Meteor Showers Originated from 73P/Schwassmann–Wachmann
Article
First Online:
Received:
Accepted:
- 63 Downloads
Abstract
The nucleus of the Comet 73P/Schwassmann–Wachmann had been split into many fragments at least past two returns. Since the related dense dust trail has been detected in the space infrared observation, the strong activity of the meteor shower is highly expected in the future. We applied the so-called dust-trail theory to this interesting object, and obtained several results on the future encounter with the dust trail. In this paper we introduce our results on the forecasts.
Keywords
Comets: individual(73P/Schwassmann–Wachmann) Meteoroids Meteors Solar systemReferences
- D.J. Asher, in Proc. Int. Meteor Conf., Frasso Sabino, Italy, 23–26 Sept, 1999, ed. by R. Arlt (IMO, Belgium, 2000), p. 5Google Scholar
- T. Fuse, N. Yamamoto, D. Kinoshita, H. Furusawa, J. Watanabe, PASJ (Publ. Astron. Soc. Japan) 59, 381–386 (2007)ADSGoogle Scholar
- P. Jenniskens, J. Vaubaillon, Astron. J. 134, 1037–1045 (2007)CrossRefADSGoogle Scholar
- K. Kinoshita (Comet Orbit Home Page, 2007), http://www9.ocn.ne.jp/∼comet/. Accessed 1 Feb 2007
- H. Lüthen, R. Arlt, M. Jäger, WGN J. Int. Meteor Organ. (JIMO) 29(1), 15–28 (2001)ADSGoogle Scholar
- R.H. McNaught, D.J. Asher, WGN J. Int. Meteor Organ. (JIMO) 27, 85 (1999)ADSGoogle Scholar
- M. Sato, WGN J. Int. Meteor Organ. (JIMO) 31, 59 (2003)ADSGoogle Scholar
- Z. Sekanina, H. Boehnhardt, H.U. Käufl, K. Birkle, JPL Cometary Sciences Group Preprint Series. 183 (1996)Google Scholar
- P.A. Wiegert, P.G. Brown, J. Vaubaiillon, H. Schijns, MNRAS 361, 638–644 (2005)CrossRefADSGoogle Scholar
Copyright information
© Springer Science+Business Media B.V. 2008