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WGS 84

ECLIPSE ATLAS / TOTAL SOLAR ECLIPSE OF 2 AUGUST 2027

Six minutes of night over the Nile

On Monday 2 August 2027 the Moon’s shadow crosses Europe, Africa and Asia in under three and a half hours, from the Strait of Gibraltar to the Horn of Africa. Inside the band the Sun goes completely dark. Press play, or drag the shadow along its path.

longest totality, near Luxor
6m 23s
path width
206–259 km
shadow on Earth
≈ 3h 25m
continents
3
09:00 UT09:30 UT10:00 UT10:30 UT11:00 UTMediterraneanRed SeaAtlanticSpainAlgeriaLibyaEgyptSaudi ArabiaYemenSomaliaItalySudanTunisiaOranSfaxBenghaziLuxorJeddahMeccaBosasoAlgiersTunisAswanCádizTarifaGibraltarMálagaTangierTétouanSevilleSpainMoroccoStrait of GibraltarN500 km

13:06 in Egypt10:06 UT · 6m 23s on the central line

Greatest eclipse near Luxor: 6 minutes 23 seconds, with the Sun almost overhead.

In the shadow now: Luxor

Your location

Pick a spot

No location chosen

Click or tap the map, choose a city below, or enter coordinates. Inside the shadow band the Sun is completely covered; outside it, only partly.

Path of totality. Its edge glows brighter where totality lasts longer.
Central line, with an eclipse mark every 30 minutes.
The Moon’s shadow at the chosen time (approximate outline). Drag it along the path.
Greatest eclipse, 6m 23s.
City inside the path; hollow dots are just outside it.
Path: NASA GSFC / F. Espenak, WGS84 · Oblique plate carrée along the path; north is tilted, see arrowRelief: Natural Earth, etched after the Lunologium engraved basemap; hatching is a finish, not contours

Where to stand

Totality is longest on the central line and shortens towards the edges of the band. A city a few kilometres inside the limit sees only seconds of it. Cities run west to east, in the order the shadow reaches them; each bar is that city’s time in totality against the 6m 23s maximum. Times are for the middle of totality, in the local time in force on the day. Choose a city to find it on the map.

Estimated from NASA’s path table for each city centre. See Sources & method.
CityCountryTotalityLocal timeFrom central line
CádizSpain
2m 54s
10:4795 km
TangierMorocco
4m 51s
09:478 km
TarifaSpain
4m 39s
10:4735 km
TétouanMorocco
4m 50s
09:4815 km
GibraltarGibraltar
4m 28s
10:4848 km
MálagaSpain
1m 51s
10:49110 km
OranAlgeria
5m 08s
09:542 km
SfaxTunisia
5m 40s
10:1219 km
DjerbaTunisia
4m 24s
10:1280 km
BenghaziLibya
6m 09s
11:312 km
LuxorEgypt
6m 20s
13:0515 km
Marsa AlamEgypt
5m 30s
13:1165 km
JeddahSaudi Arabia
5m 57s
13:2539 km
MeccaSaudi Arabia
5m 08s
13:2773 km
BosasoSomalia
3m 58s
14:0090 km

So close, and only partial

These places sit just outside the band. They will see a deep partial eclipse, but the Sun never goes fully dark. A short trip towards the central line changes that.

CityCountryOutside byHead
AlgiersAlgeria14 kmsouth
AswanEgypt14 kmnorth-east
TobrukLibya23 kmsouth-west
HurghadaEgypt65 kmsouth-west
SevilleSpain71 kmsouth
TunisTunisia109 kmsouth
MedinaSaudi Arabia185 kmsouth-west

Watching safely

Never look at the Sun during the partial phases without eclipse glasses that meet ISO 12312-2. Sunglasses are not enough. Only during totality, while the Sun is completely covered, is it safe to look with the naked eye. Put the glasses back on as soon as the first bead of sunlight returns.

Sources & method

The path of totality comes from NASA’s table of northern limit, southern limit and central line at two-minute intervals (WGS84), with its greatest-eclipse figures.

City figures are Cartologium estimates from that table, not NASA local circumstances. A place’s distance from the central line is compared with its distance to the nearer limit, and the central-line duration is scaled by √(1 − x²). Times are interpolated along the central line. Expect accuracy to within a few seconds and about a minute; near the edge of the band, use a high-resolution map. Local times use the offsets in force on the day: UTC+2 in Spain, Gibraltar and Libya, UTC+1 in Morocco, Algeria and Tunisia, and UTC+3 in Egypt (summer time), Saudi Arabia and Somalia.

The map is an oblique plate carrée: its equator is the great circle the path follows, so the shadow runs straight across the sheet and north is tilted, as the arrow shows. Distances along the path are true to scale. The Moon’s shadow is drawn as an approximate ellipse, as wide as the path and as long as the ground it covers during central-line totality. The relief is Natural Earth’s public-domain shaded relief, reprojected into that frame and etched in gold after the Lunologium engraved basemap. The fine hatching is a finish, not elevation contours. Country lines follow the world-atlas 1:50m dataset and its boundary conventions. Plate provenance.