The HiMAT (Highly Maneuverable Aircraft Technology) subscale research vehicle, seen here during a research flight, was flown by the NASA Dryden Flight Research Center, Edwards, California, from mid 1979 to January 1983. The aircraft demonstrated advanced fighter technologies that have been used in the development of many modern high performance military aircraft.
This image of the suspected Black Hole, Cygnus X-1, was the first object seen by the High Energy Astronomy Observatory (HEAO)-2/Einstein Observatory. According to the theories to date, one concept of a black hole is a star, perhaps 10 times more massive than the Sun, that has entered the last stages of stelar evolution. There is an explosion triggered by nuclear reactions after which the star's outer shell of lighter elements and gases is blown away into space and the heavier elements in the stellar core begin to collapse upon themselves. Once this collapse begins, the inexorable force of gravity continues to compact the material until it becomes so dense it is squeezed into a mere point and nothing can escape from its extreme gravitational field, not even light. The HEAO-2, the first imaging and largest x-ray telescope built to date, was capable of producing actual photographs of x-ray objects. Shortly after launch, the HEAO-2 was nicknamed the Einstein Observatory by its scientific experimenters in honor of the centernial of the birth of Albert Einstein, whose concepts of relativity and gravitation have influenced much of modern astrophysics, particularly x-ray astronomy.
Sykorsky Bearingless Main Rotor test in 40x80ft w.t.
Voyager 1 passed the Saturnian system in November 1980; nine months later Voyager 2 passed through this same system. The ensuing scientific discoveries were unprecedented with regards to the rings around Saturn and its satellite's chemical makeup. Pictured are: Saturn (shown with rings), Dione (forefront), Tethys and Mimas (lower right), Enceladus and Rhea (upper left) and Titan in distant orbit (upper right).
Bearingless Main Rotor
Portrait of Katherine Johnson
This artist's concept depicts the Hubble Space Telescope after being released into orbit, with the high gain anternas and solar arrays deployed and the aperture doors opened. The HST is the product of a partnership between NASA, European Space Agency Contractors, and the international community of astronomers. It is named after Edwin P. Hubble, an American Astronomer who discovered the expanding nature of the universe and was the first to realize the true nature of galaxies. The purpose of the HST, the most complex and sensitive optical telescope ever made, is to study the cosmos from a low-Earth orbit. By placing the telescope in space, astronomers are able to collect data that is free of the Earth's atmosphere. The HST detects objects 25 times fainter than the dimmest objects seen from Earth and provides astronomers with an observable universe 250 times larger than visible from ground-based telescopes, perhaps as far away as 14 billion light-years. The HST views galaxies, stars, planets, comets, possibly other solar systems, and even unusual phenomena such as quasars, with 10 times the clarity of ground-based telescopes. The major elements of the HST are the Optical Telescope Assembly (OTA), the Support System Module (SSM), and the Scientific Instruments (SI). The HST is 42.5-feet (13-meters) long and weighs about 25,000 pounds (11,600 kilograms). The HST was deployed from the Space Shuttle Discovery (STS-31 mission) into Earth orbit in April 1990. The Marshall Space Flight Center had responsibility for design, development, and construction of the HST. The Perkin-Elmer Corporation, in Danbury, Connecticut, developed the optical system and guidance sensors. The Lockheed Missile and Space Company of Sunnyvale, California produced the protective outer shroud and spacecraft systems, and assembled and tested the finished telescope.
Space Shuttle Orbiter Enterprise mated to an external fuel tank and two solid rocket boosters on top of a Mobil Launcher Platform, undergoes fit and function checks at the launch site for the first Space Shuttle at Launch Complex 39's Pad A. The dummy Space Shuttle was assembled in the Vehicle Assembly Building and rolled out to the launch site on May 1 as part of an exercise to make certain shuttle elements are compatible with the Spaceport's assembly and launch facilities and ground support equipment, and help clear the way for the launch of the Space Shuttle Orbiter Columbia.
QSRA (NASA-715) takeoff and landing trials onboard the USS Kitty Hawk
The HiMAT (Highly Maneuverable Aircraft Technology) subscale research vehicle, seen here during a research flight, was flown by the NASA Dryden Flight Research Center, Edwards, California, from mid 1979 to January 1983. The aircraft demonstrated advanced fighter technologies that have been used in the development of many modern high performance military aircraft.
Range : 660,000 kilometers (400,000 miles) Time : 5:05 am PST This Voyager 1 picture of Mimas shows a large impact structure at 110 degrees W Long., located on that face of the moon which leads Mimas in its orbit. The feature, about 130 kilometers in diameter (80 miles), is more than 1/4 the diameter of the entire moon. This is a particularly interesting feature in view of its large diameter compared with the size of the satellite, and may have the largest crater diameter/satillite diameter ratio in the solar system. The crater has a raised rim and central peak, typical of large impact structures on terrestrial planets. Additional smaller craters, 15-45 kilometers in diameter, can be seen scattered across the surface, particularly alon the terminator. Mimas is one of the smaller Saturnian satellites with a low density implying its chief component is ice.
Ames Center Director Sy Syverston enjoys a moment with fellow employees during Ames Heritage Week lunch.
