Thermal properties of Pluto’s and Charon’s surfaces from Spitzer observations
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TNOs are cool: A survey of the trans-Neptunian regionSurface compositions across Pluto and Charon.Observed glacier and volatile distribution on Pluto from atmosphere-topography processes.Haze heats Pluto's atmosphere yet explains its cold temperature.“TNOs are Cool”: A survey of the trans-Neptunian region“TNOs are Cool”: A survey of the trans-Neptunian region“TNOs are Cool”: A survey of the trans-Neptunian region
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Thermal properties of Pluto’s and Charon’s surfaces from Spitzer observations
description
article
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im August 2011 veröffentlichter wissenschaftlicher Artikel
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wetenschappelijk artikel
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наукова стаття, опублікована в серпні 2011
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ലേഖനം
@ml
name
Thermal properties of Pluto’s and Charon’s surfaces from Spitzer observations
@en
Thermal properties of Pluto’s and Charon’s surfaces from Spitzer observations
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type
label
Thermal properties of Pluto’s and Charon’s surfaces from Spitzer observations
@en
Thermal properties of Pluto’s and Charon’s surfaces from Spitzer observations
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prefLabel
Thermal properties of Pluto’s and Charon’s surfaces from Spitzer observations
@en
Thermal properties of Pluto’s and Charon’s surfaces from Spitzer observations
@nl
P2093
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P1433
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Thermal properties of Pluto’s and Charon’s surfaces from Spitzer observations
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P2093
Dale P. Cruikshank
Emmanuel Lellouch
John Stansberry
Josh Emery
Will Grundy
P304
P356
10.1016/J.ICARUS.2011.05.035
P577
2011-08-01T00:00:00Z