A panel of scientists has brought forward a new idea that small gas planets such as Neptune have the high probability of discovery somewhere in the future as well as the probability of being used as habitats. Published in Astrobiology, this research demonstrates the idea with computer models to foresee where gas planets may sustain life.
To make life possible in a planet such as Neptune, a range of conditions such as strong stellar activity and tidal forces can be met, as stated by researchers of University of Washington. These Neptune like gas plan roam around stars of low mass which are acknowledged as M dwarfs and are of much smaller size and dimness compared to the Sun. as a result habitable regions are nearer. The fact being the forces get frailer on Earth, this may have a remarkable effect on inhabiting conditions of a gas planet. Life on M dwarfs is hospital due stellar activity coming out of them as well as tidal forces pulling a star that exerts on its surrounding planets much similar to the force wielded by the moon on the Earth.
Rodrigo Luger, a PhD student of the University of Washington says that this is the reason why we have ocean tides working as tidal forces from both the Sun and the Moon has the ability to pull on the oceans generating a protuberance that we generally experience as the high tide. Fortunately, on Earth the water of the ocean in the only thing that gets disfigured just by a few feet, although the habitable regions of M dwarfs will experience much stronger versions of it.
These kinds of gas planets are mostly very far from the host stars leading the atmosphere to be very chilly but if they are tugged into the habitable zone of the stars when gas can be scattered with the help of exposing it to a higher gamma and ultraviolet radiation. Thus the planet will be free of gas and turn into a livable region.