The Dependence of Earth Milankovitch Cycles on Martian Mass
Stephen R. Kane, Pam Vervoort, Jonathan Horner

TL;DR
This study investigates how variations in Martian mass influence Earth's Milankovitch cycles, revealing that Mars' mass significantly alters Earth's orbital and axial tilt variations, which are crucial for understanding climate evolution.
Contribution
It provides a detailed dynamical analysis showing the dependence of Earth's Milankovitch cycles on Martian mass, highlighting the sensitivity of Earth's climate forcing spectrum to planetary neighborhood changes.
Findings
Mars' increased mass enhances short-eccentricity bands.
The 2.4 Myr grand cycle disappears at zero Mars mass.
Obliquity cycles shift from 41 kyr to 45-55 kyr with more massive Mars.
Abstract
The Milankovitch cycles of Earth result from gravitational interactions with other bodies in the Solar System. These interactions lead to slow changes in the orbit and angular momentum vector of Earth, and correspondingly influence Earth's climate evolution. Several studies have shown that Mars may play a significant role in these Milankovitch cycles, such as the 2.4 Myr eccentricity cycle related to perihelion precession dynamics. Here we provide the results of a detailed dynamical analysis that explores the Earth Milankovitch cycles as a function of the Martian mass to quantify the extent that Mars influences variations in Earth's orbital eccentricity, the longitude of perihelion, the longitude of the ascending node, and obliquity (axial tilt). Our results show that, although the 405 kyr long-eccentricity metronome driven by (Venus) and (Jupiter) persists at all Mars…
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Taxonomy
TopicsEarth Systems and Cosmic Evolution · Stellar, planetary, and galactic studies · Space Science and Extraterrestrial Life
