
Far side of the Moon.
The 'far side of the Moon' is the
lunar hemisphere that is permanently turned away from the
Earth. The opposite side is known as the
near side of the Moon. The far hemisphere was first photographed by the Soviet
Luna 3 probe in 1959, and was first directly observed by human eyes when the
Apollo 8 mission orbited the Moon in 1968. The rugged terrain is distinguished by a multitude of crater impacts, as well as relatively few
lunar maria. It includes the largest known impact feature in the Solar System: the
South Pole-Aitken basin. The far side has been suggested as a potential location for a large
radio telescope, as it would be shielded from possible radio interference from Earth.
History
Tidal forces between
Earth and the Moon have slowed the moon's rotation so that the same side is always facing the Earth. The other face, which is never visible from the Earth in its entirety, is therefore called the "far side of the Moon". The far side should not be confused with the "dark side" (the hemisphere that is not illuminated by the Sun), as the two are the same only during a
full moon. Both the near and far sides receive (on average) almost equal amounts of light from the Sun.
The two hemispheres have distinctly different appearances, with the near side covered in multiple, large
''maria'' (Latin for 'seas,' since the earliest astronomers thought, wrongly, that these plains were seas of lunar water).
The far side has a battered, densely cratered appearance with few maria. Only 2.5% of the surface of the far side is covered by maria,
[1] compared to 31.2% on the near side. The most likely explanation for this difference is related to a higher concentration of heat-producing elements on the near-side hemisphere, as has been demonstrated by geochemical maps obtained from the
Lunar Prospector gamma-ray spectrometer. While other factors such as surface elevation and crustal thickness could also affect where basalts erupt, these do not explain why the farside
South Pole-Aitken basin (which contains the lowest elevations of the Moon and possesses a thin crust) was not as volcanically active as
Oceanus Procellarum on the near side (for a more detailed discussion, see
Lunar mare).
Exploration
Until the late 1950s little was known about properties of the far side of the Moon.
Librations of the Moon periodically allowed limited glimpses of features that are located near the lunar limb on the far side.
These features, however, were seen from a low angle, hindering useful observation. (It proved difficult to distinguish a crater from a mountain range.) The remaining 82% 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 was not 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.
On
October 7 1959 the
Soviet probe
Luna 3 took the first photographs of the lunar far side, seventeen of them being resolvable ones
[2] covering one-third of the surface invisible from the Earth.
[3] The images were analysed, and the first atlas of the far side of the Moon was published by the
USSR Academy of Sciences on
November 6 1960.
[4][5] It included a catalog of 500 distinguished features of the landscape.
[6] A year later the first globe (1:13 600 000
scale [7]) containing lunar features invisible from the Earth was released in the
USSR, based on images from Luna 3.
[8] On
July 20 1965 another Soviet probe
Zond 3 transmitted 25 pictures of very good quality of the lunar far side,
[9] with much better resolution than those from Luna 3.
In particular, they revealed chains of craters, hundreds of kilometers in length.
In 1967 the second part of the "Atlas of the Far Side of the Moon" was published in
Moscow,
[10][11] based on data from Zond 3, with the catalog now including 4,000 newly discovered features of lunar far side landscape.
In the same year the first "Complete Map of the Moon" (1:5 000 000 scale
) and updated complete globe (1:10 000 000 scale), featuring 95 percent of the lunar surface
were released in the Soviet Union.
[12][13]
As a lot of prominent landscape features of the far side were discovered by
Soviet space probes, Soviet scientists selected names for them. This caused some controversy, and the
International Astronomical Union, leaving many of those names intact, later assumed the role of naming lunar features on this hemisphere.
The far side was first observed directly by
human eyes during the
Apollo 8 mission in 1968.
Astronaut William Anders described the view:
It has been seen by all crew members of the
Apollo 8 and
Apollo 10 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 situated near the center of the far side, and the 3 km-high rim would help to block stray communications from orbiting satellites. Another potential candidate for a radio telescope is the
Saha crater.
[14]
Before deploying radio telescopes to the far side, several problems must be overcome. The fine lunar dust can 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 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.
[15]
Because the near side is partly shielded from the
solar wind by the Earth, the far side
maria are expected to have the highest concentration of
Helium-3 on the surface of the Moon.
[16] 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 impossible premise for the TV program '' 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.
★ "Ideas Die Hard" (1957), a short story by
Isaac Asimov, described an ill-fated trip to the dark side of the Moon. First appearing in ''
Galaxy'' magazine, it was reprinted in ''The Winds of Change and Other Stories'', ISBN 0-586-05743-9.
★ In the anime show ''
Grendizer'', the Vega galactic empire has set up a base on the far side of the Moon from which they launch attacks on Earth.
★
Pink Floyd had a seminal album titled ''
The Dark Side of the Moon'', that, apart from the title and some lines in the songs "
Brain Damage" and "
Eclipse", had nothing to do with the Earth's physical moon. The use of the word
lunatic in the album's lyrics, gains its stem from "luna" for moon, which denotes the traditional link made in
folklore between
madness and the phases of the moon.
★ "The Far Side of the Moon" is the English title of a French-Canadian movie "La Face cachée de la lune"
References
1. The Composition and Geologic Setting of Lunar Far Side Maria, J. J. Gillis, P. D. Spudis, , , Lunar and Planetary Science, 1996
2. Luna 3. NASA
3. Great Soviet Encyclopedia, 3rd. edition, entry on "Луна (спутник Земли)", available online here
4. АТЛАС ОБРАТНОЙ СТОРОНЫ ЛУНЫ, Ч. 1, Moscow: USSR Academy of Sciences, 1960
5. Aeronautics and Astronautics Chronology, 1960. NASA
6. Chronology, 1804-1980, to the 150th anniversary of GAISh - Moscow State University observatory. MSU
7. Moon maps and globes, created with the participation of Lunar and Planetary Research Department of SAI. SAI
8. Saving Globes an article in Sphaera: the Newsletter of the Museum of the History of Science, Oxford
9. Zond 3. NASA
10. АТЛАС ОБРАТНОЙ СТОРОНЫ ЛУНЫ, Ч. 2, Мoscow: Nauka, 1967
11. Observing the Moon Throughout History. Adler Planetarium
12. Works of the Department of lunar and planetary research of GAISh MGU. SAI
13. Moon Maps. MSU
14. Astronomers push for observatory on the moon Richard Stenger
15. Sample Return Mission to the South Pole Aitken Basin, M. B. Duke, B. C. Clark, T. Gamber, P. G. Lucey, G. Ryder, G. J. Taylor, , , Workshop on New Views of the Moon 2: Understanding the Moon Through the Integration of Diverse Datasets, 1999
16. Thar's Gold in Tham Lunar Hills
External links
★
Lunar and Planetary Institute: Exploring the Moon
★
Lunar and Planetary Institute: Lunar Atlases
★
Ralph Aeschliman Planetary Cartography and Graphics: Lunar Maps
★
Northwest Africa 482, only meteorite believed to have originated from the far side of the Moon