Here we go again. A team of scientists (led by Professor Jane Greaves of Cardiff University) has discovered possible evidence of life on another planet.
In this case, the planet is Venus and the ‘evidence’ is the detection of phosphine (PH3) — a gas associated with microbial activity.
In theory, the chemistry of PH3 is such that a biological process would be required to produce it naturally in detectable quantities. In other words, it is a ‘biosignature’ gas — or, less politely, a fart.
Just as there is no smoke without fire, there are no farts without life, which is why detecting phosphine in the Venusian atmosphere is such a big deal.
Of course, all this assumes that the theory is right and that the gas can only have had a biotic origin. So it’s worth pointing out that phosphine has already been detected on Jupiter (and Saturn) without anyone pointing the finger at extraterrestrials. However, unlike an ultra-cold gas giant, Venus is hot and rocky — and thus some hitherto unsuspected chemical process would be required to produce the phosphine abiotically (i.e. without life).
So is life the simpler explanation? No, because we’d need some hitherto unsuspected biological process to explain its presence on Venus.
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