- This article concerns the far side of the Moon. For other uses see Far side (disambiguation).
The Far side of the Moon is the lunar hemisphere
that is permanently turned away from the Earth. This face is
not visible because the rotation of the moon about its axis is
synchronized with its orbital period. This lock-step
synchronization was achieved by the tidal forces
between the Earth and the Moon.
The two hemispheres have a distinctly different appearance, with
the near side covered in multiple, large maria.
The far side has a battered, densely-cratered appearance with
few mares. Only 2.5% of the surface of the far side is covered
by maria, compared to 31.2% on the near side. The most likely
explanation for this difference is that the crust of the Moon is
40 km thicker on the far side. Thus it was more difficult for
molten materials to penetrate to the surface.
The far side was sometimes referred to as the "Dark Side", due to
the lack of human knowledge concerning that hemisphere. The word
"Dark" in a cultural context was meant to express a lack of information, rather than the actual lighting conditions.
Exploration
Until the far side of the Moon was photographed by the Soviet
probe Luna 3 in 1959, little was known about its properties.
Librations of the Moon periodically allowed limited glimpses of
features that are located near the lunar limb on the far side.
But these features were seen from a low angle, hindering useful
observation. (It proved difficult to distinguish a crater from a
mountain range.) The remaining 41% of the surface on the far side
remained unknown, and its properties were subject to much speculation.
An example of a far side feature that can be viewed through libration
is the Mare Orientale, which is a prominent impact basin spanning
almost 1,000 kilometers. Yet this wasn't even named as a feature until 1906, by Julius Franz in Der Mond. The true nature of the basin was discovered in the 1960s when rectified images were projected onto a globe. It was photographed in fine detail by Lunar Orbiter 4 in 1967.
As the far side was first viewed by Soviet space probes, the Russians selected many of the names for the prominent features. This action provoked some controversy, and so the International Astronomical Union later assumed the role of naming lunar features on this hemisphere. However many of the names selected by the Soviets are still recognized.
"The backside looks like a sand pile my kids have played in for some time. It's all beat up, no definition, just a lot of bumps and holes." —Astronaut William Anders, describing the view during the Apollo 8 mission.
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The far side was first observed directly by human eyes during the
Apollo 8 mission in 1968. It has been seen by all crew members
of the Apollo 11 through Apollo 17 missions since that time,
and photographed by multiple lunar probes. Spacecraft passing behind
the Moon were out of direct radio communication with the Earth, and
had to wait until the orbit allowed transmission. During the Apollo
missions, the main engine of the Service Module was fired when the
vessel was behind the Moon, producing some tense moments in
Mission Control before the craft
reappeared.
Potential
Because the far side of the Moon is shielded from radio transmissions
from the Earth, it is considered a good location for placing
radio telescopes for use by Astronomers. Small, bowl-shaped
craters provide a natural formation for a stationary telescope
similar to Arecibo in Puerto Rico. For much larger-scale
telescopes, the 100-kilometer diameter
crater Daedalus is sitated near the center of
the far side, and the 3-km-high rim would help to block stray
communications from orbiting satellites. Other potential candidates
for a radio telescope include the Saha crater and
the South Pole-Aitken Basin.
Before deploying radio telescopes to the far side, several problems
must be overcome. The fine lunar dust can serve to contaminate
equipment, vehicles, and space suits. The conducting materials used
for the radio dishes must also be carefully shielded against the
effects of solar flares. Finally the area about the telescopes
must be protected against contamination by other radio sources.
The L2 Lagrange point of the Earth-Moon
system is located about 62,800 km above the far side. This has also
been proposed as the location of a future radio telescope, performing
a Lissajous ("Halo") orbit about the Lagrangian
point.
One of the NASA missions to the Moon under study would send a
sample-return lander to the South Pole-Aitken basin, the location
of a major impact event that created a formation nearly 2,400
kilometers across. The size of this impact has created a deep
penetration into the lunar surface, and a sample returned from
this site could be analyzed for information concerning the interior
of the Moon.
Because the near side is partly shielded from the solar wind by the Earth, the far side lunar mares are expected to have the highest concentration of Helium-3 on the surface of the Moon. This isotope is relatively rare on the Earth, but has good potential for use as a fuel in fusion reactors. Proponents of lunar settlement have cited presence of this material as a reason for development of a Moon base.
Fictional References
- The novel "Space " by James Michener tells the fictional story of an Apollo 18 mission to the far side of the Moon. The novel was the source for a 1985 TV mini-series of the same name.
- The scientifically-questionable premise for the TV program "Space: 1999" was the explosion of a nuclear waste dump on the far side of the Moon. This propelled the Moon out of Earth's orbit and deep into space.
- Pink Floyd had a seminal album titled Dark Side Of The Moon.
External links
Last updated: 05-09-2005 11:21:56