Explorer 1 (1958)
The Explorer Project
was initiated by the U.S. Army Ballistic Missile agency. Its goals
were to examine cosmic rays, temperature, and meteorological impacts in
space. It also had a miniature Geiger counter which discovered belts
of radiation. The next 7 satellites in the Explorer project did the
same. Explorers 8,20,22, and 27 measured the density of electrons in the
Earth's ionosphere.
Explorer (1963-1973)
The Explorer
projects: 18, 21, 28, 33, 34, 35, 41, 43, 47, and 50 were all sent to monitor
the interplanetary environment and were placed as far out as the moon's
orbit. They successfully monitored changes in the solar wind and
the Earth's magnetotail. Explorer 38 and 39 were designed and released
to listen to galactic radio sources(Explorer 38 was interfered with by
Earth's radio waves and so Explorer 39 went out as far as the moon). Explorer
42, 43, and 53 mapped the sky at X-ray and gamma ray wavelengths (Explorer
42 was the first NASA satellite launched from another country [San Marco].
It was launched from a Scout rocket.)
AMPTE (1984)
This project
was a cooperation between NASA, Great Britain, and Germany. Launched
by a Delta rocket, it carried one satellite from each country and was designed
to watch how barium and lithium ions affect the Earth's magnetic field.
The spacecraft observed how quickly the barium atoms were ionized by the
ultraviolet portion of the sun's light.
Giotto (1985)
Headed by the
European Space Agency, it was named after Giotto Di Bondane, a 14th century
painter who painted a picture with a comet, now believed to be Halley's,
that which it was going to examine. Its goal was to use its equipment:
a TV camera, a photopolarimeter, 3 mass spectrometers, dust impact
detectors to examine Halley's comet in space. The satellite successfully
documented the comet, but half its instruments were destroyed.
Luna (1959-1976)
This Soviet project
was designed to travel to the moon and take pictures from it's surface.
This project established many firsts in lunar travel. It was the
first spacecraft to hit the Moon, the first to travel behind and take pictures
of the moons far side, make a soft landing on the moon, and to move an
remote controlled rover on the Moon's surface. Although it missed
it's original purpose, Luna 1 became the first manmade object to orbit
the Sun.
Orbiter (1966-1967)
The 5 Orbiter
satellites the U.S. put into orbit in three month orbitals were intended
to return detailed TV pictures of the entire lunar surface. These
were later used to construe maps used to pick Apollo landing sites.
The television imaging system was developed by the Eastman Kodak company.
The entire project accomplished its goals with excellence in the quality
of pictures and its time frame.
Mariner (1962-1973)
This NASA
project was under the direction of the Jet Propulsion Laboratory(JPL).
Its planetary movement was based on the 'interplanetary billiards' theory
of the 1920s. It was able to visit Earth's planetary neighbors without
extra rocket stages. The mariner project was the first to achieve
planetary "fly-byes" of Venus, Mars and Mercury.
Phobos (1988)
These two Soviet Satellites
were claimed to be the next generation in space exploration. Its
mission was to orbit Mars, closely pass its larger moon, Phobos, and continue
to investigate the planet and solar wind environment. Each of the
crafts returned data about the solar wind, but in both satellites, communication
was lost.
Pioneer (1958-1978) [image
1] [image 2] [image
3] [image 4]
The first 4 Pioneer
missions were NASA's first attempts at sending probes to the moon.
All 4 of the satellites missed their intended targets, but Pioneer4 went
into the solar orbit and returned a great deal of useful organization.
The Pioneer missions had very different goals: Pioneer 5 to 9 were sent
to examine interplanetary environments; 10 and 11 were to sent towards
Jupiter(Saturn was later added to 11's itinerary). The Pioneer project
included the first probe to Jupiter and Saturn, and the first radar maps(of
Venus).
Ranger (1961-1965) [image
1]
NASA's Ranger Project
was designed to crash onto the surface of the moon, taking and relaying
TV pictures before impact. The first were unsuccessful. It
is believed that many of the probes scientific instruments were damaged
in a 1251/4C sterilization. Finally Ranger 7 was successful.
It returned 4,308 Pictures of what is called Mare Cognitum("The sea which
is now known"). Ranger 7 and 8 revealed that the crater Alphonsus
was suitable for the Ranger 9 landing. Overall the Ranger projects
produced a great deal of information on the moon.
Sagikake (1985)
One of Japan's first
space probes, Sagikake("Pioneer") was launched January 7 1985 from Kagoshima
Space Center. Its purpose was to investigate the interaction of the
solar wind and Halley's comet. It discovered that the solar wind
was disturbed by the comet as far away as 7 million km (4.4 million miles).
Suisei (1985)
Japan's second space
probe, Suisei ("Comet") was launched in order to investigate the growth
and decay of Halley's comet's corona and the interaction of the solar wind
and the comet itself. It carried an ultraviolet imaging experiment
to accomplish this. It was launched August 18, 1985. It reached
within 94,000 miles of the comet's nucleus.
