Rille

This article is about lunar features. For other uses, see Rille (disambiguation).
For the Italian wine grape, see Rille (grape).
Rimae on the floor of the lunar crater Gassendi, from Apollo 16.
Mamers Valles rille on Mars.
Rima Ariadaeus is categorized as a straight and branching rille and is over 300 km in length.
A full shot of Hadley Rille.[1]
Hadley Rille is a sinuous rille for which NASA says that they don't have a (final and definite) conclusion on how it formed.[1]

Rille (German for 'groove') is typically used to describe any of the long, narrow depressions in the lunar surface that resemble channels. The Latin term is rima, plural rimae. Typically a rille can be up to several kilometers wide and hundreds of kilometers in length. However, the term has also been used loosely to describe similar structures on a number of planets in the Solar System, including Mars, Venus, and on a number of moons. All bear a structural resemblance to each other.

Structures

Three types of rille are found on the lunar surface:

Rilles which show more than one structure are termed hybrid rilles. Rima Hyginus in Sinus Medii is an example, initially formed through a fault and subsequently subject to volcanic activity.

Formation

Precise formation mechanisms of rilles have yet to be determined. It is likely that different types formed by different processes. Common features shared by lunar rilles and similar structures on other bodies suggest that common causative mechanisms operate widely in the solar system. Leading theories include lava channels, collapsed lava tubes, near-surface dike intrusion, nuée ardente (pyroclastic cloud), subsidence of lava-covered basin and crater floors, and tectonic extension. On-site examination would be necessary to clarify exact methods.

Sinuous rilles

According to NASA, the origin of lunar sinuous rilles remains controversial.[1] The Hadley Rille is a 1.5 km wide and over 300 m deep sinuous rille. It is thought to be a giant conduit that carried lava from an eruptive vent far to the south. Topographic information obtained from the Apollo 15 photographs supports this possibility; however, many puzzles about the rille remain.[1]

See also

References

  1. 1 2 3 4 "ch6.2". History.nasa.gov. Retrieved 2012-09-17.
General
  • Ewen A. Whitaker, Mapping and Naming the Moon, Cambridge University Press, 1999, ISBN 0-521-62248-4.
  • American Astronomers Report: What Formed the Moon's Sinuous Rilles?, Sky & Telescope, Vol. XXVI, No. 1, July, 1963.
  • Atlas of Lunar Sinuous Rilles
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