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 occur at the Moon's descending node.
This solar saros is linked to Lunar Saros 111.
It is a part of Saros cycle 118, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on May 24, 803 AD. It contains total eclipses from August 19, 947 AD through October 25, 1650, hybrid eclipses on November 4, 1668 and November 15, 1686, and annular eclipses from November 27, 1704 through April 30, 1957. The series ends at member 72 as a partial eclipse on July 15, 2083. The longest duration of totality was 6 minutes, 59 seconds on May 16, 1398.
| Series members 62–72 occur between 1901 and 2083: | ||
|---|---|---|
| 62 | 63 | 64 |
 Mar 29, 1903 |  Apr 8, 1921 |  Apr 19, 1939 |
| 65 | 66 | 67 |
 Apr 30, 1957 |  May 11, 1975 |  May 21, 1993 |
| 68 | 69 | 70 |
 Jun 1, 2011 |  Jun 12, 2029 |  Jun 23, 2047 |
| 71 | 72 | |
 Jul 3, 2065 |  Jul 15, 2083 | |
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 118 appears in the following table.
| Classification | Number | Percent |
|---|---|---|
| All Umbral eclipses | 57 | 100.00% |
| Central (two limits) | 56 | 98.25% |
| Central (one limit) | 0 | 0.00% |
| Non-central (one limit) | 1 | 1.75% |
| Saros | Member | Date | Time (Greatest) UTC | Type | Location Lat, Long | Gamma | Mag. | Width (km) | Duration (min:sec) | Ref |
|---|---|---|---|---|---|---|---|---|---|---|
| 118 | 1 | May 24, 803 | 13:35:52 | Partial | 68.1S 0.7W | -1.5325 | 0.0122 | |||
| 118 | 2 | June 3, 821 | 20:45:44 | Partial | 67.1S 119.9W | -1.4545 | 0.1561 | |||
| 118 | 3 | June 15, 839 | 3:56:24 | Partial | 66.1S 121.2E | -1.3758 | 0.3023 | |||
| 118 | 4 | June 25, 857 | 11:08:23 | Partial | 65.1S 2.5E | -1.2972 | 0.4494 | |||
| 118 | 5 | July 6, 875 | 18:24:50 | Partial | 64.2S 117W | -1.221 | 0.5929 | |||
| 118 | 6 | July 17, 893 | 1:45:18 | Partial | 63.4S 122.8E | -1.1469 | 0.7327 | |||
| 118 | 7 | July 28, 911 | 9:12:23 | Partial | 62.6S 1.2E | -1.0774 | 0.864 | |||
| 118 | 8 | August 7, 929 | 16:45:08 | Partial | 62S 121.6W | -1.0118 | 0.988 | |||
| 118 | 9 | August 19, 947 | 0:26:53 | Total | 51.3S 139.1E | -0.9527 | 1.0357 | 393 | 2m 29s | |
| 118 | 10 | August 29, 965 | 8:15:51 | Total | 47.1S 24.8E | -0.899 | 1.0377 | 283 | 2m 41s | |
| 118 | 11 | September 9, 983 | 16:13:17 | Total | 45.7S 93.8W | -0.8518 | 1.0386 | 242 | 2m 44s | |
| 118 | 12 | September 20, 1001 | 0:19:08 | Total | 46.1S 144.9E | -0.8111 | 1.0388 | 218 | 2m 43s | |
| 118 | 13 | October 1, 1019 | 8:34:20 | Total | 47.8S 20.9E | -0.7781 | 1.0386 | 202 | 2m 40s | |
| 118 | 14 | October 11, 1037 | 16:57:23 | Total | 50.3S 104.8W | -0.7512 | 1.0382 | 191 | 2m 36s | |
| 118 | 15 | October 23, 1055 | 1:27:47 | Total | 53.4S 128.1E | -0.7301 | 1.0377 | 183 | 2m 32s | |
| 118 | 16 | November 2, 1073 | 10:05:13 | Total | 56.8S 0.1E | -0.7148 | 1.0373 | 178 | 2m 29s | |
| 118 | 17 | November 13, 1091 | 18:48:57 | Total | 60.3S 128.2W | -0.7047 | 1.0371 | 175 | 2m 26s | |
| 118 | 18 | November 24, 1109 | 3:36:12 | Total | 63.5S 104.6E | -0.6974 | 1.0372 | 175 | 2m 26s | |
| 118 | 19 | December 5, 1127 | 12:27:08 | Total | 65.9S 21.2W | -0.693 | 1.0377 | 176 | 2m 28s | |
| 118 | 20 | December 15, 1145 | 21:18:46 | Total | 67S 145W | -0.6892 | 1.0387 | 180 | 2m 32s | |
| 118 | 21 | December 27, 1163 | 6:11:27 | Total | 66.6S 91.5E | -0.686 | 1.04 | 185 | 2m 38s | |
| 118 | 22 | January 6, 1182 | 15:00:32 | Total | 64.4S 32.7W | -0.6802 | 1.0419 | 192 | 2m 48s | |
| 118 | 23 | January 17, 1200 | 23:48:29 | Total | 61S 159.1W | -0.6731 | 1.0443 | 200 | 3m 1s | |
| 118 | 24 | January 28, 1218 | 8:30:17 | Total | 56.5S 73.1E | -0.6613 | 1.047 | 209 | 3m 17s | |
