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.
This solar saros is linked to Lunar Saros 139.
It is a part of Saros cycle 146, repeating every 18 years, 11 days, containing 76 events. The series started with partial solar eclipse on September 19, 1541. It contains total eclipses from May 29, 1938 through October 7, 2154, hybrid eclipses from October 17, 2172 through November 20, 2226, and annular eclipses from December 1, 2244 through August 10, 2659. The series ends at member 76 as a partial eclipse on December 29, 2893. The longest duration of totality was 5 minutes, 21 seconds on June 30, 1992.
| Series members 21-37 occur between 1901 and 2200: | ||
|---|---|---|
| 21 | 22 | 23 |
 May 7, 1902 |  May 18, 1920 |  May 29, 1938 |
| 24 | 25 | 26 |
 June 8, 1956 |  June 20, 1974 |  June 30, 1992 |
| 27 | 28 | 29 |
 July 11, 2010 |  July 22, 2028 |  August 2, 2046 |
| 30 | 31 | 32 |
 August 12, 2064 |  August 24, 2082 |  September 4, 2100 |
| 33 | 34 | 35 |
 September 15, 2118 |  September 26, 2136 |  October 7, 2154 |
| 36 | 37 | |
 October 17, 2172 |  October 29, 2190 | |
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 146 appears in the following table.
| Classification | Number | Percent |
|---|---|---|
| All Umbral eclipses | 41 | 100.00% |
| Central (two limits) | 41 | 100.00% |
| Central (one limit) | 0 | 0.00% |
| Non-central (one limit) | 0 | 0.00% |
| Saros | Member | Date | Time (Greatest) UTC | Type | Location Lat, Long | Gamma | Mag. | Width (km) | Duration (min:sec) | Ref |
|---|---|---|---|---|---|---|---|---|---|---|
| 146 | 1 | September 19, 1541 | 20:34:01 | Partial | 61.1S 135.3E | -1.514 | 0.0378 | |||
| 146 | 2 | October 1, 1559 | 4:46:46 | Partial | 61.3S 3.4E | -1.4772 | 0.1083 | |||
| 146 | 3 | October 11, 1577 | 13:08:02 | Partial | 61.6S 130.8W | -1.4473 | 0.1654 | |||
| 146 | 4 | November 1, 1595 | 21:36:53 | Partial | 62.1S 93.1E | -1.4233 | 0.2111 | |||
| 146 | 5 | November 12, 1613 | 6:12:15 | Partial | 62.7S 44.9W | -1.4048 | 0.2464 | |||
| 146 | 6 | November 23, 1631 | 14:53:44 | Partial | 63.5S 175.4E | -1.3912 | 0.2723 | |||
| 146 | 7 | December 3, 1649 | 23:40:37 | Partial | 64.4S 34.1E | -1.382 | 0.2896 | |||
| 146 | 8 | December 15, 1667 | 8:29:59 | Partial | 65.3S 108.2W | -1.3752 | 0.3024 | |||
| 146 | 9 | December 25, 1685 | 17:22:35 | Partial | 66.4S 108.3E | -1.371 | 0.3102 | |||
| 146 | 10 | January 7, 1704 | 2:14:51 | Partial | 67.4S 35.5W | -1.3669 | 0.3177 | |||
| 146 | 11 | January 17, 1722 | 11:07:10 | Partial | 68.5S 179.9W | -1.3629 | 0.3251 | |||
| 146 | 12 | January 28, 1740 | 19:54:59 | Partial | 69.5S 36.2E | -1.3555 | 0.3387 | |||
| 146 | 13 | February 8, 1758 | 4:40:52 | Partial | 70.4S 107.8W | -1.3468 | 0.3549 | |||
| 146 | 14 | February 19, 1776 | 13:20:11 | Partial | 71.1S 109.2E | -1.3334 | 0.38 | |||
| 146 | 15 | March 1, 1794 | 21:54:00 | Partial | 71.6S 32.9W | -1.3155 | 0.4136 | |||
| 146 | 16 | March 13, 1812 | 6:19:31 | Partial | 71.9S 173.3W | -1.2913 | 0.4594 | |||
| 146 | 17 | March 24, 1830 | 14:38:43 | Partial | 72S 47.7E | -1.2622 | 0.5148 | |||
| 146 | 18 | April 3, 1848 | 22:49:07 | Partial | 71.8S 89W | -1.2264 | 0.5834 | |||
| 146 | 19 | April 15, 1866 | 6:51:40 | Partial | 71.4S 136.6E | -1.1846 | 0.6637 | |||
| 146 | 20 | April 25, 1884 | 14:46:17 | Partial | 70.7S 4.6E | -1.1365 | 0.7563 | |||
| 146 | 21 | May 7, 1902 | 22:34:16 | Partial | 70S 125.1W | -1.0831 | 0.8593 | |||
| 146 | 22 | May 18, 1920 | 6:14:55 | Partial | 69.1S 107.7E | -1.0239 | 0.9734 | |||
| 146 | 23 | May 29, 1938 | 13:50:19 | Total | 52.7S 22W | -0.9607 | 1.0552 | 675 | 4m 5s | |
| 146 | 24 | June 8, 1956 | 21:20:39 | Total | 40.8S 140.7W | -0.8934 | 1.0581 | 429 | 4m 45s | |
