The detection of phosphine () in the clouds of Venus is a potential biosignature because abiotic pathways on temperate planets produce it in negligible amounts. On Venus, thermodynamic models show that atmospheric conditions rapidly oxidize phosphine into phosphorus oxides, requiring a continuous source of replenishment. Some researchers propose that active volcanism releases sufficient phosphorus to explain the observed levels. However, Venusian volcanic gases contain too little water to reduce volcanic phosphorus into phosphine, and the direct photolysis of phosphorus oxides by ultraviolet light requires a hydrogen donor that is absent in the upper atmosphere. Which choice most logically completes the text?
- Athe presence of phosphine constitutes definitive proof of biological activity in the Venusian clouds.
- Bvolcanic activity on Venus must be far less widespread than previously estimated by atmospheric models.
- any abiotic mechanism replenishing Venusian phosphine must rely on pathways other than the proposed volcanic emissions or upper-atmosphere photolysis.Answer
- Dphosphine is capable of resisting oxidation under the high pressure and temperature of the lower Venusian atmosphere.
Answer
The correct answer states that any abiotic mechanism replenishing Venusian phosphine must rely on pathways other than the proposed volcanic emissions or upper-atmosphere photolysis.
The text states that phosphine on Venus is rapidly oxidized and requires continuous replenishment. It evaluates two proposed abiotic mechanisms for this replenishment: volcanic activity (ruled out because the gases contain too little water to reduce phosphorus) and ultraviolet photolysis (ruled out because the upper atmosphere lacks a hydrogen donor). Therefore, if phosphine is indeed present and being replenished, any abiotic explanation must involve processes other than these two refuted pathways.
Step-by-Step Solution
Key Concept
Drawing logical conclusions based solely on the elimination of proposed pathways described in the text.