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Hohmann Transfer Orbit Delta-V Calculator

The Hohmann transfer orbit is the most fuel-efficient two-impulse orbital maneuver for moving between two coplanar circular orbits.

Radius from central body center (e.g. 6,778 km for 400 km altitude LEO).

Radius from central body center (e.g. 42,164 km for GEO).

Standard gravitational parameter (398,600 km³/s² for Earth, 1.327×10¹¹ for Sun).

Calculated Result
3.854 km/s (3854 m/s)

Total Hohmann Transfer ΔV

First Burn (ΔV₁ at r₁)

2.398 km/s

Second Burn (ΔV₂ at r₂)

1.457 km/s

Transfer Time of Flight

5.29 hours

Initial Orbit Speed (v₁)

7.669 km/s

Final Orbit Speed (v₂)

3.075 km/s

Calculation Breakdown

  1. Transfer Ellipse Semi-Major Axisat = (r₁ + r₂) / 2 = (6778 + 42164) / 2 = 24471.0 km
  2. Impulsive Maneuver BurnsΔV₁ = |√(μ·(2/r₁ - 1/at)) - √(μ/r₁)| = 2.398 km/s, ΔV₂ = 1.457 km/s
  3. Total Velocity IncrementΔV_total = ΔV₁ + ΔV₂ = 3.854 km/s (TOF = 5.29 h)

What Is the Hohmann Transfer Orbit Delta-V Calculator?

A Hohmann transfer connects two circular orbits using an elliptical transfer orbit whose periapsis is at r1 and apoapsis is at r2.

The maneuver requires two impulsive burns: one to enter the transfer ellipse and a second to recircularize at destination.

How Does the Hohmann Transfer Orbit Delta-V Calculator Work?

Applying ΔV1 raises apoapsis to the target radius r2.

Half an orbital period later, the spacecraft arrives at apoapsis, where applying ΔV2 raises periapsis to circularize.

Hohmann Transfer Orbit Delta-V Calculator Formula & Variables

The core mathematical equation utilized by this calculator is expressed as:

\Delta V_1 = \sqrt{\frac{\mu}{r_1}} \left( \sqrt{\frac{2 r_2}{r_1 + r_2}} - 1 \right), \quad \Delta V_2 = \sqrt{\frac{\mu}{r_2}} \left( 1 - \sqrt{\frac{2 r_1}{r_1 + r_2}} \right), \quad TOF = \pi \sqrt{\frac{a_t^3}{\mu}}

Vis-viva orbital energy equation applied to periapsis and apoapsis impulse burns.

How to Use the Hohmann Transfer Orbit Delta-V Calculator

  1. Input initial and target orbital radii in km, and central body gravitational parameter μ.
  2. Review total ΔV in km/s and m/s, individual burn sizes, and transfer time of flight.

Step-by-Step Example Calculation

LEO to Geostationary Transfer (GTO)

Input Values:

initialOrbitRadiusKm:6678
finalOrbitRadiusKm:42164
gravitationalParameterMuKm3S2:398600
Worked Steps: Calculates ΔV1 = 2.45 km/s, ΔV2 = 1.48 km/s, Total ΔV = 3.93 km/s (TOF = 5.3 hours).

Understanding Your Result

Total ΔV dictates the required rocket propellant mass ratio according to Tsiolkovsky’s rocket equation.

Factors That Affect the Result

  • For radius ratios r2/r1 > 11.94, a three-impulse bi-elliptic transfer can theoretically require slightly less ΔV than a Hohmann transfer.

When Should You Use This Calculator?

  • Geostationary satellite launches, lunar transfer orbit sizing, and interplanetary interplanetary mission planning.

Assumptions & Limitations

  • Assumes two-body Keplerian mechanics with instantaneous impulsive velocity increments.

Frequently Asked Questions

Calculation Accuracy & Reference Note

Standard astrodynamics Vis-Viva orbital formulation.

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