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Degas (crater)

Coordinates:37°05′N127°20′W / 37.08°N 127.34°W /37.08; -127.34
From Wikipedia, the free encyclopedia
Crater on Mercury
Degas
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Degas crater,MESSENGER spacecraft image, 2011. Inset isMariner 10 image from 1974.
Feature typeCentral-peak impact crater
LocationShakespeare quadrangle,Mercury
Coordinates37°05′N127°20′W / 37.08°N 127.34°W /37.08; -127.34
Diameter54 km (34 mi)
DiscovererMariner 10
EponymEdgar Degas

Degas is a youngcrater onMercury. It was named after the French impressionist painterEdgar Degas in 1979.[1] The crater was first imaged byMariner 10 in 1974.[2]

The prominentrays of the crater consist of light colored material blasted out during the crater's formation. Craters older than Degas are covered by the ray material, while younger craters are seen superimposed on the rays.[3] Degas forms a crater pair withBrontë to the north. Both lie near the center ofSobkou Planitia.[4]

The crater's floor contains cracks that formed as the pool ofimpact melt cooled and shrank. The high-reflectance material on the walls and in the central portion of the crater probably has a composition distinct from that of the crater floor and surroundings. The illumination conditions and down-slope movement of eroded material exposing fresh rock also contribute to the bright appearance.[5] The floor of Degas exposed low-reflectance material (LRM).[6]

Degas is one of the largest craters of theKuiperian system on Mercury. The largest isBartók crater.[7]

Views

[edit]
  • Mariner 10 image
  • MESSENGER mosaic
    MESSENGER mosaic
  • Sequence of adjacent but non-overlapping images acquired by MESSENGER NAC of the interior of Degas. All images are oblique and looking northwest. The upper left three images show the central peak. The upper right and lower left images show the fractured crater floor. The two central bottom images show terraces and flow structures on the northern slope of the crater wall. The lower right image shows the crater rim. Distance across foreground in each image is approximately 2.5 km.
    Sequence of adjacent but non-overlapping images acquired by MESSENGER NAC of the interior of Degas. All images are oblique and looking northwest. The upper left three images show the central peak. The upper right and lower left images show the fractured crater floor. The two central bottom images show terraces and flow structures on the northern slope of the crater wall. The lower right image shows the crater rim. Distance across foreground in each image is approximately 2.5 km.

References

[edit]
  1. ^"Degas (crater)".Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  2. ^Davies, M. E.; Dwornik, S. E.; Gault, D. E.; Strom, R. G. (1978).Atlas of Mercury. National Aeronautics and Space Administration. pp. 1–128.ISBN 978-1-114-27448-8. Special Publication SP-423.
  3. ^Nemiroff, R.; Bonnell, J., eds. (16 December 2000)."Degas Ray Crater on Mercury".Astronomy Picture of the Day.NASA.
  4. ^Sobkou Planitia, at eSky
  5. ^Degas CraterArchived 2014-09-14 at theWayback Machine at NASA Messenger website. This article incorporatespublic domain text from thisUS government website.
  6. ^Denevi, B. W., Ernst, C. M., Prockter, L. M., and Robinson, M. S., 2018. The Geologic History of Mercury. InMercury: The View AfterMESSENGER edited by Sean C. Solomon, Larry R. Nittler, and Brian J. Anderson. Cambridge Planetary Science. Chapter 6.4.4.
  7. ^Denevi, B. W., Ernst, C. M., Prockter, L. M., and Robinson, M. S., 2018. The Geologic History of Mercury. InMercury: The View AfterMESSENGER edited by Sean C. Solomon, Larry R. Nittler, and Brian J. Anderson. Cambridge Planetary Science. Chapter 6, Table 6.4.

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