Solar eclipse of August 2, 2027
A total solar eclipse will occur over much of the central Eastern Hemisphere on Monday, August 2, 2027. 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.
Solar eclipse of August 2, 2027 | |
---|---|
![]() Map | |
Type of eclipse | |
Nature | Total |
Gamma | 0.1421 |
Magnitude | 1.079 |
Maximum eclipse | |
Duration | 383 s (6 min 23 s) |
Coordinates | 25.5°N 33.2°E |
Max. width of band | 258 km (160 mi) |
Times (UTC) | |
Greatest eclipse | 10:07:50 |
References | |
Saros | 136 (38 of 71) |
Catalog # (SE5000) | 9568 |
Path
Totality will commence over the eastern Atlantic Ocean and travel across the Strait of Gibraltar between Spain and Morocco, and continue across parts of North Africa and the Middle East. Major cities and locations under the path of totality will include:[1]
- Cadiz and Malaga, in southern Spain
- Gibraltar
- Tangier, Morocco
- Oran, Algeria
- Sfax, Tunisia
- Benghazi, Libya
- Luxor in central Egypt
- Jeddah and Mecca in southwest Saudi Arabia
- Sana'a in western Yemen
- The tip of the Horn of Africa in extreme northeast Somalia
- Islands in the British Indian Ocean Territory
The maximum duration of totality will be observed in Egypt, approximately 37 miles (60 km) southeast of Luxor, and will last 6 minutes and 22 seconds.[2]
A partial solar eclipse will be visible from the extreme east tip of Maine, United States, far eastern Quebec and the Atlantic Provinces in Canada, southern Greenland, Iceland, Ireland, Great Britain, nearly the entirety of the European continent, all but the southern quarter of Africa, the Middle East, and from South and Southeast Asia.[1]
It will be the first of three total solar eclipses that are observable in Tunisia in the 21st century, passing over the central part of the country.[3] It will be the second total eclipse in Spain within less than a year (after August 2026). Furthermore, an annular eclipse will appear in Spain in January 2028, less than half a year afterwards. National eclipse committee has been established to coordinate eclipse-related activities.[4]
Duration
This is the second longest total solar eclipse in the 21st century, the longest being the total solar eclipse of July 22, 2009, the eclipse previous to this one in Solar Saros 136. However, the longest duration of the 2009 eclipse was 6 minutes and 39.5 seconds on the Pacific Ocean, and the longest duration on land was 6 minutes and 35 seconds on uninhabited North Iwo Jima, a remote Japanese island far from the main islands of Japan, located 1,170 kilometres (730 mi) south of Tokyo. Thus, the duration seen by most observers was shorter than that.[5] The longest duration of this eclipse is 6 minutes and 23.2 seconds, occurring in the northeastern part of Egypt's New Valley Governorate, near its border with Asyut Governorate and Sohag Governorate. The location of the greatest eclipse is about 250 kilometres (160 mi) southeast of it in Red Sea Governorate, with a slightly shorter duration. This is the longest total solar eclipse on easily accessible land in the 21st century. A longer total solar eclipse will not occur until June 3, 2114.[6]
Images
Animated path
Details of totality in some places or cities
Country or Territory | Place or City | Start
of |
Start of total eclipse (Local Time) |
End of total eclipse (Local Time) |
Duration of total eclipse |
End of partial eclipse (Local Time) |
Magnitude |
---|---|---|---|---|---|---|---|
![]() | Tangier | 08:40:33 | 09:44:38 | 09:49:29 | 4 min 50s | 11:00:20 | 1,072 |
![]() | Tarifa | 09:40:50 | 10:45:05 | 10:49:44 | 4 min 39 s | 12:00:42 | 1,072 |
![]() | Tétouan | 08:40:47 | 09:45:10 | 09:50:01 | 4 min 51s | 11:01:10 | 1,072 |
![]() | Cadiz | 09:40:42 | 10:45:18 | 10:48:21 | 3 min 03 s | 11:59:35 | 1,072 |
