Umbra.

Partial solar eclipse of 11 April 2051

A partial solar eclipse takes place on 11 April 2051. The Moon covers part of the Sun's disc but never all of it, because the shadow axis passes beside the Earth rather than across it. At greatest eclipse, 99% of the Sun's diameter is covered, seen from 71.8°N 32.8°E.

The numbers

Type
Partial solar eclipse
Date
11 April 2051
Greatest eclipse
02:09:04 UTC
Eclipse magnitude
0.986
Gamma
1.0165
Greatest eclipse at
71.8°N 32.8°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
PlaceC1C2 MaxC3C4 CentralObscuredSun alt.
LongyearbyenSvalbard and Jan Mayen 01:30:39 02:22:04 03:14:18 97.1%
SyktyvkarRussia 00:57:50 01:48:44 02:42:00 94.6%
KirovRussia 00:53:59 01:44:04 02:36:41 92.3% -0°
PermRussia 00:50:44 01:41:44 02:35:25 90.7%
IzhevskRussia 00:50:12 01:40:44 02:33:23 90.0%
Nizhny TagilRussia 00:49:27 01:41:04 02:35:24 89.8%

C1 and C4 are first and last contact, when the Moon's disc touches the Sun's. C2 and C3 bracket the central phase. 569 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.