Umbra.

Total solar eclipse of 15 August 2091

A total solar eclipse crosses the Earth on 15 August 2091. Along a track 74 km wide the Moon blocks the Sun completely, and totality lasts up to 1 min 38 s.

The numbers

Type
Total solar eclipse
Date
15 August 2091
Greatest eclipse
00:31:40 UTC
Eclipse magnitude
1.022
Gamma
0.9489
Central duration
1 min 38 s
Path width
74 km at greatest eclipse
Greatest eclipse at
55.6°S 150.5°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.
HobartAustralia 22:54:13 00:12:20 01:35:48 84.4% 27°
GeelongAustralia 22:44:24 00:01:00 01:24:40 75.6% 28°
MelbourneAustralia 22:44:38 00:01:20 01:25:26 74.7% 28°
AdelaideAustralia 22:34:57 23:47:20 01:08:21 68.7% 25°
CanberraAustralia 22:46:49 00:05:20 01:30:44 67.9% 33°
ChristchurchNew Zealand 23:36:28 00:58:20 02:18:07 66.4% 32°

C1 and C4 are first and last contact, when the Moon's disc touches the Sun's. C2 and C3 bracket the central phase. 22 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.