Umbra.

Annular solar eclipse of 21 June 2039

A annular solar eclipse crosses the Earth on 21 June 2039. Along a track 201 km wide the Moon sits centred on the Sun but is too small to cover it, leaving a ring of sunlight for up to 4 min 05 s. The central line runs across the United States, Canada, Russia, Greenland, Sweden, Finland and Estonia. From Tallinn the central phase runs 3 min 42 s, with the Sun 7° above the horizon.

The numbers

Type
Annular solar eclipse
Date
21 June 2039
Greatest eclipse
17:11:28 UTC
Eclipse magnitude
0.945
Gamma
0.8314
Central duration
4 min 05 s
Path width
201 km at greatest eclipse
Greatest eclipse at
78.9°N 102.2°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, longest central phase first
PlaceC1C2 MaxC3C4 CentralObscuredSun alt.
TallinnEstonia 17:13:16 18:12:38 18:14:28 18:16:20 19:12:35 3 min 42 s 88.2%
SmolenskRussia 17:18:10 18:14:52 18:16:48 18:18:32 19:12:23 3 min 40 s 87.9%
AnchorageUnited States 15:19:05 16:22:07 16:23:48 16:25:46 17:33:29 3 min 39 s 88.9% 23°
PskovRussia 17:14:56 18:13:13 18:15:08 18:16:46 19:12:04 3 min 34 s 88.1%
MariehamnAland 17:13:02 18:13:53 18:15:28 18:17:05 19:14:34 3 min 12 s 88.3%
TampereFinland 17:10:02 18:10:25 18:11:48 18:13:27 19:10:45 3 min 02 s 88.3%
EspooFinland 17:12:01 18:13:28 19:11:46 88.2%
HelsinkiFinland 17:12:01 18:13:28 19:11:39 88.2%
VitebskBelarus 17:18:16 18:17:08 19:13:21 88.0%
MahilyowBelarus 17:20:04 18:18:48 19:14:24 87.9%
BabruyskBelarus 17:21:38 18:20:28 19:15:56 87.8%
MinskBelarus 17:21:08 18:20:28 19:16:26 87.8%

C1 and C4 are first and last contact, when the Moon's disc touches the Sun's. C2 and C3 bracket the central phase. 454 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.