Discovery of Ganymede's magnetic field by the Galileo spacecraft

被引:284
作者
Kivelson, MG
Khurana, KK
Russell, CT
Walker, RJ
Warnecke, J
Coroniti, FV
Polanskey, C
Southwood, DJ
Schubert, G
机构
[1] UNIV CALIF LOS ANGELES,DEPT EARTH & SPACE SCI,LOS ANGELES,CA 90095
[2] UNIV CALIF LOS ANGELES,DEPT PHYS,LOS ANGELES,CA 90095
[3] CALTECH,JET PROP LAB,PASADENA,CA 91109
[4] UNIV LONDON IMPERIAL COLL SCI TECHNOL & MED,DEPT PHYS,LONDON SW7 2BZ,ENGLAND
关键词
D O I
10.1038/384537a0
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
THE Galileo spacecraft has now passed close to Jupiter's largest moon-Ganymede-on two occasions, the first at an altitude of 838 km, and the second at an altitude of just 264 km. Here we report the discovery during these encounters of an internal magnetic field associated with Ganymede (the only other solid bodies in the Solar System known to have magnetic fields are Mercury, Earth and probably Io(1)), The data are consistent with a Ganymede-centred magnetic dipole tilted by similar to 10 degrees relative to the spin axis, and an equatorial surface-field strength of similar to 750 nT, The magnetic field is strong enough to carve out a magnetosphere with clearly defined boundaries within Jupiter's magnetosphere, Although the observations require an internal field, they do not indicate its source. But the existence of an internal magnetic field should in itself help constrain models of Ganymede's interior.
引用
收藏
页码:537 / 541
页数:5
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