 8.0 microns (red). The filamentary appearance of the globule results from the sculpting effects of competing physical processes. The winds from a massive star, located to the left of the image, produce a dense circular rim comprising the 'head' of the globule and a swept-back tail of gas. A pair of young stars (LkHa 349 and LkHa 349c) that formed from the dense gas has cleared a spherical cavity within the globule head. While one of these stars is significantly fainter than the other in the visible-light image, they are of comparable brightness in the infrared Spitzer image. This implies the presence of a thick and dusty disc around LkHa 349c. Such circumstellar discs are the precursors of planetary systems. They are much thicker in the early stages of stellar formation when the placental planet-forming material (gas and dust) is still present. |
|
Dark Globule in IC 1396
| Title |
Dark Globule in IC 1396 |
| Description |
NASA's Spitzer Space Telescope image of a glowing stellar nursery provides a spectacular contrast to the opaque cloud seen in visible light. The Elephant's Trunk Nebula is an elongated dark globule within the emission nebula IC 1396 in the constellation of Cepheus. Located at a distance of 2,450 light-years, the globule is a condensation of dense gas that is barely surviving the strong ionizing radiation from a nearby massive star. The globule is being compressed by the surrounding ionized gas. The dark globule is seen in silhouette at visible-light wavelengths, backlit by the illumination of a bright star located to the left of the field of view. The Spitzer Space Telescope pierces through the obscuration to reveal the birth of new protostars, or embryonic stars, and previously unseen young stars. The infrared image, which transforms the dark cloud into a 'flying dragon,' was obtained by Spitzer's infrared array camera. The image is a four-color composite of invisible light, showing emissions from wavelengths of 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange) and 8.0 microns (red). The filamentary appearance of the globule results from the sculpting effects of competing physical processes. The winds from a massive star, located to the left of the image, produce a dense circular rim comprising the 'head' of the globule and a swept-back tail of gas. A pair of young stars (LkHa 349 and LkHa 349c) that formed from the dense gas has cleared a spherical cavity within the globule head. While one of these stars is significantly fainter than the other in the visible-light image, they are of comparable brightness in the infrared Spitzer image. This implies the presence of a thick and dusty disc around LkHa 349c. Such circumstellar discs are the precursors of planetary systems. They are much thicker in the early stages of stellar formation when the placental planet-forming material (gas and dust) is still present. |
|
NASA TV's This Week @NASA, J
A NASA-sponsored mission in
06/25/10
| Description |
A NASA-sponsored mission in Alaska is exploring how changes in the Arctic's sea ice cover may be contributing to global warming.* Now, after years of continuous service to more than a dozen missions, NASA's Tracking and Data Relay Satellite, TDRS 1 is retiring.* The replica Orion crew module used in the highly-successful Launch Abort system Pad Abort-1 flight test in New Mexico May 6 has returned to the Dryden Flight Research Center. * The Glenn Research Center's Plum Brook Station and the Marshall Space Flight Center welcomed members of the STS-131 crew to share highlights from their recent 15-day mission to the International Space Station. * While soccer fans around the world watch and await the winner of the 2010 World Cup, student players from the U.S. and Canada heard scientists and engineers from the Ames Research Center's Fluid Dynamics Laboratory explain the aerodynamics of the “Jabulani'' soccer ball.* |
| Date |
06/25/10 |
|
NASA TV's This Week at NASA,
President Barack Obama made
04/16/10
| Description |
