Hohmann Transfer Orbit Calculator

Calculate the delta-v for the most fuel-efficient transfer between two circular orbits.

Last reviewed: April 2026
km
LEO ~6,771 km (400 km altitude)
km
GEO ~42,164 km
km³/s²
Total Δv
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Perigee Burn Δv1
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Apogee Burn Δv2
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Transfer Time
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Orbit Ratio (r2/r1)
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Important Disclaimer: The information provided by this Hohmann Transfer Calculator is for educational purposes only and shouldn't be used as a substitute for professional advice. Always consult with a licensed aerospace engineer or other qualified professionals for accurate guidance on space missions and spacecraft navigation.

About the Hohmann Transfer Orbit Calculator

The Hohmann transfer is a critical concept in space navigation, particularly for missions between two celestial bodies in the same orbit. This maneuver involves transferring from one orbit to another using the least amount of propellant, making it an essential technique for spacecraft missions. The Hohmann transfer consists of two burns: a prograde burn to escape the original orbit and a retrograde burn to enter the target orbit. This method minimizes the energy required for the transfer, making it an optimal choice for many space missions.

Real-World Applications

The Hohmann transfer has numerous practical applications in space exploration and satellite operations. For example, it's commonly used to transfer satellites between geostationary orbits (GEO) and lower Earth orbits (LEO). This maneuver is also essential for missions to the International Space Station (ISS), where spacecraft frequently need to transfer between different orbits to accommodate crew rotation and scientific experiments.

In addition to satellite operations, the Hohmann transfer is used in various space missions, including planetary exploration. NASA's Mars rovers, such as Curiosity and Perseverance, use the Hohmann transfer to navigate between the Earth and Mars. The mission involves a series of carefully planned burns to escape Earth's orbit and enter Mars' orbit, minimizing the energy required for the journey.

Common Mistakes

One common mistake in using the Hohmann transfer is not accounting for the gravitational forces of nearby celestial bodies. Space isn't empty, and the gravitational influence of planets, moons, and other objects can significantly affect the spacecraft's trajectory. Neglecting these forces can lead to significant errors in the transfer, potentially resulting in mission failure.

Another mistake isn't considering the spacecraft's velocity and orientation during the transfer. A spacecraft must be in the correct orientation and at the correct velocity to perform the Hohmann transfer successfully. Failure to achieve the correct velocity can result in the spacecraft missing the target orbit, while an incorrect orientation can cause the spacecraft to overshoot or undershoot the target orbit.

Examples

Example 1: A satellite needs to transfer from a LEO orbit to a GEO orbit. The satellite's current velocity is 7.8 km/s, and the target velocity is 3.1 km/s. The Hohmann transfer requires a prograde burn of 0.3 km/s to escape the LEO orbit and a retrograde burn of 0.2 km/s to enter the GEO orbit. The total energy required for the transfer is 0.5 km/s, making it an efficient and optimal choice for the mission.

Example 2: A spacecraft needs to transfer from the Earth to Mars. The spacecraft's current velocity is 11.2 km/s, and the target velocity is 2.2 km/s. The Hohmann transfer requires a prograde burn of 1.5 km/s to escape Earth's orbit and a retrograde burn of 1.0 km/s to enter Mars' orbit. The total energy required for the transfer is 2.5 km/s, making it an efficient and optimal choice for the mission.

Example 3: A rover needs to transfer from the Earth to Mars. The rover's current velocity is 11.2 km/s, and the target velocity is 2.2 km/s. The Hohmann transfer requires a prograde burn of 1.5 km/s to escape Earth's orbit and a retrograde burn of 1.0 km/s to enter Mars' orbit. The total energy required for the transfer is 2.5 km/s, making it an efficient and optimal choice for the mission.

What Happens If

What Happens If I Neglect the Gravitational Forces of Nearby Celestial Bodies? Neglecting the gravitational forces of nearby celestial bodies can result in significant errors in the spacecraft's trajectory. This can cause the spacecraft to miss the target orbit, overshoot or undershoot the target orbit, or even collide with a nearby object. For example, if a spacecraft isn't accounted for the gravitational influence of the Moon during a transfer from Earth to Mars, the spacecraft may not enter the correct orbit and could potentially collide with the Moon.

What Happens If I Don't Consider the Spacecraft's Velocity and Orientation During the Transfer? Not considering the spacecraft's velocity and orientation during the transfer can also result in significant errors in the spacecraft's trajectory. This can cause the spacecraft to miss the target orbit, overshoot or undershoot the target orbit, or even collide with a nearby object. For example, if a spacecraft isn't oriented correctly during a transfer from Earth to Mars, it may not enter the correct orbit and could potentially collide with a nearby object.

Frequently Asked Questions

The Hohmann transfer is a maneuver used in space navigation to transfer a spacecraft from one orbit to another using the least amount of propellant. This maneuver consists of two burns: a prograde burn to escape the original orbit and a retrograde burn to enter the target orbit.
To calculate the Hohmann transfer, you need to know the spacecraft's current velocity, the target velocity, and the gravitational forces of nearby celestial bodies. You can then use a Hohmann transfer calculator to calculate the required burns and the total energy required for the transfer.
A Hohmann transfer is a specific type of elliptical transfer. An elliptical transfer is a maneuver used in space navigation to transfer a spacecraft from one orbit to another using a transfer orbit that is an ellipse. A Hohmann transfer is a special case of an elliptical transfer where the transfer orbit is a perfect ellipse with the spacecraft starting and ending at the same altitude.