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Stream and sporadic meteoroids associated with Near Earth Objects

Published online by Cambridge University Press:  05 March 2015

Tadeusz J. Jopek
Affiliation:
Astronomical Observatory Institute, Faculty of Physics, A.M. University, Poznan, Poland
Iwan P. Williams
Affiliation:
School of Physics and Astronomy, Queen Mary University of London, E1 4NS, UK
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Abstract

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NEOs come close to the Earth's orbit so that any dust ejected from them, might be seen as a meteor shower. Orbits evolve rapidly, so that a similarity of orbits at one given time is not sufficient to prove a relationship, orbital evolution over a long time interval also has to be similar. Sporadic meteoroids can not be associated with a single parent body, they can only be classified as cometary or asteroidal. However, by considering one parameter criteria, many sporadics are not classified properly therefore two parameter approach was proposed.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2015 

References

Asher, D. J., Clube, S. V. M., & Steel, D. I., 1993, MNRAS, 264, 93CrossRefGoogle Scholar
Battams, K. W. & atson, A., 2009, IAU Circ., 9054Google Scholar
Drummond, J. D. 1981, Icarus, 45, 453CrossRefGoogle Scholar
Fox, K., Williams, I. P., & Hughes, D. W., 1983, MNRAS, 205, 1155CrossRefGoogle Scholar
Hughes, D. W., Williams, I. P., & Fox, K., 1981, MNRAS, 195, 625CrossRefGoogle Scholar
Jenniskens, P., 2004, AJ, 127, 3018CrossRefGoogle Scholar
Jewitt, D., Weaver, H., Agarwal, J., Mutchler, M., & Drahus, M., 2010, Nature, 467, 817Google Scholar
Jones, J. & Sarma, T., 1985, Bull. Astron. Inst. Czechosl., 36, 103Google Scholar
Jones, J., Campbell-Brown, M. & Nikolova, S., 2001, in Meteors 2001, Ed Warmbeim B., ESA-SP495 575Google Scholar
Jopek, T. J. & Williams, I. P., 2013, MNRAS, 430, 2377CrossRefGoogle Scholar
Nesvorny, D., Vokrouhlicky, D., Pokorny, P., & Janches, D., 2011, ApJ, 747, 1Google Scholar
Porubčan, V., Kornoš, L., & Williams, I. P., 2004, EM&P. 95, 697Google Scholar
Porubčan, V., Kornoš, L., & Williams, I. P., 2006, Contr. Astron. Obs. Skalnate Pleso, 36, 103Google Scholar
Southworth, R. B. & Hawkins, G. S., 1963, Smiths. Contr. Astroph., 7, 261Google Scholar
Steel, D. I., 1996, Space Sci. Rev., 78, 507Google Scholar
Voloshchuk, Yu. I., Vorgul', A. V., & Kashcheev, B. L., 1997. Astronomicheskii Vestnik, 31, 345Google Scholar
Whipple, F. L., 1954, AJ, 59, 201Google Scholar
Whipple, F. L. 1983, IAU Circ 3881.Google Scholar
Williams, I. P. 2004, WGN J. IMO, 32, 11Google Scholar
Williams, I. P. 2011, A & G 52 2.20Google Scholar
Williams, I. P., Hughes, D. W., McBride, N., & Wu, Z., 1993, MNRAS, 260, 43Google Scholar
Williams, I. P., Ryabova, G. O., Baturin, A. P., & Chernitsov, A. M., 2004, MNRAS, 355, 1171Google Scholar