The correct option is
A 2 ParsecOne light year
= speed of light
× one year
or 1ly=3×108×(24×3600)=94608×1011m
So, 4.29ly=4.29×(94608×1011)=4.058×1016m
As 1 parsec =3.08×1016m
(Parsec is a unit of length used to measure large distances to objects outside our Solar System)
Thus, 4.29ly=4.058×10163.08×1016=1.32 parsec
Now angular displacement , θ=dD
where d= diameter of earth's orbit =3×1011m and
D= distance of star from the earth =4.058×1016m
So, θ=3×10114.058×1016=7.39×10−6 rad
As 1sec=4.85×10−6rad so, 7.39×10−6rad=7.39×10−64.85×10−6=1.52sec