Intuition The one core idea
Escape velocity asks a single question: how fast must I launch something so it climbs out of a planet's gravity "valley" forever and never rolls back? To answer it, we only need two ideas — that gravity stores energy as a debt you must repay, and that total energy is conserved — so this whole page just builds the vocabulary those two ideas require, one symbol at a time.
This is the ground-floor page for Escape velocity — derivation . If any letter in that note made you pause, it is defined here from nothing. Read top to bottom: each symbol is earned before the next uses it.
Definition Scope — what this page does and does not do
This foundations page only builds and defines the vocabulary : the symbols M , m , r , R , v , the force law, kinetic and potential energy, the integral, and conservation of energy. The actual four-step derivation of v e = 2 GM / R — writing E i , setting E f = 0 , equating, and solving — is done in the parent note Escape velocity — derivation . Here we deliberately stop just before that algebra: we hand you the fully-defined tools, and the parent note swings them.
Before formulas, meet every symbol as a plain-language character with a picture.
M — the big mass (the planet)
M is the mass of the body you are escaping from — Earth, the Moon, a star. "Mass" means how much stuff is in it, measured in kilograms. In the picture it is the large ball at the centre. The topic needs M because the bigger the planet, the deeper its gravity valley, and the harder it is to leave.
m — the small mass (the thing escaping)
m is the mass of the object trying to leave — a pebble, a rocket, a gas molecule. It is tiny compared to M . The topic needs m so we can talk about its energy — but a punchline of the whole derivation is that m cancels out , so the escape speed is the same for a pebble and a spaceship.
r — distance from the centre
r is the distance from the centre of M to the object m , measured in metres. Not from the surface — from the centre . In the figure it is the length of the arrow joining the two. The topic needs r because gravity gets weaker the farther out you go, so everything depends on r .
R — the radius (a special value of r )
R is one particular distance: the surface of the planet, i.e. r = R at launch. It is where the rocket starts. The topic needs R because that is where we set the object moving. Everything on this page lives in the region outside the planet, r ≥ R — we never go under the surface.
Figure 1 — The five symbols in one scene: the big mass M (lavender ball) at the centre; the escaping object m (coral dot); the distance r (grey arrow from centre to m ); the radius R (mint arrow from centre to surface); and the speed v (yellow arrow showing motion). Notice r and R both start at the centre , not the surface.
v — speed
v is how fast the object is moving, in metres per second. In the figure it is the length of the little arrow showing motion. We write v e (with subscript e for escape ) for the special launch speed we are hunting.
Now the characters combine into the two concepts the derivation actually runs on.
Let us earn every piece:
M and m on top: the more mass on either side, the stronger the pull — makes sense, more stuff, more grip.
r 2 on the bottom: pull gets weaker as you move away, and specifically as the square of distance. Double the distance → one-quarter the pull.
G : a fixed number of nature, the gravitational constant , G ≈ 6.67 × 1 0 − 11 . It is just the "conversion rate" that turns kilograms and metres into newtons. You never change it; it is the same everywhere in the universe.
1/ r 2 and not 1/ r ?
Picture gravity as invisible lines spreading out from the planet in all directions, like paint sprayed onto the inside of a bigger and bigger sphere. The same amount of "pull-paint" is smeared over a sphere whose area grows as r 2 . So the pull per patch thins out as 1/ r 2 . This is the fact that makes gravity fade to exactly zero at infinity — which is the whole reason escape is possible.
Figure 2 — Gravity's strength F (vertical axis) plotted against distance r (horizontal axis). At distance r the pull is full (coral dot); at 2 r it has dropped to one quarter (mint dot) — the signature of a 1/ r 2 law. The curve flattens onto zero far to the right: at infinity, gravity vanishes.
Energy is "the ability to make things happen," measured in joules. Two flavours matter here. We define both pieces first , then combine them into the single total E .
Definition Kinetic energy
K — energy of motion
K = 2 1 m v 2
The faster (v ) or heavier (m ) something moves, the more K it carries. In the picture it is a "speed fuel tank." A launched rocket starts with a full tank; as it climbs and slows, the tank drains.
Why v 2 and not just v ? Because stopping a thing going twice as fast takes four times the work — this is a measured fact of nature, and the square captures it. We need K because escape is fundamentally a race: does your motion-energy last all the way to infinity?
Definition Potential energy
U — stored energy of position
U is energy an object has simply because of where it sits in the gravity field. Lift a book — you spent effort, and that effort is now "stored" in the book's raised position, ready to turn back into motion if you drop it. Near a planet, being deep in the valley is a low-energy (negative) position; being far out is a high-energy (zero) position.
Intuition The valley picture — why
U is negative
Imagine a smooth bowl whose walls we only draw from the surface outward (r ≥ R ). The lowest point we allow is the planet's surface r = R ; the flat rim infinitely far away is "space." A marble at the surface is trapped — it has less energy than a marble on the rim. We choose the rim to be the zero of energy (U = 0 at r → ∞ ). Everything below the rim is therefore negative . That is why you will always see U ( r ) = − r GM m with a minus sign: being bound = being below zero.
A subtlety we deliberately fence off: the plain formula U = − GM m / r would keep dropping for imaginary points inside the planet (r < R ), because the mass law changes there. We never launch from inside a planet, so we simply restrict everything to r ≥ R — the surface is the floor of our story.
Figure 3 — The gravity valley: potential energy U ( r ) (vertical axis) against distance r (horizontal axis), drawn only for r ≥ R . The dashed line at the top is the rim U = 0 at infinity. The lavender floor at r = R (surface) is the deepest, most negative point we allow; far to the right U climbs back toward zero — the object is nearly free.
E — the total mechanical energy (the two pieces added)
Now that K and U each have a meaning, we add them into one running total:
E = K + U = 2 1 m v 2 − r GM m
E is the grand bank balance — motion-energy plus position-energy — that we will track from launch to infinity. Below we explain why this total stays frozen throughout the flight.
Common mistake The number-one sign trap
Writing U = + r GM m (no minus). It feels right because bigger numbers should mean "more energy." But with the rim chosen as zero, a trapped object must be below zero. Keep the minus, or the final formula produces the square root of a negative number — a nonsense "imaginary" speed.
The parent note uses two mathematical moves. Here is what each one is and why it is the right tool.
Definition The integral sign
∫ — "add up a changing thing"
When a quantity keeps changing as you move (here: the force F changes at every distance r ), you cannot just multiply "force × distance." Instead you slice the journey into tiny steps of width d r ′ — the little symbol d r ′ just means "one sliver of distance, as thin as you like" — compute force × sliver, F ( r ′ ) d r ′ , for each, and sum them all . That endless sum of slivers is what ∫ means; the numbers below and above the sign, ∞ and r , say where the summing starts and stops .
Intuition Why the prime on
r ′ — a "walking foot" variable
Notice we write r ′ (r-prime) inside the integral, but plain r as the endpoint on top. They are different jobs. r ′ is a dummy variable : it is the "walking foot" that marches through every distance from ∞ down to the target, one sliver at a time. Plain r is the fixed destination where the walk stops. Using two different letters keeps "the point we are currently summing at" (r ′ ) from being confused with "the point we finally arrive at" (r ). The prime is just a costume so the walking foot never gets mistaken for the finish line.
Definition Conservation of mechanical energy — "the total never changes"
If only gravity acts (no air drag, no rocket engine still firing), then the total energy E = K + U stays the same number for the whole flight:
E = 2 1 m v 2 − r GM m = constant.
As the rocket climbs, U rises toward zero and K falls — but their sum E is frozen.
E constant? Gravity is a "conservative" force
A force is called conservative when the work it does depends only on where you start and finish , never on the wiggly path between. Gravity qualifies because F depends only on distance r — climb out by a spiral or a straight line, and gravity charges you the exact same energy toll. Whenever a force is conservative, every joule gravity takes from your motion (K drops) is stored as position energy (U rises) and vice-versa — nothing leaks away. That perfect swap between the two tanks is precisely what "K + U = constant" means. (If air drag were present it would not be conservative — it would burn energy into heat, and E would shrink. That is why the derivation says "no air.")
Intuition Why conservation is the perfect tool here
We do not care about the messy details of the path — how fast at every altitude, how long it takes. We only care about two moments: the start (surface) and the end (infinity). Conservation lets us ignore everything in between and just compare start to end. That is why the parent note's derivation is four short lines and not a page of calculus.
The map below reads top-down : the raw symbols (top row) build Newton's force law; summing that force with the integral produces the potential energy U ; kinetic energy K and potential energy U pour into one total E that conservation keeps constant; evaluating that total at the surface gives E ( R ) , and equating it to the value at infinity finally yields escape velocity v e . In words: symbols → force → energy → conservation → answer .
Newton gravity F = GMm over r squared
Kinetic energy K = half m v squared
Potential energy U = minus GMm over r
Integral: sum force times dr
Total energy E = K plus U
Launch value E at R = half m ve squared minus GMm over R
Conservation keeps E constant
Read it top-down: the raw symbols build the force law, the force law is summed into potential energy, kinetic and potential energy combine into one total energy, conservation freezes that total, evaluating it at the surface gives E ( R ) , and equating that to the value at infinity gives escape velocity.
Worked example Do the units even make sense? (dimensional analysis first)
Before plugging numbers, check that 2 GM / R actually comes out in metres per second. Write each symbol's units in the square bracket [ ] :
G has units [ m 3 kg − 1 s − 2 ] (this is fixed by Newton's law: force kg m s − 2 equals G kg 2 / m 2 , solve for G ).
M has units [ kg ] .
R has units [ m ] .
Combine inside the root (the pure number 2 has no units):
[ R GM ] = m ( m 3 kg − 1 s − 2 ) ( kg ) = m m 3 s − 2 = m 2 s − 2 .
Take the square root: m 2 s − 2 = m s − 1 = m/s . A speed — exactly what we wanted. The formula is unit-consistent, so now we may trust the numbers.
Now the numbers (Earth: G = 6.67 × 1 0 − 11 , M = 5.97 × 1 0 24 kg , R = 6.37 × 1 0 6 m ):
v e = 6.37 × 1 0 6 2 ( 6.67 × 1 0 − 11 ) ( 5.97 × 1 0 24 ) ≈ 1.12 × 1 0 4 m/s ≈ 11.2 km/s ,
the famous "11 km/s." Units check and value check — the foundations are wired up correctly. The derivation of this formula lives in the parent note; here we only confirm the tools produce the right ballpark.
Is r measured from the surface or the centre?
Why is U negative for a bound object?
Which single principle lets us compare only "launch" and "infinity" and skip the middle, and why is it allowed?
Centre or surface for r ? The centre of the big mass M .
Why is U ( r ) negative? We set U = 0 at infinity (the rim); anything trapped below the rim has less energy, so it is negative.
What does the prime on r ′ inside the integral mean? r ′ is a dummy "walking-foot" variable marching through every distance being summed; plain r is the fixed endpoint where the walk stops.
Which antiderivative rule gives − 1/ r ? ∫ r ′ − 2 d r ′ = − 1 r ′ − 1 = − r ′ 1 , checked because the slope of − 1/ r ′ is r ′ − 2 .
Why is total energy E conserved during escape? Gravity is conservative — its work depends only on start and end, not the path — so K and U trade perfectly with no leak (given no drag/engine).
Why does gravity reach exactly zero at infinity? Because F ∝ 1/ r 2 , and 1/ r 2 → 0 as r → ∞ .
Each line tests a piece of understanding you could not have stated before reading this page — not a bare restatement.
Given G , M , R , argue in one line why 2 GM / R must be a speed Its units reduce to m 2 s − 2 inside the root, whose square root is m/s .
Explain why m can be expected to vanish from the escape speed Both K = 2 1 m v 2 and U = − GM m / r carry one factor of m , so it divides out of any energy balance.
State the antiderivative rule you must invoke and check it ∫ r ′ n d r ′ = n + 1 r ′ n + 1 ; with n = − 2 it gives − 1/ r ′ , verified since the slope of − 1/ r ′ is r ′ − 2 .
Say what makes the energy method valid at all Gravity is conservative (work path-independent), so E = K + U is constant with no air drag or engine.
Name what is deferred to the parent note versus done here Here: defining every symbol, F , K , U , the integral, conservation. There: writing E i , setting E f = 0 , equating, solving for v e .