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 occurs at the Moon's ascending node.
It is a part of Saros cycle 119, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on May 15, 850 AD. It contains total eclipses on August 9, 994 AD and August 20, 1012 with a hybrid eclipse on August 31, 1030. It has annular eclipses from September 10, 1048 through March 18, 1950. The series ends at member 71 as a partial eclipse on June 24, 2112. 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. The longest duration of hybridity was only 18 seconds on August 31, 1030.
Series members 54–70 occur between 1801 and 2100: | ||
---|---|---|
54 | 55 | 56 |
December 21, 1805 | January 1, 1824 | January 11, 1842 |
57 | 58 | 59 |
January 23, 1860 | February 2, 1878 | February 13, 1896 |
60 | 61 | 62 |
February 25, 1914 | March 7, 1932 | March 18, 1950 |
63 | 64 | 65 |
March 28, 1968 | April 9, 1986 | April 19, 2004 |
66 | 67 | 68 |
April 30, 2022 | May 11, 2040 | May 22, 2058 |
69 | 70 | |
June 1, 2076 | June 13, 2094 |
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 119 appears in the following table.
Classification | Number | Percent |
---|---|---|
All Umbral eclipses | 54 | 100.00% |
Central (two limits) | 52 | 96.30% |
Central (one limit) | 0 | 0.00% |
Non-central (one limit) | 2 | 3.70% |
Saros | Member | Date | Time (Greatest) UTC | Type | Location Lat, Long | Gamma | Mag. | Width (km) | Duration (min:sec) | Ref |
---|---|---|---|---|---|---|---|---|---|---|
119 | 1 | May 15, 850 | 12:49:29 | Partial | 63.2N 138.7W | 1.5295 | 0.0066 | |||
119 | 2 | May 25, 868 | 20:11:13 | Partial | 64N 100.9E | 1.4636 | 0.1327 | |||
119 | 3 | June 6, 886 | 3:28:26 | Partial | 64.8N 18.7W | 1.3944 | 0.2647 | |||
119 | 4 | June 16, 904 | 10:45:03 | Partial | 65.8N 138.4W | 1.3251 | 0.3964 | |||
119 | 5 | June 27, 922 | 18:00:27 | Partial | 66.7N 101.8E | 1.2555 | 0.5277 | |||
119 | 6 | July 8, 940 | 1:16:23 | Partial | 67.7N 18.5W | 1.1868 | 0.6564 | |||
119 | 7 | July 19, 958 | 8:34:18 | Partial | 68.7N 139.8W | 1.1204 | 0.7797 | |||
119 | 8 | July 29, 976 | 15:55:20 | Partial | 69.6N 97.6E | 1.0571 | 0.8957 | |||
119 | 9 | August 9, 994 | 23:21:16 | Total | 70.5N 26.8W | 0.9985 | 1.0017 | - | - | |
119 | 10 | August 20, 1012 | 6:50:51 | Total | 73N 143.6E | 0.9437 | 1.0086 | 91 | 0m 32s | |
119 | 11 | August 31, 1030 | 14:27:31 | Hybrid | 64.8N 6.5E | 0.8957 | 1.0044 | 34 | 0m 18s | |
119 | 12 | September 10, 1048 | 22:09:40 | Annular | 56.8N 119.9W | 0.853 | 0.9995 | 4 | 0m 2s | |
119 | 13 | September 22, 1066 | 5:59:31 | Annular | 49.7N 115.7E | 0.8173 | 0.9941 | 35 | 0m 29s | |
119 | 14 | October 2, 1084 | 13:55:25 | Annular | 43.3N 8.6W | 0.7874 | 0.9887 | 64 | 1m 0s | |
119 | 15 | October 13, 1102 | 21:59:25 | Annular | 37.8N 133.9W | 0.7648 | 0.9833 | 91 | 1m 35s | |
119 | 16 | October 24, 1120 | 6:09:13 | Annular | 33.2N 100E | 0.7478 | 0.9781 | 117 | 2m 12s | |
119 | 17 | November 4, 1138 | 14:24:41 | Annular | 29.4N 27.2W | 0.7362 | 0.9732 | 141 | 2m 51s | |
119 | 18 | November 14, 1156 | 22:44:29 | Annular | 26.5N 155.2W | 0.7287 | 0.9687 | 164 | 3m 28s | |
119 | 19 | November 26, 1174 | 7:08:31 | Annular | 24.4N 76E | 0.725 | 0.9648 | 185 | 4m 2s | |
