Results 321 to 330 of about 3,157,542 (333)
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2013
This chapter examines Jupiter's climate and what it reveals about the solar system. During its first 105 years, the solar system was a melting pot in which material from stars with different chemical compositions was blended together. The high temperatures resulting from the release of enormous amounts of gravitational potential energy aided the ...
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This chapter examines Jupiter's climate and what it reveals about the solar system. During its first 105 years, the solar system was a melting pot in which material from stars with different chemical compositions was blended together. The high temperatures resulting from the release of enormous amounts of gravitational potential energy aided the ...
openaire +1 more source
Formation of the Giant Planets by Concurrent Accretion of Solids and Gas
, 1995New numerical simulations of the formation of the giant of the second phase. planets are presented, in which for the first time both the gas and The actual rates at which the giant planets accreted small planetesimal accretion rates are calculated in a ...
J. Pollack +5 more
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Science, 2005
Jupiter The Planet, Satellites and Magnetosphere. Fran Bagenal, Timothy E. Dowling, and William B. McKinnon, Eds. . Cambridge University Press, Cambridge, 2004. 731 pp. + CD-ROM. $150, £85. ISBN 0-521-81808-7. Cambridge Planetary Science.
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Jupiter The Planet, Satellites and Magnetosphere. Fran Bagenal, Timothy E. Dowling, and William B. McKinnon, Eds. . Cambridge University Press, Cambridge, 2004. 731 pp. + CD-ROM. $150, £85. ISBN 0-521-81808-7. Cambridge Planetary Science.
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Formation of gas and ice giant planets
Earth and Planetary Science Letters, 2002Abstract Agreement about planetary formation processes deteriorates sharply with distance from the Sun. While the terrestrial planets are widely believed to have formed from the collisional accumulation of solid bodies, there are two competing mechanisms for the formation of the gas giant planets, basically ‘bottom-up’ or ‘top-down’.
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Voyager 2's Encounter with the Gas Giants
Physics Today, 1990It was 3:40 am Pacific daylight time, 25 August 1989. I had watched with fascination a video display of Voyager 2's radio signal after the spacecraft had passed through Neptune's thick atmosphere, and for the last 90 minutes I had been attempting to nap in a sleeping bag on the floor of my office at JPL. My computer had just awakened me with a reminder
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Simulation of deep-seated zonal jets and shallow vortices in gas giant atmospheres
, 2016M. Heimpel, T. Gastine, Johannes Wicht
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