The payload bay doors of the Space Shuttle Orbiter Columbia were opened for the first time today using the orbiter's onboard door operation system. The hinges of the payload bay doors are not designed to support the weight of the doors while open horizontally in the Earth's one 'g' environment and a counterweight zero 'g' device supports the weight of the doors while they are open for processing in the OPF.
Mrs. Katherine G. Johnson at Work
Solar-powered Gossamer Penguin in flight with Janice Brown and Ray Morgan riding chase bicycle.
The payload bay doors of the Space Shuttle Orbiter Columbia were opened for the first time today using the orbiter's onboard door operation system. The hinges of the payload bay doors are not designed to support the weight of the doors while open horizontally in the Earth's one 'g' environment and a counterweight zero 'g' device supports the weight of the doors while they are open for processing in the OPF.
Boeing model 737 (TCV) Terminally configured vehicle cut away (ref: L80-8015)
The first solid rocket booster solid motor segemnts to arrive at KSC, the left and right hand aft segments are off-loaded into High Bay 4 in the Vehicle Assembly Building and mated to their respective SRB aft skirts. The two aft assemblies will support the entire 150 foot tall solid boosters, in turn supporting the external tank and Orbiter Columbia on the Mobile Launcher Platform, for the first orbital flight test of the Space Shuttle.
This illustration shows the Hubble Space Telescope's (HST's) major configuration elements. The spacecraft has three interacting systems: The Support System Module (SSM), an outer structure that houses the other systems and provides services such as power, communication, and control; The Optical Telescope Assembly (OTA), which collects and concentrates the incoming light in the focal plane for use by the Scientific Instruments (SI); and five SIs. The SI Control and Data Handling (CDH) unit controls the five SI's, four that are housed in an aft section focal plane structure and one that is placed along the circumference of the spacecraft. The purpose of the HST, the most complex and sensitive optical telescope ever made, is to study the cosmos from a low-Earth orbit. By placing the telescope in space, astronomers are able to collect data that is free of the Earth's atmosphere. The HST detects objects 25 times fainter than the dimmest objects seen from Earth and provides astronomers with an observable universe 250 times larger than visible from ground-based telescopes, perhaps as far away as 14 billion light-years. The HST views galaxies, stars, planets, comets, possibly other solar systems, and even unusual phenomena such as quasars, with 10 times the clarity of ground-based telescopes. The HST was deployed from the Space Shuttle Discovery (STS-31 mission) into Earth orbit in April 1990. The Marshall Space Flight Center had responsibility for design, development, and construction of the HST. The Perkin-Elmer Corporation, in Danbury, Cornecticut, developed the optical system and guidance sensors. The Lockheed Missile and Space Company of Sunnyvale, California produced the protective outer shroud and spacecraft systems, and assembled and tested the finished telescope.
KENNEDY SPACE CENTER, FLA. - The first Space Shuttle vehicle destined to fly in space moves toward Pad A at Complex 39, where it will be launched. The STS-1 vehicle - consisting of America's first reusable spaceship, Columbia, the external propellant tank and twin solid rocket boosters - was assembled on a Mobile Launcher Platform in the Vehicle Assembly Building. A six-million-pound tractor, called the Crawler-Transporter, is used to carry the Space Shuttle from the VAB to the launch pad, about 3.5 miles away.
N-231 High Reynolds Number Channel II Facility In this timeframe the test section was designed specifically to test two-dimensional airfoil models. It is equipped with 'through-the-wall' turntables that remotely position the airfoil, with flexible upper and lower walls that can be adjusted to minimize wall interference. Porous side-wall panels provide boundary-layer removal.
Bearingless Main Rotor
QSRA (NASA-715) takeoff and landing trials onboard the USS Kitty Hawk
The Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautical and Space Administration (NASA) to operate a long-lived space-based observatory. It was the flagship mission of NASA's Great Observatories program. The HST program began as an astronomical dream in the 1940s. During the 1970s and 1980s, the HST was finally designed and built becoming operational in the 1990s. The HST was deployed into a low-Earth orbit on April 25, 1990 from the cargo bay of the Space Shuttle Discovery (STS-31). The design of the HST took into consideration its length of service and the necessity of repairs and equipment replacement by making the body modular. In doing so, subsequent shuttle missions could recover the HST, replace faulty or obsolete parts and be re-released. Marshall Space Flight Center’s (MSFC's) Neutral Buoyancy Simulator (NBS) served as the test center for shuttle astronauts training for Hubble related missions. Shown is astronaut Anna Fisher suiting up for training on a mockup of a modular section of the HST for an axial scientific instrument change out.
Bill Davis performing checkout at the Materials Experiment Assembly (MEA) Isothermal Furnace.
Space Shuttle Simulator cockpit
Range : 106,250,000 km. ( 66 million miles) P-22830C This, Voyager 1 image shows Saturn and three of its satellites. A series of dark and light cloud bands appears through high altitude haze in the northern hemisphere. Cosiderable structure can be seen in the rings. The Cassini division, between the A-ring and B-ring, is readily visible. The shadow of rings on the planet's disk can also be seeen. The three satellites visible are, left to right, Enceladus (off the left edge of rings), Dione (just below the planet), and Tethys (at right edge of frame). The spacecraft will make its closest approach, 124,200 km. (77,174 miles) abovr the cloud tops, at 3:45 pm PST on Nov. 12, 1980. Nine months later, in August 1981, Voyager 2 will encounter Saturn and then continue on to Uranus.
