|
|
Stennis Engineers in Area Sc
Engineers with NASA's propul
1/1/92
| Description |
Engineers with NASA's propulsion programs visit area schools to teach students about the principles of rocketry and propulsion, as well as the many career opportunities available in the nation's space program. |
| Date |
1/1/92 |
|
SSME Processing
Technicians at Stennis Space
1/1/92
| Description |
Technicians at Stennis Space Center prepare a Space Shuttle Main Engine to be transported to the center's propulsion test complex where the engine will be test fired. |
| Date |
1/1/92 |
|
A-1 Test, A-2 In Foreground
A Space Shuttle Main Engine
1/1/92
| Description |
A Space Shuttle Main Engine is test fired on the A-1 test stand at Stennis Space Center's test complex with the A-2 stand in the foreground. |
| Date |
1/1/92 |
|
High Pressure Industrial Wat
In conjunction with Space Sh
1/1/92
| Description |
In conjunction with Space Shuttle Main Engine testing at Stennis, the Nordberg Water Pumps at the High Pressure Industrial Water Facility provide water for cooling the flame deflectors at the test stands during test firings. |
| Date |
1/1/92 |
|
Stennis Space Center Test Fa
This aerial view taken in 19
1/1/92
| Description |
This aerial view taken in 1992 shows propulsion test facilities at Stennis Space Center. |
| Date |
1/1/92 |
|
SSME Night Firing
A Space Shuttle Main Engine
1/1/92
| Description |
A Space Shuttle Main Engine test lights up the night sky at Stennis Space Center. The test pictured occurred on the B-1, SSC's largest of three test stands used for shuttle main engine testing. |
| Date |
1/1/92 |
|
GLL/EM15
This mosaic picture of the M
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. ##### |
|
GLL/EM17
This false-color mosaic was
12/22/92
| Date |
12/22/92 |
| Description |
This false-color mosaic was constructed from a series of 53 images taken through three spectral filters by Galileo's imaging system as the spacecraft flew over the northern regions of the Moon on December 7, 1992. The part of the Moon vlsible from Earth is on the left side in this view. The color mosaic shows compositional variations in parts of the Moon's northern hemisphere. Bright pinkish areas are highlands materials, such as those surrounding the oval lava-filled Crisium impact basin toward the bottom of the picture. B1ue to orange shades indicate volcanic lava flows. To the left of Crisium, the dark blue Mare Tranquillitatis is richer in titanium than the green and orange maria above it. Thin mineral-rich soils associated with relatively recent impacts are represented by light blue colors, the youngest craters have prominent blue rays extending from them. 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. ##### |
|
Extreme Planets
| Title |
Extreme Planets |
| Description |
This artist's concept depicts the pulsar planet system discovered by Aleksander Wolszczan in 1992. Wolszczan used the Arecibo radio telescope in Puerto Rico to find three planets - the first of any kind ever found outside our solar system - circling a pulsar called PSR B1257+12. Pulsars are rapidly rotating neutron stars, which are the collapsed cores of exploded massive stars. They spin and pulse with radiation, much like a lighthouse beacon. Here, the pulsar's twisted magnetic fields are highlighted by the blue glow. All three pulsar planets are shown in this picture, the farthest two from the pulsar (closest in this view) are about the size of Earth. Radiation from charged pulsar particles would probably rain down on the planets, causing their night skies to light up with auroras similar to our Northern Lights. One such aurora is illustrated on the planet at the bottom of the picture. Since this landmark discovery, more than 160 extrasolar planets have been observed around stars that are burning nuclear fuel. The planets spotted by Wolszczan are still the only ones around a dead star. They also might be part of a second generation of planets, the first having been destroyed when their star blew up. The Spitzer Space Telescope's discovery of a dusty disk around a pulsar might represent the beginnings of a similarly "reborn" planetary system. |
|
Stellar Rubble May Be Planet
| Title |
Stellar Rubble May Be Planetary Building Blocks |
| Description |
This artist's concept depicts a type of dead star called a pulsar and the surrounding disk of rubble discovered by NASA's Spitzer Space Telescope. The pulsar, called 4U 0142+61, was once a massive star until about 100,000 years ago when it blew up in a supernova explosion and scattered dusty debris into space. Some of that debris was captured into what astronomers refer to as a "fallback disk," now circling the remaining stellar core, or pulsar. The disk resembles protoplanetary disks around young stars, out of which planets are thought to be born. Supernovas are a source of iron, nitrogen and other "heavy metals" in the universe. They spray these elements out into space, where they eventually come together in clouds that give rise to new stars and planets. The Spitzer finding demonstrates that supernovas might also contribute heavy metals to their own planets, a possibility that was first suggested when astronomers discovered planets circling a pulsar called PSR B1257+12 in 1992. |
