origins of the marshall space flight · pdf filement related to german rocket research. ......
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Marshall’s rocket and space legacy also has roots
in Germany. Among those who joined President
Eisenhower at the dedication of the new Marshall
Center was Dr. Wernher von Braun, the Center’s first
director. Von Braun’s interest in rocketry dated back
to his early years growing up in his native Germany
prior to World War II. Von Braun had studied under
the famous rocket theoretician, Hermann Oberth,
and had joined him in early rocket experiments
conducted under the sponsorship of the German
Society for Space Travel.
Marshall Space Flight Center’s legacy of contribu-
tions to the American space program dates back to
September 8, 1960. On that date, President Dwight
Eisenhower formally dedicated the George C.
Marshall Space Flight Center in Huntsville as a new
field installation of the National Aeronautics and
Space Administration (NASA). Named for the late
General George C. Marshall, the Marshall Center
resulted from the transfer in Huntsville of 4,670 Army
civil service employees and 1,840 acres of Redstone
Arsenal property and facilities worth $100 million.
The original German rocket team shortly after their arrival in 1946 at Fort Bliss, Texas.
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Origins of the Marshall Space Flight Center
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During World War II, von Braun was technical director
at the Peenemünde Rocket Center in Germany. There
he and his growing team of specialists built the
famous V–2 rocket that established the technological
basis for post-war experimentation with even more
powerful rockets. When von Braun and his team
recognized that the war was ending and that Russian
troops would soon occupy Peenemünde, they
decided to evacuate the rocket development site.
Traveling in caravans by any number of means, the
scientists headed south bluffing their way through
German checkpoints, eventually deciding to surren-
der to American forces. As World War II ended, the
United States government manifested interest in the
technical capability of the von Braun team. A group
of American scientists was dispatched to Europe on
August 14, 1945, to collect information and equip-
ment related to German rocket research. As a result,
the components for approximately 100 V–2 ballistic
missiles were recovered and shipped from Germany
to White Sands Proving Grounds in New Mexico. In
late 1945, more than 100 members of the von Braun
team agreed to come to the United States to work
under U.S. Army supervision.
Assigned to Fort Bliss, Texas, the Germans and
Americans rebuilt, tested, and flew the V–2 rockets
previously shipped to the U.S. from Germany. The first
American-assembled V–2 was static fired on March
14, 1946, at White Sands. June 28,1946, marked the
first successful launch of a V–2 rocket fully instru-
mented for upper air research. The rocket attained
a height of 67 miles.
A young Wernher von Braun holding a model of theV-2 rocket.
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As the 1940’s closed, the Army expanded its rocket
program and moved the von Braun team to Hunts-
ville and to World War II arsenal facilities originally
used to produce various chemical compounds and
Huntsville and the Space Program in the 1950s
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Jet Propulsion Laboratory Director Dr. James Pickering; Dr. James van Allen of the StateUniversity of Iowa; and Army Ballistic Missile Agency Technical Director Dr. Wernher vonBraun triumphantly display a model of Explorer I, America’s first satellite, shortly afterthe satellite’s launch on January 31, 1958. Dr. von Braun’s rocket team at the RedstoneArsenal in Huntsville, Alabama, developed the Juno I launch vehicle, which was a modifiedJupiter-C. The Jet Propulsion Laboratory packed and tested the payload, which wasradiation detection equipment designed by Dr. van Allen.
pyrotechnical devices. In Huntsville, the Germans
joined a growing cadre of U.S. rocketry specialists.
Working under von Braun, the combined team built
missiles to counter Soviet Cold War threats. The most
Jet Propulsion Laboratory Director Dr. James Pickering; Dr. James van Allen of the StateUniversity of Iowa; and Army Ballistic Missile Agency Technical Director Dr. Wernher vonBraun triumphantly display a model of Explorer I, America’s first satellite, shortly afterthe satellite’s launch on January 31, 1958. Dr. von Braun’s rocket team at the RedstoneArsenal in Huntsville, Alabama, developed the Juno I launch vehicle, which was a modifiedJupiter-C. The Jet Propulsion Laboratory packed and tested the payload, which wasradiation detection equipment designed by Dr. van Allen.
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famous was officially named “Redstone” on April 8,
1952, in recognition of its development at Redstone
Arsenal in Huntsville. The name of the arsenal, in
turn, referred to the rock and soil in Huntsville.
In early 1958, world attention focused on the
Huntsville rocket team. Earlier in the decade, von
Braun had proposed using a Huntsville rocket to
launch an American satellite to beat the Russians into
space. Instead, Eisenhower favored a Navy program
called Vanguard. Then in October 1957, the Soviets
launched Sputnik, the first manmade object ever to
orbit the Earth. The U.S. countered on December 6
with an effort to launch a Vanguard rocket. Misfor-
tune struck, however, when the rocket exploded in
flames on the launch pad. It was, one newspaper
headline said, time for the Huntsville team to come
through. Von Braun got the go-ahead from Washing-
ton, and on January 31, 1958, his Huntsville team
launched a four stage Jupiter-C rocket from the
Florida launch site. It carried Explorer I, the Nation’s
first Earth-orbiting satellite, and marked the United
States’ initial entry in the space race.
Following Explorer I, American leadership debated
over whether the U.S. space program should be
administered by a military or civilian agency. The
debate resulted in the creation of NASA, a civilian
organization, on October 1, 1958. In turn, President
Eisenhower later signed an executive order indicating
that personnel from the Development Operations
Division of the Army Ballistic Missile Agency in
Huntsville should transfer to NASA, subject to the
approval of Congress. The activation of the Marshall
Center on July 1, 1960, meant that the Army would
continue the growing task of developing and provid-
ing military rockets and missile systems. The Marshall
Center would provide launch vehicles for NASA’s
civilian exploration of outer space.
Von Braun and his fellow Germans had received
American citizenship in the 1950’s and had made
Huntsville their home. The team met the challenge
of launching America’s first satellite into space. As
the new NASA team in Huntsville entered the 1960’s,
they faced even larger challenges, like “Saturn,”
a vehicle eventually selected to launch American
astronauts to the surface of the Moon.
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machine workers from the East Coast, electrical
engineers from the Midwest and promising young
chemists from Georgia Tech and California,” said
U.S. News and World Report.
Residents searched for ways to accommodate the
city’s rapid growth. Hannes Luehrsen, who had been
trained in architecture and city planning in Germany,
drew plans for a major detour around the city’s
original business district. With the school population
growing by 1,200 students a year, the spouses of
scientists and engineers at Redstone Arsenal helped
fill the need for teachers, and in January 1950, the
University of Alabama opened a branch in Huntsville.
Later, von Braun lobbied for a research institute and
a permanent full undergraduate program.
By 1967, Huntsville’s population was over 100,000
and still growing. Federal dollars streamed into
Huntsville. Legend has it that von Braun sent
government photographers outside the gates of
the Marshall Center to take pictures of dilapidated
houses. He then presented the pictures to city
leaders to demonstrate how the city looked when
visitors came to town. At the end of World War II,
Huntsville had about 12 industries and 3,500 homes.
By 1964, the city had more than 40 industries and
30,000 homes.
Huntsville celebrated the launch of Explorer I with
fireworks in the streets. National attention focused
on the city, once devoted almost entirely to growing
cotton. Huntsville got a place on the map and
became known as the “Rocket City.” Von Braun’s
picture appeared on the cover of Time.
The celebration in Huntsville in 1958 marked the
eighth year since the rocket team had moved to
Huntsville. Much had changed even before the launch
of Explorer I. Cotton traders and mule-drawn wagons
that had been so much in evidence in the first half
of the century were gone. When the German team
arrived in 1950, Huntsville’s population was 16,000.
By 1956, it had grown to 48,000, expanding with
rocket engineers and scientists from across the
United States.
There were other changes too. The Germans height-
ened the community’s cultural climate by promoting
and participating in musical and artistic endeavors.
Von Braun led the drive to build an astronomical
observatory and telescope on nearby Monte Sano
Mountain.
By the mid-1950’s, the word “rocket” was plastered
on everything from cafés to upholstery shops. The
character of the population changed as well. The city
“draws top talented physicists from New England,
“Rocket City” Expands
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As work on the Saturn rockets progressed in the
1960’s, von Braun sought ways to preserve public
enthusiasm for space exploration. By the mid-1960’s,
he and others had joined forces in establishing a
permanent site to publicly display hundreds of space
and missile-related exhibits provided by the Marshall
Center and the Army. That facility opened in 1970
and is known today as the U.S. Space and Rocket
Center.
The Huntsville Times announces the successfullaunching of America’s first satellite, Explorer I, bya Huntsville-built Jupiter-C on January 31, 1958.
