In the dim, red light of an alien sun, scientists made a discovery like no other.

The intriguing world, which goes by the impersonal designation K2-18b, lies 110 light-years away in the constellation Leo.

For the first time scientists have identified liquid water on a planet outside the solar system, suggesting it could support life with habitable temperatures.

It sits in its star's "habitable zone," where it is bathed in the right amount of warmth to allow for liquid water on its surface - but several other conditions must be met for that to happen.

The exoplanet - a planet outside our solar system - was first discovered in 2015, but observations by the Hubble Space Telescope have just detected traces of water vapour in its atmosphere.

Astronomers are duelling over what the discovery means.

Twice as large as our own planet and eight times as massive, K2-18b possesses powerful gravity that would make it difficult to walk upon. It orbits close to a red dwarf star, much smaller and cooler than our sun, which bathes the planet in extremely high levels of radiation.

And aside from water vapour, its atmosphere contains mostly hydrogen gas - a molecule that makes up less than 1 part per million of our own atmosphere.

Whether it has a rocky surface below its atmosphere, a frozen ocean, or is just a giant ball of gas, remains unknown, as does the significance of finding water vapour.

Two separate teams of scientists published the detection at the same time.

One paper by Angelos Tsiaras, an astronomer at the University College London, draws on publicly available data produced by Bjorn Benneke, a planetary astronomer at the University of Montreal in Canada.

Its star and atmosphere are so different to ours, “Earth-like conditions are not possible,” Tsiaras told reporters. “The only question that we’re trying to ask here, and we’re pushing forward, is the question of habitability.”

On Tuesday, Benneke's team posted its own analysis of K2-18b on arXiv, which hosts academic papers not yet published in peer-reviewed journals.

Benneke and his colleagues also found signatures of water vapour in K2-18b's skies.

But they were less optimistic than Tsiaras about the potential habitability of this world. The Montreal-based team's interpretation of its data suggests the hydrogen atmosphere forms a thick, gaseous envelope around the planet. This would generate intense pressures at the planet's surface - perhaps enough to push hydrogen into a liquid form.

"It is not a true Earth analogue," the researchers report.

Laura Kreidberg, an astronomer at the Harvard-Smithsonian Centre for Astrophysics, said that K2-18b might be better described as a "mini-Neptune" than a "super Earth."

Extensive research with computer models suggests that, at 1.6 to 1.8 times the mass of Earth, planets tend to become huge and gaseous, rather than rocky.

Though K2-18b is likely solid at its core, the temperatures and pressures at the "surface" would be so high that few complex molecules would survive, let alone any life forms.

"I think the result is amazing," said Kreidberg. "It's definitely the smallest and coolest planet that we've had a glimpse into the atmosphere of so far. . . . But I don't think it's potentially habitable."

An artist's rendering shows Exoplanet K2-18b, foreground, its host star and an accompanying planet in this system. AP

Scientists had detected water only in the atmospheres of "gas giants" - huge exoplanets that lack solid surfaces, much like Jupiter and Saturn in our solar system.

Rocky exoplanets are smaller, making them harder to find and more difficult to study. Even a planet like K2-18b can be examined only with humanity's most sensitive space telescope - the Hubble.

When K2-18b was discovered, Tsiaras and his colleagues thought it would be a good candidate for a form of analysis called transit spectroscopy, which involves studying the changes in a star's light as a planet "transits," or passes in front of it.

The planet is so close to its cool host star that it takes just 33 days to orbit. So, month after month, the researchers waited with Hubble to capture the moment of transit.

As the starlight filtered through the planet's atmosphere, some of it would be absorbed by the gases in the planet's air. By separating the light into its component parts, the scientists could look for signatures of particular molecules.

What they found suggests that the composition of K2-18b's atmosphere could range from 0.1 per cent water vapour (about the proportion in Earth's upper atmosphere) to a whopping 50 per cent. (At its highest, water vapour concentration in Earth's lower atmosphere is about 4 per cent.)

The Hubble isn't sensitive to the right types of light to detect other important molecules, such as nitrogen or methane, so the researchers can only speculate about the precise composition of the atmosphere.

The planet could have thick clouds, like Venus, that would heat its surface to an intolerable degree. Or its atmosphere might be so thin and insubstantial that it offers no protection from the perils of space, like the atmosphere of Mars.

Researchers must wait for more sophisticated tools, such as the long-delayed James Webb Space Telescope, to reveal more details about the distant world.