|
NASA's First Headquarters
| title |
NASA's First Headquarters |
| date |
10.21.1961 |
| description |
The Little White House at 1520 H Street, NW, in Washington, DC served as NASA Headquarters from 1958 until October 1961. Built in 1820 by Richard Cutts, in 1837 it became the home of Mrs. Dolly Payne Madison, wife of President James Madison. Named the Dolly Madison House, she lived there till her death in 1849. In 1886 the Dolly Madison House became the private Cosmos Club. After restoration in the early 1960's, the Dolly Madison House became the offices for the Federal Judicial Center. In 1992 the Federal Judicial Center switched locations and the U.S. Court of Appeals for the Federal Circuit moved into this historic house. In the fall of 1961, NASA moved its headquarters to Federal Building 6 located at 400 Maryland Avenue, SW, in Washington. In 1963 NASA administration expanded into Federal Building 10-B at 600 Independence Avenue, SW and the Reporters Building at 300 7th St., SW. Since 1992, NASA Headquarters has been located at 300 E Street SW. *Image Credit*: NASA |
|
The Earth-Moon System
| title |
The Earth-Moon System |
| date |
12.16.1992 |
| description |
Eight days after its final encounter with the Earth, the Galileo spacecraft looked back and captured this remarkable view of the Earth and Moon. The image was taken from a distance of about 6.2 million kilometers (3.9 million miles). The picture was constructed from images taken through the violet, red, and 1.0-micron infrared filters. The Moon is in the foreground, moving from left to right. The brightly-colored Earth contrasts strongly with the Moon, which reflects only about one-third as much sunlight as the Earth. Contrast and color have been computer-enhanced for both objects to improve visibility. Antarctica is visible through clouds (bottom). The Moon's far side is seen, the shadowy indentation in the dawn terminator is the south pole Aitken Basin, one of the largest and oldest lunar impact features. *Image Credit*: NASA |
|
Giotto
| title |
Giotto |
| description |
The Giotto space probe, launched in 1985 on an Ariane 1 V14 launcher, brushed past the hidden nucleus of Halley's comet in 1986. Its camera recorded many images that gave scientists an unique opportunity (the comet will not pass close to the Earth again until 2061) to increase their knowledge of comets. Though damaged by the multiple impacts, Giotto carried on with its mission. After a period of hibernation, it was reactived in 1990 for a fresh task - flying by comet Grigg-Skjellerup on 10 July 1992. Giotto was the first probe to study two comets. *Image Credit*: European Space Agency |
|
Volcano Southeast of Phoebe
| title |
Volcano Southeast of Phoebe Regio,Venus with Emissivity Data |
| date |
11.11.1992 |
| description |
Magellan press release image showing radio-thermal emission (emissivity). Red represents high emissivity and blue low. The image is centered at 12.5S,261E, southeast of Phoebe Regio, Venus and is 587 km on a side. The unnamed volcano is about 2 km high and shows low emissivity at the summit, which could indicate the presence of pyrrohtite or pyrite, minerals which may not be stable at lower altitudes. (Magellan press release P-40698) *Image Credit*: NASA |
|
Chicxulub Crater
| title |
Chicxulub Crater |
| date |
01.24.1992 |
| description |
This is a computer-generated gravity map image of the Chicxulub Crater found on Mexico's Yucatan Peninsula. The buried impact structure has been implicated in the mass extinction of life 65 million years ago and may be much larger than scientists first suspected. New analyses of gravity measurements in the region have turned up evidence that the feature is a multiring basin with a fourth, outer ring about 300 kilometers in diameter. At this diameter, the Chixulub Basin represents one of the largest collisions in the inner solar system since the so-called "heavy bombardment" ended almost four billion years ago. (The period of heavy bombardment was caused by the impact of debris from the early formation of the solar system raining in on the newly formed planets.) The only comparable post-bombardment basin is the 280-kilometer-diameter Mead Basin on Venus. *Image Credit*: Virgil L. Sharpton, University of Alaska, Fairbanks |
|
Venus - 3D Perspective View
| title |
Venus - 3D Perspective View of Maat Mons |
| date |
04.22.1992 |
| description |
Maat Mons is displayed in this computer generated three-dimensional perspective of the surface of Venus. The viewpoint is located 634 kilometers (393 miles) north of Maat Mons at an elevation of 3 kilometers (2 miles) above the terrain. Lava flows extend for hundreds of kilometers across the fractured plains shown in the foreground, to the base of Maat Mons. The view is to the south with the volcano Maat Mons appearing at the center of the image on the horizon and rising to almost 5 kilometers (3 miles) above the surrounding terrain. Maat Mons is located at approximately 0.9 degrees north latitude, 194.5 degrees east longitude with a peak that ascends to 8 kilometers (5 miles) above the mean surface. Maat Mons is named for an Egyptian Goddess of truth and justice. Magellan synthetic aperture radar data is combined with radar altimetry to develop a three-dimensional map of the surface. The vertical scale in this perspective has been exaggerated 10 times. Rays cast in a computer intersect the surface to crate a three-dimensional perspective view. Simulated color and a digital elevation map developed by the U.S. Geological Survey are used to enhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft. The image was produced by the Solar System Visualization project and the Magellan Science team at the JPL Multimission Image Processing Laboratory and is a single frame from a video released at the April 22, 1992 news conference. *Image Credit*: JPL |
