Hostname: page-component-cd9895bd7-gvvz8 Total loading time: 0 Render date: 2024-12-23T13:51:41.860Z Has data issue: false hasContentIssue false
  • English
  • Français

Migration of Trans-Neptunian Objects to The Earth

Published online by Cambridge University Press:  12 April 2016

Sergei I. Ipatov
Sergei I. Ipatov*
Affiliation:
Institute of Applied Mathematics, Miusskaya sq. 4, Moscow 125047, Russia; E-mail:[email protected]

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.

Migration of trans–Neptunian objects under their mutual gravitation influence and the influence of the giant planets is investigated. These investigations are based on computer simulation results and on some formulas. We estimated that about 20 % of near–Earth objects with diameter d ≥ 1 km may have come from the Edgeworth–Kuiper belt.

Type
Extended Abstracts
Information
International Astronomical Union Colloquium , Volume 172: Impact of Modern Dynamics in Astronomy , 1999 , pp. 107 - 116
Copyright
Copyright © Kluwer 1999

References

Bulirsh, R. and Stoer, J.: 1966, Numer. Math., 8, 1–13.CrossRefGoogle Scholar
Davis, D.R. and Farinella, P.: 1997, Icarus, 125, 50–60.Google Scholar
Duncan, M., Quinn, T., and Tremaine, S.: 1988, 328, L69–L73.Google Scholar
Duncan, M.J., Levison, H.F., and Budd, S.M.: 1995, Astron. J., 110, 3073–3081.Google Scholar
Eneev, T.M.: 1980, Sov. Astron. Letters, 6, No 5, p. 295–300 in Russian edition.Google Scholar
Fernandez, J.A.: 1980, Monthly Notices Roy. Astron. Soc, 192, 481–191.Google Scholar
Gladman, B. and Duncan, M.: 1990, Astron. J., 100, 1680–1696.Google Scholar
Hahn, G. and Bailey, M.E.: 1990, Nature, 348, 132–136.Google Scholar
Holman, M.J. and Wisdom, J.: 1993, Astron. J., 105, 1987–1999.Google Scholar
Ip, W.-H. and Fernandez, J.A.: 1997,Astron. Astrophys., 324, 778–784.Google Scholar
Ipatov, S.I.: 1980, Preprint of Inst. of Applied Mathematics, N43, Moscow, 33 P. (in Russian).Google Scholar
Ipatov, S.I.: 1987, Earth, Moon, and Planets, 39, 101–128.Google Scholar
Ipatov, S.I.: 1988, Kinematics Phys. Celest. Bodies, 4, N 6, 76–82.Google Scholar
Ipatov, S.I.: 1993, Solar System Research,27 65–79.Google Scholar
Ipatov, S.I.: 1995a, Solar System Research, 29, 9–20.Google Scholar
Ipatov, S.I.: 1995b, Solar System Research, 29, 261–286.Google Scholar
Ipatov, S.I.: 1996, Earth, Moon, and Planets, 72, 211–214.Google Scholar
Ipatov, S.I.: 1997a, LPSC XXVIII, 615–616.Google Scholar
Ipatov, S.I.: 1997b, LPSC XXVIII, 617–618.Google Scholar
Ipatov, S.I.: 1999a, ’Migration of Kuiper-belt objects inside the Solar System’, ″Planetary systems— the long view″, Proc. 9th Rencontres de Blois (June 22-28, 1997), Editions Frontieres, Gif. sur Yvette Cedex, Celnikier, L.M. and Tran Thanh Van, J., (eds.), 157–160 Google Scholar
Ipatov, S.I.: 1999b, Migration of celestial bodies in the solar system, URSS Publishing Company, Moscow, in press.Google Scholar
Ipatov, S.I. and Hahn, G.J.: 1997, LPSC XXVIII, 619–620.Google Scholar
Ipatov, S.I. and Hahn, G.J.: 1999a, ″Planetary systems — the long view″, Proc. 9th Rencontres de Blois (June 22-28, 1997), Editions Frontieres, Gif. sur Yvette Cedex, Celnikier, L.M. and Tran Thanh Van, J., (eds.), 179–180 Google Scholar
Ipatov, S.I. and Hahn, G.J.: 1999b, Solar System Research, 33, in press.Google Scholar
Ipatov, S.I. and Henrard, J.: 1999, Solar System Research, 33, in press.Google Scholar
Jewitt, D., Luu., J., and Chen, J.: 1996, Astron. J., 112, 1225–1238.Google Scholar
Jewitt, D., Luu., J., and Trujillo, C.: 1998, Astron. J., 115, 2125–2135.CrossRefGoogle Scholar
Kenyon, S.J. and Luu, J.X.: 1998, Astron. J., 115, 2136–2160.CrossRefGoogle Scholar
Levison, H.F. and Duncan, M.J.: 1993, Astrophys. J., 406, L35–L38.Google Scholar
Levison, H.F. and Duncan, M.J.: 1994, Icarus, 108, 18–36.Google Scholar
Levison, H.F. and Duncan, M.J.: 1997, Icarus, 127, 13–23.Google Scholar
Luu, J., Marsden, B.G., Jewitt, D., Trujillo, C.A., Hergenrother, C.W., Chen, J., and Offutt, W.B.: 1997, Nature, 387, 573–575.CrossRefGoogle Scholar
Morbidelli, A., Thomas, F., and Moons, M.: 1995, Icarus, 118, 322–340.CrossRefGoogle Scholar
Öpik, E.J.: 1963, Adv. Astron. Astrophys., 2, 219–262.Google Scholar
Stern, S.A.: 1995, Astron. J., 110, 856–868.CrossRefGoogle Scholar
Stern, S.A.: 1996a, Astron. J., 112, 1203–1211.Google Scholar
Stern, S.A.: 1996b, Astron. Astrophys., 310, 999–1010.Google Scholar
Stern, S.A. and Colwell, J.E.: 1997, Astron. J., 114, 841–849.Google Scholar
Torbett, M. and Smoluchowski, R.: 1990, Nature, 44, 722–729.Google Scholar
Weissman, P.R.: 1995, Annu. Rev. Astron. Astrophys., 33, 327–357.CrossRefGoogle Scholar
Weissman, P.R., A’Hearn, M.F., McFadden, L.A. and Rickman, H.: 1989, Asteroids II, Tucson: Univ. Arizona Press, Binzel, R.P., Gehreis, T. and Matthews, M.S. (eds.), 880–919.Google Scholar
Wetherill, G.W.: 1988, Icarus, 76, 1–18.Google Scholar
Wetherill, G.W.: 1989, Meteoritics, 24, 15–22.Google Scholar
Wetherill, G.W: 1991, Proc. of the IAU Colloquium 121 ″Comets in the post-Halley era″, Amsterdam: Kluwer Acad. Publ., Newburn, R.L., Rahe, J. and Neugebauer, M. (eds.), 537–556.Google Scholar