55P/Tempel-Tuttle

A Halley-type comet that goes round the Sun every 33 years, at perihelion about May 2031

Not in reach from Georgetown on this return: it is forecast too faint or too low.

Can I see 55P/Tempel-Tuttle from Guyana?

Not in reach from Georgetown on this return: it is forecast too faint or too low.

Tonight it does not climb 10 degrees above the horizon while the sky is dark from Georgetown.

From Lethem, under a dark interior sky: Not in reach from Lethem on this return: it is forecast too faint or too low.

How bright is 55P/Tempel-Tuttle, and how sure is that?

Nobody has reported its brightness to COBS in the last 30 days, so every number here is a forecast.

No one has followed this comet through a return like this one, so the forecast is a catalogue estimate with a wide range.

A comet's light is spread over a fuzzy patch, so it is harder to see than a star of the same magnitude. That is why the gear rungs ask for a magnitude in hand.

The orbit of 55P/Tempel-Tuttle

55P/Tempel-Tuttle passes closest to the Sun (perihelion) about 22 May 2031, at 0.976 au, where 1 au is the Earth's distance from the Sun. One orbit takes 33 years. The orbit is tilted 162.5 degrees to the Earth's and its eccentricity is 0.9055 (0 is a circle, 1 an open curve).

Orbit: NASA/JPL Horizons osculating elements, solution JPL#J985/69, retrieved 8 October 2026. Positions on this page are computed from them in your browser and agree with JPL's own tables to half an arcminute.

About 55P/Tempel-Tuttle

The parent of the Leonid meteors of November, on a 33-year orbit.

55P/Tempel-Tuttle is a Halley-type comet that goes round the Sun every 33 years. The "P" in 55P marks a periodic comet, and the number is the order in which its return was first confirmed.

Its dust is the source of the Leonids meteors: each year the Earth crosses the trail it has left along its orbit.

How we know

Orbits: NASA/JPL Horizons (Giorgini, JD and the JPL Solar System Dynamics Group), data retrieved 2026-10-08.

Catalogue brightness laws: JPL Small-Body Database and the IAU Minor Planet Center.

Observed brightness: COBS Comet Observation Database (https://cobs.si) and its contributing observers, CC BY-NC-SA 4.0.

Data updated 8 October 2026. "Early forecast" means: A catalogue estimate. Early predictions are often wrong in both directions.

Gear rungs and ranges are estimates for a typical observer: your eyes, your sky and the night will differ.

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