Alluvial Fans on Titan Reveal Materials, Processes and Regional Conditions

J. Radebaugh (1) , R. D. Lorenz (2) , T. G. Farr (3) , Randolf L. Kirk (4) , J.I. Lunine (5) , D. Ventra (6) , Alice Le Gall (7) , R. M. C. Lopes (3) , Jason W. Barnes (8) , A. G. Hayes (5) , E. R. Stofan (9) , S. D. Wall (3) , C. Wood (10)

1 Department of Geological Sciences [BYU]
2 APL - Johns Hopkins University Applied Physics Laboratory [Laurel, MD]
3 JPL - Jet Propulsion Laboratory
4 Astrogeology Science Center [Flagstaff]
5 Department of Astronomy [Ithaca]
6 Universiteit Utrecht / Utrecht University [Utrecht]
7 PLANETO - LATMOS
8 University of Idaho [Moscow, USA]
9 Proxemy Research Inc
10 Wheeling Jesuit University

Alluvial fans on Titan reveal vigorous fluvial processes occur or occurred, indicate a prolonged depositional history, and may illuminate climate conditions.

Domaines: Planétologie et astrophysique de la terre [astro-ph.EP]; Planétologie et astrophysique de la terre [astro-ph.EP]

J. Radebaugh, R. D. Lorenz, T. G. Farr, Randolf L. Kirk, J.I. Lunine, et al.. Alluvial Fans on Titan Reveal Materials, Processes and Regional Conditions. 44th Lunar and Planetary Science Conference, Mar 2013, The Woodlands, Texas, United States. LPI Contribution No. 1719, p.2641. ⟨hal-01073941⟩