Saros cycle series 116 for solar eclipses occurred at the Moon's descending node, repeating every 18 years, 11 days, containing 70 eclipses, 53 of which were umbral (all annular). The first eclipse was on 23 June 727 and the last eclipse was on 22 July 1971, making it the last saros cycle to end. (Next cycle to end is Saros 117, which will have its last eclipse in 2054.)
The longest eclipse was 12 minutes 2 seconds on 25 December 1628.
This solar saros was linked to Lunar Saros 109.
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 116 appears in the following table.
Classification | Number | Percent |
---|---|---|
All Umbral eclipses | 53 | 100.00% |
Central (two limits) | 52 | 98.11% |
Central (one limit) | 1 | 1.89% |
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 |
---|---|---|---|---|---|---|---|---|---|---|
116 | 1 | June 23, 727 | 22:34:35 | Partial | 65.4S 161.5W | -1.4763 | 0.1082 | |||
116 | 2 | July 4, 745 | 5:53:18 | Partial | 64.5S 78.2E | -1.4085 | 0.2381 | |||
116 | 3 | July 15, 763 | 13:14:24 | Partial | 63.7S 42.4W | -1.3432 | 0.3625 | |||
116 | 4 | July 25, 781 | 20:37:53 | Partial | 62.9S 163.3W | -1.2802 | 0.4816 | |||
116 | 5 | August 6, 799 | 4:06:08 | Partial | 62.2S 74.8E | -1.2217 | 0.591 | |||
116 | 6 | August 16, 817 | 11:38:18 | Partial | 61.7S 47.8W | -1.167 | 0.6921 | |||
116 | 7 | August 27, 835 | 19:17:30 | Partial | 61.3S 172W | -1.1186 | 0.7805 | |||
116 | 8 | September 7, 853 | 3:02:42 | Partial | 61S 62.3E | -1.0755 | 0.8578 | |||
116 | 9 | September 18, 871 | 10:54:51 | Partial | 60.9S 64.9W | -1.0389 | 0.9224 | |||
116 | 10 | September 28, 889 | 18:54:00 | Partial | 61S 166.1E | -1.0086 | 0.9748 | |||
116 | 11 | October 10, 907 | 3:00:37 | Annular | 62.7S 54.1E | -0.9851 | 0.9869 | 291 | 0m 47s | |
116 | 12 | October 20, 925 | 11:14:00 | Annular | 64.9S 67W | -0.9677 | 0.9827 | 250 | 1m 3s | |
116 | 13 | October 31, 943 | 19:32:08 | Annular | 67.8S 166.7E | -0.9548 | 0.9783 | 265 | 1m 19s | |
116 | 14 | November 11, 961 | 3:56:16 | Annular | 71.3S 35.8E | -0.9475 | 0.9739 | 298 | 1m 35s | |
116 | 15 | November 22, 979 | 12:23:31 | Annular | 75S 98.4W | -0.9439 | 0.9699 | 335 | 1m 49s | |
116 | 16 | December 2, 997 | 20:53:29 | Annular | 78.7S 123.3E | -0.9429 | 0.9663 | 374 | 2m 2s | |
116 | 17 | December 14, 1015 | 5:22:20 | Annular | 82.5S 19.5W | -0.942 | 0.9633 | 407 | 2m 14s | |
116 | 18 | December 24, 1033 | 13:51:14 | Annular | 85.6S 179.6W | -0.9418 | 0.9609 | 434 | 2m 24s | |
116 | 19 | January 4, 1052 | 22:16:17 | Annular | 86.3S 14.2W | -0.9395 | 0.9591 | 446 | 2m 33s | |
116 | 20 | January 15, 1070 | 6:37:03 | Annular | 83.3S 174.7E | -0.9346 | 0.958 | 440 | 2m 42s | |
116 | 21 | January 26, 1088 | 14:50:56 | Annular | 78.9S 29.2E | -0.9249 | 0.9575 | 415 | 2m 50s | |
116 | 22 | February 5, 1106 | 22:58:18 | Annular | 73.6S 106.6W | -0.9106 | 0.9575 | 378 | 2m 59s | |
116 | 23 | February 17, 1124 | 6:56:07 | Annular | 67.5S 123E | -0.8893 | 0.9581 | 335 | 3m 8s | |
116 | 24 | February 27, 1142 | 14:45:00 | Annular | 60.8S 2.9W | -0.8615 | 0.9589 | 293 | 3m 17s | |
116 | 25 | March 9, 1160 | 22:23:38 | Annular | 53.5S 124.9W | -0.8259 | 0.9599 | 256 | 3m 28s | |
116 | 26 | March 21, 1178 | 5:53:15 | Annular | 46S 116.4E | -0.7838 | 0.961 | 225 | 3m 39s | |
116 | 27 | March 31, 1196 | 13:11:09 | Annular | 38.1S 1.4E | -0.7326 | 0.9621 | 200 | 3m 52s | |
116 | 28 | April 11, 1214 | 20:20:49 | Annular | 30.2S 110.8W | -0.6751 | 0.9629 | 180 | 4m 5s | |
116 | 29 | April 22, 1232 | 3:20:16 | Annular | 22.2S 140.3E | -0.6097 | 0.9636 | 165 | 4m 18s | |