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America’s growing interest in space exploration
in the late 1950’s led to the desire for launch
vehicles able to lift increasingly larger scientific
payloads. The four stage Jupiter C (sometimes called
Juno I) used to launch Explorer I had minimum
payload lifting capabilities. In fact, Explorer I weighed
slightly less than 31 pounds. Huntsville’s Juno II was
part of America’s effort to increase payload lifting
capabilities.
Among other achievements, a Juno II successfully
launched a Pioneer IV satellite on March 3, 1959,
and an Explorer VII satellite on October 13, 1959.
Pioneer IV was a joint project of the Army Ballistic
Missile Agency in Huntsville and the Jet Propulsion
Laboratory in California. It passed within 37,000
miles of the Moon before going into permanent solar
orbit. Explorer VII, with a total weight of 91.5 pounds,
carried a scientific package for detecting micro-
meteors, measuring the Earth’s radiation balance,
and conducting other experiments.
Responsibility for Juno II passed from the Army to
the Marshall Center when the Center was activated
on July 1, 1960. On November 3, 1960, a Juno II sent
Explorer VIII into a 1,000-mile deep orbit within the
ionosphere. Explorer VIII was significant in Marshall’s
history since the Center was involved in the mission
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Juno Rockets for Space Science
This is the Juno space vehicle, which was used byNASA during the period 1958–61 to launch variousEarth satellites and space probes. Marshall SpaceFlight Center assumed responsibility for the Junoafter the Center was created in 1960.
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in at least three different ways. First, the Center
had responsibility for the Juno stage of the vehicle.
Second, it had responsibility for conducting the
launch from the Launch Operations Directorate at
Cape Canaveral. Finally, Marshall shared responsibil-
ity with Goddard Space Flight Center for designing,
preparing, and testing the satellite.
Other launch vehicles later replaced the Juno II as
the primary launcher for the Explorer satellite series.
However, another Juno II provided by the Marshall
Center was fired on April 27, 1961, and launched
Explorer XI into orbit to conduct a complex gamma-
ray astronomy experiment. The spacecraft was
referred to as the S–15 astronomy satellite and
was developed by the Massachusetts Institute of
Technology.
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Next, the scientists placed a 37-pound chimpanzee
named “Ham” in a Mercury capsule and launched
him on a Redstone. Ham returned in good health
but the Redstone engine had unexpectedly run with
the throttle wide-open, a situation that caused von
Braun to call for an additional unmanned Redstone
launch on March 24, 1961. Finally, von Braun’s
Redstone was ready to launch America’s first
astronaut, Alan Shepard, into space.
Unfortunately, another event stole some of
Redstone’s thunder. On April 12,1961, the Russians
announced that Maj. Yuri Gagarin had successfully
orbited the Earth for 108 minutes in a 5-ton space-
craft. Gagarin became the first human to make a
successful orbital flight through space.
The chance to launch Shepard on a suborbital flight
came within weeks of Gagarin’s flight. On May 5, a
Redstone rocket supplied by the Marshall Center
lifted off at Cape Canaveral, Florida, carrying Shepard
in his Mercury spacecraft, nicknamed “Freedom 7.”
Shepard rose to an altitude of almost 116 miles and
covered a range of more than 300 miles on a
suborbital flight that lasted less than 15 minutes.
After the Russians launched Sputnik and the
Americans launched Explorer I, the space race was
on. But Sputnik and Explorer were only machines in
space. Next the great superpowers rushed to beat
each other in a race to put a human in space.
As a result, NASA asked von Braun’s group in
Huntsville to modify and test an Army Redstone
missile that the space Agency could use to launch
a manned Mercury capsule.
Between April 1959 and July 1960, von Braun’s
engineers in Huntsville ground-tested the Redstone’s
propulsion systems more than 200 times. Unfortu-
nately, their first attempt to launch an unmanned
Redstone was a complete failure.
Already under pressure from newspapers and
politicians reminding them of the progress the
Russians were making, von Braun and his engineers
went to work on the technical problems that had
beset the launch. They successfully launched their
first unmanned Mercury-Redstone on December 19,
1960, and then launched another on January 31,
1961.
Mercury-Redstone
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Von Braun had been conciliatory toward the Russians
following the Gagarin flight. But his tone changed
after Shepard’s flight. He predicted that the Ameri-
cans would go even farther in the space race
“eventually landing a man on the moon.” The people
of Huntsville “will share in these achievements,” he
told The Huntsville Times.
Marshall Space Flight Center Director Dr. Wernhervon Braun addresses a jubilant crowd in front of theMadison County Courthouse celebrating thesuccessful flight of astronaut Alan Shepard, the firstAmerican in space, on May 5, 1961.
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The primary objective of the second Saturn flight
on April 25, 1962, was to gather engineering data
for future Saturn flights. However, the mission also
included “Project Highwater.” This experiment
released nearly 30,000 gallons of ballast water in
the upper atmosphere. Release of this vast quantity
of water in a near-space environment marked the
first purely scientific large-scale experiment con-
cerned with the space environment. The water was
released at an altitude of 65 miles where, within
only 5 seconds, it expanded into a massive ice cloud
4.6 miles in diameter that continued to climb to a
height of 90 miles.
Eight more Saturn I vehicles were flown. Following
another Saturn I launch on September 18, 1964,
the Marshall Center declared the Saturn I opera-
tional, noting that the vehicle had placed 39,000
pounds into orbit.
The eighth Saturn I flight on February 16, 1965,
placed a Pegasus I satellite into orbit. “The Pegasus
satellite will ‘sweep’ space, detecting and reporting
collisions with meteoroids. The information will give
scientists a better indication of the distribution, size
and velocity of such particles near Earth,” wrote one
observer.
Ten months after they provided the Jupiter C rocket
to launch Explorer I, von Braun’s Army team in
Huntsville began developing a high-performance
rocket for advanced space missions. Tentatively
called Juno V and finally designated Saturn, the
rocket work was turned over to NASA in late 1959.
This Saturn I vehicle and its follow-on the Saturn IB
served as test-bed rockets for the larger and more
powerful Saturn V that would eventually carry the first
humans to the Moon. Along the way towards devel-
oping the Saturn V, the Marshall Center also used the
Saturn I for two early scientific efforts. One was called
“Project Highwater.” The second was called “Pe-
gasus.”
The initial firing of two Saturn I first-stage engines
came on March 28, 1960, only a few days after
President Eisenhower officially directed that the NASA
facilities in Huntsville would be known as the George
C. Marshall Space Flight Center. After the Center’s
activation on July 1, the Marshall Center assumed
responsibility for Saturn. On October 27, 1961, the
first Saturn vehicle flew a flawless 215-mile ballistic
trajectory from Cape Canaveral. The 162-foot-tall
rocket weighed 925,000 pounds and employed a
dummy second stage.
The First Saturn Rockets
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The ninth flight of the Saturn I, on May 25, 1965,
successfully relied on both stages built by private
industry and managed by the Marshall Center. That
mission also marked the first night launch of a
Saturn and the launch of a Pegasus II satellite.
The final flight of the Saturn I on July 30, 1965,
climaxed what Marshall officials described as “a
program which started the U.S. on the road to
the Moon with 10 straight successes.”
The Saturn I launch vehicle provided NASA with
significant new payload lifting capabilities. However,
the Saturn IB vehicle, the second member of the
Saturn family, had even more power, enough for
orbital missions with Apollo spacecraft.
The Saturn IB vehicle was a two-stage rocket. The
first stage was called the “S–IB” and was based on
a redesigned first stage for the Saturn I. The second
stage was called the “S–IVB.” It was based on the
third stage of the mightiest Saturn vehicle of all, the
Saturn V. The first Saturn IB vehicle was launched
February 26, 1966. The next four were launched
July 5 and August 25, 1966, and January 22 and
October 11, 1968.
A clustered eight-engine Saturn I roars from the launch pad at KennedySpace Center in Florida. The Saturn I was developed by the MarshallSpace Flight Center.
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Saturn V had the power equal to the energy created
by 85 Hoover Dams.
At the height of the Saturn program, as many as
20,000 contractor companies were involved in
aspects of the program. From 1960 to 1964,
existing test stands at Marshall were remodeled,
and a sizable new test area was developed.
While Kennedy’s challenge to the Nation created
a sense of urgency, quality and safety were never
sacrificed. Components were tested and re-tested
throughout the 1960’s, all leading up to the Apollo
11 lunar landing.
Finally, a short 8 years after Kennedy’s challenge to
the Nation, the work by Marshall Center employees
came to fruition. The Saturn V successfully propelled
the Apollo 11 crew to the Moon’s surface. On July 20,
1969, mission Commander Neil Armstrong sent the
message back to Earth: “Houston, Tranquility Base
here. The Eagle has landed!”
Five successful Moon-landing missions boosted by
Marshall’s Saturn V followed the Apollo 11 mission.
