39.417°, -0.383° · 7 m a.s.l.
Visible
The Sun clears local terrain by 4.04° at C3.
100%
You'll see full totality, but the Sun will set before the partial phase ends — an unusually epic finale.
Total eclipse · 100% obscuration
See the eclipse from Alfafar minute by minute
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Photo: Enrique Íñiguez Rodríguez (Qoan) · CC BY-SA 3.0 · Wikimedia Commons
Alfafar is a municipality in the province of Valencia that belongs to the comarca of l'Horta Sud, in the Valencian Community. Located immediately south of the Valencian capital, it occupies a coastal plain barely 7 meters above sea level. With approximately 20,850 inhabitants, the municipality is part of the Valencia metropolitan area and is surrounded by flat terrain, offering broad views of the sky in multiple directions.
On August 12, 2026, Alfafar will lie within the path of totality of the solar eclipse. The moment of maximum obscuration will occur at 20:32 local time, when the Sun will be only 4.5° above the horizon with an azimuth of 286°. The margin between the Sun's altitude and the topographic horizon is about 4 degrees: sufficient to observe totality, provided the west-northwest horizon is clear of buildings or trees.
August in Alfafar follows the coastal Mediterranean pattern: dry heat and abundant sunshine. According to AEMET climatological data for the 1991–2020 period, the average temperature for the month is 26.5 °C, with highs around 30.6 °C and nighttime lows around 22.5 °C. Average monthly accumulated rainfall does not exceed 14.7 mm, and the municipality accumulates about 288 hours of sunlight in August. The probability of clear skies reaches 69%, although there is a moderate risk of afternoon thunderstorms.
The oldest recorded precedent is the total eclipse of July 18, 1860, 166 years ago, which offered a phase of totality of approximately 92 seconds from this area. Later, on October 3, 2005, an annular eclipse occurred with an obscuration of 90.4% of the Sun's disk for just under four minutes. After the eclipses of 2026, 2027, and 2028, the next significant annular event over this territory will not arrive until July 13, 2075.
At the moment of maximum eclipse, the Sun will be 4.5° in altitude above the horizon, with an azimuth of 286°, that is, in the west-northwest direction. At such a low angle to the horizon, any obstacle—a building, a row of trees, a hill—can block the view. It is recommended to find a high point or an open space with a clear horizon facing west to guarantee the observation of totality.
Editorial text by eclipses.app · Data: Wikidata, AEMET, NASA and astronomy-engine.
| Phase | UTC | Local time | Sun alt. | Sun az. |
|---|---|---|---|---|
| C1 — Partial begins | 17:38 UTC | 19:38 | +14.8° | 277.3° |
| C2 — Totality begins | 18:32 UTC | 20:32 | +4.6° | 285.5° |
| Maximum | 18:32 UTC | 20:32 | +4.5° | 285.6° |
| C3 — Totality ends | 18:33 UTC | 20:33 | +4.5° | 285.7° |
| C4 — Partial ends | 19:24 UTC | 21:24 | -4.3° | 293.7° |
Look toward WNW (293.7°)
Azimuth at C4
293.7° WNW
Sun altitude at C4
-4.33°
Terrain horizon
0.42°
Sun−terrain margin
+4.04°
A solar eclipse is described by four key moments, the contact points between the discs of the Sun and the Moon:
Where the eclipse is only partial, the Moon never fully covers the Sun: only C1 and C4 occur, with no totality in between.
| Peak | Elevation | Distance | Azimuth |
|---|---|---|---|
| Pic del Besori | 361 m | 17.8 km | 225° SW |
| Alts de València | 335 m | 17.0 km | 226° SW |
| la Rodana del PicIn the Sun's direction | 322 m | 23.8 km | 306° NW |
| Alts de la Guatleta | 308 m | 17.4 km | 233° SW |
| Lloma del Barranc dels Aspres | 306 m | 16.7 km | 228° SW |
| el Puntal | 290 m | 17.2 km | 239° WSW |
| el Cerro | 289 m | 22.1 km | 234° SW |
| la SelletaIn the Sun's direction | 283 m | 21.5 km | 307° NW |
Avg. temp.
26.5°C
Max / min
30.6° / 22.5°
Precipitation
14.7 mm
Storm risk
Medium
Station VALÈNCIA, 7 km away · Period 1991-2020 · Source: AEMET
P25 — clearer days
4%
Median cloud cover
32%
P75 — cloudier days
58%
Source: ERA5 (ECMWF), 10-year average at the eclipse hour.
Solar eclipses computed from astronomical ephemerides for the city's coordinates.
Yes — Alfafar is inside the totality path and the horizon allows the total phase to be fully visible.
Maximum occurs at 20:32 local time (18:32 UTC) in Alfafar.
Look WNW (azimuth 286°); the Sun will be 5° above the horizon at maximum from Alfafar.
Totality lasts 1 min 0 s in Alfafar (C2 to C3).
Alfafar will see totality (C2-C3) very close to the western horizon. The partial end (C4) falls below the horizon: you need a clear western view for an epic experience.
Yes, you need ISO 12312-2 certified eclipse glasses during every partial phase. Regular sunglasses do NOT protect. Glasses can only be removed during the totality phase (when the Sun is fully covered); never during annular or partial eclipses. Pages flagged "visible" assume a clear horizon, not a viewing recommendation.
For the August 12 eclipse. Recommended stay: Aug 10–14, 2026.
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