Eratosthenes (crater): Difference between revisions

Coordinates: 14°28′N 11°19′W / 14.47°N 11.32°W / 14.47; -11.32
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In 1851 Shropshire Astronomer [[Henry Blunt (Chemist)|Henry Blunt]] constructed a model of the moon's surface showing Eratosthenes. The model is based on observations made by Blunt with a reflecting telescope from his home in Shrewsbury and was displayed in the same year at the Great Exhibition, London.
In 1851 Shropshire Astronomer [[Henry Blunt (Chemist)|Henry Blunt]] constructed a model of the moon's surface showing Eratosthenes. The model is based on observations made by Blunt with a reflecting telescope from his home in Shrewsbury and was displayed in the same year at the Great Exhibition, London.


From 1910 to the 1920s, [[William Henry Pickering|William H. Pickering]] noted dark patches in the crater that varied in a regular manner over each lunar day. He put forward the speculative idea that these patches appeared to migrate across the surface, suggestive of "swarms of animal life".<ref name=Pickering_1919/><ref name=Pickering_1924/> The idea received a degree of attention primarily due to Pickering's reputation.
From 1910 to the 1920s, [[William Henry Pickering|William H. Pickering]] noted dark patches in the crater that varied in a regular manner over each lunar day. He put forward the speculative idea that these patches appeared to migrate across the surface, suggestive of "swarms of animal life"<ref name=Pickering_1919/><ref name=Pickering_1924/> which he also referred to as "lunar insects". Pickering believed that the Moon had an atmosphere, and reported seeing climatic variations such as frost and snow, along with vegetation. leading him to refer to the ""gardens of Eratosthenes". The scientific community did not share his enthusiasm for these ideas,<ref name=Westfall_2014/> but they received a degree of attention primarily due to Pickering's reputation.
[[File:Imbrium map.png|thumb|Detail map of Mare Imbrium's features. Eratosthenes is marked "L".]]
[[File:Imbrium map.png|thumb|Detail map of Mare Imbrium's features. Eratosthenes is marked "L".]]


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|url =http://articles.adsabs.harvard.edu/full/1924PA.....32..393P
|url =http://articles.adsabs.harvard.edu/full/1924PA.....32..393P
|bibcode=1924PA.....32..393P
|bibcode=1924PA.....32..393P
}}</ref>
<ref name=Westfall_2014>{{cite book
|last1=Westfall
|first2=John
|last2=Sheehan
|first2=William
|date=2014
|title=Celestial Shadows: Eclipses, Transits, and Occultations
|volume=410
|publisher=Springer
|isbn=9781493915354
|pages=73
}}</ref>
}}</ref>
}}
}}

Revision as of 01:00, 28 August 2023

Eratosthenes
Lunar Reconnaissance Orbiter image
Coordinates14°28′N 11°19′W / 14.47°N 11.32°W / 14.47; -11.32
Diameter59 km
Depth3.6 km
Colongitude12° at sunrise
EponymEratosthenes
Eratosthenes (lower left of center) and surroundings from Apollo 17. NASA image.
Eratosthenes crater. Photo taken from Earth. Author: Georgi Georgiev, Stara Zagora, Bulgaria.

Eratosthenes crater is a relatively deep lunar impact crater that lies on the boundary between the Mare Imbrium and Sinus Aestuum mare regions. It forms the western terminus of the Montes Apenninus mountain range. It is named after ancient Greek astronomer Eratosthenes of Cyrene,[1] who estimated the circumference of the Earth, and the distance from the Earth to the Sun.

Description

The crater has a well-defined circular rim, terraced inner wall, central mountain peaks, an irregular floor, and an outer rampart of ejecta. It lacks a ray system of its own, but is overlain by rays from the prominent crater Copernicus to the south-west.

The Eratosthenian period in the lunar geological timescale is named after this crater, though it does not define the start of this time period.[2] The crater is believed to have been formed about 3.2 billion years ago.

At low Sun-angles, this crater is prominent due to the shadow cast by the rim. When the Sun is directly overhead, however, Eratosthenes visually blends into the surroundings, and it becomes more difficult for an observer to locate it. The rays from Copernicus lie across this area, and their higher albedo serves as a form of camouflage.

In 1851 Shropshire Astronomer Henry Blunt constructed a model of the moon's surface showing Eratosthenes. The model is based on observations made by Blunt with a reflecting telescope from his home in Shrewsbury and was displayed in the same year at the Great Exhibition, London.

From 1910 to the 1920s, William H. Pickering noted dark patches in the crater that varied in a regular manner over each lunar day. He put forward the speculative idea that these patches appeared to migrate across the surface, suggestive of "swarms of animal life"[3][4] which he also referred to as "lunar insects". Pickering believed that the Moon had an atmosphere, and reported seeing climatic variations such as frost and snow, along with vegetation. leading him to refer to the ""gardens of Eratosthenes". The scientific community did not share his enthusiasm for these ideas,[5] but they received a degree of attention primarily due to Pickering's reputation.

Detail map of Mare Imbrium's features. Eratosthenes is marked "L".

Satellite craters

Eratosthenes and its satellite craters

By convention these features are identified on lunar maps by placing the letter on the side of the crater midpoint that is closest to Eratosthenes.

Eratosthenes Coordinates Diameter, km
A 18°20′N 8°20′W / 18.34°N 8.33°W / 18.34; -8.33 (Eratosthenes A) 5.7
B 18°42′N 8°42′W / 18.70°N 8.70°W / 18.70; -8.70 (Eratosthenes B) 5.3
C 16°53′N 12°23′W / 16.89°N 12.39°W / 16.89; -12.39 (Eratosthenes C) 5.2
D 17°26′N 10°54′W / 17.44°N 10.90°W / 17.44; -10.90 (Eratosthenes D) 3.8
E 17°56′N 10°53′W / 17.93°N 10.89°W / 17.93; -10.89 (Eratosthenes E) 3.8
F 17°41′N 9°55′W / 17.69°N 9.91°W / 17.69; -9.91 (Eratosthenes F) 4.0
H 13°19′N 12°15′W / 13.31°N 12.25°W / 13.31; -12.25 (Eratosthenes H) 3.5
K 12°51′N 9°16′W / 12.85°N 9.26°W / 12.85; -9.26 (Eratosthenes K) 4.3
M 14°01′N 13°35′W / 14.02°N 13.59°W / 14.02; -13.59 (Eratosthenes M) 3.5
Z 13°45′N 14°06′W / 13.75°N 14.10°W / 13.75; -14.10 (Eratosthenes Z) 0.6

References

  1. ^ "Eratosthenes". usgs.gov. Gazetteer of Planetary Nomenclature. International Astronomical Union. Retrieved September 21, 2017.
  2. ^ Wilhelms D. (1987). "Chapter 12. Eratosthenian System" (PDF). Geologic History of the Moon. United States Geological Survey Professional Paper 1348. pp. 249–250. Archived from the original (PDF) on 2013-05-14.
  3. ^ Pickering, W. H. (1919). "Eratosthenes I, a study for the amateur". Popular Astronomy. 27: 579–583. Bibcode:1919PA.....27..579P.
  4. ^ Pickering, W. H. (1924). "Eratosthenes". Popular Astronomy. 32 (6): 392–404. Bibcode:1924PA.....32..393P.
  5. ^ Westfall; Sheehan, William (2014). Celestial Shadows: Eclipses, Transits, and Occultations. Vol. 410. Springer. p. 73. ISBN 9781493915354.

Further reading

External links

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