The Orbital Velocity of the Earth is approximately 29,784.7357 m/s m/s.
The Earth travels in a near circular orbit around the Sun. This means that the distance the Earth travels in one year is the circumference of a circle with a radius of one astronomical unit (au).
Velocity is computed as distance divide by time, in this case:
r = 1 astronomical unit
c = 2⋅π⋅r
v = c / (1 sidereal year)
convert v to meters per second
The formula to compute the Orbital Velocity of the Earth is:
v = ( 2⋅π⋅r) / sr
where: