The total solar eclipse of 2 August 2027, from Ceuta

Ceuta: close to five minutes, on the African side of the Strait.

4 min 51 sec of totality

Ceuta is inside the path of totality. The Sun is completely covered for 4 min 51 sec, with the Sun 38 degrees above the horizon at maximum.

Local contact times

All times are for Ceuta on Monday, 2 August 2027, in local clock time, computed for latitude 35.889, longitude -5.320 at sea level. A few hundred metres of elevation moves these by well under a second.

StageLocal timeUTCWhat happens
Partial eclipse begins09:40:54 GMT+207:40:54 UTCThe Moon takes the first bite out of the Sun. Filters on.
Totality begins10:45:12 GMT+208:45:12 UTCOnly now is it safe to look with bare eyes.
Maximum eclipse10:47:36 GMT+208:47:36 UTCThe middle of totality, with the Sun 38 degrees above the horizon.
Totality ends10:50:03 GMT+208:50:03 UTCFilters back on immediately, before the first bead of Sun returns.
Partial eclipse ends12:01:04 GMT+210:01:04 UTCThe Sun is whole again.
Sun altitude at maximum
38 degrees (a bit under halfway up, so an open view that way matters)
Most of the Sun covered
100 percent
Duration of totality
4 min 51 sec
Whole eclipse lasts
2 hr 20 min
Time zone
Europe/Madrid
Coordinates used
35.889, -5.320

Eye safety. A certified solar filter is required for every part of this eclipse except the 4 min 51 sec of totality itself. During totality, and only then, filters come off and the corona is safe to look at with bare eyes. Put them back on the instant the first bead of Sun returns; do not wait to be dazzled.

How much room is there

Ceuta sits about 98 km from the nearest edge of the path, which is comfortable margin.

It is close enough to the center line that a short drive gains little.

Distances are measured due south along this town's meridian. The path runs east-southeast, so the true shortest hop is a little less than these figures: treat them as an upper bound.

What to expect here

Ceuta is on the African shore and slightly better placed than Gibraltar or Tarifa, with the practical advantage that it is reachable by ferry from mainland Spain on the morning itself.

Checking another location

This page is computed for one set of coordinates. For anywhere else, including a specific hotel, a viewpoint or a spot out on the path, the Eclipse Explorer computes local contact times and how much of the Sun is covered for any location you give it, and the main page for this eclipse carries the global circumstances, the Saros series and the shape of the path.

These are mean-limb times. The Moon's edge is mountainous, so the exact instants totality begins and ends shift by a second or two depending on which lunar valley the last sliver of Sun drains through. That correction is smaller than the difference a short drive makes, and smaller than the error in standing somewhere other than these exact coordinates. Every figure here is a computed fact you may reuse freely; see how these were computed.

The same eclipse from other towns

Every town below is computed the same way, so the durations are directly comparable.