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过去 5 亿年小行星的解体和陨石撞击地球。

Asteroid break-ups and meteorite delivery to Earth the past 500 million years.

机构信息

Astrogeobiology Laboratory, Department of Physics, Lund University, 221 00 Lund, Sweden.

Astrogeobiology Laboratory, Department of Physics, Lund University, 221 00 Lund, Sweden;

出版信息

Proc Natl Acad Sci U S A. 2021 Jun 15;118(24). doi: 10.1073/pnas.2020977118.

DOI:10.1073/pnas.2020977118
PMID:34099566
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC8214677/
Abstract

The meteoritic material falling on Earth is believed to derive from large break-up or cratering events in the asteroid belt. The flux of extraterrestrial material would then vary in accordance with the timing of such asteroid family-forming events. In order to validate this, we investigated marine sediments representing 15 time-windows in the Phanerozoic for content of micrometeoritic relict chrome-spinel grains (>32 μm). We compare these data with the timing of the 15 largest break-up events involving chrome-spinel-bearing asteroids (S- and V-types). Unexpectedly, our Phanerozoic time windows show a stable flux dominated by ordinary chondrites similar to today's flux. Only in the mid-Ordovician, in connection with the break-up of the L-chondrite parent body, do we observe an anomalous micrometeorite regime with a two to three orders-of-magnitude increase in the flux of L-chondritic chrome-spinel grains to Earth. This corresponds to a one order-of-magnitude excess in the number of impact craters in the mid-Ordovician following the L-chondrite break-up, the only resolvable peak in Phanerozoic cratering rates indicative of an asteroid shower. We argue that meteorites and small (<1-km-sized) asteroids impacting Earth mainly sample a very small region of orbital space in the asteroid belt. This selectiveness has been remarkably stable over the past 500 Ma.

摘要

据信,落在地球上的陨石材料源自小行星带中大型天体分裂或撞击事件。那么,外星物质的通量将根据此类小行星族形成事件的时间而变化。为了验证这一点,我们研究了代表显生宙 15 个时间窗口的海洋沉积物,以研究其中残留的微米陨石铬尖晶石颗粒(>32μm)的含量。我们将这些数据与涉及含铬尖晶石小行星(S 型和 V 型)的 15 次最大分裂事件的时间进行了比较。出乎意料的是,我们在显生宙的时间窗口中观察到了一种稳定的通量,主要由普通球粒陨石组成,类似于今天的通量。仅在中奥陶世,与 L 型球粒陨石母体的分裂有关,我们观察到异常的微陨石状态,L 型球粒陨石铬尖晶石颗粒的通量增加了两到三个数量级,到达地球。这对应于 L 型球粒陨石分裂后中奥陶世撞击坑数量增加了一个数量级,这是显生宙撞击率中唯一可分辨的峰值,表明存在小行星雨。我们认为,撞击地球的陨石和小行星(<1 公里大小)主要从小行星带的轨道空间的一个非常小的区域进行采样。这种选择性在过去 5 亿年中一直非常稳定。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/1c84/8214677/6cc3a63e77a3/pnas.2020977118fig03.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/1c84/8214677/e2273bd3df7b/pnas.2020977118fig01.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/1c84/8214677/6282a03c223c/pnas.2020977118fig02.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/1c84/8214677/6cc3a63e77a3/pnas.2020977118fig03.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/1c84/8214677/e2273bd3df7b/pnas.2020977118fig01.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/1c84/8214677/6282a03c223c/pnas.2020977118fig02.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/1c84/8214677/6cc3a63e77a3/pnas.2020977118fig03.jpg

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本文引用的文献

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Earth's Impact Events Through Geologic Time: A List of Recommended Ages for Terrestrial Impact Structures and Deposits.地球地质时期的撞击事件:推荐的陆地撞击构造和沉积物年龄列表。
Astrobiology. 2020 Jan;20(1):91-141. doi: 10.1089/ast.2019.2085. Epub 2019 Dec 27.
2
An extraterrestrial trigger for the mid-Ordovician ice age: Dust from the breakup of the L-chondrite parent body.外星触发中奥陶世冰期:来自 L 球粒陨石母体破裂的尘埃。
Sci Adv. 2019 Sep 18;5(9):eaax4184. doi: 10.1126/sciadv.aax4184. eCollection 2019 Sep.
3
A new type of solar-system material recovered from Ordovician marine limestone.
从奥陶纪海洋石灰岩中回收的一种新型太阳系材料。
Nat Commun. 2016 Jun 14;7:ncomms11851. doi: 10.1038/ncomms11851.
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