Heraclitus (crater)

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Heraclitus
Coordinates 49°12′S6°12′E / 49.2°S 6.2°E / -49.2; 6.2 Coordinates: 49°12′S6°12′E / 49.2°S 6.2°E / -49.2; 6.2
Diameter 90 km
Depth 3.8 km
Colongitude 355° at sunrise
Eponym Heraclitus

Heraclitus is a complex lunar impact crater that lies in the rugged southern highlands of the Moon. The crater Licetus forms the northern end of the formation. Just to the east is Cuvier, and due south is Lilius. Just to the west of Heraclitus is the small satellite crater Heraclitus K, to the south of which is a pair of larger overlapping craters, Lilius E and Lilius D. [1]

Lunar craters craters on Earths moon

Lunar craters are impact craters on Earth's Moon. The Moon's surface has many craters, almost all of which were formed by impacts.

Impact crater Circular depression on a solid astronomical body formed by a hypervelocity impact of a smaller object

An impact crater is an approximately circular depression in the surface of a planet, moon, or other solid body in the Solar System or elsewhere, formed by the hypervelocity impact of a smaller body. In contrast to volcanic craters, which result from explosion or internal collapse, impact craters typically have raised rims and floors that are lower in elevation than the surrounding terrain. Impact craters range from small, simple, bowl-shaped depressions to large, complex, multi-ringed impact basins. Meteor Crater is a well-known example of a small impact crater on Earth.

Moon Earths natural satellite

The Moon is an astronomical body that orbits planet Earth and is Earth's only permanent natural satellite. It is the fifth-largest natural satellite in the Solar System, and the largest among planetary satellites relative to the size of the planet that it orbits. The Moon is after Jupiter's satellite Io the second-densest satellite in the Solar System among those whose densities are known.

The entire formation is heavily worn, with features smoothed down by a long history of impacts. Heraclitus is a complex formation composed of three sections divided by a triple-armed interior ridge. Of the three sections, the most eroded and irregular is at the eastern end where the outer rim forms a low ridge that joins to Cuvier. [2]

The crater Heraclitus with Licetus on its northern rim Heraclitus Crater.jpg
The crater Heraclitus with Licetus on its northern rim

The circular southwest end is the most intact section, forming the circular satellite crater Heraclitus D, which is attached to the other two sections along the northeast rim. There are a pair of ghost-crater rims on the floor, and a low ridge in the southwest. [2] The crater is 90 kilometers in diameter and 3.8 kilometers deep. It may be from the Pre-Imbrian period, which lasted from 4.55 to 3.85 billion years ago. [1]

Palimpsest manuscript page thats been used multiple times

In textual studies, a palimpsest is a manuscript page, either from a scroll or a book, from which the text has been scraped or washed off so that the page can be reused for another document. Pergamene was made of lamb, calf, or goat kid skin and was expensive and not readily available, so in the interest of economy a pergamene often was re-used by scraping the previous writing. In colloquial usage, the term palimpsest is also used in architecture, archaeology, and geomorphology to denote an object made or worked upon for one purpose and later reused for another, for example a monumental brass the reverse blank side of which has been re-engraved.

Lunar geologic timescale

The lunar geological timescale divides the history of Earth's Moon into five generally recognized periods: the Copernican, Eratosthenian, Imbrian, Nectarian, and Pre-Nectarian. The boundaries of this time scale are related to large impact events that have modified the lunar surface, changes in crater formation through time, and the size-frequency distribution of craters superposed on geological units. The absolute ages for these periods have been constrained by radiometric dating of samples obtained from the lunar surface. However, there is still much debate concerning the ages of certain key events, because correlating lunar regolith samples with geological units on the Moon is difficult, and most lunar radiometric ages have been highly affected by an intense history of bombardment.

It is named after the 6th-century BC Greek philosopher Heraclitus. [1]

Greece republic in Southeast Europe

Greece, officially the Hellenic Republic, self-identified and historically known as Hellas, is a country located in Southern and Southeast Europe, with a population of approximately 11 million as of 2016. Athens is the nation's capital and largest city, followed by Thessaloniki.

Heraclitus pre-Socratic Greek philosopher

Heraclitus of Ephesus (; Greek: Ἡράκλειτος ὁ Ἐφέσιος, translit. Hērákleitos ho Ephésios; was a pre-Socratic Greek philosopher, and a native of the city of Ephesus, then part of the Persian Empire. He was of distinguished parentage. Little is known about his early life and education, but he regarded himself as self-taught and a pioneer of wisdom. From the lonely life he led, and still more from the apparently riddled and allegedly paradoxical nature of his philosophy and his stress upon the heedless unconsciousness of humankind, he was called "The Obscure" and the "Weeping Philosopher".

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 Heraclitus. [3]

Heraclitus LatitudeLongitudeDiameter
A49.3° S4.7° E6 km
C48.8° S6.3° E7 km
D50.4° S5.2° E52 km
E49.7° S6.7° E7 km
K49.5° S3.5° E17 km

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Lilius (crater) impact crater

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Deluc (crater) impact crater

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Cuvier (crater) impact crater

Cuvier is a lunar impact crater on the southern part of the Moon's near side. It is attached to the east-southeast rim of the unusually shaped formation Heraclitus. To the northeast is the crater Clairaut.

Jacobi (crater) impact crater

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Licetus (crater)

Licetus is a lunar impact crater on the near side of the Moon, in the rugged southern highland region. It lies to the south of the walled plain Stöfler, and is attached to the northern rim of the sub-divided crater Heraclitus. Just to the southeast is Cuvier. Licetus is 75 kilometers in diameter and 3.8 kilometers deep. It is from the Pre-Nectarian period, 4.55 to 3.92 billion years ago.

Cleostratus (crater) impact crater

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Moiseev (crater) lunar crater

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Clairaut (crater) lunar crater

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Crocco (crater) impact crater

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dAlembert (crater)

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Epimenides (crater) impact crater

Epimenides is a lunar impact crater that is located in the southwestern part of the Moon's near side, just to the east of the oddly shaped crater Hainzel. Just to the north and northeast is Lacus Timoris, a small lunar mare. The crater is 27 kilometers in diameter and 2,000 meters deep. It may be from the Pre-Nectarian period, 4.55 to 3.92 billion years ago.

Stiborius (crater) impact crater

Stiborius is a lunar impact crater that lies to the south-southwest of the crater Piccolomini, in the southeastern quadrant of the Moon's near side. To the south-southwest of Stiborius is the smaller Wöhler. Stiborius is 44 kilometers in diameter and 3.7 kilometers deep.

References

  1. 1 2 3 Autostar Suite Astronomer Edition. CD-ROM. Meade, April 2006.
  2. 1 2 Rükl, Antonín (1990). Atlas of the Moon. Kalmbach Books. ISBN   0-913135-17-8.
  3. Bussey, B.; Spudis, P. (2004). The Clementine Atlas of the Moon. New York: Cambridge University Press. ISBN   0-521-81528-2.