Inferring interiors and structural history of top-shaped asteroids from external properties of asteroid (101955) Bennu

Asteroid interiors are key to understand their formation and evolution. Here, the authors show that numerically simulated low-cohesion and low-friction structures with several high-cohesion internal zones can explain asteroid Bennu’s geophysical characteristics and the absence of the moons.

Bibliographic Details
Main Authors: Yun Zhang, Patrick Michel, Olivier S. Barnouin, James H. Roberts, Michael G. Daly, Ronald-L. Ballouz, Kevin J. Walsh, Derek C. Richardson, Christine M. Hartzell, Dante S. Lauretta
Format: Article
Language:English
Published: Nature Portfolio 2022-08-01
Series:Nature Communications
Online Access:https://doi.org/10.1038/s41467-022-32288-y
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author Yun Zhang
Patrick Michel
Olivier S. Barnouin
James H. Roberts
Michael G. Daly
Ronald-L. Ballouz
Kevin J. Walsh
Derek C. Richardson
Christine M. Hartzell
Dante S. Lauretta
author_facet Yun Zhang
Patrick Michel
Olivier S. Barnouin
James H. Roberts
Michael G. Daly
Ronald-L. Ballouz
Kevin J. Walsh
Derek C. Richardson
Christine M. Hartzell
Dante S. Lauretta
author_sort Yun Zhang
collection DOAJ
description Asteroid interiors are key to understand their formation and evolution. Here, the authors show that numerically simulated low-cohesion and low-friction structures with several high-cohesion internal zones can explain asteroid Bennu’s geophysical characteristics and the absence of the moons.
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spelling doaj.art-035f07c2e41b47aaa86b2620aa1a10852022-12-22T02:48:45ZengNature PortfolioNature Communications2041-17232022-08-0113111210.1038/s41467-022-32288-yInferring interiors and structural history of top-shaped asteroids from external properties of asteroid (101955) BennuYun Zhang0Patrick Michel1Olivier S. Barnouin2James H. Roberts3Michael G. Daly4Ronald-L. Ballouz5Kevin J. Walsh6Derek C. Richardson7Christine M. Hartzell8Dante S. Lauretta9Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire LagrangeUniversité Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Laboratoire LagrangeThe Johns Hopkins University, Applied Physics LaboratoryThe Johns Hopkins University, Applied Physics LaboratoryThe Centre for Research in Earth and Space Science, York UniversityThe Johns Hopkins University, Applied Physics LaboratorySouthwest Research InstituteDepartment of Astronomy, University of MarylandDepartment of Aerospace Engineering, University of MarylandLunar and Planetary Laboratory, University of ArizonaAsteroid interiors are key to understand their formation and evolution. Here, the authors show that numerically simulated low-cohesion and low-friction structures with several high-cohesion internal zones can explain asteroid Bennu’s geophysical characteristics and the absence of the moons.https://doi.org/10.1038/s41467-022-32288-y
spellingShingle Yun Zhang
Patrick Michel
Olivier S. Barnouin
James H. Roberts
Michael G. Daly
Ronald-L. Ballouz
Kevin J. Walsh
Derek C. Richardson
Christine M. Hartzell
Dante S. Lauretta
Inferring interiors and structural history of top-shaped asteroids from external properties of asteroid (101955) Bennu
Nature Communications
title Inferring interiors and structural history of top-shaped asteroids from external properties of asteroid (101955) Bennu
title_full Inferring interiors and structural history of top-shaped asteroids from external properties of asteroid (101955) Bennu
title_fullStr Inferring interiors and structural history of top-shaped asteroids from external properties of asteroid (101955) Bennu
title_full_unstemmed Inferring interiors and structural history of top-shaped asteroids from external properties of asteroid (101955) Bennu
title_short Inferring interiors and structural history of top-shaped asteroids from external properties of asteroid (101955) Bennu
title_sort inferring interiors and structural history of top shaped asteroids from external properties of asteroid 101955 bennu
url https://doi.org/10.1038/s41467-022-32288-y
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