The 2005 October 5 outburst of October Camelopardalids

Astronomy and Astrophysics – Astrophysics

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Scientific paper

Jarmo Moilanen (Finland) detected twelve meteors from a compact geocentric radiant at RA = 164.1 deg +- 2.0 deg, Dec. = +78.9 deg +-0.5 deg$, on the border of Draco and Camelopardalis, in the evening of 2005 October 5. The differential mass distribution index was a low s = 1.4+-0.2 (+0 to -6 magnitude). The new shower was confirmed by Esko Lyytinen (2 meteors, early period only, located at 25.00 deg E, +60.25 deg N) and Ilkka Yrjoelae (4 meteors: 26.4 deg E, +60.9 deg N) at nearby locations, and by Sirko Molau in Germany (7 meteors). Esko Lyytinen calculated an apparent speed of V_{g} = 47.3+-0.5 km/s from one two-station meteor, close to the parabolic limit. We conclude that the event was caused by the 1-revolution dust trail of a yet unidentified potentially Earth-threatening (Halley-type or) Intermediate Long-Period comet with orbital elements similar to those of the meteoroids: Epoch = 2005 October 5, a = infty (range 15 - infty) AU, q = 0.993+-0.001 AU, omega = 170.5+-1 deg, Omega = 192.59+-0.04 deg, and i = 78.53+-0.55 deg (J2000.0). % Z Anonymous, 1947, " Tähtitieteen Harrastajan Kirja", Rsan Julkaisuja III (URSA Publications III),
Suomalaisen Kirjallisuuden Seura Kirjapaino Oy (Association of Finnish literature printing house),
A book for amateur astronomers, 163-164
Bailey, G. P., 1902, "A possible meteor shower on October 4", Nature, 66, 577
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Jenniskens, P., Betlem, H., de Lignie, M. & Langbroek, M., 1997, "The detection of a dust trail
in the orbit of an Earth-threatening long-period comet", Astrophys. J., 479, 441-447
Lyytinen, E. & Jenniskens, P., 2003, "Meteor outbursts from long-period comet dust trails",
Icarus, 162, 443-452
MacKenzie, R. A., 1980, "Solar System Debris", British Meteor Society, Dover, pages 42
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Proc. Meteoroids 2001, Kiruna, Sweden, Aug. 2001, 315-318
Root, E., 1976, "Unusual displays", Meteor News, Journal of the AMS, 36, 13
Sander, W., 1943, "Sternschnuppenschwarm am 1942.X.5d", Die Sterne, 23, 46-46
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Die Sterne, 23, 172

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