← All detection methods · Exoplanet Archive
Two stars eclipse each other on a clock, and a planet nudges the clock.
In an eclipsing binary, two stars pass in front of one another on a strict schedule — a natural clock, often good to seconds.
A planet orbiting the pair from outside moves the whole binary around their common centre of mass. When the binary is displaced toward us the eclipse light arrives fractionally early; when displaced away, fractionally late.
The measurement is therefore of light travel time across the binary's own small orbit, and the drift repeats with the planet's period.
This is the shakiest method in the catalogue. Binaries have their own reasons for drifting — magnetic cycles in the stars change their shape and their orbit — and several announced planets were later withdrawn once longer baselines showed a non-planetary pattern.
Seventeen planets in the catalogue rest on this, and it is fair to say some remain debated.
| Landmark discovery | NN Serpentis b and c — a much-studied and long-debated case. |
| Instruments | Ground-based long-term photometry, amateur networks included |
| Archive name | Eclipse Timing Variations — the value in NASA's discoverymethod field |