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.
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.
This series is currently producing total eclipses over 4 minutes long, with each one gradually increasing in length. It will continue to do so until 16 July 2186, when it will produce the longest total eclipse calculated for the ten millennia from 3999 BCE to 6000 CE. [1] Starting on May 11, 2078, Saros 139 will begin producing the longest total eclipses of any series, surpassing those of Solar Saros 136, whose eclipses are getting slightly shorter. [2]
This solar saros is linked to Lunar Saros 132.
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 139 appears in the following table.
Classification | Number | Percent |
---|---|---|
All Umbral eclipses | 55 | 100.00% |
Central (two limits) | 55 | 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 | QLE | Sun altitude |
---|---|---|---|---|---|---|---|---|---|---|---|---|
139 | 1 | May 17, 1501 | 3:27:44 | Partial | 63.7N 13.6W | 1.5002 | 0.0905 | t- | 0 | |||
139 | 2 | May 28, 1519 | 10:20:09 | Partial | 64.6N 126.3W | 1.4188 | 0.2342 | t- | 0 | |||
139 | 3 | June 7, 1537 | 17:14:05 | Partial | 65.5N 120.2E | 1.3373 | 0.3796 | t- | 0 | |||
139 | 4 | June 19, 1555 | 0:07:16 | Partial | 66.5N 6.6E | 1.2542 | 0.529 | t- | 0 | |||
139 | 5 | June 29, 1573 | 7:03:36 | Partial | 67.5N 108.2W | 1.1724 | 0.677 | t- | 0 | |||
139 | 6 | July 20, 1591 | 14:02:08 | Partial | 68.5N 136E | 1.0911 | 0.8249 | t- | 0 | |||
139 | 7 | July 30, 1609 | 21:07:08 | Partial | 69.5N 17.9E | 1.014 | 0.9657 | t- | 0 | |||
139 | 8 | August 11, 1627 | 4:17:14 | Hybrid | 77.7N 173.3W | 0.9401 | 1.0001 | 1 | 0m 00s | t- | 19 | |
139 | 9 | August 21, 1645 | 11:34:18 | Hybrid | 68.2N 43.7E | 0.871 | 1.004 | 28 | 0m 16s | t- | 29 | |
139 | 10 | September 1, 1663 | 18:59:08 | Hybrid | 58.6N 78.9W | 0.8073 | 1.0065 | 38 | 0m 29s | p- | 36 | |
139 | 11 | September 12, 1681 | 2:33:12 | Hybrid | 49.8N 161.1E | 0.7504 | 1.0083 | 43 | 0m 40s | p- | 41 | |
139 | 12 | September 23, 1699 | 10:16:12 | Hybrid | 41.8N 40.7E | 0.6999 | 1.0095 | 46 | 0m 49s | p- | 45 | |
139 | 13 | October 4, 1717 | 18:08:27 | Hybrid | 34.6N 81.1W | 0.6563 | 1.0104 | 47 | 0m 56s | p- | 49 | |
139 | 14 | October 16, 1735 | 2:10:34 | Hybrid | 28.3N 155.2E | 0.6202 | 1.011 | 48 | 1m 02s | p- | 51 | |
139 | 15 | October 26, 1753 | 10:22:01 | Hybrid | 22.7N 29.7E | 0.591 | 1.0115 | 49 | 1m 08s | p- | 54 | |
139 | 16 | November 6, 1771 | 18:41:02 | Hybrid | 17.9N 97.3W | 0.5676 | 1.012 | 50 | 1m 13s | p- | 55 | |
139 | 17 | November 17, 1789 | 3:08:35 | Hybrid | 14.1N 133.9E | 0.5504 | 1.0126 | 52 | 1m 19s | p- | 57 | |
139 | 18 | November 29, 1807 | 11:42:09 | Hybrid | 11.1N 3.9E | 0.5377 | 1.0135 | 55 | 1m 26s | p- | 57 | |
139 | 19 | December 9, 1825 | 20:21:45 | Hybrid [3] | 9.2N 127.4W | 0.5296 | 1.0148 | 60 | 1m 34s | p- | 58 | |
139 | 20 | December 21, 1843 | 5:03:26 | Total | 8N 101E | 0.5227 | 1.0165 | 66 | 1m 43s | p- | 58 | |
139 | 21 | December 31, 1861 | 13:49:06 | Total | 7.8N 31.6W | 0.5187 | 1.0186 | 74 | 1m 55s | p- | 59 | |
139 | 22 | January 11, 1880 | 22:34:25 | Total | 8.3N 164.1W | 0.5136 | 1.0212 | 84 | 2m 07s | p- | 59 | |
139 | 23 | January 22, 1898 | 7:19:12 | Total | 9.5N 63.6E | 0.5079 | 1.0244 | 96 | 2m 21s | p- | 59 | |
