Results 21 to 30 of about 129,106 (151)
Unraveling the Geologic History of Miranda’s Inverness Corona
Miranda is the only icy body whose surface is known to contain the enigmatic features called corona—ovoid to trapezoidal areas of deformation. In this work, we seek to constrain potential formation mechanisms for Inverness Corona, the youngest known ...
Erin J. Leonard +3 more
doaj +1 more source
Longitudinal Variation of H2O Ice Absorption on Miranda
Many tidally locked icy satellites in the outer solar system show leading/trailing hemispherical asymmetries in the strength of near-infrared (NIR) H _2 O ice absorption bands, in which the absorption bands are stronger on the leading hemisphere. This is
Riley A. DeColibus +2 more
doaj +1 more source
Titania's Heat Fluxes Revealed by Messina Chasmata
Messina Chasmata is a relatively young tectonic structure on Titania based on cross-cutting relationships, although an absolute age has not been estimated.
Chloe B. Beddingfield +4 more
doaj +1 more source
Are NH3 and CO2 Ice Present on Miranda?
Published near-IR spectra of the four largest classical Uranian satellites display the presence of discrete deposits of CO _2 ice, along with subtle absorption features around 2.2 μ m.
Riley A. DeColibus +2 more
doaj +1 more source
Dynamical Interactions and Mass Loss within the Uranian System
The origin and evolution of planetary rings and moons remains an active area of study, particularly as they relate to the impact history and volatile inventory of the outer solar system.
Stephen R. Kane, Zhexing Li
doaj +1 more source
A ring system detected around the Centaur (10199) Chariklo [PDF]
Hitherto, rings have been found exclusively around the four giant planets in the Solar System1. Rings are natural laboratories in which to study dynamical processes analogous to those that take place during the formation of planetary systems and galaxies.
Vanzi, L. +232 more
core +1 more source
Near-infrared spectra of Umbriel and the other classical Uranian moons exhibit 2.2 μ m absorption bands that could result from ammonia (NH _3 ) bearing species, possibly exposed in the geologically recent past.
Richard J. Cartwright +5 more
doaj +1 more source
Cupid is doomed: An analysis of the stability of the inner uranian satellites [PDF]
We have explored the stability of the inner Uranian satellites using simulations based on the most recent observational data. We find that, across a wide range of mass assumptions, the system is unstable, resulting in the eventual crossing of orbits and probable subsequent collision of moons.
French, Robert S., Showalter, Mark R.
openaire +2 more sources
Astrometric observations of Uranian and Neptunian satellites with the Pulkovo and Crimean observatory telescopes in 2020 [PDF]
В работе представлены результаты наблюдений спутников Урана и Нептуна, выполненных в 2020 г. с помощью метрового зеркального телескопа «Сатурн» (ГАО РАН) и 350-мм гида телескопа «Синтез» (КрАО РАН). Получено более 8 тыс.
Khovritchev, M. Yu. +5 more
core +1 more source
A CO2 Cycle on Ariel? Radiolytic Production and Migration to Low-latitude Cold Traps
CO _2 ice is present on the trailing hemisphere of Ariel but is mostly absent from its leading hemisphere. The leading/trailing hemispherical asymmetry in the distribution of CO _2 ice is consistent with radiolytic production of CO _2 , formed by charged
Richard J. Cartwright +13 more
doaj +1 more source

