Prediction for close approaches with terrestrial planets of asteroids from the main belt
Yufan Fane Zhou, Zhiyuan Li, Hailiang Li, Liyong Zhou

TL;DR
This study uses numerical simulations incorporating the Yarkovsky effect to predict the frequency and characteristics of asteroid close approaches to terrestrial planets, extending the understanding of potentially hazardous asteroids beyond Earth.
Contribution
It extends the concept of close approach analysis to all terrestrial planets and provides detailed predictions of asteroid encounter frequencies and velocities.
Findings
Predicted 1893 Mercury-CAPHAs, 3014 Venus-CAPHAs, 3791 Earth-CAPHAs, 18066 Mars-CAPHAs.
Predicted encounter frequencies are about 1, 9, 15, and 66 per year for Mercury, Venus, Earth, and Mars.
Simulation results for Mars-CAPHAs are consistent with previous work.
Abstract
Potentially Hazardous Asteroids (PHAs), a special subset of Near-Earth Objects, are both dangerous and scientifically valuable. PHAs that truly undergo close approaches with the Earth (dubbed CAPHAs) are of particular interest and extensively studied. The concept and study of CAPHA can be extended to other Solar system planets, which have significant implications for future planet-based observations and explorations. In this work, we conduct numerical simulations that incorporate the Yarkovsky effect to study the transformation of main belt asteroids into CAPHAs of terrestrial planets, using precise nominal timesteps, especially to ensure the reliability of the results for Mercury and Venus. Our simulations predict a total of 1893 Mercury-CAPHAs, 3014 Venus-CAPHAs, 3791 Earth-CAPHAs and 18066 Mars-CAPHAs, with an occurrence frequency of about 1, 9, 15 and 66 per year, respectively. The…
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Taxonomy
TopicsAstro and Planetary Science · Space Exploration and Technology · Stellar, planetary, and galactic studies
