Delta V Calculator

Calculate a rocket's delta-v (velocity change) from its initial mass, final mass, and specific impulse using the Tsiolkovsky rocket equation, Δv = Isp·g0·ln(m0/mf).

Quick Facts

Rocket equation
Δv = Isp × g0 × ln(m0/mf)
The Tsiolkovsky rocket equation — total velocity change from expelling propellant.
Standard gravity
g0 = 9.80665 m/s²
Converts Isp (seconds) into exhaust velocity; always Earth-standard, even for missions elsewhere.
Exhaust velocity
ve = Isp × g0
The effective speed propellant leaves the engine relative to the rocket.
Typical Isp
Chemical: 250-450 s · Ion: 1,500-3,500 s
Higher Isp means more delta-v per kilogram of propellant burned.

Your Results

Calculated
Delta-v (Δv)
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Δv = Isp × g0 × ln(m0/mf)
Delta-v (km/s)
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Same result converted to km/s
Effective Exhaust Velocity
-
ve = Isp × g0
Mass Ratio (m0 / mf)
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Initial mass divided by final mass

Ready

Enter the initial mass, final mass, and specific impulse, then press Calculate.

Formula and Method for Rocket Delta-V

Delta-v (Δv) is the total change in velocity a rocket can produce by burning its propellant, and it is the fundamental "currency" of spaceflight. Every maneuver — launch, orbit raise, interplanetary transfer, landing — has a delta-v cost, and every vehicle has a delta-v budget set only by its propellant load and engine efficiency, not by thrust level or how long the burn takes. This calculator applies the Tsiolkovsky rocket equation, Δv = Isp·g0·ln(m0/mf), to compute the delta-v available from a given initial mass, final mass, and specific impulse.

How the calculation works

A rocket accelerates by ejecting mass (propellant) at high speed in the opposite direction. Applying conservation of momentum to a vehicle that continuously loses mass at a constant relative exhaust velocity ve, and integrating from the initial mass m0 down to the final mass mf, gives Δv = ve × ln(m0/mf). Specific impulse (Isp) restates exhaust velocity in seconds — a unit rocket engineers prefer because it is easy to compare across engines — via ve = Isp × g0, where g0 = 9.80665 m/s² is standard gravity. Substituting gives the full rocket equation: Δv = Isp × g0 × ln(m0/mf). Enter the initial (wet) mass, the final (dry) mass left after the burn, and the engine's Isp, and the calculator returns the achievable delta-v, the effective exhaust velocity, and the mass ratio.

Common mistakes

  • Confusing Isp with exhaust velocity: Isp is measured in seconds, not m/s — you must multiply by g0 = 9.80665 m/s² to get the actual exhaust speed used inside the equation.
  • Underestimating dry mass: the final mass mf must include everything that does not get expelled — structure, tanks, avionics, engines, payload, and any unburned reserve propellant — not just an "empty tank" figure.
  • Applying a single-stage equation to a multi-stage rocket: each stage has its own m0, mf, and Isp; total mission delta-v is the sum of each stage's delta-v, because a dropped, empty stage is not propellant and should not appear in a later stage's mass ratio.
  • Ignoring gravity and drag losses: the rocket equation gives the ideal, vacuum delta-v from propellant alone; a real ascent through an atmosphere and against gravity needs extra delta-v beyond the orbital velocity itself.

Typical delta-v budgets

Mission planners compare the delta-v this calculator produces against commonly cited budgets: reaching low Earth orbit (LEO) from the ground takes roughly 9,300-10,000 m/s once gravity and atmospheric drag losses are included, even though the orbital speed itself is about 7,800 m/s. From LEO, raising to geostationary transfer orbit (GTO) costs about 2,400 m/s, escaping Earth's gravity entirely (C3 = 0) costs roughly 3,200 m/s, and a trans-Mars injection burn costs roughly 3,600-3,900 m/s. Comparing a vehicle's computed delta-v against the budget for a target mission is the standard first check in any rocket or spacecraft design.

Frequently Asked Questions

What is delta-v in rocketry?
Delta-v (Δv) is the total change in velocity a rocket can produce by burning its propellant. It is the standard "currency" of spaceflight — every maneuver (launch, orbit raise, transfer, landing) costs a certain amount of delta-v, and every vehicle has a delta-v budget set by its propellant load and engine efficiency, independent of thrust level or burn duration.
What is the Tsiolkovsky rocket equation?
It is Δv = Isp·g0·ln(m0/mf), where m0 is the initial (wet) mass, mf is the final (dry) mass after the burn, Isp is the engine's specific impulse in seconds, and g0 = 9.80665 m/s² is standard gravity. It comes from integrating conservation of momentum for a vehicle that continuously ejects mass at a constant relative exhaust velocity.
How does specific impulse affect delta-v?
Specific impulse sets the effective exhaust velocity: ve = Isp × g0. A higher Isp means propellant leaves the engine faster, so the same mass ratio yields more delta-v. That is why ion thrusters (Isp of roughly 1,500-3,500 s) deliver far more delta-v per kilogram of propellant than chemical rockets (Isp of roughly 250-450 s), even though their thrust is much lower.
Why doesn't it matter which mass unit I use?
Only the ratio m0/mf appears in the equation, so any consistent mass unit — kilograms, pounds, metric tons — cancels out and gives the same delta-v. Just make sure both the initial and final mass are entered in the same unit.