
TL;DR
Recent advances in observations and climate modeling suggest early Mars experienced episodic warmth and transient melting, despite a generally cold climate due to low solar flux and greenhouse gas inefficiency, impacting its habitability.
Contribution
This paper synthesizes recent geologic evidence and climate models to clarify the nature of early Martian climate and its implications for water activity and habitability.
Findings
Episodic warm periods caused melting of snow and ice.
Water erosion features indicate transient hydrological activity.
Early Mars likely lacked a sustained northern ocean.
Abstract
The nature of the early Martian climate is one of the major unanswered questions of planetary science. Key challenges remain, but a new wave of orbital and in situ observations and improvements in climate modeling have led to significant advances over the last decade. Multiple lines of geologic evidence now point to an episodically warm surface during the late Noachian and early Hesperian periods 3-4 Ga. The low solar flux received by Mars in its first billion years and inefficiency of plausible greenhouse gases such as CO2 means that the steady-state early Martian climate was likely cold. A denser CO2 atmosphere would have caused adiabatic cooling of the surface and hence migration of water ice to the higher altitude equatorial and southern regions of the planet. Transient warming caused melting of snow and ice deposits and a temporarily active hydrological cycle, leading to erosion of…
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