Hostname: page-component-848d4c4894-nr4z6 Total loading time: 0 Render date: 2024-06-03T00:04:25.427Z Has data issue: false hasContentIssue false

The Origin of Uranus: Compositional Considerations

Published online by Cambridge University Press:  12 April 2016

M. Podolak*
Affiliation:
Dept. of Geophysics and Planetary Sciences, Tel-Aviv University, Ramat Aviv, Israel

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Several cosmogonic theories are examined for their ability to explain the details of Uranus’ composition as inferred from observations and interior models. Suggestions are made as to how future work may enable us to decide among competing scenarios.

Type
Present Knowledge of Uranus
Copyright
Copyright © Cambridge University Press 1982

References

Belton, M.J.S., Wallace, L., Hayes, S.H., and Price, M.J. (1980). Neptune’s rotation period: A correction and a speculation on the differences between photometric and spectroscopic results. Icarus 42, 7178.CrossRefGoogle Scholar
Black, D.C. (1973). Deuterium in the early solar system. Icarus 19, 154159.Google Scholar
Brown, R.A., and Goody, R.M. (1980). The rotation of Uranus II. Astrophys. J. 235, 10661070.CrossRefGoogle Scholar
Cameron, A.G.V. (1978a). The primitive solar accretion disk and the formation of the planets. In The Origin of the Solar System (Dermott, S.F., ed) pp. 4974. John Wiley & Sons, New York.Google Scholar
Cameron, A.G.W. (1978b). Physics of the primitive solar nebula and of giant gaseous protoplanets. In Protostars and Protoplanets (Gehrels, T., ed.) pp. 453487. Univ. of Arizona Press, Tucson.Google Scholar
Cameron, A.G.W. (1979). The interaction between giant gaseous protoplanets and the primitive solar nebula. Moon and Planets 21, 173183.Google Scholar
Cameron, A.G.W. (1980). Elementary and nuclidic abundances in the solar system. To appear in A Festschrift in Honor of Willy Fowler’s 70th Birthday.Google Scholar
DeCampli, W., and Cameron, A.G.W. (1979). Structure and evolution of isolated giant gaseous protoplanets. Icarus 38, 367391.CrossRefGoogle Scholar
Elliot, J.L., French, R.G., Frogel, J., Elias, J.H., Mink, D.J., and Liller, W. (1981). Orbits of nine Uranian rings. Astron. J. in press.Google Scholar
Franklin, F.A., Avis, C.C., Columbo, C., and Shapiro, I.I. (1980). Geometric oblateness of Uranus. Astrophys. J. 236, 10311034.CrossRefGoogle Scholar
Goody, R.M. (1981). The rotation of Uranus. This volume.Google Scholar
Grossman, L. (1972). Condensation in the primitive solar nebula. Geochim. et Cosmochim. Acta 36, 597619.Google Scholar
Gulkis, S., Janssen, M.A., and Olsen, E.T. (1978). Evidence for the depletion of ammonia in the Uranus atmosphere. Icarus 34, 1019.CrossRefGoogle Scholar
Handbury, M.J., and Williams, I.P. (1975). The formation of the outer planets. Astrophys. and Space Sci. 38, 2937.Google Scholar
Hubbard, W.B., and MacFarlane, J.J. (1980a). Structure and evolution of Uranus and Neptune. J. Geophys. Res. 85, 225234.Google Scholar
Hubbard, W.B., and MacFarlane, J.J. (1980b). Theoretical predictions of deuterium abundances in the Jovian planets. Icarus, in press.CrossRefGoogle Scholar
Lewis, J.S. (1972). Low temperature condensation from the solar nebula. Icarus 16, 241252.Google Scholar
Lewis, J.S., and Prinn, R.G. (1980). Kinetic inhibition of CO and N9 reduction in the solar nebula. Astrophys. J. 238, 357364.Google Scholar
