A 2 km-size asteroid challenging the rubble-pile spin barrier – A case for cohesion-Reference-Cited by-同舟云学术

A 2 km-size asteroid challenging the rubble-pile spin barrier – A case for cohesion

Published:2016-03 Issue: Volume:267 Page:243-254
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Polishook D.,Moskovitz N.,Binzel R.P.,Burt B.,DeMeo F.E.,Hinkle M.L.,Lockhart M.,Mommert M.,Person M.,Thirouin A.,Thomas C.A.,Trilling D.,Willman M.,Aharonson O.

Funder

Ministry of Science, Technology and Space of the Israeli

AXA Research Fund

NASA

Helen Kimmel Center for Planetary Science

ISF I-CORE

NASA NEOO

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

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5. Asteroid 2008 TC3 – Almahata Sitta: A spectacular breccia containing many different ureilitic and chondritic lithologies;Bischoff;Meteor. Planet. Sci.,2010

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