A Photometric Investigation of the Major Uranian Satellites

The Uranian system is one of the most unusual in the Solar System and its formation and evolution are poorly understood. Voyager 2 revealed that the major satellites have complex geologic features, including craters, fault systems, and chasmata. The Uranian system has been understudied and current k...

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Main Author: Colclasure, Abigail M.
Other Authors: Person, Michael J.
Format: Thesis
Published: Massachusetts Institute of Technology 2024
Online Access:https://hdl.handle.net/1721.1/155331
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author Colclasure, Abigail M.
author2 Person, Michael J.
author_facet Person, Michael J.
Colclasure, Abigail M.
author_sort Colclasure, Abigail M.
collection MIT
description The Uranian system is one of the most unusual in the Solar System and its formation and evolution are poorly understood. Voyager 2 revealed that the major satellites have complex geologic features, including craters, fault systems, and chasmata. The Uranian system has been understudied and current knowledge is limit by a lack of data. The 2023-2032 decadal survey ranked a flagship NASA mission to Uranus, with a required launch window of the early 2030s, as a top priority. Further study is urgently needed, both scientifically and to inform mission planning. We conducted a photometric study, primarily using MIT’s Wallace Astrophysical Observatory, and report the lightcurves of Titania and Oberon in the Sloan g’, r’, and i’ filters. Further observations from larger telescopes are needed, but these data may indicate that ice on both Titania and Oberon has redistributed since the Voyager epoch.
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spelling mit-1721.1/1553312024-06-28T03:22:23Z A Photometric Investigation of the Major Uranian Satellites Colclasure, Abigail M. Person, Michael J. Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences The Uranian system is one of the most unusual in the Solar System and its formation and evolution are poorly understood. Voyager 2 revealed that the major satellites have complex geologic features, including craters, fault systems, and chasmata. The Uranian system has been understudied and current knowledge is limit by a lack of data. The 2023-2032 decadal survey ranked a flagship NASA mission to Uranus, with a required launch window of the early 2030s, as a top priority. Further study is urgently needed, both scientifically and to inform mission planning. We conducted a photometric study, primarily using MIT’s Wallace Astrophysical Observatory, and report the lightcurves of Titania and Oberon in the Sloan g’, r’, and i’ filters. Further observations from larger telescopes are needed, but these data may indicate that ice on both Titania and Oberon has redistributed since the Voyager epoch. S.B. 2024-06-27T19:45:28Z 2024-06-27T19:45:28Z 2024-05 2024-05-20T13:45:48.899Z Thesis https://hdl.handle.net/1721.1/155331 In Copyright - Educational Use Permitted Copyright retained by author(s) https://rightsstatements.org/page/InC-EDU/1.0/ application/pdf Massachusetts Institute of Technology
spellingShingle Colclasure, Abigail M.
A Photometric Investigation of the Major Uranian Satellites
title A Photometric Investigation of the Major Uranian Satellites
title_full A Photometric Investigation of the Major Uranian Satellites
title_fullStr A Photometric Investigation of the Major Uranian Satellites
title_full_unstemmed A Photometric Investigation of the Major Uranian Satellites
title_short A Photometric Investigation of the Major Uranian Satellites
title_sort photometric investigation of the major uranian satellites
url https://hdl.handle.net/1721.1/155331
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