| 118 | 25 | February 8, 1236 | 17:07:28 | Total | 51.3S 55.5W | -0.6454 | 1.0501 | 217 | 3m 36s | |
| 118 | 26 | February 19, 1254 | 1:36:18 | Total | 45.4S 176.3E | -0.6227 | 1.0534 | 225 | 3m 59s | |
| 118 | 27 | March 1, 1272 | 9:59:32 | Total | 39.2S 48.6E | -0.5954 | 1.0569 | 232 | 4m 24s | |
| 118 | 28 | March 12, 1290 | 18:13:59 | Total | 32.7S 77.6W | -0.5611 | 1.0604 | 238 | 4m 52s | |
| 118 | 29 | March 23, 1308 | 2:21:00 | Total | 25.9S 157.8E | -0.5205 | 1.0638 | 243 | 5m 21s | |
| 118 | 30 | April 3, 1326 | 10:19:38 | Total | 19S 35.3E | -0.4731 | 1.0668 | 246 | 5m 49s | |
| 118 | 31 | April 13, 1344 | 18:11:36 | Total | 12S 85.4W | -0.42 | 1.0695 | 249 | 6m 15s | |
| 118 | 32 | April 25, 1362 | 1:56:16 | Total | 5.2S 155.9E | -0.3611 | 1.0717 | 249 | 6m 37s | |
| 118 | 33 | May 5, 1380 | 9:34:58 | Total | 1.5N 39.2E | -0.2973 | 1.0732 | 249 | 6m 52s | |
| 118 | 34 | May 16, 1398 | 17:08:41 | Total | 7.7N 75.7W | -0.2294 | 1.0741 | 247 | 6m 59s | |
| 118 | 35 | May 27, 1416 | 0:38:48 | Total | 13.5N 171E | -0.1584 | 1.0742 | 244 | 6m 56s | |
| 118 | 36 | June 7, 1434 | 8:05:20 | Total | 18.7N 59.3E | -0.0847 | 1.0735 | 239 | 6m 45s | |
| 118 | 37 | June 17, 1452 | 15:30:42 | Total | 23N 51.3W | -0.0102 | 1.0719 | 234 | 6m 26s | |
| 118 | 38 | June 28, 1470 | 22:54:56 | Total | 26.4N 161W | 0.065 | 1.0695 | 227 | 6m 2s | |
| 118 | 39 | July 9, 1488 | 6:20:51 | Total | 28.9N 89.5E | 0.1384 | 1.0663 | 219 | 5m 36s | |
| 118 | 40 | July 20, 1506 | 13:46:58 | Total | 30.4N 19.8W | 0.2112 | 1.0623 | 209 | 5m 8s | |
| 118 | 41 | July 30, 1524 | 21:17:39 | Total | 30.8N 130.2W | 0.2797 | 1.0577 | 198 | 4m 40s | |
| 118 | 42 | August 11, 1542 | 4:51:06 | Total | 30.6N 118.6E | 0.3454 | 1.0525 | 184 | 4m 12s | |
| 118 | 43 | August 21, 1560 | 12:30:55 | Total | 29.7N 5.3E | 0.405 | 1.0469 | 170 | 3m 45s | |
| 118 | 44 | September 1, 1578 | 20:15:08 | Total | 28.4N 109.6W | 0.4602 | 1.0408 | 152 | 3m 17s | |
| 118 | 45 | September 22, 1596 | 4:07:03 | Total | 26.8N 133E | 0.5085 | 1.0346 | 134 | 2m 50s | |
| 118 | 46 | October 3, 1614 | 12:04:51 | Total | 25.2N 13.5E | 0.5511 | 1.0282 | 113 | 2m 22s | |
| 118 | 47 | October 13, 1632 | 20:09:39 | Total | 23.7N 108.2W | 0.5873 | 1.022 | 91 | 1m 55s | |
| 118 | 48 | October 25, 1650 | 4:21:25 | Total | 22.3N 127.9E | 0.617 | 1.0159 | 68 | 1m 26s | |
| 118 | 49 | November 4, 1668 | 12:40:05 | Hybrid | 21.1N 1.8E | 0.6401 | 1.0102 | 45 | 0m 57s | |
| 118 | 50 | November 15, 1686 | 21:05:00 | Hybrid | 20.2N 126W | 0.6578 | 1.0048 | 22 | 0m 28s | |
| 118 | 51 | November 27, 1704 | 5:33:52 | Annular | 19.7N 104.9E | 0.6716 | 0.9999 | 1 | 0m 1s | |
| 118 | 52 | December 8, 1722 | 14:07:35 | Annular | 19.5N 25.4W | 0.6808 | 0.9955 | 21 | 0m 28s | |
| 118 | 53 | December 18, 1740 | 22:43:17 | Annular | 19.9N 156.4W | 0.6876 | 0.9917 | 40 | 0m 53s | |
| 118 | 54 | December 30, 1758 | 7:20:12 | Annular | 20.8N 72.2E | 0.6929 | 0.9885 | 56 | 1m 15s | |
| 118 | 55 | January 9, 1777 | 15:55:35 | Annular | 22.4N 58.9W | 0.6988 | 0.9859 | 70 | 1m 32s | |
| 118 | 56 | January 21, 1795 | 0:29:13 | Annular | 24.8N 170.3E | 0.7055 | 0.9837 | 81 | 1m 44s | |
| 118 | 57 | February 1, 1813 | 8:58:27 | Annular | 27.9N 40.4E | 0.7152 | 0.982 | 91 | 1m 53s | |
| 118 | 58 | February 12, 1831 | 17:21:45 | Annular | 31.9N 88.3W | 0.7288 | 0.9807 | 100 | 1m 57s | |
| 118 | 59 | February 23, 1849 | 1:38:09 | Annular | 36.7N 144.3E | 0.7475 | 0.9796 | 108 | 1m 58s | |
| 118 | 60 | March 6, 1867 | 9:46:48 | Annular | 42.3N 18.4E | 0.7716 | 0.9787 | 118 | 1m 57s | |