116 | 30 | May 3, 1250 | 10:13:11 | Annular | 14.6S 33.6E | -0.5397 | 0.9639 | 155 | 4m 32s | |
116 | 31 | May 13, 1268 | 16:56:23 | Annular | 7.2S 69.9W | -0.4622 | 0.9638 | 148 | 4m 44s | |
116 | 32 | May 24, 1286 | 23:36:15 | Annular | 0.4S 171.9W | -0.3825 | 0.9632 | 144 | 4m 55s | |
116 | 33 | June 4, 1304 | 6:09:36 | Annular | 5.9N 88.6E | -0.2977 | 0.9622 | 144 | 5m 4s | |
116 | 34 | June 15, 1322 | 12:41:47 | Annular | 11.4N 9.8W | -0.2127 | 0.9607 | 146 | 5m 11s | |
116 | 35 | June 25, 1340 | 19:10:38 | Annular | 16N 106.7W | -0.1253 | 0.9586 | 151 | 5m 17s | |
116 | 36 | July 7, 1358 | 1:41:45 | Annular | 19.6N 156.6E | -0.0404 | 0.9562 | 160 | 5m 22s | |
116 | 37 | July 17, 1376 | 8:13:14 | Annular | 22.2N 60.3E | 0.0439 | 0.9533 | 171 | 5m 30s | |
116 | 38 | July 28, 1394 | 14:48:17 | Annular | 23.7N 36.5W | 0.1249 | 0.9501 | 184 | 5m 40s | |
116 | 39 | August 7, 1412 | 21:27:46 | Annular | 24.4N 134.5W | 0.2018 | 0.9465 | 201 | 5m 55s | |
116 | 40 | August 19, 1430 | 4:13:52 | Annular | 24.2N 125.7E | 0.2729 | 0.9428 | 219 | 6m 13s | |
116 | 41 | August 29, 1448 | 11:07:05 | Annular | 23.4N 23.8E | 0.338 | 0.9389 | 239 | 6m 37s | |
116 | 42 | September 9, 1466 | 18:07:54 | Annular | 22.2N 80.5W | 0.3966 | 0.9351 | 260 | 7m 5s | |
116 | 43 | September 20, 1484 | 1:17:55 | Annular | 20.8N 172.4E | 0.4474 | 0.9313 | 283 | 7m 39s | |
116 | 44 | October 1, 1502 | 8:36:17 | Annular | 19.3N 62.8E | 0.4913 | 0.9277 | 306 | 8m 16s | |
116 | 45 | October 11, 1520 | 16:03:20 | Annular | 17.8N 49.4W | 0.5277 | 0.9244 | 329 | 8m 57s | |
116 | 46 | October 22, 1538 | 23:38:41 | Annular | 16.6N 164.1W | 0.5572 | 0.9214 | 351 | 9m 41s | |
116 | 47 | November 2, 1556 | 7:22:13 | Annular | 15.5N 78.9E | 0.5798 | 0.919 | 370 | 10m 24s | |
116 | 48 | November 13, 1574 | 15:12:17 | Annular | 14.8N 40W | 0.597 | 0.9171 | 387 | 11m 3s | |
116 | 49 | December 3, 1592 | 23:07:16 | Annular | 14.5N 160.2W | 0.6102 | 0.9159 | 401 | 11m 36s | |
116 | 50 | December 15, 1610 | 7:06:48 | Annular | 14.7N 78.2E | 0.6195 | 0.9153 | 409 | 11m 56s | |
116 | 51 | December 25, 1628 | 15:08:47 | Annular | 15.4N 44W | 0.6265 | 0.9153 | 413 | 12m 2s | |
116 | 52 | January 5, 1647 | 23:10:59 | Annular | 16.9N 166.5W | 0.6336 | 0.9161 | 413 | 11m 50s | |
116 | 53 | January 16, 1665 | 7:11:51 | Annular | 19.1N 71.2E | 0.642 | 0.9174 | 409 | 11m 24s | |
116 | 54 | January 27, 1683 | 15:10:09 | Annular | 22.1N 50.6W | 0.6526 | 0.9195 | 401 | 10m 44s | |
116 | 55 | February 7, 1701 | 23:04:53 | Annular | 25.9N 171.7W | 0.6663 | 0.9219 | 393 | 9m 55s | |
116 | 56 | February 19, 1719 | 6:52:57 | Annular | 30.5N 68.6E | 0.6856 | 0.925 | 384 | 9m 1s | |
116 | 57 | March 1, 1737 | 14:35:17 | Annular | 36N 50.1W | 0.7099 | 0.9283 | 378 | 8m 4s | |
116 | 58 | March 12, 1755 | 22:09:32 | Annular | 42.2N 167.4W | 0.7413 | 0.9319 | 375 | 7m 7s | |
116 | 59 | March 23, 1773 | 5:36:58 | Annular | 49.3N 76.2E | 0.7785 | 0.9357 | 378 | 6m 13s | |
116 | 60 | April 3, 1791 | 12:55:13 | Annular | 57.1N 39.5W | 0.8236 | 0.9394 | 394 | 5m 21s | |
116 | 61 | April 14, 1809 | 20:07:11 | Annular | 65.8N 157.3W | 0.8742 | 0.9429 | 435 | 4m 35s | |
116 | 62 | April 26, 1827 | 3:11:14 | Annular | 74.8N 73.4E | 0.9316 | 0.9458 | 559 | 3m 53s | |
116 | 63 | May 6, 1845 | 10:09:00 | Annular [1] | 73.4N 110.6W | 0.9945 | 0.9462 | - | 3m 15s | |
116 | 64 | May 17, 1863 | 17:00:45 | Partial | 69.2N 126.8E | 1.0627 | 0.8606 | |||
116 | 65 | May 27, 1881 | 23:48:41 | Partial | 68.2N 13.3E | 1.1345 | 0.737 | |||
116 | 66 | June 8, 1899 | 6:33:43 | Partial | 67.2N 98.9W | 1.2089 | 0.6076 | |||
