Home Equipment Moon Nebulae Galaxies

StarCo by Ludo Coppens                                        © 2014-2023                                   ludo.coppens(at)kineco.be

Select a rima by clicking on the name. Move the mouse over the full scale image of the larger region to show names of prominent surface features and additional data: depth from rim to crater floor and diameter, taken from the Times Atlas of the Moon (Ed. H.A.G. Lewis, Times Newspapers Ltd., 1969; charts available online at http://www.lpi.usra.edu/resources/mapcatalog/LAC/) and from Virtual Moon Atlas (Christian Legrand & Patrick Chevalley).


 Agatharchides

 Archimedes

 Ariadaeus

 Aristarchus

 Aristoteles

 G. Bond

 W. Bond

 Bradley

 Bürg

 Calippus

 Campanus

 Chacormac

 Cleomedes

 Conon


 Doppelmayer

 Eudoxus

 Fresnel

 Gassendi

 Gay-Lussac

 Goclenius

 Gould

 Hadley

 Herigonius

 Hesiodus

 Hippalus

 Hyginus

 Hypatia

 Littrow

 Maclear

 Maestlin

 Maupertuis

 Menelaus

 Mersennius

 Messier

 Milichius

 Opelt

 Parry

 Pitatus

 Plato

 Plinius

 Posidonius

 Prinz




 Ramsden

 Ritter

 Rømer

 Secchi

 Sosigenes

 Thaetetus

 Triesnecker








A rima (GER, ENG: rille) is a long (up to hundreds of km) and rather narrow (up to a few km) depression or fissure in the lunar surface. Straight (possibly grabens, tectonic depressions between parallel faults), sinuous (meandering; possibly collapse lava tubes) or arcuate (around inner edges of maria; probably due to shrinking of cooling lava of cooling lava ).

(At right: oblique view from Rima Ariadaeus I, taken from lunar orbit; © NASA)