General relativity — where it appears
Named by 4 essays across 3 fields — each of them below, with the objects they name alongside it.
Forty-three arcseconds, after everything else
Mercury's perihelion moves through 5,600 arcseconds a century. Nearly all of that is the coordinate system turning, and almost all of the rest is the other planets. What was left over was 43 — under one per cent of the raw number, and the most consequential residual in the history of the subject.
An orbit measured to be shrinking
A 7.75-hour orbital period that shortens by 68 nanoseconds each turn is beyond any single measurement, and unmissable after fifty thousand of them, because the shift accumulates as the square of the elapsed time. Forty-five years of pulse arrival times have made it 87.5 seconds, which is why the rate is a measured quantity rather than an inferred one.
The precession that switches the cycle off
A distant companion can trade an orbit's inclination for its eccentricity, over and over, and drive a pericentre almost onto the central body. General relativity's own precession competes with the mechanism for the same pericentre, and when it wins the cycle stops — sharply, at a ratio of one, which puts a floor on how close anything can be delivered.
A floor under the centre that assumes nothing
There is a lower bound on the pressure at the centre of any body in hydrostatic equilibrium, and it needs no equation of state, no composition and no temperature — only a mass and a radius. For the Sun it is nearly useless. For a neutron star it says which theory of gravity the interior needs.
Named alongside it
The objects these essays reach for when they reach for this one.
Apsidal precessionEccentricityBinary pulsarNeutron starResidualAdiabatic invariantBarycentreCentral condensationDegeneracy pressureEffective potentialEquation of stateHierarchical triple