C-141 KAO: CAT experiment
Like the Crab Nebula, the Vela Supernova Remnant has a radio pulsar at its center. In this image taken by the High Energy Astronomy Observatory (HEAO)-2/Einstein Observatory, the pulsar appears as a point source surrounded by weak and diffused emissions of x-rays. HEAO-2's computer processing system was able to record and display the total number of x-ray photons (a tiny bundle of radiant energy used as the fundamental unit of electromagnetic radiation) on a scale along the margin of the picture. The HEAO-2, the first imaging and largest x-ray telescope built to date, was capable of producing actual photographs of x-ray objects. Shortly after launch, the HEAO-2 was nicknamed the Einstein Observatory by its scientific experimenters in honor of the centernial of the birth of Albert Einstein, whose concepts of relativity and gravitation have influenced much of modern astrophysics, particularly x-ray astronomy. The HEAO-2, designed and developed by TRW, Inc. under the project management of the Marshall Space Flight Center, was launched aboard an Atlas/Centaur launch vehicle on November 13, 1978.
CAPE CANAVERAL, Fla. -- AERIALS KSC PAD 39A/B, VAB AND SHUTTLE STRIP, ALTITUDE 11,000 FEET, 270 DEGREES. Photo credit: NASA
SPACE SHUTTLE ORBITER COLUMBIA 102 IS SHOWN BACKING OUT OF ITS MANUFACTURING FACILITY AT PALMDALE, CA THE ROCKWELL INTERNATIONAL SPACE DIVISION PLANT, ENROUTE TO DRYDEN FLIGHT RESEARCH CENTER. THIS ORBITER WILL BE THE FIRST SHUTTLE SPACECRAFT THAT WILL CARRY TWO ASTRONAUTS, JOHN YOUNG AND RICHARD CRIPPEN, INTO EARTH ORBITAL TEST FLIGHT IN LATE 1979.
KENNEDY SPACE CENTER, FLA. - Space Shuttle main engines #1 and #3 being installed in Orbiter Columbia.
N-233 computer hardware VAX Control Data
KENNEDY SPACE CENTER, FLA. - STS-1 arrived at Launch Complex 39A this afternoon at the end of a three-and-a-half mile journey from the Vehicle Assembly Building. The first Space Shuttle assembly will undergo an extensive series of pad validation tests and a dress rehearsal for launch - including a 20-second test firing of the orbiter’s three main engines - before being cleared for flight. The STS-1 mission, known as a shuttle systems test flight, will seek to demonstrate safe launch into orbit and safe return of the orbiter and crew and verify the combined performance of the entire shuttle vehicle -- orbiter, solid rocket boosters and external tank. STS-1 will be launched from Pad A at the Kennedy Space Center's Launch Complex 39 no earlier than March 1981.
Once the United States' space program had progressed from Earth's orbit into outerspace, the prospect of building and maintaining a permanent presence in space was realized. To accomplish this feat, NASA launched a temporary workstation, Skylab, to discover the effects of low gravity and weightlessness on the human body, and also to develop tools and equipment that would be needed in the future to build and maintain a more permanent space station. The structures, techniques, and work schedules had to be carefully designed to fit this unique construction site. The components had to be lightweight for transport into orbit, yet durable. The station also had to be made with removable parts for easy servicing and repairs by astronauts. All of the tools necessary for service and repairs had to be designed for easy manipulation by a suited astronaut. Construction methods had to be efficient due to the limited time the astronauts could remain outside their controlled environment. In lieu of all the specific needs for this project, an environment on Earth had to be developed that could simulate a low gravity atmosphere. A Neutral Buoyancy Simulator (NBS) was constructed by NASA's Marshall Space Flight Center (MSFC) in 1968. Since then, NASA scientists have used this facility to understand how humans work best in low gravity and also provide information about the different kinds of structures that can be built. Pictured is a Massachusetts Institute of Technology (MIT) student working in a spacesuit on the Experimental Assembly of Structures in Extravehicular Activity (EASE) project which was developed as a joint effort between MFSC and MIT. The EASE experiment required that crew members assemble small components to form larger components, working from the payload bay of the space shuttle. The MIT student in this photo is assembling two six-beam tetrahedrons.
KENNEDY SPACE CENTER, FLA. - The first Space Shuttle vehicle destined to fly in space moves toward Launch Complex 39A where it will be launched. The STS-1 vehicle, consisting of America’s first reusable space ship - the orbiter Columbia, an external propellant tank and two solid rocket boosters, was assembled on a Mobile Launcher Platform in the Vehicle Assembly Building. A six-million pound tractor, called the Crawler-Transporter, is used to carry the Space Shuttle from the VAB to the launch pad, some 3.5 miles away.
