Final answer:
To find the radius of the planet's orbit around the star, you can use Newton's version of Kepler's third law. The radius of the planet's orbit is approximately 1.60 times the radius of the Earth's orbit.
Step-by-step explanation:
To find the radius of the planet's orbit around the star, we can use Newton's version of Kepler's third law:
T2/R3 = 4π2/GM
Where T is the period of the planet (55 years), R is the radius of the orbit, G is the gravitational constant, and M is the mass of the star (2.1 times the mass of the Sun).
Rearranging the equation, we have:
R = (T2/GM)1/3
Plugging in the values, we get:
R = (552/[6.67 × 10-11 × 2.1 × 1.99 × 1030])1/3
R ≈ 2.38 × 1011 meters
Since the radius of the Earth's orbit is about 1.49 × 1011 meters, the radius of the planet's orbit is approximately 1.60 times the radius of the Earth's orbit.