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From SciTechDaily:
Space telescopes such as CoRoT, Kepler, and TESS
have allowed scientists the discovery of about 4000 extrasolar planets
(planets around distant stars) within the past 14 years. Most of these
planets are the size of the gas giant planet Neptune,
about four times the size of the Earth, and in relatively close orbits
around their respective host stars. But scientists have also discovered
some exoplanets as small as the Earth that could potentially be rocky.
And a handful of these small planets are also at the right distance to
their host star to potentially have moderate surface temperatures for
the presence of liquid surface water – the essential ingredient for life
on Earth.
“The full picture of habitability, however, involves a look at the
qualities of the star too,” explains MPS scientist and lead author of
the new study Dr. René Heller. So far, almost all exoplanets less than
twice the size of Earth that have a potential for clement surface
temperatures are in orbit around a red dwarf.
Red dwarf stars are known for their extremely long lifetimes. Life on
an exoplanet in orbit around an old red dwarf star could potentially
have had twice as much time than life on Earth to form and evolve. But
the radiation from a red dwarf star is mostly infrared rather than
visible light as we know it. Many red dwarfs are also notorious for
emitting high-energy flares and for frying their planets, which would
later become habitable, with enhanced stellar luminosities as long as
these stars are young. Moreover, their faintness requires any habitable
planet to be so close to the star that the stellar gravity starts to
deform the planet substantially. The resulting tidal heating in the
planet could trigger fatal global volcanism. All things combined, the
habitability of planets around red dwarf stars is heavily debated in the
scientific community. (Read more.)
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