N-231 High Reynolds Number Channel Facility (An example of a Versatile Wind Tunnel) Tunnel 1 I is a blowdown Facility that utilizes interchangeable test sections and nozzles. The facility provides experimental support for the fluid mechanics research, including experimental verification of aerodynamic computer codes and boundary-layer and airfoil studies that require high Reynolds number simulation. (Tunnel 1)
The Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautical and Space Administration (NASA) to operate a long-lived space-based observatory. It was the flagship mission of NASA's Great Observatories program. The HST program began as an astronomical dream in the 1940s. During the 1970s and 1980s, the HST was finally designed and built becoming operational in the 1990s. The HST was deployed into a low-Earth orbit on April 25, 1990 from the cargo bay of the Space Shuttle Discovery (STS-31). The design of the HST took into consideration its length of service and the necessity of repairs and equipment replacement by making the body modular. In doing so, subsequent shuttle missions could recover the HST, replace faulty or obsolete parts and be re-released. Marshall Space Flight Center’s (MSFC's) Neutral Buoyancy Simulator (NBS) served as the test center for shuttle astronauts training for Hubble related missions. Shown is astronaut Anna Fisher training on a mock-up of a modular section of the HST for an axial scientific instrument change out.
C-141 KAO: CAT equipment
The Hubble Space Telescope (HST) is a cooperative program of the European Space Agency (ESA) and the National Aeronautical and Space Administration (NASA) to operate a long-lived space-based observatory. It was the flagship mission of NASA's Great Observatories program. The HST program began as an astronomical dream in the 1940s. During the 1970s and 1980s, the HST was finally designed and built becoming operational in the 1990s. The HST was deployed into a low-Earth orbit on April 25, 1990 from the cargo bay of the Space Shuttle Discovery (STS-31). The design of the HST took into consideration its length of service and the necessity of repairs and equipment replacement by making the body modular. In doing so, subsequent shuttle missions could recover the HST, replace faulty or obsolete parts and be re-released. MSFC's Neutral Buoyancy Simulator (NBS) served as the test center for shuttle astronauts training for Hubble related missions. Shown is astronaut Anna Fisher suiting up for training on a mockup of a modular section of the HST for an axial scientific instrument change out.
KENNEDY SPACE CENTER, FLA. - This eagle's eye view of STS-1 shows the space vehicle for the first Space Shuttle mission shortly after it was moved out of the Vehicle Assembly Builidng at 8 a.m. today for the 3.5-mile journey to Complex 39's Pad A. The Shuttle rests atop the Mobile Launcher Platform from which launch is scheduled no earlier than March 1981. Thousands of visitors and hundreds of news media representatives viewed the beginning of the move under leaden skies and in unseasonably cold temperatures in the low 40s.
This artist's concept depicts the Hubble Space Telescope (HST) being positioned for release from the Space Shuttle orbiter by the Remote Manipulator System (RMS). The HST is the product of a partnership between NASA, European Space Agency Contractors, and the international community of astronomers. It is named after Edwin P. Hubble, an American Astronomer who discovered the expanding nature of the universe and was the first to realize the true nature of galaxies. The purpose of the HST, the most complex and sensitive optical telescope ever made, is to study the cosmos from a low-Earth orbit. By placing the telescope in space, astronomers are able to collect data that is free of the Earth's atmosphere. The HST detects objects 25 times fainter than the dimmest objects seen from Earth and provides astronomers with an observable universe 250 times larger than visible from ground-based telescopes, perhaps as far away as 14 billion light-years. The HST views galaxies, stars, planets, comets, possibly other solar systems, and even unusual phenomena such as quasars, with 10 times the clarity of ground-based telescopes. The major elements of the HST are the Optical Telescope Assembly (OTA), the Support System Module (SSM), and the Scientific Instruments (SI). The HST is 42.5-feet (13- meters) long and weighs about 25,000 pounds (11,600 kilograms). The HST was deployed from the Space Shuttle Discovery (STS-31 mission) into Earth orbit in April 1990. The Marshall Space Flight Center had responsibility for design, development, and construction of the HST. The Perkin-Elmer Corporation, in Danbury, Cornecticut, developed the optical system and guidance sensors. The Lockheed Missile and Space Company of Sunnyvale, California produced the protective outer shroud and spacecraft systems, and assembled and tested the finished telescope.
Boeing model 737 TCV research cockpit
Once the United States' space program had progressed from Earth's orbit into outerspace, the prospect of building and maintaining a permanent presence in space was realized. To accomplish this feat, NASA launched a temporary workstation, Skylab, to discover the effects of low gravity and weightlessness on the human body, and also to develop tools and equipment that would be needed in the future to build and maintain a more permanent space station. The structures, techniques, and work schedules had to be carefully designed to fit this unique construction site. The components had to be lightweight for transport into orbit, yet durable. The station also had to be made with removable parts for easy servicing and repairs by astronauts. All of the tools necessary for service and repairs had to be designed for easy manipulation by a suited astronaut. Construction methods had to be efficient due to the limited time the astronauts could remain outside their controlled environment. In lieu of all the specific needs for this project, an environment on Earth had to be developed that could simulate a low gravity atmosphere. A Neutral Buoyancy Simulator (NBS) was constructed by NASA's Marshall Space Flight Center (MSFC) in 1968. Since then, NASA scientists have used this facility to understand how humans work best in low gravity and also provide information about the different kinds of structures that can be built. Pictured is a Massachusetts Institute of Technology (MIT) student working in a spacesuit on the Experimental Assembly of Structures in Extravehicular Activity (EASE) project which was developed as a joint effort between MFSC and MIT. The EASE experiment required that crew members assemble small components to form larger components, working from the payload bay of the space shuttle. The MIT student in this photo is assembling two six-beam tetrahedrons.
