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Early Martian Climate

The debate over the early Martian climate is among the most intriguing in planetary science.

Climate simulations of early Mars with estimated precipitation, runoff, and erosion rates

Early Martian Climate

The nature of the early Martian climate has been the subject of debate for decades, with geologic evidence suggesting an environment with prolonged precipitation and flowing liquid water on the surface, while climate models have struggled to reproduce such conditions.

Testing the impact heating hypothesis for early Mars with a 3-D global climate model

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10.1038/S42254-019-0085-8

Three publications in Geophysical Research Letters describe details of the Martian climate, including global dust storms and polar ice caps.

Icy red planet

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10.3844/JMRSP.2019.1.32

The objectives of the rover include an investigation into Martian climate and geology; assessing whether the site selected in Gale has ever provided environmentally friendly environmental conditions for microbial life, including investigating the role of water; and studies on planetary habitats in preparation for human exploration.

About the Space Robots

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10.1038/s41561-019-0458-8

Our findings support stepwise changes in Martian climate during the Hesperian, leading to more arid and sulfate-dominated environments as previously inferred from orbital observations.

An interval of high salinity in ancient Gale crater lake on Mars

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10.1016/J.GEOMORPH.2019.02.022

We propose that the martian climate during the late Noachian/early Hesperian was characterized by glaciated highlands at elevations >1500 m and at lower elevations where fluvial valley network has been identified (.

Morphometric evidence of 3.6 Ga glacial valleys and glacial cirques in martian highlands: South of Terra Sabaea

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10.1016/j.icarus.2018.09.021

Overall, our results quantify NOMAD's capability to address the variable aspects of Martian climate.

Methane on Mars: New insights into the sensitivity of CH4 with the NOMAD/ExoMars spectrometer through its first in-flight calibration

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10.1002/essoar.10501840.1

A key to understanding the evolution of the Martian climate over its history is the study of how the Martian atmosphere escapes to space.

Effects of Spatial Resolution on the Martian Pickup Ion Plume in Global Martian Plasma Simulations

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Martian Climate - Three publications in Geophysical Research Letters describe details of the Martian climate, including global dust storms and polar ice caps. [1] The objectives of the rover include an investigation into Martian climate and geology; assessing whether the site selected in Gale has ever provided environmentally friendly environmental conditions for microbial life, including investigating the role of water; and studies on planetary habitats in preparation for human exploration. [2] Our findings support stepwise changes in Martian climate during the Hesperian, leading to more arid and sulfate-dominated environments as previously inferred from orbital observations. [3] We propose that the martian climate during the late Noachian/early Hesperian was characterized by glaciated highlands at elevations >1500 m and at lower elevations where fluvial valley network has been identified (. [4] Overall, our results quantify NOMAD's capability to address the variable aspects of Martian climate. [5] A key to understanding the evolution of the Martian climate over its history is the study of how the Martian atmosphere escapes to space. [6]

Early Martian Climate

The debate over the early Martian climate is among the most intriguing in planetary science. [1] The nature of the early Martian climate has been the subject of debate for decades, with geologic evidence suggesting an environment with prolonged precipitation and flowing liquid water on the surface, while climate models have struggled to reproduce such conditions. [2] Evidence of this early Martian climate with CO2 vapor as the main component causing greenhouse warming has been challenged by the lack of carbonate in these profiles. [3]