Surveyor (1966-1968)
These probes were developed
by NASA's Jet Propulsion Laboratory. All seven craft were built
by Hughes Aircraft. The first satellite landed safely on the surface
of the moon in the Ocean of Storms. The second failed but all
the rest were successful.. They were able to take a 3601/4 panoramic view
of the lunar surface. Surveyor 3 made the first soil sample of the
moon. The Surveyor mission confirmed that a manned mission to the
moon was possible. Surveyor 6 even fired it's soft landing engines
and hopped on the surface to test its strength.
VeGa (1984-1987)
These missions
were aimed at investigating Halley's Comet but also deployed balloons over
Venus(the name is a combination of Venera[Venus] and Gallei[Halley]).
VeGa 1 and 2 were both launched from Baikonur with Proton boosters.
VeGa 1 was launched December 15, 1984 and VeGa 2 was launched on the twenty-third.
In June 1985, VeGa 1 had passed within 25,000 miles of Venus' cloud-tops
and VeGa 2 within 15,600 miles. Both satellites dropped landers with
balloons into the atmosphere. The first malfunctioned when its drill
began too early, but the second returned data for 57 minutes. The
balloons that were dropped contained temperature and pressure receptors,
and cloud composition analyzers in the "gondola," an instrument which hung
bellow the plastic 12' diameter hydrogen balloon. They lasted
for 46 hours sending radio signals back to Earth so they could be tracked.
The main space crafts went on to investigate
Halley's Comet. VeGa 1 made it's trip within 5,562 miles of the nucleus
on March 6, 1986 and VeGa 2 within 5,062 miles on March 9. The crafts
included instruments such as a CCD(Charge Couple Device) to observe the
nucleus, 2 TV cameras and instruments to analyze dust from the comet.
The VeGa Project was an international project that returned ample information
about the atmosphere of Venus and Halley's Comet. It was finally
shut down in 1987.
Venera (1961-1983)
These 16 Soviet
missions were aimed towards Venus and consequently established many firsts.
Venera 4 was the first probe to penetrate the Venusian atmosphere, Venera
8 had the first successful Landing on the surface of Venus,
Venera 9 was the first craft to Orbit the planet, Venera 13 was the first
craft to return color TV pictures of the Venusian surface and soil analysis,
and Venera 16 was the first radar mapping of the planet. The Venera
mission revealed much of the Venusian surface.
Viking (1975) [image
1] [image 2] [image
3]
This NASA
mission was designed to investigate the possibility of any possible life
on Mars. In order that they do not mistake Earth Bacteria for Martian
life, the crafts were sterilized at 112 degrees Celsius. Along with
the TV cameras, the Viking craft were also equipped with a spectrometer
called an Infra-red Thermal Mapper used to measure the temperature profile
of the surface and atmosphere and the Mars Atmosphere Water detector
to search for water vapor in the Martian Atmosphere. The lander carried
11 experiments that would be carried out but the soil analysis of the Martian
soil was deemed inconclusive. The probes were powered by Radioisotope
Thermonuclear Generators. But the results of the Viking tests were
very helpful. The TV pictures show the plain-like surface of the
planet, covered by small volcanic rocks and unmoved sand dunes.
Voyager(1977)
One of the most successful space
explorations ever, the Voyager project was created to use the gravitational
pull of other planets to visit the outer planets. The first project,
because of cutbacks, only visited Jupiter and Saturn. But the second
had the calculations to reach Uranus and Neptune. The craft was built
by the Jet Propulsion Laboratory (JPL).
The craft was powered via a Radioisotope
Thermonuclear Generator. The craft had many different instruments
for an array of experiments: Imaging Science, measured the weather systems
and geological surfaces were examined by TV cameras; an infrared interferometer
spectrometer used a telescope and viewed the surface at different wavelengths
to examine atmospheric competition, thermal dynamics, and structure.
An ultraviolet spectrometer(UVS), was used to observe the upper atmosphere
of the outer planets and the aurora and electrically-charged particles
in their magnetospheres. Photopolarimeter(PPS) was meant to measure
the polarization and brightness of the light from the planets. But
Voyager 1's failed and Voyager 2's were used to examine the rings.
A Planetary Radio Astronomy(PRA) was designed to listen to radio emissions
from the outer planets. A Magnetometer measured the intensity and
direction of magnetic fields that enveloped the spacecraft. Plasma
Particles evaluated how the magnetospheres of the planets and moons interacted
with the solar wind (the machine determines whether particles in a plasma[a
gas made of charged particles that equal in net charge] are moving less
than the speed of light). To study and measure the cosmic rays, which
are shielded from Earth by solar wind, the Voyager had a Cosmic ray telescope.
Although launched second, Voyager
1 reached Jupiter first. After it reached Saturn in 1980 its cameras
were switched off but the particle instruments kept working. Voyager
reached Saturn and flew through the rings gathering much information, but
in the process a malfunction caused the scanning platform to get jammed
and providing only minimal movement for the scanner. After reaching
Neptune in 1985, certain tricks, like sending data back to Earth slower,
were used to make sure we would receive all the data clearly. The
craft reached Neptune and Uranus, nearly 3.2 billion miles away. Both craft
are still traveling in space but will break communications because of distance
in about 2010. They will keep traveling onto distant stars and galaxies.
The craft also includes the Voyager Interstellar
Record, a videodisc containing Earth languages, sounds and music(including
some from Chuck Berry), the idea was sent forth by Carl Sagan, a noted
American astronomer. |