🌌 Milky Way & Astro

How to photograph a meteor shower

Diagram: meteors trace back to a single radiant point, with streak length growing farther from it

A meteor shower isn't a lucky night of shooting stars — it's Earth ploughing through a comet's leftover dust on a predictable date, from a predictable direction. Know the radiant and the settings, and the only thing left to luck is the sky staying clear.

Every year, Earth’s orbit carries it through the trail of dust a comet left behind on a past pass. Those grains hit the atmosphere at tens of kilometres a second and burn up as streaks of light — a meteor shower. Because the trail sits in a fixed part of Earth’s orbit, the shower peaks on close to the same calendar date every year: the Perseids in mid-August, the Geminids in mid-December, and a handful of smaller showers in between.

The radiant: where meteors come from, not where to point

Every shower has a radiant — the point in the sky the meteors appear to streak away from, named after the constellation it sits in (the Perseids radiate from Perseus, the Geminids from Gemini). It’s a perspective effect, the same reason motorway lane-markings seem to explode outward from a point ahead of you as you drive.

Meteors can appear anywhere in the sky, not just near the radiant — in fact the best shots often aren’t there at all. A meteor close to the radiant is foreshortened and looks short; the farther a meteor is from the radiant, the longer and more dramatic its streak. The practical takeaway: frame the radiant somewhere in your shot (so the shower reads as that shower), but off to one side, not dead centre — that gives the streaks room to run long across the rest of the frame.

When to shoot: peak night, dark hours, no moon

Three things have to line up:

  • The peak night. Rates spike sharply around the shower’s peak and fall off within a day or two either side — check the date for this year’s pass, not last year’s.
  • After midnight, usually. For most showers Earth’s night side is turning into the debris stream as the night goes on, so rates climb toward dawn. Plan for the pre-dawn hours, not just after sunset.
  • A dark, moonless sky. A bright moon washes out all but the brightest meteors the same way it washes out the Milky Way — see finding dark skies. Check the moon phase and moonset time before committing to a night.

Shower strength is quoted as ZHR — zenithal hourly rate, the count a single observer would see under a perfectly dark sky with the radiant directly overhead. Real counts from a real horizon, with some light pollution and the radiant lower in the sky, run well below the quoted ZHR — don’t plan around the headline number.

Settings and technique

Shoot wide (14–24 mm) to cover as much sky as possible — you can’t predict exactly where the next meteor will streak, so a wide frame catches more of them. Use the widest aperture your lens has (f/1.4–f/2.8), and keep the shutter at the NPF-rule limit for your focal length so the background stars stay points, not trails, over the sequence.

Then just keep shooting: fire continuous NPF-length frames back-to-back with an intervalometer for the whole dark window, and sort the keepers afterward. A meteor shower isn’t a one-shot event — it’s a long exposure of attempts, and most of your frames will show nothing at all. That’s normal.

Gear

A sturdy tripod, a wide fast lens, and an intervalometer (or your camera’s built-in interval timer) to keep firing frames unattended through the cold hours. Bring a spare battery — hours of continuous shooting drains one fast in cold air.