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ΔV · the physics of DeltaV THRUST

Delta-v and THRUST: the physics of rocket science

A rocket answers two questions. THRUST is how hard it pushes; delta-v is how far that push can take it. This page sets out the conventional physics, the equations every flight dynamics engineer uses, with the sources to read them in full, and then where each idea lives in DeltaV THRUST.

Δv=ve⁡ln⁡m0mf

I · Force

THRUST

A rocket carries its own reaction mass and throws it backwards. By Newton's third law and the conservation of momentum, the vehicle is pushed forward. The THRUST of a rocket nozzle is the momentum flux of the exhaust plus a pressure term at the nozzle exit:

F=ṁve+(pe−p0)Ae
ṁ
mass flow rate of propellant (kg/s)
ve
exhaust velocity at the nozzle exit (m/s)
pe,p0
exit pressure and ambient pressure (Pa)
Ae
nozzle exit area (m²)

To leave the pad, THRUST must exceed weight: the THRUST-to-weight ratio F/(mg0) must be above 1. Every second spent climbing slowly is lost to gravity drag.

Read: THRUST · NASA Glenn: rocket THRUST summary · NASA Glenn: Beginner's Guide to Rockets

II · Efficiency

Specific impulse

Specific impulse measures how much impulse an engine draws from each unit of propellant. Quoted in seconds, it is the effective exhaust velocity divided by standard gravity:

Isp=Fṁg0=veg0,g0=9.80665 m/s²

A kerosene first stage at sea level runs near 300 s; a hydrogen–oxygen upper stage in vacuum runs near 450 s, an exhaust velocity of about 4.41 km/s; ion engines exceed 3,000 s at tiny THRUST. High THRUST and high specific impulse rarely come in the same engine, which is why launch vehicles mix them.

Read: Specific impulse · Exhaust velocity · Standard gravity

III · Reach

The Tsiolkovsky rocket equation

In 1903 Konstantin Tsiolkovsky wrote down the law that governs every rocket. Conserve momentum over an instant in which the vehicle sheds mass dm at exhaust velocity ve:

mdv=−vedm

Integrate from the full mass m0 to the dry mass mf and the rocket equation follows:

Δv=ve⁡ln⁡m0mf=Ispg0⁡ln⁡m0mf

The logarithm is the hard truth of spaceflight. Delta-v grows only with the logarithm of the mass ratio, so doubling the propellant buys far less than double the reach. Turned around, the mass ratio a mission demands grows exponentially with its delta-v:

m0mf=eΔv/ve

Worked example. Low Earth orbit costs about 9.4 km/s once gravity and drag losses are counted. At 450 s (ve≈4.413 km/s) the mass ratio is e9.4/4.413≈8.4: about 88 % of the vehicle on the pad must be propellant.

Read: Tsiolkovsky rocket equation · Delta-v · Mass ratio · Propellant mass fraction

IV · Structure

Staging: reach is bought with structure

Tanks and engines are dead weight once their propellant is gone. A multistage rocket drops them, and each stage's mass ratio is taken on what remains. The delta-v of the stack is the sum over its stages:

Δvtotal=∑i=1nve,i⁡ln⁡m0,imf,i

A single stage whose tanks and engines cap its mass ratio near 8 reaches about 9.2 km/s at 450 s, just short of orbit. Two stages of mass ratio 4 each reach about 12.2 km/s, because the empty first stage never has to be carried to orbit. A bigger tank does not do that; dropping dead weight does.

Read: Multistage rocket · Robert H. Goddard · Hermann Oberth

V · Navigation

Orbits, escape velocity and the delta-v budget

Missions are planned as a delta-v budget: the sum of every burn. Orbital mechanics prices each one from the body's standard gravitational parameter μ=GM. The vis-viva equation gives the speed anywhere on an orbit of semi-major axis a:

v2=μ(2r−1a)

Two cases follow from it: the circular orbital speed (a=r) and the escape velocity (a→∞):

vcirc=μr,vesc=2μr=2vcirc

At 400 km above Earth a circular orbit runs at 7.67 km/s; escape from Earth's surface needs about 11.2 km/s. Moving between two circular orbits most economically, the Hohmann transfer takes two burns:

Δv1=μr1(2r2r1+r2−1),Δv2=μr2(1−2r1r1+r2)

Worked example. From a 300 km parking orbit to geostationary radius (42,164 km): Δv1≈2.43 km/s and Δv2≈1.47 km/s, 3.89 km/s in all before any plane change. Burns made deep in a gravity well are worth more (the Oberth effect), and a gravity assist borrows delta-v from a planet.

