Macroporosity and Grain Density of Rubble Pile Asteroid (162173) Ryugu

Rubble pile asteroids such as (162173) Ryugu have large bulk porosities, which are believed to result from void spaces in between the constituent boulders (macroporosity) as well as void spaces within the boulders themselves (microporosity). In general, both macroporosity and microporosity are estim...

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Bibliographic Details
Published in:Journal of Geophysical Research: Planets
Main Authors: Grott, Matthias, Biele, Jens, Michel, Patrick, Sugita, Seiji, Schröder, Stefan, Sakatani, Naoya, Neumann, Wladimir, Kameda, Shingo, Michikami, Tatsuhiro, Honda, Chikatoshi, 2 German Aerospace Center Cologne Germany, 3 Laboratoire Lagrange Université Côte d'Azur Observatoire de la Côte d'Azur CNRS Nice France, 4 University of Tokyo Tokyo Japan, 1 German Aerospace Center Berlin Germany, 5 ISAS/JAXA Sagamihara Japan, 7 Rikkyo University Tokyo Japan, 8 Kindai University Hiroshima Japan, 9 University of Aizu Aizu‐Wakamatsu Japan
Format: Article in Journal/Newspaper
Language:English
Published: 2020
Subjects:
Online Access:https://doi.org/10.1029/2020JE006519
http://resolver.sub.uni-goettingen.de/purl?gldocs-11858/8427