![]() | Ceuta | 09:40:58 | 10:45:19 | 10:50:07 | 4 min 48 s | 12:01:11 | 1,072 |
![]() | Algeciras | 09:41:01 | 10:45:25 | 10:49:54 | 4 min 29 s | 12:00:59 | 1,072 |
![]() | Gibraltar | 09:41:04 | 10:45:30 | 10:50:01 | 4 min 31 s | 12:01:07 | 1,072 |
![]() | Marbella | 09:41:37 | 10:46:46 | 10:50:05 | 3 min 18 s | 12:01:50 | 1,072 |
![]() | Benalmádena | 09:41:55 | 10:47:26 | 10:50:19 | 2 min 53 s | 12:02:26 | 1,072 |
![]() | Malaga | 09:42:04 | 10:48:07 | 10:50:00 | 1 min 53 s | 12:02:36 | 1,072 |
![]() | Melilla | 09:42:22 | 10:48:12 | 10:52:44 | 4 min 33 s | 12:05:20 | 1,073 |
![]() | Nador | 08:42:22 | 09:48:13 | 09:52:44 | 4 min 31 s | 11:05:21 | 1,073 |
![]() | Motril | 09:42:43 | 10:49:18 | 10:50:59 | 1 min 41 s | 12:04:04 | 1,073 |
![]() | Oujda | 08:42:56 | 09:50:55 | 09:52:27 | 1 min 32 s | 11:07:16 | 1,073 |
![]() | Tlemcen | 08:43:30 | 09:50:56 | 09:54:07 | 3 min 11 s | 11:08:19 | 1,073 |
![]() | Oran | 08:44:26 | 09:51:03 | 09:56:11 | 5 min 08 s | 11:09:22 | 1,073 |
![]() | Bou Saâda | 08:48:46 | 09:57:55 | 10:03:12 | 5 min 17 s | 11:18:30 | 1,075 |
![]() | Blida | 08:47:55 | 09:57:10 | 10:00:01 | 2 min 51 s | 11:15:21 | 1,074 |
![]() | Batna | 08:51:01 | 10:01:03 | 10:06:20 | 5 min 17 s | 11:22:09 | 1,075 |
![]() | Sfax | 08:56:23 | 10:08:46 | 10:14:26 | 5 min 40 s | 11:31:45 | 1,076 |
![]() | Kairouan | 08:55:43 | 10:08:49 | 10:11:33 | 2 min 44 s | 11:29:36 | 1,076 |
![]() | Northeast of Tripoli | 09:59:46 | 11:16:28 | 11:17:23 | 55 s | 12:38:32 | 1,077 |
![]() | Al-Khums | 10:01:17 | 11:18:40 | 11:19:23 | 43 s | 12:40:53 | 1,077 |
![]() | Benghasi | 10:10:41 | 11:27:51 | 11:34:00 | 6 m 09 s | 12:53:15 | 1,078 |
![]() | Siwa Oasis | 11:22:11 | 12:42:33 | 12:48:03 | 5 min 30 s | 14:08:04 | 1,079 |
![]() | Asyut | 11:35:29 | 12:56:52 | 13:02:59 | 6 min 07 s | 14:21:28 | 1,079 |
![]() | Sohag | 11:37:13 | 12:58:44 | 13:05:07 | 6 min 22 s | 14:23:25 | 1,079 |
![]() | Qena | 11:39:51 | 13:01:33 | 13:07:45 | 6 min 12 s | 14:25:48 | 1,079 |
![]() | Luxor | 11:40:12 | 13:02:02 | 13:08:23 | 6 min 21 s | 14:26:30 | 1,079 |
![]() | Jeddah | 12:00:22 | 13:22:16 | 13:28:16 | 6 min 00 s | 14:43:44 | 1,079 |
![]() | Mecca | 12:01:56 | 13:24:02 | 13:29:09 | 5 min 07 s | 14:44:41 | 1,079 |
![]() | Taif | 12:03:32 | 13:26:02 | 13:29:55 | 3 min 53 s | 14:45:43 | 1,079 |
![]() | Abha | 12:13:08 | 13:34:14 | 13:40:07 | 6 min 03 s | 14:53:46 | 1,078 |
![]() | Khamis Mushait | 12:13:26 | 13:34:26 | 13:40:27 | 6 min 01 s | 14:53:51 | 1,078 |
![]() | Jizan | 12:15:13 | 13:38:18 | 13:41:14 | 2 min 56 s | 14:56:09 | 1,078 |
![]() | Sana'a | 12:21:54 | 13:44:11 | 13:46:32 | 2 min 21 s | 15:00:26 | 1,078 |
![]() | Ataq | 12:29:00 | 13:48:10 | 13:53:57 | 5 min 47 s | 15:04:41 | 1,077 |
![]() | Bosaso | 12:39:39 | 13:58:08 | 14:02:10 | 4 min 02 s | 15:11:56 | 1,076 |
![]() | Bandar Beyla | 12:46:05 | 14:04:20 | 14:06:26 | 2 min 08 s | 15:15:55 | 1,076 |
![]() | Salomon Islands, Peros Banhos and Nelsons Island in Chagos Archipelago | 16:37:41 | 17:40:10 | 17:43:29 | 3 min 19 s | 18:39:42 | 1,067 |
Related eclipses
Eclipses in 2027
Solar eclipses 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]
Ascending node | Descending node | |||||
---|---|---|---|---|---|---|
Saros | Map | Gamma | Saros | Map | Gamma | |
121 | 2026 February 17![]() Annular |
−0.97427 | 126 | 2026 August 12![]() Total |
0.89774 | |
131 | 2027 February 6![]() Annular |
−0.29515 | 136 | 2027 August 2![]() Total |
0.14209 | |
141 | 2028 January 26![]() Annular |
0.39014 | 146 | 2028 July 22![]() Total |
−0.60557 | |
151 | 2029 January 14![]() Partial |
1.05532 | 156 | 2029 July 11![]() Partial |
−1.41908 |
Partial solar eclipses on June 12, 2029, and December 5, 2029, occur in the next lunar year eclipse set.