|
The Moon from Galileo's Pers
| title |
The Moon from Galileo's Perspective |
| date |
12.07.1992 |
| description |
During its flight, the Galileo spacecraft returned images of the Moon. The Galileo spacecraft took these images on December 7, 1992 on its way to explore the Jupiter system in 1995-97. The distinct bright ray crater at the bottom of the image is the Tycho impact basin. The dark areas are lava rock filled impact basins: Oceanus Procellarum (on the left), Mare Imbrium (center left), Mare Serenitatis and Mare Tranquillitatis (center), and Mare Crisium (near the right edge). This picture contains images through the Violet, 756 nm, 968 nm filters. The color is 'enhanced' in the sense that the CCD camera is sensitive to near infrared wavelengths of light beyond human vision. The Galileo project is managed for NASA's Office of Space Science by the Jet Propulsion Laboratory. *Image Credit*: NASA |
|
Moon - False Color Mosaic
| title |
Moon - False Color Mosaic |
| date |
12.08.1992 |
| description |
This false-color photograph is a composite of 15 images of the Moon taken through three color filters by Galileo's solid-state imaging system during the spacecraft's passage through the Earth-Moon system on December 8, 1992. When this view was obtained, the spacecraft was 425,000 kilometers (262,000 miles) from the Moon and 69,000 kilometers (43,000 miles) from Earth. The false-color processing used to create this lunar image is helpful for interpreting the surface soil composition. Areas appearing red generally correspond to the lunar highlands, while blue to orange shades indicate the ancient volcanic lava flow of a mare, or lunar sea. Bluer mare areas contain more titanium than do the orange regions. Mare Tranquillitatis, seen as a deep blue patch on the right, is richer in titanium than Mare Serenitatis, a slightly smaller circular area immediately adjacent to the upper left of Mare Tranquillitatis. Blue and orange areas covering much of the left side of the Moon in this view represent many separate lava flows in Oceanus Procellarum. The small purple areas found near the center are pyroclastic deposits formed by explosive volcanic eruptions. The fresh crater Tycho, with a diameter of 85 kilometers (53 miles), is prominent at the bottom of the photograph, where part of the Moon's disk is missing. *Image Credit*: JPL |
|
The Eagle has Landed
| title |
The Eagle has Landed |
| date |
04.01.1992 |
| description |
This is one in a series of remarkable photos documenting the daily lives of two of Kennedy Space Center's most famous residents: The Southern Bald Eagles which inhabit an enormous nest on the Kennedy Parkway North. Each fall, the eagles take up winter residence in the nest to breed and raise a new generation. Thanks to a remote-controlled Nikon camera installed yearly in the same pine tree as the nest, the activities of these magnificent birds are recorded on film. In 1992, a rare and unique event was captured by the camera when a second clutch of eggs was laid, even though a healthy eaglet was born a month earlier. Although it is impossible to determine if it is the same eagles returning each year, the continued tolerance shown by this pair to the human presence seems to indicate that they are the same couple. According to wildlife experts at the time the photo was taken, eight to nine pairs of bald eagles inhabit nests at the space center. The nest is particularly well-known because of its huge size and close proximity to a busy road. *Image Credit*: NASA |
|
Image is 60 arcsec per side.
| Name |
Image is 60 arcsec per side. |
|
ROSAT X-ray Image of RX J124
| Name |
ROSAT X-ray Image of RX J1242-11 |
|
Aaron Cohen
| Title |
Aaron Cohen |
| Full Description |
Aaron Cohen served as NASA Acting Deputy Administrator from February 19, 1992 to November 1, 1992. Mr. Cohen started at NASA's Johnson Space Center in 1962 working on the Apollo program. After Apollo he served as Manager of the Space Shuttle orbiter, directing the development and testing of the orbiter. In 1986 he assumed the position of Johnson Space Center Director. After retiring from NASA in 1993, Mr. Cohen became the Zachry Professor of Engineering at his alma mater, Texas A&M University. |
| Date |
12/20/1982 |
| NASA Center |
Johnson Space Center |
|
NASA Langley Magnetic Suspen
| Title |
NASA Langley Magnetic Suspension/Balance System |
| Full Description |