President Barack Obama made a trip to the Kennedy Space Center on Thursday to explain his plan for America's space program. Accompanied by Florida Senator and former shuttle astronaut Bill Nelson, Apollo astronaut Buzz Aldrin, and NASA Administrator Charles Bolden, President Obama addressed an audience comprised of elected officials, leaders from industry, academia and KSC employees. * STS-125, the fifth space shuttle servicing mission that gave the Hubble Space Telescope a new lease on life, and L-CROSS, the mission that definitively proved the presence of water on the moon, received awards from the Space Foundation at its 26th annual National Space Symposium in Colorado Springs. * What do a lunar habitat module, paper that captures sound as energy, and a drug delivery system for use in space have in common? They're all concepts being developed for commercialization by high school students who competed in the Conrad Foundation's Innovation Summit. * Huntsville's U.S. Space & Rocket Center hosted the 17th annual Great Moonbuggy Race. Competing were upwards of 600 student drivers, engineers and mechanics representing more than 70 teams from 18 states, Puerto Rico, Canada, Germany, India and Romania. * The John Glenn Lecture Series at the Smithsonian's National Air and Space Museum in Washington honored the 40th anniversary of the Apollo 13 mission. Joining Commander Jim Lovell was Apollo 13 Flight Controller, Gene Kranz, Lunar Module Pilot, Fred Haise, and astronaut Ken Mattingly, who was replaced on the mission by the late Jack Swiegert after contracting measles just before the mission's start. * Yuri's Night 2010 celebrated humankind's achievements in space exploration with music, dance, fashion, and art at countless locations around the world, including several NASA centers. |
| Date |
04/16/10 |
|
Mount Saint Helens
| title |
Mount Saint Helens |
| description |
Mount Saint Helens exemplifies how Earth's topographic form can change greatly even within our lifetimes. The mountain is one of several prominent volcanoes of the Cascade Range that stretches from British Columbia, Canada, southward through Washington, Oregon and into northern California. Mount Adams (left background) and Mount Hood (right background) are also seen in this view, which was created entirely from elevation data produced by the Shuttle Radar Topography Mission. Prior to 1980, Mount Saint Helens had a shape roughly similar to other Cascade peaks, a tall, bold, irregular conic form that rose to 9,677 feet (2,950 meters). However, the explosive eruption of May 18, 1980, caused the upper 1,300 feet (400 meters) of the mountain to collapse, slide and spread northward, covering much of the adjacent terrain (lower left), leaving a crater atop the greatly shortened mountain. Subsequent eruptions built a volcanic dome within the crater, and the high rainfall of this area lead to substantial erosion of the poorly consolidated landslide material. Eruptions at Mount Saint Helens subsided in 1986, but renewed volcanic activity here and at other Cascade volcanoes is inevitable. Predicting such eruptions still presents challenges, but migration of magma within these volcanoes often produces distinctive seismic activity and minor but measurable topographic changes that can give warning of a potential eruption. Image credit: NASA/JPL/NGA |
|
Chandra X-ray Image of Earth
| Name |
Chandra X-ray Image of Earth Aurora on Feb 15, 2004 |
|
3-D Perspective Pasadena, Ca
| Title |
3-D Perspective Pasadena, California |
| Full Description |
This perspective view shows the western part of the city of Pasadena, California, looking north towards the San Gabriel Mountains. Portions of the cities of Altadena and La Canada, Flintridge are also shown. The image was created from three datasets: the Shuttle Radar Topography Mission (SRTM) supplied the elevation data, Landsat data from November 11, 1986 provided the land surface color (not the sky) and U.S. Geological Survey digital aerial photography provides the image detail. The Rose Bowl, surrounded by a golf course, is the circular feature at the bottom center of the image. The Jet Propulsion Laboratory is the cluster of large buildings north of the Rose Bowl at the base of the mountains. A large landfill, Scholl Canyon, is the smooth area in the lower left corner of the scene. This image shows the power of combining data from different sources to create planning tools to study problems that affect large urban areas. In addition to the well-known earthquake hazards, Southern California is affected by a natural cycle of fire and mudflows. Wildfires strip the mountains of vegetation, increasing the hazards from flooding and mudflows for several years afterwards. Data such as shown on this image can be used to predict both how wildfires will spread over the terrain and also how mudflows will be channeled down the canyons. The Shuttle Radar Topography Mission (SRTM), launched on February 11, 2000, uses the same radar instrument that comprised the Spaceborne Imaging Radar-C/X-Band Synthetic Aperture Radar (SIR-C/X-SAR) that flew twice on the Space Shuttle Endeavour in 1994. The mission was designed to collect three dimensional