Results 91 to 100 of about 723,831 (225)

Laboratory studies of the interaction of ions with condensed gases: Planetary applications [PDF]

open access: yes, 1990
The work described is concerned with laboratory studies of the processes that produce the ejection of molecules from the surfaces of condensed gas solids, the change in the chemistry of the surface materials, and the relationship of these results to ...
Boring, J. W., Johnson, R. E.
core   +1 more source

Observations of Titan’s Stratosphere during Northern Summer: Temperatures, CH3CN and CH3D Abundances

open access: yesThe Planetary Science Journal
Titan’s atmospheric composition and dynamical state have previously been studied over numerous epochs by both ground- and space-based facilities. However, stratospheric measurements remain sparse during Titan’s northern summer and fall.
Alexander E. Thelen   +13 more
doaj   +1 more source

Near-Infrared Photometry of Irregular Satellites of Jupiter and Saturn

open access: yes, 2004
We present JHKs photometry of 10 Jovian and 4 Saturnian irregular satellites, taken with the Near-InfraRed Imager (NIRI) at the 8-m Gemini North Observatory on Mauna Kea, Hawaii.
Grav T., Matthew J. Holman, Tommy Grav
core   +1 more source

Ice Formation, Exsolution, and Multiphase Equilibria in the Methane–Ethane–Nitrogen System at Titan Surface Conditions

open access: yesThe Planetary Science Journal
Titan is unique among the icy satellites in that it has a thick atmosphere, stable surficial bodies of liquid, and a precipitation system that promotes interactions between the two.
Anna E. Engle   +11 more
doaj   +1 more source

Packed media radiative-transfer modeling with Gaussian particles: application to spectra of icy regolith of Saturnian satellites

open access: yesJournal of Quantitative Spectroscopy and Radiative Transfer, 2022
G. Ito   +3 more
semanticscholar   +1 more source

Resonant Stratification in Titan’s Global Ocean

open access: yesThe Planetary Science Journal
Titan’s ice shell floats on top of a global ocean, as revealed by the large tidal Love number k _2 = 0.616 ± 0.067 registered by Cassini. The Cassini observation exceeds the predicted k _2 by one order of magnitude in the absence of an ocean, and is 3 σ ...
Benjamin Idini, Francis Nimmo
doaj   +1 more source

Origin and Evolution of Enceladus's Tidal Dissipation. [PDF]

open access: yesSpace Sci Rev, 2023
Nimmo F, Neveu M, Howett C.
europepmc   +1 more source

Origin and evolution of the Saturn system [PDF]

open access: yes
A review is provided of current concepts concerning the formation of the Saturn system and the subsequent history of the planet, its satellites, and rings.
Consolmagno, G., Pollack, J. B.
core   +1 more source

Saturn's Icy Moon Rhea: a Prediction for Bulk Chemical Composition and Physical Structure at the Time of the Cassini Spacecraft First Flyby

open access: yes, 2005
I report a model for the formation of Saturn's family of mid-sized icy moons to coincide with the first flypast of Rhea by the Cassini Orbiter spacecraft on 26 November 2005.
Andrew J. R. Prentice   +18 more
core   +1 more source

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