Spin–orbit alignment — where it appears
Named by 3 essays across 2 fields — each of them below, with the objects they name alongside it.
A velocity measured from a shape
A transiting planet hides part of a rotating disc, so the star's line profile loses a slice at one velocity and its fitted centroid moves. The star has not moved at all — and the lopsidedness of that motion is the whole measurement of whether the orbit lies in the star's own equatorial plane.
A misalignment only cool stars forget
A third of hot Jupiters orbit at a large angle to their star's equator, and some go round backwards. Sort the same planets by the temperature of their host and the picture changes — below about 6,250 kelvin almost all are aligned, and above it almost none are. The boundary is not about the planets.
A precession slowed by stars lying on their sides
The eclipsing binary DI Herculis turns the long axis of its orbit at a quarter to a seventh of the rate relativity and the stars' own distortion predict, and for a quarter of a century that gap was offered as evidence against general relativity. The answer was in the stars: both spin nearly on their sides, and a flattened star tipped past 54.7 degrees drags the orbit's periastron backwards instead of forwards. Explained, the slow precession becomes a measurement of something no spectrum shows — how far the spins lean towards the Earth.
Named alongside it
The objects these essays reach for when they reach for this one.
The Rossiter–McLaughlin effectApsidal constantApsidal motionConvective envelopeDisc migrationDoppler effectEclipsing binaryEquilibrium tideGeneral relativityHigh-eccentricity migrationHot jupiterKozai lidov mechanism