Statistical features of drainage basins in mars channel networks
Can one guess from the landscape the past presence of water?
INFM UdR di Roma1 and Dip. di Fisica,
Università “La Sapienza", P.le A. Moro 2, 00185 Roma, Italy
2 Centro Studi e Ricerche E. Fermi, Compendio Viminale, Roma, Italy
3 Institut de Physique Théorique, Université de Lausanne, 1015 Lausanne, Switzerland
4 SMC INFM, Università “La Sapienza", P.le A. Moro 2, 00185 Roma, Italy
Corresponding author: a email@example.com
Published online: 14 May 2004
Erosion by flowing water is one of the major forces shaping the surface of Earth. Studies in the last decade have shown, in particular, that the drainage region of rivers, where water is collected, exhibits scale invariant features characterized by exponents that are the same for rivers around the world. Here we show that from the data obtained by the MOLA altimeter of the Mars Global Surveyor one can perform the same analysis for mountain sides on Mars. We then show that in some regions fluid erosion might have played a role in the present martian landscape.
PACS: 92.40.Fb – Rivers, runoff, and streamflow / 96.30.Gc – Mars / 05.45.Df – Fractals
© EDP Sciences, Società Italiana di Fisica, Springer-Verlag, 2004