Asteroid belt — where it appears
Named by 3 essays across one field — each of them below, with the objects they name alongside it.
The size at which a body is easiest to break
A pebble is held together by the strength of its rock and a moon by its own gravity, and somewhere between them is a size that has too little of either. Bodies a few hundred metres across are the weakest in the solar system — sixteen metres a second of impact energy per kilogram is enough to scatter one — and a population grinding itself down records that weakness as a knee in its size distribution.
A denominator that emptied the inner belt
The eccentricity Jupiter and Saturn force on an asteroid is a fraction, and its denominator is the difference between the asteroid's own precession rate and one of the planets'. At two astronomical units that difference is zero. Where the zero sits depends on where Saturn is — and the belt's quiet orbits say Saturn did not take long to get there.
An age read from angles that meet
A family of asteroids a few million years old has had its members' orbits turned round and round by the planets, each at a slightly different rate, until their orientations look random. Turn them back and they come together at one instant — the collision — with an uncertainty of a few tens of thousands of years, but only if each member's own slow drift in sunlight is put back too.
Named alongside it
The objects these essays reach for when they reach for this one.
Proper elementsApsidal precessionAscending nodeAsteroid familyCollisional cascadeDebris discDisruption thresholdDohnanyi slopeForced eccentricityGravity regimeLaplace–Lagrange theoryLongitude of perihelion