howardite
Quick Summary
A howardite is a type of stony meteorite composed primarily of anorthite, olivine, and bronzite. Meteorites are remnants from the early solar system, offering insights into its formation and evolution. Achondrites, which include howardites, are stony meteorites that lack chondrules, small spherical objects formed in the solar nebula. Howardites, along with eucrites and diogenites, are believed to originate from the asteroid Vesta. These meteorites provide valuable clues about the conditions and processes that occurred in the early solar nebula.1234
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achondritediogenites, eucrites, howardites, lodranites, nakhlites, shergottites, and ureilites. The howardites, eucrites, and diogenites (HEDs) are from the large asteroid Vesta. The shergottites, nakhlites, and chassignites almost certainly came from Mars. In addition, a small group of achondrites are believed to be derived from the
Read Morediogenites, eucrites, howardites, lodranites, nakhlites, shergottites, and ureilites. The howardites, eucrites, and diogenites (HEDs) are from the large asteroid Vesta. The shergottites, nakhlites, and chassignites almost certainly came from Mars. In addition, a small group of achondrites are believed to be derived from the
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meteoriteAchondritesThe howardite, eucrite, and diogenite (HED) meteorites all came from the same asteroidal body, Vesta, the second largest member of the asteroid belt. They have also been linked to the mesosiderites, a group of stony iron meteorites (see below Association
Read MoreThe howardite, eucrite, and diogenite (HED) meteorites all came from the same asteroidal body, Vesta, the second largest member of the asteroid belt. They have also been linked to the mesosiderites, a group of stony iron meteorites (see below Association
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