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View of the west coastline o …
Title View of the west coastline of Baja, California and Cedros Island from Gemini
Description View of the west coastline of Baja, California and Cedros Island taken from the Gemini 5 spacecraft in orbit over the Earth.
Date Taken 1965-08-21
View of the lower tip of Baj …
Title View of the lower tip of Baja, California and Bahia de la Paz from Gemini 5
Description View of the lower tip of Baja, California and Bahia de la Paz taken from the Gemini 5 spacecraft in orbit over the Earth.
Date Taken 1965-08-21
Gulf of California as seen f …
Title Gulf of California as seen from the Gemini 12 spacecraft
Description Gulf of California as seen from the Gemini 12 spacecraft during its 30th revolution of the earth. Baja California Sur is the peninsula on the left. At lower left is the mainland of Mexico. A 100 ft. tether line connects the Agena Target Docking Vehicle with the Gemini 12 spacecraft. View is looking south.
Date Taken 1966-11-13
Gemini 9 spacecraft during E …
Title Gemini 9 spacecraft during EVA as seen Astronaut Eugene Cernan
Description Astronaut Eugene A. Cernan took this view of the Gemini 9 spacecraft and his umbilical cord (right) over California, Arizona, and Sonora, Mexico, during his extravehicular activity on the Gemini 9 mission. Taken during the 32nd revolution of the flight.
Date Taken 1966-06-05
Guadalupe Island off Baja, C …
Title Guadalupe Island off Baja, California as seen from the Gemini 12 spacecraft
Description Guadalupe Island, unique vortices off Baja California, Mexico, as seen from the Gemini 12 spacecraft during its 29th revolution of the earth.
Date Taken 1966-11-13
View of the Gulf of Californ …
Title View of the Gulf of California from Gemini 4
Description View of the north end of the Gulf of California at the mouth of the Colorado River taken from the Gemini 4 spacecraft during one of it orbits of the earth. North is towards the bottom of the picture.
Date Taken 1965-06-03
View of Imperial Valley and …
Title View of Imperial Valley and Salton Sea in Southern California from Gemini 5
Description View of Imperial Valley and Salton Sea in southern California, looking northeast, taken from the Gemini 5 spacecraft in orbit over the Earth.
Date Taken 1965-08-21
Gemini 11 spacecraft and Age …
Title Gemini 11 spacecraft and Agena Target Vehicle during tethering
Description The Agena Target Docking Vehicel is tethered to the Gemini 11 spacecraft during its 31st revolution of the earth. Area below is the Gulf of California and Baja California at La Paz.
Date Taken 1966-09-14
Northwestern Mexico as seen …
Title Northwestern Mexico as seen from the Gemini 9-A spacecraft
Description Northwestern Mexico as seen from the Gemini 9-A spacecraft during its 32nd revolution of the earth. Large peninsula is Baja California. Body of water at lower right is Pacific Ocean. Land mass at upper left is State of Sonora. Gulf of California separates Sonora from peninsula. Nose of spacecraft is at left and at right is open hatch of spacecraft.
Date Taken 1966-06-05
Official Portrait of Astrona …
Name of Image Official Portrait of Astronaut Frank Borman
Date of Image 1964-09-09
Full Description This is the official portrait of astronaut Frank Borman. A career Air Force officer from 1950, his assignments included service as a fighter pilot, an operational pilot and instructor, an experimental test pilot and an assistant professor of thermodynamics and fluid mechanics at West Point. When selected by NASA, Frank Borman was an instructor at the Aerospace Research Pilot School at Edwards AFB, California. In 1967 he served as a member of the Apollo 204 Fire Investigation Board, investigating the causes of the fire which killed three astronauts aboard an Apollo spacecraft. Later he became the Apollo Program Resident Manager, heading the team that reengineered the Apollo spacecraft. He also served as Field Director of the NASA Space Station Task Force. Frank Borman retired from the air Force in 1970, but is well remembered as a part of American history as a pioneer in the exploration of space. He is a veteran of both the Gemini 7, 1965 Space Orbital Rendezvous with Gemini 6 and the first manned lunar orbital mission, Apollo 8, in 1968.
Paresev 1-C Inflatable Wing
Title Paresev 1-C Inflatable Wing
Full Description Aboard a truck and ready for a test flight is the Paresev 1-C on the ramp at the NASA Flight Research Center, Edwards, California. The half-scale version of the inflatable Gemini parawing was pre-flighted by being carried across the Rosamond dry lakebed on the back of a truck before a tow behind an International Harvester Carry- All. The inflatable center spar ran fore and aft and measured 191 inches, two other inflatable spars formed the leading edges. The three compartments were filled with nitrogen under pressure to make them rigid. The Paresev 1-C was very unstable in flight with this configuration.
Date 01/01/1963
NASA Center Dryden Flight Research Center
Northwestern Mexico as seen …
Title Northwestern Mexico as seen from the Gemini 12 spacecraft
Description Area of northwestern Mexico as seen from the Gemini 12 spacecraft during its 16th revolution of the earth. View is looking northwest. Body of water in foreground is Gulf of California. Pacific Ocean is in background. Peninsula in center of picture is Baja California. States of Sonora (upper right) and Sinaloa (lower center) of Mexican mainland is in right foreground. City of Guaymas, Sonora, is near center of picture.
