A post-fit residual — where it appears
Named by 3 essays across one field — each of them below, with the objects they name alongside it.
The table that is a fit
A planetary ephemeris is not evaluated from Kepler's laws and is not evaluated from a theory. It is a numerical integration whose starting conditions were least-squares fitted to a century and a half of observations, and its accuracy is a property of those observations rather than of the mathematics.
A distant planet felt only as a stretch
An undiscovered planet far beyond Neptune pulls the Sun and Saturn almost equally, and an ephemeris, which measures only where Saturn is relative to the Sun, cannot see a pull that moves both together. What it can see is the difference — a tidal stretch falling as the mass over the cube of the distance — and most even of that is absorbed by refitting Saturn's orbit. What is left decides which planets the solar system can be hiding.
A Moon that would lean towards the Sun
Part of the Earth's mass is its own gravitational binding energy — a few parts in ten billion. If that part fell towards the Sun even slightly differently from the rest, the Earth and the Moon would fall at different rates and the Moon's orbit would be pushed sunward once a month by about eleven metres for every unit of the difference. Fifty years of laser ranging to the Moon have looked for that push at the millimetre level, against a term the Sun's ordinary gravity puts at the same frequency a hundred kilometres high.
Named alongside it
The objects these essays reach for when they reach for this one.
EphemerisLeast-squares fitLunar laser rangingA nuisance parameterSpacecraft rangingAsteroid massBarycentric dynamical time (TDB)DegeneracyEquivalence principleFit intervalGravitational binding energyKuiper belt