| 146 | 25 | June 20, 1974 | 4:48:04 | Total | 32.1S 103.7E | -0.8239 | 1.0592 | 344 | 5m 9s | |
| 146 | 26 | June 30, 1992 | 12:11:22 | Total | 25.2S 9.5W | -0.7512 | 1.0592 | 294 | 5m 21s | |
| 146 | 27 | July 11, 2010 | 19:34:38 | Total | 19.7S 121.9W | -0.6788 | 1.058 | 259 | 5m 20s | |
| 146 | 28 | July 22, 2028 | 2:56:40 | Total | 15.6S 126.7E | -0.6056 | 1.056 | 230 | 5m 10s | |
| 146 | 29 | August 2, 2046 | 10:21:13 | Total | 12.7S 15.2E | -0.535 | 1.0531 | 206 | 4m 51s | |
| 146 | 30 | August 12, 2064 | 17:46:06 | Total | 10.9S 96W | -0.4652 | 1.0495 | 184 | 4m 28s | |
| 146 | 31 | August 24, 2082 | 1:16:21 | Total | 10.3S 151.8E | -0.4004 | 1.0452 | 163 | 4m 1s | |
| 146 | 32 | September 4, 2100 | 8:49:20 | Total | 10.5S 39E | -0.3384 | 1.0402 | 142 | 3m 32s | |
| 146 | 33 | September 15, 2118 | 16:28:26 | Total | 11.5S 75.2W | -0.2823 | 1.0349 | 122 | 3m 4s | |
| 146 | 34 | September 26, 2136 | 0:12:14 | Total | 13S 169.4E | -0.2309 | 1.0292 | 101 | 2m 34s | |
| 146 | 35 | October 7, 2154 | 8:03:50 | Total | 15.1S 52.1E | -0.1867 | 1.0234 | 81 | 2m 5s | |
| 146 | 36 | October 17, 2172 | 16:01:36 | Hybrid | 17.3S 66.6W | -0.1484 | 1.0174 | 60 | 1m 34s | |
| 146 | 37 | October 29, 2190 | 0:05:50 | Hybrid | 19.6S 173.2E | -0.1161 | 1.0116 | 40 | 1m 4s | |
| 146 | 38 | November 9, 2208 | 8:17:12 | Hybrid | 21.8S 51.4E | -0.0905 | 1.0059 | 20 | 0m 34s | |
| 146 | 39 | November 20, 2226 | 16:34:56 | Hybrid | 23.7S 71.7W | -0.0711 | 1.0005 | 2 | 0m 3s | |
| 146 | 40 | December 1, 2244 | 0:58:17 | Annular | 25.1S 164E | -0.0568 | 0.9955 | 16 | 0m 27s | |
| 146 | 41 | December 12, 2262 | 9:25:02 | Annular | 25.8S 39E | -0.0461 | 0.991 | 32 | 0m 56s | |
| 146 | 42 | December 22, 2280 | 17:55:44 | Annular | 25.8S 86.8W | -0.0392 | 0.987 | 46 | 1m 23s | |
| 146 | 43 | January 3, 2299 | 2:27:43 | Annular | 24.9S 146.9E | -0.0341 | 0.9836 | 58 | 1m 47s | |
| 146 | 44 | January 14, 2317 | 10:59:38 | Annular | 23.2S 20.5E | -0.0298 | 0.9807 | 69 | 2m 8s | |
| 146 | 45 | January 25, 2335 | 19:29:43 | Annular | 20.6S 105.9W | -0.0247 | 0.9784 | 77 | 2m 25s | |
| 146 | 46 | February 5, 2353 | 3:56:55 | Annular | 17.1S 128E | -0.0179 | 0.9766 | 84 | 2m 38s | |
| 146 | 47 | February 16, 2371 | 12:18:49 | Annular | 12.9S 2.7E | -0.0075 | 0.9753 | 88 | 2m 48s | |
| 146 | 48 | February 26, 2389 | 20:33:52 | Annular | 8.1S 121.3W | 0.0078 | 0.9744 | 92 | 2m 55s | |
| 146 | 49 | March 10, 2407 | 4:41:40 | Annular | 2.7S 116.1E | 0.0283 | 0.9739 | 93 | 2m 59s | |
| 146 | 50 | March 20, 2425 | 12:41:12 | Annular | 3.1N 4.7W | 0.0546 | 0.9735 | 95 | 3m 2s | |
| 146 | 51 | March 31, 2443 | 20:30:25 | Annular | 9.3N 123.1W | 0.0889 | 0.9734 | 95 | 3m 2s | |
| 146 | 52 | April 11, 2461 | 4:10:36 | Annular | 15.8N 120.8E | 0.13 | 0.9732 | 97 | 3m 2s | |
| 146 | 53 | April 22, 2479 | 11:40:30 | Annular | 22.5N 7.5E | 0.179 | 0.9731 | 98 | 3m 1s | |
| 146 | 54 | May 2, 2497 | 19:01:52 | Annular | 29.2N 103.2W | 0.2341 | 0.9727 | 100 | 2m 59s | |
| 146 | 55 | May 15, 2515 | 2:12:11 | Annular | 36N 149.4E | 0.2976 | 0.9722 | 104 | 2m 57s | |
| 146 | 56 | May 25, 2533 | 9:15:50 | Annular | 42.6N 44.8E | 0.366 | 0.9712 | 111 | 2m 56s | |
| 146 | 57 | June 5, 2551 | 16:10:40 | Annular | 49N 56.1W | 0.4411 | 0.9699 | 121 | 2m 55s | |
| 146 | 58 | June 15, 2569 | 23:00:08 | Annular | 54.8N 153.7W | 0.5197 | 0.968 | 135 | 2m 56s | |
| 146 | 59 | June 27, 2587 | 5:42:58 | Annular | 59.9N 113.1E | 0.6029 | 0.9656 | 156 | 2m 58s | |
| 146 | 60 | July 8, 2605 | 12:23:21 | Annular | 64N 24E | 0.6873 | 0.9626 | 186 | 3m 3s | |
| 146 | 61 | July 19, 2623 | 19:00:06 | Annular | 66.8N 60.2W | 0.7738 | 0.9589 | 235 | 3m 10s | |
