In their quest to find a planet where conditions can lead to the proliferation of life, astronomers have discovered water vapour on the exoplanet K2-18b.
Results from the Kepler satellite mission, which discovered nearly 2/3 of all known exoplanets to date, indicate that 5 to 20 per cent of Earths and super-Earths are located in the habitable zone of their stars.
However, despite this abundance, probing the conditions and atmospheric properties on any of these habitable zone planets is extremely difficult and has remained elusive... until now.
A new study by Professor Bjorn Benneke of the Institute for Research on Exoplanets at the Universite de Montreal, his doctoral student Caroline Piaulet and several of their collaborators reports the detection of water vapour and perhaps even liquid water clouds in the atmosphere of the planet K2-18b.
This exoplanet is about nine times more massive than our Earth and is found in the habitable zone of the star it orbits, reported the study published in the 'Astronomical Journal'.
This M-type star is smaller and cooler than our Sun, but due to K2-18b's close proximity to its star, the planet receives almost the same total amount of energy from its star as our Earth receives from the Sun.
The similarities between the exoplanet K2-18b and the Earth suggest to astronomers that the exoplanet may potentially have a water cycle possibly allowing water to condense into clouds and liquid water rain to fall.
This detection was made possible by combining eight transit observations -- the moment when an exoplanet passes in front of its star -- taken by the Hubble Space Telescope.
The Universite de Montreal is no stranger to the K2-18 system located 111 light-years away.
The existence of K2-18b was first confirmed by Professor Benneke and his team in a 2016 paper using data from the Spitzer Space Telescope.
The mass and radius of the planet were then determined by former Universite de Montreal and University of Toronto PhD student Ryan Cloutier. These promising initial results encouraged the iREx team to collect follow-up observations of the intriguing world."
Scientists currently believe that the thick gaseous envelope of K2-18b likely prevents life as we know it from existing on the planet's surface. However, the study showed that even these planets of relatively low mass which are therefore more difficult to study can be explored using astronomical instruments developed in recent years.
By studying these planets which are in the habitable zone of their star and have the right conditions for liquid water, astronomers are one step closer to directly detecting signs of life beyond our Solar System.
"This represents the biggest step yet taken towards our ultimate goal of finding life on other planets, of proving that we are not alone. Thanks to our observations and our climate model of this planet, we have shown that its water vapour can condense into liquid water. This is a first," said Bjorn Benneke.
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