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 (8 total, 16 hybrid, and 30 annular). 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.
The longest totality was 1 minute 30 seconds on 9 October 1428 and the longest annular will be 10 minutes 55 seconds on 10 January 2168.
This series is linked to Lunar Saros 127.
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 134 appears in the following table.
Classification | Number | Percent |
---|---|---|
All Umbral eclipses | 54 | 100.00% |
Central (two limits) | 53 | 98.15% |
Central (one limit) | 1 | 1.85% |
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 |
---|---|---|---|---|---|---|---|---|---|---|
134 | 1 | June 22, 1248 | 19:09:36 | Partial | 65.2S 125.9W | −1.5159 | 0.0223 | |||
134 | 2 | July 4, 1266 | 2:38:30 | Partial | 64.3S 111.8E | −1.4464 | 0.1578 | |||
134 | 3 | July 14, 1284 | 10:08:18 | Partial | 63.4S 10.4W | −1.3779 | 0.2915 | |||
134 | 4 | July 25, 1302 | 17:42:30 | Partial | 62.7S 133.4W | −1.3129 | 0.4178 | |||
134 | 5 | August 5, 1320 | 1:20:21 | Partial | 62.1S 102.9E | −1.251 | 0.5375 | |||
134 | 6 | August 16, 1338 | 9:03:11 | Partial | 61.6S 21.9W | −1.1933 | 0.6482 | |||
134 | 7 | August 26, 1356 | 16:52:10 | Partial | 61.2S 148.1W | −1.141 | 0.7477 | |||
134 | 8 | September 7, 1374 | 0:48:07 | Partial | 61S 84E | −1.0949 | 0.8345 | |||
134 | 9 | September 17, 1392 | 8:51:03 | Partial | 61S 45.5W | −1.0548 | 0.9092 | |||
134 | 10 | September 28, 1410 | 17:00:48 | Partial | 61.1S 176.7W | −1.0206 | 0.9718 | |||
134 | 11 | October 9, 1428 | 1:18:10 | Total [lower-alpha 1] | 63S 61E | −0.993 | 1.0281 | - | 1m 30s | |
134 | 12 | October 20, 1446 | 9:42:45 | Total | 65.8S 56.8W | −0.9718 | 1.0258 | 386 | 1m 25s | |
134 | 13 | October 30, 1464 | 18:13:13 | Total | 68.9S 176E | −0.956 | 1.0225 | 267 | 1m 14s | |
134 | 14 | November 11, 1482 | 2:49:49 | Total | 72.5S 44E | −0.9457 | 1.0189 | 203 | 1m 3s | |
134 | 15 | November 21, 1500 | 11:30:31 | Total | 76.4S 91.4W | −0.9393 | 1.0156 | 159 | 0m 52s | |
134 | 16 | December 2, 1518 | 20:14:58 | Total | 80.4S 128.7E | −0.9365 | 1.0124 | 125 | 0m 41s | |
134 | 17 | December 13, 1536 | 4:59:20 | Total | 84.5S 17.2W | −0.9343 | 1.0098 | 97 | 0m 33s | |
134 | 18 | December 24, 1554 | 13:45:21 | Total | 87.5S 159.2E | −0.9341 | 1.0075 | 75 | 0m 25s | |
134 | 19 | January 3, 1573 | 22:28:35 | Hybrid | 85.9S 54.1W | −0.9328 | 1.0058 | 57 | 0m 20s | |
134 | 20 | January 25, 1591 | 7:09:22 | Hybrid | 81.9S 150.6E | −0.9298 | 1.0047 | 45 | 0m 16s | |
134 | 21 | February 4, 1609 | 15:43:43 | Hybrid | 77.3S 7.2E | −0.9224 | 1.0041 | 37 | 0m 15s | |
