Hot spots on Io: Initial results from Galileo's near infrared mapping spectrometer

被引:48
作者
LopesGautier, R
Davies, AG
Carlson, R
Smythe, W
Kamp, L
Soderblom, L
Leader, FE
Mehlman, R
机构
[1] US GEOL SURVEY,BRANCH ASTROGEOL STUDIES,FLAGSTAFF,AZ 86001
[2] UNIV CALIF LOS ANGELES,INST GEOPHYS & PLANETARY PHYS,LOS ANGELES,CA 90024
关键词
D O I
10.1029/97GL02662
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The Near-Infrared Mapping Spectrometer on Galileo has monitored the volcanic activity on Io since June 28, 1996. This paper presents preliminary analysis of NIMS thermal data for the first four orbits of the Galileo mission. NIMS has detected 18 new hot spots and 12 others which were previously known to be active. The distribution of the hot spots on Io's surface may not be random, as hot spots surround the two bright, SO2-rich regions of Bosphorus Regio and Colchis Regio. Most hot spots seem to be persistently active from orbit to orbit and 10 of those detected were active in 1979 during the Voyager encounters. We report the distribution of hot spot temperatures and find that they are consistent with silicate volcanism.
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页码:2439 / 2442
页数:4
相关论文
共 13 条
[1]  
[Anonymous], SATELLITES JUPITER
[2]  
[Anonymous], 1982, SATELLITES JUPITER
[3]  
CARLSON RW, 1992, SPACE SCI REV, V60, P457, DOI 10.1007/BF00216865
[4]   A MODEL FOR LAVA FLOWS WITH 2 THERMAL COMPONENTS [J].
CRISP, J ;
BALOGA, S .
JOURNAL OF GEOPHYSICAL RESEARCH-SOLID EARTH AND PLANETS, 1990, 95 (B2) :1255-1270
[5]   LARGE-SCALE TOPOGRAPHY OF IO - IMPLICATIONS FOR INTERNAL STRUCTURE AND HEAT-TRANSFER [J].
GASKELL, RW ;
SYNNOTT, SP ;
MCEWEN, AS ;
SCHABER, GG .
GEOPHYSICAL RESEARCH LETTERS, 1988, 15 (06) :581-584
[6]  
LOPESGAUTIER R, 1997, LUNAR PLANET SCI C, V27, P831
[7]  
McEwen A.S., 1992, LUNAR PLANET SCI, VXXIII, P881
[8]  
McEwen A. S, 1989, NASA SP, V464, P11
[9]   SO2-RICH EQUATORIAL BASINS AND EPEIROGENY OF IO [J].
MCEWEN, AS .
ICARUS, 1995, 113 (02) :415-422
[10]  
MCEWEN AS, 1992, B AM ASTRON SOC, V24, P935