Tsiolkovsky Rocket Equation Calculator
Calculation Result
Δv = 0 m/s
(Equivalent to 0 km/s)
Understanding the Rocket Equation
The Tsiolkovsky Rocket Equation is the fundamental principle behind spaceflight and orbital mechanics. Developed by Konstantin Tsiolkovsky in 1903, it describes the maximum change in velocity (Delta-v) a vehicle can achieve based on its exhaust velocity and the ratio of its initial and final mass.
The Mathematical Formula
Δv = ve * ln(m0 / mf)
Where:
- Δv (Delta-v): The total change in velocity. This is the "budget" used to reach orbit or travel between planets.
- ve (Exhaust Velocity): How fast gas leaves the nozzle. Calculated as Isp × g0 (where g0 ≈ 9.80665 m/s²).
- m0 (Initial Mass): Total mass, including propellant.
- mf (Final Mass): Mass after the propellant has been burned (structure, engines, payload).
- ln: The natural logarithm.
Why Delta-v Matters
Delta-v is the most critical metric in mission planning. Unlike cars that measure travel in distance (kilometers or miles), spacecraft measure travel in Δv. For example, to reach Low Earth Orbit (LEO), a rocket needs approximately 9,400 m/s of Δv. Because of the logarithmic nature of the equation, increasing your Δv requires an exponential increase in fuel, which is often referred to as "the tyranny of the rocket equation."
Practical Example
Suppose you have a small orbital stage with the following specs:
- Specific Impulse (Isp): 320 seconds
- Initial Mass (m0): 5,000 kg
- Final Mass (mf): 1,500 kg
Step 1: Calculate effective exhaust velocity: 320s × 9.80665 m/s² = 3,138.128 m/s.
Step 2: Calculate the mass ratio: 5,000 / 1,500 = 3.333.
Step 3: Apply the natural log: ln(3.333) ≈ 1.204.
Step 4: Final Δv: 3,138.128 × 1.204 = 3,778 m/s.