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Total Solar Eclipse · August 2, 2027
Total Solar Eclipse 2027: August 2, 2027 — Longest Totality Until 2114
The August 2, 2027 total solar eclipse is one of the most significant astronomical events of the 21st century. With a maximum totality of 6 minutes 23 seconds in southern Egypt near Luxor, and 4 minutes or more of darkness at Gibraltar, Tangier, Oran, Sfax, Benghazi and Jeddah, this is the longest total solar eclipse visible from land until June 3, 2114. This page is your early planning hub — bookmark it for updates as the eclipse approaches.
Solar Viewing Safety Warning
Looking at the Sun without certified solar filters causes permanent, irreversible eye damage — including blindness — within seconds. Telescope Advisor does not manufacture, inspect, or certify any solar viewing product. Before using any solar filter, eclipse glasses, or solar binoculars: read and follow the product manufacturer's instructions completely, verify the ISO 12312-2 certification mark on the product itself, and inspect for scratches, pinholes, or damage before every use. Discard any filter that is damaged. This guide is for informational purposes only and does not constitute safety advice or a product safety guarantee. Choosetoshop LLC accepts no liability for eye injury arising from the use or misuse of any solar viewing product.
Eclipse Overview & Key Facts
The total solar eclipse of August 2, 2027 is the most anticipated eclipse since the Great American Eclipse of 2017 and the European eclipse of 2026. What makes it extraordinary is the duration of totality — the maximum possible length of a total solar eclipse is approximately 7 minutes 31 seconds. The 2027 eclipse reaches 6 minutes 22–23 seconds at its maximum point in southern Egypt, about 60 km southeast of Luxor, and more than 4 minutes across accessible land from Gibraltar eastward. The next eclipse with longer totality visible from land occurs on June 3, 2114, making this a once-in-a-lifetime event for anyone who wants to experience the longest possible darkness.
The path of totality begins in the eastern Atlantic, makes landfall at sunrise around the Strait of Gibraltar, then sweeps east across Morocco, Algeria, Tunisia and Libya before crossing southern Egypt, the Red Sea and Saudi Arabia, and finally ending over Somalia and the Indian Ocean. Confirmed locations inside the path include Cádiz, Málaga, Marbella, Gibraltar, Ceuta, Tangier, Oran, Sfax, Benghazi, Luxor, Jeddah, Mecca and Sana'a. Cities such as Casablanca, Rabat, Algiers, Tunis, Tripoli, Cairo, Alexandria and Medina lie outside the path and will see a deep partial eclipse instead. The eclipse occurs in the late morning in Europe (approximately 11:00-12:00 local time in Spain) and near midday in North Africa. This means the Sun will be high in the sky — unlike the 2026 sunset eclipse — providing excellent viewing conditions with a high altitude above atmospheric turbulence.
2027 Eclipse Fast Facts
Path of Totality
The 2027 eclipse path stretches roughly 15,000 km across the Earth's surface. The centreline begins in the eastern Atlantic and makes its first landfall around the Strait of Gibraltar, then tracks east-southeast across North Africa, southern Egypt and the Arabian Peninsula before ending in the Indian Ocean. The path is at its widest — about 258 km — near greatest eclipse in southern Egypt, where totality also lasts longest at 6 minutes 23 seconds.
Totality Duration by Location
| Location | Totality begins (local) | Duration | Magnitude |
|---|---|---|---|
| Málaga, Spain | 10:48 | 1 min 57 sec | 1.003 |
| Cádiz, Spain | 10:45 | 2 min 56 sec | 1.008 |
| Marbella, Spain | 10:47 | 3 min 21 sec | 1.010 |
| Gibraltar | 10:46 | 4 min 28 sec | 1.022 |
| Ceuta | 10:45 | 4 min 49 sec | 1.030 |
| Tangier, Morocco | 09:45 | 4 min 51 sec | 1.034 |
| Oran, Algeria | 09:51 | 5 min 08 sec | 1.037 |
| Sfax, Tunisia | 10:09 | 5 min 41 sec | 1.032 |
| Jeddah, Saudi Arabia | 13:22 | 5 min 53 sec | 1.026 |
| Benghazi, Libya | 11:28 | 6 min 11 sec | 1.039 |
| Luxor, Egypt | 13:02 | 6 min 22 sec | 1.036 |
Times are local to each site. Sources: NASA eclipse data and the standard eclipse timing tables. Durations change sharply near the path limits — Cádiz sits close to the northern edge and sees under 3 minutes, while Gibraltar, roughly 100 km southeast, sees 4 min 28 sec.
