A Hohmann transfer is the most fuelβefficient twoβimpulse maneuver to move a spacecraft between two coplanar circular orbits. It works by first raising (or lowering) the spacecraft onto an elliptical transfer orbit that tangentially touches the original orbit at periapsis and the target orbit at apoapsis.
The semiβmajor axis of the transfer ellipse is simply the average of the radii of the two circular orbits, (a = frac{r_1 + r_2}{2}). Because the spacecraft travels half an orbit on this ellipse, the transfer time depends on the orbital period of the ellipse, which is governed by Keplerβs third law.
Using the standard gravitational parameter (mu = GM) of the central body, the transfer time can be expressed analytically. This allows quick estimation of mission duration without numerical integration.
What is a Hohmann transfer?
How do I calculate the semi-major axis for the transfer orbit?
What are the two impulses in a Hohmann transfer?
Why is a Hohmann transfer considered fuel-efficient?
Can this calculator be used for any type of orbits?
What is the significance of periapsis and apoapsis in a Hohmann transfer?
How does the time for a Hohmann transfer depend on the orbits' radii?
Results are for informational purposes only and do not constitute professional advice.
