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MONDAY, AUGUST 2, 2027 · TOTAL SOLAR ECLIPSE
Total Solar Eclipse of August 2, 2027: Where, When and How to Watch It Live
On August 2, 2027 the Moon’s shadow crosses the Strait of Gibraltar, runs the length of North Africa, passes over Luxor and the Red Sea, and leaves Earth in the Indian Ocean. Near Luxor totality lasts 6 min 23.2 s by NASA’s figures, with the Sun almost overhead. Below: the path drawn from NASA’s own table, totality times for 17 cities, a countdown in your time zone, and how to watch safely, in person or live online.
The eclipse begins on Monday, August 2, 2027 at 07:30:11 UTC, and totality reaches Spain at about 08:45:21 UTC.
The eclipse at a glance
Date
Monday, August 2, 2027
Longest totality
6 min 23.2 s, at 26°49′N 31°08′E in Egypt (NASA)
Greatest eclipse
10:06:37 UTC at 25°30.3′N 33°11.0′E, Sun 81.7° high (NASA)
Path width
About 258 km (160 miles) at greatest eclipse
Totality in
Spain, Gibraltar, Morocco, Algeria, Tunisia, Libya, Egypt, Sudan, Saudi Arabia, Yemen, Somalia, British Indian Ocean Territory
Partial eclipse in
Europe, South/West Asia, Africa, the east of North America, the Atlantic and the Indian Ocean
The eclipse takes about five hours to cross the planet. These are the global stages: each happens at a different place, so your own times depend on where you are (the table and the place checker below give them).
07:30:11 UTC
The partial eclipse begins
at sunrise, at the first place on Earth to see the Moon start to cover the Sun
08:23:29 UTC
Totality begins
at sunrise in the mid-Atlantic, near 28.0°N 44.5°W, where the Moon’s shadow first touches Earth
10:06:40 UTC
Maximum eclipse
in Egypt, near 25°30.3′N 33°11.0′E, south-east of Luxor
11:49:54 UTC
Totality ends
at sunset in the Indian Ocean, near 12.5°S 90.4°E, where the shadow leaves Earth
12:43:10 UTC
The partial eclipse ends
at sunset, at the last place on Earth to see any of the eclipse
Global stages from timeanddate.com. NASA, using a slightly different value for Earth’s rotation (ΔT 71.7 s), puts greatest eclipse at 10:06:37 UTC; predictions like these agree to a few seconds.
The path of totality
The dark band is where the Sun is completely covered, plotted point by point from the northern and southern limits in NASA’s path table (two-minute steps). The line through it is the central line, where totality is longest; the dots on it are the shadow’s position at the UTC times shown. The star marks NASA’s point of greatest duration. Outside the band the eclipse is partial.
The whole path, from sunrise in the Atlantic to sunset in the Indian Ocean. On a phone, swipe the maps sideways.Spain to Somalia, with cities from the table, and Cairo and Aswan, which are just outside.The Strait of Gibraltar, with a dot for every two minutes of the shadow’s travel. Málaga is barely inside the northern limit; the La Viñuela camera (square) is just outside it.
The path, the times and the cities are NASA’s numbers and the cities’ coordinates; the shaded land is for orientation. Map data: Natural Earth (public domain). For the path over a street map, NASA has an interactive map. NASA notes that mountains and valleys on the Moon’s edge can shift the limits by 1 to 3 km and change durations by 1 to 3 seconds.
Totality city by city
Cities on timeanddate.com’s list of places in the path, west to east. The shadow moves east, so totality reaches Cádiz first and Bosaso last, about two and a quarter hours later. The longest totality of any city here is Luxor’s, 6 min 22 s.
Totality start and the Sun’s height: computed from NASA’s Besselian elements for each city’s centre. Duration and cloud: each city’s timeanddate.com page (linked), whose cloud figure is the share of years since 2000 when that date was cloudy there. Both calculations agree on every duration here to within a few seconds; at the edges of the path a few hundred metres changes totality by seconds, so check your exact spot. Local times are each city’s clock on the day (Morocco has kept GMT since September 2026).
Close, but not total
Aswan, Egypt: magnitude 0.996, just south of the path: 99.6% of the Sun’s diameter covered, but no totality.
Cairo, Egypt: magnitude 0.947, north of the path: a deep partial eclipse.
Hurghada, Egypt: magnitude 0.980, on the Red Sea, north of the path: partial only.
Madrid, Spain: magnitude 0.880, far north of the path: partial.
A 99% partial eclipse is a very different thing from totality: the sky stays bright, there is no corona, and filters are needed throughout. If you can travel, travel into the band.
Check any place
Pick a city, type coordinates, or use your device’s location. The times are calculated in your browser from NASA’s elements, so a duration can differ by a few seconds from timeanddate.com’s in the table; your location is not sent anywhere.
NASA has typically streamed major total eclipses with telescope views and commentary. No 2027 broadcast is announced yet; watch NASA’s eclipse pages nearer the day.
Mind the time. A stream from Luxor shows totality from about 10:02 UTC: that is 06:02 in New York (EDT), 11:02 in London (BST) and 00:02 in Honolulu, on the same morning. Every stream runs a few seconds behind.
Webcams in the path are the other way to watch: a fixed camera shows the light change, the sky darken and the street lights come on, with no commentary. See the next section for what we have.
Port of Cams cameras in or near the path
We checked the coordinates of every camera on Port of Cams against NASA’s path. None is inside the path of totality. The closest is the one below; if we add a working camera inside the band before August 2027, it will be listed here.