A shuttle model is magnetically suspended in the transparent hexagonal test section of the MIT/NASA Langley 6 inch MSBS. Massive power supplies are required to drive electromagnets for model position control. A unique electromagnetic position sensor, similar to a linear variable differential transformer, provides five degrees of freedom for the test model. The low speed (Mach 0.5) wind tunnel was hand crafted from mahogany. Aerodynamic forces on the test model are measured by the proportional electrical current used to hold the model in place. The system was built by MIT in the late sixties, and was relocated to Langley in the mid eighties. In a joint effort with Old Dominion University in 1992 the MSBS was used to test the aerodynamics of store separation, simulating a bomb released from an aircraft. The system has been donated to Old Dominion University. |
| Date |
6/11/1991 |
| NASA Center |
Langley Research Center |
|
NASA's First Headquarters
| Title |
NASA's First Headquarters |
| Full Description |
The Little White House at 1520 H Street, NW, in Washington, DC served as NASA Headquarters from 1958 until October 1961. Built in 1820 by Richard Cutts, in 1837 it became the home of Mrs. Dolly Payne Madison, wife of President James Madison. Named the Dolly Madison House, she lived there till her death in 1849. In 1886 the Dolly Madison House became the private Cosmos Club. After restoration in the early 1960's, the Dolly Madison House became the offices for the Federal Judicial Center. In 1992 the Federal Judicial Center switched locations and the U.S. Court of Appeals for the Federal Circuit moved into this historic house. In the fall of 1961, NASA moved its headquarters to Federal Building 6 located at 400 Maryland Avenue, SW, in Washington. In 1963 NASA administration expanded into Federal Building 10-B at 600 Independence Avenue, SW and the Reporters Building at 300 7th St., SW. Since 1992, NASA Headquarters has been located at 300 E Street, SW. |
| Date |
10/21/1961 |
| NASA Center |
Headquarters |
|
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 |
|
Night Time Test Firing
| Title |
Night Time Test Firing |
| Full Description |
A Space Shuttle Main Engine, (SSME) test firing lights up the night sky at the John C. Stennis Space Center in Hancock County, Mississippi. This test occurred on the B-1, SSC's largest of three test stands used for Shuttle main engine testing. |
| Date |
01/01/1992 |
| NASA Center |
Stennis Space Center |
|
Assembling Structures in the
| Title |
Assembling Structures in the Payload Bay |
| Full Description |
STS-49 Mission Specialist (MS) Kathryn C. Thornton (foreground) releases a strut from the Multipurpose Experiment Support Structure (MPESS) strut dispenser during Assembly of Station by Extravehicular Activity Methods (ASEM) procedures in Endeavour's payload bay. MS Thomas D. Akers, positioned on the opposite side of the MPESS, waits for Thornton to hand him the final strut. The two astronauts are building the ASEM structure during the mission's fourth EVA. The ASEM structure, locked in at four corners to payload retention latch assemblies (PRLAs), rises above the payload bay. In the background are the Intelsat cradle, the vertical tail, and the orbital maneuvering system (OMS) pods. The pale blue and white Earth is visible below. |
| Date |
05/01/1992 |
| NASA Center |
Johnson Space Center |
|
Oceanside Aerial of Columbia
| Title |
Oceanside Aerial of Columbia Launch |
| Full Description |
The Space Shuttle Columbia is launched from Pad 39B on a ten-day mission with a crew of five NASA Astronauts and a Canadian Payload Specialist. The Photograph was taken by astronaut Steven R. Nagel from a Shuttle Training Aircraft. Mission STS-52 payloads onboard include the Laser Geodynamic Satellite II. |
| Date |
10/22/1992 |
| NASA Center |
Kennedy Space Center |
|
Ochoa on Sky Genie
| Title |
Ochoa on Sky Genie |
| Full Description |
Mission Specialist Ellen Ochoa, wearing a Launch and Entry Suit (LES) and Launch and Entry Helmet (LEH), simulates an emergency egress procedure at JSC's Mockup and Integration Laboratory (MAIL). Having exited the crew compartment trainer (CCT) a shuttle mockup, through an overhead aft flight deck window, Ochoa lowers herself to the ground using the sky-genie. Training instructor Kenneth D. Trujillo assumes the role of a crewmate assisting from a position on the ground. The sky-genie is carried on all Space Shuttle flights for emergency egress purposes. |
| Date |
12/01/1992 |
| NASA Center |
Johnson Space Center |
|
Astronaut Administrator Rich
| Title |
Astronaut Administrator Richard Truly |
| Full Description |
Astronaut Richard H. Truly, pilot of the Space Shuttle Columbia on mission STS-2 and Commander of Shuttle Challenger on mission STS-8, became NASA's eighth Administrator on July 1, 1989. One day earlier he concluded a 30 year Naval career retiring as a Vice Admiral. He was the first astronaut to head the nation's civilian space agency. Truly became Deputy Associate Administrator for Space Flight on February 20, 1986. In this position, he led the painstaking rebuilding of the Space Shuttle program less than one month after the Challenger disaster. This was highlighted by the much heralded "Return to Flight" on September 29, 1988 with the launch of Shuttle Discovery, 32 months after Challenger's final flight. On February 12th, 1992 Richard Truly resigned as NASA Administrator at the request of President George Bush. |
| Date |
10/01/1979 |
