Umbra.

Annular solar eclipse of 10 April 2089

A annular solar eclipse crosses the Earth on 10 April 2089. Along a track 28 km wide the Moon sits centred on the Sun but is too small to cover it, leaving a ring of sunlight for up to 53 s. The central line runs across Australia and Fiji.

The numbers

Type
Annular solar eclipse
Date
10 April 2089
Greatest eclipse
22:41:48 UTC
Eclipse magnitude
0.992
Gamma
0.3325
Central duration
53 s
Path width
28 km at greatest eclipse
Greatest eclipse at
10.2°S 154.8°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.
AlofiNiue 20:16:44 21:48:28 23:31:43 97.6% 54°
KingstonNorfolk Island 19:55:38 21:08:08 22:31:01 96.6% 25°
SydneyAustralia 19:54:51 20:58:28 22:09:23 95.7%
WollongongAustralia 19:55:08 20:58:28 22:09:16 95.3%
Nuku‘alofaTonga 20:08:54 21:35:28 23:14:23 94.9% 47°
NewcastleAustralia 19:54:25 20:58:08 22:09:37 94.7%

C1 and C4 are first and last contact, when the Moon's disc touches the Sun's. C2 and C3 bracket the central phase. 122 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.