The threat of Centaurs for terrestrial planets and their orbital evolution as impactors
M. A. Galiazzo, E. A. Silber, R. Dvorak

TL;DR
This study analyzes the orbital evolution of Centaurs, their potential to impact terrestrial planets, and estimates impact frequencies, crater sizes, and water release, highlighting their role as impactors in the inner solar system.
Contribution
It provides new estimates of impact frequencies, crater sizes, and water release from Centaurs impacting terrestrial planets, based on their orbital evolution and population dynamics.
Findings
Impact frequency for Earth is once every 1.9 Gyr since the Late Heavy Bombardment.
Most craters from Centaurs are less than 10 km in diameter.
Approximately 7% of Centaurs can interact with terrestrial planets.
Abstract
Centaurs are solar system objects with orbits situated among the orbits of Jupiter and Neptune. Centaurs represent one of the sources of Near-Earth Objects. Thus, it is crucial to understand their orbital evolution which in some cases might end in collision with terrestrial planets and produce catastrophic events. We study the orbital evolution of the Centaurs toward the inner solar system, and estimate the number of close encounters and impacts with the terrestrial planets after the Late Heavy Bombardment assuming a steady state population of Centaurs. We also estimate the possible crater sizes. We compute the approximate amount of water released: on the Earth, which is about 0.00001 the total water present now. We also found sub-regions of the Centaurs where the possible impactors originate from. While crater sizes could extend up to hundreds of kilometers in diameter given the…
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