Lacus Temporis
Encyclopedia
Lacus Temporis is a small lunar mare
that is located in the northeastern quadrant of the Moon
's near side. The selenographic coordinates of this feature are 45.9°N 58.4°E, and it lies within a diameter of 117 km.
This small mare is composed of two large, roughly circular patches of relatively smooth surface, with a pair of small, cup-shaped craters located prominently at their intersection. Both of these regions of basalt
ic lava
covered surface have some smaller side lobes, which are most likely impact features that have become flooded.
Just to the southwest of this feature is the crater Chevallier
and to the southeast lies Carrington
.
Lunar mare
The lunar maria are large, dark, basaltic plains on Earth's Moon, formed by ancient volcanic eruptions. They were dubbed maria, Latin for "seas", by early astronomers who mistook them for actual seas. They are less reflective than the "highlands" as a result of their iron-rich compositions, and...
that is located in the northeastern quadrant of the Moon
Moon
The Moon is Earth's only known natural satellite,There are a number of near-Earth asteroids including 3753 Cruithne that are co-orbital with Earth: their orbits bring them close to Earth for periods of time but then alter in the long term . These are quasi-satellites and not true moons. For more...
's near side. The selenographic coordinates of this feature are 45.9°N 58.4°E, and it lies within a diameter of 117 km.
This small mare is composed of two large, roughly circular patches of relatively smooth surface, with a pair of small, cup-shaped craters located prominently at their intersection. Both of these regions of basalt
Basalt
Basalt is a common extrusive volcanic rock. It is usually grey to black and fine-grained due to rapid cooling of lava at the surface of a planet. It may be porphyritic containing larger crystals in a fine matrix, or vesicular, or frothy scoria. Unweathered basalt is black or grey...
ic lava
Lava
Lava refers both to molten rock expelled by a volcano during an eruption and the resulting rock after solidification and cooling. This molten rock is formed in the interior of some planets, including Earth, and some of their satellites. When first erupted from a volcanic vent, lava is a liquid at...
covered surface have some smaller side lobes, which are most likely impact features that have become flooded.
Just to the southwest of this feature is the crater Chevallier
Chevallier (crater)
Chevallier is a lunar crater that is located in the northeastern part of the Moon's near side, about a crater diameter east-southeast of the prominent crater Atlas. To the south-southeast of Chevallier is the flooded crater Shuckburgh....
and to the southeast lies Carrington
Carrington (crater)
Carrington is a lunar crater that is located just to the northeast of the crater Schumacher, in the northeastern part of the Moon. It lies in a stretch of rough terrain between two small lunar maria, with Lacus Temporis to the northwest and the smaller Lacus Spei to the east...
.