Solution:To calculate the mean velocity of the Earth in its orbit around the Sun, we can use the basic formula for orbital velocity:V = (2pi*r)/T
where :
v is the orbital velocity.
r is the average distance from the Earth to the Sun . (approximately 1 astronomical unit or 1AU \approx 1.496 * 10 ^ 8 * km )
T is the orbital period of the Earth (1 year, which is approximately 365.25 * 24 * 3600 seconds). First, we find the circumference of the Earth's orbit (assuming a circular orbit for simplicity):
Circumference - 2pi*r \approx 2pi * 1.496 * 10 ^ 8 * km \approx 9.4 * 10 ^ 8 * km
Then, we convert the orbital period into seconds:
T \approx 365.25 * 24 * 3600 seconds = 3.156 × 107 seconds
Now, we calculate the velocity:
v = (2pi*r)/T \approx (2.4 * 10 ^ 8 * km)/(3.156 * 10 ^ 2 * s) \approx 29.8km / s
Rounding this value, we get approximately 30 km/s.