Jump to content

Mare Fecunditatis

From Wikipedia, the free encyclopedia

This is an old revision of this page, as edited by ZéroBot (talk | contribs) at 00:58, 18 January 2012 (r2.7.1) (Robot: Adding pt:Mare Fecunditatis). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

Mare Fecunditatis
Mare Fecunditatis
Diameter840 km (520 mi)[1]
EponymSea of Fertility

Mare Fecunditatis (the "Sea of Fecundity" or "Sea of Fertility") is a lunar mare which is 840 km in diameter. The Fecuditatis basin formed in the Pre-Nectarian epoch, while the basin material surrounding the mare is of the Nectarian epoch. The mare material is of the Upper Imbrian epoch and is relatively thin compared to Mare Crisium or Mare Tranquillitatis. This basin is overlapped with the Nectaris, Tranquillitatis, and Crisium basins. Fecunditatis basin meets Nectaris basin along Fecunditatis' western edge, with the area along this zone faulted by arcuated grabens. On the eastern edge of Fecunditatis is the crater Langrenus. Near the center lie the interesting craters Messier A and B.

Sinus Successus lies along the eastern edge of the mare.

Lunar nearside with major maria and craters labelled.
Lunar nearside with major maria and craters labelled.

References

  1. ^ "Moon Mare/Maria". Gazetteer of Planetary Nomenclature. USGS Astrogeology. Retrieved 2010-08-20.