南极洲奥特韦丘陵蓝冰区陨石中的宇宙放射性核素:一个不同寻常、保存完好的 H5 陨石散布区

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Kees C. Welten, Marc W. Caffee, Monika E. Kress, Marlene D. Giscard, A. J. Timothy Jull, Ralph P. Harvey, John Schutt
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引用次数: 0

摘要

美国南极陨石搜寻计划(ANSMET)在南极洲格罗夫纳山脉奥特韦山丘附近一块 1.6 × 0.3 平方公里的蓝冰区域(BIA)上发现了一个由 88 块普通陨石组成的密集群,总质量超过 100 千克。较大的块体(重达 29 千克)位于椭圆形图案的一端,较小的块体(50-200 克)位于另一端。我们测量了包括该陨石群的 14 块碎片在内的 17 块 H 型刚玉的金属部分中宇宙放射性核素 10Be(半衰期-1.36 × 106 年)和 36Cl(3.01 × 105 年)的浓度,以验证奥特韦山丘 BIA 上的这个陨石群是由一颗流星体在大气中碎裂而产生的陨石散落场的假设。10Be 和 36Cl 濃度證實,在這個小區域內不同地點的 14 塊 H 軟玉中,有 10 塊是同一個隕石墜落的成對碎片,而另外四塊 H 軟玉則代表另外兩個較小的隕石墜落。放射性核素表明,大配对组的陨石进入大气层前的质量为 200-400 千克,这表明有 25%-50%的陨石进入大气层后幸存了下来。根据成对的 H 型刚玉的分布以及它们在太空中共同的宇宙射线暴露历史的证据,我们得出结论,在这一小块区域内的 88 颗陨石中,大部分代表了一个陨石散落场。陨石散落区的面积较小,这表明陨石是以陡峭的角度(60°)进入的,而大多数陨石表面的熔壳数量较少,这很可能表明陨石是在低空被大气破碎的,而大块残存的碎片可能是在撞击冰层时发生了额外的破碎。这个有据可查的散落场为应用模型模拟该天体的大气碎裂与进入角度、速度和流星体强度的函数关系提供了一个很好的机会。对奥特威山丘配对群中的两个成员进行的 14C 宇宙成因分析得出了 15.5 ± 1.5 千年的地球年龄,这代表了这块陨石坠落地球后所经历的时间。南极陨石散落区保存完好,表明奥特威山丘 BIA 代表了一个相对停滞的蓝色冰原。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Cosmogenic radionuclides in meteorites from the Otway Massif blue ice area, Antarctica: An unusual, well-preserved H5 chondrite strewn field

Cosmogenic radionuclides in meteorites from the Otway Massif blue ice area, Antarctica: An unusual, well-preserved H5 chondrite strewn field

The US Antarctic Search for Meteorites (ANSMET) discovered a dense cluster of 88 ordinary chondrites with a total mass of more than 100 kg on a blue ice area (BIA) of 1.6 × 0.3 km2 near the Otway Massif, Grosvenor Mountains, Antarctica. The larger masses (weighing up to 29 kg) were found at one end of an oval-shaped pattern and the smaller masses (50–200 g) at the other end. We measured concentrations of the cosmogenic radionuclides 10Be (half-life—1.36 × 106 year) and 36Cl (3.01 × 105 year) in the metal fraction of 17 H chondrites, including 14 fragments of this cluster, to verify the hypothesis that this meteorite cluster on the Otway Massif BIA represents a meteorite strewn field produced by the atmospheric breakup of a single meteoroid. The 10Be and 36Cl concentrations confirm that 10 out of 14 H chondrites from different locations within this small area are paired fragments of the same meteorite fall, while the four other H chondrites represent two additional—smaller—falls. The radionuclides suggest a pre-atmospheric mass of 200–400 kg for the large pairing group, suggesting that 25%–50% of the meteoroid survived atmospheric entry. Based on the distribution of the paired H chondrites and evidence of their common cosmic-ray exposure history in space, we conclude that most of the 88 meteorites within this small area represent a meteorite strewn field. The small size of the strewn field suggests that the meteoroid entered at a steep angle (>60°), while the low amount of fusion crust on most meteorite surfaces most likely indicates atmospheric break up at low altitude, while additional fragmentation of a large surviving fragment may have occurred during impact on the ice. This well-documented strewn field provides a good opportunity to apply model simulations of the atmospheric fragmentation of this object as a function of entry angle, velocity, and meteoroid strength. Cosmogenic 14C analyses in two members of the Otway Massif pairing group yield a terrestrial age of 15.5 ± 1.5 kyr, which represents the time elapsed since this meteorite fell on Earth. The excellent preservation of an Antarctic meteorite strewn field suggests that the Otway Massif BIA represents a relatively stagnant blue ice field.

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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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