Benchmark star — where it appears
Named by 2 essays across one field — each of them below, with the objects they name alongside it.
Two radii, from a light curve alone
The radius of a star is not measured. It is inferred, from a temperature and a luminosity, through a model. There is one exception — a pair of stars that eclipse each other, whose light curve and velocity curves between them give both radii, both masses and the ratio of temperatures with no model of a stellar interior anywhere in the chain.
Two scaling relations calibrated on one star
Asteroseismology gives a star's mass and radius from two numbers read off its oscillation spectrum. The two relations are exact in their exponents and approximate in their constants, and the constants were fixed by requiring that the Sun come out right — so an error of a few per cent in one observable is tens of per cent in a mass and nearly a factor in an age.
Named alongside it
The objects these essays reach for when they reach for this one.
Apsidal motionDetached binaryDistance determinationEclipsing binaryError propagationFractional radiusFrequency of maximum powerInclinationLarge separationLimb darkeningMass radius relationRadial velocity curve