Spain & Gibraltar
For European eclipse chasers, Spain is the most accessible destination for the 2027 eclipse — but it sits on the northern edge of the path, and duration changes dramatically over short distances. Cádiz lies close to that limit and gets just 2 min 56 sec. Málaga, further along the coast, gets only 1 min 57 sec, while Marbella manages 3 min 21 sec. Move 40–60 km south and the numbers transform: Gibraltar gets 4 min 28 sec and Ceuta 4 min 49 sec. Seville is not inside the path of totality — nor is Huelva or inland Andalusia — so check the exact coordinates of any hotel before you book. On this stretch of coast, a short drive south is the difference between a deep partial eclipse and four minutes of darkness.
Unlike the 2026 eclipse (which occurred at sunset low on the horizon), the 2027 eclipse happens in the late morning with the Sun well up — around 38° at Gibraltar and higher as you move east. This makes it dramatically easier to observe and photograph: you do not need a low western horizon, and the higher Sun means a steadier atmosphere for telescopic observation. Southern Spain's infrastructure and airports (Málaga, Jerez, Gibraltar) make it the most convenient European base — provided you stay south of the limit.
North Africa (Morocco, Algeria, Tunisia)
The path of totality crosses North Africa from Morocco through Algeria and Tunisia, offering steadily longer totality than Spain. Morocco is the easiest entry point: Tangier sits inside the path with 4 min 51 sec of totality. The Atlas Mountains provide elevated viewing locations with exceptional atmospheric clarity, though be aware that Rabat and Casablanca lie north of the limit and see a deep partial eclipse rather than totality. In Algeria, Oran is the standout on-path city with 5 min 08 sec; the capital, Algiers, is outside the path at 99.8% partial. Tunisia offers the region's longest run at Sfax — 5 min 41 sec — with the driest, least cloudy stretch of the whole western track lying to its south; Tunis itself is only a partial eclipse. For those willing to travel further, the Sahara south of the coastal cities offers virtually guaranteed clear skies and a uniquely stark landscape.
Weather prospects in North Africa are among the best on the eclipse path. August is the height of the dry season across the Mediterranean coast of North Africa. Coastal stratus pushed inland by the cool Canary Current is the main risk on the Atlantic side, and morning fog lingers most often on the Moroccan and Spanish Atlantic coasts; moving 50–70 km inland usually removes the problem entirely. Inland, satellite records show average August cloud fractions well below 15% for most of the Algerian and Tunisian track.
Libya, Egypt & Saudi Arabia
Egypt & Luxor: the longest totality of the eclipse
Continuing east, the path crosses Libya and then southern Egypt before crossing the Red Sea into Saudi Arabia and ending over Somalia and the Indian Ocean. This is where the eclipse peaks: Benghazi in Libya gets 6 min 11 sec, and Egypt delivers the longest totality anywhere on the path — 6 min 23 sec in the New Valley Governorate, with 6 min 22 sec at Luxor, 6 min 7 sec at Asyut and 5 min 33 sec at Siwa Oasis. Watch the geography carefully: the path crosses southern Egypt, not the Mediterranean coast. Alexandria and Cairo sit well north of the limit, and Cairo will see a 94.8% partial eclipse; the nearest totality from Cairo is a long drive south toward Asyut and Luxor, not north.
Saudi Arabia: Jeddah, Mecca and the Tihamah coast
Across the Red Sea, Saudi Arabia's portion of the path runs along the Tihamah coastal plain: Jeddah gets 5 min 53 sec and Mecca 5 min 10 sec, while Medina further north sees a 94.4% partial eclipse. Dust, rather than cloud, is the main risk on the Arabian Peninsula — the Tihamah Plain has the highest average aerosol load of any part of the track, so budget for a slightly milky sky even on a clear day.
