First results of OH emission from meteor and afterglow: search for organics in cometary meteoroids

Details First results of OH emission from meteor and afterglow: search for organics in cometary meteoroids First results of OH emission from meteor and afterglow: search for organics in cometary meteoroids

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002esasp.500..213a&link_type=abstract

In: Proceedings of Asteroids, Comets, Meteors - ACM 2002. International Conference, 29 July - 2 August 2002, Berlin, Germany. Ed

Physics

2

Meteor Showers: Leonids, Oh, Afterglow

Scientific paper

Spectroscopic observations of 2001 Leonid meteor storm were carried out using an intensified HDTV camera equipped with a reflective grating covering 300 - 850 nm wavelength range. Hydroxyl radical in the cometary meteoroids was observed in fireballs and persistent trains. A good knowledge of the relationship between meteor and comet or meteorite is needed for understanding of the cometary volatiles. In this paper, we show the first detection of OH A-X (0-0) emission from the ground-based meteor observation and discuss about the origin of the discovered OH.

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