Lowβthrust spiral transfers are used when a spacecraftβs propulsion system cannot provide the impulsive Ξv required for a Hohmann transfer. Instead, a continuous, small acceleration slowly raises (or lowers) the orbit, tracing a spiral path in the orbital plane.
The time required for such a maneuver depends on the magnitude of the thrust acceleration, the gravitational parameter of the central body, and the initial and final orbital radii. Because the thrust is applied continuously, the orbital energy changes gradually, and the semiβmajor axis evolves according to a differential equation that can be integrated analytically for a constant thrust.
For a circular initial and final orbit the integrated solution yields a simple closedβform expression. This expression is useful for mission planning, allowing engineers to estimate how long a lowβthrust spiral will take without performing a full numerical propagation.
mu = gravitational parameter of the central body (kmΒ³/sΒ²)
a_{1} = initial orbital radius (km)
a_{2} = final orbital radius (km)
a_{t} = constant thrust acceleration (km/sΒ²)
What is a low-thrust spiral transfer?
How does the time for a low-thrust spiral transfer depend on?
When would you use a low-thrust spiral transfer instead of a Hohmann transfer?
What is the advantage of using a low-thrust spiral transfer?
How does the orbital eccentricity change during a low-thrust spiral transfer?
Can you explain the role of gravitational parameter in this calculation?
What factors might affect the accuracy of this low-thrust spiral time calculator?
Results are for informational purposes only and do not constitute professional advice.
