Hostname: page-component-669899f699-ggqkh Total loading time: 0 Render date: 2025-04-26T14:18:07.676Z Has data issue: false hasContentIssue false
  • English
  • Français

The Location of the Snow Line in Protostellar Disks

Published online by Cambridge University Press:  06 April 2010

Morris Podolak
Morris Podolak*
Affiliation:
Dept. of Geophysics and Planetary Sciences, Tel Aviv University, Tel Aviv, Israel email: [email protected]
Rights & Permissions [Opens in a new window]

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 snow line in a gas disk is defined as the distance from the star beyond which the water ice is stable against evaporation. Since oxygen is the most abundant element after hydrogen and helium, the presence of ice grains can have important consequences for disk evolution. However, determining the position of the snow line is not simple. I discuss some of the important processes that affect the position of the snow line.

Keywords

Planetary systems: protoplanetary disksdustextinctionsolar system: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Symposium S263: Icy Bodies of the Solar System , August 2009 , pp. 19 - 28
Copyright
Copyright © International Astronomical Union 2010

References

Armitage, P. J. 2009, astro-ph/0701485v2Google Scholar
Anders, E. & Grevasse, N. 1989, Geochim. Cosmochim. Acta, 53, 197Google Scholar
Bell, K. R., Cassen, P. M., Klahr, H. H., & Henning, Th. 1997, ApJ, 486, 372Google Scholar
Hayashi, C. 1981 Prog. Theor. Phys. Suppl., 70, 35Google Scholar
Honda, M., Inoue, A. K., Fukagawa, M., Oka, A., Nakamoto, T., Ishii, M., Terada, H., Takato, N., Kawakita, H., Okamoto, Y. K., Shibai, H., Tamura, M., Kudo, T., & Itoh, Y. 2009, ApJ Lett., 690, L110Google Scholar
Hsieh, H. H. & Jewitt, D. 2008, Science, 312, 561Google Scholar
Jang-Condell, H. 2008, ApJ, 679, 797CrossRefGoogle Scholar
Jewitt, D., Yang, B., & Haghighipour, N. 2009, AJ, 137, 4313Google Scholar
Lecar, M., Podolak, M., Sasselov, D., & Chiang, E. 2006, ApJ, 640, 1115Google Scholar
Lodders, K. 2004, ApJ, 611, 587CrossRefGoogle Scholar
Mekler, Y. & Podolak, M. 1994, Plan. & Space Sci., 42, 865Google Scholar
Podolak, M. & Mekler, Y. 1997, Plan. & Space Sci., 45, 1401Google Scholar
Pollack, J. B., McKay, C. P., & Christofferson, B. M. 1985, Icarus, 64, 471Google Scholar
Sasselov, D. & Lecar, M. 2000, ApJ, 528, 995CrossRefGoogle Scholar
Stevenson, D. J. & Lunine, J. I. 1988, Icarus, 75, 146Google Scholar
van de Hulst, H. C. 1957, Light Scattering by Small Particles, (New York: John Wiley & Sons)Google Scholar