The discovery could imply a modification in the estimations of the number of planets potentially harbouring life in the Galaxy and in the future selection of targets for the search of life elsewhere.
Researchers led by Paul A Mason from the University of Texas at El Paso said binary stars attract each other to their centre of gravity but also deform mutually due to the action of the so called tidal forces.
Researchers said it is well known that tidal forces could also break the rotation of the bodies implied. The best documented case is that of our Moon that has reduced its rotation rate due to tidal forces from Earth, to the point that it spins as slowly as it revolves around the Earth.
If the stars in a binary system are synchronised from the very beginning and at the same period of translation in their orbits, activity of young stars in those systems could be substantially reduced.
In other words, very young stellar components of tidally synchronised binaries could looks like grown up quiet stars, at least in terms of rotation and hence magnetic activity, an effect called by the researchers as "rotational ageing".
Researchers applied these ideas to evaluate the case of all the binary systems with known planets discovered by Kepler Telescope.
They found that at least 3 systems, Kepler 34, Kepler 47 and Kepler 64, could be very hospitable to planets because one or both the components are tidally synchronised and hence its activity has been reduced below the level of single stars of the same age.
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