It’s time again for Perseid meteors!

editorAstronomy Now3 days ago10 Views

August means the Perseids: the annual shooting star spectacular reaches its peak to wow meteor enthusiasts with abundant bright events, writes Astronomy Now’s Night Sky manager Mark Armstrong.

A stunning night sky composite photograph shows dozens of bright Perseid meteors streaking across the sky above a rural landscape, with the Milky Way arching overhead. The foreground features trees, a house, and softly lit structures, creating a serene countryside scene.
The Perseid meteor shower peaks on 12/13 August. This amazing image is a composite image of the radiant of the 2023 Perseid shower captured over four consecutive nights. Image: Miguel Claro.

Down the decades, the Perseid meteor shower has become a firm favourite on the observing calendar, with astronomical groups gearing up to make the most of the perennial display of shooting stars. The big meteor showers are among the most popular events for astro-friends to come together, hoping to see meteor-a-minute rates, whether you are in it for the science or just to have some fun.

The Perseids are renowned for producing bright events, interspersed by an occasional thrilling fireball to lift flagging spirits in the small hours. This characteristic of the Perseids will help for this month’s show, as glare from a pesky Moon, in a waning gibbous phase just three to four days past full, will drown out many of the fainter meteors.

What are meteors?

A panoramic night sky photo shows a person sitting on a rocky outcrop overlooking a river and forest, with the Milky Way stretching across the sky and numerous meteors streaking across the sky.
This superb composite image of the 2020 Perseid meteor shower over Seč Island in the Pardubice Region of the Czech Republic. A BCF modified Canon 6D camera and a Samyang 12mm, f/2.8 lens shot 30-second exposures for the meteors, while a Samyang 24mm, f2.2 lens handled the foreground panorama. Image: Petr Horálek.

Our late and much missed colleague Neil Bone was for many years the director of the British Astronomical Association’s Meteor section. Here’s his take on where meteors come from: “Meteors are the short-lived (one- to two-tenths of a second) streaks of light seen in the night sky as ‘shooting stars’. They occur, typically, in a layer of atmosphere between 80–100 kilometres altitude where small incoming particles – meteoroids – are destroyed, essentially by frictional heating, on their high-velocity (11–76km/s) entry. Most meteoroids are small, perhaps just 2–5mm in diameter for those producing meteors in the naked eye range, and are of very low density.”

Perseids linked to Comet 109P/Swift–Tuttle
When comets wing their way through the inner Solar System, their surfaces are heated by the Sun and they become more active. Some cometary material is lost and particles ejected, which over time spread out around along the comet’s orbit around the Sun. When Earth intersects this stream of particles then a number of them enter our upper atmosphere, vaporising to form the streaks of light we see as meteors.

Each meteor shower is linked with a ‘parent comet’, with periodic comet 109P/Swift–Tuttle being associated with the Perseids. This comet has a 133-year period and last returned to the inner Solar System in 1992. Enhanced Perseid rates were seen in the early nineties, which corresponded with this return.

When and where to look
Perseid activity is normally confined between 17 July and 24 August, with this year’s peak expected at about 20:00 UT on 12 August. Your best chance to see meteors is on the nights of 11/12 and 12/13 August, and you should be prepared to stay up past midnight into and past the small hours, if at all possible.

The shooting stars belonging to the shower (i.e, not sporadic or random meteors, which occur frequently every night) can be traced back to an area of sky called the radiant. This position reflects the intersection between Earth’s orbit and that of the meteoroid stream.

A star map showing the constellation Perseus with the labeled star Mirfak and a marked area labeled "Radiant," where meteor trails appear to originate. The meteor trails radiate outward from the radiant point near the Perseus constellation on a dark night sky background.
The Perseid radiant lies in northern Perseus. AN graphic by Greg Smye-Rumsby.

The Perseid radiant lies in the far north of Perseus (around 4° of the magnificent Double Cluster near magnitude +4.6 eta Persei), a location close to the boundary with Cassiopeia. This area of sky is circumpolar (never setting) from the UK, but lies low in the north-eastern sky as darkness falls. Although the radiant is now around 25 degrees up from London at 10pm BST, that’s still quite close to the north-northeastern horizon. Those Perseids bursting out 20° or more below the radiant will be hard to spot or be missed entirely below the horizon.

A bright Perseid streaks across a starry sky.
A bright Perseid streaks across the sky. Image: Alan Tough.

The radiant climbs to a decent altitude of 50 degrees or so by 2am BST, when the areas of the sky from where Perseids are more likely to appear will be much better placed than prior to midnight.

Do not peer intently at the spot in the sky where the radiant lies, though this may seem counter-intuitive. Perseid meteor trails or streaks here will appear short and therefore harder to see. You will see many more shooting stars if you observe an area of sky 30-40 degrees from the radiant (from where, meteor streaks may appear longer) and around 50 degrees above the horizon.

What can I expect to see?

Under a haze-free sky at a dark-sky viewing site on a moon-free year, observers can expect to see between 50 and 70 Perseid meteors each hour near the peak. In towns or cities, observed rates may still be around ten per hour in the early-morning hours when the radiant is high. Owing to glare from the Moon, observed rates of fainter Perseids will be curtailed.

Good luck!

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