Meteorites from Phobos and Deimos at Earth?

Autor(en)
P. Wiegert, Mattia Galiazzo
Abstrakt

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(en)
Institut für Astrophysik
Externe Organisation(en)
University of Western Ontario
Journal
Planetary and Space Science
Band
142
Seiten
48 - 52
Anzahl der Seiten
5
ISSN
0032-0633
DOI
https://doi.org/10.1016/j.pss.2017.05.001
Publikationsdatum
08-2017
Peer-reviewed
Ja
ÖFOS 2012
103003 Astronomie, 103004 Astrophysik
Schlagwörter
ASJC Scopus Sachgebiete
Astronomy and Astrophysics, Space and Planetary Science
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/0b7a0020-c9cf-43c4-8d62-2d58dd919a13