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- W1988433657 abstract "Analysis of 2008 Cassini Composite Infrared Spectrometer (CIRS) 10 to 600/cm thermal emission spectra of Enceladus shows that for reasonable assumptions about the spatial distribution of the emission and the thermophysical properties of the solar-heated background surface, which are supported by CIRS observations of background temperatures at the edge of the active region, the endogenic power of Enceladus' south polar terrain is 15.8 +/- 3.1 GW. This is significantly higher than the previous estimate of 5.8 +/- 1.9 GW. The new value represents an improvement over the previous one, which was derived from higher wave number data (600 to 1100/cm-I) and was thus only sensitive to high-temperature emission. The mechanism capable of producing such a high endogenic power remains a mystery and challenges the current models of proposed heat production." @default.
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- W1988433657 date "2011-03-04" @default.
- W1988433657 modified "2023-10-18" @default.
- W1988433657 title "High heat flow from Enceladus' south polar region measured using 10–600 cm<sup>−1</sup>Cassini/CIRS data" @default.
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- W1988433657 doi "https://doi.org/10.1029/2010je003718" @default.
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