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.
Cite
CITATION STYLE
APA
Mitchell, K. L., & Wilson, L. (2003). Mars: A geologically active planet. Astronomy and Geophysics. Blackwell Publishing Ltd. https://doi.org/10.1046/j.1468-4004.2003.44416.x
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