Pyroxene pallasite grouplet explained

Subdivision:Grouplet
Pyroxene pallasite grouplet
Type:Stony-iron
Class:Pallasite
Subgroups: -->
Composition:Meteoric iron, silicate minerals (pyroxene)
Number Of Specimens:2

The pyroxene pallasite grouplet is a subdivision of the pallasite meteorites (stony-irons).[1]

The grouplet is named "pyroxene pallasites" because they are the only pallasites that contain pyroxene. The grouplet was proposed in 1995.[2] It currently has only two members: the Vermillion and Yamato 8451 meteorite. Both meteorites contain pyroxene and have a number of other similarities: for example their pyroxene composition, rare-earth element concentrations, and oxygen isotope ratios. However, there are also indicators against the grouping of these two meteorites: for example the texture and occurrence of cohenite in the Vermillion meteorite and the differing siderophile trace element concentrations.[2]

See also

Notes and References

  1. Book: D. S. Lauretta . H. Y. McSween, Jr.. Meteorites and the early solar system II. 2006. University of Arizona Press. Tucson. 978-0816525621. http://haroldconnolly.com/EES%20716%20Fall%2009%20Reading/Lecture%201/Background%20reading/Weisberg_etal_MESSII.pdf. M. K. Weisberg. T. J. McCoy, A. N. Krot. 15 December 2012. 19–52. Systematics and Evaluation of Meteorite Classification.
  2. Boesenberg. Joseph S.. Davis, Andrew M. . Prinz, Martin . Weisberg, Michael K. . Clayton, Robert N. . Mayeda, Toshiko K. . Toshiko Mayeda . The pyroxene pallasites, Vermillion and Yamato 8451: Not quite a couple. Meteoritics & Planetary Science. 1 July 2000. 35. 4. 757–769. 10.1111/j.1945-5100.2000.tb01460.x. free.