measurements of the Earth's surface. To collect the 3-D data, engineers added a 60-meter-long (200-foot) mast, an additional C-band imaging antenna and improved tracking and navigation devices. The mission is a cooperative project between the National Aeronautics and Space Administration (NASA), the National Imagery and Mapping Agency (NIMA) and the German (DLR) and Italian (ASI) space agencies. It is managed by NASA's Jet Propulsion Laboratory, Pasadena, CA, for NASA's Earth Science Enterprise, Washington, DC. Size: 5.8 km (3.6 miles) x 10 km (6.2 miles) Location: 34.16 deg. North lat., 118.16 deg. West lon. Orientation: Looking North Original Data Resolution: SRTM, 30 meters, Landsat,30 meters, Aerial Photo, 3 meters (no vertical exaggeration) |
| Date |
02/16/2000 |
| NASA Center |
Jet Propulsion Laboratory |
|
McCandless on Arm in Aft Pay
| Title |
McCandless on Arm in Aft Payload Bay |
| Full Description |
Astronaut Bruce McCandless II, STS-41B mission specialist, tests a Mobile Foot Restraint (MFR) attached to the Remote Manipulator System (RMS) aboard the Space Shuttle Challenger. McCandless appears to be walking on cargo, but is realy being flown over it by the combination MFR and RMS. His helmet visor reflects parts of the payload bay that can't be seen in the larger portion of the photo. Behind him can be seen both the Orbital Maneuvering System (OMS) pods. |
| Date |
02/13/1984 |
| NASA Center |
Johnson Space Center |
|
McCandless with Space Screw
| Title |
McCandless with Space Screw Gun |
| Full Description |
EVA Astronaut Bruce McCandless II, is using a special power tool to conduct an experiment. His feet are anchored in the mobile foot restraints, which are connected to the Remote Manipulator System's (RMS) End Effector. The Shuttle pallet satellite (SPAS-01A) serves as a test subject for McCandless's experiment. The SPAS-01A is located in the center of the open cargo bay. Behind him is the protective cradle for the Westar VI satellite. |
| Date |
02/12/1984 |
| NASA Center |
Johnson Space Center |
|
Armed and Ready
| Title |
Armed and Ready |
| Full Description |
STS-49 Mission Specialist Pierre Thuot is perched on the end effector of the Robot Arm (Remote Manipulator System/RMS), with the Intelsat VI capture bar. This would be one of many attempts to "grapple" the Intelsat VI satellite which was rendered inoperative when its Payload Assist Module (PAM) motor failed to fire thus preventing it from reaching an operational altitude. |
| Date |
05/13/1992 |
| NASA Center |
Johnson Space Center |
|
Artist's Conception of Space
| Title |
Artist's Conception of Space Station Freedom |
| Full Description |
Alan Chinchar's 1991 rendition of the Space Station Freedom in orbit. The painting depicts the completed space station. Earth is used as the image's backdrop with the Moon and Mars off in the distance. Freedom was to be a permanently crewed orbiting base to be completed in the mid 1990's. It was to have a crew of 4. Freedom was an attempt at international cooperation that attempted to incorporate the technological and economic assistance, of the United States, Canada, Japan, and nine European nations. The image shows four pressurized modules (three laboratories and a habitat module) and six large solar arrays which were expected to generate 56,000 watts of electricity for both scientific experiments and the daily operation of the station. Space Station Freedom never came to fruition. Instead, in 1993, the original partners, as well as Russia, pooled their resources to create the International Space Station. |
| Date |
1991 |
| NASA Center |
Headquarters |
|
Challenger as seen from SPAS
| Title |
Challenger as seen from SPAS |
| Full Description |
Full view of Space Shuttle Orbiter Challenger in space, taken by the Space Pallet Satellite (SPAS). A heavily cloud-covered portion of the earth forms the backdrop for this scene of Challenger. Visible in the payload bay are the protective cradles for the Palapa-B and Telesat F communications satellites, the pallet for the NASA Office of Space and Terrestrial Applications (OSTA-2), the Remote Manipulator System (RMS) robot arm in the shape of the numeral seven and the KU- band antenna. A number of GetAway Special (GAS) canisters are also visible along the port side. |
| Date |
06/22/1983 |
| NASA Center |
Johnson Space Center |
|
Communication Technology Sat
| Title |
Communication Technology Satellite |
| Full Description |
