Lancaster EPrints

Mars : a geologically active planet.

Mitchell, Karl L. and Wilson, Lionel (2003) Mars : a geologically active planet. Astronomy and Geophysics, 44 (4). pp. 16-20. ISSN 1366-8781

Full text not available from this repository.

Abstract

Recent and continuing missions to Mars are showing that the Red Planet may be more geologically active than previously thought. Volcanoes and erosion by running water have shaped the surface. And evidence is growing that fluvial and possibly volcanic processes have been active in the very recent past.

Item Type: Article
Journal or Publication Title: Astronomy and Geophysics
Subjects: G Geography. Anthropology. Recreation > GE Environmental Sciences
Departments: Faculty of Science and Technology > Lancaster Environment Centre
ID Code: 21406
Deposited By: ep_ss_importer
Deposited On: 13 Jan 2009 11:05
Refereed?: Yes
Published?: Published
Last Modified: 24 Oct 2013 11:07
Identification Number:
URI: http://eprints.lancs.ac.uk/id/eprint/21406

Actions (login required)

View Item