Umbra.

Total solar eclipse of 30 March 2052

A total solar eclipse crosses the Earth on 30 March 2052. Along a track 155 km wide the Moon blocks the Sun completely, and totality lasts up to 4 min 08 s. The central line runs across Mexico and the United States. From Puerto Vallarta the central phase runs 4 min 02 s, with the Sun 71° above the horizon.

The numbers

Type
Total solar eclipse
Date
30 March 2052
Greatest eclipse
18:30:16 UTC
Eclipse magnitude
1.047
Gamma
0.3235
Central duration
4 min 08 s
Path width
155 km at greatest eclipse
Greatest eclipse at
22.4°N 102.5°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.
Puerto VallartaMexico 16:54:11 18:19:14 18:21:16 18:23:16 19:52:46 4 min 02 s 100.0% 71°
Ciudad VictoriaMexico 17:11:16 18:38:34 18:40:16 18:41:55 20:10:03 3 min 21 s 100.0% 71°
TepicMexico 16:56:18 18:21:46 18:23:16 18:25:02 19:54:36 3 min 17 s 100.0% 70°
AguascalientesMexico 17:01:53 18:28:41 18:30:16 18:31:36 20:01:10 2 min 55 s 100.0% 72°
Heroica MatamorosMexico 17:18:11 18:46:56 20:15:17 100.0% 68°
Soledad de Graciano SánchezMexico 17:05:04 18:33:56 20:04:33 99.7% 72°
San Luis PotosíMexico 17:04:55 18:33:36 20:04:25 99.7% 72°
ZapopanMexico 16:57:50 18:25:56 19:57:16 99.5% 72°
GuadalajaraMexico 16:57:44 18:25:36 19:57:11 99.4% 72°
TlaquepaqueMexico 16:57:52 18:25:56 19:57:22 99.2% 72°

C1 and C4 are first and last contact, when the Moon's disc touches the Sun's. C2 and C3 bracket the central phase. 352 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.