Hostname: page-component-78c5997874-4rdpn Total loading time: 0 Render date: 2024-11-14T06:43:46.079Z Has data issue: false hasContentIssue false
  • English
  • Français

Chemistry of the Solar System Revealed in the Interiors of the Giant Planets

Published online by Cambridge University Press:  21 December 2011

Jonathan I. Lunine
Jonathan I. Lunine*
Affiliation:
Department of Astronomy, Cornell University, 402 Space Sciences Building, Ithaca, NY 14853USA email: jlunine@astro.cornell.edu
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 giant planets of our solar system contain a record of elemental and isotopic ratios of keen interest for what they tell us about the origin of the planets and in particular the volatile compositions of the solid phases. In situ measurements of the Jovian atmosphere performed by the Galileo Probe during its descent in 1995 demonstrate the unique value of such a record, but limited currently by the unknown abundance of oxygen in the interior of Jupiter–a gap planned to be filled by the Juno mission set to arrive at Jupiter in July of 2016. Our lack of knowledge of the oxygen abundance allows for a number of models for the Jovian interior with a range of C/O ratios. The implications for the origin of terrestrial water are briefly discussed. The complementary data sets for Saturn may be obtained by a series of very close, nearly polar orbits, at the end of the Cassini-Huygens mission in 2016-2017, and the proposed Saturn Probe. This set can only obtain what we have for Jupiter if the Saturn Probe mission carries a microwave radiometer.

Keywords

giant planetsnoble gaseswateroxygen
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S280: The Molecular Universe , June 2011 , pp. 249 - 260
Copyright
Copyright © International Astronomical Union 2011

