List of geological features on Hyperion

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Surface of Hyperion with several craters full of a mysterious reddish gunk. The material contains long chains of carbon and hydrogen and appears very similar to material found on other Saturnian satellites, most notably Iapetus. Hyperion surface.jpg
Surface of Hyperion with several craters full of a mysterious reddish gunk. The material contains long chains of carbon and hydrogen and appears very similar to material found on other Saturnian satellites, most notably Iapetus.

This is a list of named geological features on Hyperion, a moon of Saturn.

Contents

Dorsa

Bond-Lassell Dorsum on Hyperion (Cassini 2007) Bond-Lassell Dorsum on Hyperion.jpg
Bond-Lassell Dorsum on Hyperion (Cassini 2007)

There is one named dorsum (ridge) on Hyperion.

DorsumCoordinatesDiameter (km)Approval DateNamed AfterRefs
Bond-Lassell Dorsum 48°00′N143°30′W / 48°N 143.5°W / 48; -143.5 (Bond-Lassell) 01982 George Phillips Bond, William Cranch Bond and William Lassell WGPSN

Craters

This is a list of craters on Hyperion. Hyperionian craters are named after sun and moon gods in various mythologies.

Crater Coordinates Diameter
(km)
Approval
Year
Eponym Ref
Bahloo 36°N164°E / 36°N 164°E / 36; 164 (Bahloo) n.a.1982 Bahloo. The Moon; maker of girl babies (Aboriginal mythology) WGPSN
Helios 71°N132°W / 71°N 132°W / 71; -132 (Helios) n.a.1982 Helios. Greek sun god; son of Hyperion (Greek mythology) WGPSN
Jarilo 61°N177°E / 61°N 177°E / 61; 177 (Jarilo) n.a.1982 Jarilo, East Slavic god of the sun fertility and love (Slavic mythology) WGPSN
Meri 3°N171°W / 3°N 171°W / 3; -171 (Meri) n.a.1982 Meri, folk hero; the Sun (Bororó people) WGPSN

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<span class="mw-page-title-main">Impact crater</span> Circular depression in a solid astronomical body formed by the impact of a smaller object

An impact crater is a circular depression in the surface of a solid astronomical body formed by the hypervelocity impact of a smaller object. 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 in size from microscopic craters seen on lunar rocks returned by the Apollo Program to simple bowl-shaped depressions and vast, complex, multi-ringed impact basins. Meteor Crater is a well-known example of a small impact crater on Earth.

<span class="mw-page-title-main">Iapetus (moon)</span> Moon of Saturn

Iapetus is the outermost of Saturn's large moons. With an estimated diameter of 1,469 km, it is the third-largest moon of Saturn and the eleventh-largest in the Solar System. Named after the Titan Iapetus, the moon was discovered in 1671 by Giovanni Domenico Cassini.

<span class="mw-page-title-main">Hyperion (moon)</span> Moon of Saturn

Hyperion, also known as Saturn VII, is the eighth-largest moon of Saturn. It distinguished by its highly irregular shape, chaotic rotation, low density, and its unusual sponge-like appearance. It was the first non-rounded moon to be discovered.

<span class="mw-page-title-main">Phoebe (moon)</span> Moon of Saturn

Phoebe is the most massive irregular satellite of Saturn with a mean diameter of 213 km (132 mi). It was discovered by William Henry Pickering on 18 March 1899 from photographic plates that had been taken by DeLisle Stewart starting on 16 August 1898 at the Boyden Station of the Carmen Alto Observatory near Arequipa, Peru. It was the first natural satellite to be discovered photographically.

<span class="mw-page-title-main">Alphonsus (crater)</span> Crater on the Moon

Alphonsus is an ancient impact crater on the Moon that dates from the pre-Nectarian era. It is located on the lunar highlands on the eastern end of Mare Nubium, west of the Imbrian Highlands, and slightly overlaps the crater Ptolemaeus to the north. To the southwest is the smaller Alpetragius. The crater name was approved by the IAU in 1935.

