Answer:
Step-by-step explanation:
Given that,
Orbital time period, T = 3.75 earth years
Mass of star,
We need to find the radius of the exoplanet's orbit. It is a concept of Kepler's third law of motion i.e.
r is the radius of the exoplanet's orbit.
Solving for r we get :
We know that,
So,
So, the radius of the exoplanet's orbit is
.