Moody (crater)
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Moody (crater)
Moody is an impact crater on Mercury. Moody features a complex central peak and an annulus of dark material on its outer floor. The area inward of the dark ring appears reddish in enhanced color wide angle camera images acquired by the MESSENGER spacecraft, indicating the presence of material different in composition from that of either the dark material or the crater's immediate surroundings. Dark material has been found associated with other craters on Mercury, including Munch and Poe. Moody is somewhat unusual for having its dark ring confined to the crater floor, rather than forming the crater rim as at Munch and Poe."Moody Sculpts Mercury's Surface"
, MESSENGER, April 14, 2009.
The crater was named in November 2008 after Jamaican sculptor and painter

Ronald Moody
Ronald Moody (12 August 1900 – 6 February 1984) was a Jamaican-born sculptor, specialising in wood carvings. His work features in collections including the National Portrait Gallery and Tate Britain in London, as well as the National Gallery of Jamaica. He was the brother of anti-racist campaigner Harold Moody and award-winning physiologist Ludlow Moody. Biography Moody was born Ronald Clive Moody in 1900 in Kingston, Jamaica, into a well-off professional family. He attended Calabar College, Jamaica, moving to England in 1923 to study dentistry at King's College London, obtaining his degree in 1930."Ronald Moody: Sculpture and interwar Britain"
The Equiano Centre, UCL, 16 June 2015.
In London, he was inspired by the

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Impact Crater
An impact crater is a circular depression in the surface of a solid astronomical object 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. Lunar impact craters range from microscopic craters on lunar rocks returned by the Apollo Program and small, simple, bowl-shaped depressions in the lunar regolith to large, complex, multi-ringed impact basins. Meteor Crater is a well-known example of a small impact crater on Earth. Impact craters are the dominant geographic features on many solid Solar System objects including the Moon, Mercury, Callisto, Ganymede and most small moons and asteroids. On other planets and moons that experience more active surface geological processes, such as Earth, Venus, Europa, Io and Titan, visible impact craters are less common because they become eroded ...
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Mercury (planet)
Mercury is the smallest planet in the Solar System and the closest to the Sun. Its orbit around the Sun takes 87.97 Earth days, the shortest of all the Sun's planets. It is named after the Roman god ' ( Mercury), god of commerce, messenger of the gods, and mediator between gods and mortals, corresponding to the Greek god Hermes (). Like Venus, Mercury orbits the Sun within Earth's orbit as an inferior planet, and its apparent distance from the Sun as viewed from Earth never exceeds 28°. This proximity to the Sun means the planet can only be seen near the western horizon after sunset or the eastern horizon before sunrise, usually in twilight. At this time, it may appear as a bright star-like object, but is more difficult to observe than Venus. From Earth, the planet telescopically displays the complete range of phases, similar to Venus and the Moon, which recurs over its synodic period of approximately 116 days. The synodic proximity of Mercury to Earth makes Mercury most ...
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MESSENGER
''MESSENGER'' was a NASA robotic space probe that orbited the planet Mercury between 2011 and 2015, studying Mercury's chemical composition, geology, and magnetic field. The name is a backronym for "Mercury Surface, Space Environment, Geochemistry, and Ranging", and a reference to the messenger god Mercury from Roman mythology. ''MESSENGER'' was launched aboard a Delta II rocket in August 2004. Its path involved a complex series of flybys – the spacecraft flew by Earth once, Venus twice, and Mercury itself three times, allowing it to decelerate relative to Mercury using minimal fuel. During its first flyby of Mercury in January 2008, ''MESSENGER'' became the second mission, after Mariner 10 in 1975, to reach Mercury. ''MESSENGER'' entered orbit around Mercury on March 18, 2011, becoming the first spacecraft to do so. It successfully completed its primary mission in 2012. Following two mission extensions, the spacecraft used the last of its maneuvering propellant to deo ...
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Munch (crater)
Munch is a crater on Mercury. It was discovered on the first flyby of Mercury by the MESSENGER spacecraft on 14 January 2008, and was named after Edvard Munch a Norwegian painter, printmaker, and draftsman (1863-1944) by the IAU in November of the same year. Munch is west of Sander and Poe craters, within the Caloris basin Caloris Planitia is a plain within a large impact basin on Mercury, informally named Caloris, about in diameter. It is one of the largest impact basins in the Solar System. "Calor" is Latin for "heat" and the basin is so-named because the Sun .... References Impact craters on Mercury {{Mercury-planet-stub ...
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Poe (crater)
Poe is a crater on Mercury (planet), Mercury. It has diameter about 77 km and is situated in northern part of Caloris Planitia. It is centered on Hollows (Mercury), Hollows are scattered across Poe crater, and are abundant on the southern rim. History Poe is named after the famous author Edgar Allan Poe. The IAU named this crater in 2011 in honor of the Poe Toaster who put a bottle of cognac and roses at the grave of Poe. References

Poe Toaster Impact craters on Mercury Edgar Allan Poe {{Mercury-planet-stub ...
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NASA
The National Aeronautics and Space Administration (NASA ) is an independent agency of the US federal government responsible for the civil space program, aeronautics research, and space research. NASA was established in 1958, succeeding the National Advisory Committee for Aeronautics (NACA), to give the U.S. space development effort a distinctly civilian orientation, emphasizing peaceful applications in space science. NASA has since led most American space exploration, including Project Mercury, Project Gemini, the 1968-1972 Apollo Moon landing missions, the Skylab space station, and the Space Shuttle. NASA supports the International Space Station and oversees the development of the Orion spacecraft and the Space Launch System for the crewed lunar Artemis program, Commercial Crew spacecraft, and the planned Lunar Gateway space station. The agency is also responsible for the Launch Services Program, which provides oversight of launch operations and countdown management f ...
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USGS
The United States Geological Survey (USGS), formerly simply known as the Geological Survey, is a scientific agency of the United States government. The scientists of the USGS study the landscape of the United States, its natural resources, and the natural hazards that threaten it. The organization's work spans the disciplines of biology, geography, geology, and hydrology. The USGS is a fact-finding research organization with no regulatory responsibility. The agency was founded on March 3, 1879. The USGS is a bureau of the United States Department of the Interior; it is that department's sole scientific agency. The USGS employs approximately 8,670 people and is headquartered in Reston, Virginia. The USGS also has major offices near Lakewood, Colorado, at the Denver Federal Center, and Menlo Park, California. The current motto of the USGS, in use since August 1997, is "science for a changing world". The agency's previous slogan, adopted on the occasion of its hundredth anniv ...
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Peak Ring
A peak ring crater is a type of complex crater, which is different from a multi-ringed basin or central-peak crater. A central peak is not seen; instead, a roughly circular ring or plateau, possibly discontinuous, surrounds the crater's center, with the crater rim still farther out from the center. Formation The rings form by different processes, and inner rings may not be formed by the same processes as outer rings.Geology Pagewww.geologypage.com/2016/10/research-helps-explain-formation-ringed-crater-moon.html accessdate: February 5, 2017 It has long been the view that peak rings are formed in the stage subsequent to central peak formation in craters. The central peaks of craters are believed to originate from hydrodynamic flow of material lifted by inward-collapsing crater walls, while impact-shattered rock debris is briefly turned to fluid by strong vibrations that develop during crater formation. The peak-ring structure of Chicxulub crater was probably formed as inward-coll ...
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