The Apollo program was completed with the flight of
Apollo 17 in December 1972.
When President John F. Kennedy in 1961 called for
the Nation to put Americans on the Moon by the end
of the decade, the Marshall Center was ready to
answer the call. Huntsville had already earned the
title “Rocket City.” But at the time of Kennedy’s
challenge to the Nation, no rocket in the country
could take a craft to the Moon’s surface. Von Braun
answered Kennedy’s challenge by immediately
turning his attention to the Saturn V.
The Saturn V represented a dramatic departure
from early launch vehicles that were powered by
only one engine and built as a single unit. To achieve
the thrust necessary for crewed lunar missions, it
was essential to develop a multi-engine launch
vehicle that used higher performance propellants
and propulsion systems.
The towering Saturn V was the response to that
challenge. The first large vehicle in the U.S. space
program to be conceived and developed for a
specific purpose, the Saturn V was the most powerful
vehicle ever designed. More than 3 million parts,
making up 700,000 components, were contained in a
single Saturn V. When complete, the 363-foot Saturn
V stood 60 feet taller than the Statue of Liberty and
weighed 13 times more. At liftoff, the three-stage
The Saturn V Moon Rocket
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The 363-foot tall Saturn Vwas first launched on
November 9, 1967.A Saturn V was used on
July 16, 1969, to send thefirst human to the lunar
surface on Apollo 11.
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As time drew near for the manned lunar landings,
NASA decided to provide a lunar roving vehicle that
would extend the astronauts’ range of exploration
and their ability to carry equipment and lunar
samples.
The Lunar Roving Vehicle
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Apollo 15 astronautJim Irwin on the surfaceof the Moon with thelunar roving vehicle.A lunar roving vehiclewas used on the lastthree Apollo expeditionsto the Moon. The lunarroving vehicle wasdesigned and developedby Marshall SpaceFlight Center.
By 1969, Marshall was responsible for the design,
development, and testing of the new article. The
vehicle contrasted with the towering Saturn vehicles.
It was a fragile looking, open-space vehicle about
10 feet long with large mesh wheels, antenna
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appendages, tool caddies, and cameras. Powered by
two 36-volt batteries, it had four one-fourth hp drive
motors, one for each wheel. The peculiar vehicle was
collapsible for compact storage until needed, when it
could be unfolded by hand.
Marshall engineers from the Center’s laboratories
contributed substantially to the design and testing
of the navigation and deployment systems. In fact,
the backup manual deployment system developed
by Marshall proved more reliable than the automated
system and became the primary method of deploy-
ment.
The rover was designed to travel in forward or
reverse, negotiate obstacles about a foot high, cross
crevasses about 2 feet wide, and climb or descend
moderate slopes; its speed limit was about 14 km
(9 miles) per hour. To assist in development of the
navigation system, the Center created a lunar surface
simulator, complete with rocks and craters, where
operators could test drive the vehicle. The simulator
also was used during the mission as an aid in
responding to difficulties.
A lunar rover was used on each of the last three
Apollo missions in 1971 and 1972 to permit the
crew to travel several miles from the landing craft.
Outbound, they carried a load of experiments to be
set up on the Moon; on the return trip, they carried
more than 200 pounds of lunar rock and soil
samples. The vehicle performed safely and reliably
on each excursion and enhanced the astronauts’
work efficiency. It handled as well and steered as
easily on the Moon as on Earth.
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Marshall also served as the NASA interface for a
series of Skylab experiments proposed by students
from across the country.
In 1973, NASA launched Skylab into space using a
Saturn V rocket. Unfortunately, a huge panel protect-
ing the orbital workshop from micrometeoroids and
solar radiation ripped off seconds after the launch.
NASA had originally planned to launch its first three-
man crew to Skylab on May 15 using a Saturn IB
rocket. Faced with a crisis, however, NASA put those
plans on hold. Rising temperatures inside the
workshop and a crippled electrical power system
dogged engineers at Marshall and at other centers.
Some Marshall employees stayed at their posts from
dawn Monday through Wednesday looking for
immediate and long-term solutions. Hundreds at the
Center were involved in the relentless 10-day effort
to identify the repair procedures and equipment that
the astronauts eventually carried into space and
used to save Skylab.
Skylab’s first crew went into space on May 25, 1973,
and returned home on June 22. A second crew was
launched on July 28 and splashed down on Septem-
ber 25. Repair procedures were part of both mis-
sions, but attention also focused on the scientific data
that Skylab gathered. For example, the second
Launched on May 14, 1973, Skylab was the first
American space program wholly dedicated to
scientific research, and the Marshall Center played
an extremely important role in this unprecedented
scientific venture.
Skylab’s three different three-man crews spent
up to 84 days in Earth orbit and performed a
variety of more than 100 experiments. The Marshall
Center developed the major Skylab components and
the four Saturn launch vehicles used to launch the
orbital cluster and its three separate crews. Marshall
was also responsible for directing many of the
experiments.
Marshall engineers designed the centerpiece
component for Skylab, the orbital workshop, by
converting a Saturn rocket stage into a habitable
space module containing living quarters and support
systems as well as experiment areas. Marshall
assignments also included the Skylab airlock module,
docking adapter, and Apollo Telescope Mount, the
first manned astronomical observatory designed for
solar research from Earth orbit.
The Center was also responsible for investigations in
materials processing and solar physics, and designed
and built a series of Skylab biomedical experiments.
Skylab
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mission orbited a pair of common spiders, Arabella
and Anita. The experiment was designed to deter-
mine the spiders’ ability to spin a web without the
influence of gravity. It was one of the student experi-
ments coordinated by the Marshall Center for Skylab.
The third manned Skylab crew went into space on
November 16 and splashed down in February 1974
setting a new endurance record and reflecting man’s
ability to live and work in space for extended periods
of time.
This 1973 photograph clearly shows the Skylabworkshop and attached observatory as itorbits high above the Earth.
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nauts trained together in preparation for 2 days of
joint activities on their docked spacecraft, each group
becoming familiar with the other’s spacecraft, flight
procedures, and language.
On July 15, 1975, the Russian Soyuz spacecraft lifted
off from its launch pad at a Soviet launch site. The
spacecraft carried Cosmonauts Alexei Leonov and
Valeriv Kubasov. Seven and one-half hours after the
Soyuz launch, the U.S. Apollo spacecraft was
launched with its crew of Thomas Stafford, Vance
Brand, and Donald “Deke” Slayton. Rendezvous
and docking of the two ships were accomplished
on July 17. The ships remained docked for 2 days,
conducting joint experiments and exchanging national
mementos.
The Saturn IB for the mission was the last Saturn
to be launched. Marshall officials said later that the
successful performance of the Saturn IB for the
mission was another indication of the launch vehicle’s
reliability since the first and second stages of the
vehicle had been built in 1967. Both were taken out
of storage for the mission for continuous preflight
checkouts and monitoring prior to the actual launch.
The Apollo-Soyuz Test Project (ASTP) in 1975 was
the first joint American-Soviet space mission and, as
expected, most of the world focused on its political
dimensions. The Marshall Center role, however,
focused on engineering and science. For example,
Marshall provided the Saturn IB launch vehicle for
the Apollo portion of the mission. In addition,
Marshall scientists gathered data from the results
of experiments and demonstrations conducted in
the unique environment of space.
The principal objective of the Apollo-Soyuz Test
Project was to test compatible rendezvous and
docking systems that were being developed for future
United States and Soviet manned spacecraft and
stations. The project was carried out under an
agreement signed in 1972 by President Richard
Nixon and Chairman Aleksey Kosygin.
Five years of technical cooperation among engineers
in the United States and the Soviet Union led to the
development of the international docking module,
and agreements on mission operations, flight control,
means for life support, communications, tracking,
safety and crew procedures. Astronauts and cosmo-
The Apollo-Soyuz Test Project
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The science team for the Apollo-Soyuz Test Project
included principal investigators from Marshall as well
as scientists from industry and education who were
under contract to the Center. A Marshall-managed
electric furnace for the ASTP performed perfectly
after resolution of an early cool-down problem. Seven
materials processing experiments were conducted in
the furnace.
This artist’s rendition shows the Apollo and Soyuzspacecrafts about to rendezvous in high Earth orbitas part of the Apollo/Soyuz Test Project in 1975.This was the first international meeting in spacebetween two countries.
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The value of space-based observatories was rein-
forced by the success of the High-Energy Astronomy
Observatory (HEAO) series of spacecraft: HEAO–1,
HEAO–2, and HEAO–3. Launched in 1977, 1978,
and 1979 respectively, the three unmanned space-
craft were designed to study high-energy radiation in
the universe such as x-rays, gamma rays, and cosmic
rays. The Marshall Center played a major role in the
project development and management, while
Marshall’s laboratories were heavily engaged in the
technical and scientific aspects—an undertaking that
included the construction of the Marshall X-Ray
Calibration Facility—the largest and most sophisti-
cated facility of its type in the world.