| NASA Center |
Headquarters |
|
Columbia 180 Turn and Burn
| Title |
Columbia 180 Turn and Burn |
| Full Description |
The Space Shuttle Columbia and her crew of six lifted off from PAD 39B at 1:09 p.m. EDT, on a ten-day mission. The primary payload of Space Shuttle mission STS-52 is the Laser Geodynamic Satellite II (LAGEOS II). |
| Date |
10/22/1992 |
| NASA Center |
Kennedy Space Center |
|
Richard H. Truly
| Title |
Richard H. Truly |
| Full Description |
Vice Admiral Richard H. Truly served as NASA Administrator from May 14, 1989 to March 31, 1992. Prior to becoming Administrator, Adm. Truly served as NASA's Associate Administrator for Space Flight. In this position, he led the painstaking rebuilding of the Space Shuttle program after the Challenger accident. Adm. Truly's career began in the Navy and in 1965 he became one of the first military astronauts selected to the Air Force's Manned Orbiting Laboratory program in Los Angeles, California. He transferred to NASA as an astronaut in August 1969 then served as capsule communicator for all three Skylab missions in 1973 and the Apollo-Soyuz mission in 1975. He was pilot for the 747/Space Shuttle Enterprise approach and landing test flights during 1977, and his first space flight was November 12-14, 1981, as pilot of Space Shuttle Columbia (STS-2). After leaving NASA, Adm. Truly became Vice President and Director of the Georgia Tech Research Institute, Georgia Institute of Technology, in Atlanta. |
| Date |
UNKNOWN |
| NASA Center |
Headquarters |
|
Rick Hieb peers into the fli
| Title |
Rick Hieb peers into the flight deck |
| Full Description |
Rick Hieb, a Mission Specialist aboard STS-49, looks into the aft flight deck of the orbiter during his spacewalk. STS-49, which launched on May 7, 1992 and returned:to Earth on May 16, 1992, marked the first flight of Endeavour and the first shuttle mission to feature four EVAs. Hieb, along with fellow astronauts Pierre Thuot and Thomas Akers helped to recover INTELSAT VI, a communications satellite whose orbit had become unstable. |
| Date |
05/16/1992 |
| NASA Center |
Johnson Space Center |
|
Ride on the Middeck
| Title |
Ride on the Middeck |
| Full Description |
On Challenger's middeck, Mission Specialist (MS) Sally Ride, wearing light blue flight coveralls and communications headset, floats alongside the middeck airlock hatch. |
| Date |
06/24/1992 |
| NASA Center |
Johnson Space Center |
|
Daniel S. Goldin
| Title |
Daniel S. Goldin |
| Full Description |
Daniel S. Goldin was NASA longest tenured administrator, serving from April 1, 1992, to November 17, 2001. Mr. Goldin became well known for his "faster, better, cheaper" approach to cut NASA costs while still delivering a wide variety of aerospace programs. During his administration, Mr. Goldin supervised projects such as the Mars Pathfinder, Hubble Space Telescope Servicing missions, and the International Space Station. |
| Date |
UNKNOWN |
| NASA Center |
Headquarters |
|
Dr. Mae C. Jemison, First Af
| Title |
Dr. Mae C. Jemison, First African-American Woman in Space |
| Full Description |
The first African-American woman in space, Dr. Mae C. Jemison was born on October 17, 1956 in Decatur, Alabama but considers Chicago, Illinois her hometown. She received a Bachelor in Chemical Engineering (and completed the requirements for a Bachelor in African and Afro-American studies) at Stanford University in 1977. Dr. Jemison also received a Doctorate degree in medicine from Cornell University in 1981. After medical school she did post graduate medical training at the Los Angeles County University of Southern California Medical Center. As an area Peace Corps medical officer for Sierra Leone and Liberia in West Africa, she managed the health care delivery system for U.S. Peace Corps and U.S. Embassy personnel. Jemison's background includes work in the areas of nuclear magnetic resonance spectroscopy, and reproductive biology. She also developed and participated in research projects on the Hepatitis B vaccine and rabies. Jemison was a General Practitioner and attending graduate Engineering classes in Los Angeles when she was named an astronaut candidate in 1987. She flew her first flight as a science mission specialist on STS-47, Spacelab-J, in September 1992. She was co-investigator for the Bone Cell Research Experiment on that mission. In completing her first space flight, Jemison logged 190 hours, 30 minutes and 23 seconds in space. Jemison resigned from NASA in March 1993. In 1994, she founded and began a term as chair of The Earth We Share (TEWS), an annual international science camp where students, aged 12 to 16, work together to solve current global dilemmas. From 1995- 2002 she was a professor of Environmental Studies at Dartmouth College. She is currently director of the Jemison Institute for Advancing Technology in developing countries. She is the recipient of numerous awards and honors, including induction into the National Women's Hall of Fame and several corporate boards of directors on the Texas Governor's State Council for Science and Biotechnology Development. Dr. Jemison published her memoirs, Find Where DE:the Wind Goes:Moments from My Life in 2001. She currently resides in Houston, Texas. |
| Date |
07/1992 |