What to Expect: Observing the 2027 Eclipse
Totality runs from under 2 minutes at the Spanish north limit to 6 min 22 sec at Luxor, depending on your location. The 2027 eclipse offers an exceptionally long window to observe and photograph the corona. During totality, the sky darkens dramatically even though the Sun is high — unlike the 2026 sunset eclipse. The brighter stars and planets become visible, the temperature drops noticeably, and the solar corona appears as a pearly white halo extending several solar diameters from the Sun. The extended duration means you will have time to observe the corona with your eyes, through binoculars, and through a telescope, as well as capture multiple camera exposures.
A high Sun is a significant advantage for telescopic observation. Higher altitude means less air and less turbulence between you and the corona, so you can use higher magnification to study streamers, coronal loops, and possibly prominences at the solar limb. A telescope on a GoTo mount can track the Sun automatically throughout the partial phases and totality, making this an excellent opportunity for both visual observation and photography. For telescope and filter recommendations, see our eclipse glasses guide for the partial phases. For telescopes suitable for eclipse viewing, see our best telescopes for beginners guide.
2026 vs 2027: Which Eclipse Should You Choose?
If you are wondering whether to travel for the August 12, 2026 eclipse or wait for 2027, here is a comparison to help you decide:
| Factor | 2026 (Aug 12) | 2027 (Aug 2) |
|---|---|---|
| Land totality duration | ~70 sec (Spain centreline) | 2 min 56 sec (Cádiz) → 6 min 23 sec (Egypt) |
| Sun altitude | 4-7° (very low, challenging) | 38° at Gibraltar, higher eastward (excellent) |
| Weather prospects | Moderate (coastal cloud risk) | Excellent (dry season, high desert) |
| Access from Europe | Easy (Spain, Iceland) | Easy (Spain) / Moderate (N Africa) |
| Photography ease | Challenging (low Sun, short window) | Easy (high Sun, long window) |
| Crowds expected | High (Spain hotspots) | Moderate (many access points) |
| When to book | Now (June 2026) | Now for best options |
Our advice: Do both if you can. The 2026 eclipse is a dramatic sunset event but short and weather-dependent. The 2027 eclipse is a longer, higher-quality observing experience with much better weather odds. If you can only choose one, 2027 offers the better overall experience. If you are in Europe, the 2026 eclipse is closer and requires less travel. For the 2026 eclipse, see our 2026 Europe eclipse hub for full guides.
Eclipse Glasses & Safety Gear for 2027
ISO 12312-2 certified eclipse glasses are essential for observing all partial phases of the 2027 eclipse, both before and after totality. The Sun will be high in the sky and intensely bright, making proper eye protection absolutely mandatory. Never look at the partially eclipsed Sun without certified glasses, even for a moment. Here are our top recommendations for eclipse glasses and solar filters for the 2027 event:
Helioclipse Solar Eclipse Glasses (12-Pack)
The Helioclipse 12-pack is ideal for families and groups planning to travel to Spain or North Africa for the 2027 eclipse. Each pair is individually tested to ISO 12312-2 and CE certified. The included phone filter allows safe smartphone photography of the partial phases, perfect for capturing the approach to totality. With 12 pairs, you can share with travel companions and still have spares.
Affiliate link.
Lunt Solar Eclipse Glasses (5-Pack)
Lunt Solar Systems is a trusted name in solar optics. Their 5-pack is perfect for couples and small groups travelling to the eclipse path. Individually sealed, ISO 12312-2 and CE certified. The wide frame fits comfortably over prescription glasses. Lunt's metallised polymer filter material provides a neutral white solar image that many observers prefer for its natural colour rendition.
Affiliate link.
For those planning to observe through binoculars or a telescope during the partial phases, a front-mounted solar filter is essential. See our complete solar filter guide for SCT telescopes for detailed recommendations on telescope solar filters for the 2027 eclipse. For a full comparison of all certified eclipse glasses, visit our eclipse glasses guide.
