Eclipse 12 Aug 2026 · 20:28
43.250°, -5.767° · 367 m a.s.l.
1 min 48 s of night in broad daylight
The Sun clears local terrain by 5.78° at C3.
Full totality was visible here. C3 — the end of totality — stayed above the horizon.
Total eclipse · 100% obscuration

Photo: Astur1 · Public domain · Wikimedia Commons
In Mieres, day turned to night for 1 min 48 s.
At 20:28 local time, the Moon fully covered the Sun over Mieres. For 1 min 48 s, the sky darkened as if it were night, leaving the Sun as a ring of light around a black disc.
Eclipse 2 Aug 2027
Score 50/ 100
Eclipse visible
The Sun will be 37-41° high, so terrain rules out no city at all: of the 560 assessed, 522 tie on the same score. What decides is being inside the path.
Eclipse 26 Jan 2028
Score 22/ 100
Blocked by terrain
See the eclipse from Mieres minute by minute
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Mieres is a municipality in Asturias, located inland in the Caudal River valley, at an elevation of 367 meters and approximately 20 kilometers south of Oviedo. With a population of around 44,000, it was known in the 20th century as one of Spain's leading coal mining centers. Today, its industrial heritage and mountain landscape coexist, shaping the town's unique character and scenery.
On August 12, 2026, Mieres will lie within the path of totality. At maximum eclipse, occurring at 20:27 local time, the Sun will be 10 degrees above the horizon, with a clearance of 7.7 degrees above the terrain horizon—totality is expected to be unobstructed. Based on geometric conditions, the observation of totality from the city looks promising.
August in Mieres records an average precipitation of 53.4 millimeters according to AEMET data (1991–2020), making it one of Spain's rainiest regions even at the height of summer. The thunderstorm risk in this month is high, a characteristic of Asturias' Atlantic climate. When planning to observe the eclipse, careful attention to the weather forecast up to the day before is essential.
The last total solar eclipse visible from Mieres occurred on August 30, 1905—121 years ago. Totality lasted 3 minutes 49 seconds. Before that, on April 1, 1764, an annular eclipse occurred with 86.9% obscuration. After the eclipses of 2026, 2027, and 2028, the next annular eclipse won't occur until February 27, 2082, and the next total eclipse until November 17, 2180.
At maximum eclipse, 20:27 local time, the Sun will be at an azimuth of 281 degrees—nearly west-northwest—10 degrees above the horizon. At this evening hour, sunlight strikes from a low angle; during totality, a distinctive twilight hue will envelop the surroundings. Looking west-northwest will allow you to easily observe this phenomenon.
Editorial text by eclipses.app · Data: Wikidata, AEMET, NASA and JPL planetary ephemerides.
In Mieres, totality began at 20:27 local time and lasted 1 min 48 s, until 20:29. The eclipse maximum fell at 20:28.
In Mieres, the Sun was 10° above the horizon, toward the West. With that much margin above the horizon, any spot with open sky worked.
This area typically sees around 94% median cloud cover at that hour, based on ten years of historical data — not a forecast for this specific eclipse.
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<iframe src="https://eclipses.app/embed/widget?lat=43.2500&lon=-5.7667&size=standard&theme=dark&locale=en" width="320" height="340" frameborder="0" loading="lazy" title="Eclipse 2026"></iframe>| Phase | Local time | UTC | Progress | Sun alt. | Sun az. |
|---|---|---|---|---|---|
| C1 — Partial begins | 19:31:34 | 17:31:34 UTC | +20.3° | 271.5° | |
| C2 — Totality begins | 20:27:15 | 18:27:15 UTC | +10.3° | 280.8° | |
| Maximum | 20:28:11 | 18:28:11 UTC | +10.1° | 280.9° | |
| C3 — Totality ends | 20:29:03 | 18:29:03 UTC | +10.0° | 281.1° | |
| The Sun sets behind the terrain(terrain event, not an eclipse phase) | 21:08 | 19:08 UTC | +3.2° | 287.6° | |
| C4 — Partial endsnot visible | 21:21:14 | 19:21:14 UTC | +1.1° | 289.8° |
Phases marked with ⛰️ were not seen: the Sun was already hidden behind the real terrain at that moment.
C2/C3 times and duration corrected for the lunar limb (the Moon's real edge profile).
Times in CEST local time
Oriented as seen with the naked eye, zenith up (official ephemerides usually draw it with celestial north up, rotated with respect to this).
It was toward West (280.9°)
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 |
|---|---|---|---|
| Peña Rueda | 2151 m | 24.5 km | 215° SW |
| Estorbín de Valverde | 2115 m | 24.7 km | 157° SSE |
| Cueto los Barriales | 2111.16 m | 24.3 km | 159° SSE |
| Vaso de Rueda | 2096 m | 24.7 km | 215° SW |
| Reboqueras | 2091 m | 24.2 km | 159° SSE |
| Pico el Cuadro | 2089 m | 24.8 km | 161° SSE |
| Pico de Pisones o Camparón | 2042 m | 23.3 km | 161° SSE |
| Pico Tres Concejos | 2014 m | 22.4 km | 164° SSE |
10-year average over 70 samples: the 3 days before and after 12 August, at the same eclipse hour · Source: ERA5 (ECMWF)
Full cloud-cover forecast for eclipse day, including the hour-by-hour outlook toward the sun. Available with PRO.
See plansSolar eclipses computed from astronomical ephemerides for the city's coordinates.
Yes — Mieres was inside the totality path and the horizon allowed the total phase to be fully visible.
Maximum occurred at 20:28 local time (18:28 UTC) in Mieres.
The Sun was toward the West (azimuth 281°), 10° above the horizon at maximum from Mieres.
Totality lasted 1 min 48 s in Mieres (C2 to C3). (corrected for the Moon's limb profile)
Mieres saw totality (C2-C3) very close to the western horizon. The partial end (C4) fell below the horizon: a clear western view was needed 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.