Saros 136
Solar Saros 136, repeating every 18 years, 11 days, contains 71 events. The series started with partial solar eclipse on June 14, 1360, and reached a first annular eclipse on September 8, 1504. It was a hybrid event from November 22, 1612, through January 17, 1703, and total eclipses from January 27, 1721, through May 13, 2496. The series ends at member 71 as a partial eclipse on July 30, 2622, with the entire series lasting 1262 years. The longest eclipse occurred on June 20, 1955, with a maximum duration of totality at 7 minutes, 7.74 seconds. All eclipses in this series occurs at the Moon's descending node.[8]
Series members 29–43 occur between 1865 and 2117 | ||
---|---|---|
29 | 30 | 31 |
![]() Apr 25, 1865 |
![]() May 6, 1883 |
![]() May 18, 1901 |
32 | 33 | 34 |
![]() May 29, 1919 |
![]() Jun 8, 1937 |
![]() Jun 20, 1955 |
35 | 36 | 37 |
![]() Jun 30, 1973 |
![]() Jul 11, 1991 |
![]() Jul 22, 2009 |
38 | 39 | 40 |
![]() Aug 2, 2027 |
![]() Aug 12, 2045 |
![]() Aug 24, 2063 |
41 | 42 | 43 |
![]() Sep 3, 2081 |
![]() Sep 14, 2099 |
![]() Sep 26, 2117 |
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.[9]
Octon series with 21 events between May 21, 1993 and August 2, 2065 | ||||
---|---|---|---|---|
May 20–21 | March 8–9 | December 25–26 | October 13–14 | August 1–2 |
98 | 100 | 102 | 104 | 106 |
May 21, 1955 | March 9, 1959 | December 26, 1962 | October 14, 1966 | August 2, 1970 |
108 | 110 | 112 | 114 | 116 |
May 21, 1974 | March 9, 1978 | December 26, 1981 | October 14, 1985 | August 1, 1989 |
118 | 120 | 122 | 124 | 126 |
![]() May 21, 1993 |
![]() March 9, 1997 |
![]() December 25, 2000 |
![]() October 14, 2004 |
![]() August 1, 2008 |
128 | 130 | 132 | 134 | 136 |
![]() May 20, 2012 |
![]() March 9, 2016 |
![]() December 26, 2019 |
![]() October 14, 2023 |
![]() August 2, 2027 |
138 | 140 | 142 | 144 | 146 |
![]() May 21, 2031 |
![]() March 9, 2035 |
![]() December 26, 2038 |
![]() October 14, 2042 |
![]() August 2, 2046 |
148 | 150 | 152 | 154 | 156 |
![]() May 20, 2050 |
![]() March 9, 2054 |
![]() December 26, 2057 |
![]() October 13, 2061 |
![]() August 2, 2065 |
158 | 160 | 162 | 164 | 166 |
![]() May 20, 2069 |
March 8, 2073 | December 26, 2076 | October 13, 2080 | August 1, 2084 |
References
- "Total Solar Eclipse on August 2, 2027: Path Map and Times". www.timeanddate.com. Retrieved 2024-03-23.
- "Longest Duration of Total Solar Eclipse of 2027 Aug 02". NASA Goddard Space Flight Center. NASA. Retrieved 7 September 2017.
- "Map of Solar Eclipse of August 2, 2027" (Map). "Solar Eclipse Maps". NASA. Retrieved October 21, 2017.
- https://eclipse-spain.es/index.php/en/
- Fred Espenak. "Total Solar Eclipse of 2009 Jul 22 - Google Maps and Solar Eclipse Paths". NASA Eclipse Web Site. Archived from the original on 22 July 2009.
- Fred Espenak. "Total Solar Eclipses with Durations Exceeding 06m 00s: 2001 to 3000". NASA Eclipse Web Site. Archived from the original on 10 March 2014.
- van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
- SEsaros136 at NASA.gov
- Note S1: Eclipses & Predictions in Freeth, Tony (2014). "Eclipse Prediction on the Ancient Greek Astronomical Calculating Machine Known as the Antikythera Mechanism". PLOS ONE. 9 (7): e103275. Bibcode:2014PLoSO...9j3275F. doi:10.1371/journal.pone.0103275. PMC 4116162. PMID 25075747.