Saros 136: The Historical Significance of the 2027 Eclipse
The August 2, 2027 total solar eclipse belongs to Saros series 136, one of the most historically significant eclipse families. Saros 136 has produced some of the most observed and scientifically important eclipses in modern history. Understanding the Saros cycle adds a deeper layer of appreciation for the 2027 event — you are participating in a sequence of eclipses that occurs every 18 years 11 days, a rhythm that ancient Babylonian astronomers recognised over 2,500 years ago.
Saros 136 began on June 14, 1360 with a small partial eclipse near the South Pole. It will produce a total of 71 eclipses over 1,280 years, ending on July 30, 2622. The series is currently near its peak, producing some of the longest totalities in the 21st and 22nd centuries. Notable members of Saros 136 include the eclipse of July 22, 2009 (the longest totality of the 21st century at 6 minutes 39 seconds, visible from Asia and the Pacific) and the eclipse of August 2, 2027 itself. The next major Saros 136 eclipse after 2027 will occur on August 13, 2045, with a maximum totality of approximately 6 minutes 6 seconds over North America. Each successive Saros 136 eclipse shifts approximately 120 degrees westward in longitude, which is why the 2009 event occurred in Asia, the 2027 event in Europe/Africa, and the 2045 event in the Americas.
What makes Saros 136 special for eclipse chasers is that it is currently in its "prime" — the period when the Earth passes closest to the centre of the Moon's shadow, producing the longest durations. This prime period lasts for several centuries, and we are fortunate to be alive during it. The 2027 eclipse is particularly significant because it offers the best combination of long duration and land accessibility for any Saros 136 eclipse in the 21st century. For historical comparison, the members of this series include the May 29, 1919 eclipse used by Arthur Eddington's expedition to test Einstein's general theory of relativity — one of the most consequential eclipse measurements ever made — and the July 22, 2009 eclipse, whose 6 min 39.5 sec maximum was the longest of the 21st century but fell over the remote Pacific. Each Saros 136 eclipse has advanced our understanding of the Sun, and the 2027 event will be no different.
2027 Eclipse vs. The 1991 Eclipse: A Generational Comparison
The July 11, 1991 total solar eclipse was one of the most significant astronomical events of the late 20th century, with a maximum totality of 6 minutes 53 seconds. The path crossed Hawaii, Mexico, Central America, Colombia, and Brazil. For many astronomers and eclipse chasers active today, 1991 was the defining eclipse of their lives. A comparison between 1991 and 2027 reveals fascinating parallels and important differences:
| Factor | 1991 (July 11) | 2027 (August 2) |
|---|---|---|
| Maximum totality | 6 min 53 sec | 6 min 23 sec |
| Land accessibility | Hawaii, Mexico, Colombia | Spain, N Africa, Egypt, Saudi Arabia |
| Sun altitude | ~80° (Hawaii), excellent | High along the whole path |
| Weather prospects | Moderate (Hawaii rain shadow) | Excellent (dry season Mediterranean) |
| Travel from Europe | Long-haul (10+ hours flight) | Short-haul (2-3 hours to Spain) |
| Saros series | Saros 136 (same as 2027) | Saros 136 |
| Digital photography | Film era (limited) | Full digital, smartphone, video |
The 1991 eclipse was the last great eclipse of the film photography era. Observers in Hawaii captured some of the most iconic eclipse images ever taken, using Kodachrome and Fujichrome film that required careful metering and bracketing. The 2027 eclipse, by contrast, occurs in an era of digital cameras, smartphone astrophotography, and live streaming. The technological context is one of the most striking differences — in 1991, few people had access to auto-guiding telescopes or real-time image processing. Today, affordable GoTo mounts, planetary cameras, and stacking software put professional-quality eclipse photography within reach of amateur astronomers. For tips on capturing the 2027 eclipse, see our eclipse travel and photography guide.