Date Taken 1966-11-12
Distant Planetoid
title Distant Planetoid
date 02.17.2004
description The small dot moving slightly off to the left of center in this image is newly-discovered Kuiper Belt object 2004 DW. 2004 DW was found in images taken Feb 17, 2004 (nearly 74 years to the day after Pluto was discovered) by Mike Brown (Caltech), Chad Trujillo (Gemini Observatory) and David Rabinowitz (Yale). They are the same people who found Quaoar in the summer of 2002. 2004 DW is one of the largest Kuiper Belt objects currently known. Initial indications are that it may be over half the diameter of Pluto, larger than Quaoar, and 2.4 billion kilometers (1.5 billion miles) further away than Pluto. Read more about 2004 DW. *Image Credit*: California Institute of Technology
Paresev 1-A on Lakebed with …
Title Paresev 1-A on Lakebed with Tow Plane
Full Description The Paresev 1-A (Paraglider Research Vehicle) and the tow airplane, 450-hp Stearman Sport Biplane sitting on Rogers dry lakebed, Edwards, California. The control system in the Paresev 1-A had a more conventional control stick position and was cable-operated. The main landing gear used shocks and bungees with the 150-square-foot wing membrane being made of 6-ounce unsealed Dacron.
Date 01/01/1962
NASA Center Dryden Flight Research Center
Gus Grissom & Milt Thompson …
Title Gus Grissom & Milt Thompson With Paresev
Full Description The Paresev 1-A standing Rogers Dry Lakebed at the NASA Flight Research Center, Edwards, California. Mercury Astronaut Gus Grissom is at left and NASA test pilot Milton Thompson is at right. The Paresev evaluated a potential replacement for parachutes used on spacecraft. The Paresev was steerable and was evaluated for use on the Gemini spacecraft. The idea was not workable, however.
Date 01/01/1962
NASA Center Dryden Flight Research Center
Astronomers Measure Mass of …
Title Astronomers Measure Mass of Largest Dwarf Planet
Astronomers Measure Mass of …
Title Astronomers Measure Mass of Largest Dwarf Planet
Official Portrait of Astrona …
Name of Image Official Portrait of Astronaut Neil Armstrong
Date of Image 1969-01-09
Full Description Neil Armstrong, donned in his space suit, poses for his official Apollo 11 portrait. Armstrong began his flight career as a naval aviator. He flew 78 combat missions during the Korean War. Armstrong joined the NASA predecessor, NACA (National Advisory Committee for Aeronautics), as a research pilot at the Lewis Laboratory in Cleveland and later transferred to the NACA High Speed Flight Station at Edwards AFB, California. He was a project pilot on many pioneering high speed aircraft, including the 4,000 mph X-15. He has flown over 200 different models of aircraft, including jets, rockets, helicopters, and gliders. In 1962, Armstrong was transferred to astronaut status. He served as command pilot for the Gemini 8 mission, launched March 16, 1966, and performed the first successful docking of two vehicles in space. In 1969, Armstrong was commander of Apollo 11, the first manned lunar landing mission, and gained the distinction of being the first man to land a craft on the Moon and the first man to step on its surface. Armstrong subsequently held the position of Deputy Associate Administrator for Aeronautics, NASA Headquarters Office of Advanced Research and Technology, from 1970 to 1971. He resigned from NASA in 1971.
Hubble's Infrared Eyes Home …
Title Hubble's Infrared Eyes Home in on Suspected Extrasolar Planet
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. Back to top [ #top ]
Our Chaotic Neighbor
Title Our Chaotic Neighbor
Description This vibrant image from NASA's Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. The infrared image, a mosaic of more than 100,000 individual tiles, offers astronomers a unique chance to study the lifecycle of stars and dust in a single galaxy. Nearly one million objects are revealed for the first time in this Spitzer view, which represents about a 1,000-fold improvement in sensitivity over previous space-based missions. Most of the new objects are dusty stars of various ages populating the Large Magellanic Cloud, the rest are thought to be background galaxies. The blue color in the picture, seen most prominently in the central bar, represents starlight from older stars. The chaotic, bright regions outside this bar are filled with hot, massive stars buried in thick blankets of dust. The red clouds contain cooler interstellar gas and molecular-sized dust grains illuminated by ambient starlight. The Large Magellanic Cloud, located 160,000 light-years from Earth, is one of a handful of dwarf galaxies that orbit our own Milky Way. It is approximately one-third as wide as the Milky Way, and, if it could be seen in its entirety, would cover the same amount of sky as a grid of about 480 full moons. About one-third of the whole galaxy can be seen in the Spitzer image. This picture is a composite of infrared light captured by Spitzer's infrared array camera. Light with wavelengths of 8 and 5.8 microns is red and orange: 4.5-micron light is green, and 3.6-micron light is blue.
Our Chaotic Neighbor
Title Our Chaotic Neighbor
Description This vibrant image from NASA's Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. The infrared image, a mosaic of more than 100,000 individual tiles, offers astronomers a unique chance to study the lifecycle of stars and dust in a single galaxy. Nearly one million objects are revealed for the first time in this Spitzer view, which represents about a 1,000-fold improvement in sensitivity over previous space-based missions. Most of the new objects are dusty stars of various ages populating the Large Magellanic Cloud, the rest are thought to be background galaxies. The blue color in the picture, seen most prominently in the central bar, represents starlight from older stars. The chaotic, bright regions outside this bar are filled with hot, massive stars buried in thick blankets of dust. The red clouds contain cooler interstellar gas and molecular-sized dust grains illuminated by ambient starlight. The Large Magellanic Cloud, located 160,000 light-years from Earth, is one of a handful of dwarf galaxies that orbit our own Milky Way. It is approximately one-third as wide as the Milky Way, and, if it could be seen in its entirety, would cover the same amount of sky as a grid of about 480 full moons. About one-third of the whole galaxy can be seen in the Spitzer image. This picture is a composite of infrared light captured by Spitzer's infrared array camera. Light with wavelengths of 8 and 5.8 microns is red and orange: 4.5-micron light is green, and 3.6-micron light is blue.
