Umbra.

Total solar eclipse of 25 November 2030

A total solar eclipse crosses the Earth on 25 November 2030. Along a track 156 km wide the Moon blocks the Sun completely, and totality lasts up to 3 min 44 s. The central line runs across Namibia, Botswana, South Africa and Australia. From Durban the central phase runs 2 min 26 s, with the Sun 34° above the horizon.

The numbers

Type
Total solar eclipse
Date
25 November 2030
Greatest eclipse
06:50:19 UTC
Eclipse magnitude
1.047
Gamma
0.3867
Central duration
3 min 44 s
Path width
156 km at greatest eclipse
Greatest eclipse at
43.6°S 71.2°E

See it in 3D

The simulator places the Sun, Earth and Moon at their true relative positions for this date and draws the shadow cones at real scale. You can scrub through the eclipse, drop an observer anywhere, and watch the umbra sweep the surface.

Loads about 300 KB on demand — nothing is downloaded until you press it.

Local circumstances

All times are UTC. Contact times are computed for each city from the Besselian elements against the WGS84 ellipsoid, at sea level and without refraction.

Contact times and maximum obscuration, longest central phase first
PlaceC1C2 MaxC3C4 CentralObscuredSun alt.
DurbanSouth Africa 04:32:33 05:33:33 05:34:39 05:35:59 06:44:35 2 min 26 s 100.0% 34°
PietermaritzburgSouth Africa 04:32:06 05:32:51 05:33:59 05:35:09 06:43:25 2 min 18 s 100.0% 33°
WindhoekNamibia 04:24:21 05:18:52 05:19:39 05:20:44 06:21:18 1 min 52 s 100.0% 17°
WelkomSouth Africa 04:29:34 05:28:42 05:29:39 05:30:31 06:36:48 1 min 49 s 100.0% 29°
NewcastleSouth Africa 04:29:41 05:30:59 06:40:13 99.0% 32°
Richards BaySouth Africa 04:31:23 05:33:59 06:44:23 99.0% 34°
VanderbijlparkSouth Africa 04:28:08 05:28:39 06:36:16 98.9% 29°
VereenigingSouth Africa 04:28:06 05:28:39 06:36:19 98.7% 29°
SowetoSouth Africa 04:27:38 05:27:59 06:35:40 97.7% 29°
JohannesburgSouth Africa 04:27:34 05:27:59 06:35:46 97.2% 29°

C1 and C4 are first and last contact, when the Moon's disc touches the Sun's. C2 and C3 bracket the central phase. 135 of the 2,250 cities in the database see at least a 3% partial eclipse.

How these figures were produced

Positions come from astronomy-engine, a VSOP87/ELP implementation. From the geocentric Sun and Moon vectors the site computes Besselian elements — x, y, d, μ, l1, l2, tan f1 and tan f2 — and solves the observer's position on the fundamental plane against the WGS84 ellipsoid. Central durations agree with NASA's Five Millennium Canon to within about half a second. Full method and validation.