Recent multi-kiloton impact events: are they truly random?

TL;DR

This study analyzes impact events over 2000 and finds that multi-kiloton impacts are not randomly distributed, suggesting planetary influences and potential periodicity in impact hazards, challenging the assumption of randomness.

Contribution

It provides the first statistical evidence that large impact events are non-random and influenced by planetary perturbations, especially Jupiter, indicating possible impact periodicity.

Findings

Impact cadence is incompatible with random distribution at 0.05 significance level.

Impact distribution aligns with the longitudes of NEOs' ascending nodes.

Impact hazard may peak at specific times annually.

Abstract

It is customarily assumed that Earth-striking meteoroids are completely random, and that all the impacts must be interpreted as uncorrelated events distributed according to Poisson statistics. If this is correct, their impact dates must be uniformly spread throughout the year and their impact coordinates must be evenly scattered on the surface of our planet. Here, we use a time- and yield-limited sample of Earth-impacting superbolides detected since 2000 to explore statistically this critical though frequently overlooked topic. We show that the cadence of these multi-kiloton impact events is incompatible with a random fall pattern at the 0.05 significance level or better. This result is statistically robust and consistent with the observed distribution of the longitudes of the ascending nodes of near-Earth objects (NEOs). This lack of randomness is induced by planetary perturbations, in particular Jupiter's, and suggests that some of the recent, most powerful Earth impacts may be associated with resonant groups of NEOs and/or very young meteoroid streams. An intriguing consequence of this scenario is that the impact hazard of Chelyabinsk-like objects should peak at certain times in the year.