日本地球惑星科学連合2021年大会

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[E] 口頭発表

セッション記号 P (宇宙惑星科学) » P-PS 惑星科学

[P-PS03] Regolith Science

2021年6月5日(土) 13:45 〜 15:15 Ch.04 (Zoom会場04)

コンビーナ:和田 浩二(千葉工業大学惑星探査研究センター)、中村 昭子(神戸大学大学院理学研究科)、Patrick Michel(Universite Cote D Azur Observatoire De La Cote D Azur CNRS Laboratoire Lagrange)、John Kevin Walsh(Southwest Research Institute Boulder)、座長:坂谷 尚哉(立教大学 理学部 物理学科)

14:00 〜 14:15

[PPS03-02] Dust cloud mass from OSIRIS-REx sample collection event at Bennu

★Invited Papers

*Bashar Rizk1、Kevin J. Walsh2、Ronald Ballouz1、Brent Bos3、Christian Drouet d'Aubigny1 (1.University of Arizona、2.Southwest Research Institute、3.Goddard Space Flight Center)

キーワード:Regolith, Bennu, TAG, Dust, Sampling, Contamination

The high-pressure gas released during the OSIRIS-REx sampling event, on 20 October 2020, lofted a cloud of sub-millimeter and smaller particles from the surface of asteroid Bennu . We attempted to determine the mass of this sub-millimeter dust cloud, and its initial layer thickness. The analysis relied on two images acquired before and after the event agitated Bennu’s regolith at Nightingale, the sampling site. We measured the optical depth of the expanding cloud as a function of distance from the center of the expansion during the moment of sample acquisition. Specific values of mass and thickness relied on simplifying assumptions and varied with particle size. We integrated the imaged profile of radially varying optical depth to significantly narrow, or even collapse, the range of average optical depth. We recruited observations from other instruments and analyses to do the same for particle size. With our result, we hope to constrain the nature of the microphysical environment at and near the surface of Bennu’s regolith by establishing the presence, or confirming the absence, of a population of sub-millimeter particles and measuring its magnitude.