Mozart (crater)
Planet | Mercury |
---|---|
Coordinates | 7°45′N 190°35′W / 7.75°N 190.59°W |
Quadrangle | Tolstoj |
Diameter | 241 km (150 mi) |
Eponym | Wolfgang Amadeus Mozart |
Mozart is a
IAU in 1976 after Austrian composer Wolfgang Amadeus Mozart.[1]
The arc of dark hills visible on the crater's floor represents remnants of a central
peak ring. Mozart is one of 110 peak ring basins on Mercury.[2] A close inspection of the area around Mozart crater shows many long chains of secondary craters
, formed by impact of material thrown out during the formation of the main crater.
Confirmed dark spots are present within Mozart.[3] The dark spots are present around the remnants of the peak ring.
Mozart crater is located just south of the
Caloris basin. To the southeast is Tir Planitia
.
Views
-
The first image of Mozart crater, acquired on MESSENGER's first flyby on 14 January 2008
-
Another MESSENGER image of central and northwestern Mozart, at a low sun angle. Shows the fractures in its smooth floor in bottom right, parts of its peak-ring, and the hummocky ejecta blanket in the upper left.
-
Mozart crater interior
References
- USGS. Retrieved 21 September 2022.
- ^ Chapman, C. R., Baker, D. M. H., Barnouin, O. S., Fassett, C. I., Marchie, S., Merline, W. J., Ostrach, L. R., Prockter, L. M., and Strom, R. G., 2018. Impact Cratering of Mercury. In Mercury: The View After MESSENGER edited by Sean C. Solomon, Larry R. Nittler, and Brian J. Anderson. Cambridge Planetary Science. Chapter 9.
- ^ Zhiyong Xiao, Robert G. Strom, David T. Blewett, Paul K. Byrne, Sean C. Solomon, Scott L. Murchie, Ann L. Sprague, Deborah L. Domingue, Jörn Helbert, 2013. Dark spots on Mercury: A distinctive low-reflectance material and its relation to hollows. Journal of Geophysical Research Planets. doi.org/10.1002/jgre.20115