In new research, a team of scientists at the University of Cambridge has tested the ‘life in the Venusian clouds’ hypothesis. Jordan et al. demonstrate that the three sulfur-based metabolic pathways proposed for Venusian aerial life are capable of reproducing the observed sulfur dioxide-depletion in the cloud layer of Venus, but in each case they require a source of chemical reducing power roughly equal in abundance to below-cloud sulfur dioxide:...
