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Which meteorites have been identified as coming from the Moon, Mars, and Vesta?

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Meteor and meteoroid The Cabin Creek meteorite, an iron (nickel-iron alloy) meteorite that was observed to fall in northwestern Arkansas on March 27, 1886. Its characteristic pattern of “thumbprint” dimples, or regmaglypts, is the result of melting and consequent ablation of its surface as it traveled through the atmosphere. The meteorite is likely a fragment of one of the M class asteroids, which show significant nickel-iron in their surface material.

Meteorites identified as originating from the Moon, Mars, and the asteroid Vesta are classified as achondrites, a group of meteorites that have undergone igneous processing.1

Vesta

The asteroid Vesta is the parent body of the HED meteorite group, which consists of howardite, eucrite, and diogenite meteorites. These rocks provide evidence of Vesta's complex geological history, including melting, crystallization, and impact brecciation.12

Mars

Martian meteorites are volcanic rocks often referred to as SNCs, named after their three primary classes: shergottites, nakhlites, and chassignites. Their origin was confirmed by matching trapped gases within the rocks to the Martian atmosphere measured by Viking landers. A notable specimen is ALH84001, which has been the subject of significant scientific study and debate.13

The Moon

Lunar meteorites are fragments ejected from the Moon by large impacts. They resemble rock types collected during the Apollo and Luna missions, such as mare basalts and highland breccias, but are believed to originate from areas not sampled by those missions.1