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Titan's 'Mount Doom'

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Titan's 'Mount Doom' news & views CASSINI–HUYGENS Titan’s 'Mount Doom' Cryovolcanoes, or ice volcanoes, erupt molten ices of different varieties (water, methane, ammonia and so on) instead of molten rocks, as happens on Earth. As such, they are present in the cold bodies of the outer Solar System such as icy moons. The existence of cryovolcanoes on Titan is still a matter of some debate. We have observed flow morphologies, but they can be difficult to interpret unambiguously as volcanic, as opposed to fluvial, and we know that Titan has fluvial activity. However, when the data for the Sotra Patera region of Titan were analysed, many of us concluded that this region, at least, was volcanic in origin. This Cassini radar image of the area, obtained during the T25 and T28 Titan flybys at the beginning of 2007, is a perfect example of Cassini instruments working in synergy. It combines two Image credit: NASA/JPL-Caltech/USGS/University of Arizona Synthetic Aperture Radar images, which are used to reconstruct the topography with a digital elevation model (shown high. Doom Mons is adjacent to the dunes have a different composition from here with a vertical exaggeration deepest depression so far found on Titan, the candidate cryovolcanic materials. of 10:1), with Visual and Infrared Sotra Patera, an elongated pit ~30 km Mapping Spectrometer (VIMS) data, in diameter and 1.7 ± 0.2 km deep. which show compositional differences These features, and the surrounding Rosaly M. Lopes in false colour (see a movie for the whole flow-like features around them (called NASA Jet Propulsion Laboratory, 4800 Oak Grove region at http://photojournal.jpl.nasa.gov/ Mohini Fluctus), have been interpreted Drive, Pasadena, CA 91109, USA. catalog/PIA13695). as cryovolcanic. They are shown here in e-mail: [email protected] The image shows one of the tallest shades of green and yellow from VIMS peaks on Titan, Doom Mons, which is data, whereas the dune fields are in blue. Published online: 5 September 2017 ~70 km in diameter and 1.45 ± 0.20 km This colour difference indicates that the DOI: 10.1038/s41550-017-0249-3 578 NATURE ASTRONOMY | VOL 1 | SEPTEMBER 2017 | 578 | www.nature.com/natureastronomy © 2017 Macmillan Publishers Limited, part of Springer Nature. All rights reserved..
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