For the First Time, Water Was Detected in This Habitable Exoplanet
In the atmosphere of this exoplanet, which is 111 light years away, astronomers made an amazing discovery: water.
It is known that about 50% of the exoplanetary atmosphere called K2-18b is filled with water vapor. However, unlike other giant exoplanets that have water in their atmosphere, K2-18b belongs to the Super Earth group and the habitable zone. It has rocky surfaces like Earth, Mars and Venus.
"Finding water other than on Earth is very exciting," said Angelos Tsiaras, an astronomer at University College London.
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K2-18b was first discovered in 2015 and is an exoplanet that is difficult to explain. We know that it orbits the red dwarf star K2-18 quite closely - one rotation of about 33 days. It's not so hot that the water doesn't evaporate from the surface, nor is it so cold that it doesn't freeze.
It is known that the rate of star irradiation in K2-18b is similar to that on Earth and has twice the size of our planet. In 2017, a group of researchers even designated it as a 'rocky planet with an atmosphere - like Earth, but bigger'. They also say that the planet has an interior that is mostly water, then covered by a thick ice shell like Enceladus or Europa.
K2-18b was first discovered by the Kepler telescope, which detected it via the transit method. This occurs when the star system is aligned so that it allows the planet to pass through us and the star (transit) - causing the dimming of the star's light, which eventually detects the telescope.
This transit process can also help us study the planet's atmosphere. When starlight passes through it, some of the waves can be absorbed by certain gases and produce lines on the spectrum. The difference can be seen when you compare the spectral profile of the star with the spectral profile of the transit.
Even so, understanding it is not easy because detecting planets alone requires very sensitive instruments to detect starlight.
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Tsiaras and his team used the WFC3 instrument on the Hubble space telescope. They took pictures of the K2-18b transit in front of the star, then combined them to produce an average weight to create a spectral profile for the planet.
They then find out what the spectral profile shows using modeling. The results show that about 20-50% of the K2-18b atmosphere is water vapor. In comparison, on earth there is about 5% water vapor. That said, K2-18b is a very humid place.
"The analysis we present provides the first direct observational results of the molecular signatures of habitable zone exoplanets. We link theoretical studies to observations," the researchers said in the study published in the journal Nature Astronomy.
"Although the subject of habitable planets around this star is the subject of active discussion, finding progress about it requires a much better observation process," they concluded.
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