Spectral slope variations for OSIRIS-REx target Asteroid (101955) Bennu: Possible evidence for a fine-grained regolith equatorial ridge

Richard P. Binzel, Francesca E. DeMeo, Brian J. Burt, Edward A. Cloutis, Ben Rozitis, Thomas H. Burbine, Humberto Campins, Beth Ellen Clark, Joshua P. Emery, Carl W. Hergenrother, Ellen S. Howell, Dante Lauretta, Michael C. Nolan, Megan Mansfield, Valerie Pietrasz, David Polishook, Daniel J. Scheeres

Research output: Contribution to journalArticle

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Abstract

Ongoing spectroscopic reconnaissance of the OSIRIS-REx target Asteroid (101955) Bennu was performed in July 2011 and May 2012. Near-infrared spectra taken during these apparitions display slightly more positive ("redder") spectral slopes than most previously reported measurements. While observational systematic effects can produce such slope changes, and these effects cannot be ruled out, we entertain the hypothesis that the measurements are correct. Under this assumption, we present laboratory measurements investigating a plausible explanation that positive spectral slopes indicate a finer grain size for the most directly observed sub-Earth region on the asteroid. In all cases, the positive spectral slopes correspond to sub-Earth latitudes nearest to the equatorial ridge of Bennu. If confirmed by OSIRIS-REx in situ observations, one possible physical implication is that if the equatorial ridge is created by regolith migration during episodes of rapid rotation, that migration is most strongly dominated by finer grain material. Alternatively, after formation of the ridge (by regolith of any size distribution), larger-sized equatorial material may be more subject to loss due to centrifugal acceleration relative to finer grain material, where cohesive forces can preferentially retain the finest fraction (Rozitis, B., Maclennan, E., Emery, J.P. [2014]. Nature 512, 174-176).

Original languageEnglish (US)
Pages (from-to)22-29
Number of pages8
JournalIcarus
Volume256
DOIs
StatePublished - Aug 1 2015

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OSIRIS
regolith
asteroids
asteroid
ridges
slopes
reconnaissance
near infrared
infrared spectra
grain size
material
effect

Keywords

  • Asteroids
  • Asteroids, surfaces
  • Regolith
  • Spectroscopy

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Binzel, R. P., DeMeo, F. E., Burt, B. J., Cloutis, E. A., Rozitis, B., Burbine, T. H., ... Scheeres, D. J. (2015). Spectral slope variations for OSIRIS-REx target Asteroid (101955) Bennu: Possible evidence for a fine-grained regolith equatorial ridge. Icarus, 256, 22-29. https://doi.org/10.1016/j.icarus.2015.04.011

Spectral slope variations for OSIRIS-REx target Asteroid (101955) Bennu : Possible evidence for a fine-grained regolith equatorial ridge. / Binzel, Richard P.; DeMeo, Francesca E.; Burt, Brian J.; Cloutis, Edward A.; Rozitis, Ben; Burbine, Thomas H.; Campins, Humberto; Clark, Beth Ellen; Emery, Joshua P.; Hergenrother, Carl W.; Howell, Ellen S.; Lauretta, Dante; Nolan, Michael C.; Mansfield, Megan; Pietrasz, Valerie; Polishook, David; Scheeres, Daniel J.

In: Icarus, Vol. 256, 01.08.2015, p. 22-29.

Research output: Contribution to journalArticle

Binzel, RP, DeMeo, FE, Burt, BJ, Cloutis, EA, Rozitis, B, Burbine, TH, Campins, H, Clark, BE, Emery, JP, Hergenrother, CW, Howell, ES, Lauretta, D, Nolan, MC, Mansfield, M, Pietrasz, V, Polishook, D & Scheeres, DJ 2015, 'Spectral slope variations for OSIRIS-REx target Asteroid (101955) Bennu: Possible evidence for a fine-grained regolith equatorial ridge', Icarus, vol. 256, pp. 22-29. https://doi.org/10.1016/j.icarus.2015.04.011
Binzel, Richard P. ; DeMeo, Francesca E. ; Burt, Brian J. ; Cloutis, Edward A. ; Rozitis, Ben ; Burbine, Thomas H. ; Campins, Humberto ; Clark, Beth Ellen ; Emery, Joshua P. ; Hergenrother, Carl W. ; Howell, Ellen S. ; Lauretta, Dante ; Nolan, Michael C. ; Mansfield, Megan ; Pietrasz, Valerie ; Polishook, David ; Scheeres, Daniel J. / Spectral slope variations for OSIRIS-REx target Asteroid (101955) Bennu : Possible evidence for a fine-grained regolith equatorial ridge. In: Icarus. 2015 ; Vol. 256. pp. 22-29.
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AU - Binzel, Richard P.

AU - DeMeo, Francesca E.

AU - Burt, Brian J.

AU - Cloutis, Edward A.

AU - Rozitis, Ben

AU - Burbine, Thomas H.

AU - Campins, Humberto

AU - Clark, Beth Ellen

AU - Emery, Joshua P.

AU - Hergenrother, Carl W.

AU - Howell, Ellen S.

AU - Lauretta, Dante

AU - Nolan, Michael C.

AU - Mansfield, Megan

AU - Pietrasz, Valerie

AU - Polishook, David

AU - Scheeres, Daniel J.

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AB - Ongoing spectroscopic reconnaissance of the OSIRIS-REx target Asteroid (101955) Bennu was performed in July 2011 and May 2012. Near-infrared spectra taken during these apparitions display slightly more positive ("redder") spectral slopes than most previously reported measurements. While observational systematic effects can produce such slope changes, and these effects cannot be ruled out, we entertain the hypothesis that the measurements are correct. Under this assumption, we present laboratory measurements investigating a plausible explanation that positive spectral slopes indicate a finer grain size for the most directly observed sub-Earth region on the asteroid. In all cases, the positive spectral slopes correspond to sub-Earth latitudes nearest to the equatorial ridge of Bennu. If confirmed by OSIRIS-REx in situ observations, one possible physical implication is that if the equatorial ridge is created by regolith migration during episodes of rapid rotation, that migration is most strongly dominated by finer grain material. Alternatively, after formation of the ridge (by regolith of any size distribution), larger-sized equatorial material may be more subject to loss due to centrifugal acceleration relative to finer grain material, where cohesive forces can preferentially retain the finest fraction (Rozitis, B., Maclennan, E., Emery, J.P. [2014]. Nature 512, 174-176).

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