Hohmann Transfer Calculator






Hohmann Transfer Calculator – Calculate Delta-V and Transfer Time


Hohmann Transfer Calculator

Precise Delta-V and Orbital Mechanics Calculation Tool


Select the planet or star being orbited.


Distance from the center of the central body (e.g., LEO ~6778 km).

Please enter a valid positive radius.


Distance from the center for the final orbit (e.g., GEO ~42164 km).

Please enter a valid positive radius.

Total Delta-V Required
0.000 km/s

Δv_total = |Δv₁| + |Δv₂|

First Burn (Δv₁):
0.000 km/s
Second Burn (Δv₂):
0.000 km/s
Transfer Time:
0.00 hours


Orbital Transfer Visualization

Central Body

Figure: Blue (Initial), Green (Target), Red (Hohmann Transfer Ellipse)


Parameter Value Unit

Understanding the Hohmann Transfer Calculator

The Hohmann transfer calculator is an essential tool for aerospace engineers, physics students, and space enthusiasts. It computes the most fuel-efficient way to move a spacecraft from one circular orbit to another in the same plane. This maneuver, named after Walter Hohmann, who published the concept in 1925, uses an elliptical transfer orbit that touches both the starting and ending circular orbits.

By using our Hohmann transfer calculator, you can instantly determine the impulse required (Delta-V) and the time it takes to travel between planets or satellites. Whether you are planning a mission from Low Earth Orbit (LEO) to Geostationary Orbit (GEO) or an interplanetary journey, understanding the orbital mechanics behind this calculation is crucial for mission success.

Hohmann Transfer Calculator Formula and Mathematical Explanation

The calculation of a Hohmann transfer involves several steps based on Kepler’s laws and Newton’s law of universal gravitation. The process requires two separate engine burns (impulsive maneuvers).

The Core Formulas

1. Semi-major axis of the transfer orbit (atrans):
atrans = (r₁ + r₂) / 2

2. Orbital Velocities (v):
Velocity in circular orbit: v = √(μ / r)

3. Delta-V for the first burn (Δv₁):
Δv₁ = √(μ / r₁) * (√(2r₂ / (r₁ + r₂)) - 1)

4. Delta-V for the second burn (Δv₂):
Δv₂ = √(μ / r₂) * (1 - √(2r₁ / (r₁ + r₂)))

Variable Meaning Unit Typical Range
r₁ Initial Orbit Radius km 6,500 – 50,000
r₂ Target Orbit Radius km 6,500 – 400,000
μ Gravitational Parameter m³/s² Body Dependent
Δv Change in Velocity km/s 0.5 – 15.0

Practical Examples (Real-World Use Cases)

Example 1: LEO to GEO

A satellite moves from a 300 km altitude circular orbit (r₁ ≈ 6,678 km) to a Geostationary orbit (r₂ ≈ 42,164 km). Inputting these values into the Hohmann transfer calculator shows that the first burn requires ~2.42 km/s and the second burn ~1.47 km/s, totaling a Delta-V of 3.89 km/s. The transfer time is approximately 5.27 hours.

Example 2: Earth to Mars (Sun-centric)

When traveling from Earth’s orbit (r₁ ≈ 1.496 × 10⁸ km) to Mars’ orbit (r₂ ≈ 2.279 × 10⁸ km) around the Sun, the Hohmann transfer calculator helps calculate the “Launch Window” Delta-V. The total transfer Δv is roughly 5.6 km/s relative to the Sun, with a travel time of about 259 days.

How to Use This Hohmann Transfer Calculator

  1. Select Central Body: Choose Earth, Mars, Sun, or enter a custom gravitational parameter (μ).
  2. Enter Initial Radius: Input the radius of your starting orbit in kilometers. Note: This is from the center of the body, not the surface altitude.
  3. Enter Target Radius: Input the radius of your final circular destination orbit.
  4. Review Results: The calculator updates in real-time to show the total Delta-V, individual burn requirements, and the time of flight.
  5. Analyze the Chart: Use the SVG visualization to see the scale of your transfer maneuver.

Key Factors That Affect Hohmann Transfer Calculator Results

  • Central Body Mass: The larger the μ (mass), the higher the velocities and Delta-V requirements.
  • Radius Ratio: The efficiency of a Hohmann transfer is highest when the ratio r₂/r₁ is less than ~11.9. For higher ratios, a bi-elliptic transfer might be more efficient.
  • Orbital Inclination: This Hohmann transfer calculator assumes orbits are in the same plane. Plane changes significantly increase fuel costs.
  • Atmospheric Drag: For very low orbits (under 200 km on Earth), drag can decay the orbit during the transfer.
  • Specific Impulse (Isp): While the calculator provides Delta-V, the actual fuel mass depends on your engine’s efficiency.
  • Time Constraints: Hohmann transfers are the most fuel-efficient but often the slowest. Missions requiring speed may use hyperbolic trajectories.

Frequently Asked Questions (FAQ)

1. Is the Hohmann transfer always the most efficient?
No, for very large radius ratios (r₂/r₁ > 11.94), a bi-elliptic transfer can theoretically save fuel, though it takes much longer.

2. Does this calculator account for altitude?
No, it uses radius (distance from the center). To get radius from altitude, add the planet’s radius (e.g., +6371 km for Earth).

3. Why do I need two burns?
The first burn changes the circular orbit into an elliptical one. The second burn circularizes the orbit at the new altitude.

4. Can I use this for landing on a planet?
This Hohmann transfer calculator is for orbit-to-orbit transfers. Landing involves atmospheric entry or powered descent logic.

5. What is “μ” (mu)?
It is the standard gravitational parameter (G * M), which simplifies orbital math by combining the constant of gravitation and the body’s mass.

6. Does the mass of the spacecraft matter?
For the Delta-V calculation, no. However, mass matters when calculating how much fuel is needed to achieve that Delta-V.

7. Can this calculate an Earth-to-Moon transfer?
Yes, by setting r₁ as Earth orbit and r₂ as the Moon’s orbital distance (~384,400 km).

8. What units are used in the results?
We provide Delta-V in km/s and transfer time in hours or days for clarity.

© 2023 Hohmann Transfer Calculator Tool. For educational and mission planning purposes.


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