In 1976 Marshall launched the Laser Geodynamics
Satellite (LAGEOS), which the center had conceived
and manufactured in Huntsville. Basically a mirror in
space, the 900-pound, 2-foot diameter satellite was
designed to precisely reflect laser beams from
ground stations for extremely accurate ranging
measurements. This allowed the satellite to measure
movements of Earth’s crust. Movements of less than
an inch could be detected by timing the laser beam’s
3,700-mile round trip. LAGEOS was designed to
serve as a ranging system for improved understand-
ing of earthquakes, continental drift, and other
geophysical phenomena.
Increased scientific results from space served as the
theme for the Marshall Center during the late 1970’s
as it moved from Saturn and Skylab to Space Shuttle.
Earlier Marshall missions like Project Highwater
and Pegasus had demonstrated that space was
a laboratory for doing science. In addition, the
Apollo 14 mission in 1971 had included three
Marshall-developed experiments investigating the
potential for materials processing in space. That
same year, closer to Earth, the Marshall Center had
launched the 36-inch Stratoscope II astronomical
telescope from Redstone Arsenal. Carried by a
special balloon, the telescope photographed scientific
targets from an operating altitude of 82,800 feet.
Again, in the last half of the l970’s, the scientists
at the Marshall Center used this early science as
a foundation to branch into more expanded space
science missions. Space would provide Marshall
scientists with a global view of our planet for atmo-
spheric observations, a microgravity environment
for experiments in life sciences and materials sci-
ences, and an opportunity to study the radiation
and vacuum of space. Some of the missions were
significant on their own merit. Others would serve
as forerunners to more ambitious payloads in the
1980’s and 1990’s.
Space Science in the 1970s
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Also in 1976 Marshall launched the Gravitational
Redshift Probe. The purpose of the 125-pound
satellite was to test the principle of equivalence in
Einstein’s general theory of relativity. According to
theory, but never demonstrated, a clock will appear
to run faster in a weaker gravitational field, at a
greater distance from Earth. Scientists from Marshall
and the Smithsonian Astrophysical Observatory
jointly devised an ingenious experiment to test the
theory. A very stable atomic clock was launched
through Earth’s gravitational field to a peak altitude
of 6,200 miles, and its reading during the free flight
was compared with that of an identical reference
clock on the ground. The experiment confirmed the
theory. Marshall had overall management responsibil-
ity for the construction, integration, and systems
testing of the satellite.
From 1975 through 1983, Marshall conducted one
of its most successful efforts involving small pay-
loads, the Space Processing Applications Rockets
project. Marshall accomplished 10 suborbital flights,
which altogether carried several dozen small materi-
als processing experiments. Intriguing results were
achieved in the 5-minute periods of near weightless-
ness as the rocket passed through its apex.
Shown is an artist’s concept of the three High-Energy Astronomy Observatory satellites launchedin the late 1970s. The HEAO satellites weredeveloped by the Marshall Space Flight Center.
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engine. Three liquid-fueled main engines produce
nearly 1 million pounds of thrust—equivalent to
the energy of 23 Hoover Dams. Unlike the Saturn
engines, the Space Shuttle Main Engines were
designed to be throttled over a range from
65 percent to 109 percent of their rated power.
Thus the engine could be adjusted to meet different
mission needs. From the outset, it was recognized
that the engines required the greatest technological
advances of any element in the Shuttle program.
The greatest problem was to develop the combustion
devices and complex turbomachinery—the pumps,
turbines, seals, and bearings—that could contain
and deliver propellants to the engines at pressures
several times greater than in the Saturn engines.
Assembly of the first engine, Space Shuttle Main
Engine 0001, was completed in May of 1975. This
first engine, known as the integrated subsystem
test-bed engine, was used in the first ignition test
in June 1975.
The first engine firing at 100-percent power level was
conducted early in 1977 and was followed by other
tests, not all of which were successful. Problems were
discovered in the high-pressure oxidizer turbopump
during tests in March and September, but by the end
of the year the anomalies appeared to have been
resolved. Extensive engine testing continued to focus
The Space Shuttle represented an entirely new
generation of space vehicle: the world’s first reusable
spacecraft. Unlike earlier expendable rockets, the
Shuttle was designed to be launched over and over
again, and would serve as a system for ferrying
payloads and personnel to and from Earth orbit.
The Marshall Center was involved in preliminary
studies on the Space Shuttle as early as 1970,
2 years before President Nixon endorsed plans
for the new space vehicle on January 5, 1972. The
Space Shuttle would “change the nature of what
man could be in space,” then NASA Administrator
James Fletcher said.
Crucially involved with the Space Shuttle program
virtually from its inception, Marshall played a leading
role in the design, development, testing, and fabrica-
tion of many major Shuttle propulsion components.
Marshall was assigned responsibility for developing
the Shuttle orbiter’s high-performance main en-
gines—the most complex rocket engines ever built.
Marshall was also responsible for developing the
Shuttle’s massive External Tank and the Solid Rocket
Motors and boosters.
The Space Shuttle Main Engine is considered by many
to be the world’s most sophisticated reusable rocket
Space Shuttle
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The Space Shuttle Enterprise travels slowly past themain headquarters building at Marshall SpaceFlight Center in March 1978. The Enterprise wasscheduled to undergo vibration testing in Marshall’sDynamic Test Stand.
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attention on certain components. The first flight
engines were installed in orbiter Columbia in
August 1980.
The External Tank provides liquid hydrogen and liquid
oxygen to the main engines during the first 8 1/2
minutes of Shuttle flight. To develop the tank,
engineers had to overcome a number of technical
challenges. At 154 feet long and more than 27 feet
in diameter, the External Tank is the largest compo-
nent of the Space Shuttle and the structural back-
bone of the entire Shuttle system. By the end of
1975, fixtures were nearing completion at Marshall’s
Michoud Assembly near New Orleans for manufactur-
ing the External Tanks. Several of the fixtures at the
assembly site were more than half the length of a
football field and several stories high. 1977 was one
of the busiest years in the history of developing the
External Tank. Fabrication of the first flight External
Tank started in July. The first flight tank was delivered
to Kennedy Space Center in July 1979.
The Shuttle’s Solid Rocket Motors and boosters
are the largest ever built and the first designed
for refurbishment and reuse. Standing nearly
150 feet high, the twin boosters provide the majority
of thrust for the first 2 minutes of flight— about
5.8 million pounds. That’s equivalent to 44 million
horsepower, or the combined power of 400,000
subcompact cars. The major design drivers for the
Solid Rocket Motors were high thrust and reuse. The
desired thrust was achieved by using state-of-the-art
solid propellant and by using a long cylindrical motor
with a specific core design that allows the propellant
to burn in a carefully controlled manner. The test plan
included modifications to an existing Saturn test
stand to accommodate structural testing of the Solid
Rocket Motors and boosters. Testing began in 1977
at Marshall and other facilities in the United States.
Thrust vector control system testing was completed
at Marshall. Parachute recovery testing was con-
ducted in California.
1978 was perhaps the busiest year for Marshall’s
Shuttle test program. Throngs of NASA employees
and local citizens turned out to greet the arrival of
the Space Shuttle orbiter prototype Enterprise at the
Marshall Center. The orbiter was test-mated with the
External Tank and Solid Rocket Boosters to undergo
a series of vibration/stress tests in Marshall’s
Dynamic Test Stand.
The excitement surrounding the first Space Shuttle
launch drew the biggest tourist crowd to Cape
Canaveral since the launch of Apollo 11. The crowd
had to wait, however, because a computer problem
delayed Columbia’s launch for 2 days.
Columbia began its voyage with a flawless launch
at 7 a.m. (EST) on April 12, 1981, with Commander
John W. Young and Pilot Robert L. Crippen guiding the
vehicle into orbit. The historic flight was concluded
2 days later when Columbia landed at Edwards Air
Force Base, California.
In a period of less than 5 years after the first Space
Shuttle flight there had been 24 launches and 24
successful missions. Then on January 28, 1986, at
73 seconds into the flight of the 25th mission, orbiter
Challenger broke up under severe aerodynamic
loads. The flames from a leaking right-hand Solid
Rocket Motor caused a severe rupture of the
External Tank, destroying it. The crew and the vehicle
were lost.
The months that followed brought unparalleled
changes in NASA’s institutional management and in
its technical operations. On March 24, 1986, NASA
directed the Marshall Center to form a Solid Rocket
Motor redesign team to re-qualify the motor of the
Space Shuttle’s Solid Rocket Booster. In addition to
Marshall personnel, the team included personnel
from other NASA Centers, industry, and academia.
