Rockets & Spaceflight

Rocket Delta V Calculator

Calculate an ideal burn from vehicle masses, a known mass ratio or effective exhaust velocity. Inspect the propellant balance and see what the rocket equation includes.

Astronomy & Space · model workbench

Estimate the ideal velocity increment of one burn and reconcile the vehicle's initial mass, remaining mass and expelled propellant.

Private calculations in your browser · explicit inputs and model boundaries
Example preview · Measured massesWhere the initial vehicle mass goes
Expelled propellant6,000 kg
Remaining vehicle4,000 kg

The two segments sum to initial vehicle mass. Their sizes update with your scenario; this is a mass balance, not a vehicle drawing.

  1. 1EnterProvide the known values
  2. 2CalculateResults update automatically
  3. 3VerifyReview the details and units
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Enter values in s.

Enter values in kg.

Enter values in kg.

Calculation result

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Understand the relationship

The reasoning behind the result

Why the mass ratio sits inside a logarithm

d(Δv) = −vₑ dm/m; Δv = vₑ ln(m₀/mf)

During a burn, propellant leaving the vehicle carries momentum away. A small expelled mass produces a velocity increment proportional to its fraction of the vehicle's current mass. That fraction changes as the vehicle becomes lighter, so multiplying one fixed acceleration by a time would miss the mass change.

Integrating the fractional mass change from initial mass m₀ to final mass mf produces the natural logarithm. Both masses must use the same unit: their quotient R = m₀/mf is dimensionless. Doubling both masses leaves ideal delta-v unchanged, although it doubles the propellant consumed.

Four quantities, four different meanings

vₑ = Isp × g₀; R = m₀/mf; mp = m₀ − mf; fp = 1 − 1/R

Isp is specific impulse in seconds; vₑ is effective exhaust velocity in metres per second. R describes the ratio of the whole vehicle's initial and final masses. Propellant mass mp is an absolute amount, while propellant fraction fp is a share of initial vehicle mass.

The result label always identifies the selected quantity. A velocity, a mass and a dimensionless ratio are not interchangeable outputs even when they are calculated from the same burn scenario.

Solving backward from a required delta-v

R = exp(Δv/vₑ); mp = mf × expm1(Δv/vₑ)

When the final mass is known, first determine the ratio needed for the entered velocity budget. Multiplying that ratio by final mass gives initial mass. Subtracting final mass gives expelled propellant. The implementation uses expm1 for the subtraction so very small budgets retain numerical precision.

When initial mass is fixed instead, final mass is m₀ exp(−Δv/vₑ), and the available mass left after the burn becomes a useful companion result. This answers a different starting-data question from fixing the delivered final mass.

Read the trade-off before adding propellant

With final mass and exhaust velocity held fixed, each additional unit of delta-v requires exponentially more initial mass. With a mass ratio held fixed, delta-v is proportional to effective exhaust velocity. These are mathematical sensitivities within the model; they do not account for changes in engine mass, tank mass or achievable performance.

The live mass balance shows what is expelled and what remains. It is drawn from the current valid inputs, while the supporting rows expose the mass ratio and exhaust velocity needed to check the calculation independently.

Follow the numbers

A burn from 10,000 kg to 4,000 kg

  1. With Isp = 320 s, effective exhaust velocity is 320 × 9.80665 = 3,138.128 m/s.
  2. The mass ratio is 10,000 / 4,000 = 2.5. Its natural logarithm is approximately 0.916290732.
  3. Ideal delta-v is 3,138.128 × ln(2.5) = 2,875.437602 m/s. Expelled propellant is 10,000 − 4,000 = 6,000 kg.

The burn supplies about 2.875 km/s of ideal velocity increment. The 6,000 kg propellant amount is a separate mass result.

Quick guide

How to use this calculator

  1. Choose whether you know vehicle masses, a mass ratio or effective exhaust velocity.
  2. Enter masses for the whole vehicle immediately before and after this burn.
  3. Read ideal delta-v, then reconcile expelled propellant and remaining vehicle mass.

Calculation method

Calculation and interpretation

Estimate the ideal velocity increment of one burn and reconcile the vehicle's initial mass, remaining mass and expelled propellant.

Δv = Isp g₀ ln(m₀/mf) = vₑ ln(R)

Worked example

A burn from 10,000 kg to 4,000 kg

The burn supplies about 2.875 km/s of ideal velocity increment. The 6,000 kg propellant amount is a separate mass result.

Δv = Isp g₀ ln(m₀/mf) = vₑ ln(R)

Supported inputs

Precision and limits

Ideal velocity budget

These are ideal, constant-effective-exhaust-velocity burns. Gravity loss, aerodynamic drag, steering loss, finite-burn orbital effects and engine transients are excluded. Delta-v is not an attained ground speed or a launch capability.

Mass definitions

Initial and final mass refer to the entire vehicle accelerated during one burn. Final mass includes structure, payload and any propellant that remains unburned. Expelled propellant is the difference between those masses.

Specific impulse convention

Specific impulse is entered in seconds. Its conversion to effective exhaust velocity uses standard gravity, 9.80665 m/s², even for a burn far from Earth. This constant is a unit convention, not a gravity-loss allowance.

Numerical and practical limits

A mass ratio must be at least one; final mass and exhaust velocity must be positive. A zero-propellant case has zero ideal delta-v. Extremely large required mass ratios may be numerically representable but physically impractical.

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