Ibn-Rushd (crater)

Summary

Ibn-Rushd is a lunar impact crater located to the northwest of the larger crater Cyrillus. To the northwest is the crater Kant and to the north is Mons Penck, a mountain promontory. The crater is somewhat eroded with age, and the southern rim is overlain by a pair of smaller craters named Cyrillus B and C. The crater floor is relatively flat, and lacks a central peak. In 1976 the crater was named after Ibn Rushd (Latinized as Averroes),[1] the 12th-century Muslim polymath from the Islamic Spain, whose many scientific accomplishments included analysis of the lunar surface. Prior to that, it was identified as Cyrillus B.

Ibn-Rushd
LRO WAC mosaic
Coordinates11°42′S 21°42′E / 11.7°S 21.7°E / -11.7; 21.7
Diameter33 km
Colongitude339° at sunrise
EponymIbn Rushd
Selenochromatic Image (Si) of the crater area
Lunar Orbiter 4 image

References edit

  1. ^ "Ibn-Rushd (crater)". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
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  • McDowell, Jonathan (July 15, 2007). "Lunar Nomenclature". Jonathan's Space Report. Retrieved 2007-10-24.
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  • Rükl, Antonín (1990). Atlas of the Moon. Kalmbach Books. ISBN 978-0-913135-17-4.
  • Webb, Rev. T. W. (1962). Celestial Objects for Common Telescopes (6th revised ed.). Dover. ISBN 978-0-486-20917-3.
  • Whitaker, Ewen A. (1999). Mapping and Naming the Moon. Cambridge University Press. ISBN 978-0-521-62248-6.
  • Wlasuk, Peter T. (2000). Observing the Moon. Springer. ISBN 978-1-85233-193-1.