Craterra

Mare Tranquillitatis

Mons Esam: An Isolated Lunar Cone

Rising roughly 400 meters above northern Mare Tranquillitatis, Mons Esam is an isolated tectonic lunar cone with an eight-kilometer base.

Feature Profile & Selenographic Data

Feature type
mons
Coordinates
14.61° N · 35.71° E
Diameter
7.92 km
IAU approval
1979/01/01 00:00:00
LAC quadrangle
LAC-61 · Taruntius

Geological Chronicle

Mons Esam is a small, isolated mountain situated in the northern part of Mare Tranquillitatis. Positioned southeast of Vitruvius crater and west-northwest of Lyell crater, it lies southwest of the bay called Sinus Amoris. The peak rises roughly 400 meters above the surrounding plains over a base diameter of 8 kilometers.

Geologically, the mountain is a lunar cone formed through tectonic processes. Located at selenographic coordinates 14.6° N, 35.7° E, the feature derives its name from an Arabic masculine name that was not chosen to represent a specific individual.

Just to the south of Mons Esam, a pair of tiny craters assigned names by the International Astronomical Union sit atop two lunar domes. These structures are most likely volcanoes not formed by impacts.

Scientific Sources & References

Name Origin

Arabic male name.

Interactive Lunar Surface

Explore Mons Esam in 3D

Inspect lunar elevation data and the official selenographic position.