Analysis of Transient Fog Features on Titan

Saturn’s moon Titan is the only known solar system body other than Earth with an active hydrologic cycle, based on methane instead of water. To better characterize this environment, this thesis examines transient low-altitude methane clouds (hereafter referred to as fogs) that have been observed nea...

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Main Author: Romashkova, Elena
Other Authors: Soderblom, Jason
Format: Thesis
Published: Massachusetts Institute of Technology 2022
Online Access:https://hdl.handle.net/1721.1/144842
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author Romashkova, Elena
author2 Soderblom, Jason
author_facet Soderblom, Jason
Romashkova, Elena
author_sort Romashkova, Elena
collection MIT
description Saturn’s moon Titan is the only known solar system body other than Earth with an active hydrologic cycle, based on methane instead of water. To better characterize this environment, this thesis examines transient low-altitude methane clouds (hereafter referred to as fogs) that have been observed near Titan’s surface in data from the Visual and Infrared Mapping Spectrometer (VIMS) onboard the Cassini mission. We compile a data set of 19 fog features, expanded from previous studies, and investigate a range of factors that could influence fog formation. We find a tendency for fogs to be observed at high latitudes and primarily in the north, in agreement with modeling of Titan’s humidity. They also show a potential correlation to the locations of methane lakes, with several features that appear to trace shorelines. They may also be preferentially observed in seasons with higher insolation. These results can guide future modeling efforts, as well as continued data collection, to further constrain fog formation mechanisms.
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spelling mit-1721.1/1448422022-08-30T03:09:41Z Analysis of Transient Fog Features on Titan Romashkova, Elena Soderblom, Jason Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Saturn’s moon Titan is the only known solar system body other than Earth with an active hydrologic cycle, based on methane instead of water. To better characterize this environment, this thesis examines transient low-altitude methane clouds (hereafter referred to as fogs) that have been observed near Titan’s surface in data from the Visual and Infrared Mapping Spectrometer (VIMS) onboard the Cassini mission. We compile a data set of 19 fog features, expanded from previous studies, and investigate a range of factors that could influence fog formation. We find a tendency for fogs to be observed at high latitudes and primarily in the north, in agreement with modeling of Titan’s humidity. They also show a potential correlation to the locations of methane lakes, with several features that appear to trace shorelines. They may also be preferentially observed in seasons with higher insolation. These results can guide future modeling efforts, as well as continued data collection, to further constrain fog formation mechanisms. S.B. 2022-08-29T16:15:33Z 2022-08-29T16:15:33Z 2022-05 2022-08-11T18:52:20.263Z Thesis https://hdl.handle.net/1721.1/144842 In Copyright - Educational Use Permitted Copyright MIT http://rightsstatements.org/page/InC-EDU/1.0/ application/pdf Massachusetts Institute of Technology
spellingShingle Romashkova, Elena
Analysis of Transient Fog Features on Titan
title Analysis of Transient Fog Features on Titan
title_full Analysis of Transient Fog Features on Titan
title_fullStr Analysis of Transient Fog Features on Titan
title_full_unstemmed Analysis of Transient Fog Features on Titan
title_short Analysis of Transient Fog Features on Titan
title_sort analysis of transient fog features on titan
url https://hdl.handle.net/1721.1/144842
work_keys_str_mv AT romashkovaelena analysisoftransientfogfeaturesontitan