Mare Frigoris

E870827

Mare Frigoris is a long, dark lunar mare stretching across the Moon’s northern latitudes, formed by ancient basaltic lava flows.

All labels observed (2)

Label Occurrences
Mare Frigoris canonical 2
Mare Frigoris region 1

How this entity was disambiguated

Statements (46)

Predicate Object
instanceOf lunar mare
albedo low
appearance dark
belongsTo Moon nearside maria belt
lunar maria
borderedBy Lacus Mortis
Lacus Somniorum
Mare Crisium
Mare Imbrium
Mare Serenitatis
Mare Tranquillitatis
contrastWith lunar highlands
coordinateSystem selenographic coordinates
discoverer early telescopic astronomers
extendsFrom near crater Plato in the west
extendsTo near Mare Crisium in the east
formationProcess ancient volcanic flooding
geologicAge Imbrian
hasFeature few large impact craters compared to highlands
relatively smooth surface
hasNeighboringCrater Aristoteles
linked to: Aristotle

Eudoxus
Plato
isPartOf near side of the Moon
liesNorthOf Mare Imbrium
Mare Serenitatis
Mare Tranquillitatis
liesWestOf Mare Crisium
locatedIn Moon northern hemisphere
locatedOn Moon
namedAfter Latin word "frigus" (cold)
namedBy Giovanni Battista Riccioli
nameMeaning Sea of Cold
namingYear 1651
observedFrom Earth
orientation east–west
regionType lowland plain
scientificInterest records history of lunar volcanism
used to study thickness of lunar crust in northern nearside
selenographicLatitudeRange high northern latitudes
shape elongated
spectralType basaltic mare material
surfaceComposition basaltic lava flows
surfaceGravity lunar gravity
surfaceType solidified basaltic plain
visibility visible to naked eye from Earth under favorable conditions

How these facts were elicited

Referenced by (3)

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

Mare Imbrium adjacentTo Mare Frigoris
Imbrium Basin ejecta zone extendsInto Mare Frigoris region
linked to: Mare Frigoris
Montes Alpes adjacentTo Mare Frigoris