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利用雷达探测发现了萨特尔米尔陨石,这是一块碳质球粒陨石风化层角砾岩。

Radar-enabled recovery of the Sutter's Mill meteorite, a carbonaceous chondrite regolith breccia.

机构信息

SETI Institute, Mountain View, CA 94043, USA.

出版信息

Science. 2012 Dec 21;338(6114):1583-7. doi: 10.1126/science.1227163.

Abstract

Doppler weather radar imaging enabled the rapid recovery of the Sutter's Mill meteorite after a rare 4-kiloton of TNT-equivalent asteroid impact over the foothills of the Sierra Nevada in northern California. The recovered meteorites survived a record high-speed entry of 28.6 kilometers per second from an orbit close to that of Jupiter-family comets (Tisserand's parameter = 2.8 ± 0.3). Sutter's Mill is a regolith breccia composed of CM (Mighei)-type carbonaceous chondrite and highly reduced xenolithic materials. It exhibits considerable diversity of mineralogy, petrography, and isotope and organic chemistry, resulting from a complex formation history of the parent body surface. That diversity is quickly masked by alteration once in the terrestrial environment but will need to be considered when samples returned by missions to C-class asteroids are interpreted.

摘要

多普勒天气雷达成像是在加利福尼亚州内华达山脉山麓发生罕见的 4 千吨 TNT 当量小行星撞击后,快速找回萨特米尔陨石的关键。这些陨石在以接近木星族彗星(提泽兰德参数=2.8±0.3)的轨道高速进入地球时幸存下来,速度达到了创纪录的每秒 28.6 公里。萨特米尔陨石是一种由 CM(米吉希)型碳质球粒陨石和高度还原的异质材料组成的表土角砾岩。它显示出矿物学、岩石学、同位素和有机化学的巨大多样性,这是母体表面复杂形成历史的结果。一旦进入地球环境,这种多样性就会迅速被改变所掩盖,但在解释任务返回 C 类小行星样本时需要加以考虑。

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