Our Chaotic Neighbor
Title Our Chaotic Neighbor
Description This vibrant image from NASA's Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. The infrared image, a mosaic of more than 100,000 individual tiles, offers astronomers a unique chance to study the lifecycle of stars and dust in a single galaxy. Nearly one million objects are revealed for the first time in this Spitzer view, which represents about a 1,000-fold improvement in sensitivity over previous space-based missions. Most of the new objects are dusty stars of various ages populating the Large Magellanic Cloud, the rest are thought to be background galaxies. The blue color in the picture, seen most prominently in the central bar, represents starlight from older stars. The chaotic, bright regions outside this bar are filled with hot, massive stars buried in thick blankets of dust. The red clouds contain cooler interstellar gas and molecular-sized dust grains illuminated by ambient starlight. The Large Magellanic Cloud, located 160,000 light-years from Earth, is one of a handful of dwarf galaxies that orbit our own Milky Way. It is approximately one-third as wide as the Milky Way, and, if it could be seen in its entirety, would cover the same amount of sky as a grid of about 480 full moons. About one-third of the whole galaxy can be seen in the Spitzer image. This picture is a composite of infrared light captured by Spitzer's infrared array camera. Light with wavelengths of 8 and 5.8 microns is red and orange: 4.5-micron light is green, and 3.6-micron light is blue.
What's Old Is New in the Lar …
Title What's Old Is New in the Large Magellanic Cloud
Description This vibrant image from NASA's Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. The infrared image, a mosaic of 300,000 individual tiles, offers astronomers a unique chance to study the lifecycle of stars and dust in a single galaxy. Nearly one million objects are revealed for the first time in this Spitzer view, which represents about a 1,000-fold improvement in sensitivity over previous space-based missions. Most of the new objects are dusty stars of various ages populating the Large Magellanic Cloud, the rest are thought to be background galaxies. The blue color in the picture, seen most prominently in the central bar, represents starlight from older stars. The chaotic, bright regions outside this bar are filled with hot, massive stars buried in thick blankets of dust. The red color around these bright regions is from dust heated by stars, while the red dots scattered throughout the picture are either dusty, old stars or more distant galaxies. The greenish clouds contain cooler interstellar gas and molecular-sized dust grains illuminated by ambient starlight. Astronomers say this image allows them to quantify the process by which space dust ? the same stuff that makes up planets and even people ? is recycled in a galaxy. The picture shows dust at its three main cosmic hangouts: around the young stars, where it is being consumed (red-tinted, bright clouds), scattered about in the space between stars (greenish clouds), and in expelled shells of material from old stars (randomly-spaced red dots). The Large Magellanic Cloud, located 160,000 light-years from Earth, is one of a handful of dwarf galaxies that orbit our own Milky Way. It is approximately one-third as wide as the Milky Way, and, if it could be seen in its entirety, would cover the same amount of sky as a grid of about 480 full moons. About one-third of the entire galaxy can be seen in the Spitzer image. This picture is a composite of infrared light captured by Spitzer. Light with wavelengths of 3.6 (blue) and 8 (green) microns was captured by the telescope's infrared array camera, 24-micron light (red) was detected by the multiband imaging photometer.
What's Old Is New in the Lar …
Title What's Old Is New in the Large Magellanic Cloud
Description This vibrant image from NASA's Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. The infrared image, a mosaic of 300,000 individual tiles, offers astronomers a unique chance to study the lifecycle of stars and dust in a single galaxy. Nearly one million objects are revealed for the first time in this Spitzer view, which represents about a 1,000-fold improvement in sensitivity over previous space-based missions. Most of the new objects are dusty stars of various ages populating the Large Magellanic Cloud, the rest are thought to be background galaxies. The blue color in the picture, seen most prominently in the central bar, represents starlight from older stars. The chaotic, bright regions outside this bar are filled with hot, massive stars buried in thick blankets of dust. The red color around these bright regions is from dust heated by stars, while the red dots scattered throughout the picture are either dusty, old stars or more distant galaxies. The greenish clouds contain cooler interstellar gas and molecular-sized dust grains illuminated by ambient starlight. Astronomers say this image allows them to quantify the process by which space dust ? the same stuff that makes up planets and even people ? is recycled in a galaxy. The picture shows dust at its three main cosmic hangouts: around the young stars, where it is being consumed (red-tinted, bright clouds), scattered about in the space between stars (greenish clouds), and in expelled shells of material from old stars (randomly-spaced red dots). The Large Magellanic Cloud, located 160,000 light-years from Earth, is one of a handful of dwarf galaxies that orbit our own Milky Way. It is approximately one-third as wide as the Milky Way, and, if it could be seen in its entirety, would cover the same amount of sky as a grid of about 480 full moons. About one-third of the entire galaxy can be seen in the Spitzer image. This picture is a composite of infrared light captured by Spitzer. Light with wavelengths of 3.6 (blue) and 8 (green) microns was captured by the telescope's infrared array camera, 24-micron light (red) was detected by the multiband imaging photometer.
What's Old Is New in the Lar …
Title What's Old Is New in the Large Magellanic Cloud
Description This vibrant image from NASA's Spitzer Space Telescope shows the Large Magellanic Cloud, a satellite galaxy to our own Milky Way galaxy. The infrared image, a mosaic of 300,000 individual tiles, offers astronomers a unique chance to study the lifecycle of stars and dust in a single galaxy. Nearly one million objects are revealed for the first time in this Spitzer view, which represents about a 1,000-fold improvement in sensitivity over previous space-based missions. Most of the new objects are dusty stars of various ages populating the Large Magellanic Cloud, the rest are thought to be background galaxies. The blue color in the picture, seen most prominently in the central bar, represents starlight from older stars. The chaotic, bright regions outside this bar are filled with hot, massive stars buried in thick blankets of dust. The red color around these bright regions is from dust heated by stars, while the red dots scattered throughout the picture are either dusty, old stars or more distant galaxies. The greenish clouds contain cooler interstellar gas and molecular-sized dust grains illuminated by ambient starlight. Astronomers say this image allows them to quantify the process by which space dust ? the same stuff that makes up planets and even people ? is recycled in a galaxy. The picture shows dust at its three main cosmic hangouts: around the young stars, where it is being consumed (red-tinted, bright clouds), scattered about in the space between stars (greenish clouds), and in expelled shells of material from old stars (randomly-spaced red dots). The Large Magellanic Cloud, located 160,000 light-years from Earth, is one of a handful of dwarf galaxies that orbit our own Milky Way. It is approximately one-third as wide as the Milky Way, and, if it could be seen in its entirety, would cover the same amount of sky as a grid of about 480 full moons. About one-third of the entire galaxy can be seen in the Spitzer image. This picture is a composite of infrared light captured by Spitzer. Light with wavelengths of 3.6 (blue) and 8 (green) microns was captured by the telescope's infrared array camera, 24-micron light (red) was detected by the multiband imaging photometer.