139 | 24 | February 3, 1916 | 16:00:21 | Total | 11.1N 67.7W | 0.4987 | 1.028 | 108 | 2m 36s | p- | 60 | |
139 | 25 | February 14, 1934 | 0:38:41 | Total | 13.2N 161.7E | 0.4868 | 1.0321 | 123 | 2m 53s | p- | 61 | |
139 | 26 | February 25, 1952 | 9:11:35 | Total | 15.6N 32.7E | 0.4697 | 1.0366 | 138 | 3m 09s | p- | 62 | |
139 | 27 | March 7, 1970 | 17:38:30 | Total | 18.2N 94.7W | 0.4473 | 1.0414 | 153 | 3m 28s | p- | 63 | |
139 | 28 | March 18, 1988 | 1:58:56 | Total | 20.7N 140E | 0.4188 | 1.0464 | 169 | 3m 46s | n- | 65 | |
139 | 29 | March 29, 2006 | 10:12:23 | Total | 23.2N 16.7E | 0.3843 | 1.0515 | 184 | 4m 07s | n- | 67 | |
139 | 30 | April 8, 2024 | 18:18:29 | Total | 25.3N 104.1W | 0.3431 | 1.0566 | 198 | 4m 28s | n- | 70 | |
139 | 31 | April 20, 2042 | 2:17:30 | Total | 27N 137.3E | 0.2956 | 1.0614 | 210 | 4m 51s | n- | 73 | |
139 | 32 | April 30, 2060 | 10:10:00 | Total | 28N 20.9E | 0.2422 | 1.066 | 222 | 5m 15s | n- | 76 | |
139 | 33 | May 11, 2078 | 17:56:55 | Total | 28.1N 93.7W | 0.1838 | 1.0701 | 232 | 5m 40s | n- | 79 | |
139 | 34 | May 22, 2096 | 1:37:14 | Total | 27.3N 153.4E | 0.1196 | 1.0737 | 241 | 6m 07s | nn | 83 | |
139 | 35 | June 3, 2114 | 9:14:09 | Total | 25.4N 41.3E | 0.0525 | 1.0766 | 248 | 6m 32s | nn | 87 | |
139 | 36 | June 13, 2132 | 16:46:24 | Total | 22.3N 70.1W | -0.0186 | 1.0788 | 255 | 6m 55s | nn | 89 | |
139 | 37 | June 25, 2150 | 0:17:25 | Total | 18.3N 178.1E | -0.091 | 1.0802 | 260 | 7m 14s | nn | 85 | |
139 | 38 | July 5, 2168 | 7:45:23 | Total | 13.2N 66.4E | -0.166 | 1.0807 | 264 | 7m 26s | -n | 81 | |
139 | 39 | July 16, 2186 | 15:14:54 | Total | 7.4N 46.5W | -0.2396 | 1.0805 | 267 | 7m 29s | -n | 76 | |
139 | 40 | July 27, 2204 | 22:44:32 | Total | 1N 160.1W | -0.3129 | 1.0793 | 269 | 7m 22s | -n | 72 | |
139 | 41 | August 8, 2222 | 6:17:05 | Total | 6S 84.9E | -0.3837 | 1.0774 | 270 | 7m 06s | -n | 67 | |
139 | 42 | August 18, 2240 | 13:52:25 | Total | 13.3S 31.3W | -0.4522 | 1.0746 | 270 | 6m 40s | -p | 63 | |
139 | 43 | August 29, 2258 | 21:33:05 | Total | 20.9S 149.2W | -0.5161 | 1.0712 | 269 | 6m 09s | -p | 59 | |
139 | 44 | September 9, 2276 | 5:18:47 | Total | 28.5S 91.2E | -0.5755 | 1.0671 | 266 | 5m 33s | -p | 55 | |
139 | 45 | September 20, 2294 | 13:09:58 | Total | 36.2S 29.9W | -0.63 | 1.0627 | 263 | 4m 56s | -p | 51 | |
139 | 46 | October 1, 2312 | 21:08:26 | Total | 43.8S 152.9W | -0.6783 | 1.0578 | 258 | 4m 20s | -p | 47 | |
139 | 47 | October 13, 2330 | 5:13:41 | Total | 51.2S 82.5E | -0.7208 | 1.0528 | 251 | 3m 46s | -p | 44 | |
139 | 48 | October 23, 2348 | 13:26:56 | Total | 58.2S 43.6W | -0.7564 | 1.0476 | 242 | 3m 14s | -p | 41 | |
139 | 49 | November 3, 2366 | 21:46:04 | Total | 64.8S 170.2W | -0.7868 | 1.0426 | 231 | 2m 46s | -p | 38 | |
139 | 50 | November 14, 2384 | 6:13:20 | Total | 70.9S 63.5E | -0.8102 | 1.0377 | 217 | 2m 22s | -p | 36 | |
139 | 51 | November 25, 2402 | 14:45:41 | Total | 76.2S 59.6W | -0.8291 | 1.0332 | 202 | 2m 02s | -p | 34 | |
139 | 52 | December 5, 2420 | 23:23:52 | Total | 80.2S 174W | -0.8431 | 1.029 | 185 | 1m 44s | -p | 32 | |
139 | 53 | December 17, 2438 | 8:05:40 | Total | 81.7S 84.3E | -0.8539 | 1.0254 | 168 | 1m 30s | -p | 31 | |
139 | 54 | December 27, 2456 | 16:51:25 | Total | 79.8S 22W | -0.8614 | 1.0222 | 151 | 1m 19s | -p | 30 | |
