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Howardites are achondritic stony meteorites that originate from the surface of the asteroid 4 Vesta, and as such are part of the HED meteorite clan. There are about 200 distinct members known.

Key facts

Meteorite subdivision.Subdivision
Group
Meteorite subdivision.Name
Howardite
Meteorite subdivision.Image
Howardite QUE94200.gif
Meteorite subdivision.Image_caption
QUE94200, a Howardite about across, found in the Queen Alexandra Range in Antarctica.
Meteorite subdivision.Compositional_type
Stony
Meteorite subdivision.Type
Achondrite
Meteorite subdivision.Class
Asteroidal achondrite
Meteorite subdivision.Clan
HED meteorite <!-- list/link all subgroups of this group as a
Meteorite subdivision.Subgroups
-->
Meteorite subdivision.Parent_body
4 Vesta
Meteorite subdivision.Number_of_specimens
~200

via Wikipedia infobox

Wikidata facts

Image
NWA 5489 howardite meteorite.jpg
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Commons category
Howardites
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Article

5 sections
Contents
  • Characteristics
  • Name
  • See also
  • References
  • External links

Howardites are achondritic stony meteorites that originate from the surface of the asteroid 4 Vesta, and as such are part of the HED meteorite clan. There are about 200 distinct members known.

==Characteristics== They are a regolith breccia consisting mostly of eucrite and diogenite fragments, although carbonaceous chondrules and impact melt can also occur. The rock formed from impact ejecta which was later buried by newer impacts and lithified due to the pressure from overlying layers. Regolith breccias are not found on Earth due to a lack of regolith on bodies which have an atmosphere.

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