The Communication Technology Satellite was launched from NASA's Kennedy Space Center, Florida, on January 17, 1976 and operated until October 1979. This high-powered spacecraft was the result of a five- year effort of international cooperation between NASA and Canada's Department of Communications. Canada designed and built the spacecraft and NASA tested, launched, and operated the CTS. The Canadians later renamed the spacecraft after the mythical Greek messenger god, Hermes. The transmitter improved 10-20 times the broadcast power of typical communication satellites of the era. With more power transmitted by the satellite, it was possible to use smaller and cheaper ground stations thus paving the way for applications such as direct broadcast television. The CTS is the second satellite designed to transmit high-quality color television. The first was the Application Technology Satellite (ATS), which was launched December 17, 1966. |
| Date |
12/16/75 |
| NASA Center |
Kennedy Space Center |
|
Robot Arm Over Earth with Su
| Title |
Robot Arm Over Earth with Sunburst |
| Full Description |
View of the Remote Manipulator System (RMS) end effector over an Earth limb with a solar starburst pattern behind it. |
| Date |
06/01/1996 |
| NASA Center |
Johnson Space Center |
|
SAFER Rescue System Tested
| Title |
SAFER Rescue System Tested |
| Full Description |
Astronauts Carl J. Meade and Mark C. Lee (red strip on suit) test the new Simplified Aid for EVA Rescue (SAFER) system some 130 nautical miles above Earth. The pair was actually performing an in-space rehearsal or demonstration of a contingency rescue using never-before flown hardware. Meade, who here wears the small back-pack unit with its complementary chest-mounted control unit, and Lee anchored to the Space Shuttle Discovery's Remote Manipulator System (RMS) robot arm, took turns using the SAFER hardware during their shared space walk. |
| Date |
09/16/1994 |
| NASA Center |
Johnson Space Center |
|
SAFER Tests by Meade and Lee
| Title |
SAFER Tests by Meade and Lee |
| Full Description |
Astronauts Carl J. Meade and Mark C. Lee (red stripe on suit) test the Simplified Aid for EVA Rescue (SAFER) system some 130 nautical miles from Earth. The pair were actually performing an in-space rehearsal or demonstration of a contingency rescue using the never- before flown hardware. Meade, who here wears the small back-pack unit with its complementary chest-mounted control unit, and Lee, anchored to Discovery's Remote Manipulator System (RMS) robot arm, took turns using the SAFER hardware during their shared space walk of September 16, 1994. |
| Date |
09/16/1994 |
| NASA Center |
Johnson Space Center |
|
Structures in Space
| Title |
Structures in Space |
| Full Description |
Astronaut Jerry L. Ross, anchored to the foot restraint on the Remote Manipulator System (RMS), approaches the tower-like Assembly Concept for Construction of Erectable Space Structures (ACCESS) device. The structure was just deployed by Ross and astronaut Sherwood Spring as the Atlantis flies over white clouds and blue ocean waters of the Atlantic. |
| Date |
12/01/1985 |
| NASA Center |
Johnson Space Center |
|
Freedom Space Station Concep
| Title |
Freedom Space Station Concept |
| Full Description |
A concept drawing of Space Station Freedom. Freedom was to be a permanently crewed orbiting base in orbit to be completed in the mid 1990's. It was to have a crew of 4. Freedom was an attempt at international cooperation that attempted to incorporate the technological and economic assistance, of the United States, Canada, Japan, and nine European nations. The image shows four pressurized modules (three laboratories and a habitat module) and six large solar arrays which were expected to generate 56,000 watts of electricity for both scientific experiments and the daily operation of the station. Space Station Freedom never came to fruition. Instead, in 1993, the original partners, as well as Russia, pooled their resources to create the International Space Station. |
| Date |
UNKNOWN |
| NASA Center |
Headquarters |
|
Gernhardt on Robot Arm
| Title |
Gernhardt on Robot Arm |
| Full Description |
The pale blue Earth serves as backdrop for astronaut Michael Gernhardt during his Extravehicular Activity (EVA). He is standing on a Manipulator Foot Restraint (MFR) attached to the Remote Manipulator System (RMS). He is positioned over the Payload Bay and Endeavour's forward section is reflected in his visor. A thermal cube is attached to the RMS and records temperatures during spacesuit evaluations. Unlike earlier spacewalking astronauts, Gernhardt was able to use an electronic cuff checklist, a prototype developed for the assembly of the International Space Station (ISS). |
