Showing 1–20 of 33 results
/ Date/ Name
May 27, 2023Large Uncertainties in the Thermodynamics of Phosphorus (III) Oxide (P$_4$O$_6$) Have Significant Implications for Phosphorus Species in Planetary AtmospheresApr 16, 2013Martian Methyl Chloride. A lesson in uncertaintyApr 19, 2021Recovery of Spectra of Phosphine in Venus' CloudsJan 8, 2021Evolution of default genetic control mechanismsSep 14, 2020Phosphine Gas in the Cloud Decks of VenusFeb 26, 2013Photochemistry in Terrestrial Exoplanet Atmospheres II: H2S and SO2 Photochemistry in Anoxic AtmospheresNov 9, 2021Venusian phosphine: a 'Wow!' signal in chemistry?Mar 26, 2021Assessment of Isoprene as a Possible Biosignature Gas in Exoplanets with Anoxic AtmospheresOct 11, 2019Phosphine as a Biosignature Gas in Exoplanet AtmospheresJun 19, 2023Stability of nucleic acid bases in concentrated sulfuric acid: Implications for the habitability of Venus' cloudsJun 12, 2023Venus' Atmospheric Chemistry and Cloud Characteristics Are Compatible with Venusian LifeJan 14, 2024Alternative solvents for life: framework for evaluation, current status and future researchMay 18, 2017Exoplanet Biosignatures: A Framework for Their AssessmentAug 11, 2025Warm, water-depleted rocky exoplanets with surface ionic liquids: A proposed class for planetary habitabilityMar 3, 2026Ionic Liquid BiospheresSep 14, 2020The Venusian Lower Atmosphere Haze as a Depot for Desiccated Microbial Life: A Proposed Life Cycle for Persistence of the Venusian Aerial BiosphereJun 14, 2021Possibilities for an Aerial Biosphere in Temperate Sub Neptune-Sized Exoplanet AtmospheresNov 16, 2020Re-analysis of Phosphine in Venus' CloudsDec 10, 2020On the Robustness of Phosphine Signatures in Venus' CloudsDec 20, 2021Production of Ammonia Makes Venusian Clouds Habitable and Explains Observed Cloud-Level Chemical Anomalies