| NASA Center |
Johnson Space Center |
|
Dr. Thomas O. Paine
| Title |
Dr. Thomas O. Paine |
| Full Description |
Dr. Thomas O. Paine served as Deputy Administrator from January 31, 1968 to October 8, 1968, then as Acting Administrator from October 8, 1968, to March 21, 1969. He assumed the position of NASA Administrator on March 221, 1969 and served in that capacity until September 15, 1970. Prior to his time at NASA, Dr. Paine worked for General Electric conducting research on magnetic and composite materials. After serving as NASA Administrator, he returned to General Electric. In 1985 the White House chose him as chair of a National Commission on Space. Dr. Paine died in May 1992. |
| Date |
UNKNOWN |
| NASA Center |
Headquarters |
|
Endeavour Arrival
| Title |
Endeavour Arrival |
| Full Description |
The newest addition to the Space Shuttle orbiter fleet, Endeavour, arrives at KSC atop the 747 Shuttle Carrier Aircraft on May 7. OV-105 will be demated from the Boeing aircraft, and towed to the Vehicle Assembly Building for installation of several major flight components. Next step will be a lengthy stay in the Orbiter Processing Facility for a rigorous series of first flow tests. Endeavour is scheduled to lift off on its maiden space flight in 1992. |
| Date |
5/7/1991 |
| NASA Center |
Kennedy Space Center |
|
Endeavour is Delivered to th
| Title |
Endeavour is Delivered to the Kennedy Space Center |
| Full Description |
NASA's 747 Shuttle Carrier Aircraft No. 911, with the space shuttle orbiter Endeavour securely mounted atop its fuselage, taxies to the runway to begin the ferry flight from Rockwell's Plant 42 at Palmdale, California, where the orbiter was built, to the Kennedy Space Center, Florida. At Kennedy, the space vehicle was processed and launched on orbital mission STS-49, which landed at NASA's Ames-Dryden Flight Research Facility (later redesignated Dryden Flight Research Center), Edwards, California, May 16 1992. NASA 911, the second modified 747 that went into service in November 1990, has special support struts atop the fuselage and internal strengthening to accommodate the added weight of the orbiters. |
| Date |
01/01/1961 |
| NASA Center |
Dryden Flight Research Center |
|
Southern Bald Eagles
| Title |
Southern Bald Eagles |
| Full Description |
This is one in a series of remarkable photos documenting the daily lives of two of KSC's most famous residents: The Southern Bald Eagles which inhabit an enormous nest on the Kennedy Parkway North. Each fall, the eagles take up winter residence in the nest to breed and raise a new generation. Thanks to a remote-controlled Nikon camera installed yearly in the same pine tree as the nest, the activities of these magnificent birds are recorded on film. This year, a rare and unique event was captured by the camera when a second clutch of eggs was laid, even though a healthy eaglet was born a month earlier. Although it is impossible to determine if it is the same eagles returning each year, the continued tolerance shown by this pair to the human presence seems to indicate that they are the same couple. According to wildlife experts, eight to nine pairs of bald eagles inhabit nests at KSC. The nest on Kennedy Parkway North is particularly well-known because of its huge size and close proximity to a busy road. |
| Date |
4/1/1992 |
| NASA Center |
Kennedy Space Center |
|
F-16XL Scamp Flow Visualizat
| Title |
F-16XL Scamp Flow Visualization Test |
| Full Description |
F-16 Scamp model being tested in the BART. Photo shows a basic flow visualization test using smoke and a laser light sheet to illuminate the smoke. Part of the NASA High Speed Research Program. |
| Date |
10/6/1992 |
| NASA Center |
Langley Research Center |
|
False-Color Lunar Image
| Title |
False-Color Lunar Image |
| Full Description |
This false-color photograph is a composite of 15 images of the Moon taken through three color filters by the Galileo spacecraft?s solid-state imaging system during the spacecraft?s passage through the Earth-Moon system on December 8, 1992. When this view was obtained, the spacecraft was 425,000 kilometers (262,000 miles) from the Moon and 69,000 kilometers (43,000 miles) from Earth. The false-color processing used to create this lunar image is helpful for interpreting the surface soil composition. Areas appearing red generally correspond to the lunar highlands, while blue to orange shades indicate the ancient volcanic lava flow of a mare, or lunar sea. Bluer mare areas contain more titanium than do the orange regions. Mare Tranquillitatis, seen as a deep blue patch on the right, is richer in titanium than mare Serenitatis, a slightly smaller circular area immediately adjacent to the upper left o Mare Tranquillitatis. Blue and orange areas covering much of the left side of the Moon in this view represent many separate lava flows in Oceanus Procellarum. The small purple areas found near the center are pyroclastic deposits formed by explosive volcanic eruptions. The fresh crater Tycho, with a diameter of 85 kilometers (53 miles), is prominent at the bottom of the photograph, where part of the moon disk is missing. |
| Date |
04/1993 |
| NASA Center |
Jet Propulsion Laboratory |
|
Female Astronauts
| Title |