| Date |
09/16/1995 |
| NASA Center |
Johnson Space Center |
|
Hubble First Servicing EVA
| Title |
Hubble First Servicing EVA |
| Full Description |
Astronaut F. Story Musgrave, anchored on the end of the Remote Manipulator System (RMS) arm, prepares to be elevated to the top of the Hubble Space Telescope (HST) to install protective covers on the magnetometers. Astronaut Jeffrey A. Hoffman inside payload bay, assisted Musgrave with final servicing tasks on the telescope, wrapping up five days of space walks. |
| Date |
12/09/1993 |
| NASA Center |
Johnson Space Center |
|
Hubble Redeployment
| Title |
Hubble Redeployment |
| Full Description |
Attached to the "robot arm" the Hubble Space Telescope is unberthed and lifted up into the sunlight during this the second servicing mission designated HST SM-02. |
| Date |
02/19/1997 |
| NASA Center |
Johnson Space Center |
|
Thornton Prepares to Release
| Title |
Thornton Prepares to Release Hubble Array |
| Full Description |
To run all their systems, satellites need a way to generate power for months, even years. Most Earth-orbiting spacecraft, like the Hubble Space Telescope, rely on solar cells to recharge their onboard batteries. But solar panels have their own set of problems. They must be lightweight and flexible to fit inside a relatively small launch vehicle. Consequently, they tend to be fragile, and several satellites have had to cope with damaged panels once in orbit. That is what happened to the Hubble Space Telescope. Fortunately, the telescope was designed for on-orbit repairs, and astronauts were able to remove the damaged panel and replace it with a new one. In this image, Astronaut Kathy Thornton releases the old panel into low-Earth orbit during the first Hubble Space Telescope Servicing Mission in 1993. Earth's gravitation pulled the jettisoned panel toward Earth's atmosphere, where it entered and ultimately burned up. |
| Date |
10/14/1994 |
| NASA Center |
Johnson Space Center |
|
Intelsat VI Capture Attempt
| Title |
Intelsat VI Capture Attempt |
| Full Description |
The first single crewmember EVA capture attempt of the Intelsat VI as seen from Endeavour's aft flight deck windows. EVA Mission Specialist Pierre Thuot standing on the Remote Manipulator System (RMS) end effector platform, with the satellite capture bar attempting to attach it to the free floating communications satellite. |
| Date |
05/16/1992 |
| NASA Center |
Johnson Space Center |
|
Wisoff on the Arm
| Title |
Wisoff on the Arm |
| Full Description |
Against the blackness of space, Mission Specialist Peter J.K. Wisoff, wearing an extravehicular mobility unit, stands on a Portable Foot Restraint (PFR), Manipulator Foot Restrait (MFR) attached to the End Effector of the Remote Manipulator System (RMS), colloquially known as the "robot arm". Wisoff is being maneuvered above Endeavour's payload bay as part of Detailed Test Objective (DTO) extravehicular activity procedures. DTO results will assist in refining several procedures being developed to service the Hubble Space Telescope on mission STS-61 in December 1993. The Earth's surface and Discovery's payload bay are reflected in Wisoff's helmet visor. |
| Date |
06/25/1993 |
| NASA Center |
Johnson Space Center |
|
Hubble Resolves Quasars' Hos
| Title |
Hubble Resolves Quasars' Host Galaxies |
|
Bright Star Birth Region in
| Title |
Bright Star Birth Region in a Dim Galaxy |
|
Hubble Space Telescope Finds
| Title |
Hubble Space Telescope Finds Stellar Graveyard |
|
Hubble Pinpoints Distant Sup
| Title |
Hubble Pinpoints Distant Supernovae |
| General Information |
What is an American Astronomical Society Meeting release? A major news announcement issued at an American Astronomical Society meeting, the premier astronomy conference. Peering halfway across the universe to analyze light from exploded stars that died long before our Sun even existed, the Hubble telescope has allowed astronomers to determine that the expansion of the cosmos has not slowed since the initial impetus of the Big Bang. Thus, the universe's expansion should continue to balloon outward indefinitely. These results are based on unprecedented distance measurements to supernovae that are so far away they allow astronomers to determine if the universe was expanding at a faster rate long ago. These images showcase three of the supernovae used in the survey. The arrows in the bottom row of pictures pinpoint these exploding stars, the top row of images shows the regions where the supernovae reside. Read more: * Release Text [ http://hubblesite.org/newscenter/archive/releases/1998/02/text/ ] |
