Answer:
T = 7.61*10^6 s
Step-by-step explanation:
In order to calculate the Mercury's period. in its orbit around the sun, you take into account on the Kepler's law. You use the following formula:
(1)
T: period of Mercury
r: distance between Mercury and Sun
Ms: mass of the sun = 1.98*10^30 kg
G: Cavendish's constant = 6.674*10^-11 m^3 kg^-1 s^-2
You replace the values of all parameters in the equation (1):
![T=\sqrt{(4\pi^2(5.79*10^(10)m)^3)/((6.674*10^(-11)m^3kg^(-1)s^(-2))(1.98*10^(30)kg))}\\\\T=7.61*10^6s*(1h)/(3600s)*(1d)/(24h)=88.13\ days](https://img.qammunity.org/2021/formulas/physics/college/3dd8x75paq71k7q4ymwybxase86vaxtlg7.png)
The period of Mercury is 7.61*10^6 s, which is approximately 88.13 Earth's days