Final answer:
Using Kepler's third law, we can determine the mass of the Sun based on the period and radius of Mercury's orbit to be approximately 1.98×10^30 kg.
Step-by-step explanation:
Using Kepler's third law, we can determine the mass of the Sun based on the period and radius of Mercury's orbit. The formula to calculate the mass of the Sun is:
MSun = 4π²R³ / G * T²
Where:
- R is the average radius of Mercury's orbit
- T is the period of Mercury's orbit
- G is the gravitational constant
Plugging in the values given, the mass of the Sun is approximately 1.98×10^30 kg.