2021
DOI: 10.1093/mnras/stab2237
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A dynamical analysis of the Taurid Complex: evidence for past orbital convergences

Abstract: The goal of this work is to determine if the dynamics of individual Taurid Complex (TC) objects are consistent with the formation of the complex via fragmentation of a larger body, or if the current orbital affinities between the TC members result from other dynamical processes. To this end, the orbital similarity through time of comet 2P/Encke, fifty-one Near-Earth Asteroids (NEAs) and sixteen Taurid fireballs was explored. Clones of each body were numerically simulated backwards in time, and epochs when sign… Show more

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Cited by 11 publications
(14 citation statements)
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“…These asteroids can be considered as large members of the stream rather than parent bodies. Egal et al (2021) confirm their orbital convergence with 2P/Encke and also with 2004 TG10, which is now related to the Northern Taurids, about 5000 years ago. Here we note the close orbital similarity of another asteroid, 2014 NK52, with the Northern Taurids, namely with those observed around mid-November (while the orbit of 2004 TG10 is more similar to NTA meteors observed earlier in November).…”
Section: Possible Related Asteroidssupporting
confidence: 70%
“…These asteroids can be considered as large members of the stream rather than parent bodies. Egal et al (2021) confirm their orbital convergence with 2P/Encke and also with 2004 TG10, which is now related to the Northern Taurids, about 5000 years ago. Here we note the close orbital similarity of another asteroid, 2014 NK52, with the Northern Taurids, namely with those observed around mid-November (while the orbit of 2004 TG10 is more similar to NTA meteors observed earlier in November).…”
Section: Possible Related Asteroidssupporting
confidence: 70%
“…However, this apparent negative observation is less clear as only a large enhancement in fireball rates would be detectable for these daylight streams. Following the call for observations of Clark et al (2019), several new asteroids residing in the 7:2 MMR with Jupiter were discovered during the last return of the TSC in June 2019 (Egal et al 2021). Future swarm years are expected to occur in 2022, 2025 and 2032 for the autumn showers and 2026 and 2029 for the daytime Taurids.…”
Section: Descriptionmentioning
confidence: 99%
“…The semi-major axis extent of the 7:2 MMR at an eccentricity of 0.85-0.87 ranges from about 2.23 to 2.28 AU (Asher 1991;Egal et al 2021). The distribution of the orbital elements of the NTA and STA largely spans the full extent of the resonance (see Figure C3.1), making it possible in principle to observe the TSC returns with different detection methods measuring particles at different sizes.…”
Section: The Taurid Swarm At Different Sizesmentioning
confidence: 99%
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