Stellar inclination — where it appears
Named by 4 essays across 2 fields — each of them below, with the objects they name alongside it.
An angle hidden by the tilt of the star
The line profile of a transited star gives the angle between orbit and spin as projected on the sky. The true angle needs the tilt of the star's spin axis, and every way of measuring that tilt is blind in the same place — a star seen equator-on, which is exactly where an aligned system sits.
A spread the projection does not hide
A single projected spin–orbit angle says little about the true one, because the star's tilt is unknown. A population of nearly aligned systems is different: for small tilts the projected angle is one component of a two-component vector, so the rms true obliquity is exactly √2 times the rms projected angle — no star's inclination needed.
A transit that runs differently backwards
A star spinning near break-up is brighter at its poles than its equator, so a planet crossing it at an angle covers bright surface on the way in and dim surface on the way out. The light curve stops being symmetric in time, and the part that differs forwards and backwards measures the true spin–orbit angle from photometry alone — on exactly the stars where the line-profile method struggles.
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 effectStellar obliquityProjected obliquityApsidal constantApsidal motionAsteroseismologyDegeneracyEclipsing binaryGeneral relativityGravity darkeningHot jupiterKraft break