134 | 22 | February 16, 1627 | 0:13:31 | Hybrid | 72.3S 130.9W | −0.9119 | 1.004 | 34 | 0m 15s | |
134 | 23 | February 26, 1645 | 8:35:06 | Hybrid | 66.7S 94.3E | −0.8956 | 1.0043 | 34 | 0m 17s | |
134 | 24 | March 9, 1663 | 16:48:41 | Hybrid | 60.5S 37.1W | −0.8735 | 1.0049 | 35 | 0m 21s | |
134 | 25 | March 20, 1681 | 0:52:59 | Hybrid | 53.8S 165.3W | −0.8445 | 1.0057 | 37 | 0m 26s | |
134 | 26 | March 31, 1699 | 8:48:45 | Hybrid | 46.8S 69.7E | −0.8089 | 1.0065 | 38 | 0m 32s | |
134 | 27 | April 11, 1717 | 16:34:40 | Hybrid | 39.5S 52.1W | −0.766 | 1.0072 | 39 | 0m 39s | |
134 | 28 | April 23, 1735 | 0:11:36 | Hybrid | 32.2S 171W | −0.7164 | 1.0077 | 38 | 0m 44s | |
134 | 29 | May 3, 1753 | 7:39:40 | Hybrid | 24.9S 73E | −0.6601 | 1.0079 | 36 | 0m 48s | |
134 | 30 | May 14, 1771 | 15:00:02 | Hybrid | 17.8S 40.4W | −0.598 | 1.0076 | 33 | 0m 49s | |
134 | 31 | May 24, 1789 | 22:11:58 | Hybrid | 11S 151W | −0.5297 | 1.0068 | 28 | 0m 46s | |
134 | 32 | June 6, 1807 | 5:18:31 | Hybrid | 4.7S 100.4E | −0.4577 | 1.0055 | 21 | 0m 38s | |
134 | 33 | June 16, 1825 | 12:19:03 | Hybrid | 1N 6W | −0.3812 | 1.0036 | 13 | 0m 25s | |
134 | 34 | June 27, 1843 | 19:17:03 | Hybrid | 5.9N 111W | −0.3037 | 1.0011 | 4 | 0m 7s | |
134 | 35 | July 8, 1861 | 2:10:26 | Annular | 10N 145.8E | −0.2231 | 0.9979 | 7 | 0m 14s | |
134 | 36 | July 19, 1879 | 9:04:32 | Annular | 13N 42.9E | −0.1439 | 0.9942 | 20 | 0m 39s | |
134 | 37 | July 29, 1897 | 15:56:58 | Annular | 15.3N 59W | −0.064 | 0.9899 | 35 | 1m 5s | |
134 | 38 | August 10, 1915 | 22:52:25 | Annular | 16.4N 161.4W | 0.0124 | 0.9853 | 52 | 1m 33s | |
134 | 39 | August 21, 1933 | 5:49:11 | Annular | 16.9N 95.9E | 0.0869 | 0.9801 | 71 | 2m 4s | |
134 | 40 | September 1, 1951 | 12:51:51 | Annular | 16.5N 8.5W | 0.1557 | 0.9747 | 91 | 2m 36s | |
134 | 41 | September 11, 1969 | 19:58:59 | Annular | 15.6N 114.1W | 0.2201 | 0.969 | 114 | 3m 11s | |
134 | 42 | September 23, 1987 | 3:12:22 | Annular | 14.3N 138.4E | 0.2787 | 0.9634 | 137 | 3m 49s | |
134 | 43 | October 3, 2005 | 10:32:47 | Annular | 12.9N 28.7E | 0.3306 | 0.9576 | 162 | 4m 32s | |
134 | 44 | October 14, 2023 | 18:00:41 | Annular | 11.4N 83.1W | 0.3753 | 0.952 | 187 | 5m 17s | |
134 | 45 | October 25, 2041 | 1:36:22 | Annular | 9.9N 162.9E | 0.4133 | 0.9467 | 213 | 6m 7s | |
134 | 46 | November 5, 2059 | 9:18:15 | Annular | 8.7N 47.1E | 0.4454 | 0.9417 | 238 | 7m 0s | |
134 | 47 | November 15, 2077 | 17:07:56 | Annular | 7.8N 70.8W | 0.4705 | 0.9371 | 262 | 7m 54s | |
134 | 48 | November 27, 2095 | 1:02:57 | Annular | 7.2N 169.8E | 0.4903 | 0.933 | 285 | 8m 47s | |
134 | 49 | December 8, 2113 | 9:03:27 | Annular | 7.1N 48.9E | 0.5049 | 0.9296 | 304 | 9m 35s | |
