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Volumn 311, Issue 5766, 2006, Pages 1425-1428

Composition and physical properties of Enceladus' surface

(25)  Brown, Robert H a   Clark, Roger N b   Buratti, Bonnie J c   Cruikshank, Dale P d   Barnes, Jason W a   Mastrapa, Rachel M E d   Bauer, J c   Newman, S c   Momary, T c   Baines, K H c   Bellucci, G e   Capaccioni, F f   Cerroni, P f   Combes, M g   Coradini, A f   Drossart, P g   Formisano, V e   Jaumann, R h   Langavin, Y i   Matson, D L c   more..

e INAF   (Italy)

Author keywords

[No Author keywords available]

Indexed keywords

AMMONIA; AMORPHOUS MATERIALS; CARBON DIOXIDE; CARBON MONOXIDE; CRYSTALLINE MATERIALS; INFRARED SPECTROMETERS; PHYSICAL PROPERTIES; SPACE RESEARCH;

EID: 33644858580     PISSN: 00368075     EISSN: 10959203     Source Type: Journal    
DOI: 10.1126/science.1121031     Document Type: Article
Times cited : (210)

References (27)
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    • note
    • To establish upper limits on temperature, we used a Levenberg-Marquardt algorithm to fit the co-added tiger stripes spectrum to the spectrum of the interstripe region with the use of a multiplicative albedo-surrogate scaling factor and surface temperature as free parameters. The best fit temperature is indistinguishable from 0 K. We then increased the temperature of either the full pixel or a linear swath through the pixel until the quality of the fit degraded to the 3σ level and used that value for the upper limit.


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