116 | 67 | June 19, 1917 | 13:16:21 | Partial | 66.2N 150.1E | 1.2857 | 0.4729 | |||
116 | 68 | June 30, 1935 | 19:59:46 | Partial | 65.2N 39.1E | 1.3623 | 0.3375 | |||
116 | 69 | July 11, 1953 | 2:44:14 | Partial | 64.3N 71.7W | 1.4388 | 0.2015 | |||
116 | 70 | July 22, 1971 | 9:31:55 | Partial | 63.5N 177E | 1.513 | 0.0689 |
The Saros cycle series 120 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 eclipses, including 55 umbral eclipses. The series started on 27 May 933 and will end on 7 July 2195. It included 25 annular eclipses between 1059 and 1492, followed by 4 hybrid eclipses between 1510 and 1564, and is currently in a period of 26 total eclipses until 2033. The most recent eclipse was a total eclipse on 20 March 2015 and the next will be a total eclipse on 30 March 2033. The longest duration of totality was 2 minutes, 50 seconds on 9 March 1997 and the longest annular eclipse was 6 minutes 24 seconds on 11 September 1113.
Saros cycle series 110 for solar eclipses occurred at the Moon's descending node, repeating every 18 years, 11 days, containing 72 eclipses, 39 of which were umbral, all annular. This series began on 30 August 463 and ended on 17 October 1743. The annular eclipse with the longest duration was 29 December 1274 lasting 11 minutes and 44 seconds.
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 112 for solar eclipses occurred at the Moon's descending node, repeating every 18 years, 11 days, containing 72 eclipses, 43 of which were umbral. The first eclipse was on 31 July 539 and the last was on 19 September 1819. The longest totality was 7 minutes 20 seconds on 9 June 1062, the longest annular eclipse was 1 minute 1 second on 23 June 1675.
Saros cycle series 113 for solar eclipses occurred at the Moon's ascending node, repeating every 18 years, 11 days, contained 71 eclipses, 40 of which were umbral, all annular. The first eclipse was on 22 July 586 and the last was on 28 August 1848. The eclipse with the longest duration was 9 minutes 32 seconds on 20 November 1397.
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 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.
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 126 for solar eclipses occurs at the Moon's descending node, repeating every 18 years and 11 days, containing 72 eclipses, 41 of which are umbral. The first eclipse was on 10 March 1179 and the last will be on 3 May 2459, lasting 1,280 years. The most recent eclipse was a total eclipse on 1 August 2008 and the next will be a total eclipse on 12 August 2026.
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 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.
Saros cycle series 133 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 72 eclipses, 53 of which are umbral. The first eclipse in the series was on 13 July 1219 and the last will be on 5 September 2499. The most recent eclipse was a total eclipse on 13 November 2012 and the next will be a total eclipse on 25 November 2030.
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. 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.
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 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.
Saros cycle series 146 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 76 eclipses, 41 of which are umbral. The first eclipse of the series was on 19 September 1541 and the last will be on 29 December 2893. The most recent eclipse was a total eclipse on 11 July 2010 and the next will be a total eclipse on 22 July 2028.