A multilayer model for thermal infrared emission of Saturn's rings. III: Thermal inertia inferred from Cassini CIRS

Details A multilayer model for thermal infrared emission of Saturn's rings. III: Thermal inertia inferred from Cassini CIRS A multilayer model for thermal infrared emission of Saturn's rings. III: Thermal inertia inferred from Cassini CIRS

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011icar..215..107m&link_type=abstract

Icarus, Volume 215, Issue 1, p. 107-127.

Physics

Scientific paper

The thermal inertias of Saturn's ring particles are 11-20 in MKS
units. The apparent thermal inertia increases with increasing
solar phase angle. The thermal inertias of small fast rotators
are 27-77 in MKS units. The thermal inertias of large slow
rotators are 5-9 in MKS units.

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