Read: Delta-v budget · Vis-viva equation · Hohmann transfer orbit · JPL Horizons ephemerides

VI · The limit

The relativistic rocket

Near the speed of light, velocities no longer add; rapidities do. The relativistic rocket equation keeps Tsiolkovsky's logarithm and wraps it in a hyperbolic tangent, so no mass ratio ever reaches c:

Δv=c⁡tanh⁡(vec⁡ln⁡m0mf)

For ve≪c it reduces exactly to the classical equation.

Read: Relativistic rocket · Physical constants

VII · No return

The event horizon

Set the escape velocity equal to the speed of light and solve for the radius: that is the Schwarzschild radius, the event horizon of a non-rotating black hole, where no delta-v is enough:

rs=2GMc2

For the Sun it is about 2.95 km. Matter spiralling in heats into a glowing accretion disk, the burning ring the Event Horizon Telescope imaged around M87* and Sagittarius A*.

Read: Schwarzschild radius · Event horizon · Accretion disk

Instrument

Δv calculator

The rocket equation, live. Enter an engine's specific impulse and the vehicle's masses.

Exhaust velocity ve
4,413 m/s
Mass ratio m0/mf
8.333
Delta-v Δv
9,357 m/s
Propellant fraction
88.0 %

DeltaV THRUST

THRUST physics: where each law lives in THRUST

The name carries the physics: THRUST is the force. ΔV is the journey. These are analogies of design, not promises of price; every number on this site is read from the chain.

Reference

Constants used on this page

QuantitySymbolValueSource
Speed of light in vacuumc299,792,458 m/s (exact)NIST CODATA
Newtonian constant of gravitationG6.674 30 × 10⁻¹¹ m³ kg⁻¹ s⁻²NIST CODATA
Standard gravityg09.806 65 m/s² (exact)Standard gravity
Earth's gravitational parameterμ⊕3.986 004 418 × 10¹⁴ m³/s²Standard gravitational parameter
Earth's equatorial radiusR⊕6,378.137 kmOrbital speed

Questions

Delta-v and THRUST: common questions

What is delta-v?

Delta-v (Δv) is the change in velocity a spacecraft can achieve with the propellant it carries. Missions are planned as a delta-v budget, the sum of every burn: about 9.4 km/s to reach low Earth orbit, and about 3.9 km/s more from there to geostationary orbit.

What is THRUST?

THRUST is the force a rocket engine produces by throwing mass backwards: F = ṁvₑ + (pₑ − p₀)Aₑ, the mass flow rate times the exhaust velocity plus the nozzle's pressure term. It is measured in newtons.

What is the Tsiolkovsky rocket equation?

Δv = vₑ ln(m₀/m_f): delta-v equals the exhaust velocity times the natural logarithm of the full mass over the dry mass. Konstantin Tsiolkovsky published it in 1903. Because of the logarithm, the propellant a mission needs grows exponentially with its delta-v.

What is specific impulse?

Specific impulse (Isp) is the impulse an engine produces per unit weight of propellant, in seconds: Isp = vₑ/g₀ with g₀ = 9.80665 m/s². Hydrogen–oxygen engines reach about 450 s in vacuum; ion engines exceed 3,000 s at very low THRUST.

Why do rockets have stages?

Empty tanks and spent engines are dead weight. Dropping them lets each stage start with a fresh mass ratio, so the delta-v of the stages adds up: two stages of mass ratio 4 at 450 s reach about 12.2 km/s, where one stage capped near mass ratio 8 reaches about 9.2 km/s.

What is escape velocity?

The speed at which an object's kinetic energy equals the depth of the gravity well, √(2μ/r), so it never falls back: about 11.2 km/s from Earth's surface. Where it reaches the speed of light, r = 2GM/c², is a black hole's event horizon.

What does ΔV mean in DeltaV THRUST?

The name carries the physics: THRUST is the force, ΔV is the journey. The token is the propellant; the bridge is staged like a rocket, each chain carrying only what is locked behind it; the liquidity is locked for 100 years. These are analogies of design, not promises of price.