The Porosity of Eros and Implications for Its Internal Structure

Details The Porosity of Eros and Implications for Its Internal Structure The Porosity of Eros and Implications for Its Internal Structure

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1721w&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1721

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We estimate the porosity of Eros to be between 21-33%. Based on this
porosity range and morphologic observations of the surface, we suggest
that the asteroid is heavily fractured (but not a rubble pile).

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