- 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...
- m****if in the
Montes Apenninus range,
along the
eastern edge of the Mare
Imbrium. It is
located to the west of the
crater Conon. To the west of this peak...
-
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...
- 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...
- 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...
- on the
lunar mare
where Oce****
Procellarum to the
southwest joins Mare
Imbrium to the east.
There are
three primary peaks in this formation,
which rise...
-
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...
-
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...
-
terrain found in
lunar highlands. The
period ended with the
formation of the
Imbrium basin,
which initiated the
Imbrian Period.
Magnetic anomalies found in...
-
impact of the
South Pole–Aitken basin.
Other large impact basins such as
Imbrium, Serenitatis, Crisium, Smythii, and
Orientale possess regionally low elevations...
