Hostname: page-component-586b7cd67f-2brh9 Total loading time: 0 Render date: 2024-11-24T13:06:16.214Z Has data issue: false hasContentIssue false
  • English
  • Français

The Use of Geocentric Variables to Search for Meteoroid Streams and Their Parents

Published online by Cambridge University Press:  12 April 2016

CL. Froeschlé ,
T.J. Jopek  and
G.B. Valsecchi
CL. Froeschlé
Affiliation:
Observatoire de la Côte d’Azur, B.P. 4229, F-06304 Nice, France
T.J. Jopek
Affiliation:
Obserwatorium Astronomiczne Uniwersytetu A. Mickiewicza, Sloneczna 36, PL-60286 Poznań, Poland
G.B. Valsecchi
Affiliation:
I.A.S. - Planetologia, via Fosso del Cavaliere, I-00133 Roma, Italy

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.

A set of geocentric variables suitable for the identification of meteoroid streams has been recently proposed and successfully applied to photographic meteor orbits. We describe these variables and the secular invariance of some of them, and discuss their use to improve the search for meteoroid stream parents.

Keywords

: MeteorsMeteoroid streams
Type
Extended Abstracts
Information
International Astronomical Union Colloquium , Volume 172: Impact of Modern Dynamics in Astronomy , 1999 , pp. 55 - 64
Copyright
Copyright © Kluwer 1999

References

Babadzhanov, P.B., Obrubov, Yu.V.: 1993, Dynamics and relationships between interplanetary bodies I. Machholz and its meteor showers, in Meteoroids and their parent bodies, Štohl, J. and Williams, I.P., eds., Astronomical Institute of the Slov. Acad. Sci., Bratislava, Slovakia, 49–52 Google Scholar
Carusi, A., Valsecchi, G.B., Greenberg, R.: 1990, Planetary close encounters: geometry of approach and post-encounter orbital parameters, Cel. Mech. & Dyn. Astro., 49, 111 Google Scholar
Drummond, J.: 1981, A test of comet and meteor shower associations, Icarus, 45, 545–553 Google Scholar
Jenniskens, P., Betlem, H., de Lignie, M., Langbroek, M. and van Vliet, M.: 1997, Meteor stream activity V. The Quadrantids, a very young stream, A&A, 327, 1242–1252 Google Scholar
Jopek, T.: 1993, Remarks on the meteor orbital similarity D-criterion, Icarus, 106, 603–607 Google Scholar
Jopek, T.J., Froeschlé, Cl.: 1997, A&A, 320, 631–641 Google Scholar
Jopek, T.J., Valsecchi, G.B., Froeschlé, Cl.: 1999, Meteor streams identification: a new approach.II. Application to 865 photographic meteor orbits, MNRAS, in pressCrossRefGoogle Scholar
Kozai, Y., 1962, Secular perturbations of asteroids with high inclination and eccentricity, AJ, 67, 591–598 Google Scholar
Lindblad, B.A.: 1971, Smithson. Contr. Astrophys., 12, 1–13 Google Scholar
Öpik, E.J.: 1976, Interplanetary Encounters, Elsevier, New York Google Scholar
Southworth, R.B., Hawkins, G.S.: 1963, Statistics of meteor streams, Smithson. Contr. Astrophys., 7, 261–285 Google Scholar
Thomas, F., Morbidelli, A., 1996, The Kozai resonance in the outer solar system and the dynamics of long-period comets, Cel. Mech. & Dyn. Astro., 64, 209–229 Google Scholar
Valsecchi, G.B., Jopek, T.J., Froeschlé, Cl.: 1999, Meteoroid streams identification: a new approach. I. Theory, MNRAS, in pressGoogle Scholar
Williams, I.P., Collander-Brown, S.J., 1998 The parent of the Quadrantid meteoroid stream, MNRAS, 294, 127-138Google Scholar