Rocket Equation:
From: | To: |
The Rocket Equation, also known as Tsiolkovsky's equation, calculates the maximum change in velocity (delta-v) of a rocket based on its effective exhaust velocity and the ratio of initial to final mass. It is fundamental to rocket propulsion and space mission planning.
The calculator uses the rocket equation:
Where:
Explanation: The equation shows that the velocity change a rocket can achieve depends on the exhaust velocity and the natural logarithm of the mass ratio.
Details: Delta-v is crucial for mission planning in astronautics. It determines what maneuvers a spacecraft can perform, including orbit insertion, orbital transfers, and interplanetary trajectories.
Tips: Enter effective exhaust velocity in m/s, initial and final mass in kg. All values must be valid (positive numbers, initial mass > final mass).
Q1: What is effective exhaust velocity?
A: Effective exhaust velocity is the speed at which propellant is ejected from the rocket. It's related to specific impulse by Ve = Isp × g0.
Q2: Why is the natural logarithm used?
A: The natural logarithm accounts for the exponential nature of mass reduction as propellant is consumed.
Q3: What are typical delta-v requirements?
A: LEO insertion: ~9.4 km/s, GEO insertion: ~4.2 km/s, Lunar transfer: ~3.1 km/s, Mars transfer: ~3.6-4.3 km/s.
Q4: How does staging affect delta-v?
A: Staging increases total delta-v by discarding empty mass (tanks, engines) during flight, improving mass ratio.
Q5: What are limitations of this equation?
A: Assumes constant exhaust velocity, no external forces (gravity, drag), and instantaneous mass ejection.