Volume 334, Issue 9 p. 936-939
Original Paper

A statistical dynamical study of meteorite impactors: A case study based on parameters derived from the Bosumtwi impact event

M.A. Galiazzo

Corresponding Author

M.A. Galiazzo

Institute for Astrophysics, University of Vienna, Türkenschanzstraße 17, A-1180 Vienna, Austria

Institute for Astrophysics, University of Vienna, Türkenschanzstraße 17, A-1180 Vienna, AustriaSearch for more papers by this author
Á. Bazsó

Á. Bazsó

Institute for Astrophysics, University of Vienna, Türkenschanzstraße 17, A-1180 Vienna, Austria

Search for more papers by this author
M.S. Huber

M.S. Huber

Department of Lithospheric Research, University of Vienna, Althanstraße 14, A-1090 Vienna, Austria

Search for more papers by this author
A. Losiak

A. Losiak

Department of Lithospheric Research, University of Vienna, Althanstraße 14, A-1090 Vienna, Austria

Search for more papers by this author
R. Dvorak

R. Dvorak

Institute for Astrophysics, University of Vienna, Türkenschanzstraße 17, A-1180 Vienna, Austria

Search for more papers by this author
C. Koeberl

C. Koeberl

Department of Lithospheric Research, University of Vienna, Althanstraße 14, A-1090 Vienna, Austria

Naturhistorisches Museum Wien, Burgring 7, 1010 Vienna, Austria

Search for more papers by this author
First published: 07 November 2013
Citations: 1

Abstract

The study of meteorite craters on Earth provides information about the dynamic evolution of bodies within the Solar System. the Bosumtwi crater is a well studied, 10.5 km in diameter, ca. 1.07 Myr old impact structure located in Ghana. The impactor was ∼1 km in diameter, an ordinary chondrite and struck the Earth with an angle between 30° and 45° from the horizontal. We have used a two phase backward integration to constrain the most probable parent region of the impactor. We find that the most likely source region is a high inclination object from the Middle Main Belt. (© 2013 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)

The full text of this article hosted at iucr.org is unavailable due to technical difficulties.