Umbra.

Annular solar eclipse of 14 October 2088

A annular solar eclipse crosses the Earth on 14 October 2088. Along a track 98 km wide the Moon sits centred on the Sun but is too small to cover it, leaving a ring of sunlight for up to 2 min 38 s. The central line runs across Chile and Argentina. From Mendoza the central phase runs 2 min 16 s, with the Sun 51° above the horizon.

The numbers

Type
Annular solar eclipse
Date
14 October 2088
Greatest eclipse
14:45:06 UTC
Eclipse magnitude
0.973
Gamma
0.5348
Central duration
2 min 38 s
Path width
98 km at greatest eclipse
Greatest eclipse at
39.7°S 56.0°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, longest central phase first
PlaceC1C2 MaxC3C4 CentralObscuredSun alt.
MendozaArgentina 12:44:04 14:07:53 14:09:06 14:10:09 15:44:57 2 min 16 s 94.5% 51°
Mar del PlataArgentina 13:08:02 14:39:26 16:17:00 94.3% 58°
San JuanArgentina 12:41:46 14:06:46 15:43:27 93.6% 52°
SantiagoChile 12:43:28 14:07:06 15:41:39 91.9% 49°
Viña del MarChile 12:41:48 14:04:46 15:38:55 91.7% 48°
Puente AltoChile 12:43:50 14:07:26 15:42:02 91.6% 49°
ValparaísoChile 12:41:47 14:04:46 15:38:46 91.6% 48°

C1 and C4 are first and last contact, when the Moon's disc touches the Sun's. C2 and C3 bracket the central phase. 206 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.