| 词条 | Primitive achondrite |
| 释义 |
|Subdivision = Class |Name = Primitive achondrites |Alternative_names = |Image = NWA 3151 meteorite, brachinite.jpg |Image_caption = Slice of a brachinite meteorite (Northwest Africa 3151) |Type = Achondrite |Class = |Clan = |Subgroups = {{flatlist|
}} |Structural_classification = |Parent_body = Various |Composition = Heterogeneous |Petrologic_type = |Number_of_specimens = |TKW = |Image2 = |Image2_caption = }}Primitive achondrites are a subdivision of meteorites. They are classified on the same rank (historically called "Class") and lying between chondrites and achondrites. They are called primitive because they are achondrites that have retained much of their original chondritic properties. Very characteristic are relic chondrules and chemical compositions close to the composition of chondrites. These observations are explained as melt residues, partial melting, or extensive recrystallization.[1][1] HistoryThe concept of primitive achondrites was first summarized in 1983.[2] In 2006 a classification was published that assigned 7 groups to the primitive achondrites, but the classification remains controversial. The authors define primitive achondrites as meteorites "that exceeded their solidus temperature on the parent body" and thus would partially melt. Meteorites that have been fully melted are included if they did not reach isotopic equilibrium on their parent body.[1] DescriptionThere are many indicators why some achondrites are deemed primitive. Some contain relic chondrules (e.g. Acapulcoite, Lodranite) and some have oxygen isotope ratios that are similar to chondrites. There are similarities in trace element concentrations between primitive achondrites and chondrites. A textural indicator can be observed in petrographic thin sections. If an achondrite is primitive it formed through recrystallization and will have many 120° grain boundaries. Normal achondrites form by crystallizing from a magma and will show magmatic textures.[1] Lodranites are for example seen as residues of partial melting, while acapulcoites are seen as partial melts, but both were produced by partial melting. Ureileites and brachinites remain uncertain and could either be explained as residues or cumulates.[1] SubdivisionsThe following groups are assigned to the primitive achondrites:[3]
See also
References1. ^1 {{cite journal|last=Pilski|first=Andrzej S.|author2=Tadeusz A. Przylibski |author3=Katarzyna Łuszczek |title=Primitive Enstatite Achondrites|journal=Meteorites|year=2011|volume=0|url=http://meteorites.pwr.wroc.pl/issues/0/meteorites00-02.pdf|accessdate=30 December 2012}} {{meteorites}}2. ^{{cite journal|last=Prinz|first=M.|author2=C. E. nehru |author3=J. S. Delaney |author4=M. Weisberg |title=Silicates in IAB and IIICD irons, winonaites, lodranites and Brachina: A primitive and modified primitive group (abstract)|journal=Lunar and Planetary Science|year=1983|volume=14|series=616-617|url=http://www.lpi.usra.edu/meetings/lpsc1983/pdf/1312.pdf|accessdate=30 December 2012}} 3. ^1 2 3 {{cite book|editor=D. S. Lauretta |editor2=H. Y. McSween Jr.|title=Meteorites and the early solar system II|year=2006|publisher=University of Arizona Press|location=Tucson|isbn=978-0816525621|url=http://haroldconnolly.com/EES%20716%20Fall%2009%20Reading/Lecture%201/Background%20reading/Weisberg_etal_MESSII.pdf|author=M. K. Weisberg|author2=T. J. McCoy|author3=A. N. Krot|accessdate=15 December 2012|pages=19–52|chapter=Systematics and Evaluation of Meteorite Classification}} 1 : Achondrite meteorites |
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