Propulsion sizing

Propulsion Sizing Calculator

How much propellant does the mission need? The Tsiolkovsky rocket equation turns a delta-v budget into propellant mass, wet mass, and tank volume.

How this model works & what it omits

Tsiolkovsky rocket equation. propellant mass from dry mass, exhaust velocity from Isp, first-order tank + burn-time sizing. cold-gas / monoprop / bipropellant / electric. engineering trade-study accuracy.

This calculator solves the Tsiolkovsky rocket equation - Δv = ve · ln(m_wet / m_dry) - turning a delta-v (Δv) budget into propellant mass, wet mass, mass ratio, tank volume, and burn time, with exhaust velocity from specific impulse (Isp): ve = Isp · g0. The propellant families span cold gas, hydrazine monopropellant, MMH/NTO bipropellant, and electric, with Isp and density values in the ranges of SMAD ch. 17 (Wertz et al., 2011) and Sutton's Rocket Propulsion Elements - which makes it equally at home as a CubeSat propulsion calculator or a smallsat deorbit-burn sizer.

Every orbital manoeuvre - station-keeping, plane change, deorbit, transfer - costs a velocity increment, the delta-v (Δv). Sizing a propulsion system means turning that Δv budget into a propellant mass and, from there, into tank volume and burn time. The governing relation is the Tsiolkovsky rocket equation: Δv = ve · ln(m_wet / m_dry), where ve is the exhaust velocity. Solved for propellant mass from the dry mass it becomes m_p = m_dry · (e^(Δv/ve) − 1).

Exhaust velocity follows from specific impulse: ve = Isp · g0, with standard gravity g0 = 9.80665 m/s². Because propellant mass grows exponentially with Δv/ve, a higher-Isp propellant collapses the propellant requirement dramatically - the central trade in propulsion selection. Cold gas (Isp ≈ 50-90 s) is simple but heavy; hydrazine monopropellant (≈ 200-235 s) and MMH/NTO bipropellant (≈ 300-340 s) are denser and more efficient; electric propulsion (≈ 1000-3000 s) is the most mass-efficient but delivers only milli-newtons of thrust, so burns last weeks.

Tank volume is sized from the stored propellant density and an ullage fraction - the gas headspace left for pressurant and thermal expansion. The internal tank volume is V = m_p / ρ / (1 − ullage). Cold gas is the only family stored as a gas, so its low density (~56 kg/m³ at high pressure) makes its tanks far bulkier than the dense liquids. Burn time at constant thrust is t = m_p · ve / F; for low-thrust electric systems the tool also suggests a count of discrete burns, each capped at one day of thrusting.

What this tool does not capture: gravity and steering losses, finite-burn losses for non-impulsive manoeuvres, residual and trapped propellant, pressurant mass, feed-system and tankage structural mass, blow-down pressure decay, and throttling. The result is a first-order trade-study sizing - detailed mission design needs a full propulsion feed-system model and an integrated mass budget.

pick a scenario, then dial delta-v / dry mass / Isp.

Mission

total delta-v the propulsion system must deliver.

Propulsion

propellant family sets density; Isp sets exhaust velocity.

Tank & burn

ullage = gas headspace; thrust sets burn time.

Propulsion sizing: propellant mass 52.2 kg, wet mass 252.2 kg, mass ratio 1.261×.

Propulsion sizing

Tsiolkovsky: m_p = m_dry (e^(Δv/ve) − 1)

52.2 kg

Propellant mass

252.2 kg

Wet mass

1.261×

Mass ratio

20.7%

Propellant fraction

2.16 km/s

Exhaust velocity

57.4 L

Tank volume

31.3 h

Total burn time

wet mass = dry + propellant

Dry 79%
Prop 21%
Dry 200.0 kgPropellant 52.2 kgWet 252.2 kg

Tsiolkovsky - propellant mass vs Δv

0.101.010.01001000100001.0e+51.010.0100100010000Δv (m/s)propellant (kg)
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Common questions

How do I calculate propellant mass from delta-v?

Solve the rocket equation for propellant from the dry mass: m_p = m_dry · (e^(Δv/ve) − 1). For the CubeSat cold-gas preset - a 6 kg spacecraft needing 50 m/s of reaction-control delta-v - that comes to about 0.45 kg of propellant, but roughly 9 litres of tank. Enter your own dry mass, delta-v, and propellant family and the tool solves the same chain through tank volume and burn time.

What specific impulse (Isp) should I assume?

By family: cold gas ≈ 50–90 s, hydrazine monopropellant ≈ 200–235 s, MMH/NTO bipropellant ≈ 300–340 s, electric propulsion ≈ 1000–3000 s. Higher Isp means exponentially less propellant for the same delta-v - the central trade in propulsion selection - but the families differ enormously in thrust, complexity, and power demand.

Why does propellant mass grow exponentially with delta-v?

Because every kilogram of propellant you carry for the end of a burn must itself be accelerated through the start of it - the compounding that puts Δv/ve in the rocket equation's exponent. It is also why high Isp pays so well: the electric station-keeping preset pushes a 450 kg spacecraft through 1500 m/s on about 40 kg of xenon (an 8% propellant fraction) where a chemical system would need several times more.

Why are cold-gas tanks so bulky?

Cold gas is the only family stored as a gas, at a storage density around 56 kg/m³ - versus roughly a tonne per cubic metre for the liquid propellants. Since tank volume is V = m_p / ρ / (1 − ullage), the same propellant mass costs an order of magnitude more volume - a real constraint inside a CubeSat structure, even when the propellant mass itself looks small.

What does burn time mean for electric propulsion?

At constant thrust, t = m_p · ve / F - and because electric thrusters deliver only milli-newtons, the total adds up to weeks or months of thrusting. The tool therefore also suggests a count of discrete burns, each capped at one day: the electric preset's 1500 m/s works out to roughly a hundred day-long burns.

References

  • Wertz, J. R., Everett, D. F., Puschell, J. J. (eds.) (2011). Space Mission Analysis and Design / Space Mission Engineering: The New SMAD, ch. 17 - Spacecraft Propulsion.
  • Sutton, G. P., Biblarz, O. (2017). Rocket Propulsion Elements, 9th ed. Wiley.
  • Goebel, D. M., Katz, I. (2008). Fundamentals of Electric Propulsion: Ion and Hall Thrusters. JPL / Wiley.
  • Tsiolkovsky, K. E. (1903). Exploration of Outer Space by Means of Rocket Devices.
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