Meteor showers from active asteroids and dormant comets in near-Earth space: a review
Quan-Zhi Ye

TL;DR
This review discusses how meteor showers originating from active asteroids and dormant comets in near-Earth space can reveal the history and activity of these small bodies, highlighting recent survey advancements and analytical challenges.
Contribution
It provides a comprehensive overview of the connection between meteor showers and their parent small bodies, emphasizing recent survey data and the need for detailed analysis.
Findings
Statistical tests help identify parent-shower pairs.
Meteor outbursts indicate recent activity from parent bodies.
Orphan showers suggest historic disintegration events.
Abstract
Small bodies in the solar system are conventionally classified into asteroids and comets. However, it is recently found that a small number of objects can exhibit properties of both asteroids and comets. Some are more consistent with asteroids despite episodic ejections and are labeled as "active asteroids", while some might be aging comets with depleting volatiles. Ejecta produced by active asteroids and/or dormant comets are potentially detectable as meteor showers at the Earth if they are in Earth-crossing orbits, allowing us to retrieve information about the historic activities of these objects. Meteor showers from small bodies with low and/or intermittent activities are usually weak, making shower confirmation and parent association challenging. We show that statistical tests are useful for identifying likely parent-shower pairs. Comprehensive analyses of physical and dynamical…
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