|
Hubble's Panoramic Portrait
| Title |
Hubble's Panoramic Portrait of a Vast Star-Forming Region |
|
Hubble's Panoramic Portrait
| Title |
Hubble's Panoramic Portrait of a Vast Star-Forming Region |
|
Hubble's Panoramic Portrait
| Title |
Hubble's Panoramic Portrait of a Vast Star-Forming Region |
|
Burst of Star Formation Driv
| Title |
Burst of Star Formation Drives Bubble in Galaxy's Core |
|
New View of Primordial Heliu
| Title |
New View of Primordial Helium Traces the Structure of Early Universe |
|
Hubble's Largest Galaxy Port
| Title |
Hubble's Largest Galaxy Portrait Offers a New High-Definition View |
| General Information |
What is Hubble Heritage? A monthly showcase of new and archival Hubble images. Go to the Heritage site. Giant galaxies weren?t assembled in a day. Neither was this Hubble Space Telescope image of the face-on spiral galaxy Messier 101 (M101). It is the largest and most detailed photo of a spiral galaxy that has ever been released from Hubble. The galaxy?s portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 in March 1994, September 1994, June 1999, November 2002, and January 2003. The newly composed image also includes elements from images from ground-based photos. |
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Hubble's Largest Galaxy Port
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Hubble's Largest Galaxy Portrait Offers a New High-Definition View |
| General Information |
What is Hubble Heritage? A monthly showcase of new and archival Hubble images. Go to the Heritage site. Giant galaxies weren?t assembled in a day. Neither was this Hubble Space Telescope image of the face-on spiral galaxy Messier 101 (M101). It is the largest and most detailed photo of a spiral galaxy that has ever been released from Hubble. The galaxy?s portrait is actually composed of 51 individual exposures taken with Hubble's Advanced Camera for Surveys and the Wide Field and Planetary Camera 2 in March 1994, September 1994, June 1999, November 2002, and January 2003. The newly composed image also includes elements from images from ground-based photos. |
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Hubble Eyes Star Birth in th
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Hubble Eyes Star Birth in the Extreme |
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Hubble Sees Faintest Stars i
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Hubble Sees Faintest Stars in a Globular Cluster |
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Hubble Sees Faintest Stars i
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Hubble Sees Faintest Stars in a Globular Cluster |
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Hubble Sees Faintest Stars i
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Hubble Sees Faintest Stars in a Globular Cluster |
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Hubble Sees Faintest Stars i
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Hubble Sees Faintest Stars in a Globular Cluster |
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Hubble Sees Faintest Stars i
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Hubble Sees Faintest Stars in a Globular Cluster |
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Hubble Zooms In on Heart of
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Hubble Zooms In on Heart of Mystery Comet |
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Hubble Zooms In on Heart of
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Hubble Zooms In on Heart of Mystery Comet |
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How White Dwarfs Get Their '
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How White Dwarfs Get Their 'Kicks' |
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Holiday Wishes from the Hubb
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Holiday Wishes from the Hubble Space Telescope |
| General Information |
What is Hubble Heritage? A monthly showcase of new and archival Hubble images. Go to the Heritage site. Resembling festive lights on a holiday wreath, this NASA/ESA Hubble Space Telescope image of the nearby spiral galaxy M74 is an iconic reminder of the impending season. Bright knots of glowing gas light up the spiral arms, indicating a rich environment of star formation. M74 is located roughly 32 million light-years away in the direction of the constellation Pisces, the Fish. The image is a composite of Advanced Camera for Surveys data taken in 2003 and 2005. |
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