Changing orbits with two burns
A satellite in a circular orbit cannot simply point toward a higher orbit and fly there. Raising an orbit means speeding up at one point so the opposite side of the orbit rises, then speeding up again when you get there. In 1925 the German engineer Walter Hohmann showed that, for two circular orbits in the same plane, the cheapest two-burn route is an ellipse that just touches both circles. It is still the starting point of mission planning.
The formulas
With μ the gravitational parameter of the central body (3.986 × 10¹⁴ m³/s² for the Earth) and r₁, r₂ the radii of the two orbits from the center of the body:
- Speed on a circular orbit: v = √(μ ÷ r).
- First burn: Δv₁ = v₁ × (√(2r₂ ÷ (r₁ + r₂)) − 1).
- Second burn: Δv₂ = v₂ × (1 − √(2r₁ ÷ (r₁ + r₂))).
- Transfer time, half of the ellipse: t = π × √(a³ ÷ μ), with a = (r₁ + r₂) ÷ 2.
The calculator adds the body’s radius to the altitudes you enter.
Worked example: low Earth orbit to geostationary
From a circular orbit at 400 km to the geostationary altitude of 35,786 km:
- Speed in the initial orbit: 7.669 km/s. Speed in the final orbit: 3.075 km/s.
- First burn: 2.397 km/s, at the low point of the transfer ellipse.
- Second burn: 1.456 km/s, at the high point, to circularize.
- Total delta-v: 3.854 km/s.
- Transfer time: 5.29 hours.
Notice that the spacecraft ends up moving more slowly in the higher orbit, even though both burns speed it up: it trades speed for height as it climbs.
Other Earth transfers
| From | To | Total Δv | Transfer time |
|---|---|---|---|
| 200 km | Geostationary, 35,786 km | 3.93 km/s | 5.3 h |
| 400 km | GPS altitude, 20,200 km | 3.42 km/s | 3.0 h |
| 400 km | 1,000 km | 0.32 km/s | 0.8 h |
| 400 km | Moon’s distance | 3.91 km/s | about 5 days |
What the model leaves out
- Plane changes: launches from Cape Canaveral start in an orbit inclined about 28.5° to the equator. Removing that inclination for a geostationary satellite adds about 0.36 km/s when it is combined with the second burn at the high point. Equatorial launch sites such as Kourou need less.
- Finite burns: real engines take minutes, not an instant.
- Other bodies’ gravity: for a trip to the Moon, its gravity changes the arrival, which is why lunar missions use patched conics or numerical models.
Bi-elliptic transfers
When the final orbit is more than about 11.9 times larger than the initial one, a three-burn bi-elliptic transfer, which goes beyond the target and then falls back, can use less delta-v than a Hohmann transfer, at the cost of a much longer trip.