NSW · HSCModule 5
Orbital energy and orbit transfer calculator
Compute K, U and E for a satellite in two different orbits, and the energy required to move from one to the other.
Inputs
Result
Orbit 1
K
1.472e+10J
U
-2.944e+10J
E
-1.472e+10J
v
7673m/s
Orbit 2
K
2.361e+9J
U
-4.722e+9J
E
-2.361e+9J
v
3073m/s
Energy to move from r₁ to r₂
1.236e+10J
E = -GMm/(2r), K = +GMm/(2r), U = -GMm/r. Negative E means bound.
How this calculator works
For a circular orbit of radius r, K = GMm/(2r), U = -GMm/r, and E = -GMm/(2r). The calculator evaluates each at two radii r₁ and r₂ and reports the difference ΔE = E₂ - E₁, which is the work the rocket must do (positive if r₂ > r₁).
See the full derivation and worked example in our conservation of energy in orbital motion dot point answer.
Common questions
- What is the total mechanical energy of a circular orbit?
- E = -GMm/(2r). It is negative because the orbit is bound; zero corresponds to escape, and positive means unbound (hyperbolic trajectory).
- How do K and U relate in a circular orbit?
- K = +GMm/(2r), U = -GMm/r, so |U| = 2K and E = -K. This is the virial theorem for inverse-square gravity.
- Why does a higher orbit have more total energy but lower speed?
- Moving outward, kinetic energy decreases (the satellite slows) but potential energy increases (becomes less negative) by twice as much, so total energy increases. Counter-intuitively, you must speed the satellite up briefly to slow it down in the long run.
- How much energy is needed to escape from a circular orbit?
- The change from E = -GMm/(2r) to E = 0 is GMm/(2r). Equivalently, you need to multiply the orbital speed by √2 to reach escape velocity at that radius.