Skip to content
EntityQ747347· pop 11· linked from 319 articles

Also known as angrites

Angrites are a rare group of achondrites consisting mostly of Al-Ti bearing diopside, hedenbergite, olivine, anorthite and troilite with minor traces of phosphate and metals. The group is named for the Angra dos Reis meteorite. They are the oldest igneous rocks, with crystallization ages of around 4.56 billion years. Angrites are subdivided into two main groups, the quenched and plutonic angrites. The quenched angrites cooled rapidly upon the surface of the angrite parent body (APB), whereas the plutonic angrites cooled slower, deeper in the crust. The APB is thought to have been a similar siz

Key facts

Meteorite subdivision.Subdivision
Group
Meteorite subdivision.Name
Angrite
Meteorite subdivision.Image
NWA 2999 meteorite, angrite.jpg
Meteorite subdivision.Image_caption
A slice of NWA 2999. Note the similarity to a terrestrial basalt.
Meteorite subdivision.Compositional_type
Stony meteorite
Meteorite subdivision.Type
Achondrite
Meteorite subdivision.Clan
<!-- list/link all subgroups of this group as a
Meteorite subdivision.Subgroups
Quenched Plutonic
Meteorite subdivision.Parent_body
Possibly 289 Nenetta, 3819 Robinson or Mercury
Meteorite subdivision.Number_of_specimens
30+

via Wikipedia infobox

Wikidata facts

Image
D'Orbigny meteorite, fragment.jpg
Show 1 more fact
Commons category
Angrites
Sources (1)

via Wikidata · CC0

~2 min read

Article

5 sections
Contents
  • Origin
  • Notable meteorites
  • See also
  • External links
  • References

Angrites are a rare group of achondrites consisting mostly of Al-Ti bearing diopside, hedenbergite, olivine, anorthite and troilite with minor traces of phosphate and metals. The group is named for the Angra dos Reis meteorite. They are the oldest igneous rocks, with crystallization ages of around 4.56 billion years. Angrites are subdivided into two main groups, the quenched and plutonic angrites. The quenched angrites cooled rapidly upon the surface of the angrite parent body (APB), whereas the plutonic angrites cooled slower, deeper in the crust. The APB is thought to have been a similar size to the asteroid 4 Vesta.

==Origin== Angrite meteorites are distinct from other meteoritic groups based on their oxygen isotopic compositions. Based on their Mn-Fe ratios in pyroxene and other isotopic compositions, the source of angrites is constrained to the inner Solar System. However, recent studies have suggested that the APB experienced mixing of multiple sources during its history.

Available in 10 languages

via Wikidata sitelinks · CC0

Connections

Categories