Raphael is a crater on Mercury. Its name was adopted by the International Astronomical Union (IAU) in 1976, and is named for the Italian painter Raphael (Raffaello Sanzio da Urbino). It is Tolstojan in age.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 6.3. The crater was first imaged by Mariner 10 in 1974.
Unlike other Mercurian craters of similar size, Raphael is not multi-ringed.Trask, N.J., 1976, History of basin development on Mercury: Conference on Comparisons of Mercury and The Moon: Lunar Science Institute Contribution no. 262, p.36.
The crater Flaiano lies just south of the center of Raphael.
There is also a high-albedo area east of Flaiano, that is associated with irregular depressions. The area was named Madu Facula by the IAU in 2023. The depressions are similar to those within Navoi, Lermontov, Scarlatti, and Praxiteles. The depressions resemble those associated with volcanic explosions.
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