Orbital inclination is the tilt of an orbitβs plane relative to a reference plane, usually the equatorial plane of the central body. Changing this tilt requires a maneuver that redirects the spacecraftβs velocity vector without altering its magnitude dramatically.
The most efficient way to change inclination is to perform the burn at the point in the orbit where the spacecraftβs speed is highest, typically at periapsis. The required deltaβv for a pure inclination change is given by the vector difference between the original and desired velocity directions.
Because the maneuver only rotates the velocity vector, the magnitude of the required deltaβv depends on the orbital speed and the sine of half the inclination change angle. This relationship is captured in the classic formula shown below.
What is orbital inclination?
When is the best time to perform an inclination change maneuver?
How does delta-v affect a spacecraft’s orbit?
What factors determine the required delta-v for an inclination change?
Can you explain the vector difference in calculating inclination change?
Why is it important to consider orbital speed during an inclination change?
How does changing inclination impact a spacecraft’s orbit period?
Results are for informational purposes only and do not constitute professional advice.