The President directed NASA to implement the re-
commendations of the Presidential Commission on
the Space Shuttle Challenger Accident. As part of
satisfying those recommendations, NASA developed
a plan to provide a redesigned Solid Rocket Motor.
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Marshall Space Flight Center propulsion elementslift each Space Shuttle mission into space. Theelements include the Space Shuttle Main Engines,the External Tank, and the Solid Rocket Boosters.
In mid-August 1986 the redesign team presented
a design for the Space Shuttle booster that, among
other improvements, would include tighter fitting
joints, which incorporated a so-called “capture
feature” designed to increase safety and perfor-
mance. The new design would eliminate the weak-
nesses that led to the Challenger accident and
incorporate a number of other improvements.
Laboratory, component, and subscale tests would
follow as well as simulator tests, using full-size, flight-
type segments in order to verify the joint design
under flight loads, pressure, and temperature. Full-
scale tests would be used to verify analytical models,
determine hardware assembly characteristics, identify
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joint deflection characteristics, and obtain additional
technical data concerning the redesigned hardware.
After a nearly error-free countdown, Discovery and
the STS–26 crew lifted off from pad 39B on Septem-
ber 29, 1988, at the Kennedy Space Center marking
the first Space Shuttle flight in 32 months.
Marshall’s Shuttle responsibilities did not end with
the development of the operational propulsion
elements. Instead, the Center has continued ongoing
technology advancements to improve the Shuttle
propulsion system at reduced costs. In particular,
Marshall played a key role in the upgrading of the
Space Shuttle Main Engines, which were successfully
test-fired in 1988 using a modified Space Shuttle
Main Engine in Marshall’s Technology Test-Bed,
actually a reconfigured Saturn V first stage test
stand. Improvements also included the development
of silicon nitride (ceramic) bearings for the Space
Shuttle Main Engine. The Center also developed a
new liquid oxygen pump using the latest technology
of investment casting (versus welded components).
Space Shuttle mission STS–89 in January 1998
marked the first flight of redesigned Space Shuttle
Main Engines designed to increase the reliability and
safety of Shuttle flights.
In 1994, the Center embarked on development of
a new super lightweight Space Shuttle External Tank.
The tank made its premier as part of the STS–91
mission in 1998. The new tank featured aluminum
lithium—a lighter stronger material than the alloy
used to manufacture previous External Tanks. The
new tank was essential for launching Space Station
components designed to be assembled in a more
demanding orbit than previously planned. The new
design resulted in a payload weight savings in excess
of 7,000 pounds. Structural and modal testing for the
tank was completed at Marshall. The Center also
developed weld schedules and materials character-
izations for the new tank. All of the work on the new
tank was achieved successfully on a tight schedule
of about 31/2 years.
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European Space Agency (ESA). This ultimately led to
an agreement between NASA and ESA under which
ESA assumed responsibility for funding, developing,
and building Spacelab. Under the arrangement,
Marshall did the feasibility and preliminary design
work during the Sortie studies, and ESA did the
engineering design and hardware development
based on Marshall requirements. Marshall, however,
retained responsibility for technical and program-
matic monitoring of Spacelab development activities
in Europe, which involved 50 manufacturing firms in
10 European countries.
In addition to its program management responsibili-
ties, Marshall was assigned responsibility for building
related Spacelab flight components, including an
optical window for scientific observations, and
development of a pressurized transfer tunnel for
passage of crew and equipment between the orbiter
cabin and the laboratory module.
Marshall also had responsibility for Spacelab’s
command and data management subsystem and
its high data rate multiplexer and high data rate
recorder. In addition, a software development facility
was established to develop and verify programs
for the Spacelab experiment components. Other
As Space Shuttle development began at Marshall in
the 1970’s, planners at the Center were studying
ways to use the proposed new vehicle’s capabilities
for scientific research. The ninth flight of the Shuttle
carried a multiconfiguration spaceborne scientific
laboratory called Spacelab into orbit. Early studies
at the Marshall Center had called for development
of a versatile, reusable, laboratory facility. This facility
would fit inside the payload bay of the Shuttle orbiter
and provide scientists with workbench space, power,
computer support, and racks and storage for a
scientist’s own experiment equipment.
In 1970, the Marshall Center requested proposals
from industry for the preliminary design of a research
and applications module as a way to provide versatile
laboratory facilities for Earth-orbital research and
applications work. In 1971, the Marshall Center
began in-house studies on a laboratory called the
Sortie Can, later renamed the Sortie Lab. The Sortie
concept for Spacelab included a combination of
habitable modules in which scientists could conduct
investigations, and unpressurized pallets for instru-
ments requiring direct exposure to space.
In 1972, NASA began negotiations with the European
Space Research Organization, the forerunner to the
Space-bound Payloads, for the 1980s and 1990s
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responsibilities ranged from the development of
ground support equipment to sophisticated scientific
instruments.
Spacelab also required engineers and other special-
ists at Marshall to perform systems analyses, design
and develop integration hardware, oversee assembly
and checkout, plan the flight timeline, conduct
simulation and training exercises, and provide real-
time support for the missions. Marshall’s payload
crew training complex became a training site for
Spacelab mission specialists from the astronaut
corps and payload specialists from the scientific
community. Prior to the establishment of a new
Spacelab Mission Operations Control Center facility
at Marshall, Marshall mission managers monitored,
controlled, and directed experiments aboard
Spacelab from a Payload Operations Control
Center at the Johnson Space Center.
Early Spacelab Missions
The primary purpose of the first Spacelab mission,
launched on November 28, 1983, was to demon-
strate the scientific capability of the laboratory and
check the thousands of structural, mechanical, and
electronic parts making up the laboratory. During the
10-day mission, the science crew conducted more
than 70 separate investigations in life sciences,
Payload Specialist Dr. Ulf Merbold installs a sample into the Materials Science Double Rack during theSpacelab 1 mission launched on November 28, 1983. Spacelab was the first flight for payload specialists,who were career scientists from outside the astronaut corps. Marshall Space Flight Center was responsiblefor Spacelab development and control.
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atmospheric physics, Earth observations, astronomy,
solar physics, space plasma physics, and materials
science and technology. Two additional Spacelab
missions were flown in 1985. The primary purpose
of the mission launched April 29, 1985, was to
conduct materials science experiments in a stable
low-gravity environment and to conduct research in
life sciences, fluid mechanics, atmospheric science,
and astronomy. The mission was also used to
evaluate two crystal growth furnaces, a life support
and housing facility for small animals, and two types
of apparatus for the study of fluids. Another 7-day
Spacelab mission, launched on July 29, 1985, served
as a laboratory and observatory for investigations in
solar physics, atmospheric physics, plasma physics,
high-energy astrophysics, infrared astronomy,
technology research, and life sciences. In addition
to Spacelab missions 1, 2, and 3, Spacelab hardware
and systems flew on the Spacelab D1 mission, and
several partial payload missions were launched in
the 1983–1985 time period.
Spacelab and Astrophysics
NASA launched Astro–1 on December 2, 1990.
The astrophysics mission aboard Columbia (STS–35)
represented the first Spacelab mission controlled
from NASA’s new Spacelab Mission Operations at
Marshall. It was also the first Spacelab dedicated to
a single scientific discipline. In fact, four of the seven
astronauts on board were astronomers. Managed
by Marshall, Astro–1 telescopes examined the
ultraviolet and x-ray emissions from stars and
galaxies. Specific targets included Supernova 1987a,
the nearby supergiant star Betelgeuse, and others.
In all, 135 deep space targets were examined during
the 394 observations.
Five years after Astro–1, NASA launched STS–67
carrying the Astro–2 mission, mounted on a
Spacelab pallet in the Shuttle cargo bay. Devoted
to astronomy, the mission was designed to observe
energetic objects in space in the ultraviolet portion
of the electromagnetic spectrum.
Spacelab and Atmospheric Science
Planet Earth was the subject of three Spacelab
missions in 1992, 1993, and 1994 as part of the
Atmospheric Laboratory for Applications and Science
(ATLAS) program. All three missions were mounted
on a Spacelab pallet mounted in the Shuttle cargo
bay. ATLAS–1 was launched in March 1992 aboard
Atlantis (STS–45). The Marshall-managed instrument
package was designed to take a detailed scientific
“snapshot” of Earth’s atmosphere. This international
collaboration between the U.S., France, Germany,
Belgium, the U.K., Switzerland, the Netherlands and
Japan involved 12 instruments designed to provide
investigations in four fields—atmospheric science,
solar science, space plasma physics, and ultraviolet
astronomy. The second ATLAS mission was launched
aboard Discovery in April 1993 and was designed
to take measurements of Earth’s atmosphere to
compare with readings from satellites and other
ATLAS flights. Scientists were particularly interested
in collecting data on the relationship between the
Sun’s energy output and Earth’s middle atmosphere
and how these factors affect the Earth’s ozone layer.
