Bartók is the largest crater of the Kuiperian system on Mercury, at 118 km diameter. It is followed by Amaral crater.[2]
Within the central peak complex of Bartók is a dark spot of low reflectance material (LRM).[3] Dark spots are associated with hollows.
To the northeast of Bartók is the large basin Beethoven. The crater Vālmiki is to the northwest of Bartók, and Gogol is to the west.
Views
Approximate color image of Bartók at a high sun angle showing that the central peak is much darker than the floor and ejecta of the crater, with some areas that are much brighter
Another color image
Closer oblique view also at a high sun angle
References
^"Bartok". Gazetteer of Planetary Nomenclature. NASA. Retrieved 7 April 2020.
^Denevi, B. W., Ernst, C. M., Prockter, L. M., and Robinson, M. S., 2018. The Geologic History of Mercury. In Mercury: The View After MESSENGER edited by Sean C. Solomon, Larry R. Nittler, and Brian J. Anderson. Cambridge Planetary Science. Chapter 6, Table 6.4.
^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