<span class="mw-page-title-main">Moons of Saturn</span> Natural satellites of the planet Saturn

The moons of Saturn are numerous and diverse, ranging from tiny moonlets only tens of meters across to the enormous Titan, which is larger than the planet Mercury. There are 146 moons with confirmed orbits, the most of any planet in the solar system. This number does not include the many thousands of moonlets embedded within Saturn's dense rings, nor hundreds of possible kilometer-sized distant moons that were seen through telescopes but not recaptured. Seven Saturnian moons are large enough to have collapsed into a relaxed, ellipsoidal shape, though only one or two of those, Titan and possibly Rhea, are currently in hydrostatic equilibrium. Three moons are particularly notable. Titan is the second-largest moon in the Solar System, with a nitrogen-rich Earth-like atmosphere and a landscape featuring river networks and hydrocarbon lakes. Enceladus emits jets of ice from its south-polar region and is covered in a deep layer of snow. Iapetus has contrasting black and white hemispheres as well as an extensive ridge of equatorial mountains among the tallest in the solar system.

This is a directory of lists of geological features on planets excepting Earth, moons and asteroids ordered by increasing distance from the Sun.

<span class="mw-page-title-main">Banting (crater)</span> Lunar impact crater

Banting is a small, bowl-shaped lunar impact crater located near the middle of the Mare Serenitatis on the Earth's moon.

<span class="mw-page-title-main">Far side of the Moon</span> Hemisphere of the Moon that always faces away from Earth

The far side of the Moon is the lunar hemisphere that always faces away from Earth, opposite to the near side, because of synchronous rotation in the Moon's orbit. Compared to the near side, the far side's terrain is rugged, with a multitude of impact craters and relatively few flat and dark lunar maria ("seas"), giving it an appearance closer to other barren places in the Solar System such as Mercury and Callisto. It has one of the largest craters in the Solar System, the South Pole–Aitken basin. The hemisphere has sometimes been called the "dark side of the Moon", where "dark" means "unknown" instead of "lacking sunlight" – each location on the Moon experiences two weeks of sunlight while the opposite location experiences night.

<span class="mw-page-title-main">Delisle (crater)</span> Crater on the Moon

Delisle is a small lunar impact crater in the western part of the Mare Imbrium. It was named after French astronomer Joseph-Nicolas Delisle. It lies to the north of the crater Diophantus, and just to the northwest of the ridge designated Mons Delisle. Between Delisle and Diophantus is a sinuous rille named Rima Diophantus, with a diameter of 150 km. To the northeast is another rille designated Rima Delisle, named after this crater.

<span class="mw-page-title-main">Diophantus (crater)</span> Crater on the Moon

Diophantus is a lunar impact crater that lies in the southwestern part of the Mare Imbrium. It was named after ancient Greek mathematician Diophantus. It forms a pair with the larger crater Delisle to the north. Diophantus has a wide inner wall and a low central rise. To the north of Diophantus is the sinuous rille designated Rima Diophantus, named after the crater. Diophantus C lies near the exterior of the southwest wall.

<span class="mw-page-title-main">Davy (crater)</span> Crater on the Moon

Davy is a small lunar impact crater that is located on the eastern edge of the Mare Nubium. It was named after British physicist Humphry Davy. It overlies the lava-flooded remains of the satellite crater Davy Y to the east, a formation which contains a crater chain designated Catena Davy. To the southeast of Davy is the prominent crater Alphonsus.

<span class="mw-page-title-main">Ibn Firnas (crater)</span> Lunar impact crater

Ibn Firnas is a lunar impact crater on the far side of the Moon. Attached to the exterior of its southwestern rim is the prominent crater King. Only a few kilometers to the north, separated by a rugged stretch of terrain, is the larger crater Ostwald.

<span class="mw-page-title-main">Mons La Hire</span> Solitary lunar mountain in the western Mare Imbrium

Mons La Hire is a solitary lunar mountain in the western Mare Imbrium. It is located to the northeast of the crater Euler, and to the west-northwest of Lambert.

<span class="mw-page-title-main">Lunar craters</span> Craters on Earths moon

Lunar craters are impact craters on Earth's Moon. The Moon's surface has many craters, all of which were formed by impacts. The International Astronomical Union currently recognizes 9,137 craters, of which 1,675 have been dated.

Chiron is the name given to a supposed moon of Saturn sighted by Hermann Goldschmidt in 1861. It has since been determined that no such moon exists.

In the mythology of the Bororó people of Brazil, Meri is a folk hero and sun-god.

The following outline is provided as an overview of and topical guide to the Moon:

References

  1. “Key to Giant Space Sponge Revealed” Space.com / Yahoo News, Jul. 4 2007, archived copy.