Advertisement

Earth, Moon, and Planets

, Volume 46, Issue 3, pp 285–295 | Cite as

Notes on an initial satellite system of Neptune

  • Pletser Vladimir 
Letter to the Editor

Abstract

The comparison of masses and sizes of the Neptunian satellites and of Pluto and Charon to the secondaries of the planetary, Jovian, Saturnian and Uranian systems support the hypotheses, first, that an initial Neptune's satellite system may have been disrupted, second, that Triton may have been the system perturber and, third, that Pluto (or a parent body of Pluto and Charon) was initially a giant satellite of Neptune. Based on recent theoretical works on perturbed proto-planetary nebula and noting the similarity of some characteristics of Neptune and Uranus, a theoretical mean distance ratio of primeval gaseous rings around Neptune is tentatively deduced to be about 1.475, close to the value of the Uranian system. An exponential distance relation gives possible ranges of distances at which small satellites and/or ring structures could be found by Voyager 2, close to Neptune.

Keywords

Ring Structure Theoretical Work Distance Relation Satellite System Parent Body 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Preview

Unable to display preview. Download preview PDF.

Unable to display preview. Download preview PDF.

References

  1. Bec-Borsenberger, and Chollet, F.: 1986, in Les étoiles, le Système Solaire, Bordas, Gauthier-Villars, 23.Google Scholar
  2. Berlage, Jr, H. P.: 1932, Proc. Koninkl. Ned. Akad. Wetenschap. (Amsterdam) 35, 553.Google Scholar
  3. Buie, M. W., Cruikshank, D. P., Lebofsky, L. A., and Tedesco, E. F.: 1988, Nature 329, 522.Google Scholar
  4. Covault, C. E., Glass, I. S., French, R. G., and Elliot, J. L.: 1986, Icarus 67, 126.Google Scholar
  5. Farinella, P., Milani, A., Nobili, A. M., and Valsecchi, G. B.: 1979, The Moon and the Planets 20, 415.Google Scholar
  6. Farinella, P., Milani, A., Nobili, A. M., and Valsecchi, G. B.: 1980, Icarus 44, 810.Google Scholar
  7. Goldreich, P., Tremaine, S., and Borderies, N.: 1986, Astr. J. 92, 490.Google Scholar
  8. Guinan, E. F., Harris, C. C., and Maloney, F. P.: 1982, Bull. American Astron. Soc. 14, 658.Google Scholar
  9. Harrington, R. S. and Van Flandern, T. C.: 1979, Icarus 39, 131.Google Scholar
  10. Hubbard, W. B., Brahic, A., Sicardy, B., Elicer, L. R., Roques, F., and Vilas, F.: 1986, Nature 319, 636.Google Scholar
  11. Hubbard, W. B., Nicholson, P. D., Lellouch, E., Sicardy, B., Brahic, A., Vilas, F., Bouchet, P., McLaren, R. A., Millis, R. L., Wasserman, L. H., Elias, J. H., Matthews, K., McGill, J. D., and Perrier, C.:1987, Icarus 72, 635.Google Scholar
  12. Kerr, R. A.: 1983, Science 222, 311.Google Scholar
  13. Landgraf, W.: 1988, IAU Circ. 4542, 3 Febr. 1988.Google Scholar
  14. Lyttleton, R. A.: 1936, Mon. Not. Roy. Astron. Soc. 162, 261.Google Scholar
  15. McKinnon, W. B. and Mueller, S.: 1988, Nature 335, 240.Google Scholar
  16. Murray, C. D.: 1986, Nature 324, 209.Google Scholar
  17. Nieto, M. M.: 1972, The Titius-Bode Law of Planetary Distances: Its History and Theory, Pergamon Press, Oxford.Google Scholar
  18. Nowotny, E.: 1979, The Moon and the Planets 21, 257.Google Scholar
  19. Pandey, A. K., Mahra, H. S. and Mohan, V.: 1984, Earth, Moon, and Planets 31, 217.Google Scholar
  20. Pletser, V.: 1986, Earth, Moon, and Planets 36, 193.Google Scholar
  21. Pletser, V.: 1988, Earth, Moon, and Planets 41, 295.Google Scholar
  22. Pletser, V.: 1989, ‘Annular Structures in Perturbed Low Mass Disc-shaped Gaseous Nebulas’, (in prep.).Google Scholar
  23. Pollack, J. B.: 1985, Protostars and Planets II, in D. C. Black and M. S. Matthews (eds.), Univ. of Arizona Press, Tucson, 791.Google Scholar
  24. Prentice, A. J. R.: 1980, JPL Publication 80–80, Jet Propulsion Laboratory, Pasadena.Google Scholar
  25. Prentice, A. J. R.: 1984, Earth, Moon, and Planets 30, 209.Google Scholar
  26. Reitsema, H. J., Hubbard, W. B., Lebofsky, L. A., and Tholen, D. J.: 1982, Science 215, 289.Google Scholar
  27. Schaefer, M. W. and Schaefer, B. E.: 1988, Nature 333, 436.Google Scholar
  28. Sicardy, B.: 1987, IAU Circ. 4418, 10 July 1987.Google Scholar
  29. Stern, S. A.: 1988, Icarus 73, 269.Google Scholar
  30. Veverka, J.: 1988, Nature 333, 394.Google Scholar

Copyright information

© Kluwer Academic Publishers 1989

Authors and Affiliations

  • Pletser Vladimir 
    • 1
  1. 1.Institut d'Astronomie et de Géophysique G. Lemaître, University of Louvain-la-NeuveBelgium

Personalised recommendations