☄️ Meteor showers — and how they fare from here

What they really are, when to look, and why Singapore's equator changes the game. Science Centre Observatory, Jurong.

The next shower

Working it out…

What is a meteor shower?

A comet (or a crumbling asteroid) leaves a trail of grit strung along its orbit. Once or twice each year the Earth ploughs through one of these trails — on the same dates every year, because we cross the same point in our orbit — and for a few nights the sky fills with "shooting stars."

Almost every one is tiny: a grain of sand to a pea, hitting the air at up to 70 km per second and burning up in a streak about 100 km overhead. Nothing reaches the ground. The dust is old — the Orionids and Eta Aquariids are both debris shed by Halley's Comet on passes centuries ago.

💡 A "meteoroid" is the grain in space; the "meteor" is the streak of light; a "meteorite" is the rare survivor that lands. Shower meteors essentially never become meteorites — they are far too small.

Why they seem to come from one point — the "radiant"

All the grains in a trail move in parallel. But perspective makes parallel lines appear to spread from a single vanishing point — like railway tracks converging in the distance, or snow rushing at a car's windscreen. That point is the shower's radiant, and it's how showers get their names: the Perseids radiate from Perseus, the Geminids from Gemini.

You don't look at the radiant — meteors near it are foreshortened to short streaks. Look about two-thirds of the way up, 40–60° to the side of it, where they flare longest. Trace any meteor backwards: if the line hits the radiant, it belongs to the shower; if not, it's a random "sporadic."

Why after midnight is better

Before midnight you're on the trailing side of the Earth — meteors have to catch up to you. After midnight you rotate onto the leading side, driving head-on into the stream, so you sweep up more of them and they arrive faster and brighter. The pre-dawn hours are almost always the best, and the radiant is usually higher then too.

💡 The quoted rate — the ZHR, or Zenithal Hourly Rate — is an ideal: what one observer would see under a perfectly dark sky with the radiant straight overhead. Real life is always less. Two things cut it most: a bright Moon, and a low radiant — which is where Singapore comes in.

Singapore's twist: some showers win, some lose

The number you actually see falls off with the radiant's height — roughly as its sine. A radiant sitting at 30° up delivers about half its overhead rate; at 15°, only a quarter. From our near-equatorial latitude, far-northern radiants stay low — so the world-famous Perseids and Quadrantids underperform here, and the Ursids barely clear the horizon.

But the equator has its reward: the showers whose radiants ride high in our pre-dawn sky. The Orionids and Delta Aquariids climb to around 70° here; the Geminids — the year's richest — ride high too; and even the Eta Aquariids (Halley's other shower), still rising as dawn breaks, are seen far better from our low latitude than from Europe or North America. Here's how the year's showers actually fare in Singapore's small hours — soonest first:

ShowerPeakRateWhere to look (pre-dawn)

How to watch — no telescope needed

Peak dates and Zenithal Hourly Rates are standard almanac values (exact peaks shift a little year to year); the radiant height, "from SCOB" rating and the next-shower panel are computed on your device for the observatory (radiant transit altitude = 90° − |latitude − declination|, rate falling with the sine of altitude). Deeper data: International Meteor Organization · American Meteor Society · NASA — meteors.
Companion pages: this month's showers · why Singapore sees almost the whole sky · why the city sky is bright.
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