Solar eclipse of August 12, 2026

Solar eclipse of August 12, 2026
Solar eclipse of August 12, 2026
	Map
Type of eclipse
Nature	Total
Gamma	0.8977
Magnitude	1.0386
Maximum eclipse
Duration	138 s (2 min 18 s)
Coordinates	65°12′N 25°12′W / 65.2°N 25.2°W
Max. width of band	294 km (183 mi)
Times (UTC)
Greatest eclipse	17:47:06
References
Saros	126 (48 of 72)
Catalog # (SE5000)	9566

A total solar eclipse will occur at the Moon's descending node of orbit on Wednesday, August 12, 2026,^[1] with a magnitude of 1.0386. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 2.2 days after perigee (on August 10, 2026, at 12:15 UTC), the Moon's apparent diameter will be larger.^[2]

The total eclipse will pass over the Arctic, Greenland, Iceland, Atlantic Ocean, northern Spain and very extreme north eastern Portugal. The points of greatest duration and greatest eclipse will be just 45 km (28 mi) off the western coast of Iceland by 65°10.3' N and 25°12.3' W, where the totality will last 2m 18.21s. A partial eclipse will cover more than 90% of the Sun in Ireland, Great Britain, Portugal, France, Italy, the Balkans and North Africa and to a lesser extent in most of Europe, West Africa and northern North America.

The total eclipse will pass over northern Spain from the Atlantic coast to the Mediterranean coast as well as the Balearic Islands. The total eclipse will be visible from the cities of A Coruña, Valencia, Zaragoza, Palma and Bilbao, but both Madrid and Barcelona will be just outside the path of totality.

The last total solar eclipse in continental Europe occurred on August 11, 1999. It will be the first total solar eclipse visible in Iceland since June 30, 1954, also Solar Saros series 126 (descending node), and the only one to occur in the 21st century as the next one visible over Iceland will be in 2196. The last total solar eclipse in Spain happened on August 30, 1905 and followed a similar path across the country. The next total eclipse visible in Spain will happen less than a year later on August 2, 2027.

Circumstances

The eclipse path proceeds from North Siberia throughout the Arctic Region, Iceland, eastern Atlantic to Spain and the Mediterranean.

Solar eclipse and the aurora borealis

In the North Russia area where totality will begin at sunrise, the aurora borealis could also be visible up to the beginning of the nautical twilight, depending on the intensity of the auroral activity at that date. If an extremely high intensity geomagnetic storm takes place simultaneously, there might be chances of seeing the aurora simultaneously with the eclipsed Sun. In the east of Taymyr Peninsula (north-east of Krasnoyarsk Krai) the maximum of total phase will occur at August 13 at 0:00 local time during midnight sun.^[3]

Solar eclipse below the horizon

Due to the considerable eclipse gamma (more than 0.8), observers where the totally eclipsed Sun is just below the horizon will have the chance to observe the lunar shadow in the high atmosphere, as well as shortened civil twilight and extended nautical twilight. The darkening of the twilight sky could improve the chances of observing the inner Zodiacal light.^[4]

Bright planets and stars visible during totality

Far northern Russia will be treated to a dawn eclipse. Mercury and Jupiter will be very low above the rising eclipsed Sun, but Mercury will be showing most of its sunlit side and Jupiter will have its usual brightness. Mars and Saturn will be more advantageously placed in the northeast and southeast respectively. Of the bright asterisms, the Big Dipper will be very high in the north-northwest and the Summer Triangle will be high in the southwest. Aldebaran, Arcturus, Capella and Pollux are other first-magnitude stars which may be seen, although they will be low.

In Spain the eclipse will occur about 1 hour before sunset. Mercury and Jupiter will be west of the eclipsed Sun, therefore very low below it. Venus will be brilliant well up in the southwest, with Spica to its east. Arcturus will be high in the south, and the Summer Triangle will be well up in the east. Lower in the south, Antares will be minutes away from transit.^[5]