139 | 55 | January 8, 2475 | 1:37:52 | Total | 76.2S 141.8W | -0.8679 | 1.0196 | 136 | 1m 10s | -p | 29 | |
139 | 56 | January 18, 2493 | 10:24:30 | Total | 72.2S 90.8E | -0.8742 | 1.0174 | 123 | 1m 02s | -p | 29 | |
139 | 57 | January 30, 2511 | 19:09:33 | Total | 68.1S 39.5W | -0.8816 | 1.0157 | 114 | 0m 57s | -p | 28 | |
139 | 58 | February 10, 2529 | 3:52:31 | Total | 64.3S 170.7W | -0.8908 | 1.0143 | 108 | 0m 53s | -p | 27 | |
139 | 59 | February 21, 2547 | 12:29:30 | Total | 61.1S 59.6E | -0.9046 | 1.0132 | 106 | 0m 50s | -p | 25 | |
139 | 60 | March 3, 2565 | 21:01:39 | Total | 58.7S 68.8W | -0.922 | 1.0121 | 107 | 0m 46s | -t | 22 | |
139 | 61 | March 15, 2583 | 5:25:52 | Total | 57.4S 166.2E | -0.9456 | 1.0109 | 115 | 0m 42s | -t | 19 | |
139 | 62 | March 26, 2601 | 13:43:55 | Total | 58S 45.6E | -0.974 | 1.0091 | 142 | 0m 35s | -t | 12 | |
139 | 63 | April 6, 2619 | 21:51:02 | Partial | 61.2S 60.7W | -1.0108 | 0.9781 | -t | 0 | |||
139 | 64 | April 17, 2637 | 5:51:33 | Partial | 61.6S 170.8E | -1.0525 | 0.9013 | -t | 0 | |||
139 | 65 | April 28, 2655 | 13:40:56 | Partial | 62S 45.1E | -1.1024 | 0.8094 | -t | 0 | |||
139 | 66 | May 8, 2673 | 21:23:23 | Partial | 62.7S 79.1W | -1.1574 | 0.708 | -t | 0 | |||
139 | 67 | May 20, 2691 | 4:55:09 | Partial | 63.4S 159.1E | -1.2203 | 0.5922 | -t | 0 | |||
139 | 68 | May 31, 2709 | 12:21:17 | Partial | 64.2S 38.6E | -1.2869 | 0.4697 | -t | 0 | |||
139 | 69 | June 11, 2727 | 19:39:01 | Partial | 65.2S 80.2W | -1.359 | 0.3372 | -t | 0 | |||
139 | 70 | June 22, 2745 | 2:51:30 | Partial | 66.1S 162E | -1.4345 | 0.1992 | -t | 0 | |||
139 | 71 | July 3, 2763 | 9:58:23 | Partial | 67.1S 45.2E | -1.5132 | 0.0562 | -t | 0 |
A total solar eclipse will occur on Sunday, April 20, 2042. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. It will be seen significantly in Western Indonesia, Eastern Malaysia, Brunei and the Philippines.
A total solar eclipse will occur on Friday, April 30, 2060. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.
A total solar eclipse will occur on Wednesday, May 11, 2078. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.
A total solar eclipse will occur on Tuesday, May 22, 2096. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. This will be the first eclipse of saros series 139 to exceed series 136 in length of totality. The length of totality for saros 139 is increasing, while that of Saros 136 is decreasing.
A total solar eclipse occurred on March 18, 1988. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Totality was visible in Indonesia and southern Philippines.
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 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 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. 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.
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 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 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 135 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 eclipses, including 53 umbral eclipses. The longest duration of totality will be 2 minutes, 27 seconds on May 12, 2431 while the longest annular was 10 minutes 14 seconds on 24 December 1601.
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 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.