
Differences in the way Earth and Mars orbit the sun.
Image Credit: NASA
Scientific Frontline: "At a Glance" Summary
- Main Discovery: New simulations reveal that Mars exerts a definitive gravitational influence on Earth’s long-term climate patterns and ice ages, significantly shaping the orbital cycles that drive glacial periods.
- Methodology: Researchers utilized advanced computer models to simulate solar system dynamics over millions of years, isolating Mars' specific impact by observing Earth's orbital variations (Milankovitch cycles) with the Red Planet both present and theoretically removed.
- Specific Data: While the 430,000-year cycle driven by Venus and Jupiter remained stable in Mars-free simulations, the 100,000-year and 2.3 million-year climate cycles disappeared entirely without Mars' gravitational pull.
- Mechanism & Dynamics: The study demonstrated that increasing the mass of Mars in simulations stabilized Earth's axial tilt (obliquity) by reducing its rate of change, while simultaneously shortening the duration of specific orbital cycles.
- Implication for Exoplanets: These findings suggest that small, outer-orbit planets may be critical for maintaining the climatic stability of Earth-sized worlds in the habitable zones of other solar systems.






.jpg)
.jpg)