Images

Animated path

Details of the totality in some places or cities

**Solar Eclipse of August 12, 2026**
Country or Territory	Place or City	Start of partial eclipse (Local Time)	Start of total eclipse (Local Time)	End of total eclipse (Local Time)	Duration of total eclipse	End of partial eclipse (Local Time)	Magnitude
Russia	East of Taymyr Peninsula, Krasnoyarsk Krai	23:08:43	23:59:21	00:00:56 (August 13)	1 min 35s	00:51:51 (August 13)	1,031
Greenland	Mestersvig	16:32:41	17:32:52	17:34:01	1 min 09 s	18:32:25	1,038
Iceland	Ísafjörður	16:43:17	17:44:07	17:45:38	1 min 31 s	18:43:57	1,038
Iceland	Grundarfjörður	16:45:14	17:46:03	17:47:55	1 min 52 s	18:46:03	1,038
Iceland	Reykjavík	16:47:11	17:48:15	17:49:17	1 min 02 s	18:47:38	1,038
Iceland	Reykjanesbær	16:47:11	17:48:04	17:49:43	1 min 39 s	18:47:52	1,038
Spain	Gijón	19:31:02	20:26:47	20:28:32	1 min 45 s	21:20:45	1,034
Spain	Santander	19:31:19	20:26:55	20:27:57	1 min 02 s	21:18:17 (Sunset)	1,034
Spain	Oviedo	19:31:19	20:27:04	20:28:52	1 min 48 s	21:21:04	1,034
Spain	Bilbao	19:31:47	20:27:22	20:27:52	30 s	21:14:15 (Sunset)	1,034
Spain	A Coruña	19:30:56	20:27:40	20:28:56	1 min 15 s	21:21:59	1,034
Spain	León	19:32:43	20:28:19	20:30:04	1 min 44 s	21:22:06	1,034
Spain	Burgos	19:33:21	20:28:24	20:30:07	1 min 43 s	21:15:25 (Sunset)	1,033
Spain	Zaragoza	19:34:40	20:29:01	20:30:25	1 min 24 s	21:02:52 (Sunset)	1,032
Spain	Tarragona	19:35:33	20:29:28	20:30:28	1 min 00 s	20:53:18 (Sunset)	1,032
Spain	Valladolid	19:34:30	20:29:52	20:31:19	1 min 27 s	21:18:12	1,033
Portugal	Aveleda e Rio de Onor	18:33:47	19:30:21	19:30:33	12 s	20:23:29	1,034
Spain	Palma de Mallorca	19:38:03	20:31:04	20:32:40	1m 36 s	20:44:48 (Sunset)	1,031
Spain	Castellón de La Plana	19:37:31	20:31:19	20:32:52	1 m 34 s	20:56:20 (Sunset)	1,032
Spain	Alcobendas	19:36:32	20:31:57	20:32:21	24 s	21:11:42 (Sunset)	1,033
Spain	Valencia	19:38:23	20:32:27	20:33:28	1 min 01 s	20:56:31 (Sunset)	1,032
Spain	Ibiza	19:39:14	20:32:44	20:33:48	1 min 04 s	20:48:28 (Sunset)	1,031

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.^[6]

August 12, 2026 Solar Eclipse Times
Event	Time (UTC)
First Penumbral External Contact	2026 August 12 at 15:35:23.9 UTC
First Umbral External Contact	2026 August 12 at 16:59:18.1 UTC
First Central Line	2026 August 12 at 17:01:16.5 UTC
First Umbral Internal Contact	2026 August 12 at 17:03:19.0 UTC
Equatorial Conjunction	2026 August 12 at 17:05:01.6 UTC
Ecliptic Conjunction	2026 August 12 at 17:37:53.9 UTC
Greatest Duration	2026 August 12 at 17:45:53.9 UTC
Greatest Eclipse	2026 August 12 at 17:47:05.8 UTC
Last Umbral Internal Contact	2026 August 12 at 18:31:21.6 UTC
Last Central Line	2026 August 12 at 18:33:21.7 UTC
Last Umbral External Contact	2026 August 12 at 18:35:17.7 UTC
Last Penumbral External Contact	2026 August 12 at 19:59:09.2 UTC

August 12, 2026 Solar Eclipse Parameters
Parameter	Value
Eclipse Magnitude	1.03863
Eclipse Obscuration	1.07876
Gamma	0.89774
Sun Right Ascension	09h29m47.3s
Sun Declination	+14°48'04.5"
Sun Semi-Diameter	15'47.0"
Sun Equatorial Horizontal Parallax	08.7"
Moon Right Ascension	09h31m17.3s
Moon Declination	+15°36'58.5"
Moon Semi-Diameter	16'16.9"
Moon Equatorial Horizontal Parallax	0°59'45.1"
ΔT	72.4 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of August 2026
August 12 Descending node (new moon)	August 28 Ascending node (full moon)

Total solar eclipse Solar Saros 126	Partial lunar eclipse Lunar Saros 138

Related eclipses

Solar eclipses of 2026–2029

This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.^[7]

