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Synodic Period Calculator

Find how long it takes two orbiting bodies to return to the same relative alignment, from their two orbital periods.

Synodic period
779.91 days
Synodic period (years)
2.135

How it works

A body's orbital (sidereal) period is how long it takes to complete one full lap around whatever it orbits. The synodic period is a different question: how long until two bodies orbiting the same center return to the same position relative to EACH OTHER, as seen from one of them — the time between one 'alignment' (like a planet being at opposition, or two gears' marked teeth meeting again) and the next.

Each body completes 1/T of a lap per day, so the faster one gains on the slower one at a rate of |1/T₁ − 1/T₂| laps per day. It catches up by exactly one full lap — restoring the same relative alignment — once that gap reaches 1, which gives the synodic period Tsyn = 1 / |1/T₁ − 1/T₂|.

The default inputs (365.25 and 686.98 days) are Earth's and Mars's well-known sidereal orbital periods, which work out to a synodic period of roughly 780 days — close to the real-world ~26-month gap between Mars oppositions, the periodic events when Mars, Earth, and the Sun roughly line up and Mars is closest and brightest in Earth's sky.

FAQ

Why is the synodic period longer than either orbital period?

It isn't always longer than both — it's always longer than the shorter of the two periods, since the faster body has to lap the slower one, which takes more than one of the faster body's own orbits whenever the slower body is also moving substantially in the same direction. It approaches the shorter period only in the limit where the other body is nearly stationary (an enormously longer period).

What happens if the two periods are equal?

Two bodies with identical periods never change position relative to each other (their relative alignment is frozen at whatever it started as), so there's no finite synodic period — this calculator flags that case explicitly rather than dividing by zero.

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