Grove Mountains (GRV) 020043

Insights into acapulcoite-lodranite genesis from the most primitive member

Timothy J. McCoy, Catherine M. Corrigan, Tamara L. Dickinson, Gretchen K. Benedix, Devin Schrader, Jemma Davidson

Research output: Contribution to journalArticle

Abstract

Although acapulcoites and lodranites played a key role in understanding partial differentiation of asteroids, the lack of samples of the chondritic precursor limits our understanding of the processes that formed these meteorites. Grove Mountains (GRV) 020043 is a type 4 chondrite, with abundant, well-delineated, pyroxene-rich chondrules with an average diameter of 690 μm, microcrystalline mesostasis, polysynthetically striated low-Ca pyroxene, and slightly heterogeneous plagioclase compositions. Similarities in mineralogy, mineral composition, and oxygen isotopic composition link GRV 020043 to the acapulcoite-lodranite clan. These features include a high low-Ca pyroxene to olivine ratio, high kamacite to taenite ratio, and relatively FeO-poor mafic silicates (Fa10.3, Fs10.4) relative to ordinary chondrites, as well as the presence of ubiquitous metal and sulfide inclusions in low-Ca pyroxene and ƒO2 typical of acapulcoites. GRV 020043 shows that evidence of partial melting is not an essential feature for classification within the acapulcoite-lodranite clan. GRV 020043 experienced modest thermal metamorphism similar to type 4 ordinary chondrites. GRV 020043 suggests a range of peak temperatures on the acapulcoite-lodranite parent body similar to that of ordinary chondrites, but shifted to higher temperatures, perhaps consistent with earlier accretion. The mineralogy and mineral compositions of GRV 020043, despite modest thermal metamorphism, suggests that most features of acapulcoites previously attributed to reduction were, instead, inherited from the precursor chondrite. Although partial melting was widespread on the acapulcoite-lodranite parent body, ubiquitous Fe,Ni-FeS blebs in the cores of silicates were not implanted by shock or trapped during silicate melting, but were inherited from the precursor chondrite with subsequent overgrowths during metamorphism.

Original languageEnglish (US)
Article number125536
JournalChemie der Erde
DOIs
StateAccepted/In press - Jan 1 2019

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acapulcoite
chondrites
mountains
Silicates
pyroxene
Melting
ordinary chondrite
mountain
Mineralogy
Chemical analysis
chondrite
Minerals
silicates
metamorphism
silicate
parent body
melting
mineralogy
Meteorites
Asteroids

Keywords

  • Acapulcoite
  • Asteroid
  • Chondrite
  • Melting
  • Meteorite
  • Mineralogy
  • Petrology

ASJC Scopus subject areas

  • Geophysics
  • Geochemistry and Petrology

Cite this

Grove Mountains (GRV) 020043 : Insights into acapulcoite-lodranite genesis from the most primitive member. / McCoy, Timothy J.; Corrigan, Catherine M.; Dickinson, Tamara L.; Benedix, Gretchen K.; Schrader, Devin; Davidson, Jemma.

In: Chemie der Erde, 01.01.2019.

Research output: Contribution to journalArticle

McCoy, Timothy J. ; Corrigan, Catherine M. ; Dickinson, Tamara L. ; Benedix, Gretchen K. ; Schrader, Devin ; Davidson, Jemma. / Grove Mountains (GRV) 020043 : Insights into acapulcoite-lodranite genesis from the most primitive member. In: Chemie der Erde. 2019.
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AB - Although acapulcoites and lodranites played a key role in understanding partial differentiation of asteroids, the lack of samples of the chondritic precursor limits our understanding of the processes that formed these meteorites. Grove Mountains (GRV) 020043 is a type 4 chondrite, with abundant, well-delineated, pyroxene-rich chondrules with an average diameter of 690 μm, microcrystalline mesostasis, polysynthetically striated low-Ca pyroxene, and slightly heterogeneous plagioclase compositions. Similarities in mineralogy, mineral composition, and oxygen isotopic composition link GRV 020043 to the acapulcoite-lodranite clan. These features include a high low-Ca pyroxene to olivine ratio, high kamacite to taenite ratio, and relatively FeO-poor mafic silicates (Fa10.3, Fs10.4) relative to ordinary chondrites, as well as the presence of ubiquitous metal and sulfide inclusions in low-Ca pyroxene and ƒO2 typical of acapulcoites. GRV 020043 shows that evidence of partial melting is not an essential feature for classification within the acapulcoite-lodranite clan. GRV 020043 experienced modest thermal metamorphism similar to type 4 ordinary chondrites. GRV 020043 suggests a range of peak temperatures on the acapulcoite-lodranite parent body similar to that of ordinary chondrites, but shifted to higher temperatures, perhaps consistent with earlier accretion. The mineralogy and mineral compositions of GRV 020043, despite modest thermal metamorphism, suggests that most features of acapulcoites previously attributed to reduction were, instead, inherited from the precursor chondrite. Although partial melting was widespread on the acapulcoite-lodranite parent body, ubiquitous Fe,Ni-FeS blebs in the cores of silicates were not implanted by shock or trapped during silicate melting, but were inherited from the precursor chondrite with subsequent overgrowths during metamorphism.

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