How do I calculate orbital velocity?
Use the formula v = sqrt(ΞΌ / r), where ΞΌ is the standard gravitational parameter (GM) and r is the orbital radius, which is the sum of the celestial body’s mean radius and altitude.
What is the standard gravitational parameter?
The standard gravitational parameter (ΞΌ) is a product of the gravitational constant (G) and the mass (M) of the central body. It represents the strength of the gravitational field.
How does altitude affect orbital velocity?
Higher altitudes result in lower orbital velocities because the distance from the center of the celestial body increases, reducing the centripetal force needed to maintain orbit.
Can this calculator be used for any celestial body?
Yes, as long as you have the mean radius and gravitational parameter for the celestial body in question.
What is the difference between orbital velocity and escape velocity?
Orbital velocity is the speed needed to maintain a stable circular orbit. Escape velocity is the minimum speed required to completely leave the gravitational influence of a celestial body.
How do I convert altitude above sea level to orbital radius?
Add the altitude above sea level to the Earth’s mean radius (approximately 6,371 km) to get the orbital radius.
What units should I use for the calculations?
Use consistent units such as kilometers for distance and meters per second for velocity. Ensure that ΞΌ is in appropriate units matching these distances.