Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

Eucrite

From Wikipedia, the free encyclopedia
Achondritic stony meteorite
This articleneeds additional citations forverification. Please helpimprove this article byadding citations to reliable sources. Unsourced material may be challenged and removed.
Find sources: "Eucrite" – news ·newspapers ·books ·scholar ·JSTOR
(July 2017) (Learn how and when to remove this message)
This articlemay be too technical for most readers to understand. Pleasehelp improve it tomake it understandable to non-experts, without removing the technical details.(July 2017) (Learn how and when to remove this message)
Eucrite
— Group —
Stannern eucrite, found in the Czech Republic.
Compositional typeStony
TypeAchondrite
ClassAsteroidal achondrite
ClanHED meteorite
Subgroups
  • Non-cumulate eucrites
    • Main series eucrites
    • Stannern trend eucrites
    • Nuevo Laredo trend eucrites
  • Cumulate eucrites
  • Polymict eucrites
Parent body4 Vesta and others
CompositionBasaltic rock, mostlyCalcium-poorpyroxene,pigeonite, and Calcium-richplagioclase (anorthite)
Total known specimens>100
GRA98033 abrecciated eucrite about 5 cm across, found in the Graves Nunataks region of Antarctica.

Eucrites areachondritic stonymeteorites, many of which originate from the surface of theasteroid4 Vesta and are part of theHED meteorite clan. They are the most common achondrite group with over 100 meteorites found.

Eucrites consist ofbasaltic rock from thecrust of4 Vesta or a similar parent body. They are mostly composed ofcalcium-poorpyroxene,pigeonite, and calcium-richplagioclase (anorthite).[1]

Based on differences of chemical composition and features of the component crystals, they are subdivided into several groups:[2]

  • Non-cumulate eucrites are the most common variety and can be subdivided further:
    • Main series eucrites formed near the surface and are mostlyregolithbrecciaslithified under the pressure of overlying newer deposits.
    • Stannern trend eucrites are a rare variety.
    • Nuevo Laredo trend eucrites are thought to come from deeper layers of 4 Vesta's crust, and are a transition group towards the cumulate eucrites.
  • Cumulate eucrites are rare types with oriented crystals, thought to have solidified in magma chambers deep within4 Vesta's crust.
  • Polymict eucrites areregolithbreccias consisting of mostly eucrite fragments and less than one part in ten ofdiogenite. They are less common.

Etymology

[edit]

Eucrites get their name from the Greek wordeukritos meaning "easily distinguished". This refers to the silicate minerals in them, which can be easily distinguished because of their relatively large grain size.

Eucrite is also a now obsolete term forbytownite-gabbro, anigneous rock formed in the Earth'scrust. The term was used as a rock type name for some of thePaleogene igneous rocks ofScotland.[3]

See also

[edit]

References

[edit]
  1. ^B. Mason: Meteorites. John Wiley, New York 1962.
  2. ^Mittlefehldt, McCoy, Goodrich and Kracher: Non-chondritic Meteorites from Asteroidal Bodies, In: Reviews in Mineralogy Vol. 36, Planetary Materials, Mineralogical Society of America, 1998.
  3. ^Sutherland, D. S. (1982)Igneous Rocks of the British Isles, Chichester, John Wiley, page 536.

External links

[edit]
Meteorite...
Classification
Bytype,class,
clan,group
andgrouplet
Chondrite
Achondrite
Primitive
Asteroidal
Lunar
Martian
Iron
Stony-iron
Structural
Obsolete terms
Mineralogy
andpetrology
Lists
Retrieved from "https://en.wikipedia.org/w/index.php?title=Eucrite&oldid=1112927479"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp