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Published in 2020 at "Icarus"
DOI: 10.1016/j.icarus.2020.113740
Abstract: Abstract Proto-Mars growing within the solar nebula may have maintained both the hydrogen-dominated solar component and the impact degassed component enriched in H2, CH4 and CO as a proto-atmosphere. Such a proto-atmosphere would experience hydrodynamic…
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Keywords:
escape;
escape early;
hydrodynamic escape;
early martian ... See more keywords
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Published in 2019 at "Eos"
DOI: 10.1029/2019eo136720
Abstract: An air-sampling study has captured long-term trends in the concentrations of five key atmospheric gases for the first time.
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Keywords:
mystery martian;
rover reveals;
oxygen mystery;
curiosity rover ... See more keywords
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Published in 2020 at "Journal of Geophysical Research"
DOI: 10.1029/2020je006491
Abstract: We develop an existing 1-D photochemistry model to include a comprehensive description of organic chemistry on Mars that includes the oxidation products of methane (CH$_4$) and ethane (C$_2$H$_6$),...
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Keywords:
chemistry;
photochemistry methane;
methane ethane;
martian atmosphere ... See more keywords
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Published in 2023 at "Geophysical Research Letters"
DOI: 10.1029/2023gl103457
Abstract: It has been known for decades that carbon dioxide (CO2) ice clouds exist in the Martian atmosphere. According to remote sensing observations and previous modeling studies, the Martian CO2 ice crystals may be sufficiently large…
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Keywords:
ice;
carbon dioxide;
ice crystals;
co2 ice ... See more keywords
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Published in 2020 at "Nature Communications"
DOI: 10.1038/s41467-020-14510-x
Abstract: The atmosphere of Mars is strongly affected by the spatial and temporal variability of airborne dust. However, global dust variability within a sol (Martian day) is still poorly understood. Although short-term dynamic processes are crucial,…
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Keywords:
dust tides;
storms dust;
dust;
dust storms ... See more keywords