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:
Journal Article
Journal or Publication Title:
Astronomy and Geophysics
Uncontrolled Keywords:
/dk/atira/pure/subjectarea/asjc/1900/1906
Subjects:
?? geochemistry and petrologyastronomy and astrophysicsgeophysicsge environmental sciences ??
Departments:
ID Code:
21406
Deposited By:
Deposited On:
13 Jan 2009 11:05
Refereed?:
Yes
Published?:
Published
Last Modified:
15 Jul 2024 09:55