Solar eclipse12 August 2026 — Brussels

01 Western horizon

At maximum eclipse, you will have to choose between GENERAL and ARCADES, as both views are photogenic — unless you run and manage to photograph both. Tip: GENERAL at 20:10 and ARCADES at 20:13.
From this location, you will be able to observe most of the eclipse. However, the setting will be more photogenic at CINQUANTENAIRE.
The narrowest viewpoint in the selection does not allow you to observe the eclipse at maximum. However, from 20:30 onwards, the perspective along Rue de la Loi will provide an ideal setting for the solar crescent.
19:18:00Belgian time
0.0%obscuration
02Where to lookfrom the selected viewpointShowHide
A landmark — no instrument needed

03What you will seefollows the sliderShowHide
At the time shown

04How it unfoldsBelgian timeShowHide
19:18It begins. A small notch appears on the Sun’s edge, invisible without eclipse glasses.
19:46Almost half the Sun is bitten away. At ground level, still nothing: your eyes adapt without you noticing.
19:58Two thirds hidden. The light really begins to fade and shadows sharpen.
20:13Maximum. Only a crescent remains. The light may look metallic, the air may feel cooler and some birds may quieten.
20:41More than half is back. The Sun sinks, turns orange and begins to flatten.
20:55Almost whole again and already noticeably oval, low above the rooftops of western Brussels.
21:05The eclipse ends. The Sun is whole again, already noticeably flattened and red.
21:09The Sun sets about four minutes after the eclipse ends.

About one hour and forty-seven minutes in all. No need to arrive at 19:18: the real show begins around 19:55 and does not let up.

05Your eyesread this firstShowHide
Never look at the Sun without protection
  • ISO 12312-2 certified eclipse glasses are essential throughout the eclipse, including when the Sun is low on the horizon. For photography, use a solar filter designed to fit in front of the lens and follow the camera manufacturer’s instructions. Never point an unprotected lens at the Sun.
  • These do not protect you: sunglasses, however dark, smoked glass, X-ray film, CDs, photographic film, stacked filters or a phone screen.
  • Never use binoculars, a spotting scope or a telescope, even while wearing eclipse glasses: the instrument concentrates the light, can damage the filter and cause an immediate serious injury.
  • Check that the lenses are not scratched, punctured or creased. If in doubt, discard them.
  • A retinal burn is painless and may be permanent. There is no warning.
  • Supervise children closely: they may remove the glasses without thinking.

There is a way to watch without wearing anything: make a small hole in one piece of card and, with your back to the Sun, project its image onto another. The full crescent will appear, with no risk to your eyes.

06Worth knowingShowHide

Weather: a light veil of cloud may soften the crescent without preventing observation, but thicker cloud may hide the Sun.

Cooler air: a drop in temperature may be noticeable around maximum; how much will depend on the weather, wind and location.

Shape: as it sinks, the Sun flattens. The atmosphere bends its lower limb more than its upper one, so at the horizon it still measures 31.6 arcminutes across but only 26.3 high. It does not grow: that is an illusion, and it disappears in photographs.

Trees: patches of light on the ground turn into crescents. It is the loveliest detail of the eclipse, and hardly anyone looks for it.

Next eclipse: Belgium will not see one this deep again before 2081. The last was in 1999. This one is worth the trip.

ColophonShowHide

Astronomy: the solar position is calculated on your device using the NOAA/Meeus algorithms, with atmospheric refraction corrected according to Bennett. The local eclipse circumstances come from the Royal Observatory of Belgium and the NASA/GSFC Besselian elements calculated by Fred Espenak.

Obscuration: the crescent’s progression uses a simplified two-disc geometrical model with a diameter ratio of k = 1.03. Relative motion is calibrated separately before and after maximum against the published first- and last-contact times.

Geography and elevation: bearings and distances use spherical geodesy. Coordinates, elevations and landmarks were cross-checked against Geopunt Vlaanderen/DHMV II, topographic-map.com, Google Maps, BruGIS/UrbIS and the Belgian NGI/IGN. Aeronautical data come from skeyes and the Belgian AIP.

Rendering: the apparent flattening of the Sun simulates differential refraction. Disc and sky colours are interpolated from predefined visual values and are not a spectral calculation. The urban skylines are SVG illustrations adapted to the viewing axes.

Credits: concept, art direction, graphic design, research, writing and prompting: Branislav Milić. Development and verification assisted by Anthropic Claude and OpenAI ChatGPT.

v 1.0 · 12 August 2026

© Branislav Milić