Official Portrait of Astrona …
Name of Image Official Portrait of Astronaut Michael Collins
Date of Image 1967-01-09
Full Description This is the official NASA portrait of astronaut Michael Collins. Collins chose an Air Force career following graduation from West Point. He served as an experimental flight test officer at the Air Force Flight Test Center, Edwards Air Force Base, California, and, in that capacity, tested performance and stability and control characteristics of Air Force aircraft, primarily jet fighters. Having logged approximately 5,000 hours flying time, Collins was one of the third group of astronauts named by NASA in October 1963. Collins completed two space flights, logging 266 hours in space, of which, 1 hour and 27 minutes was spent in Extra Vehicular Activity (EVA). On July 18, 1966, he served as backup pilot for the Gemini VII mission which included a successful rendezvous and docking with a separately launched Agena target vehicle and, using the power of the Agena, maneuvered the Gemini spacecraft into another orbit for a rendezvous with a second, passive Agena. His skillful performance in completing two periods of EVA included the recovery of a micrometeorite detection experiment from the passive Agena. July 16-24, 1969, Collins served as command module (CM) pilot on Apollo 11, the historic first lunar landing mission. He remained aboard the CM, Columbia, on station in lunar orbit and performed the final re-docking maneuvers following a successful lunar orbit rendezvous with the Lunar Module (LM), Eagle. Collins left NASA in January 1970.
Neil A. Armstrong
Photo Date 1958
Apollo 11 Commander Armstron …
Name of Image Apollo 11 Commander Armstrong Presents President With Commemorative Plaque
Date of Image 1974-06-04
Full Description On June 4, 1974, 5 years after the successful Apollo 11 lunar landing mission, commander Neil Armstrong (right) presented a plaque to U.S. President Richard Milhous Nixon (left) on behalf of all people who had taken part in the space program. In making the presentation, Armstrong said ?Mr. President, you have proclaimed this week to be United States Space week in conjunction with the fifth anniversary of our first successful landing on the Moon. It is my privilege to represent my colleagues, the crewmen of projects Mercury, Gemini, Apollo, and Skylab, and the men and women of NASA, and the hundreds of thousands of Americans from across the land who contributed so mightily to the success of our efforts in space in presenting this plaque which bears the names of each individual who has had the privilege of representing this country? in a space flight. The presentation was made at the California white house in San Clemente.
X-15 Mated to B-52 Captive F …
Photo Description High-altitude contrails frame the B-52 mothership as it carries the X-15 aloft for a research flight on 13 April 1960 on Air Force Maj. Robert M. White's first X-15 flight. The X-15s were air-launched so that they would have enough rocket fuel to reach their high speed and altitude test points. For this early research flight, the X-15 was equipped with a pair of XLR-11 rocket engines until the XLR-99 was available. The X-15s made a total of 199 flights over a period of nearly 10 years--1959 to 1968--and set unofficial world speed and altitude records of 4,520 mph (Mach 6.7) and 354,200 feet. Information gained from the highly successful X-15 program contributed to the development of the Mercury, Gemini, and Apollo piloted spaceflight programs, and also the Space Shuttle program.
Project Description NASA B-52, Tail Number 008, is an air launch carrier aircraft, "mothership," as well as a research aircraft platform that has been used on a variety of research projects. The aircraft, a "B" model built in 1952 and first flown on June 11, 1955, is the oldest B-52 in flying status and has been used on some of the most significant research projects in aerospace history. Some of the significant projects supported by B-52 008 include the X-15, the lifting bodies, HiMAT (highly maneuverable aircraft technology), Pegasus, validation of parachute systems developed for the space shuttle program (solid-rocket-booster recovery system and the orbiter drag chute system), and the X-38. The B-52 served as the launch vehicle on 106 X-15 flights and flew a total of 159 captive-carry and launch missions in support of that program from June 1959 to October 1968. Information gained from the highly successful X-15 program contributed to the Mercury, Gemini, and Apollo human spaceflight programs as well as space shuttle development. Between 1966 and 1975, the B-52 served as the launch aircraft for 127 of the 144 wingless lifting body flights. In the 1970s and 1980s, the B-52 was the launch aircraft for several aircraft at what is now the Dryden Flight Research Center, Edwards, California, to study spin-stall, high-angle-of attack, and maneuvering characteristics. These included the 3/8-scale F-15/spin research vehicle (SRV), the HiMAT (Highly Maneuverable Aircraft Technology) research vehicle, and the DAST (drones for aerodynamic and structural testing). The aircraft supported the development of parachute recovery systems used to recover the space shuttle solid rocket booster casings. It also supported eight orbiter (space shuttle) drag chute tests in 1990. In addition, the B-52 served as the air launch platform for the first six Pegasus space boosters. During its many years of service, the B-52 has undergone several modifications. The first major modification was made by North American Aviation (now part of Boeing) in support of the X-15 program. This involved creating a launch-panel-operator station for monitoring the status of the test vehicle being carried, cutting a large notch in the right inboard wing flap to accommodate the vertical tail of the X-15 aircraft, and installing a wing pylon that enables the B-52 to carry research vehicles and test articles to be air-launched/dropped. Located on the right wing, between the inboard engine pylon and the fuselage, this wing pylon was subjected to extensive testing prior to its use. For each test vehicle the B-52 carried, minor changes were made to the launch-panel operator?s station. Built originally by the Boeing Company, the NASA B-52 is powered by eight Pratt & Whitney J57-19 turbojet engines, each of which produce 12,000 pounds of thrust. The aircraft?s normal launch speed has been Mach 0.8 (about 530 miles per hour) and its normal drop altitude has been 40,000 to 45,000 feet. It is 156 feet long and has a, wing span of 185 feet. The heaviest load it has carried was the No. 2 X-15 aircraft at 53,100 pounds. Project manager for the aircraft was Roy Bryant.
