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December 7, 2025Scientific Reports0 citationsOpen Access

On the coincidence between the close passage of HD7977 and the Pliocene-Pleistocene transition

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ZCZhuoya Cao

Key Points

  • Impact parameter dramatically affects terrestrial impact probability of comets, raising it significantly for close flybys.
  • Results indicate a strong influence of a galactic tide on the dynamical evolution of the Oort Cloud over time.
  • Utilizing an analytical method saves computation time compared to traditional N-body simulations in calculating comet impact probabilities.
  • Findings imply that environmental changes during the Pliocene-Pleistocene transition might have been influenced by comet activity.

Abstract

The Oort Cloud's dynamical evolution is significantly influenced by both the galactic tide and stellar flybys. This study investigates the particular case of HD7977's close encounter 2.47 Myr ago, which likely repopulated the Inner Oort Cloud and potentially triggered a significant comet shower on Earth. Our results demonstrate that the shower's intensity strongly depends on HD7977's impact parameter (b), with possible flyby distances ranging from 2,300 AU to ∼ 13,000 AU. For the closest approach (Formula: see text AU), the terrestrial impact probability of 1 km comets increases by an order of magnitude compared to the steady state, slightly exceeding the asteroid impact probability at this size scale. We propose an analytical method to compute the probability of comet showers impacting Earth, which saves considerable computation time compared to N-body simulations. We identify a threshold diameter Formula: see text km for which yields Formula: see text in our model, with Formula: see text following a logarithmic dependence on b. These findings suggest that HD7977's flyby may have caused an enhanced comet flux during the Pliocene-Pleistocene transition, which could plausibly be related to the environmental changes at this era.

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Zhuoya Cao (2025) studied this question.

synapsesocial.com/papers/694020f72d562116f28fb2c3https://doi.org/10.1038/s41598-025-29033-y
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