The mutual Hill radius — where it appears
Named by 3 essays across 2 fields — each of them below, with the objects they name alongside it.
A feeding zone, and the spacing it forces
The radius that decides what a planet may keep also decides what it could reach while it was growing — and measuring the gaps between planets in that unit turns a distribution spanning three orders of magnitude in astronomical units into a band a factor of ten wide, with a floor that is partly a theorem and partly a fit.
A stability limit with a notch cut in it
The two numbers usually quoted for how far out a moon may orbit are coplanar numbers. A tilted orbit is not somewhere between them: inside a band of inclination fifty-six degrees wide the Sun converts the tilt into an eccentricity, the apocentre rather than the semi-major axis has to stay inside the lobe, and the limit falls to half. The band is empty in the sky.
A spacing law that random orbits obey
The planets' distances roughly double from one to the next, and a rule written down in 1766 predicted the asteroid belt and Uranus before either was found. It failed on Neptune, and the reason it worked at all turns out to be that almost any set of orbits forbidden to crowd each other looks geometric on a logarithmic scale — as a test against thousands of random systems shows.
Named alongside it
The objects these essays reach for when they reach for this one.
Hill stabilityApsidal precessionCritical inclinationDynamical spacingFeeding zoneHarmonic lawHill sphereIrregular satellitesIsolation massJacobi constantKozai lidov mechanismLaplace plane