Female Astronauts |
| Full Description |
Astronauts Dr. N. Jan Davis (left) and Dr. Mae C. Jemison (right) were mission specialists on board the STS-47 mission. Born on November 1, 1953 in Cocoa Beach, Florida, Dr. N. Jan Davis received a Master degree in Mechanical Engineering in 1983 followed by a Doctorate in Engineering from the University of Alabama in Huntsville in 1985. In 1979 she joined NASA Marshall Space Flight Center as an aerospace engineer. A veteran of three space flights, Dr. Davis has logged over 678 hours in space since becoming an astronaut in 1987. She flew as a mission specialist on STS-47 in 1992 and STS-60 in 1994, and was the payload commander on STS-85 in 1997. In July 1999, she transferred to the Marshall Space Flight Center, where she became Director of Flight Projects. Dr. Mae C. Jemison, the first African-American woman in space, was born on October 17, 1956 in Decatur, Alabama but considers Chicago, Illinois her hometown. She received a Bachelor degree in Chemical Engineering (and completed the requirements for a Bachelor degree in African and Afro-American studies) at Stanford University in 1977, and a Doctorate degree in medicine from Cornell University in 1981. After receiving her doctorate, she worked as a General Practitioner while attending graduate engineering classes in Los Angeles. She was named an astronaut candidate in 1987, and flew her first flight as a science mission specialists on STS-47, Spacelab-J, in September 1992, logging 190 hours, 30 minutes, 23 seconds in space. In March 1993, Dr. Jemison resigned from NASA, thought she still resides in Houston, Texas. She went on to publish her memoirs, Find Where the Wind Goes: Moments from My Life, in 2001. The astronauts are shown preparing to deploy the lower body negative pressure (LBNP) apparatus in this 35mm frame taken in the science module aboard the Earth-orbiting Space Shuttle Endeavor. Fellow astronauts Robert L. Gibson (Commander), Curtis L. Brown (Junior Pilot), Mark C. Lee (Payload Commander), Jay Apt (Mission Specialist), and Mamoru Mohri (Payload Specialist) joined the two on their maiden space flight. The Spacelab-J mission was a joint effort between Japan and the United States. |
| Date |
09/15/1992 |
| NASA Center |
Johnson Space Center |
|
First Class of Female Astron
| Title |
First Class of Female Astronauts |
| Full Description |
From left to right are Shannon W. Lucid, Margaret Rhea Seddon, Kathryn D. Sullivan, Judith A. Resnik, Anna L. Fisher, and Sally K. Ride. NASA selected all six women as their first female astronaut candidates in January 1978, allowing them to enroll in a training program that they completed in August 1979. Shannon W. Lucid was born on January 14, 1943 in Shanghai, China but considers Bethany, Oklahoma to be her hometown. She spent many years at the University of Oklahoma, receiving a Bachelor in chemistry in 1963, a Master in biochemistry in 1970, and a Doctorate in biochemistry in 1973. Dr. Lucid flew on the STS-51G Discovery, STS-34 Atlantis, STS-43 Atlantis, and STS-58 Columbia shuttle missions, setting the record for female astronauts by logging 838 hours and 54 minutes in space. She also currently holds the United States single mission space flight endurance record for her 188 days on the Russian Space Station Mir. From February 2002 to September 2003, she served as chief scientist at NASA Headquarters before returning to JSC to help with the Return to Flight program after the STS-107 accident. Born November 8, 1947, in Murfreesboro, Tennessee, Margaret Rhea Seddon received a Doctorate of Medicine in 1973 from the University of Tennessee. She flew on space missions STS-51 Discovery, STS-40 Columbia, and STS-58 Columbia for a total of over 722 hours in space. Dr. Seddon retired from NASA in November 1997, taking on a position as the Assistant Chief Medical Officer of the Vanderbilt Medical Group in Nashville, Tennessee. Kathryn Sullivan was born October 3, 1951 in Patterson, New Jersey but considers Woodland Hills, California to be her hometown. She received a Bachelor in Earth Sciences from the University of California, Santa Cruz in 1973 and a Doctorate in Geology from Dalhousie University in Halifax, Nova Scotia in 1978. She flew on space missions STS-41G, STS-31, and STS-45 and logged a total of 532 hours in space. Dr. Sullivan left NASA in August 1992 to assume the position of Chief Scientist of the National Oceanic and Atmospheric Administration (NOAA). She later went on to serve as President and CEO of the Center of Science and Industry in Columbus, Ohio. Dr. Judith Resnik was born April 5, 1949 in Akron, Ohio. She received a Bachelor of Science degree in Electrical Engineering from Carnegie-Mellon University in 1970, and a Doctorate in Electrical Engineering from University of Maryland in 1977. Dr. Resnik left a job as a senior systems engineer in product development with Xerox Corporation at El Segundo, California to work for NASA in 1978. She died on January 28, 1986 on her second mission, during the launch of Challenger STS-51-L. Anna Fisher was born August 24, 1949 in New York City, New York hometown. She received a Doctorate in Medicine in 1976 and a Master of Science in Chemistry in 1987, both from the University of California, Los