The Evolution of Titan's Cold South Polar Cloud

Abstract Early during Titan's southern fall, images captured by Cassini's Imaging Science Subsystem revealed the formation of a large cloud above Titan's south pole. Subsequent analysis of Cassini data revealed the cloud contained HCN ice, but the cloud's evolution has not been e...

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Main Authors: Lavender Elle Hanson, Robert S. French, Darryn W. Waugh, Erika L. Barth, Carrie M. Anderson
Format: Article
Language:English
Published: Wiley 2025-05-01
Series:Geophysical Research Letters
Online Access:https://doi.org/10.1029/2024GL113415
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author Lavender Elle Hanson
Robert S. French
Darryn W. Waugh
Erika L. Barth
Carrie M. Anderson
author_facet Lavender Elle Hanson
Robert S. French
Darryn W. Waugh
Erika L. Barth
Carrie M. Anderson
author_sort Lavender Elle Hanson
collection DOAJ
description Abstract Early during Titan's southern fall, images captured by Cassini's Imaging Science Subsystem revealed the formation of a large cloud above Titan's south pole. Subsequent analysis of Cassini data revealed the cloud contained HCN ice, but the cloud's evolution has not been examined. We reviewed imagery of Titan's south pole between 2012 and the end of mission at Ls = 93°. We find evidence of cloud formation as early as Ls = 32° (April 2012), one terrestrial month earlier than previously reported, after which the cloud persists until Ls = 79° (mid 2016). The cloud top altitude descended from about 320 km at Ls = 32° to below 230 km by Ls = 79°, at which point it became obscured by atmospheric methane absorption. The cloud also grew laterally, remaining just beyond the terminator, suggesting the cloud marks a region of cold air in the polar stratosphere. These measurements place new constraints on Titan's polar stratospheric temperature structure and circulation during southern fall.
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spelling doaj-art-7ea902d6858f43a3bdeb3510158e8a972025-08-20T03:12:52ZengWileyGeophysical Research Letters0094-82761944-80072025-05-01529n/an/a10.1029/2024GL113415The Evolution of Titan's Cold South Polar CloudLavender Elle Hanson0Robert S. French1Darryn W. Waugh2Erika L. Barth3Carrie M. Anderson4Department of Earth and Planetary Sciences Johns Hopkins University Baltimore MD USASETI Institute Mountain View CA USADepartment of Earth and Planetary Sciences Johns Hopkins University Baltimore MD USASouthwest Research Institute Boulder CO USAPlanetary Systems Laboratory NASA Goddard Space Flight Center Greenbelt MD USAAbstract Early during Titan's southern fall, images captured by Cassini's Imaging Science Subsystem revealed the formation of a large cloud above Titan's south pole. Subsequent analysis of Cassini data revealed the cloud contained HCN ice, but the cloud's evolution has not been examined. We reviewed imagery of Titan's south pole between 2012 and the end of mission at Ls = 93°. We find evidence of cloud formation as early as Ls = 32° (April 2012), one terrestrial month earlier than previously reported, after which the cloud persists until Ls = 79° (mid 2016). The cloud top altitude descended from about 320 km at Ls = 32° to below 230 km by Ls = 79°, at which point it became obscured by atmospheric methane absorption. The cloud also grew laterally, remaining just beyond the terminator, suggesting the cloud marks a region of cold air in the polar stratosphere. These measurements place new constraints on Titan's polar stratospheric temperature structure and circulation during southern fall.https://doi.org/10.1029/2024GL113415
spellingShingle Lavender Elle Hanson
Robert S. French
Darryn W. Waugh
Erika L. Barth
Carrie M. Anderson
The Evolution of Titan's Cold South Polar Cloud
Geophysical Research Letters
title The Evolution of Titan's Cold South Polar Cloud
title_full The Evolution of Titan's Cold South Polar Cloud
title_fullStr The Evolution of Titan's Cold South Polar Cloud
title_full_unstemmed The Evolution of Titan's Cold South Polar Cloud
title_short The Evolution of Titan's Cold South Polar Cloud
title_sort evolution of titan s cold south polar cloud
url https://doi.org/10.1029/2024GL113415
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