Final answer:
The mass of the planet is approximately 1.41×10²⁴ kg.
Step-by-step explanation:
To find the planet's mass, you can use Kepler's third law of planetary motion, which relates the orbital period T, the semi-major axis a (which is the radius in a circular orbit), and the mass of the central body
M (the planet in this case).
The formula is given by:
T2 = 4π2/GM . a3
where:
T is the orbital period,
G is the gravitational constant (
G≈6.674×10−11m3kg−1s−2),
M is the mass of the central body (the planet),
a is the semi-major axis (radius in a circular orbit).
First, convert the orbital period from hours to seconds:
T=14hours×3600s/hour
Now, plug in the known values and solve for M:
(14×3600)2 = 4π2/6.674×10−11 ×(7.1×106)3×M
After calculating, you should be able to find the mass M of the planet.