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The United States' first manned space flight project was successfully
accomplished in a 4 2/3 year period of dynamic activity which saw more than
2,000,000 people from many major government agencies and much of the aerospace
industry combine their skills, initiative, and experience into a national
effort. In this period, six manned space flights were accomplished as part of a
25-flight program. These manned space flights were accomplished with complete
pilot safety and without change to the basic Mercury concepts. It was shown that
man can function ably as a pilot-engineer-experimenter without undesirable
reactions or deteriorations of normal body functions for periods up to 34 hours
of weightless flight.
Directing this large and fast moving project required the development of a
management structure and operating mode that satisfied the requirement to mold
the many different entities into a workable structure. The management methods
and techniques so developed are discussed. Other facets of the Mercury
experience such as techniques and philosophies developed to insure well-trained
flight and ground crews and correctly prepared space vehicles are discussed.
Also, those technical areas of general application to aerospace activities that
presented obstacles to the accomplishment of the project are briefly discussed.
Emphasis is placed on the need for improved detail design guidelines and
philosophy, complete and appropriate hardware qualification programs, more
rigorous standards, accurate and detailed test procedures, and more responsive
configuration control techniques.
The actual beginning of the effort that resulted in manned space flight
cannot be pinpointed although it is known that the thought has been in the mind
of man throughout recorded history. It was only in the last decade, however,
that technology had developed to the point where man could actually transform
his ideas into hardware to achieve space flight. Specific studies and tests
conducted by government and industry culminating in 1958 indicated the
feasibility of manned space flight. Implementation was initiated to establish a
national manned space-flight project, later named Project Mercury, on October 7,
1958.
The life of Project Mercury was about 4 2/3 years, from the time of its
official go-ahead to the completion of the 34-hour orbital mission of Astronaut
Cooper. During this period, much has been learned about man's capabilities in
the space environment and his capabilities in earthbound activities which
enabled the successful accomplishment of the objectives of the Mercury Project
in this relatively short period. It is the purpose of this paper to review the
more significant facets of the project beginning with the objectives of the
project and the guidelines which were established to govern the activity. As in
any form of human endeavor, there are certain signs which serve as the outward
indication of activity and progress. For the Mercury Project, these signs were
the major full-scale flight tests.
These tests will be reviewed with particular emphasis on schedule, the
individual mission objectives, and the results from each mission. Then, the
organization with which management directed the activities of Project Mercury
will be explained, particularly with respect to those internal interfaces
between major segments of NASA and those external interfaces with contractors
and other governmental departments.
The resources expended during the project will be explained with discussions
on manpower and cost. In addition, the major results of the project will be
discussed as will those areas which presented severe obstacles to technical
progress.
| space
exploration, the investigation of physical conditions in space and
on stars, planets, and their moons through the use of artificial satellites
(spacecraft that orbit the earth), space
probes (spacecraft that pass through the solar system and that may
or may not orbit another celestial body), and spacecraft with human
crews.
Satellites and Probes
Although studies from earth using optical and radio telescopes
had accumulated much data on the nature of celestial bodies, it was not
until after World War II that the development of powerful rockets
made direct space exploration a technological possibility. The first
artificial satellite, Sputnik I, was launched by the USSR (now
Russia) on Oct. 4, 1957, and spurred the dormant U.S. program into
action, leading to an international competition popularly known as the
"space race." Explorer I, the first American satellite,
was launched on Jan. 31, 1958. Although earth-orbiting satellites have
by far accounted for the great majority of launches in the space
program, even more information on the moon, other planets, and the sun
has been acquired by space probes.
Lunar Probes
In the decade following Sputnik I, the United States and the USSR
between them launched about 50 space probes to explore the moon.
