Totality 2027

Solar eclipse of 2 August 2027 in Nedroma

In Nedroma the eclipse is total. The Moon covers the whole Sun for 3 min 47 s, from 09:50 to 09:54 local time. The whole eclipse lasts from 08:43 to 11:08.

Coverage
100.0%
Magnitude
1.073
Totality
yes, 3 min 47 s
Sun's altitude at maximum
42°
Direction
east (98°)
Length of the eclipse
2 h 24 min

Times in Nedroma

Local time Africa/Algiers (UTC+1). Times rounded down to the whole second.
PhaseLocal timeSun's altitudeDirection
Eclipse begins08:43:1428°east (87°)
Totality begins09:50:0742°east (97°)
Maximum09:52:0042°east (98°)
Totality ends09:53:5443°east (98°)
Eclipse ends11:07:3457°south-east (114°)

How the Moon covers the Sun

08:4309:0609:2909:5210:1710:4211:08
Up in the picture is up in the sky. Times in local time.

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 42° above the horizon in the east (azimuth 98°). 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 Assi Bou Nif, 136 km to the north-east, it lasts 5 min 8 s – 1 min 21 s longer than here.

Your own eclipse guide

A personal guide and poster for Nedroma 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.

Buy on Etsy

Places nearby

PlaceDistanceCoverageMaximum
Maghnia18 km100.0%09:52
Remchi29 km100.0%09:52
Ahfir33 km100.0%08:52
Oujda40 km100.0%08:52
Tlemcen42 km100.0%09:53

Safety

Read all safety advice

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.