ATLAS–3 was launched on Atlantis (STS–66) in
November 1994, once again to provide scientists
with new insights into how human activities are
changing the Earth’s environment.
Spacelab and Microgravity
The 1990’s marked a decade of Marshall-managed
microgravity related Spacelab missions. For example,
in September 1992, Japan’s National Space Develop-
ment Agency shared joint sponsorship with NASA in
the American-Japanese Spacelab-J mission. That
series of microgravity investigations included
24 materials science experiments and 19 life
science experiments.
Multiple Spacelab missions were also flown as part
of the International Microgravity (IML), United States
Microgravity Laboratory (USML), and United States
Microgavity Payload (USMP) series. On IML–1 in
January 1992, astronauts conducted life sciences
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and microgravity processing experiments developed
by scientists from NASA, the European Space Agency,
the Canadian Space Agency, the French National
Center for Space Studies, the German Space Agency
and the National Space Development Agency
of Japan. In all more than 220 scientists from
14 countries participated in the investigations.
On IML–2 in July 1994, Shuttle astronauts divided
into two teams and worked around the clock to
perform more than 80 experiments aboard Spacelab.
Using furnaces and facilities aboard the Spacelab
module, the investigators produced a variety of
material structures from crystals, metal alloys, and
other substances. They also studied fluid processes
not readily observable on the ground due to the
influence of Earth’s gravity.
USML–1, launched in the summer of 1992, included
experiments in crystal growth, fluid dynamics, and
combustion science. USML–2 in the fall of 1995
focused on microgravity research into fluid flows—
investigations with direct applications on Earth for
the manufacture of high-tech crystals, metals, alloys,
and ceramics.
USMP missions flew in October 1992, March 1995,
February 1996 and November 1997. These missions
advanced American expertise in low-gravity research.
In addition, some low-gravity experiments requiring
direct exposure to space were controlled remotely
by ground-based scientists during the mission.
Spacelab and Preparations for the
International Space Station
The Life and Microgravity Spacelab mission aboard
Columbia in 1996 focused on research intended to
set the stage for the forthcoming International Space
Station. In July 1997, after an abbreviated mission
in April, NASA launched the Microgravity Science
Laboratory with the focus on experiments inside
the Spacelab module and in the Shuttle’s middeck
area. The mission focused on new ways to conduct
experiments in space and on opportunities to
develop procedures that might eventually be used
on board the International Space Station.
Other Marshall Payloads
America’s Space Shuttle transportation system was
designed to serve as a “space truck”—a reliable
and reusable means for ferrying satellites, space
probes, scientific experiments, supplies, and humans
to and from Earth orbit.
Marshall-provided payloads have often occupied the
Shuttle’s cargo bays. Many of those Marshall-
managed experiments have taken place in the cargo
bay or in the Shuttle middeck. As part of the second
flight of the Columbia (STS–2) mission in November
1981, the orbiter carried the Induced Environment
Contamination Monitor, the first major Marshall-
managed Shuttle payload. The payload was designed
to measure the environment in and around the cargo
bay. STS–2 also carried another Marshall project, the
Nighttime/Daytime Optical Survey of Lightning. The
project was intended to provide atmospheric re-
searchers with valuable insights into lightning and
thunderstorms as observed from Earth orbit.
Columbia’s third flight in March 1982 marked the first
flight of the Monodisperse Latex Reactor materials
processing experiments. Developed by scientists from
Lehigh University and the Marshall Center, the
experiment produced extremely uniform latex
spheres that became the first commercial products
manufactured in space and made available to the
commercial market as laboratory calibration.
Columbia flew its fourth flight in the summer of 1982
and featured NASA’s first joint Shuttle endeavor with
industry. The Continuous Flow Electrophoresis System
(CFES) was conducted as a joint endeavor arrange-
ment pioneered and managed by the Marshall Center,
NASA, and private enterprise. Orbital tests of the
CFES (developed by McDonnell Douglas) involved the
separation of biological materials such as blood cells
and enzymes.
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The Materials Experiment Assembly flight hardware
was carried aboard Challenger on STS–7. The project
represented one of the first cooperative international
research projects to be conducted aboard a Space
Shuttle. The experiments included the “Vapor Growth
of Alloy-Type Semiconductor Crystals,” “Liquid Phase
Miscibility Gap Materials,” and “Containerless
Processing of Glass Forming Melts.”
Orbiter Discovery was the focal point for several
experiments in April 1985 leading to important
insights toward new medical treatments. The investi-
gations included the Protein Crystal Growth Experi-
ment designed to produce large uniform crystals for
pharmaceutical development. The mission also
included the Phase Partitioning Experiment for
separating biological materials.
The summer of 1984 marked the first time the
Marshall Center had overall management responsibil-
ity for a major Shuttle payload: the Solar Array Flight
Experiment. Deployed from the orbiter’s cargo bay,
the 102-foot long array was designed to convert the
Sun’s energy into electricity to study a new source
of additional electrical power for future Space Shuttle
missions.
In late 1985 Space Shuttle mission 61–B focused on
a pair of space walks by two Atlantis astronauts who
demonstrated advanced orbital construction tech-
niques in the spacecraft’s cargo bay. One technique
was called the Experimental Assembly of Structures
EVA (extravehicular activity). The other was called
the Assembly Concept for Construction of Erectable
Space Structures.
The summer of 1992 featured the first Tethered
Satellite System (TSS–1) mission. This was a joint
NASA/Italian Space Agency effort on STS–46. This
“satellite on a string” experiment was designed to
study the electrodynamics of a tether system in the
electrically charged portion of Earth’s atmosphere
as a potential source of spacecraft power. During TSS
deployment, however, the satellite reached a maxi-
mum distance of only 840 feet from the orbiter rather
than the planned 12.5 miles because of a jammed
tether line. Four years later, NASA and the Italian
Space Agency re-flew the Tethered Satellite System
aboard Columbia on STS–75. This time the tether
abruptly snapped just short of full deployment with
the satellite 12.8 miles from the orbiter. Although the
satellite could not be retrieved and broke up as it
re-entered the Earth’s atmosphere, considerable
amounts of useful information were gained from
the experiment despite the mishap.
Payload Boosters
The Space Shuttle operates in low-Earth orbit. Some
payloads, however, are intended for higher orbits,
while others are propelled out of Earth’s gravitational
influence altogether in order to embark on interplan-
etary voyages. In 1977, Marshall assumed responsi-
bility for overseeing the development of several new
propulsion elements needed to give certain Shuttle
payloads the necessary post-deployment boost. One
of these elements was the Inertial Upper Stage, (IUS)
a U.S. Air Force-developed rocket. Acting as NASA’s
management and coordination Center on the project,
Marshall provided the Agency’s design and opera-
tional requirements to the Air Force and participated
in the development of two IUS configurations for
NASA. Marshall also provided substantial input into
the design and development of Orbital Science
Corporation’s Transfer Orbit Stage (TOS), intended to
broaden the variety of payloads that could be placed
into orbit from the Shuttle.
In late 1986, NASA announced that it had selected
the IUS to carry probes to Jupiter, Venus and the Sun.
NASA also announced that the Marshall Center would
manage the IUS and the payload-to-IUS integration
for the planetary missions. NASA selected the upper
stage, built by Boeing Aerospace under Air Force
contract, for three planetary missions—Galileo,
Magellan, and Ulysses. These missions would be the
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first to employ an IUS to carry payloads to other
bodies in the solar system. On May 4, 1989, the
Space Shuttle Atlantis crew successfully deployed
the Magellan spacecraft for its rendezvous with
Venus using the IUS stage during the first day of the
STS–30 mission. On October 18, 1989, the STS–34
crew aboard Atlantis used the Marshall-managed IUS
to boost the Galileo spacecraft toward a rendezvous
with Jupiter. Approximately 1 year later, on October 6,
1990, the STS–41 crew used an IUS to send the
Ulysses probe on its 5-year journey to explore the
Polar Regions of the Sun. By 1995, the IUS had also
been used to launch more than a half dozen Tracking
and Data Relay Satellites.
In September 1992, the Mars Observer Spacecraft
was launched aboard a Titan III rocket. Marshall/
Orbital Science Corporation’s TOS rocket booster
then injected the spacecraft into a Mars-bound
journey for an 11-month journey to the Red Planet.
Unfortunately, contact with the spacecraft was
abruptly broken approximately 1 year later during
a critical Mars insertion maneuver meaning that the
spacecraft was irretrievably lost. In September 1993,
the crew of Discovery deployed the Advanced
Communications Technology Satellite. Shortly
thereafter, the satellite was boosted to geosynchro-
nous orbit by an attached Transfer Orbit Stage. This
marked the first time a TOS had flown aboard a
Space Shuttle.