The first probes were intended either to pass very close to the moon
(flyby) or to crash into it (hard landing). Later probes made soft
landings with instruments intact and achieved stable orbits around the
moon. Each of these four objectives required increasingly greater rocket
power and more precise maneuvering; successive launches in the Soviet
Luna series were the first to accomplish each objective. Luna 2
made a hard lunar landing in Sept., 1959, and Luna 3 took
pictures of the moon's far side as the probe flew by in Nov., 1959. Luna
9 soft-landed in Feb., 1966, and Luna 10 orbited the moon in
Apr., 1966; both sent back many television pictures to earth. In
addition to the 24 lunar probes in the Luna program, the Soviets also
launched five circumlunar probes in its Zond program.
Early American successes generally lagged behind Soviet accomplishments
by several months but provided more detailed scientific information. The
U.S. program did not bear fruit until 1964, when Rangers 7, 8,
and 9 transmitted thousands of pictures, many taken at altitudes
of less than 1 mi (1.6 km) just before impact and showing craters only a
few feet in diameter. Two years later, the Surveyor series began a
program of soft landings on the moon. Surveyor 1 touched down in
June, 1966; in addition to television cameras, it carried instruments to
measure soil strength and composition. The Surveyor program established
that the moon's surface was solid enough to support a spacecraft
carrying astronauts.
In Aug., 1966, the United States successfully launched the first Lunar
Orbiter, which took pictures of both sides of the moon as well as the
first pictures of the earth from the moon's vicinity. The Orbiter's
primary mission was to locate suitable landing sites for the Apollo
Lunar Module, but in the process it also discovered the lunar mascons,
regions of large concentration of mass on the moon's surface. Between
May, 1966, and Nov., 1968, the United States launched seven Surveyors
and five Lunar Orbiters. Clementine, launched in 1994, engaged in
a systematic mapping of the lunar surface. In 1998, Lunar Prospector
orbited the moon in a low polar orbit investigating possible polar ice
deposits, but a controlled crash near the south pole detected no water.
Interplanetary Probes
While the bulk of space exploration initially was directed at the
earth-moon system, the focus gradually shifted to other members of the
solar system. The U.S. Mariner program studied Venus and Mars, the two
planets closest to the earth; the Soviet Venera series also studied
Venus. From 1962 to 1971, these probes confirmed the high surface
temperature and thick atmosphere of Venus, discovered signs of recent
volcanism and possible water erosion on Mars, and investigated Mercury.
Between 1971 and 1973 the Soviet Union launched six successful probes as
part of its Mars program. Exploration of Mars continued with the U.S.
Viking landings on the Martian surface. Two Viking spacecraft arrived on
Mars in 1976. Their mechanical arms scooped up soil samples for
automated tests that searched for photosynthesis, respiration, and
metabolism by any microorganisms that might be present; one test
suggested at least the possibility of organic activity. The Soviet Phobos
1 and 2 missions were unsuccessful in 1988. The U.S. Magellan
spacecraft succeeded in orbiting Venus in 1990, returning a complete
radar map of the planet's hidden surface. The Japanese probes Sakigake
and Suisei and the European Space Agency's probe Giotto
both rendezvoused with Halley's
comet in 1986, and Giotto also came within 125 mi (200 km) of
the nucleus of the comet Grigg-Skjellerup in 1992. The U.S. probe Ulysses
returned data about the poles of the sun in 1994, and the ESA Solar
and Heliospheric Observatory (SOHO) was put into orbit in
1995. Launched in 1996 to study asteroids and comets, the Near Earth
Asteroid Rendezvous (NEAR) probe made flybys of the asteroids
Mathilde (1997) and Eros (1999) and began orbiting the latter in 2000.
The Mars Pathfinder and Mars Global Surveyor, both of
which reached Mars in 1997, were highly successful, the former in
analyzing the Martian surface and the latter in mapping it. The Mars
Climate Orbiter and Mars Polar Lander, however, were lost
upon their arrival at Mars in 1999, as was Deep Space 2, twin
probes that were to penetrate the Martian surface near the south pole.
These losses set back NASA's Mars exploration program–which includes
six probes originally scheduled to be launched between 2001 and
2005–by at least two years. Japan's Nozomi orbiter, launched in
1998 and originally scheduled to reach Mars in 1999, will arrive four
years later because of a need to conserve fuel.
