Saros cycle series 136 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 eclipses, 56 of which are umbral (6 annular, 6 hybrid, 44 total). The first eclipse in the series was on 14 June 1360 and the last will be on 30 July 2622. The most recent eclipse was a total eclipse on 22 July 2009 and the next will be a total eclipse on 2 August 2027.
The longest totality was 7 minutes 7.74 seconds on 20 June 1955 (also the longest total eclipse of the 20th century) while the longest annular eclipse was just 32 seconds on 8 September 1504.
This series is currently producing the longest total solar eclipses of any active series. It produced the six longest total solar eclipses of the 20th century, three of them over seven minutes long. [2] It also produced the longest total eclipse of the 21st century at 6 min 38.86 sec on 22 July 2009, and overall will produce the 21st century's three longest total eclipses. Each eclipse is getting slightly shorter and this series will be surpassed in total eclipse length by Solar Saros 139 (whose eclipses are getting slightly longer) on May 11, 2078. [3] Saros 136 in turn surpassed the previous longest-eclipse series, Saros 133, with its member event on May 18th, 1901. It produced the most central total eclipse between the years 1209 and 2718 and the greatest magnitude of any eclipse since the year 540 on July 11, 1991.
This solar saros is linked to Lunar Saros 129.
Umbral eclipses (annular, total and hybrid) can be further classified as either: 1) Central (two limits), 2) Central (one limit) or 3) Non-Central (one limit). The statistical distribution of these classes in Saros series 136 appears in the following table.
Classification | Number | Percent |
---|---|---|
All Umbral eclipses | 56 | 100.00% |
Central (two limits) | 56 | 100.00% |
Central (one limit) | 0 | 0.00% |
Non-central (one limit) | 0 | 0.00% |
Note: Dates are given in the Julian calendar prior to 15 October 1582, and in the Gregorian calendar after that.
Saros | Member | Date | Time (Greatest) UTC | Type | Location Lat, Long | Gamma | Mag. | Width (km) | Duration (min:sec) | Ref |
---|---|---|---|---|---|---|---|---|---|---|
136 | 1 | June 14, 1360 | 5:56:04 | Partial | 65.8S 78.2E | -1.5227 | 0.0495 | |||
136 | 2 | June 25, 1378 | 12:45:16 | Partial | 64.8S 34.2W | -1.4392 | 0.1976 | |||
136 | 3 | July 5, 1396 | 19:37:40 | Partial | 63.9S 147.2W | -1.3568 | 0.3449 | |||
136 | 4 | July 17, 1414 | 2:35:03 | Partial | 63.1S 99E | -1.277 | 0.4881 | |||
136 | 5 | July 27, 1432 | 9:39:02 | Partial | 62.4S 16.3W | -1.2011 | 0.625 | |||
136 | 6 | August 7, 1450 | 16:48:49 | Partial | 61.8S 132.8W | -1.1286 | 0.756 | |||
136 | 7 | August 18, 1468 | 0:08:08 | Partial | 61.3S 108.4E | -1.0627 | 0.8753 | |||
136 | 8 | August 29, 1486 | 7:34:56 | Partial | 61S 12.1W | -1.0018 | 0.9856 | |||
136 | 9 | September 8, 1504 | 15:12:15 | Annular | 55.3S 102.6W | -0.9486 | 0.9924 | 83 | 0m 32s | |
136 | 10 | September 19, 1522 | 22:57:33 | Annular | 53.9S 146.1E | -0.9011 | 0.9946 | 42 | 0m 23s | |
136 | 11 | September 30, 1540 | 6:54:11 | Annular | 54.6S 29.2E | -0.862 | 0.996 | 27 | 0m 17s | |
