Changes in Titan's Surface Brightness Point to Cryovolcanism
The authors compared many volcanic-like features, such as flows, calderas and craters, with similar geological features found on the Earth to study the possibility of cryovolcanic activity within regions close to Titan’s equator.
Titan has an atmosphere rich in organic carbon-based compounds and has clouds and rains of liquid methane that mimic Earth’s water cycle. Its landscape is remarkably Earth-like with dunes and lakes, erosion due to weathering and tectonic-like features. Astronomers believe that beneath its icy surface there is an ocean of liquid water, possibly mixed with ammonia. The low number of impact craters seen on Titan suggests that the surface is relatively young and is therefore dynamic and active.
“All of these features, plus a need for a methane reservoir and volcanic activity to replenish the methane we have detected in the atmosphere, is compatible with the theory of active cryovolcanism on Titan,” said Solomonidou, of the Observatoire de Paris and National and Kapodistrian University of Athens.
Solomonidou and colleagues have investigated the potentially cryogenic regions of Tui Regio, Hotei Regio and Sotra Patera using Cassini’s Visual and Infrared Mapping Spectrometer (VIMS).
“We were able to penetrate the atmosphere with VIMS and view any changes in these surface features. Interestingly, the albedo (brightness) of two of the areas has changed with time,” explained Solomonidou. “Tui Regio got darker from 2005 to 2009 and Sotra Patera -- the most favorable cryovolcanic candidate on Titan -- got brighter between 2005 and 2006.”
Surface variations, together with spectral albedo properties and the presence of volcanic-like features, suggest that these cryovolcanic candidate regions are connected to Titan’s deep liquid ocean.
“These results have important implications for Titan’s potential to support life as these cryovolcanic areas might contain environments that could harbor conditions favorable for life,” said Solomonidou.
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