Saros cycle series 150 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 eclipses, 40 of which are umbral (all annular). The first eclipse in the series was on 24 August 1729 and the last will be on 29 September 2991. The most recent eclipse was a partial eclipse on 15 February 2018 and the next will be a partial eclipse on 27 February 2036. The longest duration of annularity will be 9 minutes, 58 seconds on December 19, 2522.
This solar saros is linked to Lunar Saros 143.
Series members 11-21 occurring between 1901 and 2100: | ||
---|---|---|
11 | 12 | 13 |
December 12, 1909 | December 24, 1927 | January 3, 1946 |
14 | 15 | 16 |
January 14, 1964 | January 25, 1982 | February 5, 2000 |
17 | 18 | 19 |
February 15, 2018 | February 27, 2036 | March 9, 2054 |
20 | 21 | |
March 19, 2072 | March 31, 2090 |
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 150 appears in the following table.
Classification | Number | Percent |
---|---|---|
All Umbral eclipses | 40 | 100.00% |
Central (two limits) | 39 | 97.50% |
Central (one limit) | 0 | 0.00% |
Non-central (one limit) | 1 | 2.50% |
Saros | Member | Date | Time (Greatest) UTC | Type | Location Lat, Long | Gamma | Mag. | Width (km) | Duration (min:sec) | Ref |
---|---|---|---|---|---|---|---|---|---|---|
150 | 1 | August 24, 1729 | 13:48:31 | Partial | 61.7S 95.2W | -1.543 | 0.0067 | |||
150 | 2 | September 4, 1747 | 21:07:57 | Partial | 61.4S 146.1E | -1.488 | 0.1086 | |||
150 | 3 | September 15, 1765 | 4:32:34 | Partial | 61.1S 26.2E | -1.4378 | 0.2009 | |||
150 | 4 | September 26, 1783 | 12:04:17 | Partial | 61.1S 95.4W | -1.3935 | 0.2814 | |||
150 | 5 | October 7, 1801 | 19:42:34 | Partial | 61.2S 141.3E | -1.3552 | 0.3505 | |||
150 | 6 | October 19, 1819 | 3:27:17 | Partial | 61.5S 16.4E | -1.3226 | 0.4085 | |||
150 | 7 | October 29, 1837 | 11:19:24 | Partial | 61.9S 110.5W | -1.2967 | 0.4542 | |||
150 | 8 | November 9, 1855 | 19:17:51 | Partial | 62.5S 121E | -1.2767 | 0.4892 | |||
150 | 9 | November 20, 1873 | 3:22:52 | Partial | 63.2S 9.5W | -1.2625 | 0.5138 | |||
150 | 10 | December 1, 1891 | 11:31:08 | Partial | 64.1S 140.9W | -1.2515 | 0.5326 | |||
150 | 11 | December 12, 1909 | 19:44:48 | Partial | 65S 86E | -1.2456 | 0.5424 | |||
150 | 12 | December 24, 1927 | 3:59:41 | Partial | 66.1S 47.7W | -1.2416 | 0.549 | |||
150 | 13 | January 3, 1946 | 12:16:11 | Partial | 67.1S 177.6E | -1.2392 | 0.5529 | |||
150 | 14 | January 14, 1964 | 20:30:08 | Partial | 68.2S 43.1E | -1.2354 | 0.5591 | |||
150 | 15 | January 25, 1982 | 4:42:53 | Partial | 69.3S 91.7W | -1.2311 | 0.5663 | |||
150 | 16 | February 5, 2000 | 12:50:27 | Partial | 70.2S 134.1E | -1.2233 | 0.5795 | |||
150 | 17 | February 15, 2018 | 20:52:33 | Partial | 71S 0.6E | -1.2116 | 0.5991 | |||
