How to watch the 12 August 2026 eclipse in the UK
On the evening of Wednesday 12 August 2026, the Moon will cover between 89.6% and 96.4% of the Sun as seen from the United Kingdom — the deepest partial solar eclipse the country has had since 1999, which is how the Royal Observatory Greenwich puts it too. This guide covers the three things that actually matter: protecting your eyes, knowing the timings, and — the part almost every article skips — standing somewhere you can physically see it from.
1. Eye safety, in plain English
This is the section that is not optional. Because no part of the UK is inside the path of totality, there is no moment during this eclipse — none at all — when it is safe to look at the Sun with unprotected eyes. Not at maximum, not at 96.4%, not "just for a second". The Sun does not hurt while it is damaging you: the retina has no pain receptors, so solar retinopathy is painless while it happens and shows up hours later as a blurred or blind patch in the centre of your vision. It can be permanent.
What works: eclipse glasses or a handheld solar viewer carrying the EN ISO 12312-2 marking (often printed as ISO 12312-2:2015) on the frame. They look absurdly dark — through a proper pair, indoors, you should see essentially nothing except a bright lamp filament. Before eclipse day, hold them up to a bright light and check for scratches, pinholes or creases in the filter; if you find any, throw them away rather than risk it. Our guide to certified eclipse glasses explains how to read the markings in two minutes, and the American Astronomical Society maintains an independent, non-commercial list of suppliers and filters that have actually been tested at eclipse.aas.org.
What does not work, ever: sunglasses of any darkness, several pairs of sunglasses stacked, smoked glass, exposed photographic film, CDs, mylar crisp packets, welding glass below shade 14, or looking at the reflection in water. Nor does a phone screen: pointing a camera at the Sun risks the sensor and, worse, tempts you to line up the shot by eye.
Optics are a special case and a serious one. Binoculars, a telescope or a camera telephoto concentrate sunlight enormously; eclipse glasses held behind an eyepiece will melt or crack in seconds. Any filter must be fitted in front of the objective lens, securely enough that it cannot be knocked off, and rated for solar viewing.
The genuinely safe, genuinely fun alternative needs no equipment: pinhole projection. Punch a small hole in a sheet of card, hold it up with your back to the Sun, and let the light fall on a second sheet — you get a small, sharp image of the eclipsed Sun. A kitchen colander projects dozens at once. So do the gaps between the leaves of a tree, which is why, near maximum, the shadow under a tree fills with hundreds of little crescents. That is worth photographing even more than the Sun itself.
With children, the practical rule that works is that the glasses go on before anyone looks up and come off only when everyone is looking down at the projection screen. Twenty seconds of unsupervised curiosity is all it takes.
2. The low Sun: the decision that matters most
Here is the piece of advice that is worth more than any equipment you could buy for this eclipse. Across our whole UK dataset, the Sun's altitude at maximum is between 9.4° and 15.9°. Ten degrees is roughly the width of your closed fist held out at arm's length. That is how far above the horizon the entire spectacle will be happening.
The consequence is blunt: a row of houses, a line of poplars, a gentle ridge or a bank of low cloud sitting on the western horizon will hide the eclipse completely, even under a perfectly clear sky overhead. In a city, a street that runs east–west is worth more than a park hemmed in by buildings. On the coast, a west-facing beach or headland is close to ideal. Inland, height helps: any hill, embankment or upper floor that buys you an open view low down to the west-north-west — where the Sun always sits on an August evening in Britain — is the whole game.
The flip side is that a low Sun is beautiful. You will be looking at a crescent Sun through the thick, hazy air near the horizon, tinted amber, with landscape or sea in the same frame. It is a far better photograph than an eclipse high in a blank sky — provided you can see it at all.
Sun altitude varies a little around the country: Belfast gets the Sun 14.9° up at maximum, London only 10.3°. Your own town's figure is on its page — the full ranking lists all 220 of them.
3. The evening step by step
The timings below are London's, computed for the capital's coordinates: first contact 18:17, maximum 19:13, last contact 20:06 — a whole event of about 1 h 49 min. They happen to match the times the Royal Observatory Greenwich publishes for London to the minute, which is a reassuring external check on this dataset. Elsewhere in the UK everything shifts by a few minutes: maximum runs from 19:03 in the north-east to 19:16 in the far south-west. All times are British Summer Time (BST, UTC+1) — the clock time everywhere in the UK on 12 August 2026.
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Around 17:32 — get into position
Arrive early enough to find the viewpoint, not the parking space. Check what is on your western skyline while the Sun is still comfortably above it, and move if a building is in the way. Glasses out of the bag and checked now, not in the dark.
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18:17 — first contact
The Moon touches the western edge of the Sun's disc. Through the filter you will see a tiny notch appear; with the naked eye, absolutely nothing. Nothing about the daylight changes for the next half hour.
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Around 18:47 — the bite becomes obvious
Roughly half the disc is gone. Still no visible change in the light: this is the stage at which people who have not been told about the eclipse genuinely do not notice it. Set up your pinhole projection now — the crescents are already clear on a white sheet.
