Io's thermal emission from the Galileo photopolarimeter-radiometer

被引:102
作者
Spencer, JR
Rathbun, JA
Travis, LD
Tamppari, LK
Barnard, L
Martin, TZ
McEwen, AS
机构
[1] Lowell Observ, Flagstaff, AZ 86001 USA
[2] NASA, Goddard Space Flight Ctr, Inst Space Studies, New York, NY 10025 USA
[3] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[4] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
关键词
D O I
10.1126/science.288.5469.1198
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Galileo's photopolarimeter-radiometer instrument mapped to's thermal emission during the 124, 125, and 127 flybys with a spatial resolution of 2.2 to 300 kilometers. Mapping of Loki in 124 shows uniform temperatures for most of Loki Patera and high temperatures in the southwest corner, probably resulting from an eruption that began 1 month before the observation. Most of Loki Patera was resurfaced before 127. Pele's caldera floor has a low temperature of 160 kelvin, whereas flows at Pillan and Zamama have temperatures of up to 200 kelvin, Global maps of nighttime temperatures provide a means for estimating global heat flow.
引用
收藏
页码:1198 / 1201
页数:4
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