136 | 12 | October 11, 1558 | 14:58:55 | Annular | 56.5S 90.3W | -0.8289 | 0.9971 | 18 | 0m 12s | |
136 | 13 | October 21, 1576 | 23:13:06 | Annular | 59.2S 147.9E | -0.8031 | 0.9981 | 11 | 0m 8s | |
136 | 14 | November 12, 1594 | 7:34:49 | Annular | 62.4S 25.1E | -0.7829 | 0.9991 | 5 | 0m 4s | |
136 | 15 | November 22, 1612 | 16:04:35 | Hybrid | 65.7S 98.4W | -0.7691 | 1.0002 | 1 | 0m 1s | |
136 | 16 | December 4, 1630 | 0:38:59 | Hybrid | 68.7S 139.6E | -0.7585 | 1.0017 | 9 | 0m 7s | |
136 | 17 | December 14, 1648 | 9:17:55 | Hybrid | 70.9S 19.6E | -0.751 | 1.0035 | 18 | 0m 14s | |
136 | 18 | December 25, 1666 | 17:59:16 | Hybrid | 71.6S 98.3W | -0.7452 | 1.0058 | 30 | 0m 24s | |
136 | 19 | January 5, 1685 | 2:42:50 | Hybrid | 70.7S 143.1E | -0.7409 | 1.0086 | 44 | 0m 35s | |
136 | 20 | January 17, 1703 | 11:24:25 | Hybrid [4] | 67.9S 22.2E | -0.7345 | 1.012 | 61 | 0m 50s | |
136 | 21 | January 27, 1721 | 20:05:11 | Total | 64S 102.4W | -0.7269 | 1.0158 | 79 | 1m 7s | |
136 | 22 | February 8, 1739 | 4:41:13 | Total | 59.2S 131E | -0.7149 | 1.0203 | 99 | 1m 27s | |
136 | 23 | February 18, 1757 | 13:14:12 | Total | 53.8S 2.9E | -0.6999 | 1.0251 | 119 | 1m 51s | |
136 | 24 | March 1, 1775 | 21:39:20 | Total | 47.9S 124.8W | -0.6783 | 1.0304 | 139 | 2m 20s | |
136 | 25 | March 12, 1793 | 6:00:07 | Total | 41.7S 107.8E | -0.6524 | 1.0359 | 158 | 2m 51s | |
136 | 26 | March 24, 1811 | 14:12:13 | Total | 35.2S 18W | -0.619 | 1.0416 | 176 | 3m 27s | |
136 | 27 | April 3, 1829 | 22:18:36 | Total | 28.5S 142.6W | -0.5803 | 1.0474 | 192 | 4m 5s | |
136 | 28 | April 15, 1847 | 6:16:13 | Total | 21.6S 95E | -0.5339 | 1.053 | 206 | 4m 44s | |
136 | 29 | April 25, 1865 | 14:08:34 | Total | 14.8S 25.8W | -0.4826 | 1.0584 | 219 | 5m 23s | |
136 | 30 | May 6, 1883 | 21:53:49 | Total | 8.1S 144.6W | -0.425 | 1.0634 | 229 | 5m 58s | |
136 | 31 | May 18, 1901 | 5:33:48 | Total | 1.7S 98.4E | -0.3626 | 1.068 | 238 | 6m 29s | |
136 | 32 | May 29, 1919 | 13:08:55 | Total | 4.4N 16.7W | -0.29549 | 1.07186 | 244.4 | 6m 50.75s | |
136 | 33 | June 8, 1937 | 20:41:02 | Total | 9.9N 130.5W | -0.22532 | 1.07513 | 249.8 | 7m 4.06s | |
136 | 34 | June 20, 1955 | 4:10:42 | Total | 14.8N 117E | -0.15278 | 1.07756 | 253.7 | 7m 7.74s | |
136 | 35 | June 30, 1973 | 11:38:41 | Total | 18.8N 5.6E | -0.07853 | 1.07921 | 256.5 | 7m 3.55s | |
136 | 36 | July 11, 1991 | 19:06:58 | Total | 22N 105.2W | -0.00412 | 1.07997 | 258 | 6m 53.08s | |
136 | 37 | July 22, 2009 | 2:35:14 | Total | 24.2N 144.1E | 0.06977 | 1.07991 | 258.5 | 6m 38.86s | |
136 | 38 | August 2, 2027 | 10:07:50 | Total | 25.5N 33.2E | 0.14209 | 1.07903 | 257.7 | 6m 22.64s | |
136 | 39 | August 12, 2045 | 17:42:39 | Total | 25.9N 78.5W | 0.21161 | 1.07736 | 255.6 | 6m 5.71s | |
136 | 40 | August 24, 2063 | 1:22:11 | Total | 25.6N 168.4E | 0.2771 | 1.075 | 252 | 5m 49s | |
136 | 41 | September 3, 2081 | 9:07:31 | Total | 24.6N 53.6E | 0.3378 | 1.072 | 247 | 5m 33s | |
136 | 42 | September 14, 2099 | 16:57:53 | Total | 23.4N 62.8W | 0.3942 | 1.0684 | 241 | 5m 18s | |
