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JupiterThe physical structure of Jupiter is discussed on the basis of data obtained by Pioneers 10 and 11. It is argued that the elemental composition of Jupiter is similar to that of the sun, and it is shown that this argument is supported by measurements of the planet's density and H/He ratio. Jupiter's shape and gravitational field are described, and a model of the planet is proposed in which there are a small iron-silicate core at the center, a very thick liquid-hydrogen stratum divided into metallic (inner) and molecular (outer) layers, and a gaseous atmosphere. According to this model, the excess heat radiated by Jupiter is simply a remnant of the heat generated when the planet coalesced from the solar nebula. The appearance of the planetary disk is described together with the Jovian magnetic field, and the Great Red Spot is shown to be a cyclonic disturbance similar to a hurricane. Effects of the Galilean satellites on the magnetic field are considered.
Document ID
19750058412
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Wolfe, J. H.
(NASA Ames Research Center Space-Physics Branch, Moffett Field, Calif., United States)
Date Acquired
August 8, 2013
Publication Date
September 1, 1975
Publication Information
Publication: Scientific American
Volume: 233
Subject Category
Lunar And Planetary Exploration
Accession Number
75A42484
Distribution Limits
Public
Copyright
Other

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