The control networks of the Galilean satellites and implications for global shape

被引:34
作者
Davies, ME
Colvin, TR
Oberst, J
Zeitler, W
Schuster, P
Neukum, G
McEwen, AS
Phillips, CB
Thomas, PC
Veverka, J
Belton, MJS
Schubert, G
机构
[1] Rand Corp, Santa Monica, CA 90407 USA
[2] DLR, Inst Planetenerkundung Andershof, D-12489 Berlin, Germany
[3] Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
[4] Natl Opt Astron Observ, Tucson, AZ 85726 USA
[5] Univ Calif Los Angeles, Los Angeles, CA 90095 USA
关键词
Io; Europa; Ganymede; Callisto; satellites of Jupiter;
D O I
10.1006/icar.1998.5982
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Images from the Galileo mission to Jupiter have been combined with earlier Voyager images to produce improved geodetic control networks for the Galilean satellites. The improved geometric stability and lack of scene-dependent distortions of the Galileo images compensate for their relatively small number. Triaxial solutions are derived for the principal axes of the satellites by assuming an equilibrium constrained by the gravity potential coefficients. The control network is used in the preparation of planimetric maps by relating the images to the latitude/longitude grid. (C) 1998 Academic Press.
引用
收藏
页码:372 / 376
页数:5
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