Pairing and classification assessment of CM chondrites from the Meteorite Hills, Transantarctic Mountains

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
K. Righter, M. Welby, H. C. Bates, A. J. King, P. F. Schofield, J. Schutt, R. Harvey, J. Karner, B. Rougeux, K. Pando, C. Satterwhite
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引用次数: 0

Abstract

The Meteorite Hills dense collection area in the Transantarctic Mountains has yielded 1130 meteorites over several ANSMET field seasons. Twenty-three CM carbonaceous chondrites were recovered as part of the 2000–2001 and 2001–2002 field seasons. Many of these CMs have unique or rare features, but most are small (<50 g), making their preservation of highest priority, so material can be available for future researchers. One major contributor to preservation is knowing which samples are paired with others. Because CM chondrites are fine grained and petrographic features are subtle, standard petrography is not as helpful in classification. To strengthen the understanding of pairing and classification, we initiated a focused study of the 23 CM chondrites recovered from Meteorite Hills. Combining magnetic susceptibility (MS), modal mineralogy as determined using X-ray diffraction (XRD), and published information about a subset of samples, we have reassessed the classification and pairing. Many samples have MS log χ values between 3.7 and 3.9, but there are a few exceptions such as MET 00432 (4.85), MET 01076 and 77 (4.06 and 4.63, respectively), and MET 01073 (3.21). Fifteen of the samples exhibit intermediate to high levels of aqueous alteration with phyllosilicate fractions (PSF) of 0.88–0.93. A trio of samples exhibit even higher levels of alteration with PSFs of 0.96–0.98. Find locations and cosmic ray exposure (CRE) ages of these two groups are similar and the latter very short at 0.1–0.2 Ma, raising the possibility that they are all part of the same heterogeneous fall. Since the three heavily altered samples are rare and have distinctive mineralogy relative to other MET CMs, they should be preserved regardless of whether they are from one large fall or two separate falls. Two samples (MET 01076 and MET 01077) contain a much greater fraction of olivine and pyroxene, have longer CRE ages, and most likely are heated CM chondrites. Three samples are unpaired and have unique characteristics: MET 00432 has a high magnetite fraction and other mineralogical and chemical properties comparable to C2 ungrouped chondrites such as Tagish Lake and Tarda, while MET 001087 (PSF = 0.77) and MET 00633 (PSF = 0.76) are less aqueously altered than the other meteorites, with the former in particular showing a significant tochilinite peak in its XRD pattern. Although MET 00633 could arguably be part of the larger pairing group of samples given its similar find location, we recommend keeping it unpaired given its distinct mineralogy.

横贯南极山脉陨石山CM球粒陨石配对及分类评价
在横跨南极山脉的陨石山密集收集区,在ANSMET的几个野外季节里已经收集了1130颗陨石。在2000-2001年和2001-2002年的野外季节中,发现了23颗CM碳质球粒陨石。其中许多cm具有独特或罕见的特征,但大多数都很小(50克),因此保存它们的优先级最高,因此材料可以为未来的研究人员提供。保存的一个主要因素是知道哪些样本与其他样本配对。由于CM球粒陨石颗粒细,岩石学特征不明显,标准岩石学对分类的帮助不大。为了加强对配对和分类的理解,我们对从Meteorite Hills回收的23颗CM球粒陨石进行了重点研究。结合磁化率(MS)、使用x射线衍射(XRD)确定的模态矿物学,以及关于样品子集的公开信息,我们重新评估了分类和配对。许多样本的MS log χ值在3.7和3.9之间,但也有一些例外,如MET 00432 (4.85), MET 01076和77(分别为4.06和4.63),以及MET 01073(3.21)。15个样品表现出中高水平的水蚀变,层状硅酸盐组分(PSF)为0.88-0.93。三个样本显示出更高水平的变化,psf为0.96-0.98。发现这两组的位置和宇宙射线暴露(CRE)年龄相似,后者非常短,在0.1-0.2 Ma之间,这提高了它们都是同一异质下降的可能性。由于这三个严重蚀变的样品非常罕见,并且相对于其他MET cm具有独特的矿物学特征,因此无论它们是来自一个大瀑布还是两个单独的瀑布,都应该保存下来。两个样品(MET 01076和MET 01077)含有更多的橄榄石和辉石,具有更长的CRE年龄,并且很可能是加热的CM球粒陨石。MET 00432具有较高的磁铁矿分数和其他矿物学和化学性质,与塔吉什湖和塔尔达等C2未分组球粒陨石相当,而MET 001087 (PSF = 0.77)和MET 00633 (PSF = 0.76)的水蚀作用比其他陨石少,其中MET 001087 (PSF = 0.76)在其XRD谱图中表现出明显的毒力石峰。尽管MET 00633可能是更大的配对样本组的一部分,因为它的发现位置相似,我们建议保持不配对,因为它的矿物学不同。
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来源期刊
Meteoritics & Planetary Science
Meteoritics & Planetary Science 地学天文-地球化学与地球物理
CiteScore
3.90
自引率
31.80%
发文量
121
审稿时长
3 months
期刊介绍: First issued in 1953, the journal publishes research articles describing the latest results of new studies, invited reviews of major topics in planetary science, editorials on issues of current interest in the field, and book reviews. The publications are original, not considered for publication elsewhere, and undergo peer-review. The topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors, and meteorites, asteroids, comets, craters, and tektites. Our authors and editors are professional scientists representing numerous disciplines, including astronomy, astrophysics, physics, geophysics, chemistry, isotope geochemistry, mineralogy, earth science, geology, and biology. MAPS has subscribers in over 40 countries. Fifty percent of MAPS'' readers are based outside the USA. The journal is available in hard copy and online.
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