Hostname: page-component-586b7cd67f-rdxmf Total loading time: 0 Render date: 2024-11-26T07:32:01.188Z Has data issue: false hasContentIssue false
  • English
  • Français

Interrelations Among Asteroids, Comets and Meteoroids

Published online by Cambridge University Press:  30 March 2016

A.N. Simonenko  and
B.J. Levin
A.N. Simonenko
Affiliation:
The Astronomical Council of the USSR Academy of Sciences, 48 Pyatnitskaya St., 109017 Moscow, USSR
B.J. Levin
Affiliation:
The Astronomical Council of the USSR Academy of Sciences, 48 Pyatnitskaya St., 109017 Moscow, USSR

Extract

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.

If we investigate the interrelations among different classes of small solar system bodies, we must be aware that we deal with nonrepresentative and practically noncomparable data samples consisting of bodies differing either in size, or in orbits, or in their nature. So, practically, all our knowledge about small bodies - from kilometer-sized Apollo asteroids (including Atens) and Amor asteroids (designated below as AA bodies) to fine dust particles - refer to bodies on orbits intersecting the ecliptic plane at a heliocentric distance ≃ 1 A.U. To solve the problem of origin of this ensemble it would be advantageous if analogous data could be obtained at least for one more heliocentric distance. Since planetary atmospheres are excellent detectors for small cosmic objects, the necessary data could be obtained with the aid of artificial satellites orbiting a planet, e.g. Mars or Venus. Thus the source for the ensemble of Earth-crossing objects may not be correctly pictured. Are comets or asteroids the general supplier? We know the answer to this question only in two cases: (1) meteor streams such as the Leonids originate from comets, (2) meteorites originate from asteroids. But these two categories represent a minute part of the considered ensemble by mass. As to its other members- the selection of the source is a matter of tradition rather than a logic conclusion.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 6 , 1983 , pp. 391 - 398
Copyright
Copyright © Reidel 1983

References

Babadzhanov, P.B. and Getman, T.I.: 1980, Meteoritika 39, pp. 15–18.Google Scholar
Ceplecha, Z.: 1977, Comets, Asteroids, Meteorites, (ed.) Delsemme, A.H., Univ. Toledo Press, Toledo, USA, pp. 143–150.Google Scholar
Ceplecha, Z.: 1978, Meteoritika 37, pp. 60–68.Google Scholar
Ceplecha, Z. and McCrosky, R.E.: 1976, J. Geophys. Res. 81, pp. 6257–6275.CrossRefGoogle Scholar
Dermott, S.F. and Murray, C.D.: 1981, Nature 240, pp. 664–668.Google Scholar
Ephemerides of Minor Planets for 1982: 1981, (ed.) Batrakov, J.V., Nauka, Leningrad, USSR, pp. 14–55.Google Scholar
Franklin, F.A., Marsden, B.G., Williams, J.G. and C.M., Bardwell: 1975, Astron. J. 80, pp. 729–746.Google Scholar
Froeschlé, C. and Scholl, H.: 1977, Astron. Astrophys. 57, pp. 33–39.Google Scholar
Gehrels, T.: 1981, Icarus 47, pp. 518–522.CrossRefGoogle Scholar
Gradie, J.C., Chapman, C.R. and Williams, J.G.: 1979, Asteroids, (ed.) Gehrels, T., Univ. Arizona Press, Tucson, USA, pp. 359–390.Google Scholar
Janiczek, P.M., Seidelmann, P.K. and Duneombe, R.L.: 1972, Astron. J. 77, pp. 764–773.Google Scholar
Kresák, L.: 1974, Asteroids, Comets, Meteorio Matter, (eds) Cristescu, C., Klepczynski, W.J. and Milet, B., Ed. Acad. Rep. Social. Romania, Bucarest, Romania, pp. 193–202.Google Scholar
Kresáková, M.: 1980, Bull. Astron. Inst. Czech. 31, pp. 193–206.Google Scholar
Levin, B.J. and Simonenko, A.N.: 1981, Icarus 47, pp. 487–491.Google Scholar
Marsden, B.G.: 1975, Catalogue of Cometary Orbits (2nd ed.), Central Bureau for Astronomical Telegrams IAU, Cambridge, USA, 83 pages.Google Scholar
McCrosky, R.E., Shao, C.-Y. and Posen, A.: 1978, Meteoritika 37, pp. 44–59.Google Scholar
McCrosky, R.E., Shao, C.-Y. and Posen, A.: 1979, Meteoritika 38, pp. 106–156.Google Scholar
Öpik, E.J.: 1963, Adv. Astron. Astrophys. 2, pp. 219–262.Google Scholar
Petrov, G.I. and Stulov, V.P.: 1975, Cosm. Issled. 13, pp. 587–594.Google Scholar
Shoemaker, E.M., Williams, J.G., Helin, E.F. and Wolfe, R.F.: 1979, Asteroids, (ed.) T. Gehrels, Univ. Arizona Press, Tucson, USA, pp. 253–282.Google Scholar
Simonenko, A.N.: 1975, Orbital Elements for 45 Meteorites, Nauka, Moscow, USSR, 68 pages.Google Scholar
Simonenko, A.N.: 1977, Soviet Astron. Letters 3, pp. 16–18.Google Scholar
Simonenko, A.N.: 1979a, Soviet Astron. Letters 5, pp. 360–361.Google Scholar
Simonenko, A.N.: 1979b, Meteorites are Fragments of Asteroids, Nauka, Moscow, USSR, 224 pages.Google Scholar
Simonenko, A.N., Kruchinenko, V.G. and Sherbaum, L.M.: 1980, Meteoritika 39, pp. 121–133.Google Scholar
Wasson, J.T. and Wetherill, G.W.: 1979, Asteroids, (ed.) Gehrels, T., Univ. Arizona Press, Tucson, USA, pp. 926–974.Google Scholar
Weidenschilling, S.J.: 1981, Icarus 46, pp. 124–126.CrossRefGoogle Scholar
Wetherill, G.W.: 1975, Proa. Soviet-American Conf. on Cosmochem. of the Moon and Planets, Nauka, Moscow, USSR, pp. 411–424; NASA SP-370 (1977), pp. 553-567.Google Scholar
Wood, J.A.: 1979, Asteroids, (ed.) Gehrels, T., Univ. Arizona Press, Tucson, USA, pp. 849–891.Google Scholar