References

Adriani, A., Coradini, A., Filacchione, G., Lunine, J. I., Bini, A., Pasqui, C., Colamai, L., Colosimo, F., Dinelli, B. M., Grassi, D., Magni, G., Moriconi, M. L., & Orosei, R. 2008 Astrobiology, 8, 613CrossRefGoogle Scholar
Asplund, M., Grevesse, N., Jacques Sauval, A., & Scott, P. 2009 ARAA, 47, 481.CrossRefGoogle Scholar
Brown, R. H. B., Lauretta, D. S., Schmidt, B., & Moores, J. 2011, PSS, in press.Google Scholar
Ciesla, F. J. & Carnley, S. B. 2006, in: Lauretta, D. S. and McSween, H.Y. (eds.), Meteorites and the Early Solar System II (Tucson: University of Arizona Press), p. 209.CrossRefGoogle Scholar
Cowen, R. 2011 Science News January 15, 2011, 26CrossRefGoogle Scholar
Cyr, K. E., Sears, W. D., & Lunine, J. I. 1998 Icarus, 135, 537CrossRefGoogle Scholar
de Leeuw, N. H., Catlow, R. A., King, H. E., Putnis, A., Muralidharan, K., Deymier, P., Stimpfl, M., & Drake, M. J. 2010 Chem. Comm., 46, 8923.CrossRefGoogle Scholar
dePater, I., Dunn, D., Romani, P., & Zahnle, K. 2001, Icarus, 149, 66CrossRefGoogle Scholar
Fouchet, T., Moses, J. I., & Conrath, B. J. 2009, in: Dougherty, M. K., Esposito, L. W. & Krimigis, S. M. (eds.), Saturn from Cassini-Huygens (Dordrecht: Springer), p. 83CrossRefGoogle Scholar
Grevesse, N., Asplund, M., & Sauval, A. J. 2005, in Alecian, G., Richard, O., Vauclair, S. (eds.), Element stratification of stars, 40 years of atomic diffusion (Les Ulis: EDP Sciences), p. 21Google Scholar
Hanel, R. A., Conrath, B. J., Kunde, V. G., Pearl, J. C., & Pirraglia, J. A. 1983 Icarus, 53, 262CrossRefGoogle Scholar
Hersant, F., Gautier, D., & Lunine, J. I. 2004, Planetary and Space Science, 52, 623CrossRefGoogle Scholar
Hsieh, H. & Jewitt, D. C. 2006, Science, 312, 561CrossRefGoogle Scholar
Hubbard, W. B., Dougherty, M. K., Gautier, D., & Jacobson, R. 2009, in: Dougherty, M. K., Esposito, L. W. & Krimigis, S. M. (eds.), Saturn from Cassini-Huygens (Dordrecht: Springer), p. 75CrossRefGoogle Scholar
Janssen, M. A., Hofstader, M. D., Gulkis, S., Ingersoll, A. P., Allison, M. A., Bolton, S. J., Levin, S. M., & Kamp, L. W. 2005, Icarus, 173, 447CrossRefGoogle Scholar
Krot, A. N., Fegley, B. Jr., Lodders, K., & Palme, H. 2000, in: Mannings, V., Boss, A. P. & Ressell, S. S. (eds.), Protostars and Planets IV (Tucson: University of Arizona Press), p. 1019.Google Scholar
Lodders, K. 2004, ApJ, 611, 587CrossRefGoogle Scholar
Lodders, K. & Fegley, B. 1998, Meteorit. Planet. Sci., 33, 871CrossRefGoogle Scholar
Lunine, J. I., O'Brien, D. P., Raymond, S. N., Morbidelli, A., Quinn, T. & Graps, A. L. 2011 Advanced Science Letters 4, 325.CrossRefGoogle Scholar
Lunine, J. & Hunten, D. M. 1987, Icarus, 69, 566CrossRefGoogle Scholar
Madhusudhan, N., Harrington, J., Stevenson, K., Nymeyer, S., Campo, C., Wheatley, P., Deming, D., Blecic, J., Hardy, R., Lust, N., Anderson, D., Collier-Cameron, A., Britt, C., Bowman, W., Hebb, L., Hellier, C., Maxted, P., Pollacco, D., & West, R. 2011, Nature, 64, 469Google Scholar
Madhusudhan, N., Mousis, O., Johnson, T. V., & Lunine, J. I. 2011, ApJ in pressGoogle Scholar
Mahaffy, P. R., Niemann, H. B., Alpert, A., Atreya, S. K., Demick, J., Donahue, T. M., Harpold, D. N., & Owen, T. C. 2000, J. Geophys. Res., 105, 15061.CrossRefGoogle Scholar
Marty, B., Guillot, T., Coustenis, A., & 55 others 2008 Experimental Astronomy DOI 10.1007/s10686-008-9094-9Google Scholar
Mousis, O., Madhusudhan, N., Lunine, J. I., & Johnson, T. V. 2011, ApJ, submitted.Google Scholar
Mousis, O., Marboeuf, U., Lunine, J. I., Alibert, Y., Fletcher, L. N., Orton, G. S., Pauzat, F. and Ellinger, Y. 2009, ApJ, 696, 1348.CrossRefGoogle Scholar
Niemann, H. B., Atreya, S. K., Carignan, G. R., Donahue, T. M., Haberman, J. A., Harpold, D. N., Hartle, R. E., Hunten, D. M., Kasprzak, W. T., Mahaffy, P. R., Owen, T. C., & Way, S. H. 1998, J. Geophys. Res., 103, 22831CrossRefGoogle Scholar
Owen, T., Mahaffy, P. R., Niemann, H. B., Atreya, S., Donahue, T., Bar-Nun, A., & de Pater, I. 1999, Nature, 402, 269CrossRefGoogle Scholar
Owen, T. & Encrenaz, T. 2003, Space Science Rev., 106, 121CrossRefGoogle Scholar
Proffitt, C. R. 1994, ApJ, 425, 849CrossRefGoogle Scholar
Showman, A. P. & Dowling, T. E. 2000, Science, 289, 1737CrossRefGoogle Scholar
Space Studies Board 2011 Vision and Voyages for Planetary Science in the Decade 2013-2022 (Washington: National Academies Press)Google Scholar
Stevenson, D. J. & Salpeter, E. E. 1977 ApJ Suppl, 35, 221CrossRefGoogle Scholar
Wong, , von Zahn, U., Hunten, D. M., & Lehmacher, G. 1998 JGR 103, 22815Google Scholar
Walsh, K. J., Morbidelli, A., Raymond, S. N., O'Brien, D. P., & Mandell, A. M. 2011, Nature, 475, 206CrossRefGoogle Scholar
Wilson, H. F. & Militzer, B. 2010, Physical Review Letters, 104, 147Google Scholar
Wong, M. H., Lunine, J. I., Atreya, S. K., Johnson, T., Mahaffy, P. R., Owen, T. C., & Encrenaz, T. 2008 Reviews in Mineralogy & Geochemistry 68, 219.CrossRefGoogle Scholar