150 | 18 | February 27, 2036 | 4:46:49 | Partial | 71.6S 131.4W | -1.1942 | 0.6286 | |||
150 | 19 | March 9, 2054 | 12:33:40 | Partial | 72S 97.9E | -1.1711 | 0.6678 | |||
150 | 20 | March 19, 2072 | 20:10:31 | Partial | 72.2S 30.4W | -1.1405 | 0.7199 | |||
150 | 21 | March 31, 2090 | 3:38:08 | Partial | 72.1S 156.3W | -1.1028 | 0.7843 | |||
150 | 22 | April 11, 2108 | 10:55:37 | Partial | 71.7S 80.5E | -1.0573 | 0.862 | |||
150 | 23 | April 22, 2126 | 18:04:22 | Annular [lower-alpha 1] | 71.1S 40W | 1.0051 | 0.9514 | - | - | |
150 | 24 | May 3, 2144 | 1:02:06 | Annular | 53.6S 175.9W | -0.9441 | 0.9363 | 727 | 6m 9s | |
150 | 25 | May 14, 2162 | 7:52:46 | Annular | 42.3S 72.8E | -0.8775 | 0.9396 | 468 | 6m 37s | |
150 | 26 | May 24, 2180 | 14:34:28 | Annular | 32.6S 32.9W | -0.8035 | 0.9422 | 359 | 6m 59s | |
150 | 27 | June 4, 2198 | 21:11:35 | Annular | 24.2S 135.7W | -0.726 | 0.9442 | 299 | 7m 13s | |
150 | 28 | June 16, 2216 | 3:41:04 | Annular | 16.7S 124.6E | -0.642 | 0.9458 | 260 | 7m 20s | |
150 | 29 | June 27, 2234 | 10:09:34 | Annular | 10.3S 26.1E | -0.5572 | 0.9468 | 235 | 7m 18s | |
150 | 30 | July 7, 2252 | 16:34:12 | Annular | 4.9S 70.6W | -0.4686 | 0.9473 | 218 | 7m 10s | |
150 | 31 | July 18, 2270 | 22:59:54 | Annular | 0.7S 166.9W | -0.3811 | 0.9474 | 208 | 6m 57s | |
150 | 32 | July 29, 2288 | 5:25:23 | Annular | 2.5N 97.4E | -0.293 | 0.9469 | 203 | 6m 46s | |
150 | 33 | August 10, 2306 | 11:55:10 | Annular | 4.6N 1E | -0.2083 | 0.9461 | 202 | 6m 37s | |
150 | 34 | August 20, 2324 | 18:28:22 | Annular | 5.7N 96W | -0.1261 | 0.9449 | 205 | 6m 33s | |
150 | 35 | September 1, 2342 | 1:06:55 | Annular | 6.1N 165.7E | -0.048 | 0.9434 | 209 | 6m 34s | |
150 | 36 | September 11, 2360 | 7:52:25 | Annular | 5.7N 65.6E | 0.0244 | 0.9415 | 217 | 6m 41s | |
150 | 37 | September 22, 2378 | 14:45:48 | Annular | 4.8N 36.6W | 0.0904 | 0.9396 | 225 | 6m 54s | |
150 | 38 | October 2, 2396 | 21:48:07 | Annular | 3.5N 141.2W | 0.1493 | 0.9375 | 234 | 7m 12s | |
150 | 39 | October 14, 2414 | 4:58:50 | Annular | 2.2N 111.8E | 0.2015 | 0.9355 | 245 | 7m 34s | |
150 | 40 | October 24, 2432 | 12:19:58 | Annular | 0.8N 2.1E | 0.2455 | 0.9335 | 255 | 8m 1s | |
150 | 41 | November 4, 2450 | 19:49:31 | Annular | 0.5S 109.9W | 0.2828 | 0.9318 | 264 | 8m 30s | |
150 | 42 | November 15, 2468 | 3:28:23 | Annular | 1.5S 135.7E | 0.3126 | 0.9304 | 273 | 8m 59s | |
150 | 43 | November 26, 2486 | 11:15:08 | Annular | 2.1S 19.2E | 0.3363 | 0.9294 | 280 | 9m 26s | |
150 | 44 | December 7, 2504 | 19:10:09 | Annular | 2.3S 99.5W | 0.3535 | 0.9289 | 284 | 9m 46s | |
150 | 45 | December 19, 2522 | 3:10:40 | Annular | 2S 140.4E | 0.3668 | 0.9289 | 286 | 9m 58s | |
150 | 46 | December 29, 2540 | 11:15:59 | Annular | 1S 19E | 0.3765 | 0.9295 | 285 | 9m 57s | |