Space probes have also been aimed at the outer planets, with spectacular
results. One such probe, Pioneer 10, passed through the asteroid
belt in 1973, then became the first object made by human beings to
escape the solar system. In 1974, Pioneer 11 photographed
Jupiter's equatorial latitudes and its moons, and in 1979 it made the
first direct observations of Saturn. Voyagers 1 and 2,
which were launched in 1977, took advantage of a rare alignment of
Jupiter, Saturn, Uranus, and Neptune to explore all four planets.
Passing as close as 3,000 mi (4,800 km) to each planet's surface, the
Voyagers discovered new rings, explored complex magnetic fields, and
returned detailed photographs of the outer planets and their unique
moons. Launched in 1989, the Galileo spacecraft followed a
circuitous route that enabled it to return data about Venus (1990), the
moon (1992), and the asteroids 951 Gaspra (1991) and 243 Ida (1993)
before it orbited Jupiter (1995—99); it also returned data about the
Jupiter's atmosphere and its largest moons (Io, Ganymede, Europa, and
Callisto). The joint U.S.-ESA probe Cassini, launched in 1997,
will explore Saturn, its rings, and some of its moons upon arriving in
2004.
Human Space Exploration
Human spaceflight has progressed from the simple to the complex,
starting with suborbital flights; subsequent highlights included the
launching of a single astronaut in orbit, the launching of several
astronauts in a single capsule, the rendezvous and docking of two
spacecraft, the attainment of lunar orbit, and finally the televised
landing of an astronaut on the moon. The first person in earth orbit was
a Soviet cosmonaut, Yuri Gagarin,
in Vostok 1 on Apr. 12, 1961. The American Mercury program had
its first orbital success in Feb., 1962, when John Glenn
circled the earth three times; a flight of 22 orbits was achieved by
Mercury in May, 1963. In Oct., 1964, three Soviet cosmonauts were
launched in a Voskhod spacecraft. During the second Voskhod flight in
Mar., 1965, a cosmonaut left the capsule to make the first "walk in
space."
The first launch of the Gemini program, carrying two American
astronauts, occurred a few days after the Soviet spacewalk. The United
States made its first spacewalk during Gemini 4, and subsequent
flights established techniques for rendezvous and docking in space. The
first actual docking of two craft in space was achieved in Mar., 1966,
when Gemini 8 docked with a crewless vehicle. In Oct., 1967, two
Soviet Cosmos spacecraft performed the first automatic crewless
rendezvous and docking. Gemini and Voskhod were followed by the American
Apollo and the Soviet Soyuz programs, respectively.
The Early Soyuz Program
Until late 1969 it appeared that the USSR was also working toward
landing cosmonauts on the moon. In Nov., 1968, a Soviet cosmonaut in Soyuz
3 participated in an automated rendezvous and manual approach
sequence with the crewless Soyuz 2. Soyuz 4 and 5
docked in space in Jan., 1969, and two cosmonauts transferred from Soyuz
5 to Soyuz 4; it was the first transfer of crew members in
space from separately launched vehicles. But in July, 1969, the rocket
that was to power the lunar mission exploded, destroying an entire
launch complex, and the USSR abandoned the goal of human lunar
exploration to concentrate on orbital flights. The program suffered a
further setback in June, 1971, when Soyuz 11 accidentally
depressurized during reentry, killing all three cosmonauts. In July,
1975, the United States and the USSR carried out the first
internationally crewed spaceflight, when an Apollo and a Soyuz
spacecraft docked while in earth orbit. Later Soyuz spacecraft have been
used to ferry cosmonauts to and from Salyut and Mir.
Space Stations
After the geophysical exploration of the moon via the Apollo program was
completed, the United States continued human space exploration with Skylab,
an earth-orbiting space station that served as workshop and living
quarters for three astronauts. The main capsule was launched by a
booster; the crews arrived later in an Apollo-type craft that docked to
the main capsule. Skylab had an operational lifetime of eight
months, during which three three-astronaut crews remained in the space
station for periods of about one month, two months, and three months.
