Bradford A. Smith,Laurence A. Soderblom,Torrence V. Johnson,Andrew P. Ingersoll,Stewart A. Collins,Eugene M. Shoemaker,Garry E. Hunt,Harold Masursky,Michael H. Carr,Merton E. Davies,A. F. Cook,Joseph M. Boyce,G. Edward Danielson,Tobias Owen,Carl Sagan,Reta Beebe,Joseph Veverka,Robert G. Strom,John F. McCauley,David Morrison,G. A. Briggs,Verner E. Suomi
出处
期刊:Science [American Association for the Advancement of Science (AAAS)] 日期:1979-06-01卷期号:204 (4396): 951-972被引量:630
标识
DOI:10.1126/science.204.4396.951
摘要
The cameras aboard Voyager 1 have provided a closeup view of the Jupiter system, revealing heretofore unknown characteristics and phenomena associated with the planet's atmosphere and the surfaces of its five major satellites. On Jupiter itself, atmospheric motions-the interaction of cloud systems-display complex vorticity. On its dark side, lightning and auroras are observed. A ring was discovered surrounding Jupiter. The satellite surfaces display dramatic differences including extensive active volcanism on Io, complex tectonism on Ganymede and possibly Europa, and flattened remnants of enormous impact features on Callisto.