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Giant planet formation: a first classification of isothermal protoplanetary equilibria
B. Pečnik, G. Wuchterl
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Mercury Concentrations in Feathers of Albatrosses and Large Petrels at South Georgia: Contemporary Patterns and Comparisons with Past Decades. [PDF]
Mills WF+4 more
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Polling the Public to Select Flagship Species for Tourism and Conservation-A 'Big Five' for the Peruvian Amazon? [PDF]
Recharte M, Lee PC, Vick SJ, Bowler M.
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The giant planets contain the bulk of the angular momentum of the solar system and the dominant mass among the planets. The magnetosphere of the Jovian system dwarfs the Sun in size. Jupiter, Saturn, and Neptune radiate considerably more energy than they receive from the Sun.
Eugene F. Milone, William J. F. Wilson
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Interiors of the Giant Planets [PDF]
Unlike the terrestrial planets, the giant planets—Jupiter, Saturn, Uranus, and Neptune—have retained large amounts of the carbon, nitrogen, and oxygen compounds that were present in their zone of formation. A smaller fraction of the available hydrogen and helium was retained. The distribution and relative amounts of these components in the interiors of
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GIANT PLANET MAGNETOSPHERES [PDF]
The classification of the giant planet magnetospheres into two varieties is examined: the large symmetric magnetospheres of Jupiter and Saturn and the smaller irregular ones of Uranus and Neptune. The characteristics of the plasma and the current understanding of the magnetospheric processes are considered for each planet.
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