An Earth sensor (horizon sensor) finds the direction of Earth's centre by detecting the planet's warm infrared limb against cold space. For decades the standard nadir reference on Earth-pointing satellites, it now shares the role with star trackers and GNSS-derived attitude.
Understanding Earth Sensor
Scanning cones and staring arrays
The classic scanner spins a mirror so its narrow field traces a cone intersecting the horizon at two crossings per revolution; crossing timings encode pitch and roll — a mechanism refined over thousands of flight units. Static sensors replaced motion with arrays of thermopiles imaging the entire limb simultaneously, trading scan precision for reliability. Both must model the atmosphere: the "infrared horizon" sits tens of kilometres above the solid surface and breathes with latitude and season, the dominant error source at the 0.05° level.
A sensor's place in history
Horizon sensing is as old as orbital flight — early crewed capsules used it for retrofire alignment, and every generation of communications satellite carried refinements. Its story is the arc of spaceflight sensing: dedicated single-purpose physics giving way to computed references from more general instruments, while never quite disappearing, because pointing at the planet you circle is a problem best solved by looking at it.