Photo Date 1960
X-15 Mated to B-52 Captive F …
Photo Description One of three X-15 rocket-powered research aircraft being carried aloft under the wing of its B-52 mothership. The X-15 was air launched from the B-52 so the rocket plane would have enough fuel to reach its high speed and altitude test points. For flight in the dense air of the usable atmosphere, the X-15 used conventional aerodynamic controls. For flight in the thin air outside of the appreciable Earth's atmosphere, the X-15 used a reaction control system. Hydrogen peroxide thrust rockets located on the nose of the aircraft provided pitch and yaw control. Those on the wings provided roll control. The X-15s made a total of 199 flights over a period of nearly 10 years and set world's unofficial speed and altitude records of 4,520 miles per hour (Mach 6.7) and 354,200 feet. Information gained from the highly successful X-15 program contributed to the development of the Mercury, Gemini, and Apollo manned spaceflight programs and also the Space Shuttle program.
Project Description NASA B-52, Tail Number 008, is an air launch carrier aircraft, "mothership," as well as a research aircraft platform that has been used on a variety of research projects. The aircraft, a "B" model built in 1952 and first flown on June 11, 1955, is the oldest B-52 in flying status and has been used on some of the most significant research projects in aerospace history. Some of the significant projects supported by B-52 008 include the X-15, the lifting bodies, HiMAT (highly maneuverable aircraft technology), Pegasus, validation of parachute systems developed for the space shuttle program (solid-rocket-booster recovery system and the orbiter drag chute system), and the X-38. The B-52 served as the launch vehicle on 106 X-15 flights and flew a total of 159 captive-carry and launch missions in support of that program from June 1959 to October 1968. Information gained from the highly successful X-15 program contributed to the Mercury, Gemini, and Apollo human spaceflight programs as well as space shuttle development. Between 1966 and 1975, the B-52 served as the launch aircraft for 127 of the 144 wingless lifting body flights. In the 1970s and 1980s, the B-52 was the launch aircraft for several aircraft at what is now the Dryden Flight Research Center, Edwards, California, to study spin-stall, high-angle-of attack, and maneuvering characteristics. These included the 3/8-scale F-15/spin research vehicle (SRV), the HiMAT (Highly Maneuverable Aircraft Technology) research vehicle, and the DAST (drones for aerodynamic and structural testing). The aircraft supported the development of parachute recovery systems used to recover the space shuttle solid rocket booster casings. It also supported eight orbiter (space shuttle) drag chute tests in 1990. In addition, the B-52 served as the air launch platform for the first six Pegasus space boosters. During its many years of service, the B-52 has undergone several modifications. The first major modification was made by North American Aviation (now part of Boeing) in support of the X-15 program. This involved creating a launch-panel-operator station for monitoring the status of the test vehicle being carried, cutting a large notch in the right inboard wing flap to accommodate the vertical tail of the X-15 aircraft, and installing a wing pylon that enables the B-52 to carry research vehicles and test articles to be air-launched/dropped. Located on the right wing, between the inboard engine pylon and the fuselage, this wing pylon was subjected to extensive testing prior to its use. For each test vehicle the B-52 carried, minor changes were made to the launch-panel operator?s station. Built originally by the Boeing Company, the NASA B-52 is powered by eight Pratt & Whitney J57-19 turbojet engines, each of which produce 12,000 pounds of thrust. The aircraft?s normal launch speed has been Mach 0.8 (about 530 miles per hour) and its normal drop altitude has been 40,000 to 45,000 feet.. It is 156 feet long and has a, wing span of 185 feet. The heaviest load it has carried was the No. 2 X-15 aircraft at 53,100 pounds. Project manager for the aircraft was Roy Bryant.
Photo Date 1959
Hubble's Infrared Eyes Home …
Title Hubble's Infrared Eyes Home in on Suspected Extrasolar Planet
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. Back to top [ #top ]
Hubble Finds 'Tenth Planet' …
Title Hubble Finds 'Tenth Planet' is Slightly Larger than Pluto
Astronomers Measure Mass of …
Title Astronomers Measure Mass of Largest Dwarf Planet
Astronomers Measure Mass of …
Title Astronomers Measure Mass of Largest Dwarf Planet
Astronomers Measure Mass of …
Title Astronomers Measure Mass of Largest Dwarf Planet
Solar System Object Larger t …
Title Solar System Object Larger than Pluto Discovered
Explanation Is that a tenth planet? A faint, slowly moving dot discovered by computer [ http://www.astro.caltech.edu/~pick/survey.html ] shows clear signs of being a deep Solar System [ http://www.nineplanets.org/overview.html ] object at least as large as Pluto [ http://antwrp.gsfc.nasa.gov/apod/ap010319.html ]. The object, designated 2003 UB313, is currently situated nearly 100 times the Earth-Sun distance [ http://en.wikipedia.org/wiki/Astronomical_unit ] -- over twice the average Pluto-Sun distance. That far out, the only way a single round object could be as bright as 2003 UB313 would be if it is at least as large as Pluto and completely reflective [ http://en.wikipedia.org/wiki/Albedo ]. Since 2003 UB313 is surely not completely reflective [ http://gemini.edu/index.php?option=content&task=view&id=142 ], it could be substantially larger. One of the discovery frames [ http://www.jpl.nasa.gov/news/news.cfm?release=2005-126 ] is shown above digitally expanded and artificially brightened. 2003 UB313 was identified [ http://www.astro.caltech.edu/~pick/survey.html ] initially on frames taken by the automated 1.2-meter Samuel Oschin Telescope [ http://www.astro.caltech.edu/palomarnew/sot.html ] at Palomar Observatory in California [ http://en.wikipedia.org/wiki/California ], USA [ http://www.cia.gov/cia/publications/factbook/geos/us.html ].
