H$_2$O$_2$-induced Greenhouse Warming on Oxidized Early Mars
Yuichi Ito, George L. Hashimoto, Yoshiyuki O. Takahashi, Masaki, Ishiwatari, Kiyoshi Kuramoto

TL;DR
This study proposes that H₂O₂ could have significantly contributed to warming early Mars' oxidized atmosphere, enabling liquid water stability without reduced greenhouse gases, based on atmospheric modeling of H₂O₂'s infrared absorption.
Contribution
It introduces the novel idea that H₂O₂ alone could have warmed early Mars' oxidized environment, challenging previous assumptions about greenhouse gas requirements.
Findings
1 ppm of H₂O₂ can raise surface temperature above 273 K at 3 bar CO₂.
H₂O₂ can be sustained in the upper atmosphere due to photochemical production.
Oxidized early Mars could have maintained a warm, wet environment with H₂O₂ as a greenhouse agent.
Abstract
The existence of liquid water within an oxidized environment on early Mars has been inferred by the Mn-rich rocks found during recent explorations on Mars. The oxidized atmosphere implied by the Mn-rich rocks would basically be comprised of CO and HO without any reduced greenhouse gases such as H and CH. So far, however, it has been thought that early Mars could not have been warm enough to sustain water in liquid form without the presence of reduced greenhouse gases. Here, we propose that HO could have been the gas responsible for warming the surface of the oxidized early Mars. Our one-dimensional atmospheric model shows that only 1 ppm of HO is enough to warm the planetary surface because of its strong absorption at far-infrared wavelengths, in which the surface temperature could have reached over 273~K for a CO atmosphere with a pressure of 3~bar.…
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