- 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...
- – 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...
-
impact of the
South Pole–Aitken basin.
Other large impact basins such as
Imbrium, Serenitatis, Crisium, Smythii, and
Orientale possess regionally low elevations...
- "J-missions", in July 1971. The site is
located on the
eastern edge of Mare
Imbrium on a lava
plain known as
Palus Putredinis. Hadley–Apennine is bordered...
-
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...
- serēnitātis, the "Sea of Serenity") is a
lunar mare
located to the east of Mare
Imbrium on the Moon. Its
diameter is 674 km (419 mi). Mare
Serenitatis is located...
-
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...
- characteristics. The
names of
maria refer to sea
features (Mare Humorum, Mare
Imbrium, Mare Insularum, Mare Nubium, Mare Spumans, Mare Undarum, Mare Vaporum...
