The secondary classification of unequilibrated chondrites

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Emmanuel Jacquet, Béatrice Doisneau
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引用次数: 0

Abstract

The multiplication of decimal petrologic schemes for different or the same chondrite groups evinces a lack of unified guiding principle in the secondary classification of type 1–3 chondrites. We show that the current OC, R and CO classifications can be a posteriori unified, with only minor reclassifications, if the decimal part of the subtype is defined as the ratio m = FaI/FaII of the mean fayalite contents of type I and type II chondrules, rounded to the nearest tenth (with adaptations from Cr systematics for the lowest subtypes following the past literature). This parameter is more efficiently evaluable than the oft-used relative standard deviation of fayalite contents and defines a general metamorphic scale from M0.0 to M1, where the suffixed number is the rounded m. Type 3 chondrites thus span the range M0.0–M0.9 (i.e. subtypes 3.0–3.9) and M1 designates type 4. Corresponding applications are then proposed for other chondrite groups (with, e.g., CV secondary classification reduced to essentially three grades from M0.0 to M0.2, that is, subtypes 3.0–3.2). Known type 1 and 2 chondrites are at M0.0 (i.e. the metamorphic grade of type 3.0 chondrites), even so-called “CY” chondrites, since our metamorphic scale is insensitive to brief heating. Independently, we define an aqueous alteration scale from A0.0 to A1.0, where the suffixed number is the (rounded) phyllosilicate fraction (PSF). For CM and CR chondrites, the alteration degrees can be characterized in terms of the thin-section-based criteria of previous schemes which are thus incorporated in the present framework, if in a coarser, but hereby more robust form. We propose their corresponding petrologic subtype to be 3-PSF, rounded to the nearest tenth (so that type 1 would correspond to subtypes 2.0 and 2.1). Since nonzero alteration and metamorphic degrees remain mutually exclusive at the level of precision chosen, a single petrologic subtype ≈3+m-PSF indeed remains a good descriptor of secondary processes for all unequilibrated chondrites, obviating the explicit mention of our separate scales unless finer subdivisions are adopted for the most primitive chondrites.

Abstract Image

非平衡球粒陨石的二级分类
不同或相同球粒陨石群的十进制岩石学方案的乘法表明1-3型球粒陨石的二级分类缺乏统一的指导原则。我们表明,如果亚型的小数点部分定义为I型和II型球粒的平均含铁量的比值m = FaI/FaII,那么当前的OC、R和CO分类可以是后检统一的,只有少量的重新分类,四舍五入到最接近的十分之一(根据过去的文献,对最低亚型的Cr系统学进行了改编)。这一参数比常用的球粒石含量的相对标准偏差更有效地进行评估,并定义了一个从M0.0到M1的一般变质尺度,其中后缀的数字是四舍四入的m。因此,3型球粒陨石的范围为M0.0 - m0.9(即3.0-3.9亚型),M1表示4型。然后,对其他球粒陨石群提出了相应的应用(例如,CV二级分类从M0.0到M0.2基本上减少到三个等级,即3.0-3.2亚型)。已知的1型和2型球粒陨石在M0.0(即3.0型球粒陨石的变质等级),甚至是所谓的“CY”球粒陨石,因为我们的变质尺度对短暂加热不敏感。独立地,我们定义了A0.0 ~ A1.0的含水蚀变标度,其中后缀数为(四舍五入的)层状硅酸盐分数(PSF)。对于CM和CR球粒陨石,蚀变程度可以根据先前方案的基于薄截面的标准来表征,从而纳入本框架,如果以更粗糙,但因此更健壮的形式。我们认为它们对应的岩石学亚型为3-PSF,四舍五入到最接近的十分之一(因此1型对应于2.0和2.1亚型)。由于非零蚀变和变质程度在选择的精度水平上仍然是相互排斥的,因此单一岩石学亚类型≈3+m-PSF确实仍然是所有不平衡球粒陨石的二次过程的良好描述,除非对最原始的球粒陨石采用更精细的细分,否则避免明确提及我们的单独尺度。
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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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