3.2.4 · D1Orbital Mechanics & Astrodynamics

Foundations — Orbit shape from eccentricity — circle (e=0), ellipse (0 - e - 1), parabola (e=1), hyperbola (e - 1)

3,092 words14 min readBack to topic

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.


1. Distance, angle, and the two masses

Together are polar coordinates — a "how far, which way" address. This is why the whole topic is written as : give me the direction, I'll tell you the distance.

Figure — Orbit shape from eccentricity — circle (e=0), ellipse (0 - e - 1), parabola (e=1), hyperbola (e - 1)

2. The focus — the special point the orbit is drawn around

This matters because — once we have built the orbit equation later on — the distance 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.


3. Slicing a cone — where all four shapes come from

Figure — Orbit shape from eccentricity — circle (e=0), ellipse (0 - e - 1), parabola (e=1), hyperbola (e - 1)

4. Two things geometry gives us: , , and

Before energy enters, the shape of an ellipse needs three lengths.

We now have purely from geometry. Later, once angular momentum and gravity's strength are defined (Sections 6 and 8), the very same will re-appear as — the physics value of the same width. That double life of is exactly what ties the orbit's shape to the body's motion, but we cannot write that formula honestly until those symbols exist.


5. The trig tool: cosine, and why it (not sine) appears

Now that we have , , and , we can finally read the orbit equation the parent states: Every symbol in it has now been earned. (At , , so — which is precisely why is the "width at the focus" we defined above.)

This single fact drives the entire "read off the denominator" argument in the parent: the denominator shrinks as grows toward (because falls toward ), and grows.


6. Rates of change: the dot, and specific angular momentum

See the connection Angular Momentum in Orbits: is what fixes the width (the in it is defined in Section 8).


7. Energy: , , , and the sign that decides everything

Figure s04 draws exactly this. The curved chalk line is the potential well : steep and deep near the centre, flattening to the dotted "rim" (energy ) 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 () so the body can never reach the right edge → it is trapped → ellipse. The pink dashed level sits exactly on the rim () → it just barely reaches infinity → parabola. The yellow level sits above the rim () → it reaches infinity with height to spare → hyperbola.

See Specific Orbital Energy and Escape Velocity (the boundary), and Vis-viva Equation (which turns into a speed at any ).


8. Gravity's constants: and

Why bundle and ? Because they only ever appear together in orbit maths, so carrying one symbol is cleaner. It appears in (now every symbol in it — , , — is defined) and in .


9. Putting the master relation in plain words

Read the sign of straight off:

  • inside-the-square-root is less than 1 ellipse/circle.
  • parabola.
  • hyperbola.

That single formula is the whole parent topic compressed. Everything else is decoration.


Prerequisite map

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

Four shapes

Eccentricity e equals c over a

Rates of change the dot

Specific angular momentum h

e from energy and momentum

Specific energy epsilon

Potential energy U equals minus GMm over r

Gravity strength mu equals GM

Orbit shape from eccentricity

All streams feed the parent topic.


Equipment checklist

Test yourself — cover the right side and answer each before revealing.

What are the two masses and ?
is the big central body that pulls; is the small orbiting body that is pulled.
What do the two numbers 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, ), 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, (focal distance over semi-major axis).
What is the semi-latus rectum , and why ?
The width at the focus (); since .
What does equal, and why is it NOT ?
It equals , the square of the semi-minor axis — not .
Why does (not ) appear in ?
Because makes smallest at , our chosen closest point (perihelion).
For , which angles are allowed and why?
Only , so that keeps positive; beyond, would be negative (unphysical).
What does a dot over a symbol mean, e.g. ?
The rate of change per second; is angular speed.
What is specific angular momentum , and why conserved?
, spin per unit mass; conserved because gravity exerts no sideways torque.
How do and differ?
; is total, is per unit mass .
What is the gravitational potential energy ?
, negative and zero at infinity — the "height-in-the-well" energy.
What is specific energy and why does its sign matter?
; its sign decides bound (), marginal (), or unbound ().
What are and ?
is the universal gravitational constant; bundles it with the central mass to give that body's pull strength.
State the eccentricity–energy relation.
.