Craterra

Montes Alpes Graben

A Fault Graben Cleaving the Lunar Alps

Bisecting the Montes Alpes between Mare Imbrium and Mare Frigoris, Vallis Alpes preserves a flat, lava-flooded trough channeled by a narrow central rille.

Feature Profile & Selenographic Data

Feature type
vallis
Coordinates
49.21° N · 3.63° E
Diameter
155.42 km
IAU approval
1961/01/01 00:00:00
LAC quadrangle
LAC-12 · Plato

Geological Chronicle

Vallis Alpes bisects the Montes Alpes range, extending from the Mare Imbrium basin toward the edge of Mare Frigoris. Constricted at both ends, the valley broadens along its middle stretch to a maximum width of about 10 kilometers.

The valley floor is a flat, lava-flooded surface bisected by a slender, cleft-like rille that spans 196.65 kilometers in length, exceeding the valley proper while measuring 0.58 kilometers wide and 77.69 meters deep.

The valley is most likely a graben later flooded with magma, though stress fractures from mantle expansion, regolith cooling, or the Imbrium impact event may have contributed. Francesco Bianchini discovered the valley in 1727, and the International Astronomical Union confirmed its name in 1961.

Chronology & Exploration

  1. 1727 Discovery

    Francesco Bianchini discovers the valley.

  2. 1961 IAU Confirmation

    The International Astronomical Union confirms the name Vallis Alpes.

Scientific Sources & References

Name Origin

"Alpine Valley."

Interactive Lunar Surface

Explore Vallis Alpes in 3D

Inspect lunar elevation data and the official selenographic position.