Hostname: page-component-84b7d79bbc-lrf7s Total loading time: 0 Render date: 2024-07-27T23:27:13.111Z Has data issue: false hasContentIssue false
  • English
  • Français

Can D-D fusion contribute to Jupiter's excess heat?

Published online by Cambridge University Press:  26 May 2016

Rachid Ouyed
Rachid Ouyed*
Affiliation:
NORDITA, Blegdamsvej 17, DK-2100 Copenhagen, Denmark

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.

We explore the highly speculative idea of Deuterium - Deuterium (D-D) fusion inside Jupiter as an internal heating source. We suggest that D could have been brought deep inside the planet by planetesimals (during the process of planet formation) and deposited through planetesimal/ices vaporization. Here, the general aspects of the model are presented.

Type
Part III: Structure and atmospheres of planets
Information
Symposium - International Astronomical Union , Volume 202: Planetary Systems in the Universe – Observation, Formation and Evolution , 2004 , pp. 280 - 282
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Bosch, H. S., & Hale, G. M. 1992, Nuclear Fusion, 32, 611.CrossRefGoogle Scholar
Chabrier, G., Saumon, D., Hubbard, W. B. & Lunine, J. I. 1992, ApJ, 391, 817.CrossRefGoogle Scholar
Duffy, T. S., Vos, W. L., Zha, C.-S., Hemley, R. J. & Mao, H.-K. 1994, Science, 263, 1590.CrossRefGoogle Scholar
Gudkova, T. V., Mosser, B., Provost, J., Chabrier, G., Gautier, D. & Guillot, T. 1995, A&A, 303, 594.Google Scholar
Hubbard, W. B., 1984, Planetary Interiors. New York: Van Nostrand Reinhold.Google Scholar
Lutz, B. L., Owen, T. & de Bergh, C. 1990, Icarus, 86, 329.CrossRefGoogle Scholar
Mosser, B., Mekarnia, D., Maillard, J. P., Gay, J., Gauthier, D. & Delache, Ph., 1993, A&A, 267, 604.Google Scholar
Mosser, B., Maillard, J. P. & Mekarnia, D. 2000, Icarus, 144, 104.CrossRefGoogle Scholar
Nellis, W. J., Ross, M. & Holmes, N. C. 1995, Science, 269, 1249.CrossRefGoogle Scholar
Ouyed, R., Fundamenski, W., Cripps, G. & Sutherland, P G. 1998, ApJ, 501, 367.CrossRefGoogle Scholar
Owen, T., Lutz, B. L. & de Bergh, C. 1986, Nature, 320, 244.CrossRefGoogle Scholar
Podolak, M., Hubbard, W. B. & Pollack, J. B. 1993, in Protostars and planets III, Levy, E. H. and Lunine, J. I., eds., University of Arizona Press, Tucson, 1109.Google Scholar