150 | 47 | January 9, 2559 | 19:24:29 | Annular | 0.6N 103.4W | 0.3841 | 0.9308 | 280 | 9m 43s | |
150 | 48 | January 20, 2577 | 3:35:00 | Annular | 2.8N 133.7E | 0.3901 | 0.9326 | 273 | 9m 18s | |
150 | 49 | January 31, 2595 | 11:44:03 | Annular | 5.9N 10.9E | 0.3981 | 0.9352 | 263 | 8m 42s | |
150 | 50 | February 11, 2613 | 19:51:44 | Annular | 9.6N 111.8W | 0.4076 | 0.9382 | 250 | 8m 0s | |
150 | 51 | February 23, 2631 | 3:55:11 | Annular | 14N 126.3E | 0.4211 | 0.9419 | 236 | 7m 13s | |
150 | 52 | March 5, 2649 | 11:55:21 | Annular | 19N 5.2E | 0.4378 | 0.946 | 220 | 6m 25s | |
150 | 53 | March 16, 2667 | 19:47:40 | Annular | 24.6N 114.3W | 0.4613 | 0.9506 | 203 | 5m 36s | |
150 | 54 | March 27, 2685 | 3:35:09 | Annular | 30.7N 127.5E | 0.4895 | 0.9554 | 185 | 4m 48s | |
150 | 55 | April 8, 2703 | 11:13:59 | Annular | 37.2N 11.4E | 0.5256 | 0.9605 | 167 | 4m 1s | |
150 | 56 | April 18, 2721 | 18:47:26 | Annular | 44.1N 103.1W | 0.5665 | 0.9657 | 150 | 3m 17s | |
150 | 57 | April 30, 2739 | 2:11:56 | Annular | 51.4N 145E | 0.6157 | 0.9708 | 133 | 2m 37s | |
150 | 58 | May 10, 2757 | 9:32:11 | Annular | 58.9N 35.1E | 0.669 | 0.9758 | 116 | 2m 1s | |
150 | 59 | May 21, 2775 | 16:45:20 | Annular | 66.7N 71.6W | 0.7292 | 0.9804 | 102 | 1m 31s | |
150 | 60 | May 31, 2793 | 23:54:30 | Annular | 74.7N 173.3W | 0.7933 | 0.9846 | 90 | 1m 6s | |
150 | 61 | June 12, 2811 | 6:58:46 | Annular | 82.8N 102.4E | 0.8623 | 0.988 | 84 | 0m 47s | |
150 | 62 | June 22, 2829 | 14:01:25 | Annular | 83.4N 97.9E | 0.9335 | 0.9904 | 97 | 0m 35s | |
150 | 63 | July 3, 2847 | 21:02:28 | Partial | 64.9N 33.4E | 1.0066 | 0.9775 | |||
150 | 64 | July 14, 2865 | 4:03:03 | Partial | 64N 80.8W | 1.0808 | 0.8446 | |||
150 | 65 | July 25, 2883 | 11:05:22 | Partial | 63.3N 164.7E | 1.1544 | 0.7116 | |||
150 | 66 | August 5, 2901 | 18:10:19 | Partial | 62.6N 49.9E | 1.2266 | 0.5801 | |||
150 | 67 | August 17, 2919 | 1:18:50 | Partial | 62.1N 65.7W | 1.2963 | 0.4526 | |||
150 | 68 | August 27, 2937 | 8:32:10 | Partial | 61.7N 177.6E | 1.3627 | 0.3306 | |||
150 | 69 | September 7, 2955 | 15:51:40 | Partial | 61.4N 59.5E | 1.4246 | 0.2164 | |||
150 | 70 | September 17, 2973 | 23:18:46 | Partial | 61.3N 60.5W | 1.4812 | 0.1119 | |||
150 | 71 | September 29, 2991 | 6:52:19 | Partial | 61.4N 178E | 1.5333 | 0.0156 |
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 117 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 eclipses, including 56 umbral eclipses. The first eclipse in this series was on June 24, 792 AD. The final eclipse in this series will be on August 3, 2054. The most recent eclipse was a partial eclipse on 13 July 2018 and the next one will be a partial eclipse on 23 July 2036.