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Company of Sunnyvale, California, was selected to
produce the protective outer shroud and the space-
craft systems for the telescope, as well as to
assemble and test the finished product.
Beyond assigning project contracts, Marshall
managed hardware and assembly preparations.
The Center also worked to define the project’s
science and engineering requirements. Marshall
crew systems experts developed the tools, worksta-
tions, and procedures which would be needed for
orbital servicing of the telescope, and conducted
numerous tests of orbital maintenance and repair
techniques using Marshall’s Neutral Buoyancy
Simulator. Marshall’s technical resources were also
tapped for everything from the telescope’s structural
engineering to its fine guidance sensors.
Later, Marshall Center’s involvement continued as the
facility’s personnel played key roles in tests of the
observatory on the ground and on the launch pad—
the latter monitored from Marshall’s Huntsville
Operations Support Center. The Marshall Center also
managed the activation and orbital verification of the
telescope and science instruments from Goddard
Space Flight Center during Hubble’s first several
months in orbit.
Long before mankind had the ability to go into
space, astronomers dreamed of placing a telescope
above Earth’s obscuring atmosphere. In 1923, the
German scientist Hermann Oberth proposed an
observatory in space. Oberth’s work inspired
Wernher von Braun’s interest in space travel.
Scientific instruments installed on early rockets,
balloons, and satellites in the late 1940’s through
the early 1960’s produced enough exciting scientific
revelations to hint at how much remained to be
discovered.
In 1962, just 4 years after NASA was established,
a National Academy of Sciences study group recom-
mended the development of a large space telescope
as a long-range goal of the fledgling space program.
Similar groups repeated the recommendation in
1965 and 1969.
NASA assigned responsibility for design, develop-
ment, and construction of the large space telescope
to the Marshall Center. Marshall selected two primary
contractors to build the Hubble Space Telescope.
Perkin-Elmer Corporation in Danbury, Connecticut,
was chosen to develop the optical system and
guidance sensors. Lockheed Missiles and Space
Hubble Space Telescope
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This artist’s concept showsthe open end of NASA’sHubble Space Telescopeas it orbits the Earth.The more than 12-tonunmanned telescope wasdesigned to see deeper intospace than ever before.Marshall Space FlightCenter has respon-sibilityfor the Hubble SpaceTelescope project.
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Construction and assembly of the space telescope
was a painstaking process that spanned almost a
decade. The precision-ground mirror was completed
in 1981, and the optical assembly was delivered for
integration into the satellite in 1984. The science
instruments were delivered for testing at NASA in
1983. Assembly of the entire spacecraft was com-
pleted in 1985.
Launch of the Hubble Space Telescope was originally
scheduled for 1986. It was delayed during the Space
Shuttle redesign that followed the Challenger acci-
dent. Engineers used the interim period to subject
the telescope to intensive testing and evaluation,
ensuring the greatest possible reliability.
The telescope was shipped from Lockheed in
California to the Kennedy Space Center in Florida
in October 1989. There, it was launched aboard
the STS–31 mission of the Space Shuttle Discovery
on April 24, 1990.
The Hubble Space Telescope, with a resolving power
calculated to be 10 times better than any telescope
on Earth, was poised to open a new era in as-
tronomy. Within a few months, however, a flaw was
discovered in Hubble’s main mirror that significantly
reduced the telescope’s ability to focus.
The focusing defect was due to spherical aberration,
an optical distortion caused by an incorrectly shaped
mirror. The mirror was too flat near the edge by
about 1/50th the width of a human hair. Instead of
being focused into a sharp point, light collected by
the mirror was spread over a larger area in a fuzzy
halo. Images of objects such as stars, planets and
galaxies were blurred. However, on relatively bright
objects, Hubble’s cameras were still able to provide
images far superior to any telescope on the ground.
The mirror itself couldn’t be fixed or changed; so
the challenge facing NASA was to develop corrective
optics for Hubble’s instruments, much like eyeglasses
or contact lenses correct human sight.
On December 2, 1993, the STS–61 crew launched
on Space Shuttle Endeavour for an 11-day mission
with a record five spacewalks planned. The astro-
nauts endured long hours of challenging spacewalks
to install instruments containing the corrective optics
and replaced the telescope’s solar arrays, gyro-
scopes, and other electronic components. The crew
completed everything it set out to do and the mission
was declared a success. After 5 weeks of engineering
checkout, optical alignment and instrument calibra-
tion, the confirmation of success came as the first
images were received on the ground from the space
telescope.
In February 1997, STS–82 astronauts on board
Discovery conducted a second Hubble servicing
mission during a 10-day flight. The objective of the
mission was to significantly upgrade the scientific
capabilities of the Hubble Space Telescope with the
installation of two state-of-the-art instruments. The
astronauts also performed routine maintenance and
installed several makeshift insulating blankets to
protect the observatory’s delicate instruments from
temperature extremes.
Space Shuttle servicing mission (STS–103) in
December 1999 restored NASA’s premier optical
space observatory to full capability beefed-up with
new electronics and critically needed replacement
gyroscopes.
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In the late 1960’s, some of America’s nuclear bomb
detection satellites unexpectedly discovered intermit-
tent bursts of gamma rays—high-energy particles
of light associated with nuclear reactions. However,
these gamma rays weren’t coming from nuclear
Burst and Transient Source Experiment
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Scientists at the MarshallCenter are studying datafrom the Burst andTransient SourceExperiment (BATSE).BATSE has alreadyyielded new information
about the origin of high-energy gamma-ray bursts in
the universe.
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bomb tests on Earth. Instead, they seemed to be
originating from unknown points in deep space.
In order to better investigate the source of these
mysterious gamma-ray bursts, NASA launched the
Compton Gamma-Ray Observatory (GRO). The
unmanned orbiting observatory was deployed from
the cargo bay of the Shuttle orbiter Atlantis (STS–37)
in April 1991. Weighing in around 17 tons, GRO was
the largest science satellite every carried by a
Shuttle, filling half of Atlantis’ cargo bay.
One of the four main astronomical instruments
aboard GRO was the Burst and Transient Source
Experiment (BATSE), built in-house at Marshall in the
mid-1980’s. Operated by the BATSE team in Hunts-
ville, BATSE has already yielded new information
about the origin of high-energy gamma-ray bursts
in the universe.
A robotic telescope managed to take the first-ever
optical images of a gamma-ray burst as it was
exploding on Saturday, January 23, 1999, guided
by a BATSE location in the sky.
BATSE’s discoveries have shown that gamma-ray
bursts do not originate in our own galaxy as was
previously assumed, but emanate instead from the
most distant parts of the observable universe,
indicating the occurrence of violent cosmic events
on a nearly unimaginable scale.
BATSE has also discovered several black hole and
neutron star binary systems, and other strange
celestial objects, which emit bursts of gamma rays.
BATSE findings and the other GRO instruments are
now putting together a picture of our universe more
incredible than anyone had ever previously guessed.
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Chandra
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The Chandra team not only produced and polished
the mirrors, but also created the systems to put them
together. The team also had to align all the compo-
nents to within miniscule tolerances, assemble them
into a spacecraft that could survive the rigors of
launch and space, then test them and validate their
performance.
In many instances, the Chandra team had to come
up with new processes for things that had never been
done before. They developed, built and validated a
measurement system that was used to make sure
the cylindrical mirrors were ground correctly and
polished to the right shape. The eight mirrors are
the largest of their kind—the biggest is 4 feet in
diameter and 3 feet long. The mirror group weighs
more than 1 ton.
The team created and executed a system to carefully
assemble the mirrors into a total package that could
survive the rigors of a rocket ride, weightlessness,
and the temperature extremes of space. The space-
craft is made of graphite epoxy to meet stringent
weight requirements, and yet Chandra is the largest
and heaviest payload ever deployed from the Space
Shuttle. Fully fueled, Chandra weighed 12,930
pounds. With the Inertial Upper Stage set of
boosters added to the craft, the assembly totaled
In July 1999, NASA launched Chandra, the world’s
most powerful x-ray telescope—packed with the
strength and accuracy to read a newspaper from
one-half a mile away or see the letters of a stop sign
from 12 miles. A month later Chandra, a member of
NASA’s family of Great Observatories, released its
spectacular first celestial images.
The journey from Chandra’s program inception to
initial image was a challenging one. Along the way,
the Marshall-managed program focused on precision
engineering and attention to detail.
Launched by the Space Shuttle, the observatory
travels one-third of the way to the Moon during its
orbit around the Earth every 64 hours. At its highest
point, Chandra’s highly elliptical, or egg-shaped, orbit
is 200 times higher than that of its visible-light-
gathering sister, the Hubble Space Telescope.