The Highly Maneuverable Aircraft Technology (HiMAT) research vehicle is shown here mated to a wing pylon on NASA’s B-52 mothership aircraft. The HiMAT was a technology demonstrator to test structures and configurations for advanced fighter concepts. Over the course of more than 40 years, the B-52 proved a valuable workhorse for NASA’s Dryden Flight Research Center (under various names), launching a wide variety of vehicles and conducting numerous other research flights.
N-233 computer hardware - digital VAX-11/780
A mockup of the Spacelab II configuration was built at Marshall's Completed Payload Crew Training Complex (PCTC) located at Building 4612.
Once the United States' space program had progressed from Earth's orbit into outerspace, the prospect of building and maintaining a permanent presence in space was realized. To accomplish this feat, NASA launched a temporary workstation, Skylab, to discover the effects of low gravity and weightlessness on the human body, and also to develop tools and equipment that would be needed in the future to build and maintain a more permanent space station. The structures, techniques, and work schedules had to be carefully designed to fit this unique construction site. The components had to be lightweight for transport into orbit, yet durable. The station also had to be made with removable parts for easy servicing and repairs by astronauts. All of the tools necessary for service and repairs had to be designed for easy manipulation by a suited astronaut. Construction methods had to be efficient due to the limited time the astronauts could remain outside their controlled environment. In lieu of all the specific needs for this project, an environment on Earth had to be developed that could simulate a low gravity atmosphere. A Neutral Buoyancy Simulator (NBS) was constructed by NASA's Marshall Space Flight Center (MSFC) in 1968. Since then, NASA scientists have used this facility to understand how humans work best in low gravity and also provide information about the different kinds of structures that can be built. Pictured is a Massachusetts Institute of Technology (MIT) student working in a spacesuit on the Experimental Assembly of Structures in Extravehicular Activity (EASE) project which was developed as a joint effort between MFSC and MIT. The EASE experiment required that crew members assemble small components to form larger components, working from the payload bay of the space shuttle. The MIT student in this photo is assembling two six-beam tetrahedrons.
N-233 computer hardware Vax Control Data
Bearingless Main Rotor
C-141 KAO: CAT experiment - compressor damage
This artist's concept depicts the Hubble Space Telescope (HST) being raised to a vertical position in the cargo bay of the Space Shuttle orbiter. The HST is the product of a partnership between NASA, European Space Agency Contractors, and the international community of astronomers. It is named after Edwin P. Hubble, an American Astronomer who discovered the expanding nature of the universe and was the first to realize the true nature of galaxies. The purpose of the HST, the most complex and sensitive optical telescope ever made, is to study the cosmos from a low-Earth orbit. By placing the telescope in space, astronomers are able to collect data that is free of the Earth's atmosphere. The HST detects objects 25 times fainter than the dimmest objects seen from Earth and provides astronomers with an observable universe 250 times larger than visible from ground-based telescopes, perhaps as far away as 14 billion light-years. The HST views galaxies, stars, planets, comets, possibly other solar systems, and even unusual phenomena such as quasars, with 10 times the clarity of ground-based telescopes. The major elements of the HST are the Optical Telescope Assembly (OTA), the Support System Module (SSM), and the Scientific Instruments (SI). The HST is 42.5-feet (13-meters) long and weighs about 25,000 pounds (11,600 kilograms). The HST was deployed from the Space Shuttle Discovery (STS-31 mission) into Earth orbit in April 1990. The Marshall Space Flight Center had responsibility for design, development, and construction of the HST. The Perkin-Elmer Corporation, in Danbury, Cornecticut, developed the optical system and guidance sensors. The Lockheed Missile and Space Company of Sunnyvale, California produced the protective outer shroud and spacecraft systems, and assembled and tested the finished telescope.
Bearingless Main Rotor
Range : 34 million km. ( 21.1 million miles) P-22993C This Voyager 1 photograph of Saturn was taken on the last day it could be captured within a single narrow angle camera frame as the spacecraft neared the planet for it's closest approach on Nov. 12, 1980. Dione, one of Saturn's innermost satellites, appears as three color spots just below the planet's south pole. An abundance of previously unseen detail is apparent in the rings. For example, a gap in the dark, innermst ring, C-ring or Crepe Ring, is clearly shown. Also, material is seen inside the relatively wide Cassini Division, seperating the middle, B-ring from the outermost ring, the A-ring. The Encke division is shown near the outer edge of A-ring. The detail in the ring's shadows cast on the planet is of particular interest. The broad dark band near the equator is the shadow of B-ring. The thinner, brighter line just to the south is the shadow of the less dense A-ring.
Bearingless Main Rotor
KENNEDY SPACE CENTER, FLA. - Shuttle Orbiter Columbia lift and mate to external tank in the Vehicle Assembly Building (VAB).
Bearingless Main Rotor
C-141 KAO: Dr Fred Witteborn and Ames Science Team onbaord for CAT experiment
This supernova in the constellation Cassiopeia was observed by Tycho Brahe in 1572. In this x-ray image from the High Energy Astronomy Observatory (HEAO-2/Einstein Observatory produced by nearly a day of exposure time, the center region appears filled with emissions that can be resolved into patches or knots of material. However, no central pulsar or other collapsed object can be seen. The HEAO-2, the first imaging and largest x-ray telescope built to date, was capable of producing actual photographs of x-ray objects. Shortly after launch, the HEAO-2 was nicknamed the Einstein Observatory by its scientific experimenters in honor of the centernial of the birth of Albert Einstein, whose concepts of relativity and gravitation have influenced much of modern astrophysics, particularly x-ray astronomy. The HEAO-2, designed and developed by TRW, Inc. under the project management of the Marshall Space Flight Center, was launched aboard an Atlas/Centaur launch vehicle on November 13, 1978.
