Thermal properties of Rhea's poles: Evidence for a meter-deep unconsolidated subsurface layer-Reference-Cited by-同舟云学术

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Thermal properties of Rhea's poles: Evidence for a meter-deep unconsolidated subsurface layer

Published:2016-07 Issue: Volume:272 Page:140-148
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Howett C.J.A.,Spencer J.R.,Hurford T.,Verbiscer A.,Segura M.

Funder

Cassini Project

Cassini Data Analysis Program

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference33 articles.

1. The spectrum of (136199) Eris between 350 and 2350nm: Results with X-Shooter;Alvarez-Candal;Astron. Astrophys.,2011

2. Effect of porosity on the adsorption, desorption, trapping and release of volatile gases by amorphous solid water;Ayotte;J. Geophys. Res.,2001

3. Lunar surface roughness derived from LRO Diviner Radiometer;Bandfield;Icarus,2015

4. Constraining the surface properties of Saturn's icy moons, using Cassini/CIRS emissivity spectra;Carvano;Icarus,2007

5. Hapke modeling of Rhea surface properties through Cassini-VIMS spectra;Ciarniello;Icarus,2011

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3. Investigation of heat transfer processes in multi-sized solar-sintered regolith for lunar ISRU program;International Journal of Heat and Mass Transfer;2023-11

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5. Dione’s Thermal Inertia and Bolometric Bond Albedo Derived from Cassini/CIRS Observations of Solar Eclipse Ingress;The Planetary Science Journal;2022-08-01

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