Regolith migration on asteroid 101955 Bennu inferred from boulder alignment

被引:2
|
作者
Marshall, J. R. [1 ,2 ]
Beddingfield, C. [1 ,2 ]
Fenton, L. K. [1 ]
Walsh, K. J. [3 ]
Lauretta, D. S. [4 ]
机构
[1] SETI Inst, Mountain View, CA 94043 USA
[2] NASA Ames Res Ctr, Mountain View, CA USA
[3] Southwest Res Inst, San Antonio, TX USA
[4] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ USA
关键词
Asteroid Bennu; Regolith migration; Boulder alignment; Regolith stresses;
D O I
10.1016/j.pss.2023.105659
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The alignment of elongated-boulder long axes was measured for the surface regolith of asteroid Bennu in order to quantify patterns of regolith fabric that might shed light on the geophysical and geomorphological history of the asteroid. We found a preferred north-south alignment of boulder long-axis orientations in mid-latitudes +/--20 degrees-60 degrees suggesting that regolith is or has been migrating towards the equator following latitudinal lines. Our baseline premise is that migration is likely a manifestation of centrifugal forces resulting from Bennu's relatively high spin rate. From a comparison with terrestrial regolith analogs (colluvial materials) it is inferred that this alignment is indicative of a horizontally extensional stress state in mid latitudes. In contrast, we found a chaotic alignment of boulders in the equatorial latitudes +/--0 degrees-20 degrees implicating a compressional stress regime that has caused piling and upward accumulation of regolith to form part of, if not the whole of Bennu's equatorial ridge. Our observations of boulder alignments and analyses of regolith stresses lead us to the proposition that horizontal drift of regolith in latitudes +/--20-90 degrees is primarily driven by the localized balance between gravity and hori-zontal shear - whereas regolith drift in equatorial regions +/--0-20 degrees is driven primarily by shear forces trans-mitted longitudinally through boulder-to-boulder compressional contact.
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页数:7
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