136 | 43 | September 26, 2117 | 0:55:42 | Total | 21.9N 178.4E | 0.4442 | 1.0645 | 233 | 5m 3s | |
136 | 44 | October 7, 2135 | 9:00:03 | Total | 20.3N 57.6E | 0.4884 | 1.0603 | 224 | 4m 50s | |
136 | 45 | October 17, 2153 | 17:12:18 | Total | 18.8N 65.7W | 0.5259 | 1.056 | 214 | 4m 36s | |
136 | 46 | October 29, 2171 | 1:31:03 | Total | 17.6N 169.1E | 0.5577 | 1.0516 | 203 | 4m 23s | |
136 | 47 | November 8, 2189 | 9:57:28 | Total | 16.5N 41.6E | 0.583 | 1.0474 | 192 | 4m 10s | |
136 | 48 | November 20, 2207 | 18:30:26 | Total | 15.8N 87.8W | 0.6027 | 1.0434 | 180 | 3m 56s | |
136 | 49 | December 1, 2225 | 3:08:36 | Total | 15.4N 141.4E | 0.6178 | 1.0398 | 169 | 3m 43s | |
136 | 50 | December 12, 2243 | 11:52:14 | Total | 15.5N 9E | 0.6284 | 1.0365 | 157 | 3m 30s | |
136 | 51 | December 22, 2261 | 20:38:50 | Total | 16.1N 124.2W | 0.636 | 1.0337 | 147 | 3m 17s | |
136 | 52 | January 3, 2280 | 5:28:11 | Total | 17.2N 101.9E | 0.6414 | 1.0314 | 138 | 3m 4s | |
136 | 53 | January 13, 2298 | 14:16:27 | Total | 19N 31.9W | 0.6474 | 1.0296 | 131 | 2m 52s | |
136 | 54 | January 25, 2316 | 23:05:17 | Total | 21.4N 166W | 0.6526 | 1.0282 | 126 | 2m 42s | |
136 | 55 | February 5, 2334 | 7:50:29 | Total | 24.6N 60.8E | 0.6603 | 1.0272 | 122 | 2m 33s | |
136 | 56 | February 16, 2352 | 16:32:06 | Total | 28.5N 71.8W | 0.6709 | 1.0266 | 121 | 2m 25s | |
136 | 57 | February 27, 2370 | 1:07:02 | Total | 33.2N 157E | 0.6865 | 1.0262 | 121 | 2m 17s | |
136 | 58 | March 9, 2388 | 9:36:21 | Total | 38.5N 27E | 0.7064 | 1.026 | 124 | 2m 10s | |
136 | 59 | March 20, 2406 | 17:57:23 | Total | 44.5N 101.3W | 0.7327 | 1.0258 | 128 | 2m 3s | |
136 | 60 | March 31, 2424 | 2:10:10 | Total | 51.3N 131.9E | 0.7652 | 1.0254 | 133 | 1m 55s | |
136 | 61 | April 11, 2442 | 10:14:04 | Total | 58.7N 6.2E | 0.8046 | 1.0248 | 142 | 1m 45s | |
136 | 62 | April 21, 2460 | 18:09:49 | Total | 66.8N 119.8W | 0.8503 | 1.0236 | 154 | 1m 34s | |
136 | 63 | May 3, 2478 | 1:55:59 | Total | 75.7N 107.7E | 0.9034 | 1.0218 | 176 | 1m 20s | |
136 | 64 | May 13, 2496 | 9:34:25 | Total | 81N 70.4W | 0.9622 | 1.0185 | 243 | 1m 2s | |
136 | 65 | May 25, 2514 | 17:04:32 | Partial | 68.5N 123.2E | 1.0272 | 0.9507 | |||
136 | 66 | June 5, 2532 | 0:28:58 | Partial | 67.5N 1.3E | 1.0962 | 0.8224 | |||
136 | 67 | June 16, 2550 | 7:45:35 | Partial | 66.4N 118.1W | 1.1708 | 0.684 | |||
136 | 68 | June 26, 2568 | 14:58:55 | Partial | 65.5N 123.7E | 1.2472 | 0.5426 | |||
136 | 69 | July 7, 2586 | 22:07:07 | Partial | 64.5N 7.2E | 1.327 | 0.3957 | |||
136 | 70 | July 19, 2604 | 5:14:31 | Partial | 63.7N 108.8W | 1.4062 | 0.2509 | |||
136 | 71 | July 30, 2622 | 12:18:09 | Partial | 63N 136.4E | 1.4872 | 0.1039 |
{{cite web}}
: CS1 maint: archived copy as title (link)Saros cycle series 111 for solar eclipses occurred at the Moon's ascending node, repeating every 18 years and 11 days, containing 79 eclipses, 42 of which were umbral. The first eclipse was on 30 August 528 and the last was on 5 Jan 1935. The longest totality was 6 minutes 11 seconds on 9 June 1592 and the longest annular eclipse was 3 minutes 4 seconds on 15 April 907.
