Large-scale Volcanism and the Heat Death of Terrestrial Worlds
M.J. Way, Richard E. Ernst, Jeffrey D. Scargle

TL;DR
This paper investigates how large-scale volcanism, particularly large igneous provinces, could have contributed to the heat death of terrestrial planets like Venus by causing extreme greenhouse effects and ending volatile cycling.
Contribution
It introduces new statistical and simulation methods to estimate the likelihood of near-simultaneous LIP events and their potential to induce planetary heat death.
Findings
LIPs closer than 0.1-1 million years are likely to occur simultaneously.
Simulated LIP events can cumulatively cause extreme greenhouse conditions.
LIPs may have played a role in Venus's heat death, not just Earth's extinction events.
Abstract
Large-scale volcanism has played a critical role in the long-term habitability of Earth. Contrary to widely held belief, volcanism, rather than impactors, has had the greatest influence on and bears most of the responsibility for large-scale mass extinction events throughout Earth's history. We examine the timing of large igneous provinces (LIPs) throughout Earth's history to estimate the likelihood of nearly simultaneous events that could drive a planet into an extreme moist or runaway greenhouse, leading to the end of volatile cycling and causing the heat death of formerly temperate terrestrial worlds. In one approach, we make a conservative estimate of the rate at which sets of near-simultaneous LIPs (pairs, triplets, and quartets) occur in a random history statistically the same as Earth's. We find that LIPs closer in time than 0.1-1 million yr are likely; significantly, this is…
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