Residual — where it appears
Named by 4 essays across 2 fields — each of them below, with the objects they name alongside it.
A comet that arrives a day early
Encke's comet returned two and a half hours ahead of prediction, every revolution, for decades before anybody could say what was pushing it. The force is a rocket — a few tonnes a second of vapour leaving the sunward side of a rotating nucleus, delivered almost entirely in the few weeks around perihelion, and it accumulates in the arrival time as the square of the number of returns.
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.
An acceleration that was the spacecraft's own heat
Two probes leaving the solar system were tracked for thirty years and both drifted from their predicted paths by a tenth of a nanometre per second squared. The residual was real, it was constant, and it was the same on both. It was also the waste heat of the reactors that powered them, radiating slightly more one way than the other.
Named alongside it
The objects these essays reach for when they reach for this one.
Apsidal precessionBinary pulsarEccentricityGeneral relativityNon-gravitational accelerationAnisotropic emissionBarycentreComet nucleusDoppler trackingEffective potentialGauss planetary equationsInverse square law