Meteorites from Phobos and Deimos at Earth?

Author(s)
P. Wiegert, Mattia Galiazzo
Abstract

We examine the conditions under which material from the martian moons Phobos and Deimos could reach our planet in the form of meteorites. We find that the necessary ejection speeds from these moons (900 and 600 m/s for Phobos and Deimos respectively) are much smaller than from Mars' surface (5000 m/s). These speeds are below typical impact speeds for asteroids and comets (10-40 km/s) at Mars' orbit, and we conclude that delivery of meteorites from Phobos and Deimos to the Earth can occur.

Organisation(s)
Department of Astrophysics
External organisation(s)
University of Western Ontario
Journal
Planetary and Space Science
Volume
142
Pages
48 - 52
No. of pages
5
ISSN
0032-0633
DOI
https://doi.org/10.1016/j.pss.2017.05.001
Publication date
08-2017
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy, 103004 Astrophysics
Keywords
ASJC Scopus subject areas
Astronomy and Astrophysics, Space and Planetary Science
Portal url
https://ucrisportal.univie.ac.at/en/publications/0b7a0020-c9cf-43c4-8d62-2d58dd919a13