Former Dryden pilot and NASA …
Photo Date 1991
Former Dryden pilot and NASA …
Photo Date 1991
Paresev 1-C with inflatable …
Title Paresev 1-C with inflatable wing testbed aboard a truck in preparation for flight tests
Description Aboard a truck and ready for a test flight is the Paresev 1-C on the ramp at the NASA Flight Research Center, Edwards, California. The half-scale version of the inflatable Gemini parawing was pre-flighted by being carried across the Rosamond dry lakebed on the back of a truck before a tow behind a International Harvester Carry-All. The inflatable center spar ran fore and aft and measured 191 inches, two other inflatable spars formed the leading edges. The three compartments were filled with nitrogen under pressure to make them rigid. The Paresev 1-C was very unstable in flight with this configuration.
Date 01.01.1963
Technicians prepare the infl …
Title Technicians prepare the inflatable wing on Paresev 1-C
Description This photo shows the Paresev (Paraglider Research Vehicle) space frame receiving a new wing. Frank Fedor and a technician helper are attaching a half-scale version of an inflatable wing in a hangar at NASA Flight Research Center at Edwards, California. The Paresev in this configuration was called the 1-C and was expected to closely approximate the aerodynamic characteristics that would be encountered with the Gemini space capsule with a parawing extended. The whole wing was not inflatable, the three chambers that acted as spars and supported the wing inflated.
Date 01.01.1963
Astronomers Use Hubble and K …
Title Astronomers Use Hubble and Keck to Identify Dwarf Galaxy
General Information What is a News Nugget? News Nuggets are bulletins from the world of astronomy. A team of astronomers at the University of California at Santa Barbara report that they have resolved a dwarf galaxy 6 billion light-years away. Weighing only 1/100 as much as our Milky Way Galaxy, the dwarf is much smaller than anything studied before in any detail at this distance. They report in the Dec. 20 issue of the Astrophysical Journal that the galaxy looks very similar to one of the dwarf galaxies in the Virgo cluster, which is located only 60 million light-years away. "We believe we may have identified the progenitors of local dwarf galaxies," says Tommaso Treu. "We see them as clearly as we would see dwarfs in the Virgo cluster using ground-based telescopes. The sharp view of NASA's Hubble Space Telescope, and the laser guide stars adaptive optics system on the W.M. Keck Telescope, were aimed at a natural lens in space, called a gravitational lens, to study the dwarf. The researchers took advantage of the fact that the distant dwarf galaxy lies behind a massive foreground galaxy that bends light rays much as a glass lens does. This gravitational lensing amplifies the image of the much farther dwarf galaxy, making it appear 10 times brighter and 10 times larger than it would normally be seen by either Hubble or Keck.
Neil A. Armstrong
Title Neil A. Armstrong
Description Neil A. Armstrong joined the National Advisory Committee for Aeronautics at the Lewis Flight Propulsion Laboratory, Cleveland, Ohio, in 1955. He transferred to the NACA High-Speed Flight Station at Edwards Air Force Base, California, in July 1955, as an aeronautical research scientist. He became a research pilot later that year. Neil was named as one of nine astronauts for NASA's Gemini and Apollo Projects, leaving the Center for the National Aeronautics and Space Administration's Manned Spacecraft Center, Houston, Texas, in September 1962. Upon graduation from High School in 1947, Armstrong received a scholarship from the U.S. Navy. He enrolled at Purdue University to begin the study of aeronautical engineering. In 1949, the Navy called him to active duty and he became a navy pilot. In 1950, he was sent to Korea where he flew 78 combat missions from the carrier USS Essex in a Grumman F9F-2 Panther. He received the Air Medal and two Gold Stars. In 1952, Armstrong returned to Purdue University and graduated with a bachelors degree in aeronautical engineering in 1955. He later earned a masters degree in aerospace engineering from the University of Southern California. At the High-Speed Flight Station (which later became the NASA Dryden Flight Research Center) Armstrong served as project pilot on the North American F-100A and -C aircraft, McDonnell F-101, and the Lockheed F-104A. He also flew the Bell X-1B (4 flights, first on August 15, 1957), Bell X-5 (one flight, the last in the program, on October 25, 1955) and the Paresev. On November 30, 1960, Armstrong made his first flight in the X-15. He made a total of seven flights in the rocket plane reaching an altitude of 207,500 feet in the X-15-3 and a Mach number of 5.74 (3,989 mph) in the X-15-1. He left the Flight Research Center with a total of 2450 flying hours in more than 50 aircraft types. He was a member of the USAF-NASA Dyna-Soar Pilot Consultant Group, and studied X-20 Dyna-Soar approaches and abort maneuvers through use of the F-102A and F5D jet aircraft. Armstrong later accumulated a total of 8 days and 14 hours in space, including 2 hours and 48 minutes walking on the Moon. In March 1966, he was commander of the Gemini 8 mission that performed the first successful docking of two vehicles in space. As spacecraft commander for the Apollo 11 lunar mission, on July 20, 1969, he became the first human to set foot on the Moon. In 1970 he was appointed Deputy Associate Administrator for Aeronautics at NASA Headquarters. He resigned in 1971. Neil wrote several technical reports and presented a number of research papers. In June 1962, the Octave Chanute Award was presented to Neil by the Institute of the Aerospace Sciences. Other awards received by Neil have included the NASA Distinguished Service Medal and the NASA Exceptional Service Medal.
