Voluminous volcanism on early Mars revealed in Valles Marineris

Details Voluminous volcanism on early Mars revealed in Valles Marineris Voluminous volcanism on early Mars revealed in Valles Marineris

Feb 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999natur.397..584m&link_type=abstract

Nature, Volume 397, Issue 6720, pp. 584-586 (1999).

Mathematics

Logic

89

Scientific paper

The relative rates and importance of impact cratering, volcanism, erosion, and the deposition of sediments to the early geological history of Mars are poorly known. That history is recorded in the upper crust of the planet, which is best exposed along the 4,000-km-long canyon system called Valles Marineris. Previous studies of the stratigraphy of this region have assumed that it consists of megabreccia and fractured bedrock resulting from impacts, overlain by or interbedded with relatively thin layers of lava, and with the layering restricted to the uppermost level of the crust. Here we report new high-resolution images that reveal ubiquitous horizontal layering to depths of at least 8km in the canyons. Megabreccia should be only coarsely layered and fractured bedrock should be unlayered, so these observations indicate that volcanic or sedimentary processes were much more important in early martian history than previously believed. Morphological and compositional data suggest that the layers were formed mainly by volcanic flood lavas. Mars was therefore probably very volcanically active during at least the first billion years and after the period when the heaviest impact bombardment had ended.

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