High-resolution shape models of Phobos and Deimos from stereophotoclinometry
C. M. Ernst(Johns Hopkins University Applied Physics Laboratory), Kielan K. W. Hoch(University of California San Diego), M. Al Asad(University of British Columbia), R. W. Gaskell(Planetary Science Institute), Benjamin Hyatt(Northwestern University), R. T. Daly(Lockheed Martin (United States)), Hari Nair(Johns Hopkins University Applied Physics Laboratory), O. S. Barnouin(Johns Hopkins University Applied Physics Laboratory)
Cited by 30
Related Papers
The Rubble-Pile Asteroid Itokawa as Observed by Hayabusa
|Science|2006|966
Deep Impact: Excavating Comet Tempel 1
|Science|2005|847
Identification of hydrated silicate minerals on Mars using MRO‐CRISM: Geologic context near Nili Fossae and implications for aqueous alteration
|Journal of Geophysical Research Atmospheres|2009|681
OSIRIS-REx: Sample Return from Asteroid (101955) Bennu
|Space Science Reviews|2017|651