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Journal Articles Journal of Geophysical Research: Planets Year : 2022

The Formation of Terraces on Asteroid (101955) Bennu

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O. S. Barnouin
  • Function : Author
M. G. Daly
  • Function : Author
J. A. Seabrook
  • Function : Author
P. Michel
J. H. Roberts
  • Function : Author
R. T. Daly
  • Function : Author
M. E. Perry
  • Function : Author
H. C. M. Susorney
  • Function : Author
E. R. Jawin
  • Function : Author
R. -L. Ballouz
  • Function : Author
K. J. Walsh
  • Function : Author
M. M. Sevalia
  • Function : Author
M. M. Al Asad
  • Function : Author
C. L. Johnson
  • Function : Author
E. B. Bierhaus
  • Function : Author
R. W. Gaskell
  • Function : Author
E. E. Palmer
  • Function : Author
J. Weirich
  • Function : Author
B. Rizk
C. Y. Drouet d'Aubigny
  • Function : Author
M. C. Nolan
  • Function : Author
D. N. Dellagiustina
  • Function : Author
D. J. Scheeres
  • Function : Author
J. W. Mcmahon
  • Function : Author
H. C. Connolly
  • Function : Author
D. C. Richardson
  • Function : Author
C. W. V. Wolner
  • Function : Author
D. S. Lauretta
  • Function : Author

Abstract

The surface of the rubble-pile asteroid (101955) Bennu has been characterized in detail by the OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, and Security-Regolith Explorer) mission. By examining global and local digital terrain models, we observed that Bennu possesses terraces, that is, a series of roughly latitude-parallel, step-like slope breaks. These partially circumscribe the poles and extend east-west over several longitudinal quadrants at mid- to high (≥30°) latitudes. The terraces are subtle in amplitude, with heights ranging from 1 to 5 m. They often exhibit back-wasting that results in V-shaped scarps that open downslope in some locations. When boulders >5-10 m are absent at or near a terrace, the steeper portion (the drop) of the terrace lacks rocks, whereas the flatter portion (the bench) of the terrace has accumulations of rocks at its crest. When boulders >5-10 m are present, their steep downslope faces often make up the drop from the terrace crest, and they retain debris upslope, thereby enhancing the terrace structure. A geotechnical stability analysis indicates that Bennu's surface is likely unstable and that surface cohesion is <0.6 Pa. Bennu's terraces strongly resemble scarps generated in laboratory and numerical simulations of a cohesionless granular bed as the slope of the bed increases quasi-statically. We conclude that terraces are probably actively forming on Bennu as its surface slowly fails owing to creep induced by spin acceleration.
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Dates and versions

insu-03656900 , version 1 (02-05-2022)

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Attribution - CC BY 4.0

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O. S. Barnouin, M. G. Daly, J. A. Seabrook, Y. Zhang, F. Thuillet, et al.. The Formation of Terraces on Asteroid (101955) Bennu. Journal of Geophysical Research: Planets, 2022, 127, ⟨10.1029/2021JE006927⟩. ⟨insu-03656900⟩
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