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Simulations Show Mars Helps Shape Earth’s Ice‑Age Cycles

New models reveal the small planet’s gravity drives key orbital patterns pacing long‑term climate shifts.

Overview

  • Mars’s gravitational pull emerged as a major driver of Earth’s long‑period orbital variations in peer‑reviewed simulations led by Stephen Kane.
  • Removing Mars from the models erased a roughly 2.4‑million‑year grand cycle and a separate ~100,000‑year eccentricity rhythm linked to ice‑age pacing.
  • Increasing Mars’s mass shortened and intensified those eccentricity cycles, indicating a stronger climatic imprint with a heavier Mars.
  • A ~405,000‑year eccentricity cycle persisted regardless of Mars, reflecting dominant influences from Venus and Jupiter on that component.
  • The experiments also showed a stabilizing effect on Earth’s axial‑tilt wobble, and researchers say such small‑planet effects must be accounted for when assessing exoplanet climates.