La Vinuela, Spain · Snapshot (a still image that refreshes)
A still image of the La Viñuela reservoir in the Axarquía hills above Málaga, refreshed every few minutes. The camera is about 6 km north of the path’s northern limit, so it is outside totality: NASA’s elements give it a partial eclipse of magnitude 0.998 (the Moon covering 99.8% of the Sun’s diameter) at about 08:49 UTC. Expect the light to fade sharply, not the sky to go dark.
Across Europe, a partial eclipse will be visible from many of our international cameras that morning, though a camera pointed at a view rather than the Sun shows it only as a dimming of the light.
Eye safety: when you can look, and when you cannot
Before and after totality, always use a solar filter. NASA and the American Astronomical Society both say to look at the Sun only through special-purpose solar viewers that meet the ISO 12312-2 international standard. The AAS keeps a list of suppliers whose viewers have been checked.
Sunglasses are not filters. NASA: regular sunglasses, however dark, are not safe for viewing the Sun.
Only during totality can the filter come off, and only when the Moon completely covers the Sun’s bright face: when nothing of the Sun is visible through your viewer. Put it back the moment the bright edge reappears. Outside the path there is no safe moment at all, even at 99%.
No optics through eclipse glasses. Cameras, binoculars and telescopes need their own solar filter fitted securely to the front; looking through them with eclipse glasses on causes serious eye injury.
Inspect your filter. If it is scratched, punctured or torn, the AAS says to throw it away.
A pinhole projector is a safe way to watch without any viewer: stand with your back to the Sun and look at the projected image, never through the hole.
From NASA’s eclipse safety page and the AAS eye-safety page, checked on October 22, 2026. In early August the Sun near Luxor is almost overhead at totality (82° up), so plan for heat and shade as well.
Weather: where the skies are usually clear
By timeanddate.com’s record of past years, the Nile valley is the safest bet: Luxor and Asyut were cloudy on August 2 in 0% of years since 2000, and Sfax on the Tunisian coast in 2%. The Strait of Gibraltar is less reliable (Ceuta 59%, Tangier 42%), and Bosaso on the Somali coast was cloudy 72% of the time. These are past records for one date, not a forecast; a real forecast exists only in the last week or so.
Total solar eclipses before and after
August 12, 2026the Arctic, Greenland, Iceland and Spain; up to 2 min 18 s of totality. The first total eclipse seen from mainland Europe since 1999 (timeanddate.com) (already happened).
August 2, 2027Spain, North Africa, the Middle East and the Horn of Africa; up to 6 min 23 s of totality. This page.
July 22, 2028Australia and New Zealand; up to 5 min 10 s of totality. The next total solar eclipse after this one.
Monday, August 2, 2027. The partial eclipse begins somewhere on Earth at 07:30 UTC, totality first touches down in the Atlantic at 08:23 UTC, and the maximum eclipse is at about 10:07 UTC over Egypt. Totality leaves the Earth in the Indian Ocean at 11:50 UTC and the last of the partial eclipse ends at 12:43 UTC (timeanddate.com).
Where is the longest totality in 2027?
In Egypt’s Nile valley. NASA puts the greatest duration, 6 minutes 23.2 seconds, at 26°49′N 31°08′E, between Asyut and Luxor, and the instant of greatest eclipse (6 minutes 22.6 seconds) at 25°30′N 33°11′E, south-east of Luxor. Luxor itself gets about 6 minutes 22 seconds of totality, starting at 13:02 local time.
Which countries will see the total eclipse on August 2, 2027?
Southern Spain and Gibraltar, northern Morocco, Algeria, Tunisia, Libya, Egypt, a sliver of Sudan, Saudi Arabia, Yemen and Somalia, then the Chagos Archipelago in the Indian Ocean. A partial eclipse is visible across Europe, Africa, the Middle East, South and West Asia and the far east of North America.
Can I watch the 2027 eclipse live online?
Yes. timeanddate.com already has a live-stream page for this eclipse, and broadcast the August 2026 total eclipse from Spain. NASA has typically streamed major total eclipses as well; check its eclipse pages nearer the day. Streams run a few seconds behind real time.
Is it safe to look at a total solar eclipse?
Only during totality itself, when the Moon completely covers the Sun’s bright face. At every other moment, including the partial phases and the last sliver before totality, look only through solar viewers that meet the ISO 12312-2 standard, never through sunglasses, and never through a camera, binoculars or a telescope without a solar filter fitted to the front. NASA and the American Astronomical Society give the same advice.
Will Madrid, Cairo or Aswan see totality?
No. All three are outside the path. Madrid sees a partial eclipse of magnitude 0.88, Cairo 0.947, and Aswan, just south of the path, 0.996: almost total, but the thin crescent of Sun left uncovered is still far too bright to look at without a filter, and the sky does not go dark.
When is the next total solar eclipse after 2027?
July 22, 2028, across Australia and New Zealand, with up to 5 minutes 10 seconds of totality (NASA). The one before 2027 was on August 12, 2026, over Greenland, Iceland and Spain.
Is there a Port of Cams live camera in the path of totality?
Not inside it. We checked every camera on the site against NASA’s path: the closest is a still-image camera at the La Viñuela reservoir above Málaga, about 6 km outside the northern limit, which will see a partial eclipse of magnitude 0.998, almost but not quite total. If a camera inside the path is added before August 2027, it will appear on this page.
Eclipse predictions by Fred Espenak, NASA’s GSFC: the path table and Besselian elements, from which every contact time on this page is calculated. Global stages, countries, city durations and cloud records: timeanddate.com. Safety: NASA and the AAS. Checked on October 22, 2026. Camera feeds belong to their operators, named on each camera page.
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