Categories: Science

Aliens or chemistry? – Australian Geographic

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Contributor

Fred Watson

Contributor

Fred Watson

Fred Watson is Australia’s Astronomer-at-Large.






By Fred Watson

6 August 2025


One of essentially the most profound questions we will ask is whether or not there reside organisms elsewhere within the universe. So far, there’s no agency proof of life originating anyplace past the confines of our world. In making an attempt to reply the query, astronomers search for biomarkers – attributes of an extraterrestrial setting that may solely have… View Article

One of essentially the most profound questions we will ask is whether or not there reside organisms elsewhere within the universe.

So far, there’s no agency proof of life originating anyplace past the confines of our world.

In making an attempt to reply the query, astronomers search for biomarkers – attributes of an extraterrestrial setting that may solely have originated within the presence of life.

And it doesn’t should be clever life; even humble microbes modify their setting in a way that could possibly be detected by scientific devices, whether or not they be laser zappers on a Mars rover or infrared spectrometers on a large telescope. 

It’s the second of those that has made headlines in current months. Of the just about 6000 exoplanets now recognized past our photo voltaic system, solely a handful qualify as liveable worlds, the place water can stay liquid slightly than boiling away or freezing stable.

Water is the working fluid of all life on Earth, so discovering it in liquid type is an effective place to begin within the quest for exolife. And one in all these liveable planets – often known as K2-18b – has attracted appreciable consideration with experiences of intriguing molecules in its ambiance. 

Exoplanet K2-18b. Illustration credit score: A. Smith/N. Madhusudhan, University of Cambridge

Like many different exoplanets, K2-18b crosses the road of sight to Earth because it orbits its mum or dad star, passing in entrance of it from our perspective. The planet’s ambiance imprints a spectrum signature of its element gases on the starlight filtering by means of it.

This has now been analysed with the James Webb Space Telescope and, in observations reported last April, UK and US astronomers introduced the detection of dimethyl sulphide (DMS) and dimethyl disulphide (DMDS) in K2-18b’s ambiance.

On Earth, these gases solely happen because of organic exercise by microorganisms, which makes them biomarkers. 

These are tantalising outcomes, however there are good causes for warning. Even with such a succesful instrument because the Webb (presently one of the best accessible for this sort of work), they’re difficult observations to make.

Discoveries are couched by way of their confidence degree, which on this case is considerably lower than the gold normal of certainty. It’s potential future observations will rule out the existence of DMS and DMDS altogether.

More basically, the organic origin of those gases on Earth doesn’t essentially eradicate a purely chemical formation elsewhere. They could end up to not be biomarkers, and scientists at the moment are trying rigorously at what different kinds of reactions may generate these molecules.

























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