Craterra

Mare Cognitum

Volcanic Structures of Mons Moro

A low-albedo mountain in Mare Cognitum featuring steplike ledges and shallow craters that point to complex lunar volcanism.

Feature Profile & Selenographic Data

Feature type
mons
Coordinates
11.84° S · 19.84° W
Diameter
13.68 km
IAU approval
1976/01/01 00:00:00
LAC quadrangle
LAC-76 · Montes Riphaeus

Geological Chronicle

Located at 11.84° S and 19.84° W in Mare Cognitum, southwest of the crater Bonpland, Mons Moro is a linear lunar peak spanning 13.68 kilometers in length. The feature exhibits a lower albedo than the surrounding mare. The International Astronomical Union officially approved the mountain's name in 1976, referring to Italian geologist Anton Lazzaro Moro.

Described in Apollo Over the Moon, two explanations for the origin of Mons Moro seem equally plausible. The complex may consist of a densely cratered block of terrae partly inundated by mare lavas and blanketed by dark volcanic ejecta, or a pile of viscous lava flows. Steplike ledges along the east side represent successive lava flows, while shallow craters with steep raised rims distinguish them from impact craters. A lower concentration of fresh craters across the darkened area indicates the blanketing was deposited appreciably later than the mare lavas.

Chronology & Exploration

  1. 1976 IAU Name Approval

    The International Astronomical Union officially approves the name Mons Moro, referring to Italian geologist Anton Lazzaro Moro.

Scientific Sources & References

Name Origin

Antonio Lazzaro; Italian Earth scientist (1687-1764).

Interactive Lunar Surface

Explore Mons Moro in 3D

Inspect lunar elevation data and the official selenographic position.