THE CURRENT PERSEID METEOR-SHOWER

被引:33
作者
WILLIAMS, IP
WU, ZD
机构
[1] Astronomy Unit, Queen Mary and Westfield College, University of London, Mile End Road, London
关键词
METHODS; NUMERICAL; CELESTIAL MECHANICS; STELLAR DYNAMICS; COMETS; INDIVIDUAL; SWIFT-TUTTLE; METEORS; METEOROIDS;
D O I
10.1093/mnras/269.2.524
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Perseid meteor shower is one of the regular showers, occurring in August each year. Over the last few years, a new peak in the activity curve has appeared about half a day before the established peak. It was generally agreed that this new peak represented meteoroids ejected at a recent perihelion passage of the parent comet, and the recovery of Comet Swift-Tuttle re-enforced this view. A model by Wu & Williams suggested that this new peak should reach its maximum activity in 1994 rather than in 1993 and that a strong display, but not a storm, should be expected. We present here an improved model which again suggests that the 1994 Perseids should be marginally stronger than in 1993, with the peak occurring at a solar longitude of about 139.55-degrees. It is predicted that after 1994 the new peak will start to reduce.
引用
收藏
页码:524 / 528
页数:5
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