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19:02 onwards — the light starts to change
In the last ten to fifteen minutes before maximum the difference becomes real: the light flattens, shadows sharpen because the Sun is reduced to a thin arc rather than a disc, colours cool, and the temperature drops a degree or two. Look at the tree shadows, not just at the Sun.
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19:13 — maximum eclipse in London
91.4% of the Sun's area is covered — a thin crescent through the filter, low over the western horizon. It will feel like a strange, slightly wrong late afternoon rather than night. Nowhere in the UK does the sky go dark: even the deepest place in the country, Hugh Town in the far south-west, still leaves 3.6% of the Sun's face shining.
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20:06 — last contact
The Moon clears the disc and the eclipse is over, with the Sun still just above the horizon from London. Keep the glasses on right to this point; the last few per cent are exactly as dangerous as the first.
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Later that night — a bonus
The same night falls in the middle of the Perseid meteor shower. If you have driven somewhere dark for the eclipse, it is worth staying.
| City | Nation | First contact | Maximum | Ends | Sun covered | Sun height |
|---|---|---|---|---|---|---|
| London | England | 18:17 | 19:13 | 20:06 | 91.4% | 10.3° |
| Edinburgh | Scotland | 18:08 | 19:05 | 20:00 | 90.7% | 13.9° |
| Cardiff | Wales | 18:17 | 19:13 | 20:07 | 93.2% | 12.1° |
| Belfast | Northern Ireland | 18:10 | 19:08 | 20:03 | 93.1% | 14.9° |
4. What you will — and will not — see
Honesty is more useful than hype here, because the gap between a deep partial eclipse and a total one is the single most misunderstood thing about eclipses. At 91.4% or even 96.4%, the Sun is still an unbelievably bright object. Human vision is logarithmic and compensates almost perfectly, so the world does not get "90% darker" — it gets a bit flat, a bit cold, a bit odd. Above 94% — which in this dataset means the far south-west only — the effect crosses into genuinely strange: a metallic, colourless quality to the light that people remember for years.
What will not happen anywhere in the UK: the corona will not appear, stars and planets will not come out, the horizon will not glow 360 degrees, birds will not roost, and there will be no moment when the glasses come off. All of those belong to totality, and totality is an all-or-nothing phenomenon — 99% of the way there is still nothing like it.
What will happen, and is worth setting up for: the crescent shadows under trees, the sharpening of shadows as the Sun narrows into a line source, a real drop in temperature, and a low amber crescent Sun that photographs beautifully against a landscape. Take a proper look through the filter every few minutes rather than staring — the change over an hour and a half is the story.
5. Cloud, forecasts and a plan B
We will not pretend to know what the British weather will do in mid-August. Nobody can forecast a specific evening months ahead, and pages that publish tidy "chance of clear sky" percentages for individual UK towns are dressing up climatology as prediction. The useful advice is procedural: check the Met Office forecast in the last three or four days, and pay particular attention to low cloud and haze rather than overall cover, because with the Sun 9.4–15.9° up, a band of cloud sitting on the horizon is fatal even under blue sky.
Have a second viewpoint in mind that faces a different stretch of horizon, ideally an hour or so away, and be willing to move. And if it is comprehensively clouded out, the Royal Observatory Greenwich will be live-streaming the eclipse with commentary — not the same thing, but better than nothing.
6. The trip that changes the whole thing
If there is one recommendation in this guide worth acting on, it is this one: if you can get inside the path of totality, go. Not because the UK view is bad — it is the best this country has had in over twenty-five years — but because the two experiences are not on the same scale. Totality is the difference between hearing about a thing and being under it.
Two destinations are realistically within reach for a British traveller on the same evening, and the figures below come from the same computation as everything else on this site:
- Iceland — the star recommendation. Roughly a two to three hour flight, and uniquely for this eclipse the capital itself is inside the path: Reykjavík gets 1m 02s of totality at 17:48 local time with the Sun 24.5° above the horizon. That last figure is the point: no horizon problem, no scramble for a west-facing hill — the eclipse happens comfortably up in the sky, which neither the UK nor Spain can offer. Everything we have on Iceland →
- Northern Spain — the long path. This eclipse crosses Spain from Galicia to the Balearics and gives the longest run of totality over inhabited land. From London the nearest point in the path is Noja ( Cantabria), about 928 km away, with 0m 51s of totality; further along the path the durations get longer. Be aware that Spain's eclipse is also a low-Sun, near-sunset one, so the horizon advice above applies there as well. Our full English coverage of Spain →
If you are staying at home instead — which most people will, and quite reasonably — then the guide above is genuinely all you need: a certified filter, an open western horizon, and a clear evening. Find your own town's exact times on the UK ranking or the map.
Circumstances computed for the coordinates of each locality with JPL DE440s ephemerides, the same pipeline that powers the Spanish and Icelandic pages on this site. All times are British Summer Time (UTC+1).