Basic Hohmann Transfer

Calculation of a Hohmann transfer is straightforward.

In a circular orbit, the centrifugal force is equal to the gravitational force, and the velocity can be obtained from the relation

\begin{equation}
\frac{v^{2}}{r} = \frac{G M}{r^{2}} \quad \text{or} \quad v = \sqrt{\frac{G M}{r}}
\end{equation}

where,

  • r is the radius of the orbit from the center of the primary
  • v is the velocity of the object in orbit
  • G is the gravitational constant
  • M is the mass of the primary

In an elliptical orbit, motion is governed by the equation

\begin{equation} 
r(\theta) = \frac{h^{2}}{G M  (1 + e   \cos(\theta))}
\end{equation}

where,

  • \theta is the angle of the orbiting object from periapsis (true anomaly)
  • e is the eccentricity, (r_{2}-r_{1})/(r_{2}+r_{1})
  • h is the specific angular momentum

At periapsis, the angle is zero, and the velocity, with no radial component, can be determined by

\begin{equation}
v_{ellipse@A}= \sqrt{\frac{G  M  (1 + e)}{r_{1}}}
\end{equation}

At apoapsis, since the angular momentum of an orbit around a central force is a constant, the velocity can be determined by

\begin{equation}
v_{ellipse@B}= r_{1}  \frac{v_{ellipse@A}}{r_{2}}
\end{equation}

The impulsive thrusts are then calculated as follows:

  • \Delta v_{1} = v_{ellipse@A} - v_{1}
  • \Delta v_{2} = v_{2} - v_{ellipse@B}
  • \Delta v_{Total} = \Delta v_{1} + \Delta v_{2}
Typical Hohmann Transfer between circular orbits

It is assumed – and currently taught – that Hohmann transfers apply only to circular orbits (or coaxial elliptical orbits). This is simply not true. Please see General Hohmann Transfer for transfers between non-coaxial elliptical orbits.

Feeling adventurous? It is assumed – and currently taught – that degenerate electrons support the mass in a white dwarf. This also is not true. Please see Degenerate Electrons for a description of how they really behave. Then read Supernovas to see how easy they are to explain as a consequence.

This misunderstanding has been going on for almost 100 years…