Solar eclipse of 2 August 2027 in Ksar El Kebir
In Ksar El Kebir the eclipse is total. The Moon covers the whole Sun for 3 min 42 s, from 08:45 to 08:49 local time. The whole eclipse lasts from 07:40 to 10:00.
- Coverage
- 100.0%
- Magnitude
- 1.072
- Totality
- yes, 3 min 42 s
- Sun's altitude at maximum
- 38°
- Direction
- east (94°)
- Length of the eclipse
- 2 h 20 min
Times in Ksar El Kebir
| Phase | Local time | Sun's altitude | Direction |
|---|---|---|---|
| Eclipse begins | 07:40:09 | 24° | east (85°) |
| Totality begins | 08:44:56 | 37° | east (94°) |
| Maximum | 08:46:47 | 38° | east (94°) |
| Totality ends | 08:48:38 | 38° | east (94°) |
| Eclipse ends | 10:00:18 | 53° | east (108°) |
How the Moon covers the Sun
What you will notice
When the Moon covers the whole Sun, it becomes as dark as dusk in the middle of the day. The brightest planets and stars appear, the Sun's corona shines around the black Moon and the temperature drops by several degrees. Just before and after you can see the "diamond ring".
Where the Sun is
At maximum the Sun is 38° above the horizon in the east (azimuth 94°). The Sun is high, so most outdoor spots with a clear view upwards will work.
Compared with totality
Closer to the centre of the path, totality lasts longer: in Mdiq, 92 km to the north-east, it lasts 4 min 53 s – 1 min 10 s longer than here.
Your own eclipse guide
A personal guide and poster for Ksar El Kebir or your exact address: times to the second, a timeline, a map of the path and safety advice. Printable PDF in English, Swedish, German or Spanish. about €13.
Places nearby
| Place | Distance | Coverage | Maximum |
|---|---|---|---|
| Lalla Mimouna | 23 km | 100.0% | 08:47 |
| Larache | 31 km | 100.0% | 08:47 |
| Souk El Arbaa | 36 km | 100.0% | 08:47 |
| Ouezzane | 37 km | 100.0% | 08:47 |
| Chefchaouen | 61 km | 100.0% | 08:48 |
Safety
- Never look directly at the Sun without certified eclipse glasses that meet the ISO 12312-2 standard. Ordinary sunglasses do not protect your eyes, not even several pairs on top of each other.
- Only during totality itself, when the Sun is completely covered, is it safe to take the glasses off. Put them back on as soon as the first point of light appears.
How we calculated this
The times are calculated for the place's coordinates and elevation (GeoNames) with Skyfield and the JPL ephemeris DE421 – the same program that makes the paid guide. The calculation is checked against NASA eclipse data (Fred Espenak, NASA GSFC). The times assume a clear sky; nobody can forecast the weather this far ahead.