Hyperbolic orbit — where it appears
Named by 6 essays across 3 fields — each of them below, with the objects they name alongside it.
Every orbit one force allows, and the number that picks between them
Circle, ellipse, parabola, hyperbola. A single inverse-square force permits exactly these four, and one number decides which — including whether the body ever comes back.
The orbit that has no period
Above an eccentricity of 1 the conic is open, the energy is positive and the semi-major axis is negative — and the vis-viva relation survives the sign change without a single alteration. What replaces the period is a speed, and that speed is what says where a visitor came from.
The one solve that does not ask which conic it is
Kepler's equation is for ellipses, Barker's cubic for parabolas, and a hyperbolic sine for the rest — three parameterisations of one motion, each worst exactly where its neighbour takes over. The universal variable removes the question, and the removal is not a convenience.
One trajectory, stitched from three two-body problems
An interplanetary flight is a problem with no closed solution. It is flown by cutting it into pieces that each have one, and the seams are places where the model is knowingly false.
An answer obtained along a path that was not taken
Integrate the force of a passing mass along the straight line the body would have followed if the encounter had not happened, and out comes an exact deflection with no free constant in it. The approximation is circular, it is wrong in a known direction by a known amount, and it is the reason stellar dynamics has closed forms at all.
The planet pays, and it shows
A gravity assist takes energy from a planet and gives it to a spacecraft, and the planet's loss is exactly the spacecraft's gain. For a two-tonne probe past Jupiter that loss is unmeasurable. Do it with a hundred Earth masses of icy debris and the same bookkeeping moves Neptune outward by several astronomical units.
Named alongside it
The objects these essays reach for when they reach for this one.
Orbital energyConic sectionsEccentricityGravity assistAngular momentumCharacteristic energyClose encounterKepler's equationSemi-major axisAdiabatic invariantBarkers equationCentral force