The partial solar eclipses on June 12, 2029 and December 5, 2029 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2026 to 2029
Ascending node			Descending node
Saros	Map	Gamma	Saros	Map	Gamma
121	February 17, 2026 Annular	−0.97427	126	August 12, 2026 Total	0.89774
131	February 6, 2027 Annular	−0.29515	136	August 2, 2027 Total	0.14209
141	January 26, 2028 Annular	0.39014	146	July 22, 2008 Total	−0.60557
151	January 14, 2029 Partial	1.05532	156	July 11, 2029 Partial	−1.41908

Saros 126

This eclipse is a part of Saros series 126, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on March 10, 1179. It contains annular eclipses from June 4, 1323 through April 4, 1810; hybrid eclipses from April 14, 1828 through May 6, 1864; and total eclipses from May 17, 1882 through August 23, 2044. The series ends at member 72 as a partial eclipse on May 3, 2459. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity was produced by member 11 at 6 minutes, 30 seconds on June 26, 1359, and the longest duration of totality was produced by member 45 at 2 minutes, 36 seconds on July 10, 1972. All eclipses in this series occur at the Moon’s descending node of orbit.^[8]

Series members 36–57 occur between 1801 and 2200:
36	37	38
April 4, 1810	April 14, 1828	April 25, 1846
39	40	41
May 6, 1864	May 17, 1882	May 28, 1900
42	43	44
June 8, 1918	June 19, 1936	June 30, 1954
45	46	47
July 10, 1972	July 22, 1990	August 1, 2008
48	49	50
August 12, 2026	August 23, 2044	September 3, 2062
51	52	53
September 13, 2080	September 25, 2098	October 6, 2116
54	55	56
October 17, 2134	October 28, 2152	November 8, 2170
57
November 18, 2188

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.

22 eclipse events between June 1, 2011 and October 24, 2098
May 31–June 1	March 19–20	January 5–6	October 24–25	August 12–13
118	120	122	124	126
June 1, 2011	March 20, 2015	January 6, 2019	October 25, 2022	August 12, 2026
128	130	132	134	136
June 1, 2030	March 20, 2034	January 5, 2038	October 25, 2041	August 12, 2045
138	140	142	144	146
May 31, 2049	March 20, 2053	January 5, 2057	October 24, 2060	August 12, 2064
148	150	152	154	156
May 31, 2068	March 19, 2072	January 6, 2076	October 24, 2079	August 13, 2083
158	160	162	164
June 1, 2087			October 24, 2098

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
March 25, 1819 (Saros 107)	February 23, 1830 (Saros 108)	January 22, 1841 (Saros 109)		November 21, 1862 (Saros 111)
		August 20, 1895 (Saros 114)	July 21, 1906 (Saros 115)	June 19, 1917 (Saros 116)
May 19, 1928 (Saros 117)	April 19, 1939 (Saros 118)	March 18, 1950 (Saros 119)	February 15, 1961 (Saros 120)	January 16, 1972 (Saros 121)
December 15, 1982 (Saros 122)	November 13, 1993 (Saros 123)	October 14, 2004 (Saros 124)	September 13, 2015 (Saros 125)	August 12, 2026 (Saros 126)
July 13, 2037 (Saros 127)	June 11, 2048 (Saros 128)	May 11, 2059 (Saros 129)	April 11, 2070 (Saros 130)	March 10, 2081 (Saros 131)
February 7, 2092 (Saros 132)	January 8, 2103 (Saros 133)	December 8, 2113 (Saros 134)	November 6, 2124 (Saros 135)	October 7, 2135 (Saros 136)
September 6, 2146 (Saros 137)	August 5, 2157 (Saros 138)	July 5, 2168 (Saros 139)	June 5, 2179 (Saros 140)	May 4, 2190 (Saros 141)

Inex series

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2200
January 1, 1824 (Saros 119)	December 11, 1852 (Saros 120)	November 21, 1881 (Saros 121)
November 2, 1910 (Saros 122)	October 12, 1939 (Saros 123)	September 22, 1968 (Saros 124)
September 2, 1997 (Saros 125)	August 12, 2026 (Saros 126)	July 24, 2055 (Saros 127)
July 3, 2084 (Saros 128)	June 13, 2113 (Saros 129)	May 25, 2142 (Saros 130)
May 5, 2171 (Saros 131)	April 14, 2200 (Saros 132)