Lakes and seas of Titan

Abstract. This thesis reviews studies about the lakes and seas of Saturn’s moon, Titan. Conditions on Titan’s surface are first estimated to validate that substances in Titan’s atmosphere can exist in liquid phase. This is followed by descriptions of devices that have been used to study Titan from E...

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Main Author: Siitonen, M. (Miikka)
Format: Others
Language:English
Published: University of Oulu 2019
Online Access:http://jultika.oulu.fi/Record/nbnfioulu-201908242817
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spelling ndltd-oulo.fi-oai-oulu.fi-nbnfioulu-2019082428172019-08-27T03:18:35ZLakes and seas of TitanSiitonen, M. (Miikka)info:eu-repo/semantics/openAccess© Miikka Siitonen, 2019Abstract. This thesis reviews studies about the lakes and seas of Saturn’s moon, Titan. Conditions on Titan’s surface are first estimated to validate that substances in Titan’s atmosphere can exist in liquid phase. This is followed by descriptions of devices that have been used to study Titan from Earth, space and on its surface. Research concerning the detection and distribution of the lakes are then discussed. Features of the lakes such as surface areas, chemical compositions and formations like shores are looked into. Results from models that describe liquid currents driven by tidal forces, wind, temperature differences and rain induced density differences are given. This leads into discussion of liquid surface waves. Titan’s potential for supporting life is also considered. Observation of a disappearing and reappearing region in Titan’s sea, the Magic Island phenomenon, is construed and possible causes for this phenomenon are examined. Lastly, future mission projects that are capable of studying the lakes in situ are described with the emphasis on the Titan Submarine project.University of Oulu2019-08-23info:eu-repo/semantics/bachelorThesisinfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://jultika.oulu.fi/Record/nbnfioulu-201908242817eng
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language English
format Others
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description Abstract. This thesis reviews studies about the lakes and seas of Saturn’s moon, Titan. Conditions on Titan’s surface are first estimated to validate that substances in Titan’s atmosphere can exist in liquid phase. This is followed by descriptions of devices that have been used to study Titan from Earth, space and on its surface. Research concerning the detection and distribution of the lakes are then discussed. Features of the lakes such as surface areas, chemical compositions and formations like shores are looked into. Results from models that describe liquid currents driven by tidal forces, wind, temperature differences and rain induced density differences are given. This leads into discussion of liquid surface waves. Titan’s potential for supporting life is also considered. Observation of a disappearing and reappearing region in Titan’s sea, the Magic Island phenomenon, is construed and possible causes for this phenomenon are examined. Lastly, future mission projects that are capable of studying the lakes in situ are described with the emphasis on the Titan Submarine project.
author Siitonen, M. (Miikka)
spellingShingle Siitonen, M. (Miikka)
Lakes and seas of Titan
author_facet Siitonen, M. (Miikka)
author_sort Siitonen, M. (Miikka)
title Lakes and seas of Titan
title_short Lakes and seas of Titan
title_full Lakes and seas of Titan
title_fullStr Lakes and seas of Titan
title_full_unstemmed Lakes and seas of Titan
title_sort lakes and seas of titan
publisher University of Oulu
publishDate 2019
url http://jultika.oulu.fi/Record/nbnfioulu-201908242817
work_keys_str_mv AT siitonenmmiikka lakesandseasoftitan
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