Simulating weathering of basalt on Mars and Earth by thermal cycling
Abstract
Physical weathering induced by heating and cooling may cause rock breakdown on Mars and Earth. We report results from parallel weathering simulations on basalt blocks exposed to diurnal cycles representing Mars-like (two simulation runs from −55 to +20 oC and −75 to +10 oC, 1–100% relative humidity, 4–8 mbar pressure, CO_2 atmosphere) and hot arid Earth (23–72o C, 30–100% relative humidity) conditions. Under Earth conditions, thermally pre-stressed blocks showed measurable strength declines, whilst salt pre-treated blocks showed strength gains. Under Mars-like conditions, pre-stressed blocks recorded greater or similar strength declines and salt pre-treated blocks showed more muted strength declines than under Earth conditions. The results imply that on Earth and Mars diurnal cycling of temperature alone can cause deterioration of basalt with a pre-existing stress history. The type of stress history is important, with salt pre-treatment affecting the response of thermally pre-stressed blocks under both Earth and Mars conditions.
Additional Information
© 2010 American Geophysical Union. Received 25 April 2010; accepted 28 July 2010; published 22 September 2010. We thank RockUnique for supplying the basalt, Lisa Mol and David Banfield for laboratory assistance, and Neil Bowles for useful discussions. The work was in part supported by NASA through Planetary Geology and Geophysics grant NNX08AM40G.Attached Files
Published - 2010GL043522.pdf
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Additional details
- Eprint ID
- 34914
- Resolver ID
- CaltechAUTHORS:20121016-093655210
- NASA Planetary Geology and Geophysics
- NNX08AM40G
- Created
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2012-10-16Created from EPrint's datestamp field
- Updated
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2021-11-09Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences