Intuition The ONE core idea
A body moving under gravity always traces a conic section , and a single dimensionless number — the eccentricity e — tells you which one (circle, ellipse, parabola, or hyperbola). Everything on the parent page is just carefully unpacking how e is born from two conserved quantities (energy and angular momentum) and what shape each value of e draws.
This page builds every symbol the parent note leans on, starting from a smart-12-year-old's toolkit and nothing more. Read top to bottom — each block only uses things defined above it.
M and m — the two masses
==M is the big central mass (the Sun, or a planet) that sits still at the centre and does the pulling. m is the small orbiting body== (a planet, comet, or spacecraft) that gets pulled. Both are measured in kilograms.
Picture: a heavy bowling ball M resting on a stretched sheet, and a light marble m rolling around the dip it makes.
r — the distance
r is simply ==how far the orbiting body m is from the central mass M ==, measured with a ruler. It is a positive length. In symbols it is a number of metres (or kilometres, or astronomical units).
Picture: a straight line drawn from the Sun to a planet. Its length is r .
θ — the angle
θ (Greek letter "theta") is the ==angle that the line r has swept around==, measured from a chosen starting direction. We measure angles in degrees (0 ∘ to 36 0 ∘ ) or radians.
Picture: stand at the Sun, point at where the planet was closest, call that θ = 0 . As the planet moves around, the pointer turns; how far it has turned is θ .
Together ( r , θ ) are polar coordinates — a "how far, which way" address. This is why the whole topic is written as r ( θ ) : give me the direction, I'll tell you the distance.
Intuition WHY polar and not
x , y ?
Gravity pulls along the line to the centre . That line is exactly the direction r points. So the natural coordinate to describe a gravity problem is "distance-and-angle-from-the-centre", not a grid of x , y boxes. The maths comes out far cleaner.
A focus is a fixed point that a conic curve is built around. The central mass M sits at one focus. For our orbit, the focus is the origin — the place where r = 0 .
Picture: the pin you'd stick in the ground; the orbit is drawn relative to that pin, not relative to the middle of the loop.
This matters because — once we have built the orbit equation later on — the distance r will always be measured from the focus , not from the geometric centre. The Sun is at the focus, off to one side of the ellipse — never in its middle.
Intuition WHY one equation gives four shapes
Take a hollow ice-cream cone and cut straight through it with a flat blade. Depending on the tilt of the cut you get a circle, an ellipse, a parabola, or a hyperbola. These four are the Conic Sections — literally "sections (slices) of a cone". Gravity's orbit equation is the algebra of these slices, which is why exactly these four shapes (and no others) appear.
e (the shape score)
Eccentricity e is a single dimensionless number (e ≥ 0 ) that records how "un-circular" the slice is: how tilted the cutting blade was.
e = 0 : blade horizontal → circle
0 < e < 1 : blade tilted a bit → ellipse (a closed oval)
e = 1 : blade parallel to the cone's side → parabola (just barely open)
e > 1 : blade steep enough to cut both halves of the cone → hyperbola (wide open)
Picture: a dial from 0 upward; as you turn it, the loop stretches, then snaps open.
Before energy enters, the shape of an ellipse needs three lengths.
a — semi-major axis
==a is half of the longest diameter of the ellipse== — the distance from the centre to the far end.
Picture: the ellipse's long "radius".
c — focal distance
==c is the distance from the centre of the ellipse to a focus==. Bigger c = focus sits further from the middle = more squashed.
Picture: how far off-centre the pin is.
p — semi-latus rectum
==p is the distance r measured from the focus at a right angle to the long axis==. On the ellipse it is the "half-width at the focus".
Picture: stand at the focus, look at a right angle to the long axis; the distance to the curve is p .
p = a ( 1 − e 2 ) — a "why", not a leap
p is a width and a is a length; they must be related. Look at figure s03: the closest point (perihelion) sits at distance a − c from the focus, and the farthest (aphelion) at a + c . A standard property of the ellipse — derivable from the definition "sum of distances to the two foci is constant" — is that the semi-latus rectum equals
p = a a 2 − c 2 .
Because e = c / a means c = e a , the numerator is a 2 − e 2 a 2 = a 2 ( 1 − e 2 ) , so
p = a a 2 ( 1 − e 2 ) = a ( 1 − e 2 ) .
So p shrinks as e grows: the more stretched the orbit, the narrower it is at the focus. (Beware a lookalike: the quantity ( a − c ) ( a + c ) = a 2 − c 2 equals the square of the semi-minor axis b , i.e. b 2 , not p 2 — do not confuse the two.)
We now have p purely from geometry. Later, once angular momentum and gravity's strength are defined (Sections 6 and 8), the very same p will re-appear as p = h 2 / μ — the physics value of the same width. That double life of p is exactly what ties the orbit's shape to the body's motion , but we cannot write that formula honestly until those symbols exist.
cos θ — cosine
For an angle θ , cos θ is a number between − 1 and + 1 that tells you ==how much of the direction θ points "along the reference axis"==. It equals + 1 at θ = 0 ∘ , 0 at 9 0 ∘ , and − 1 at 18 0 ∘ .
Picture: the shadow a unit-length pointer casts on the horizontal axis as it rotates.
Now that we have p , e , and cos θ , we can finally read the orbit equation the parent states:
r ( θ ) = 1 + e c o s θ p
Every symbol in it has now been earned. (At θ = 9 0 ∘ , cos 9 0 ∘ = 0 , so r = p — which is precisely why p is the "width at the focus" we defined above.)
Intuition WHY cosine, not sine?
We chose θ = 0 to be the direction of closest approach (perihelion). We want r to be smallest there, which means the denominator 1 + e cos θ must be largest there. Cosine is + 1 at θ = 0 — perfect, it makes the denominator biggest exactly at perihelion. Sine would be 0 at θ = 0 and misplace the closest point. So cosine is the tool that "lines the orbit up" with our chosen start.
This single fact drives the entire "read off the denominator" argument in the parent: the denominator shrinks as θ grows toward 18 0 ∘ (because cos falls toward − 1 ), and r grows.
Common mistake The domain trap: when
e > 1 , not every θ is allowed
Why it bites: for a circle or ellipse (e < 1 ), 1 + e cos θ is always positive — smallest at θ = 18 0 ∘ where it equals 1 − e > 0 — so every angle gives a valid positive r and the curve closes.
The edge case: for a hyperbola (e > 1 ), the denominator hits zero when cos θ = − 1/ e , and goes negative beyond that. A negative r is unphysical. So the body only exists on the orbit for the angles where 1 + e cos θ > 0 , i.e. cos θ > − 1/ e . Those forbidden angles are the incoming/outgoing asymptotes — the directions the body flies in from and escapes to.
The knife-edge (e = 1 , parabola): the denominator 1 + cos θ reaches zero only at θ = 18 0 ∘ (and nowhere goes negative), so r → ∞ in exactly one direction. The domain is every angle except that single escape direction.
Definition The dot — a rate of change
A dot over a symbol means how fast it changes per second . So θ ˙ ("theta-dot") is how fast the angle is turning — the angular speed.
Picture: the second hand of a clock; θ ˙ is its turning rate.
Intuition WHY we need a "rate" at all
A shape alone can't tell you if the body comes back . That is decided by motion — speeds and how they trade off. Rates of change are the language of motion, so they must enter.
h — specific angular momentum
==h = r 2 θ ˙ is the spin-content of the orbit, measured per kilogram of the orbiting body m .== "Specific" always means "per unit mass". Because gravity torques nothing sideways, h never changes during the orbit — it is conserved .
Picture: a figure-skater; arms in (small r ) → spins fast (big θ ˙ ); arms out (big r ) → spins slow. The product r 2 θ ˙ stays fixed.
L — total angular momentum
L = m h = m r 2 θ ˙ is the whole body's spin-content, where m is the orbiting mass from Section 1. The only difference from h is that mass factor m .
L ::: for the whole body (= mh ); h ::: per kilogram. Parent uses both — keep them straight via the mass m .
See the connection Angular Momentum in Orbits : h is what fixes the width p = h 2 / μ (the μ in it is defined in Section 8).
E — total energy
E is the body's kinetic energy (from moving) plus gravitational potential energy (from being in the well) , added together. It is conserved.
Picture: a marble in a bowl. Total energy = (how fast it's rolling) + (how high up the wall it is), and this total never changes without friction.
U — gravitational potential energy
==U is the "height-in-the-well" energy== of the body: how much energy it owes for being trapped near the mass. With the usual choice that U → 0 infinitely far away, it is
U = − r GM m ,
where G and M are gravity's constant and the central mass (Section 8 finishes G ; M is from Section 1). It is negative because the body is below the far-away rim. So the total energy is honestly E = 2 1 m v 2 + U = 2 1 m v 2 − r GM m , where v is the body's speed.
Picture: the deeper into the bowl (smaller r ), the more negative U — the harder to climb out.
ε — specific energy
ε = E / m is the total energy per kilogram (dividing by the orbiting mass m ). Same idea, mass divided out.
ε ::: energy per unit mass E / m .
Intuition WHY the SIGN of energy is the whole story
Set the potential energy U to zero infinitely far away (as above). Then:
ε < 0 : the body is stuck below the rim of the well — it can never climb out → bound → closed orbit (circle/ellipse).
ε = 0 : it has exactly enough to reach the rim, arriving with zero speed → marginal escape → parabola.
ε > 0 : it climbs out with energy to spare , still moving at infinity → unbound → hyperbola.
This is why the parent's table pairs each shape with a sign of ε .
Figure s04 draws exactly this. The curved chalk line is the potential well U = − GM m / r : steep and deep near the centre, flattening to the dotted "rim" (energy = 0 ) far out. A body's total energy is a horizontal level line — because energy is conserved, it stays flat as the body moves. Read the figure this way: the blue level sits below the rim (ε < 0 ) so the body can never reach the right edge → it is trapped → ellipse. The pink dashed level sits exactly on the rim (ε = 0 ) → it just barely reaches infinity → parabola. The yellow level sits above the rim (ε > 0 ) → it reaches infinity with height to spare → hyperbola.
See Specific Orbital Energy and Escape Velocity (the ε = 0 boundary), and Vis-viva Equation (which turns ε into a speed at any r ).
G — the gravitational constant
==G is a fixed number of nature== (G ≈ 6.674 × 1 0 − 11 in SI units) that sets how strong gravity is everywhere in the universe . It is the same for a pebble and a galaxy.
Picture: the universal "exchange rate" that converts masses-and-distances into a pulling force.
μ — the standard gravitational parameter
==μ = GM == bundles the gravitational constant G with the central mass M (from Section 1) into one number. It sets the strength of this particular Sun/planet's pull.
Picture: a single knob for "how hard this central body grabs things."
Why bundle G and M ? Because they only ever appear together in orbit maths, so carrying one symbol μ is cleaner. It appears in p = h 2 / μ (now every symbol in it — p , h , μ — is defined) and in e = 1 + 2 ε h 2 / μ 2 .
Read the sign of ε straight off:
ε < 0 ⇒ inside-the-square-root is less than 1 ⇒ e < 1 ⇒ ellipse/circle .
ε = 0 ⇒ e = 1 = 1 ⇒ parabola .
ε > 0 ⇒ e > 1 ⇒ hyperbola .
That single formula is the whole parent topic compressed. Everything else is decoration.
The diagram below shows the dependency order of this page: geometry symbols (left) build the orbit equation, motion symbols (right) build the eccentricity–energy relation, and both streams merge into the four-shape classification that is the parent topic. Read an arrow as "is needed before". It is the reading order made visible — nothing downstream uses a symbol that is not upstream of it.
Polar coordinates r and theta
Orbit equation r of theta
Focus at the central mass
Cosine lines up perihelion
Conic sections from cone slices
Eccentricity e equals c over a
Specific angular momentum h
e from energy and momentum
Potential energy U equals minus GMm over r
Gravity strength mu equals GM
Orbit shape from eccentricity
All streams feed the parent topic .
Test yourself — cover the right side and answer each before revealing.
What are the two masses M and m ? M is the big central body that pulls; m is the small orbiting body that is pulled.
What do the two numbers ( r , θ ) tell you? How far the body is and in which direction, measured from the central mass.
Where does the central mass sit on the orbit? At a focus (the origin, r = 0 ), never at the centre of the ellipse.
Where do the four orbit shapes come from geometrically? They are the four ways to slice a cone with a flat plane — the conic sections.
Is eccentricity a length or a ratio, and what is it? A dimensionless ratio, e = c / a (focal distance over semi-major axis).
What is the semi-latus rectum p , and why p = a ( 1 − e 2 ) ? The width r at the focus (θ = 9 0 ∘ ); p = ( a 2 − c 2 ) / a = a ( 1 − e 2 ) since c = e a .
What does ( a − c ) ( a + c ) equal, and why is it NOT p 2 ? It equals a 2 − c 2 = b 2 , the square of the semi-minor axis — not p 2 .
Why does cos θ (not sin θ ) appear in r ( θ ) ? Because cos 0 ∘ = 1 makes r smallest at θ = 0 , our chosen closest point (perihelion).
For e > 1 , which angles are allowed and why? Only cos θ > − 1/ e , so that 1 + e cos θ > 0 keeps r positive; beyond, r would be negative (unphysical).
What does a dot over a symbol mean, e.g. θ ˙ ? The rate of change per second; θ ˙ is angular speed.
What is specific angular momentum h , and why conserved? h = r 2 θ ˙ , spin per unit mass; conserved because gravity exerts no sideways torque.
How do h and L differ? L = mh ; L is total, h is per unit mass m .
What is the gravitational potential energy U ? U = − GM m / r , negative and zero at infinity — the "height-in-the-well" energy.
What is specific energy ε and why does its sign matter? ε = E / m ; its sign decides bound (< 0 ), marginal (= 0 ), or unbound (> 0 ).
What are G and μ ? G is the universal gravitational constant; μ = GM bundles it with the central mass to give that body's pull strength.
State the eccentricity–energy relation.