| 118 | 61 | March 16, 1885 | 17:45:43 | Annular | 48.9N 106.1W | 0.803 | 0.9778 | 132 | 1m 55s | |
| 118 | 62 | March 29, 1903 | 1:35:23 | Annular | 56.2N 130.3E | 0.8413 | 0.9767 | 153 | 1m 53s | |
| 118 | 63 | April 8, 1921 | 9:15:01 | Annular | 64.5N 5.6E | 0.8869 | 0.9753 | 192 | 1m 50s | |
| 118 | 64 | April 19, 1939 | 16:45:53 | Annular | 73.1N 129.1W | 0.9388 | 0.9731 | 285 | 1m 49s | |
| 118 | 65 | April 30, 1957 | 0:05:28 | Annular (non-central) | 70.6N 40.3E | 0.9992 | 0.9799 | - | - | |
| 118 | 66 | May 11, 1975 | 7:17:33 | Partial | 69.7N 80.2W | 1.0647 | 0.8636 | |||
| 118 | 67 | May 21, 1993 | 14:20:15 | Partial | 68.8N 162.3E | 1.1372 | 0.7352 | |||
| 118 | 68 | June 1, 2011 | 21:17:18 | Partial | 67.8N 46.8E | 1.213 | 0.601 | |||
| 118 | 69 | June 12, 2029 | 4:06:13 | Partial | 66.8N 66.2W | 1.2943 | 0.4576 | |||
| 118 | 70 | June 23, 2047 | 10:52:31 | Partial | 65.8N 178W | 1.3766 | 0.3129 | |||
| 118 | 71 | July 3, 2065 | 17:33:52 | Partial | 64.8N 71.9E | 1.4619 | 0.1638 | |||
| 118 | 72 | July 15, 2083 | 0:14:23 | Partial | 64N 37.7W | 1.5465 | 0.0168 |
A total solar eclipse occurred on Sunday, July 22, 1990. 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 southern Finland, the Soviet Union, and eastern Andreanof Islands and Amukta of Alaska.
A partial solar eclipse occurred on May 21, 1993. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A total solar eclipse occurred on Tuesday, June 30, 1992. 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 southeastern Uruguay and southern tip of Rio Grande do Sul, Brazil.
A partial solar eclipse will occur on Sunday, September 3, 2062. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
A partial solar eclipse occurred at the Moon's descending node of the orbit on Sunday, May 11, 1975. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
An annular solar eclipse occurred on April 30, 1957. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. This annular solar eclipse was non-central. Instead, over half of the antumbral shadow fell off into space throughout the eclipse. Gamma had a value of 0.9992. Annularity was visible from northern Soviet Union and Bear Island, the southernmost island of Svalbard, Norway.
A total solar eclipse will occur on January 5, 2057. 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 partial solar eclipse will occur on July 15, 2083. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth. This will be the 72nd and final event from Solar Saros 118.
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 occur 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 occur at the Moon's ascending node.
Saros cycle series 126 for solar eclipses occurs at the Moon's descending node, repeating every 18 years and 11 days, containing 72 events. All eclipses in this series occur 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 occur at the Moon's ascending 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 occur at the Moon's ascending node.
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 occur at the Moon's descending 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 occur at the Moon's descending node.
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 occur at the Moon's descending 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 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 occur at the Moon's descending 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 occur at the Moon's descending node.
An annular solar eclipse occurred on Wednesday, April 19, 1939. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.
