Proctor (Martian crater)
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Proctor is a large crater in the
Noachis quadrangle The Noachis quadrangle is one of a series of list of quadrangles on Mars, 30 quadrangle maps of Mars used by the United States Geological Survey (USGS) Astrogeology Research Program. The Noachis quadrangle is also referred to as MC-27 (Mars Cha ...
of
Mars Mars is the fourth planet from the Sun and the second-smallest planet in the Solar System, only being larger than Mercury. In the English language, Mars is named for the Roman god of war. Mars is a terrestrial planet with a thin at ...
. It measures in diameter and was named after Richard A. Proctor, a British astronomer (1837–1888).


Dune fields

The crater contains a 35 x 65 km dark
dune field A dune is a landform composed of wind- or water-driven sand. It typically takes the form of a mound, ridge, or hill. An area with dunes is called a dune system or a dune complex. A large dune complex is called a dune field, while broad, fl ...
. It was one of the first sand dune fields ever recognized on Mars based on Mariner 9 images. The crater's dunes are being monitored by
HiRISE High Resolution Imaging Science Experiment is a camera on board the '' Mars Reconnaissance Orbiter'' which has been orbiting and studying Mars since 2006. The 65 kg (143 lb), US$40 million instrument was built under the direction ...
to identify changes over time. File:Russellcratermap.jpg, Topographical map showing location of Proctor crater and other nearby craters File:Proctor crater dunes 510A46.jpg, Another Viking image of the dunes in Proctor and in nearby craters File:Proctor Crater Ripples and Dunes.JPG, Proctor crater
transverse aeolian ridges Transverse aeolian ridges (TARs) are visually bright features commonly found in topographic depressions on Mars. These small-scale and relict bedforms were first seen in narrow-angle images from the Mars Orbiter Camera (MOC) and were called “ridg ...
and Dunes, as seen by
HiRISE High Resolution Imaging Science Experiment is a camera on board the '' Mars Reconnaissance Orbiter'' which has been orbiting and studying Mars since 2006. The 65 kg (143 lb), US$40 million instrument was built under the direction ...
File:Proctor Crater, Mars.jpg, HiRISE image of the crater with
transverse aeolian ridges Transverse aeolian ridges (TARs) are visually bright features commonly found in topographic depressions on Mars. These small-scale and relict bedforms were first seen in narrow-angle images from the Mars Orbiter Camera (MOC) and were called “ridg ...
surrounding a large dune File:Proctor Crater Dune Field.jpg, The edge of a dark dune field on the floor of Proctor crater File:Wikiproctordunes.jpg, Dune field on floor of Proctor crater, as seen by CTX camera on
Mars Reconnaissance Orbiter ''Mars Reconnaissance Orbiter'' (MRO) is a spacecraft designed to study the geology and climate of Mars, provide reconnaissance of future landing sites, and relay data from surface missions back to Earth. It was launched on August 12, 2005, an ...
. File:Wikiproctordunesclose.jpg, Close-up of dunes on floor of Proctor crater, as seen by CTX camera on Mars Reconnaissance Orbiter. This is an enlargement of part of previous image.


See also

* List of craters on Mars: O-Z


References


External links

* * {{Portal bar, Solar System Noachis quadrangle Impact craters on Mars