Solar radiation pressure — where it appears
Named by 3 essays across one field — each of them below, with the objects they name alongside it.
The orbit that has to be paid for every year
A geostationary satellite is not in equilibrium in any direction. The Sun and Moon tilt its plane by 0.85 degrees a year, the Earth's equatorial ellipticity makes two longitudes stable and two unstable, and the end of a satellite's life is the end of its propellant.
The spin that has to be put somewhere
A spacecraft holding an attitude is not resisting a force. It is absorbing a slow, one-directional trickle of angular momentum from the gradient of gravity across its own body, from sunlight, from the last of the atmosphere — and every store it has for that trickle fills up.
A graveyard height with a term for sunlight
A geostationary satellite at the end of its life is raised about three hundred kilometres and switched off. The height is written as a formula — 235 kilometres plus a thousand times its reflectivity and area-to-mass ratio — and each term is a separate piece of orbital mechanics, the last one sunlight bending the orbit a little every year.
Named alongside it
The objects these essays reach for when they reach for this one.
Geostationary orbitGraveyard orbitStation-keepingAngular momentumArea-to-mass ratioAtmospheric dragAttitude controlDisposal manoeuvreEccentricity vectorEnd of lifeGravity gradient torqueInclination drift