339 citations · 2.8k across the 52 of their papers we have counts for
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Ammonia and Phosphine in the Clouds of Venus as Potentially Biological Anomalies
Carol E. Cleland, Paul B. Rimmer
We are of the opinion that several anomalies in the atmosphere of Venus provide evidence of yet-unknown processes and systems that are out of equilibrium. The investigation of thes…
Growth and Evolution of Secondary Volcanic Atmospheres: II. The Importance of Kinetics
Philippa Liggins, Sean Jordan, Paul B. Rimmer +1
Volcanism is a major and long-term source of volatile elements such as C and H to Earth's atmosphere, likely has been to Venus's atmosphere, and may be for exoplanets. Models simul…
Proposed energy-metabolisms cannot explain the atmospheric chemistry of Venus
Sean Jordan, Oliver Shorttle, Paul B. Rimmer
Life in the clouds of Venus, if present in sufficiently high abundance, must be affecting the atmospheric chemistry. It has been proposed that abundant Venusian life could obtain e…
Linking atmospheric chemistry of the hot Jupiter HD 209458b to its formation location through infrared transmission and emission spectra
Spandan Dash, Liton Majumdar, Karen Willacy +6
The elemental ratios of carbon, nitrogen, and oxygen in the atmospheres of hot Jupiters may hold clues to their formation locations in the protostellar disc. In this work, we adopt…
Reduced atmospheres of post-impact worlds: The early Earth
J. P. Itcovitz, A. S. P. Rae, R. I. Citron +4
Impacts may have had a significant effect on the atmospheric chemistry of the early Earth. Reduced phases in the impactor (e.g., metallic iron) can reduce the planet's HO inven…
Constraints on the production of phosphine by Venusian volcanoes
William Bains, Oliver Shorttle, Sukrit Ranjan +4
The initial reports of the presence of phosphine in the cloud decks of Venus has led to the suggestion that volcanism was the source of phosphine, through volcanic phosphides eject…