The first crew reached Skylab in May, 1972.
Skylab's scientific mission alternated between predominantly
solar astrophysical research and study of the earth's natural resources;
in addition, the crews evaluated their response to prolonged conditions
of weightlessness. The solar observatory contained eight high-resolution
telescopes, each designed to study a different part of the spectrum
(e.g., visible, ultraviolet, X-ray, or infrared light). Particular
attention was given to the study of solar flares (see sun).
The earth applications, which involved remote sensing of natural
resources, relied on visible and infrared light in a technique called
multispectral scanning (see space
science). The data collected helped scientists to forecast crop and
timber yields, locate potentially productive land, detect insect
infestation, map deserts, measure snow and ice cover, locate mineral
deposits, trace marine and wildlife migrations, and detect the dispersal
patterns of air and water pollution. In addition, radar studies yielded
information about the surface roughness and electrical properties of the
sea on a global basis. Skylab fell out of orbit in July, 1979;
despite diligent efforts, several large pieces of debris fell on land.
After that time the only continuing presence of humans in earth orbit
were the Soviet Salyut and Mir space stations, in which
cosmonauts worked for periods ranging to more than 14 months. In
addition to conducting remote sensing and gathering medical data,
cosmonauts used their microgravity environment to produce electronic and
medical artifacts impossible to create on earth. In preparation for the
International Space Station (ISS)–a cooperative program of the United
States, Russia, Japan, Canada, Brazil, and the ESA–astronauts and
cosmonauts from Afghanistan, Austria, Britain, Bulgaria, France,
Germany, Japan, Kazakhstan, Syria, and the United States worked on Mir
alongside their Russian counterparts. Assembly of the ISS began in Dec.,
1998, with the linking of an American and a Russian module (see space
station) Once the ISS was manned in 2000, maintaining Mir in
orbit was no longer necessary and it was made to decay out of orbit in
Mar., 2001.
The Space Shuttle
After the Skylab space station fell out of orbit in 1979, the
United States did not resume sending astronauts into space until 1981,
when the space
shuttle, capable of ferrying people and equipment into orbit and
back to earth, was launched. The shuttle itself is a hypersonic
delta-wing airplane about the size of a DC-9. Takeoff is powered by
three liquid-fuel engines fed from an external tank and two solid-fuel
engines; the last are recovered by parachute. The shuttle itself returns
to earth in a controlled glide, landing either in California or in
Florida.
The shuttle can put a payload of 20 tons (18,000 kg) in earth orbit
below 600 mi (970 km); the payload is then boosted into final orbit by
its own attached rocket. The Galileo probe, designed to
investigate Jupiter's upper atmosphere, was launched from the space
shuttle. Astronauts have also used the shuttle to retrieve and repair
satellites, to experiment with construction techniques needed for a
permanent space station, and to conduct scientific experiments during
extended periods in space.
At first it was hoped that shuttle flights could operate on a monthly
basis, but schedule pressures contributed to the explosion of the Challenger
shuttle in 1986, when cold launch conditions led to the failure of a
rubber O-ring, and the resulting flame ruptured the main fuel tank. The
shuttle program was suspended for three years, while the entire system
was redesigned. A second accident occurred in 2003, when Columbia
was lost during reentry because heat shielding on the left wing failed
to prevent superheated gas from entering the wing; the hot gas
structurally weakened the wing and caused the shuttle to break up. Prior
to the Columbia disaster, the shuttle fleet operated on
approximately a bimonthly schedule.
Bibliography
See T. Wolfe, The Right Stuff (repr. 1983); B. C. Murray, Journey
into Space (repr. 1990); V. Neal, Where Next, Columbus?: The
Future of Space Exploration (1994); J. Harford, Korolev: How One
Man Masterminded the Soviet Drive to Beat America to the Moon
(1997); T. A. Heppenheimer, Countdown: A History of Space Flight
(1997); F. J. Hale, Introduction to Space Flight (1998); R. D.
Launius, Frontiers of Space Exploration (1998). |
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