Water-Loss Mechanism Discovered on Venus, Extending Potential for Past Habitability

Scientists have identified a new mechanism that allowed water to escape Venus at twice the rate previously estimated, potentially extending the planet’s habitable conditions in the past. This process, known as HCO+ dissociative recombination, effectively dries out the planet by converting water into carbon monoxide and hydrogen, with the latter escaping into space. The discovery suggests that Venus may have harbored oceans for longer than previously thought, providing more time for life to evolve.

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