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Geosciences (Switzerland), ISSN 2076-3263, 08/2018, Volume 8, Issue 8, p. 280
Journal Article
Icarus, ISSN 0019-1035, 11/2017, Volume 297, pp. 71 - 82
The climate of early Mars has been hotly debated for decades. Although most investigators believe that the geology indicates the presence of surface water,... 
Mars | Evolution | Climate | Atmospheres | Atmosphere | COLLISION-INDUCED ABSORPTION | EARTH | GREENHOUSE | CO2 | GALE CRATER | HABITABLE ZONES | ASTRONOMY & ASTROPHYSICS | RAYLEIGH-SCATTERING | WATER | Planets | Hydrogen | Mars (Planet) | Climate models | Physics - Earth and Planetary Astrophysics
Journal Article
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, ISSN 0035-8711, 07/2018, Volume 477, Issue 4, pp. 4627 - 4640
Traditional definitions of the habitable zone assume that habitable planets contain a carbonate-silicate cycle that regulates CO2 between the atmosphere,... 
COLLISION-INDUCED ABSORPTION | ANTARCTIC SEA-ICE | RUNAWAY GREENHOUSE | planets and satellites: atmospheres | EARTH-MASS PLANETS | ALBEDO FEEDBACK | CO2 | M DWARFS | astrobiology | ASTRONOMY & ASTROPHYSICS | EARLY MARS | STARS | stars: low-mass | CLIMATE | Physics - Earth and Planetary Astrophysics
Journal Article
Journal Article
Nature Geoscience, ISSN 1752-0894, 2014, Volume 7, Issue 1, pp. 59 - 63
  The presence of valleys on ancient terrains of Mars suggests that liquid water flowed on the martian surface 3.8 Gyr ago or before. The above-freezing... 
Physics - Earth and Planetary Astrophysics
Journal Article
Proceedings of the National Academy of Sciences of the United States of America, ISSN 0027-8424, 09/2014, Volume 111, Issue 35, p. 12641
  The habitable zone (HZ) around a star is typically defined as the region where a rocky planet can maintain liquid water on its surface. That definition is... 
Planets | Planetology | Astrobiology | Definitions | Space telescopes | Photosynthesis | Greenhouse gases
Journal Article
Astrophysical Journal, ISSN 0004-637X, 05/2018, Volume 858, Issue 2, p. 72
The habitable zone (HZ) is the circumstellar region where standing bodies of liquid water could exist on the surface of a rocky planet. Conventional... 
planets and satellites: terrestrial planets | planets and satellites: atmospheres | astrobiology | GREENHOUSE | CO2 | MODEL | ATMOSPHERE | ORGANIC HAZES | EVOLUTION | KINETICS | ASTRONOMY & ASTROPHYSICS | EARLY MARS | SPECTRUM | WATER | Physics - Earth and Planetary Astrophysics
Journal Article
Icarus, ISSN 0019-1035, 01/2017, Volume 281, pp. 248 - 261
Journal Article
Nature Geoscience, ISSN 1752-0894, 08/2017, Volume 10, Issue 8, pp. 556 - 560
Ongoing and future space missions aim to identify potentially habitable planets in our Solar System and beyond. Planetary habitability is determined not only... 
PLANETS | ALBEDO | EARTH | INNER EDGE | GEOSCIENCES, MULTIDISCIPLINARY | MODERN SOFT SNOWBALL | INITIATION | HABITABLE ZONE | CARBON-DIOXIDE | FEEDBACK | WATER | Climate | Greenhouse effect | Oceans | Extrasolar planets | Insolation | Ice | Climate models | Fluxes | Global climate | Water vapor | Greenhouse gases | Water loss | Planets | Space missions | Venus | Climatic evolution | Evolution | Europa | F stars | Physics - Earth and Planetary Astrophysics
Journal Article
Astrobiology, ISSN 1531-1074, 08/2014, Volume 14, Issue 8, pp. 714 - 731
Journal Article
Nature Geoscience, ISSN 1752-0894, 02/2013, Volume 7, Issue 1, pp. 59 - 63
The presence of valleys on ancient terrains of Mars suggests that liquid water flowed on the martian surface 3.8Gyr ago or before. The above-freezing... 
Mars | Temperature | Valleys | Carbon dioxide | Greenhouses | Air pollution | Martian meteorites | Mars atmosphere | Climate models
Journal Article
08/2019
The debate over the early Martian climate is among the most intriguing in planetary science. Although the geologic evidence generally supports a warmer and... 
Physics - Earth and Planetary Astrophysics
Journal Article