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A dry Venusian interior constrained by atmospheric chemistry
Tereza Constantinou, Oliver Shorttle, Paul B. Rimmer
Venus's climatic history provides powerful constraint on the location of the inner-edge of the liquid-water habitable zone. However, two very different histories of water on Venus…
A Surface Hydrothermal Source of Nitriles and Isonitriles
Paul B. Rimmer, Oliver Shorttle
Giant impacts can generate transient hydrogen-rich atmospheres, reducing atmospheric carbon. The reduced carbon will form hazes that rain out onto the surface and can become incorp…
Astrobiological Potential of Venus Atmosphere Chemical Anomalies and Other Unexplained Cloud Properties
Janusz J. Petkowski, Sara Seager, David H. Grinspoon +7
Long-standing unexplained Venus atmosphere observations and chemical anomalies point to unknown chemistry but also leave room for the possibility of life. The unexplained observati…