Sikorsky Bearingless Main Rotor test in 40x80ft w.t.
CAPE CANAVERAL, Fla. -- At Cape Canaveral Air Force Station in Florida, the INTELSAT V spacecraft is enclosed in a protective shroud for transport from Hangar AO to the Explosive Safe Facility for final servicing and encapsulation. This is the first of a new series of INTELSAT spacecraft. The INTELSAT V is the largest and highest-capacity commercial communications satellite built to date. The 4,300-pound spacecraft is scheduled for launch on an Atlas Centaur rocket from Complex 36 no earlier than December 4. It will operate in geosynchronous orbit over the Atlantic Ocean. Photo Credit: NASA
N-231 High Reynolds Number Channel Facility (Tunnel 2, Airfoil Test Section)
C-141 KAO: CAT equipment
The HiMAT (Highly Maneuverable Aircraft Technology) subscale research vehicle, seen here during a research flight, was flown by the NASA Dryden Flight Research Center, Edwards, California, from mid 1979 to January 1983. The aircraft demonstrated advanced fighter technologies that have been used in the development of many modern high performance military aircraft.
C-141 composite art of M-17 FAR-IR May
ROCKWELL INTERNATIONAL TECHNICIANS MOUNT SOME OF THE NEARLY 8,000 CERAMIC-COATED TILES THAT REMAIN TO BE INSTALLED ON THE EXTERNAL SURFACES OF THE SPACE SHUTTLE ORBITER COLUMBIA TO COMPLETE THE THERMAL PROTECTION SYSTEM THAT WILL ABSORB THE INTENSE HEAT OF REENTERING THE EARTH'S ATMOSPHERE AFTER A MISSION IN SPACE. TILE INSTALLATION IS DONE ON AN AROUND-THE-CLOCK BASIS IN THE ORBITER PROCESSING FACILITY WHERE COLUMBIA, THE FIRST IN A NEW BREED OF MANNED, REUSABLE SPACECRAFT, IS BEING READIED FOR THE FIRST LAUNCH OF THE SPACE SHUTTLE LATER THIS YEAR.
Once the United States' space program had progressed from Earth's orbit into outerspace, the prospect of building and maintaining a permanent presence in space was realized. To accomplish this feat, NASA launched a temporary workstation, Skylab, to discover the effects of low gravity and weightlessness on the human body, and also to develop tools and equipment that would be needed in the future to build and maintain a more permanent space station. The structures, techniques, and work schedules had to be carefully designed to fit this unique construction site. The components had to be lightweight for transport into orbit, yet durable. The station also had to be made with removable parts for easy servicing and repairs by astronauts. All of the tools necessary for service and repairs had to be designed for easy manipulation by a suited astronaut. Construction methods had to be efficient due to the limited time the astronauts could remain outside their controlled environment. In lieu of all the specific needs for this project, an environment on Earth had to be developed that could simulate a low gravity atmosphere. A Neutral Buoyancy Simulator (NBS) was constructed by NASA Marshall Space Flight Center (MSFC) in 1968. Since then, NASA scientists have used this facility to understand how humans work best in low gravity and also provide information about the different kinds of structures that can be built. As part of this experimentation, the Experimental Assembly of Structures in Extravehicular Activity (EASE) project was developed as a joint effort between MFSC and the Massachusetts Institute of Technology (MIT). The EASE experiment required that crew members assemble small components to form larger components, working from the payload bay of the space shuttle. Pictured is an entire unit that has been constructed and is sitting in the bottom of a mock-up shuttle cargo bay pallet.
KENNEDY SPACE CENTER, FLA. - Assembly of the first Space Shuttle vehicle, scheduled to make its first orbital test flight in March 1981, was completed today with the mating of the Orbiter Columbia to its external tank in the Vehicle Assembly Building's High Bay 3. Columbia, shown here still attached to its hoisting sling, was moved to the VAB on Nov. 24 having completed tests and tile installation in the adjacent Orbiter Processing Facility. The other Shuttle components, the twin solid rocket boosters and the external propellant tank, were stacked on the Mobile Launcher Platform in High Bay 3 in January and November of this year, respectively. The current schedule calls for the rollout of the assembled Space Shuttle to Pad A at Launch Complex 39 shortly after Christmas.
In the late 1970s, NASA, the Marshall Space Flight Center, and its contractors began focusing on designs for Shuttle-tended space platforms capable of extended periods in space and utilizing a variety of temporarily emplaced payloads. As a result, McDornell Douglas studied the Science and Applications Space Platform (SASP). The emphasis was placed on payloads that did not require a crewman's presence during normal operations. Most of the payloads would occupy one or more Spacelab-like pallets. This artist concept depicts the SASP.
Space Shuttle Orbiter 102 Columbia is shown backing out of its manufacturing facililty at Palmdale, CA, the Rockwell international Space Division Plant, enroute to Dryden Flgiht Research Center. This Orbiter will be the first shuttle spacecraft that will carry two astronauts, John Young and Richard Crippen, into earth orbital test flight in late 1979.
