Umbra.

Total solar eclipse of 11 May 2059

A total solar eclipse crosses the Earth on 11 May 2059. Along a track 82 km wide the Moon blocks the Sun completely, and totality lasts up to 2 min 23 s. The central line runs across Fiji, Ecuador, Peru, Colombia and Brazil.

The numbers

Type
Total solar eclipse
Date
11 May 2059
Greatest eclipse
19:20:23 UTC
Eclipse magnitude
1.024
Gamma
0.5080
Central duration
2 min 23 s
Path width
82 km at greatest eclipse
Greatest eclipse at
10.7°S 100.4°W

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
PlaceC1C2 MaxC3C4 CentralObscuredSun alt.
IquitosPeru 19:06:44 20:35:23 21:50:48 100.0% 30°
CuencaEcuador 18:52:25 20:26:03 21:46:18 100.0% 38°
GuayaquilEcuador 18:50:56 20:25:03 21:45:53 97.7% 39°
PiuraPeru 18:44:42 20:20:03 21:42:23 95.6% 40°
ManausBrazil 19:35:24 20:51:23 21:56:41 92.1% 14°
QuitoEcuador 18:57:36 20:29:43 21:48:33 90.8% 38°

C1 and C4 are first and last contact, when the Moon's disc touches the Sun's. C2 and C3 bracket the central phase. 359 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.