134 | 50 | December 19, 2131 | 17:06:51 | Annular | 7.6N 72.8W | 0.5165 | 0.9267 | 321 | 10m 14s | |
134 | 51 | December 30, 2149 | 1:13:04 | Annular | 8.6N 164.7E | 0.5253 | 0.9245 | 334 | 10m 42s | |
134 | 52 | January 10, 2168 | 9:19:03 | Annular | 10.3N 42.1E | 0.5337 | 0.923 | 344 | 10m 55s | |
134 | 53 | January 20, 2186 | 17:23:44 | Annular | 12.8N 80.3W | 0.5426 | 0.9221 | 350 | 10m 53s | |
134 | 54 | February 2, 2204 | 1:25:26 | Annular | 16N 157.8E | 0.5535 | 0.9218 | 353 | 10m 38s | |
134 | 55 | February 12, 2222 | 9:23:18 | Annular | 20N 36.7E | 0.5669 | 0.922 | 355 | 10m 14s | |
134 | 56 | February 23, 2240 | 17:14:11 | Annular | 24.7N 83W | 0.5859 | 0.9228 | 356 | 9m 41s | |
134 | 57 | March 6, 2258 | 0:58:23 | Annular | 30.2N 158.8E | 0.6101 | 0.9239 | 359 | 9m 4s | |
134 | 58 | March 16, 2276 | 8:34:02 | Annular | 36.4N 42.3E | 0.6411 | 0.9253 | 362 | 8m 23s | |
134 | 59 | March 27, 2294 | 16:02:23 | Annular | 43.2N 72.6W | 0.6776 | 0.9269 | 370 | 7m 42s | |
134 | 60 | April 7, 2312 | 23:19:32 | Annular | 50.8N 174.7E | 0.7231 | 0.9286 | 385 | 7m 0s | |
134 | 61 | April 19, 2330 | 6:29:25 | Annular | 59N 62.9E | 0.7742 | 0.9302 | 412 | 6m 19s | |
134 | 62 | April 29, 2348 | 13:29:00 | Annular | 68.1N 48.8W | 0.8338 | 0.9315 | 466 | 5m 40s | |
134 | 63 | May 10, 2366 | 20:22:08 | Annular | 77.9N 169.5W | 0.8981 | 0.9323 | 583 | 5m 3s | |
134 | 64 | May 21, 2384 | 3:05:26 | Annular | 80.8N 0.8W | 0.9701 | 0.9317 | 1115 | 4m 28s | |
134 | 65 | June 1, 2402 | 9:44:38 | Partial | 67.8N 135.9W | 1.0452 | 0.8834 | |||
134 | 66 | June 11, 2420 | 16:17:02 | Partial | 66.8N 115.6E | 1.1256 | 0.747 | |||
134 | 67 | June 22, 2438 | 22:46:47 | Partial | 65.8N 8.2E | 1.2079 | 0.6068 | |||
134 | 68 | July 3, 2456 | 5:13:16 | Partial | 64.9N 98.1W | 1.2925 | 0.4621 | |||
134 | 69 | July 14, 2474 | 11:40:30 | Partial | 64N 155.9E | 1.3764 | 0.3182 | |||
134 | 70 | July 24, 2492 | 18:08:32 | Partial | 63.2N 49.8E | 1.4594 | 0.1755 | |||
134 | 71 | August 6, 2510 | 0:38:56 | Partial | 62.6N 56.5W | 1.5405 | 0.0362 |
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 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.
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 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 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 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 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 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.
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 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 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.