BIROn - Birkbeck Institutional Research Online

    Modelling of possible mud volcanism on Titan

    Fortes, Andrew Dominic and Grindrod, Peter M. (2006) Modelling of possible mud volcanism on Titan. Icarus 182 (2), pp. 550-558. ISSN 0019-1035.

    Full text not available from this repository.

    Abstract

    Possible sedimentary basins on Titan are potential sites for the formation of mud volcanoes. In order to constrain the appearance of such features in remotely sensed imagery being acquired by the Cassini spacecraft, we have modelled the formation of mud volcanoes on Titan for a series of plausible mud compositions, climatic conditions and geological settings, as well as addressing the full range of eruption variables; mud viscosity, conduit diameter and eruption duration. We find that for an acetylene mud source containing 20 wt liquid methane in pore spaces, overlain by a sheet of water ice 500-m thick, a mud volcano can grow as high as 140 m. Assuming reasonable eruption parameters, such an edifice may develop into a pancake-like dome several kilometres in diameter. If observed and properly characterised, mud volcanoes would provide an important window on the subsurface distribution and dynamics of solids and liquids in sedimentary basins on Titan. © 2005 Elsevier Inc. All rights reserved.

    Metadata

    Item Type: Article
    Keyword(s) / Subject(s): Titan, Volcanism, Ices, Regoliths, Geological processes
    School: Birkbeck Schools and Departments > School of Science > Earth and Planetary Sciences > UCL/Birkbeck Centre for Planetary Sciences
    Birkbeck Schools and Departments > School of Science > Earth and Planetary Sciences
    Depositing User: Dr Peter Grindrod
    Date Deposited: 27 Aug 2015 12:17
    Last Modified: 27 Aug 2015 12:17
    URI: http://eprints.bbk.ac.uk/id/eprint/12867

    Statistics

    Downloads
    Activity Overview
    0Downloads
    112Hits

    Additional statistics are available via IRStats2.

    Archive Staff Only (login required)

    Edit/View Item Edit/View Item