Date 01.01.1958
Long Leonid
Title Long Leonid
Explanation Just last week this long lovely Leonid shower [ http://spacescience.com/headlines/y2000/ ast21nov_1.htm ] meteor arced through the night. Captured on [ http://www.comet-track.com/meteor/leonids00/ leonids00.html ] November 17/18 by photographer [ http://www.comet-track.com ] Bob Yen, the meteor trail spans about 70 times the apparent diameter of the full moon in the skies above Mt. Wilson, California, USA. The Leonid's path flashes from the outskirts of constellation Gemini [ http://www.seds.org/Maps/Stars_en/Fig/ gemini.html ] to the triangle-shaped head of Taurus [ http://www.astro.uiuc.edu/~kaler/sow/ taurus-p.html ] (lower right). Of course, the trail points back toward Leo, the shower's [ http://comets.amsmeteors.org/meteors/showers/ leonids.html ] eponymous radiant, while passing near such night sky notables as galactic star cluster M35 [ http://www.seds.org/messier/m/m035.html ] (upper left) and Taurus's brightest star, red giant Aldebaran [ http://www.astro.uiuc.edu/~kaler/sow/ aldebaran.html ]. Though the sky was ruled by a bright but waning Moon and brilliant Jupiter, the Leonid meteor shower [ http://www.spaceweather.com/meteors/gallery_18nov00.html ] still awed observers at dark sky locations with peak rates of hundreds of meteors per hour.
A 2001 Leonids Meteor Shower …
Title A 2001 Leonids Meteor Shower Fireball
Explanation The 2001 Leonids Meteor Shower [ http://science.nasa.gov/headlines/y2001/ast15nov_1.htm ] gave quite a show to many parts of the world yesterday during the early morning hours. Many sleepy observers [ http://leonid.arc.nasa.gov/live/newlive.html ] venturing into their own backyards [ http://www.skypub.com/tips/startright2.html ] were treated to several bright meteors per minute streaking across the sky. This rate made the 2001 Leonids [ http://space.com/scienceastronomy/astronomy/leonids_wrap_011118.html ] the most active meteor shower in over three decades [ http://comets.amsmeteors.org/meteors/showers/leonidsrecoll.html ]. Pictured above is a bright Leonid fireball [ http://antwrp.gsfc.nasa.gov/apod/ap981125.html ] that briefly lit up Hawaii [ http://www.state.hi.us/ ] yesterday morning. A CONCAM nighttime all-sky monitor [ http://concam.net/about.html ] on Mauna Kea [ http://www.ifa.hawaii.edu/mko/ ], a dormant volcano [ http://volcano.und.nodak.edu/vwdocs/volc_images/north_america/hawaii/mauna_kea.html ], caught the bright meteor, seen as the very bright streak across the lower part of the fisheye [ http://www.zeta.org.au/~andrewa/ajaa31.htm ] image. The meteor track crossed the Galactic plane [ http://antwrp.gsfc.nasa.gov/apod/ap990224.html ] (the faint glow that runs from the lower left to upper right), passed below the planet Jupiter [ http://www.nineplanets.org/jupiter.html ], and through the constellation Orion [ http://antwrp.gsfc.nasa.gov/apod/ap000611.html ]. CONCAMs in Hawaii [ http://concam.net/mk/ ], Arizona [ http://concam.net/kp/ ], and California [ http://concam.net/mw/ ] all recorded numerous bright meteors [ http://SpaceWeather.com/meteors/gallery_18nov01.html ] during this year's Leonids [ http://leonids.hq.nasa.gov/leonids/gallery/ ].
Three Planets from Mt. Hamil …
Title Three Planets from Mt. Hamilton
Explanation Venus, Mercury, and Saturn wandered close [ http://antwrp.gsfc.nasa.gov/apod/ap050624.html ] together in western evening skies last week. On Saturn [ http://saturn.jpl.nasa.gov/kids/ fun-facts-saturn.cfm ]day, June 25, astronomer R. Jay GaBany recorded this snapshot of their eye-catching planetary conjunction, from historic Lick Observatory [ http://www.ucolick.org/ ] on Mt. Hamilton [ http://mthamilton.ucolick.org/hamcam/ ], California, USA. The view looks toward the Pacific shortly after sunset with the lights of San Jose and the southern San Francisco Bay area in the foreground. Of course, Venus is [ http://antwrp.gsfc.nasa.gov/apod/ap050107.html ] the brightest of the trio. Mercury [ http://www.jpl.nasa.gov/solar_system/planets/ planets_index.html ] is nearby on the right and Saturn is below and left, closest to the horizon. Farther to the right of the planetary triangle are Pollux and Castor, twin stars [ http://stardate.org/nightsky/constellations/gemini.html ] of Gemini, with Regulus [ http://www.astro.uiuc.edu/~kaler/sow/regulus.html ], bright star of the constellation Leo, at the very upper left corner of the picture. In the coming days [ http://skyandtelescope.com/observing/ataglance/ article_110_1.asp ], Venus and Mercury remain close, while Saturn continues to drop below them, toward the horizon.
