V-type near-Earth asteroids: Dynamics, close encounters and impacts with terrestrial planets

Autor(en)
Mattia Galiazzo, E. A. Silber, David Bancelin
Abstrakt

Background: Asteroids colliding with planets vary in composition and taxonomical type. Among Near-Earth Asteroids (NEAs) are the V-types, basaltic asteroids that are classified via spectroscopic observations. Materials and Methods: we performed numerical simulations and statistical analysis of close encounters and impacts between V-type NEAs and the terrestrial planets over the next 10 Myr. We study the probability of V- type NEAs colliding with Earth, Mars and Venus, as well as the Moon. We perform a correlational analysis of possible craters produced by V-type NEAs, using available catalogs for terrestrial impact craters. Results: The results suggest that V-type NEAs can have many close encounters below 1 LD and even some of them impacts with all the terrestrial planets, the Earth in particular. There are four candidate craters on Earth that were likely caused by V-type NEAs. Conclusion: At least 70% of the V-type NEAs can have close encounters with the terrestrial planets (and 58% with the Moon). They can collide with all the terrestrial planets. In particular for the Earth the average rate is one every ∼12 Myr. The two craters with the highest probability of being generated by an impact with a basaltic impactor are: the Strangways crater (24 km diameter) in Australia and the Nicholson crater (12.5 km diameter) in Canada.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
University of Western Ontario
Journal
Astronomische Nachrichten
Band
338
Seiten
375 - 384
Anzahl der Seiten
10
ISSN
0004-6337
DOI
https://doi.org/10.1002/asna.201613273
Publikationsdatum
05-2017
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/6f6812a5-014a-4251-b770-e58eda0a0dba