Total solar eclipse of 21 April 2088
A total solar eclipse crosses the Earth on 21 April 2088. Along a track 158 km wide the Moon blocks the Sun completely, and totality lasts up to 3 min 58 s. The central line runs across Mauritania, Western Sahara, Algeria, Tunisia, Greece, Turkey and Georgia, and more. From Gebze the central phase runs 3 min 44 s, with the Sun 59° above the horizon.
The numbers
- Type
- Total solar eclipse
- Date
- 21 April 2088
- Greatest eclipse
- 10:28:54 UTC
- Eclipse magnitude
- 1.047
- Gamma
- 0.4130
- Central duration
- 3 min 58 s
- Path width
- 158 km at greatest eclipse
- Greatest eclipse at
- 36.0°N 15.1°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.
| Place | C1 | C2 | Max | C3 | C4 | Central | Obscured | Sun alt. |
|---|---|---|---|---|---|---|---|---|
| GebzeTürkiye | 09:38:12 | 10:59:48 | 11:01:34 | 11:03:33 | 12:22:37 | 3 min 44 s | 100.0% | 59° |
| AdapazarıTürkiye | 09:40:02 | 11:01:39 | 11:03:34 | 11:05:22 | 12:24:09 | 3 min 43 s | 100.0% | 58° |
| SultanbeyliTürkiye | 09:38:04 | 10:59:42 | 11:01:34 | 11:03:10 | 12:22:20 | 3 min 28 s | 100.0% | 59° |
| MaltepeTürkiye | 09:37:51 | 10:59:29 | 11:01:14 | 11:02:56 | 12:22:09 | 3 min 27 s | 100.0% | 59° |
| SancaktepeTürkiye | 09:38:02 | 10:59:41 | 11:01:14 | 11:03:03 | 12:22:15 | 3 min 21 s | 100.0% | 59° |
| VladikavkazRussia | 10:08:23 | 11:26:03 | 11:27:34 | 11:29:21 | 12:41:10 | 3 min 19 s | 100.0% | 46° |
| MakhachkalaRussia | 10:13:26 | 11:30:19 | 11:31:54 | 11:33:14 | 12:43:55 | 2 min 55 s | 100.0% | 43° |
| SfaxTunisia | 08:57:13 | 10:17:25 | 10:18:34 | 10:19:48 | 11:45:00 | 2 min 24 s | 100.0% | 64° |
| AtaşehirTürkiye | 09:37:49 | — | 11:01:14 | — | 12:22:05 | — | 100.0% | 59° |
| UmraniyeTürkiye | 09:37:51 | — | 11:01:14 | — | 12:22:05 | — | 100.0% | 59° |
| ÜsküdarTürkiye | 09:37:39 | — | 11:00:54 | — | 12:21:54 | — | 100.0% | 59° |
| ŞişliTürkiye | 09:37:39 | — | 11:00:54 | — | 12:21:52 | — | 100.0% | 59° |
| IstanbulTürkiye | 09:37:31 | — | 11:00:54 | — | 12:21:48 | — | 100.0% | 59° |
| ÇorluTürkiye | 09:35:34 | — | 10:58:34 | — | 12:19:55 | — | 99.9% | 59° |
C1 and C4 are first and last contact, when the Moon's disc touches the Sun's. C2 and C3 bracket the central phase. 1067 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.