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
.