2027 Eclipse Weather Analysis: Where to Go for Clear Skies
Weather is the single biggest variable in eclipse observing, and the 2027 eclipse benefits from occurring during the height of the dry season across almost its entire land path. Unlike the 2026 eclipse (which occurs at sunset with low-altitude cloud risks), the 2027 eclipse takes place in the late morning with the Sun high in the sky, giving you a shorter atmospheric path and less susceptibility to horizon cloud. Here is a detailed weather analysis for each major region along the path of totality, based on historical satellite data from the European Centre for Medium-Range Weather Forecasts (ECMWF) and national meteorological agencies:
Southern Spain (Cádiz, Marbella, Gibraltar)
Spain's eclipse weather is good, but the geometry is unforgiving: the northern limit of totality runs just north of Cádiz, so the on-path strip is narrow. The dominant risk is marine stratus pushed in by the cool Canary Current, which forms overnight and usually burns off through the morning. Cádiz recorded sun-visible conditions on 88% of survey days, Gibraltar around 74% — a figure that understates the reality, because the cloud there is often patchy and a short move finds clear sky. The Atlantic cloud rarely penetrates east of Tarifa, so Marbella and the Alboran coast do better. Inland Andalusian sites average under 15% cloud, but check the path limit first: inland Spain is often outside totality. Also watch for calima — suspended Saharan dust that leaves a hazy sky on otherwise clear days.
Morocco (Tangier and the north coast)
Morocco's on-path cities are all in the north — Tangier, Ceuta and the Rif coast — where the main risk is the same marine stratus and coastal fog that affects Atlantic Spain, often lifting into a stratus layer through the morning. Tangier is partly sheltered by the terrain of the Tangier Peninsula, so its sunrises are frequently misty rather than overcast, but the eclipse there begins at 09:44 local time and the fog does not always clear in time. The reliable strategy is to move 50–70 km inland, where fog influence is negligible: the eastern side of Tangier, Tetouan and the inland Rif are far less affected than the coast between Asilah and Larache, which is the most cloud-prone stretch on this part of the track.
Algeria, Tunisia & Libya
The inland Algerian and Tunisian track — running through Oran, M'sila, Kasserine and Sfax — has some of the best weather prospects on the entire eclipse path. August is the peak of the dry season, and satellite records show morning cloud fractions well under 15% along most of this stretch, with the lowest values in the country south of Sfax. The principal hazards here are not cloud but dust and sand: the high plateau between the Tell Atlas and the Saharan Atlas, and the Sahara itself, are the main source regions, and the sirocco can lift a widespread haze. Inland sites 50–100 km from the coast remain the most reliable choice.
Libya, Egypt & Saudi Arabia
This is the clearest part of the track. Over Libya and western Egypt, satellite records show August cloud almost unknown — some stretches have seen no August cloud on eclipse day at all in the past 23 years. Benghazi and the Egyptian desert are the standout picks; Siwa Oasis and Bahariya Oasis combine almost no cloud prospect with relative immunity to dust storms, and Benghazi performs nearly as well. Further east the picture changes: cloud rises sharply across the Red Sea toward Jeddah, and on the Saudi Tihamah plain dust rather than cloud is the limiting factor — the highest average aerosol load anywhere on the track, so expect a somewhat milky sky. Heat is the other real constraint: Luxor averages 42°C on August 2, so plan shade, water, and camera cooling.
FAQ — 2027 Total Solar Eclipse
When is the next total solar eclipse after 2026?
How long will totality last for the 2027 eclipse?
Where is the best place to see the 2027 eclipse?
Do I need special glasses for the 2027 eclipse?
When should I book travel for the 2027 eclipse?
Sources & Verification
Path geometry, totality durations and local timings on this page come from NASA's eclipse data and the standard city-by-city eclipse timing tables, cross-checked against Xavier Jubier's path maps. The weather and dust guidance is drawn from Jay Anderson's August cloud climatology for this eclipse track.
- NASA Eclipse Web Site — greatest eclipse 10:07:50 UTC, maximum totality 383 s (6 min 23 s), path width 258 km
- City-by-city eclipse timing tables — local totality times and durations for every location listed above
- Eclipsophile — Total Solar Eclipse 2027 — August cloud climatology and dust analysis along the track
- timeanddate.com — Solar Eclipse, August 2 2027 — path map and local circumstances
Figures verified September 2026. Path and timing data are fixed by orbital mechanics; local timing and weather guidance will be refreshed as the event approaches.