Publication Date:
2019-07-17
Description:
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). Additional information is contained in the original extended abstract.
Keywords:
Lunar and Planetary Science and Exploration
Type:
Lunar and Planetary Science XXXII; LPI-Contrib-1080
Format:
text