Star HD 110067, 105 light-years from Earth, has six exoplanets that orbit synchronously.
A recent study suggests that the star's age is around 2.5 billion years - far younger than the initially estimated of 8 billion years
Astronomer Klaus-Peter Schröder and his colleagues used HD 110067's spin rate and activity levels to estimate its age.
The team analyzed wavelengths of ionized calcium to judge star activity levels which intrinsic of the star’s age.
With the new age estimation, astronomers will better understand how the surrounding exoplanets have evolved.
Current exoplanet detection methods favour planets with smaller orbits which revolve closer to HD 110067, close enough for conditions to be too hot for life to arise.
However, while temperature is a factor, younger stars spew lethal doses of X-rays and gamma rays. As such, HD 110067's newly refined age may limit the possibility of life on its unseen alien worlds.
HD 110067’s youthful age may also lead astronomers to search for exoplanets with increasing distances from the star within its habitable zone.
It is suggested that it may have taken as little as 1 billion years for some of the inner planets to begin rehearsing their careful dance through a phenomenon called tidal locking.
The research was published in the journal Astronomy & Astrophysics.