Umbra.

Annular solar eclipse of 9 May 2032

A annular solar eclipse crosses the Earth on 9 May 2032. Along a track 15 km wide the Moon sits centred on the Sun but is too small to cover it, leaving a ring of sunlight for up to 22 s.

The numbers

Type
Annular solar eclipse
Date
9 May 2032
Greatest eclipse
13:25:23 UTC
Eclipse magnitude
0.996
Gamma
0.9377
Central duration
22 s
Path width
15 km at greatest eclipse
Greatest eclipse at
51.3°S 7.0°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.
GrytvikenSouth Georgia and the South Sandwich Islands 11:24:55 12:41:03 14:01:39 84.2% 15°
Cape TownSouth Africa 13:05:16 14:25:43 15:36:10 63.4% 16°
StanleyFalkland Islands 11:12:28 12:17:43 13:28:32 58.5%
Port ElizabethSouth Africa 13:18:29 14:32:43 15:38:09 58.5% 10°
UitenhageSouth Africa 13:18:30 14:32:43 15:38:16 58.1% 10°
East LondonSouth Africa 13:24:01 14:35:43 15:38:59 54.3%

C1 and C4 are first and last contact, when the Moon's disc touches the Sun's. C2 and C3 bracket the central phase. 134 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.