The ejection velocity of meteoroids from cometary nuclei deduced from observations of meteor shower outbursts

Details The ejection velocity of meteoroids from cometary nuclei deduced from observations of meteor shower outbursts The ejection velocity of meteoroids from cometary nuclei deduced from observations of meteor shower outbursts

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001mnras.325..379m&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 325, Issue 1, pp. 379-384.

Astronomy and Astrophysics

Astronomy

15

Comets: Individual: 55P/Tempel-Tuttle, Comets: Individual: 109P/Swift-Tuttle, Meteors, Meteoroids

Scientific paper

Q11The ejection velocities of meteoroids belonging to the Leonid and Perseid meteoroid streams are deduced from the observed differences between the longitude of the ascending node of the outburst meteoroids and that of the parent comet. The difference is very sensitive to the true anomaly of the ejection point, as well as the ejection velocity, and probable values for both are discussed.

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