Saros cycle series 136 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 events. All eclipses in this series occurs at the Moon's descending node.
This solar saros is linked to Lunar Saros 129.
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. [2]
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 |
Solar Saros 136 is for now producing the longest total solar eclipses. It produced the six longest total solar eclipses of the 20th century, three of them over seven minutes long. [3] It also produced the longest total eclipse of the 21st century at 6 min 38.86 sec, and overall will produce the 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. [4] Saros 136 in turn surpassed the previous longest-eclipse series, Saros 133, with its member event on May 18th, 1901. Saros 136 will ultimately produce a total of 44 total eclipses. 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. All eclipses in this series occurs at the Moon's descending node. Solar Saros 136 contains 71 events of which 15 will be partial eclipses, and the remaning 56 will be umbral: 6 annular, 6 hybrid and 44 total.
Like all saroi, Solar Saros 136 repeats every 18 years, 11 days, 8 hours.
Occurred at the Moon's descending node, the same as even-numbered saroi, such as Solar Saros 134 and 138.
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% |
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 | 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)The Saros cycle series 120 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 events. 55 of these are umbral eclipses. The series started with a partial solar eclipse on May 27, 933 AD, and transitioned into an annular eclipse on August 11, 1059. It was a hybrid event for 3 dates: May 8, 1510, through May 29, 1546, and are total eclipses from June 8, 1564 through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. The longest duration of totality was 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occurs at the Moon's descending node.
Saros cycle series 118 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 72 events. All eclipses in this series occurs at the Moon's descending node.
Saros cycle series 119 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 events. All eclipses in this series occurs at the Moon's ascending node.
Saros cycle series 132 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 events. All eclipses in this series occurs at the Moon's descending node.
Saros cycle series 133 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 72 events. All eclipses in this series occurs at the Moon's ascending node.
Saros cycle series 134 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 events. All eclipses in this series occurs at the Moon's descending node.
Saros cycle series 135 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days. Solar Saros 135 contains 71 events in which of 18 will be partial eclipses and 53 will be umbral eclipses. All eclipses in this series occurs at the Moon's ascending node.
Saros cycle series 137 for solar eclipses occurs at the Moon's ascending node. It repeats every 18 years, 11 days, and contains 70 events. 55 of these are umbral eclipses and other 15 of these are partial solar eclipses. All eclipses in this series occurs at the Moon's ascending node.
Saros cycle series 138 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 70 events. 16 of these are partial solar eclipses. All eclipses in this series occurs at the Moon's descending node.
Saros cycle series 139 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 events. It has 16 partial solar eclipses, 12 will be hybrid and 43 will be total. The first total eclipse occurred on December 21, 1843 over southern Asia and lasted 1 minute and 43 seconds. The last total eclipse will occur on March 26, 2601 over Antarctica and the Southern Ocean lasting 35 seconds.
Saros cycle series 140 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 events. All eclipses in this series occurs at the Moon's descending node.
Saros cycle series 142 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, contains 72 events. 41 of these are total eclipses, the longest of which occurs on May 28, 2291 and will last 6 minutes 34 seconds. All eclipses in this series occurs at the Moon's descending node. Unlike Saros 145, this Solar Saros series is also producing young total solar eclipses with less than 3 minutes length until the Solar eclipse of January 27, 2093.
Saros cycle series 143 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years and 11 days, containing 72 events. It consisted of 10 partial eclipses, 12 total eclipses, 4 hybrid events, 26 annular eclipses, and ends with 20 partial eclipses. The longest total eclipse of the series was in 1887 at 3 minutes and 50 seconds. All eclipses in this series occurs at the Moon's ascending node.
Saros cycle series 144 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 70 events. All eclipses in this series occur at the Moon's descending node.
Saros cycle series 145 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 77 events. It is currently a young cycle producing total eclipses less than 3 minutes in length. The series started with a partial solar eclipse on January 4, 1639, and reached a first annular eclipse on June 6, 1891. It was a hybrid event on June 17, 1909, and total eclipses from June 29, 1927, through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. The longest duration eclipse in the cycle will be member 50 at 7 minutes and 12 seconds in length on June 25, 2522, after which the durations of eclipses will decrease until the end of the cycle. In its central phase it will produce mainly total eclipses. All eclipses in this series occur at the Moon's ascending node.
Saros cycle series 146 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 76 events. All eclipses in this series occurs at the Moon's descending node.
Saros cycle series 147 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 80 events. All eclipses in this series occurs at the Moon's ascending node.
Saros cycle series 150 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 events. All eclipses in this series occurs at the Moon's descending node.
Saros cycle series 154 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 events, with 61 before 3000 AD. All eclipses in this series occurs at the Moon's descending node.
Saros cycle series 155 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days. Saros 155 contains 71 events in which of 15 will be partial solar eclipses and other 56 are umbral. There are 60 solar eclipses before 3000 AD. All eclipses in this series occurs at the Moon's ascending node.