Umbra.

Total solar eclipse of 22 May 2096

A total solar eclipse crosses the Earth on 22 May 2096. Along a track 239 km wide the Moon blocks the Sun completely, and totality lasts up to 6 min 06 s. The central line runs across Indonesia and the Philippines. From Magugpo Poblacion the central phase runs 4 min 32 s, with the Sun 41° above the horizon.

The numbers

Type
Total solar eclipse
Date
22 May 2096
Greatest eclipse
01:34:01 UTC
Eclipse magnitude
1.074
Gamma
0.1196
Central duration
6 min 06 s
Path width
239 km at greatest eclipse
Greatest eclipse at
27.3°N 153.4°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.
Magugpo PoblacionPhilippines 23:11:28 00:14:39 00:17:01 00:19:11 01:31:16 4 min 32 s 100.0% 41°
DavaoPhilippines 23:10:57 00:14:01 00:16:21 00:18:27 01:30:23 4 min 25 s 100.0% 40°
Bandar LampungIndonesia 22:59:11 23:52:10 23:53:41 23:55:24 00:54:12 3 min 13 s 100.0% 12°
General SantosPhilippines 23:09:41 00:12:57 00:14:41 00:16:10 01:28:15 3 min 13 s 100.0% 39°
MalingaoPhilippines 23:10:38 00:15:21 01:28:42 100.0% 39°
BudtaPhilippines 23:10:41 00:15:21 01:28:43 100.0% 39°
ButuanPhilippines 23:13:14 00:18:41 01:33:03 99.5% 41°
LibertadPhilippines 23:13:12 00:18:41 01:32:59 99.4% 41°
Iligan CityPhilippines 23:11:57 00:16:41 01:30:09 99.1% 40°
Cagayan de OroPhilippines 23:12:19 00:17:21 01:30:53 99.0% 40°

C1 and C4 are first and last contact, when the Moon's disc touches the Sun's. C2 and C3 bracket the central phase. 674 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.