Technicians check instrumentation and systems on NASA 808, a PA-30 aircraft, prior to a research flight. The aircraft was used as the testbed in development of control systems for remotely piloted vehicles that were "flown" from the ground. The concept led to highly successful programs such as the HiMAT and the subscale F-15 remotely piloted vehicles. Over the years, NASA 808 has also been used for spin and stall research related to general aviation aircraft and also research to alleviate wake vortices behind large jetliners. This 1980 photograph taken inside a hangar shows technicians measuring moment of inertia.
Sykorsky Bearingless Main Rotor test in 40x80ft w.t.
Space Shuttle Orbiter Enterprise, mated to a 15-story-tall external propellant tank and twin inert solid rocket boosters on top of a Mobile Launcher Platform, is rolled back to the Vehicle Assembly Building from Lauch Complex 39's Pad A July 23 at the completion of nearly three months of fit and function checks at the shuttle launch site as part of the exercise designed to help clear the way for the liftoff of its sister ship Columbia. The massive Crawler Transporter began moving its 11 million pound load the 3.5 miles from pad A to the VAB at 10:23 a.m. and reached the doorway to High Bay 1 at 3:48p.m. following serveral days of fit checks of modified extermiable platforms in the assembly bay, the nonlaunchable shuttle will be destacked. Enterprise will be returned to Rockwell International and stripped of parts for integration into orbiter destined for space, while the external tank and solid booster will be returned to their respective prime contractors and refurbished for use on a later shuttle mission.
DAST cockpit
From left to right; Gilbert A. Haynes holding the NTA Fred C. Downs Special Event Award and Samuel J. Scott with award for their participation in the local Hampton Roads Chapter of the (NTA) National Technical Association. The guidance and counseling of minority youth is one of NTA's prime objectives. Formed in 1925, NTA has 15 chapters comprised of architects,engineers, scientists, and educators. NTA activities are directed toward encouraging and assisting public and private institutions in identifying potential minority technical talent.
KENNEDY SPACE CENTER, FLA. - The first Space Shuttle vehicle destined to fly in space inches out of the Vehicle Asembly Building on its way to Pad A at Complex 39, where it will be launched. The STS-1 vehicle - consisting of America's first reusable spaceship, Columbia, the external propellant tank and twin solid rocket boosters - was assembled on a Mobile Launcher Platform in the Vehicle Assembly Building. A six-million-pound tractor, called the Crawler-Transporter, is used to carry the Space Shuttle from the VAB to the launch pad, about 3.5 miles away.
Mt. St. Helens Volcano - post eruption
Shuttle related interaction with the space telescope.
The 747 Shuttle Carrier Aircraft, carrying the Space Shuttle Orbiter Enterprise piggyback, lifts off from the Shuttle Landing Facility's 15,000-foot-long runway at 11:03, August 10. Enterprise flown to KSC on April 10 for use in checking out assembly, test and launch facilities which will be used for the launch of its sister ship Columbia on the first Space Shuttle flight, will make a five-stop flight to NASA's Dryden Flight Research Center in California.
Mt. St. Helens Volcano - post eruption
DAST in Flight. Last Flight
KENNEDY SPACE CENTER, FLA. - STS-1 stands framed in vegetation lining the superhighay-wide crawlerway linking the Vehicle Assembly Building with the twin pads of Launch Complex 39. The first Space Shuttle assembly emerged from the VAB shortly after 8 a.m. today for the 3.5-mile journey to Complex 39's Pad A. The Shuttle was on the hardstand at Pad A approximately seven and a half hours after rollout began. Launch is scheduled for no eariler than March 1981.
SPACE SHUTTLE ORBITER ENTERPRISE MATED TO AN EXTERNAL FUEL TANK AND TWO SOLID ROCKET BOOSTERS ON TOP OF A MOBIL LAUNCHER PLATFORM, UNDERGOES FIT AND FUNCTION CHECKS AT THE LAUNCH SITE FOR THE FIRST SPACE SHUTTLE AT LAUNCH COMPLEX 39'S PAD A. THE DUMMY SPACE SHUTTLE WAS ASSEMBLED IN THE VEHICLE ASSEMBLY BUILDING AND ROLLED OUT TO THE LAUNCH SITE ON MAY 1 AS PART OF AN EXERCISE TO MAKE CERTAIN SHUTTLE ELEMENTS ARE COMPATIBLE WITH THE SPACEPORT'S ASSEMBLY AND LAUNCH FACILITIES AND GROUND SUPPORT EQUIPMENT, AND HELP CLEAR THE WAY FOR THE LAUNCH OF THE SPACE SHUTTLE ORBITER COLUMBIA.
Mrs. Katherine G. Johnson at Work
KENNEDY SPACE CENTER, FLA. - Prime crew astronauts for the first space shuttle mission, Commander John Young and Pilot Robert Crippen, take a break from their intensive training schedule to pose for pictures in the flight deck of the orbiter Columbia. The Space Shuttle is controlled and most payloads are handled from the flight deck. Looking forward, the ship’s commander is seated on the left and the pilot on the right. Shown are the TV-like displays, and duplicate sets of conventional-looking hand controllers, pedals, levers and switches with which either astronaut can fly the craft alone. The two-man crew are wearing their ejection escape suits which will be worn only during the orbital flight test program and then only during the launch and landing phases of the mission.
