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Lessons From Pluto for Uranus MoonsIntroduction: Small patches of starkly different albedo on both Oberon and Umbriel may be evidence for frost segregation and volatile migration. The high obliquity of the Uranian system makes it a good candidate for volatile transport activity. CO2 and ammonium species have been detected on some Uranian satellites, and CH4 is at least theoretically viable as a resident volatile. The OWL-recommended UOP Orbiter spacecraft should be equipped with instruments capable of evaluating the nature and extent of volatiles in the Uranian satellite system.
Document ID
20240000331
Acquisition Source
Ames Research Center
Document Type
Extended Abstract
Authors
J M Moore
(Ames Research Center Mountain View, United States)
P M Schenk
(Lunar and Planetary Institute Houston, Texas, United States)
J R Spencer
(Southwest Research Institute San Antonio, United States)
Date Acquired
January 9, 2024
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: New Horizons Science Team Meeting/Workshop
Location: Laurel, MD
Country: US
Start Date: January 23, 2024
End Date: January 25, 2024
Sponsors: Southwest Research Institute
Funding Number(s)
WBS: 135353.02.03.01.99
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
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