Scientists have found that a planet more than twice as big as Earth could be habitable, opening up new possibilities in the search for life on other planets.
The new discovery suggests that alien life could flourish on worlds bigger than Earth but smaller than Neptune, just like the exoplanetK2-18b.
Researchers looked at the mass, radius and atmospheric data of the distant exoplanet and used models to find that it is possible the planet could have liquid water, in habitable conditions, underneath the hydrogen-rich atmosphere on its surface.
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The exoplanet is found 124 lightyears away, relatively close by in terms of exoplanets. It is also relatively similar to Earth: with a radius 2.6 times as big as our planet’s and a mass 8.6 times Earth’s.
The new study gives the first look at what conditions could be like underneath that atmosphere, however. And it suggests that they could be habitable in just the way scientists had hoped.
Dr Nikku Madhusudhan from Cambridge’s Institute of Astronomy, who led the study, said: “Water vapour has been detected in the atmospheres of a number of exoplanets but, even if the planet is in the habitable zone, that doesn’t necessarily mean there are habitable conditions on the surface.
“To establish the prospects for habitability, it is important to obtain a unified understanding of the interior and atmospheric conditions on the planet – in particular, whether liquid water can exist beneath the atmosphere.”
Because of the size of K2-18b, some suggest it would be more like a smaller version of Neptune than a larger version of Earth.
It is thought a mini-Neptune would have a significant hydrogen envelope surrounding a layer of high-pressure water, with an inner core of rock and iron.
If this envelope is too thick, it would be too hot, and pressure at the surface of the water layer beneath would be far too great to support life.
According to the new study published in The Astrophysical Journal Letters, despite the size of K2-18b, its hydrogen envelope is not necessarily too thick and the water layer could support life.
Astronomers used the existing observations of the atmosphere, to confirm the atmosphere is hydrogen-rich with a significant amount of water vapour.
They also found that levels of other chemicals such as methane and ammonia were lower than expected.
But whether these levels can be attributed to biological processes remains to be seen.
The researchers found that the maximum extent of the hydrogen envelope allowed by the data is around 6% of the planet’s mass, though most of the solutions require much less.
The minimum amount of hydrogen is about one-millionth by mass, similar to the mass fraction of the Earth’s atmosphere.