In Search of the Potentially Hazardous Asteroids in the Taurid Resonant Swarm

Abstract The Taurid Complex is a large interplanetary system that contains comet 2P/Encke, several meteoroid streams, and possibly a number of near-Earth asteroids. The size and nature of the system have led to the speculation that it was formed through a large-scale cometary breakup. Numerical investigations have suggested that planetary dynamics can create a resonant region with a large number of objects concentrated in a small segment of the orbit, known as the Taurid swarm, which approaches the Earth in certain years and provides favorable conditions for studying the Taurid Complex. Recent meteor observations confirmed the existence of the swarm for millimeter- to meter-sized objects. Here we present a dedicated telescopic search for potentially hazardous asteroids and other macroscopic objects in the Taurid swarm using the Zwicky Transient Facility survey. We determine from our nondetection that there are no more than 9–14 H ≤ 24 (equivalent to a diameter of D ≳ 100 m) objects in the swarm, suggesting that the Encke–Taurid progenitor was ∼10 km in size. A progenitor of such a size is compatible with the prediction of state-of-the-art solar system dynamical models, which expects ∼0.1 D > 10 km objects on Encke-like orbits at any given time.

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Publication Details

Journal
The Planetary Science Journal
Published
2025-04-01
DOI
https://doi.org/10.3847/psj/adbe74
Citations
3
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
3.46

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article

In Search of the Potentially Hazardous Asteroids in the Taurid Resonant Swarm

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3 citations
The Planetary Science Journal
Astro and Planetary Science
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article

In Search of the Potentially Hazardous Asteroids in the Taurid Resonant Swarm

Avery Wold, Denis Vida, Jasmine Li, Richard Dekany, M. J. Graham, David L. Clark, Frank J. Masci, Josiah Purdum, Quanzhi Ye, Eric C. Bellm, B. Racine
article en
3 citations

Abstract

Abstract The Taurid Complex is a large interplanetary system that contains comet 2P/Encke, several meteoroid streams, and possibly a number of near-Earth asteroids. The size and nature of the system have led to the speculation that it was formed through a large-scale cometary breakup. Numerical investigations have suggested that planetary dynamics can create a resonant region with a large number of objects concentrated in a small segment of the orbit, known as the Taurid swarm, which approaches the Earth in certain years and provides favorable conditions for studying the Taurid Complex. Recent meteor observations confirmed the existence of the swarm for millimeter- to meter-sized objects. Here we present a dedicated telescopic search for potentially hazardous asteroids and other macroscopic objects in the Taurid swarm using the Zwicky Transient Facility survey. We determine from our nondetection that there are no more than 9–14 H ≤ 24 (equivalent to a diameter of D ≳ 100 m) objects in the swarm, suggesting that the Encke–Taurid progenitor was ∼10 km in size. A progenitor of such a size is compatible with the prediction of state-of-the-art solar system dynamical models, which expects ∼0.1 D > 10 km objects on Encke-like orbits at any given time.

The Planetary Science JournalVol. 6(4)
California Institute of Technology (US), Western University (CA), Centre National de la Recherche Scientifique (FR), University of Washington (US), Aix-Marseille Université (FR), Poole Hospital (GB), Infrared Processing and Analysis Center (US), City University of Seattle (US)
National Science Foundation, National Aeronautics and Space Administration, California Institute of Technology, Northwestern University, University of Warwick, Trinity College Dublin, Weizmann Institute of Science, Nuclear Safety and Security Commission, Stockholms Universitet, Natural Sciences and Engineering Research Council of Canada, Deutsches Elektronen-Synchrotron, Institut National de Physique Nucléaire et de Physique des Particules
Openalex Percentile: Top 8%
Astro and Planetary Science
3.46
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