A decadal survey of the Daytime Arietid meteor shower using the Canadian Meteor Orbit Radar

被引:18
作者
Bruzzone, J. S. [1 ]
Brown, P. [1 ]
Weryk, R. J. [1 ]
Campbell-Brown, M. D. [1 ]
机构
[1] Univ Western Ontario, Dept Phys & Astron, London, ON N6A 3K7, Canada
关键词
meteorites; meteors; meteoroids; COMET; 96P/MACHHOLZ; STATISTICAL-MODEL; ASSOCIATION; MACHHOLZ; STREAMS; MARSDEN;
D O I
10.1093/mnras/stu2200
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present results from a 12 year survey of the Daytime Arietid meteor shower using the Canadian Meteor Orbit Radar, a VHF backscattering orbital meteor radar, covering the interval 2002-2013. This survey recorded more than 2 x 10(4) Daytime Arietid orbits having representative masses of 8 x 10(-8) kg and sizes of approximate to 0.4 mm. The core activity for the Arietids is found in the range 73.degrees 5 <= lambda(circle dot) <= 84.degrees 5 and shows a broad 4-d maximum centred near lambda(circle dot) = 80.degrees 5 of 0.04 meteoroids km(-2) h(-1) producing meteors of equivalent radio magnitude of +6.5 from a mean radiant at alpha(g) = 44.degrees 9 +/- 1.degrees 1, delta(g) = 25.degrees 5 +/- 1.degrees 0. During the plateau of shower peak activity, the mass index of the stream reaches a minimum with s = 1.6-1.7. Contamination from another nearby shower (likely the Daytime Zeta Perseids) and/or sub-streams showing different orbits compared to the core of the stream is evident in the interval 60.degrees 5 <= lambda(circle dot) <= 71.degrees 5. Similar contamination beyond lambda(circle dot) = 84.degrees 5 may be due to the Helion sporadic source. We also characterized the deceleration profiles for Daytime Arietid meteor echoes using several independent speed techniques including Fresnel pre-t(0), Fresnel amplitude oscillation and time-of-flight speeds which together with modelling produced a best estimate for the stream's out-of-atmosphere speed of v(infinity) = 40.5 +/- 0.7 km s(-1). The mean radar orbit from our study is noticeably smaller in semi-major axis and eccentricity than is found for larger Arietids measured with optical systems, a difference which if real indicates a particle-size sorting of the stream orbit. The broad activity maximum, long duration of activity and particle-size dependence of the orbital elements suggest the stream is too old to have been solely formed during the breakup of the parent comet of the Marsden sunskirters about a millennium ago as proposed by Sekanina & Chodas.
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页码:1625 / 1640
页数:16
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