Kepler's Third law in Newton's form helps us here. It states that for an object (a star in our case) orbiting another much more massive object (the galactic center)
where is the orbital period,
is the radius of orbit,
is the mass of a central object and
is the gravitational constant.
It is easy to find from this equation,
We know the speed
it is obvious that
so
and the final formula is
To find the numeric answer we have to convert the given radius from light-days into meters. It is and the answer is
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