“One of the planets we discovered, the TOI-6223b, is the size of Neptune but very close to its own star, which is why it’s called a hot Neptune,” he said. “While it has a radius similar to that of Neptune’s, we need to look at what gases are present in its atmosphere.”
“Meanwhile, the other one, the TOI-1743b, is a super-Earth — it is about 70 percent larger than our planet and it is terrestrial,” he noted. “It probably can’t retain volatile gases in its atmosphere — it is also very close to its star and therefore hot.”
Yalcinkaya said the TOI-5799 system stands out as one of the stars hosting two of the newly discovered exoplanets, TOI-5799b and TOI-5799c, both about 70 percent larger than Earth and likely terrestrial.
While TOI-5799b orbits close to its star and is therefore hot, TOI-5799c lies within the star’s habitable zone and completes an orbit every 14 days.
“The exoplanet is at a distance where water could potentially exist as liquid due to its surface temperature of around 63 degrees Celsius, but the atmosphere could change things a bit as we don’t know what kind of atmosphere it has,” he said. “It could be much hotter than expected or colder, we don’t know yet.”
“If there’s life there, there may be some bio-signs in its atmosphere, we can observe this in the future to see if there’s life there or not,” he noted. “Life may exist on many planets, but if there’s life in the ‘TOI-5799c,’ it is possible to find out.”
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