|
Computing
Delta-vee required |
Equation Explained
BurnoutVelocity = Final Velocity (Delta-vee) required by the missile to achieve it's range in km/sec.
GRad: Solved independently below to simplify equation.
RangeAngle: Solved independently below to simplify equation.
GRad: = (GravityParameter / BurnoutRadius)
GravityParameter: Gravitational Parameter
of planet in km3/s2.
BurnoutRadius:
See Equation Below
|
Gravitational Parameters of |
|
|
Earth |
398,600.4418 |
|
Moon |
4,902.7779 |
|
Mars |
42,828 |
|
Titan |
8,978.2 |
|
Pluto |
871 |
|
Ceres Asteroid |
63.1 |
RangeAngle: = (RangeSurface / PlanetRadius)
RangeSurface: Missile range in
kilometers.
PlanetRadius = Radius of
planet in kilometers.
BurnoutRadius: = (PlanetRadius + BurnoutAltitude)
PlanetRadius = Radius of planet in
kilometers.
BurnoutAltitude = Burnout
altitude of missile in kilometers.
|
EXAMPLE: We want to calculate the ∆v required for a 7,000 km ICBM. The first step is to begin calculating the sub-variables, using a burn-out altitude of 330 kilometers. For BurnoutRadius, since we know Earth's radius is 6,378 km; BurnoutRadius solves for: BurnoutRadius: = (6378 + 330) = 6,708 For Grad, since we know Earth's Gravitational Parameter is 398,600, and because we solved for BurnoutRadius earlier; Grad solves for: GRad: = (398,600 / 6,708) = 59.42 For RangeAngle, since we know Earth's radius is 6,378 km, RangeAngle solves for RangeAngle: = (7,000 / 6,378) = 1.097 Now that we have solved the sub-variables; we can solve the main equation: Thus, our hypothetical 7,000 km ICBM would require a ∆v of 6.05 km/sec². However, it is a good rule of thumb to add an extra 0.5 km/sec² to your estimates to take into account air drag during the in-atmosphere phase, and to provide a margin for under-performing components. |
Bibliography:
Space
Vehicle Design by
Griffin, referencing Fundamentals
of Astrodynamics by
Bate, Mueller and White