Mare Serenitatis

E566523

Mare Serenitatis is a large lunar mare, or basaltic plain, on the Moon’s near side, easily visible from Earth as a dark, circular feature formed by ancient volcanic activity.

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Statements (45)

Predicate Object
instanceOf basaltic plain
lunar mare
adjacentTo Mare Imbrium NERFINISHED
Mare Tranquillitatis NERFINISHED
Mare Vaporum NERFINISHED
age Imbrian period
albedo low
albedoContrastWith surrounding lunar highlands
appearance dark region
basinType multi-ring impact basin
belongsTo lunar maria
boundedBy Montes Caucasus NERFINISHED
Montes Haemus NERFINISHED
Montes Taurus NERFINISHED
containsFeature Serenitatis Basin NERFINISHED
diameter approximately 674 km
formedBy ancient volcanic activity
formedFrom impact basin flooding by lava
geologicAge about 3.8 to 3.6 billion years
hasCraterOnMargin Bessel NERFINISHED
Menelaus NERFINISHED
Posidonius NERFINISHED
Sulpicius Gallus NERFINISHED
hasRegolith fine lunar soil
hasRille Rimae Menelaus NERFINISHED
Rimae Sulpicius Gallus NERFINISHED
hasShape roughly circular
liesNear Apollo 17 Taurus–Littrow landing site
locatedIn Serenitatis Basin NERFINISHED
locatedOn Moon NERFINISHED
near side of the Moon
mappedBy Lunar Orbiter missions NERFINISHED
Lunar Reconnaissance Orbiter NERFINISHED
namedInLanguage Latin
nameMeaning Sea of Serenity NERFINISHED
observedBy ground-based telescopes
partOf near-side maria pattern visible to naked eye
quadrant northeastern near side of the Moon
scientificInterest study of impact basin evolution
study of lunar volcanism
selenographicLatitude about 28.0° N
selenographicLongitude about 17.5° E
surfaceComposition basaltic lava flows
visibleFrom Earth NERFINISHED
visitedBy Apollo 17 mission vicinity

Referenced by (3)

Full triples — surface form annotated when it differs from this entity's canonical label.

Mare Tranquillitatis boundedBy Mare Serenitatis
Mare Tranquillitatis adjacentTo Mare Serenitatis
Mare Imbrium adjacentTo Mare Serenitatis