Hostname: page-component-848d4c4894-cjp7w Total loading time: 0 Render date: 2024-07-04T04:53:09.887Z Has data issue: false hasContentIssue false
  • English
  • Français

Status of Molecular Opacities of Interest in the Modeling of a Proto-Solar Nebula

Published online by Cambridge University Press:  14 August 2015

W. F. Huebner  and
L. W. Fullerton
W. F. Huebner
Affiliation:
Los Alamos Scientific Laboratory, Los Alamos, N.M., U.S.A.
L. W. Fullerton
Affiliation:
Los Alamos Scientific Laboratory, Los Alamos, N.M., U.S.A.

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.

The report centers on general procedures applicable to the calculation of constitutive properties (equation of state and opacity) of media that serve as models for the solar nebula during planet formation and for the atmospheres of some planets. Specifically considered are the equilibrium compositions of a mixture of atoms, molecules, and their ionic species in the gaseous phase, condensation into grains with refractory cores and mantles of volatile compounds, and the ‘optical’ properties of the grain-gas medium. A summary of available and still needed basic (input) data and some currently available results are presented.

Type
Part I Origin and General Physics of the Planetary System
Information
Symposium - International Astronomical Union , Volume 65: Exploration of the Planetary System , 1974 , pp. 13 - 20
Copyright
Copyright © Reidel 1974 

References

Alexander, D., Collins, J., Fay, T., and Johnson, H. R.: 1971, Bull. Am. Astron. Soc. 3, 380.Google Scholar
Anders, E.: 1968, Accounts Chem. Res. 1, 289.Google Scholar
Anders, E.: 1971, Ann. Rev. Astron. Astrophys. 9, 1.Google Scholar
Armstrong, B. H. and Nicholls, R. W.: 1967, ‘Thermal Radiation Phenomena, Vol. 2, The Equilibrium Radiative Properties of Air-Theory’, Lockheed Missiles and Space Company report LMSC-3-27-67-1.Google Scholar
Auman, J. A. and Bodenheimer, P.: 1967, Astrophys. J. 149, 641.Google Scholar
Avilova, I. V., Biberman, L. M., Vorobjev, V. S., Zamalin, V. M., Kobzev, G. A., Lagar'kov, A. N., Mnatsakanian, A. Ch., and Norman, G. E.: 1969a, J. Quant. Spectrosc. Radiat. Transfer 9, 89.Google Scholar
Avilova, I. V., Biberman, L. M., Vorobjev, V. S., Zamalin, V. M., Kobzev, G. A., Lagar'kov, A. N., Mnatsakanian, A. Ch., and Norman, G. E.: 1969b, J. Quant. Spectrosc. Radiat. Transfer 9, 113.Google Scholar
Carbon, D., Gingerich, O. J., and Latham, D. W.: 1969, in Kumar, S. S. (ed.), Low Luminosity Stars, Gordon and Breach Science Publishers, New York, p. 435.Google Scholar
Cox, A. N. and Stewart, J. N.: 1965, Astrophys. J. Suppl. 11, 22.Google Scholar
Dressler, K.: 1969, Can. J. Phys. 47, 547.Google Scholar
Duff, R. E. and Bauer, S. H.: 1962, J. Chem. Phys. 36, 1754.Google Scholar
Gaustad, J. E.: 1963, Astrophys. J. 138, 1050.Google Scholar
Generosa, J. I. and Harris, R. A.: 1973, Air Force Weapons Laboratory, Kirtland AFB, N.M., private communication.Google Scholar
Gilmore, F. R.: 1965, J. Quant. Spectrosc. Radiat. Transfer 5, 125.Google Scholar
Gilmore, F. R.: 1967, ‘Thermal Radiation Phenomena, Vol. 1, The Equilibrium Radiative Properties of Air’, Lockheed Missiles and Space Company report LMSC-3-27-67-1.Google Scholar
Greenberg, J. M.: 1970, in Donahue, T. M., Smith, P. A., and Thomas, L. (eds.), Space Research X, North-Holland Publishing Company-Holland, p. 225.Google Scholar
Hayashi, C. and Nakano, T.: 1965, Progr. Theor. Phys. 34, 764.Google Scholar
Hayatsu, R., Studier, M. H., Oda, A., Fuse, K., and Anders, E.: 1968, Geochim. Cosmochim. Acta 32, 175.Google Scholar
Huffman, D. R. and Stapp, J. L.: 1971, Nature Phys. Sci. 229, 45.Google Scholar
Johnston, R. R., Landshoff, R. K. M., and Platas, O. R.: 1972, ‘Radiative Properties of High Temperature Air’, Lockheed Missiles and Space Company report LMSC D 267205.Google Scholar
Larimer, J. W.: 1967, Geochim. Cosmochim. Acta 31, 1215.Google Scholar
Larimer, J. W. and Anders, E.: 1967, Geochim. Cosmochim. Acta 31, 1239.Google Scholar
Linsky, J. L.: 1969, Astrophys. J. 156, 989.Google Scholar
Merts, A. L. and Magee, N. H.: 1973, Bull. Am. Astron. Soc. 5, 338.Google Scholar
Studier, M. H., Hayatsu, R., and Anders, E.: 1968, Geochim. Cosmochim. Acta 32 151.Google Scholar
Tsuji, T.: 1964, Proc. Japan Acad. 40, 99.Google Scholar
Tsuji, T.: 1966, Publ. Astron. Soc. Japan 18, 127; corrected: 1967, Publ. Astron. Soc. Japan 19, 119.Google Scholar
Tsuji, T.: 1971, Publ. Astron. Soc. Japan 23, 553.Google Scholar
Wacker, P. F. and Pratto, M. R.: 1964, ‘Spectral Tables, Line Strength of Asymmetric Rotors’, NBS Monograph 70 Vol. II, U.S. Government Printing Office, Washington, D. C. Google Scholar