Angeles. Dr. Fisher flew on STS-51A, the Space Shuttle Discovery's November 8, 1984, mission, and logged 192 hours in space, her second schedule mission was cancelled after the Space Shuttle Challenger STS-51L accident. She remains with NASA, where she has filled many positions over decades of service. Dr. Sally Ride was the first American woman in space. Born on May 26, 1951 in Los Angeles, California, she went on to receive a Bachelor in Physics and English in 1973 from Stanford University and, later, a Master in Physics in 1975 and a Doctorate in Physics in 1978, also from Stanford. She began her astronaut career as a mission specialist on STS-7, which launched from Kennedy Space Center, Florida on June 18, 1983, and later went on to fly on STS-41G. She withdrew from training for her third scheduled mission in order to serve on the investigative committee for the Space Shuttle Challenger accident and never returned to training, although she went on to work for headquarters and later to serve on the Columbia Accident Investigation Board before returning to the private sector as a physics professor. |
| Date |
02/28/1979 |
| NASA Center |
Johnson Space Center |
|
STS-45 Landing
| Title |
STS-45 Landing |
| Full Description |
As the sun rises the morning of April 2, it casts a rosy glow over a steller performer, the orbiter Atlantis parked on Runway 33 of the Shuttle Landing Facility. Atlantis touched down at 6:23:6 a.m. EST, completing a highly successful flight that was extended by a day to further the scientific research being performed on the Atmospheric Laboratory for Applications and Science-1 (ATLAS-1) payload. On board OV-104 for Mission STS-45 was a crew of seven. |
| Date |
4/2/1992 |
| NASA Center |
Kennedy Space Center |
|
STS-45 Launch
| Title |
STS-45 Launch |
| Full Description |
With its twin solid rocket boosters and three main engines churning at seven million pounds of thrust, the Space Shuttle Atlantis thunders skyward from Launch Pad 39A. Liftoff of Mission STS-45 occurred at 8:13:40 a.m. EST, March 24, 1992. On board for the 46th Shuttle flight are a crew of seven and the Atmospheric Laboratory for Applications and Science-1 (ATLAS-1). The launch is the second in 1992 for the Shuttle program and Atlantis' 11th flight. |
| Date |
3/24/1992 |
| NASA Center |
Kennedy Space Center |
|
Galileo Images the Moon
| Title |
Galileo Images the Moon |
| Full Description |
This view of the Moon's north pole is a mosaic assembled from 18 images taken by Galileo's imaging system through a green filter as the spacecraft flew by on December 7, 1992. The left part of the Moon is visible from Earth, this region includes the dark, lava-filled Mare Imbrium (upper left), Mare Serenitatis (middle left), Mare Tranquillitatis (lower left), and Mare Crisium, the dark circular feature toward the bottom of the mosaic. Also visible in this view are the dark lava plains of the Marginis and Smythii Basins at the lower right. The Humboldtianum Basin, a 650-kilometer (400-mile) impact structure partly filled with dark volcanic deposits, is seen at the center of the image. The Moon's north pole is located just inside the shadow zone, about a third of the way from the top left of the illuminated region. |
| Date |
12/14/1992 |
| NASA Center |
Jet Propulsion Laboratory |
|
The Americas and Hurricane A
| Title |
The Americas and Hurricane Andrew |
| Full Description |
Image taken on August 25, 1992 by NOAA GOES-7 weather satellite of the Americas and Hurricane Andrew as it makes landfall on the Louisiana coast. |
| Date |
08/25/1992 |
| NASA Center |
Goddard Space Flight Center |
|
The Earth and Moon
| Title |
The Earth and Moon |
| Full Description |
During its flight, the Galileo spacecraft returned images of the Earth and Moon. Separate images of the Earth and Moon were combined to generate this view. The Galileo spacecraft took the images in 1992 on its way to explore the Jupiter system in 1995-97. The image shows a partial view of the Earth centered on the Pacific Ocean about latitude 20 degrees south. The west coast of South America can be observed as well as the Caribbean, swirling white cloud patterns indicate storms in the southeast Pacific. The distinct bright ray crater at the bottom of the Moon is the Tycho impact basin. The lunar dark areas are lava rock filled impact basins. This picture contains same scale and relative color/albedo images of the Earth and Moon. False colors via use of the 1-micron filter as red, 727-nm filter as green, and violet filter as blue. The Galileo project is managed for NASA's Office of Space Science by the Jet Propulsion Laboratory. |
| Date |
01/02/1990 |
| NASA Center |
Jet Propulsion Laboratory |
|
HL-20 at Langley
| Title |
HL-20 at Langley |
| Full Description |
The NASA Langley Research Center lifting body, called the HL-20, is shown here in front of the hangar. The HL-20 was one of two concepts considered by NASA as a type of Personnel Launch System (PLS). In essence, it would serve as a space taxi to and from the space station. The full scale engineering model is 29.5 feet long, and 23.5 feet across the wingspan. |
| Date |
04/28/1992 |
| NASA Center |
Langley Research Center |
|
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