McCrea, W.H. (1978). The formation of the solar system: A proto-planet theory. In The Origin of the Solar System (Dermott, S.F., ed.) pp. 75110, John Wiley & Sons, New York.Google Scholar
Macy, W. Jr., and Smith, W.H. (1978). Detection of HD on Saturn and Uranus and the D/H ratio. Astrophys. J. 222, L73L75.CrossRefGoogle Scholar
Mizuno, H. (1980). Formation of the giant planets. Prog. Theoretical Phys. 64, 544557.Google Scholar
Munch, G., and Hippelein, H. (1980). The effects of seeing on the reflected spectrum of Uranus and Neptune. Astron. Astrophys. 81, 289197.Google Scholar
Nicholson, P.D., Persson, S.E., Matthews, K., Goldreich, P., and Neugebauer, G. (1978). The rings of Uranus: Results of the 1978 April 10 occultation. Astron. J. 83, 12401248.Google Scholar
Norris, T.L., (1980). Kinetic model of ammonia synthesis in the solar nebula. Earth and Planet. Sci. Lett. 47, 4350.Google Scholar
Perri, F., and Cameron, A.G.W. (1974). Hydrodynamic instability of the solar nebula in the presence of a planetary core. Icarus 22, 416425.Google Scholar
Podolak, M. (1976). Methane rich models of Uranus. Icarus 27, 473478.Google Scholar
Podolak, M., and Cameron, A.G.W. (1974). Models of the giant planets. Icarus 22, 123148.Google Scholar
Podolak, M., and Reynolds, R.T. (1981). On the structure of Uranus and Neptune. Icarus, 45, in press.Google Scholar
Prentice, A.J.R. (1978). Towards a modern Laplacian theory for the formation of the solar system. In The Origin of the Solar System (Dermott, S.F., ed.) pp. 111162. John Wiley & Sons, New York.Google Scholar
Prinn, R.G., and Lewis, J.S. (1973). Uranus atmosphere structure and composition. Astrophys. J. 179, 333342.Google Scholar
Reynolds, R.T., and Summers, A.L. (1965). Models of Uranus and Neptune. J. Geophys. Res. 70, 199208.Google Scholar
Richet, P., Bottinga, Y., and Javoy, M.A. (1977). A review of hydrogen, carbon, nitrogen, oxygen, sulfur, and chlorine stable isotope fractionation among gaseous molecules. Rev. E. & P. Sci. 5, 65110.Google Scholar
Russel, N.N. (1935). The Solar System and its Origin. Macmillan, New York.Google Scholar
Safronov, V.S. (1972). Evolution of the Protoplanetary Cloud and Formation of the Earth and Planets, Nauka, Moscow. Transl, from Russian Israel Program for Scientific Translation, Jerusalem.Google Scholar
Slattery, W. (1978). Protoplanetary core formation by rainout of iron drops. Moon and Planets 19, 443456.Google Scholar
Smith, H.J., and Slavsky, D.B. (1979). Rotation period of Uranus. Bull. Amer. Astron. Soa. 11, 568.Google Scholar
Spitzer, L. Jr. (1939). The dissipation of planetary filaments. Astrophys. J. 90, 675688.CrossRefGoogle Scholar
Trafton, L., and Ramsay, D.A. (1980). The D/H ratio in the atmosphere of Uranus: Detection of the R,-(1) line of HD. Icarus, 41, 423429.CrossRefGoogle Scholar
Woolfson, M.M. (1978a). The capture theory and the origin of the solar system. In The Origin of the Solar System (Dermott, S.F., ed.) pp. 179198. John Wiley & Sons, New York.Google Scholar
Woolfson, M.M. (1978b). The evolution of the solar system. In The Origin of the Solar System (Dermott, S.P., ed.) pp. 199217.Google Scholar
Zharkov, V.N., and Trubitsyn, V.P. (1978). Physics of Planetary Interiors Hubbard, C.W.B., Transl, and ed.) Pachart, Tucson, Ariz.Google Scholar