Next total solar eclipse: dates and where to go
The next is 12 August 2026 across Iceland and Spain. Totality is not a better partial eclipse — it is a different event.
5 min read · Published 24 August 2026
The short answer
The next total solar eclipses are 12 August 2026 across Iceland and northern Spain, 2 August 2027 across North Africa with over six minutes of totality, 22 July 2028 across Australia and New Zealand, then 25 November 2030, 14 November 2031 and 30 March 2033. You must be inside the narrow path of totality — a 99% partial eclipse is not remotely the same experience, and this is the single most misunderstood thing about eclipses.
Total solar eclipses to 2033
| Date | Broad path |
|---|---|
| 12 August 2026 | Greenland, Iceland, northern Spain |
| 2 August 2027 | Southern Spain, North Africa, Arabian peninsula |
| 22 July 2028 | Australia, New Zealand |
| 25 November 2030 | Southern Africa, Australia |
| 14 November 2031 | Pacific, Panama |
| 30 March 2033 | Alaska, Arctic |
The 2 August 2027 eclipse is the standout. Its totality exceeds six minutes near the centre line, among the longest of the century over land, and the path passes close to Luxor in Egypt where August skies are reliably clear. Accommodation along that path books years ahead.
The 2026 and 2027 events are covered in more detail in the 2026 and 2027 calendars, both computed from the same ephemeris.
Why 99% is not close enough
This is the point everyone underestimates until they have seen one.
At 99% partial coverage the sky is still bright, the temperature has barely changed, and you need eye protection throughout. It is interesting.
At 100% — totality — the Sun's disc is completely covered. The corona becomes visible, a pearly white structure extending out several solar diameters. Bright stars and planets appear. The temperature drops noticeably. Birds behave as though it is dusk. A 360-degree twilight glow sits on every horizon. And for those minutes only, you can and should look directly at it with no filter.
The difference is not one percent more of the same thing. The remaining sliver of photosphere is still roughly ten thousand times brighter than the corona, so until it is gone you see none of what makes totality extraordinary.
Planning one
In order of importance
- Get inside the path of totality, ideally near the centre line where duration is longest.
- Check historical cloud statistics, not forecasts — you are booking a year or more out. Eclipse climatology data exists for every path and it is the single best predictor.
- Book early. For a well-placed eclipse, accommodation along the path fills two years ahead and prices rise sharply.
- Plan to be mobile on the day. Experienced chasers keep a car and a weather forecast and move if cloud threatens. A fixed booking with no mobility is a gamble.
- Arrive the day before. Eclipse-day traffic on small roads is notorious, and missing totality by twenty minutes in a queue is a real and common failure.
- Bring certified eclipse glasses for the partial phases, and know precisely when totality starts and ends — see how to view the Sun safely.
Why eclipses are not more frequent
The Moon orbits Earth roughly every month, so you might expect a solar eclipse every month. The reason you do not is that the Moon's orbit is tilted about five degrees to the ecliptic.
Most new Moons therefore pass above or below the Sun from our viewpoint. An eclipse needs a new Moon occurring near one of the two nodes where the Moon's orbit crosses the ecliptic — the points Vedic astrology calls Rahu and Ketu, which is not a coincidence, since that tradition named them for exactly this behaviour.
Globally there are two to five solar eclipses a year, of which only some are total. Any given location sees a total eclipse on average roughly once every 375 years, which is why travelling to them is normal.
The coincidence that makes them possible
The Sun is about 400 times wider than the Moon and about 400 times further away, so the two appear almost exactly the same size in our sky. That is what allows the Moon to cover the Sun's disc precisely enough to reveal the corona.
There is no physical reason for this and, as far as we know, nowhere else in the solar system has anything like it. It is also temporary: the Moon recedes from Earth by around 3.8 centimetres a year, and in a few hundred million years it will be too small in our sky to produce total eclipses at all.
We happen to exist during the window when they are possible, which is a genuinely striking thing about the era we live in.
Common questions
- When is the next total solar eclipse?
- 12 August 2026, with a path crossing Greenland, Iceland and northern Spain. It is followed by 2 August 2027 across North Africa, 22 July 2028 across Australia and New Zealand, then 2030, 2031 and 2033.
- Is a 99% partial eclipse nearly as good as totality?
- No. The remaining sliver of the Sun's surface is roughly ten thousand times brighter than the corona, so at 99% the sky stays bright, the corona is invisible and eye protection is still required throughout. Totality is a categorically different event.
- Why are total solar eclipses so rare from any one place?
- The Moon's orbit is tilted about five degrees to the ecliptic, so most new Moons pass above or below the Sun. Eclipses require a new Moon near a lunar node, and the path of totality is narrow — any given location averages one roughly every 375 years.
- Will total solar eclipses always happen?
- No. The Moon recedes from Earth by around 3.8 centimetres a year, and in a few hundred million years it will appear too small to cover the Sun's disc entirely. Total eclipses are a feature of the era we happen to live in.