Mare Ingenii (Latin ''ingeniī'', the "Sea of Cleverness") is one of the few

lunar mare The lunar maria (; singular: mare ) are large, dark, basaltic plains on Earth's Moon, formed by ancient asteroid impacts on the far side on the Moon that triggered volcanic activity on the opposite (near) side. They were dubbed , Latin for 'seas' ...

features on the

far side ''The Far Side'' is a single-panel comic created by Gary Larson and syndicated by Chronicle Features and then Universal Press Syndicate, which ran from December 31, 1979, to January 1, 1995 (when Larson retired as a cartoonist). Its surrealis ...

of the Moon. The mare sits in the Ingenii basin, which is of the

Pre-Nectarian The pre-Nectarian period of the lunar geologic timescale runs from 4.533 billion years ago (the time of the initial formation of the Moon) to 3.920 billion years ago, when the Nectaris Basin was formed by a large impact. It is followed by the Necta ...

epoch, which lies in turn in the outer part of the older and much larger

South Pole–Aitken basin The South Pole–Aitken basin (SPA Basin, ) is an immense impact crater on the far side of the Moon. At roughly in diameter and between deep, it is one of the largest known impact craters in the Solar System. It is the largest, oldest, and dee ...

. The mare material located in Ingenii and the surrounding craters is of the

Upper Imbrian The Imbrian is a lunar geologic period divided into two epochs, the Early and Late. Early Imbrian In the lunar geologic timescale, the Early Imbrian epoch occurred from 3,850 million years ago to about 3,800 million years ago. It overlaps the en ...

epoch. The dark circular feature which dominates this mare is the crater

Thomson Thomson may refer to: Names * Thomson (surname), a list of people with this name and a description of its origin * Thomson baronets, four baronetcies created for persons with the surname Thomson Businesses and organizations * SGS-Thomson Mic ...

(112 km diameter), with the overflow from Ingenii/Thomson directly to the east. Mare Ingenii is incompletely and thinly covered over much of its expanse with mare lava sheets. The light grey crater to the south of Mare Ingenii is Obruchev. The mare has swirling patterns of bright material, similar to

Reiner Gamma Reiner Gamma (γ) is a geographical feature of the Moon known as a lunar swirl. It is one of the most visible lunar swirls from Earth, visible from most telescopes. It was originally thought to be a lunar highland, but scientists eventually reali ...

and to patterns within

Mare Marginis Mare Marginis (Latin ''marginis'', the "Sea of the Edge") is a lunar mare that lies on the very edge of the lunar nearside. The selenographic coordinates of this feature are 13.3° N, 86.1° E, and the diameter is 358 km. The name is Latin ...

, which are not associated with topographic or volcanic features. The

lunar swirls Lunar swirls are enigmatic features found across the Moon's surface, which are characterized by having a high albedo, appearing optically immature (i.e. having the optical characteristics of a relatively young regolith), and (often) having a si ...

are believed to be associated with magnetic fields. Prior to formal naming in 1961 by the

IAU The International Astronomical Union (IAU; french: link=yes, Union astronomique internationale, UAI) is a nongovernmental organisation with the objective of advancing astronomy in all aspects, including promoting astronomical research, outreach ...

, the crater was known as ''Basin XIV''. Mare Ingenii is located at the antipode of the Mare Imbrium impact basin. The furrowed crater walls of the basin (and possibly those of Van de Graaff crater) may have been caused by focused seismic waves resulting from the Imbrium impact. The mare contains the second instance of a lunar pit discovered on the moon and one of several outside the Earth to date. File:Ingenii basin topo.jpg, Topographic map File:Ingenii basin GRAIL gravity.jpg, Gravity map based on

GRAIL The Gravity Recovery and Interior Laboratory (GRAIL) was an American lunar science mission in NASA's Discovery Program which used high-quality gravitational field mapping of the Moon to determine its interior structure. The two small spacecraf ...

File:Mare Ingenii Clementine.jpg, Orthogonal view of Mare Ingenii, showing variation in

albedo Albedo (; ) is the measure of the diffuse reflection of solar radiation out of the total solar radiation and measured on a scale from 0, corresponding to a black body that absorbs all incident radiation, to 1, corresponding to a body that refl ...

File:Mare Ingenii A17-M-1554.jpg, Mare Ingenii as viewed by Apollo 17, facing south

Lunar Reconnaissance Orbiter Camera (LROC) articles

The Swirls of Mare Ingenii

Depths of Mare Ingenii

References

External links

High resolution lunar overflight video
by Seán Doran, based on LRO data, that passes over Mare Ingenii at the start Ingenii Ingenii Ingenii {{Moon-stub

See also

Lunar Reconnaissance Orbiter Camera (LROC) articles

References

External links