Turbo-prop semi-span model test-435 in 14ft w.t. with Ron Smith
SPACE SHUTTLE ORBITER ENTERPRISE STANDS ON KSC'S PAD 39A HIGHLIGHTED AGAINST THE DARKENED FLORIDA SKY DURING TESTING OF THE HIGH-INTENSITY LIGHTING SYSTMES. THE BANKS OF XENON LIGHTS ARE USED DURING LAUCH PREPARATIONS.
S80-36848 (24 July 1980) --- Photo of the Manned Maneuvering Unit (MMU) simulator at the Martin Marietta plant in Denver, Colorado. View of simulator with test subject strapped in to it.
S80-42914 (Dec 1980) --- Astronaut David C. Leestma.
C-141 KAO: CAT experiment - Damage Compressor
CAPE CANAVERAL, Fla. – STS-1, orbiter Columbia, sits at Launch Complex 39A after being rolled out of the VAB. Photo credit: NASA
The Space Shuttle Orbiter Enterprise is lowered to the floor of the transfer aisle in the Vehicle Assembly Building during destacking operations. The Enterprise, mated to an external tank and twin inert solid rocket boosters, formed a nonlaunchable Space Shuttle which was used for fit and fuction checks of assembly, test and launch facilities at the nation's Spaceport. Enterprise will be transported to the Shuttle Landing Facility, mounted piggyback on its 747 Shuttle Carrier Aircraft, and flown to NASA's Dryden Flight Research Center, CA.
KENNEDY SPACE CENTER, FLA. - Shuttle Orbiter Columbia move from OPF and mate to external tank in VAB.
Range : 76 million km. ( 47 million miles) P-22892C This, Voyager 1 image shows Saturn and five of its satellites. Saturn's largest moon, Titan, is clearly seen in the upper right corner. The smaller satellites, Dione & Tethys, are shown in the upper left corner, top and bottom respectively. Two of the innermost satellites, Mimas & Enceladus, appear to the lower right of the planet, with Mimas closest to Satun. The bright object to the left of the rings is not a moon, but an artifact of processing. Voyager 1 will make its closest approach November 12th, 1980, ata distance of 124,200 km. (77,176 mi.). this photo is just one of 17,000 images taken of Saturn, its rings, and its satellites by Voyager 1.
Sykorsky Bearingless Main Rotor test in 40x80ft w.t. (Full-Scale Rotor Test Apparatus)
KENNEDY SPACE CENTER, FLA. - Assembly of the first Space Shuttle vehicle, scheduled to make its first orbital test flight in March 1981, was completed today with the mating of the Orbiter Columbia to its external tank in the Vehicle Assembly Building's High Bay 3. Columbia, shown here still attached to its hoisting sling, was moved to the VAB on Nov. 24 having completed tests and tile installation in the adjacent Orbiter Processing Facility. The other Shuttle components, the twin solid rocket boosters and the external propellant tank, were stacked on the Mobile Launcher Platform in High Bay 3 in January and November of this year, respectively. The current schedule calls for the rollout of the assembled Space Shuttle to Pad A at Launch Complex 39 shortly after Christmas.
One of the key tests in the effort to return the Space Shuttle to flight following the Challenger accident was testing the development Motor-8 (DM-8). The 126-foot long, 1.2-million-pound motor, designated DM-8, underwent a full-duration horizontal test firing for two minutes at the Thiokol test facility in Utah. It was fitted with more than 500 instruments to measure such things as acceleration, pressure, deflection thrust, strain, temperature, and electrical properties.
KENNEDY SPACE CENTER, FLA. - Shuttle Orbiter Columbia erection and mate in the Vehicle Assembly Building (VAB).
SYKORSKY BEARINGLESS MAIN ROTOR TEST IN 40X80FT W.T.
This illustration depicts the design features of the Hubble Space Telescope's (HST's) Support Systems Module (SSM). The SSM is one of the three major elements of the HST and encloses the other two elements, the Optical Telescope Assembly (OTA) and the Scientific Instruments (SI's). The purpose of the HST, the most complex and sensitive optical telescope ever made, is to study the cosmos from a low-Earth orbit. By placing the telescope in space, astronomers are able to collect data that is free of the Earth's atmosphere. The HST detects objects 25 times fainter than the dimmest objects seen from Earth and provides astronomers with an observable universe 250 times larger than visible from ground-based telescopes, perhaps as far away as 14 billion light-years. The HST views galaxies, stars, planets, comets, possibly other solar systems, and even unusual phenomena such as quasars, with 10 times the clarity of ground-based telescopes. The spacecraft is 42.5-feet (13-meters) long and weighs 25,000 pounds (11,600 kilograms). Two communication anternas, two solar array panels that collect energy for the HST, and storage bays for electronic gear are on the outside. The HST was deployed from the Space Shuttle Discovery (STS-31 mission) into Earth orbit in April 1990. The Marshall Space Flight Center had responsibility for design, development, and construction of the HST. The Perkin-Elmer Corporation, in Danbury, Connecticut, developed the optical system and guidance sensors. The Lockheed Missile and Space Company of Sunnyvale, California produced the protective outer shroud and spacecraft systems, and assembled and tested the finished telescope.