Pilot Neil Armstrong with X- …
Photo Description NASA test pilot Neil Armstrong is seen here next to the X-15 ship #1 (56-6670) after a research flight. Neil A. Armstrong joined the National Advisory Committee for Aeronautics (NACA) at the Lewis Flight Propulsion Laboratory (later NASA?s Lewis Research Center, Cleveland, Ohio, and today the Glenn Research Center) in 1955. Later that year, he transferred to the NACA?s High-Speed Flight Station (today, NASA?s Dryden Flight Research Center) at Edwards Air Force Base in California as an aeronautical research scientist and then as a pilot, a position he held until becoming an astronaut in 1962. He was one of nine NASA astronauts in the second class to be chosen. As a research pilot Armstrong served as project pilot on the F-100A and F-100C aircraft, F-101, and the F-104A. He also flew the X-1B, X-5, F-105, F-106, B-47, KC-135, and Paresev. He left Dryden with a total of over 2450 flying hours. He was a member of the USAF-NASA Dyna-Soar Pilot Consultant Group before the Dyna-Soar project was cancelled, and studied X-20 Dyna-Soar approaches and abort maneuvers through use of the F-102A and F5D jet aircraft. Armstrong was actively engaged in both piloting and engineering aspects of the X-15 program from its inception. He completed the first flight in the aircraft equipped with a new flow-direction sensor (ball nose) and the initial flight in an X-15 equipped with a self-adaptive flight control system. He worked closely with designers and engineers in development of the adaptive system, and made seven flights in the rocket plane from December 1960 until July 1962. During those fights he reached a peak altitude of 207,500 feet in the X-15-3, and a speed of 3,989 mph (Mach 5.74) in the X-15-1. Armstrong was born August 5, 1930, in Wapakoneta, Ohio. He attended Purdue University, earning his Bachelor of Science degree in aeronautical engineering in 1955. During the Korean War, which interrupted his engineering studies, he flew 78 combat missions in F9F-2 jet fighters. He was awarded the Air Medal and two Gold Stars. He later earned a Master of Science degree in aerospace engineering from the University of Southern California. Armstrong has a total of 8 days and 14 hours in space, including 2 hours and 48 minutes walking on the Moon. In March 1966 he was commander of the Gemini 8 orbital space flight with David Scott as pilot?the first successful docking of two vehicles in orbit. On July 20, 1969, during the Apollo 11 lunar mission, he became the first human to set foot on the Moon. From 1969 to 1971 he was Deputy Associate Administrator for Aeronautics at NASA Headquarters, and resigned from NASA in August 1971 to become Professor of Engineering at the University of Cincinnati, a post he held until 1979. He became Chairman of the Board of Cardwell International, Ltd., in Lebanon, Ohio, in 1980 and served in that capacity until 1982. During the years 1982-1992, Armstrong was chairman of Computing Technologies for Aviation, Inc., in Charlottesville,, Virginia. From 1981 to 1999, he served on the board of directors for Eaton Corp. He served as chairman of the board of AIL Systems, Inc. of Deer Park, New York, until 1999 and in 2000 was elected chairman of the board of EDO Corp., a manaufacturer of electronic and mechanical systems for the aerospace, defense and industrial markets, based in New York City. From 1985 to 1986, Armstrong served on the National Commission on Space, a presidential committee to develop goals for a national space program into the 21st century. He was also Vice Chairman of the committee investigating the Space Shuttle Challenger disaster in 1986. During the early 1990s he hosted an aviation documentary series for television entitled First Flights.
Project Description The X-15 was a rocket-powered aircraft 50 ft long with a wingspan of 22 ft. It was a missile-shaped vehicle with an unusual wedge-shaped vertical tail, thin stubby wings, and unique fairings that extended along the side of the fuselage. The X-15 weighed about 14,000 lb empty and approximately 34,000 lb at launch. The XLR-99 rocket engine, manufactured by Thiokol Chemical Corp., was pilot controlled and was capable of developing 57,000 lb of rated thrust (actual thrust reportedly climbed to 60,000 lb). North American Aviation built three X-15 aircraft for the program. The X-15 research aircraft was developed to provide in-flight information and data on aerodynamics, structures, flight controls, and the physiological aspects of high-speed, high-altitude flight. A follow-on program used the aircraft as a testbed to carry various scientific experiments beyond the Earth's atmosphere on a repeated basis. For flight in the dense air of the usable atmosphere, the X-15 used conventional aerodynamic controls such as rudder surfaces on the vertical stabilizers to control yaw and canted horizontal surfaces on the tail to control pitch when moving in synchronization or roll when moved differentially. For flight in the thin air outside of the appreciable Earth's atmosphere, the X-15 used a reaction control system. Hydrogen peroxide thrust rockets located on the nose of the aircraft provided pitch and yaw control. Those on the wings provided roll control. Because of the large fuel consumption, the X-15 was air launched from a B-52 aircraft at 45,000 ft and a speed of about 500 mph. Depending on the mission, the rocket engine provided thrust for the first 80 to 120 sec of flight. The remainder of the normal 10 to 11 min. flight was powerless and ended with a 200-mph glide landing. Generally, one of two types of X-15 flight profiles was used: a high-altitude flight plan that called for the pilot to maintain a steep rate of climb, or a speed profile that called for the pilot to push over and maintain a level altitude. The X-15 was flown over a period of nearly 10 years--June 1959 to Oct. 1968--and set the world's unofficial speed and altitude records of 4,520 mph (Mach 6.7) and 354,200 ft (over 67 mi) in a program to investigate all aspects of piloted hypersonic flight. Information gained from the highly successful X-15 program contributed to the development of the Mercury, Gemini, and Apollo manned spaceflight programs, and also the Space Shuttle program. The X-15s made a total of 199 flights and were manufactured by North American Aviation. X-15-1, serial number 56-6670, is now located at the National Air and Space Museum, Washington DC. North American X-15A-2, serial number 56-6671, is at the United States Air Force Museum, Wright-Patterson AFB, Ohio. The X-15-3, serial number 56-6672, crashed on 15 November 1967, resulting in the death of Maj. Michael J. Adams.
Photo Date 1960s
X-15 with test pilot Bill Da …
Photo Date 1966
X-15 contrail after launch
Photo Date probably 1962
X-15 mock-up with test pilot …
Photo Date 1993
Installation of X-15 full-sc …
Photo Date Sep. 1995
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