Saros cycle series 118 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 72 eclipses, including 57 umbral eclipses. The first eclipse was on 24 May 803 and the last will be on 15 July 2083. The most recent eclipse was a partial eclipse on 1 June 2011 and the next will be a partial eclipse on 12 June 2029.
Saros cycle series 119 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 eclipses, including 54 umbral eclipses. The first eclipse was on 15 May 850 and the last will be on 24 June 2112. The most recent eclipse was a partial eclipse on 30 April 2022 and the next will be a partial eclipse on 11 May 2040. The longest duration of totality was only 32 seconds on August 20, 1012. The longest duration of annularity was 7 minutes, 37 seconds on September 1, 1625.
Saros cycle series 122 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 70 eclipses, 42 of which are umbral. The first eclipse was on 17 April 991 and the last will be on 17 May 2235. The most recent eclipse was a partial eclipse on 6 January 2019 and the next will be a partial eclipse on 16 January 2037.
Saros cycle series 123 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 70 eclipses, 44 of which are umbral. The first eclipse in the series was on 29 April 1074 and the last will be on 31 May 2318. The most recent eclipse was a partial eclipse on 25 November 2011 and the next will be a partial eclipse on 5 December 2029.
Saros cycle series 124 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 73 eclipses, 44 of which are umbral. The first eclipse in the series was on 6 March 1049 and the last will be on 11 May 2347. The most recent eclipse was a partial eclipse on 25 October 2022 and the next will be a partial eclipse on 4 November 2040.
Saros cycle series 125 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 73 eclipses, 40 of which are umbral. The first eclipse in the series was on 4 February 1060 and the last will be on 9 April 2358. The most recent eclipse was a partial eclipse on 13 September 2015 and the next will be a partial eclipse on 23 September 2033.
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 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 138 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 70 eclipses, 54 of which are umbral. The first eclipse of the series was on 6 June 1472 and the last will be on 11 July 2716. The most recent eclipse was an annular eclipse on 10 May 2013 and the next will be an annular eclipse on 21 May 2031.
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.
Saros cycle series 149 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 eclipses, 43 of which are umbral. The first eclipse in the series was on 21 August 1664 and the last will be on 28 September 2926. The most recent eclipse was a partial eclipse on 19 March 2007 and the next will be a partial eclipse on 29 March 2025.
Saros cycle series 151 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 72 eclipses, 46 of which will be umbral. The first eclipse in the series was on 14 August 1776 and the last will be on 1 October 3056. The most recent eclipse was a partial eclipse on 4 January 2011 and the next will be a partial eclipse on 14 January 2029.
Saros cycle series 152 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 70 eclipses, 55 of which will be umbral. The first eclipse in the series was on 26 July 1806 and the last will be on 20 August 3049. The most recent eclipse was a total eclipse on 4 December 2021 and the next will be a total eclipse on 15 December 2039.
Saros cycle series 153 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 70 eclipses, 49 of which will be umbral, all annular. The first eclipse in the series was on 28 July 1870 and the last will be on 22 August 3114. The most recent eclipse was a partial eclipse on 23 October 2014 and the next will be a partial eclipse on 3 November 2032.
Saros cycle series 154 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 eclipses, 56 of which will be umbral. The first eclipse in the series was on 19 July 1917 and the last eclipse will be on 25 August 3179. The most recent was a partial eclipse on 11 September 2007 and the next will be a partial eclipse on 21 September 2025.
Saros cycle series 155 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 eclipses, 56 of which will be umbral. The first eclipse in the series was on 17 June 1928 and the last will be on 24 July 3190. The most recent eclipse was a partial eclipse on 11 August 2018 and the next will be a partial eclipse on 21 August 2036.
Saros cycle series 156 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 69 eclipses, 52 of which will be umbral. The first, and so far only, eclipse in the series was on 1 July 2011 and the last will be on 14 July 3237. The next eclipse will be a partial eclipse on 11 July 2029. This series is the most recent series to begin.
Saros cycle series 157 for solar eclipses will at the Moon's ascending node, repeating every 18 years, 11 days, containing 70 eclipses, 56 of which will be umbral. The first eclipse will occur on 21 June 2058 and the last will be on 17 July 3302.