- Mare
Imbrium /ˈɪmbriəm/ (Latin
imbrium, the "Sea of Showers" or "Sea of Rains") is a vast lava
plain within the
Imbrium Basin on the Moon and is one of...
- been
formed from ejecta, or debris, from the
impact which formed Mare
Imbrium.
During Apollo 14, the crew
members sampled ejecta from Cone crater, a...
-
formed by the
impact that
created Mare
Imbrium. Mons
Huygens rises 5,300 m (17,380 ft) from its Mare
Imbrium base, per
altimetry data from the Lunar...
-
somewhat worn, the east
being scoured by
debris from the
Imbrium basin,
hence forming part of the
Imbrium Sculpture. The
interior floor of
Halley is relatively...
-
deposit resulting from the
formation of the
Imbrium basin or of the
Orientale basin,
which occurred after the
Imbrium basin-forming event. The
Descartes highlands...
-
feature that
bisects the
Montes Alpes range. It
extends 166 km from the Mare
Imbrium basin,
trending east-northeast to the edge of the Mare Frigoris. The valley...
-
eastern edges of the Mare
Imbrium. Its
diameter is 81 km. The
diameter of
Archimedes is the
largest of any
crater on the Mare
Imbrium. The rim has a significant...
-
impact of the
South Pole–Aitken basin.
Other large impact basins such as
Imbrium, Serenitatis, Crisium, Smythii, and
Orientale possess regionally low elevations...
-
Montes Apenninus is the most
prominent remnant of the
outer ring of the
Imbrium basin,
which also
includes Montes Carpatus to its
south and
Montes Caucasus...
- – Lunokhod-1
rover traveled 10.5 km (6.5 mi)
across lunar surface Mare
Imbrium 038.28N 325.00E Luna-18 5,750
Proton 2
September 1971
Sample return Failure...