| 146 | 62 | July 30, 2641 | 1:35:56 | Annular | 68.1N 140W | 0.8602 | 0.9545 | 326 | 3m 20s | |
| 146 | 63 | August 10, 2659 | 8:11:51 | Annular | 67.6N 146.8E | 0.9454 | 0.9487 | 584 | 3m 30s | |
| 146 | 64 | August 20, 2677 | 14:50:18 | Partial | 61.7N 81.5E | 1.0277 | 0.9182 | |||
| 146 | 65 | August 31, 2695 | 21:32:02 | Partial | 61.3N 27.3W | 1.1064 | 0.7816 | |||
| 146 | 66 | September 12, 2713 | 4:18:12 | Partial | 61.1N 137.1W | 1.1807 | 0.6536 | |||
| 146 | 67 | September 23, 2731 | 11:10:46 | Partial | 61N 111.6E | 1.2491 | 0.5366 | |||
| 146 | 68 | October 3, 2749 | 18:09:52 | Partial | 61.1N 1.4W | 1.3115 | 0.4305 | |||
| 146 | 69 | October 15, 2767 | 1:16:22 | Partial | 61.4N 116.2W | 1.3673 | 0.3366 | |||
| 146 | 70 | October 25, 2785 | 8:31:14 | Partial | 61.8N 126.8E | 1.4158 | 0.2555 | |||
| 146 | 71 | November 5, 2803 | 15:54:34 | Partial | 62.3N 7.6E | 1.4572 | 0.1871 | |||
| 146 | 72 | November 15, 2821 | 23:26:43 | Partial | 63N 114W | 1.4912 | 0.1314 | |||
| 146 | 73 | November 27, 2839 | 7:05:15 | Partial | 63.8N 122.6E | 1.5198 | 0.0847 | |||
| 146 | 74 | December 7, 2857 | 14:52:22 | Partial | 64.8N 3.2W | 1.5412 | 0.0502 | |||
| 146 | 75 | December 18, 2875 | 22:44:21 | Partial | 65.8N 130.6W | 1.5581 | 0.023 | |||
| 146 | 76 | December 29, 2893 | 6:42:03 | Partial | 66.8N 100.1E | 1.5706 | 0.0028 |
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 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 total solar eclipse will occur on Saturday, July 22, 2028. The central line of the path of the eclipse will cross the Australian continent from the Kimberley region in the north-west and continue in a south-easterly direction through Western Australia, the Northern Territory, south-west Queensland and New South Wales, close to the towns of Wyndham, Kununurra, Tennant Creek, Birdsville, Bourke and Dubbo, and continuing on through the centre of Sydney, where the eclipse will have a duration of over three minutes. It will also cross Queenstown and Dunedin, New Zealand. Totality will also be viewable from two of Australia's external territories: Christmas Island and the Cocos (Keeling) Islands.
An annular solar eclipse occurred on August 21, 1933. 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. Annularity was visible from Italian Libya, Egypt, Mandatory Palestine including Jerusalem and Amman, French Mandate for Syria and the Lebanon, Iraq including Baghdad, Persia, Afghanistan, British Raj, Siam, Dutch East Indies, North Borneo, and Australia.
An annular solar eclipse will occur on Monday, May 31, 2049. 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.
An annular solar eclipse occurred on September 11, 1969.
A total solar eclipse is forecast to occur on Saturday, September 4, 2100. 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 August 12, 2064, that occurs on the Pacific coast and in the southern cone, especially in the cities of Valparaíso and the capital Santiago. 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.
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 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.
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 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 137 for solar eclipses occurs at the Moon's ascending node. It repeats every 18 years, 11 days, and contains 70 events. 55 of these are umbral eclipses and other 15 of these are partial solar eclipses. All eclipses in this series occur at the Moon's ascending 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 147 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 80 events. All eclipses in this series occur at the Moon's ascending 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.