Saros cycle series 114 for solar eclipses occurred at the Moon's descending node, repeating every 18 years, 11 days, containing 72 eclipses, 46 of which were umbral. The first eclipse was on 23 July 651 and the last was on 12 September 1931. The longest totality was 4 minutes 18 seconds on 21 April 1697, the longest annular was 4 minutes 33 seconds on 13 February 994.
Saros cycle series 115 for solar eclipses occurred at the Moon's ascending node, repeating every 18 years, 11 days, containing 72 eclipses, 55 of which were umbral. The first eclipse was on 21 June 662 and the last was on 12 August 1942. The longest totality was 6 minutes 24 seconds on 5 July 1293, the longest annular was 1 minute 54 seconds on 27 May 1816.
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Saros cycle series 121 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 eclipses. 55 of these are umbral eclipses. The first eclipse in the series was on 25 April 944 and the last will be on 7 June 2206. The most recent eclipse was an annular eclipse on 7 February 2008 and the next will be an annular eclipse on 17 February 2026.
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Saros cycle series 128 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 73 eclipses, 40 of which are umbral. The first eclipse in the series was on 29 August 984 and the last will be on 1 November 2282. The most recent eclipse was an annular eclipse on 20 May 2012 and the next will be an annular eclipse on 1 June 2030.
Saros cycle series 129 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 80 eclipses, 41 of which are umbral. The first eclipse in the series was on 3 October 1103 and the last will be on 21 February 2528. The most recent eclipse was a hybrid eclipse on 20 April 2023 and the next will be a total eclipse on 30 April 2041.
Saros cycle series 131 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 70 eclipses, 41 of which are umbral. The first eclipse in the series was on 1 August 1125 and the last will be on 2 September 2369. The most recent eclipse was an annular eclipse on 26 January 2009 and the next eclipse will be an annular eclipse on 6 February 2027.
Saros cycle series 132 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 eclipses, 42 of which are umbral. The first eclipse in the series was on 13 August 1208 and the last eclipse will be on 25 September 2470. The most recent eclipse was an annular eclipse on 26 December 2019 and the next will be an annular eclipse on 5 January 2038.
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Saros cycle series 134 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 eclipses, 54 of which are umbral. The first eclipse in the series was on 22 June 1248 and the last will be on 6 August 2510. The most recent was an annular eclipse on 14 October 2023 and the next will be an annular eclipse on 2041 October 25.
Saros cycle series 137 for solar eclipses occurs at the Moon's ascending node. It repeats every 18 years, 11 days, and contains 70 eclipses, 55 of which are umbral eclipses. The first eclipse in the series was on 25 May 1389 and the last will be on 28 June 2633. The most recent eclipse was an annular eclipse on 21 June 2020 and the next will be an annular eclipse on 2 July 2038. The longest duration of totality was 2 minutes, 55 seconds on September 10, 1569 and the longest annular eclipse will be 7 minutes 5 seconds on 28 February 2435. This series has an unusual order of umbral eclipses, with 10 total eclipses followed by 6 hybrid eclipses, 4 annular eclipses, 3 more hybrid eclipses, and then finally 32 annular eclipses.
Saros cycle series 139 for solar eclipses occurs at the Moon's ascending node repeating every 18 years and 11 days, containing 71 eclipses, including 55 umbral eclipses, 12 of which will be hybrid and 43 of which will be total. The first eclipse was on 17 May 1501 and the last will be on 3 July 2763. The most recent eclipse was on 8 April 2024, lasting 4 minutes 28 seconds over central North America, entering in Mexico, crossing the United States, and leaving in eastern Canada, and the next will be on 20 April 2042, lasting 4 minutes 51 seconds over the western Pacific Ocean and passing over western Indonesia, eastern Malaysia, Brunei, and the Philippines.
Saros cycle series 140 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 eclipses, including 47 umbral eclipses. The first eclipse in this series was on 16 April 1512 and the last will be on 1 June 2774. The most recent eclipse was an annular eclipse on 26 February 2017 and the next will be an annular eclipse on 9 March 2035.
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