Comparision of the Martian Gullies With Terrestrial Ones

Details Comparision of the Martian Gullies With Terrestrial Ones Comparision of the Martian Gullies With Terrestrial Ones

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufm.h33c1397c&link_type=abstract

American Geophysical Union, Fall Meeting 2005, abstract #H33C-1397

Mathematics

Logic

1824 Geomorphology: General (1625), 1826 Geomorphology: Hillslope (1625), 1850 Overland Flow, 5415 Erosion And Weathering, 6225 Mars

Scientific paper

Some of the geomorphological features in Mars are the gullies. Some theories developed tried to explained its origin, either by liquid water, liquid carbon dioxide or flows of dry granular material. We made a comparative analysis of the Martian gullies with the terrestrial ones. We present the characteristics of some terrestrial gullies formed at cold enviroment, sited at the Nevado de Toluca volcanoe near Toluca City, Mexico. We compare them with Martian gullies, choisen from four different areas, to recognize possible processes evolved in its formation. Also, we measured the lenghts of those Martian gullies and their range was from 24 m 1775 m.

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