With its combination of large mirror area, accurate
alignment, and efficient x-ray detectors, Chandra has
10 times greater resolution and is 50 to 100 times
more sensitive than any previous x-ray telescope.
Chandra’s mirrors are the smoothest ever created. If
the surface of the state of Colorado were as relatively
smooth, Pike’s Peak would be less than 1-inch tall.
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50,162 pounds and measured 45.3 feet long by
64 feet wide with its solar arrays deployed.
On the other end of the size spectrum,
microtechnology was used in manufacturing pro-
cesses to make components for Chandra’s imaging
systems. Spectrographic transmission gratings,
used to precisely determine the energies of incoming
x-rays, had never been built before. The gratings
include tiny gold bars that are closer together than
a wavelength of visible light. It would take hundreds
of the bars to equal the thickness of a sheet of paper.
Plastic membranes, thin as a soap bubble, support
the bars.
While all of these incredibly small and large items
were being designed and built, the team also had
to make sure that they all came together to form
the very best overall system. The spacecraft had
to be precise and reliable. Also, the ground control
system and its operating staff had to be able to
efficiently and safely operate Chandra for 5 years
or more. The team tested, tested and re-tested the
spacecraft and ground system together to make sure
they were compatible. On the optics system testing
they made sure that they had at least two ways to
crosscheck all results. In some instances the team
had even more checks.
Calibrating and validating the telescope’s scientific
operation proved to be another challenge. Unlike
optical astronomy, where there are established, well-
known targets in the universe that can be used for
calibration purposes, there aren’t any for x-ray
images. A new world-class X-Ray Calibration Facility
was built at the Marshall Center to precisely calibrate
Chandra’s x-ray optics. The facility also provided
opportunities for additional crosschecks of the total
optical system and for an independent check of
Chandra’s optical performance.
From x-rays entering the optics to the quality of the
images produced by the science instruments, the
testing verified the exceptional accuracy of Chandra’s
optics. Chandra is so finely tuned it can detect objects
separated by one-half arc second. That is like
identifying two dimes side-by-side from 2 miles away.
This is the Chandra X-ray Observatory, NASA’snewest space telescope, which will provide uniqueand crucial new information about the structureand evolution of our universe. Marshall SpaceFlight Center manages the Chandra program.
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Marshall Milestones ●○
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used as the primary test stand for the development
of the F–I engine, the largest liquid rocket engine
ever developed. The F–I generated 1.5 million
pounds of thrust.
Neutral Buoyancy Simulator
The Neutral Buoyancy Simulator was designed to
provide a simulated weightless environment needed
to perform engineering tests in preparation for space
missions. The extravehicular activity protocols for the
Skylab rescue and Apollo Telescope Mount film
retrieval were developed in the facility.
The Saturn V Dynamic Test Stand
The Saturn V Dynamic Test Stand was used in
1966–67 for ground vibration testing of the Saturn V
launch vehicle and the Apollo spacecraft. Completion
of this program was the final step prior to the launch
of Apollo 11—the first manned lunar landing
mission. In 1972–73 the stand was used for tests
involving the Skylab space station, and in 1978–79
for ground vibration testing of the complete Space
Shuttle vehicle.
Saturn V Display
The Saturn V on display at the U.S. Space and Rocket
Center is the actual test rocket that was used in
dynamic testing of the Saturn facilities at Marshall.
The NASA Marshall Space Flight Center announced
on January 22, 1986, that the U.S. Department of the
Interior’s National Park Service had designated four
Marshall Center facilities as National Historic Land-
marks. On July 15, 1987, a fifth designation was
announced.
The first four facilities are the Redstone Test Stand,
Propulsion and Structural Test Facility, Saturn V
Dynamic Test Stand, and Neutral Buoyancy Simulator.
The Saturn V on display at the U.S. Space and Rocket
Center represents the fifth designation.
Historic Redstone Test Stand
The Redstone Test Stand was used during the 1950’s
in early development of the Redstone missile propul-
sion system. This was the test stand where the
modified Redstone missile that launched the first
American into space, Alan Shepard, was static tested
as the last step before the flight occurred.
Propulsion and Structural Test Facility
The Propulsion and Structural Test Facility, developed
in support of Jupiter missile development, was
modified and used for testing on the first clustered
engine stage in the American space program, the
S–IB stage of the Saturn I launch vehicle. It was also
National Historic Landmarks
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The stages of the rocket were used to check out all
the Saturn facilities at Huntsville. Although the rocket
was not intended to be flown, it was a working vehicle
that prepared the way for the Apollo expeditions to
the Moon. Officials from the Department of the
Interior referred to the vehicle as “a unique engi-
neering masterpiece that formed the key link in the
chain that enabled Americans to travel to the Moon.
The success of the Saturn V made possible the
success of the American space program.” Marshall
delivered the Saturn V at the U.S. Space and Rocket
Center in 1969 after all three stages were taken from
the Center’s Dynamic Test Stand.
The Historic Redstone TestStand was the site wherethe rockets were tested forthe Mercury-Redstonevehicle that boostedAmerica’s first astronaut,Alan B. Shepard, on asuborbital flight in 1961.
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But America wanted to get to the Moon before the
end of the 1960’s, so von Braun led the Marshall
team as they developed the massive rockets that
helped the Nation achieve this goal. Even as the
United States raced to the Moon, Marshall engi-
neers—inspired by von Braun’s ideas—continued
to study space stations, including concepts using
refurbished rocket stages. This led to a precursor
of today’s International Space Station: Skylab, a
two-level workshop made from a converted Saturn
rocket stage.
Building on their Skylab experience, Marshall engi-
neers and scientists continued space station studies
in the 1970’s and 80’s. Their designs were used to
help create the International Space Station. Today,
the Marshall Center’s facilities and technical expertise
are being used to support fabrication and testing of
Space Station components.
The Boeing Company, the prime Space Station
contractor, built Unity, the first U.S.-built component,
and the U.S. Laboratory modules in the same
Marshall Center building where decades ago others
assembled the Saturn V rocket. In addition to Boeing,
Long before his appointment as the first director
of the Marshall Center in 1960, Wernher von Braun
wrote in Collier’s magazine about his dreams for a
space station. “Development of the space station is
as inevitable as the rising of the Sun. Man has
already poked his nose into space and he is not likely
to pull it back.” Von Braun’s plans for a large space
station were published in a book the same year.
As the Space Station—a permanent, orbiting
research facility—has evolved over the last
40 years, hundreds of Marshall employees and many
Huntsville businesses have contributed to its success.
It began with von Braun’s space station ideas,
inspired by fiction writers and scientists who had
envisioned permanent outposts in space since the
turn of the century.
In the classic 1952 Collier’s article, von Braun wrote
of a majestic 250-foot-wide wheel that would orbit
1,075 miles above Earth and rotate to provide
artificial gravity, similar to the station visualized in the
movie, 2001, A Space Odyssey. “From this platform,
a trip to the Moon itself will be just a step, as scien-
tists reckon distance in space,” von Braun wrote.
Space Station
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more than 30 Alabama businesses have contributed
to the Space Station effort, providing millions of
dollars of services and equipment. In late 1998, the
Space Shuttle Endeavour carried Unity into orbit to
begin Space Station assembly.
During the last 40 years, scientists have learned not
only that humans can live in microgravity, but also
that microgravity is itself a key area of scientific
activity with benefits in the form of improved products
and processes back on Earth. Marshall, NASA’s lead
center for Microgravity Science, is fostering the
development of many International Space Station
investigations. When the Station becomes opera-
tional, it will offer scientists the first opportunity to
do experiments over extended periods in this unique
environment.
This space station concept was designed and drawnby Dr. Wernher von Braun in 1952 for an articleabout space travel in Collier’s magazine.
The Marshall Center’s proven expertise with
Spacelab—the reusable laboratory flown inside the
Space Shuttle from 1981 to 1998—is being tapped
to build Space Station experiment hardware and plan
microgravity investigations. Marshall developed a
multiple-user rack facility, which was tested aboard
Spacelab and will be used for experiments inside the
Space Station. In addition, Marshall is managing the
development of special pallets that will be used for
experiments mounted on the outside of Space
Station.
One idea has not changed since von Braun’s dream
long ago: the goal of establishing a permanent
presence in space. As von Braun wrote in his Collier’s
article more than 45 years ago, “If we do it (build a
space station), we can not only preserve the peace
but we can take a long step toward uniting mankind.”
The International Space Station is the result of 16
nations joining together on the largest, peacetime,
multinational program ever attempted. In his 1969
blueprint for the future of the space program, von
Braun wrote, “Exploration of space is the challenge
of our day. If we continue to put our faith in it and
pursue it, it will reward us handsomely.”
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