Abstract
The Arietid meteor shower is one of the strongest of the year. The origin of this daytime shower is unknown; the orbit is therefore of great interest, since an accurate orbit distribution is needed to integrate the shower backward in time to test associations with comets or asteroids. The orbital parameters of the Arietid shower as a function of time, with errors, have been generated using 415 radar orbits gathered at the CMOR facility in Tavistock, Canada.
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Campbell-Brown, M.D. (2005). Arietid Meteor Orbits Measurements. In: Hawkes, R., Mann, I., Brown, P. (eds) Modern Meteor Science An Interdisciplinary View. Springer, Dordrecht. https://doi.org/10.1007/1-4020-5075-5_31
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DOI: https://doi.org/10.1007/1-4020-5075-5_31
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Online ISBN: 978-1-4020-5075-6
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