Porous Boulders on (162173) Ryugu: Compaction Modeling and Implications for Parent Body's Radius, Accretion Time, and Interior Porosity Distribution

W. Neumann(University of Münster), E. Kührt, J. Biele, M. Grott, Maximilian Hamm(Deutsches Zentrum für Luft- und Raumfahrt e. V. (DLR)), R. Jaumann(Freie Universität Berlin)
Unknown
November 1, 2019
Cited by 0

Related Papers

Ages and stratigraphy of lunar mare basalts: A synthesis
|Geological Society of America eBooks|2011|286
Low thermal conductivity boulder with high porosity identified on C-type asteroid (162173) Ryugu
|Nature Astronomy|2019|177
Highly porous nature of a primitive asteroid revealed by thermal imaging
|Nature|2020|140
Images from the surface of asteroid Ryugu show rocks similar to carbonaceous chondrite meteorites
|Science|2019|125
The structure of the regolith on 67P/Churyumov-Gerasimenko from ROLIS descent imaging
|Science|2015|101