119 | 20 | December 6, 1192 | 15:33:28 | Annular | 23.1N 52.9W | 0.7228 | 0.9614 | 203 | 4m 30s | |
119 | 21 | December 17, 1210 | 23:58:47 | Annular | 22.5N 178.1E | 0.7215 | 0.9585 | 217 | 4m 51s | |
119 | 22 | December 28, 1228 | 8:22:01 | Annular | 22.5N 49.7E | 0.719 | 0.9563 | 227 | 5m 4s | |
119 | 23 | January 8, 1247 | 16:43:15 | Annular | 23.1N 78.1W | 0.7154 | 0.9547 | 234 | 5m 9s | |
119 | 24 | January 19, 1265 | 0:57:35 | Annular | 23.9N 156E | 0.7068 | 0.9538 | 234 | 5m 8s | |
119 | 25 | January 30, 1283 | 9:06:55 | Annular | 25.1N 31.5E | 0.6948 | 0.9533 | 232 | 5m 2s | |
119 | 26 | February 9, 1301 | 17:06:50 | Annular | 26.4N 90.3W | 0.6757 | 0.9533 | 226 | 4m 53s | |
119 | 27 | February 21, 1319 | 0:59:44 | Annular | 28N 150.1E | 0.6516 | 0.9537 | 218 | 4m 42s | |
119 | 28 | March 3, 1337 | 8:40:41 | Annular | 29.5N 34.1E | 0.6182 | 0.9543 | 207 | 4m 32s | |
119 | 29 | March 14, 1355 | 16:13:55 | Annular | 31.2N 79.3W | 0.5792 | 0.9552 | 196 | 4m 22s | |
119 | 30 | March 24, 1373 | 23:35:23 | Annular | 32.7N 170.9E | 0.5311 | 0.9561 | 186 | 4m 15s | |
119 | 31 | April 5, 1391 | 6:47:41 | Annular | 33.9N 64.2E | 0.4761 | 0.957 | 176 | 4m 11s | |
119 | 32 | April 15, 1409 | 13:49:19 | Annular | 34.6N 39.1W | 0.413 | 0.9577 | 168 | 4m 11s | |
119 | 33 | April 26, 1427 | 20:43:40 | Annular | 34.7N 140.2W | 0.3444 | 0.9583 | 161 | 4m 15s | |
119 | 34 | May 7, 1445 | 3:29:38 | Annular | 33.8N 121.2E | 0.2692 | 0.9585 | 157 | 4m 24s | |
119 | 35 | May 18, 1463 | 10:08:52 | Annular | 31.9N 24.2E | 0.189 | 0.9584 | 154 | 4m 38s | |
119 | 36 | May 28, 1481 | 16:42:59 | Annular | 28.8N 71.9W | 0.1053 | 0.9577 | 155 | 4m 57s | |
119 | 37 | June 8, 1499 | 23:13:39 | Annular | 24.7N 167.8W | 0.0195 | 0.9567 | 158 | 5m 22s | |
119 | 38 | June 19, 1517 | 5:41:31 | Annular | 19.5N 96.1E | -0.0683 | 0.9552 | 164 | 5m 50s | |
119 | 39 | June 30, 1535 | 12:08:20 | Annular | 13.5N 0.6W | -0.1565 | 0.9533 | 173 | 6m 19s | |
119 | 40 | July 10, 1553 | 18:36:34 | Annular | 6.8N 98.5W | -0.243 | 0.9509 | 185 | 6m 46s | |
119 | 41 | July 22, 1571 | 1:07:18 | Annular | 0.5S 162.1E | -0.3266 | 0.9481 | 201 | 7m 8s | |
119 | 42 | August 11, 1589 | 7:41:04 | Annular | 8.2S 61.4E | -0.4072 | 0.945 | 221 | 7m 25s | |
119 | 43 | August 22, 1607 | 14:20:48 | Annular | 16.1S 41.4W | -0.4824 | 0.9416 | 245 | 7m 34s | |
119 | 44 | September 1, 1625 | 21:06:57 | Annular | 24.2S 146.4W | -0.552 | 0.938 | 274 | 7m 37s | |
119 | 45 | September 13, 1643 | 4:01:21 | Annular | 32.3S 106.3E | -0.6145 | 0.9343 | 307 | 7m 35s | |
119 | 46 | September 23, 1661 | 11:02:34 | Annular | 40.3S 3W | -0.6711 | 0.9306 | 347 | 7m 29s | |
119 | 47 | October 4, 1679 | 18:13:56 | Annular | 48S 114.9W | -0.7191 | 0.927 | 391 | 7m 21s | |
119 | 48 | October 15, 1697 | 1:33:41 | Annular | 55.5S 131.2E | -0.7603 | 0.9236 | 441 | 7m 12s | |
119 | 49 | October 27, 1715 | 9:02:48 | Annular | 62.5S 15.5E | -0.7939 | 0.9206 | 494 | 7m 2s | |
119 | 50 | November 6, 1733 | 16:40:15 | Annular | 69S 101.2W | -0.8208 | 0.9179 | 548 | 6m 53s | |
119 | 51 | November 18, 1751 | 0:26:00 | Annular | 74.9S 142.8E | -0.8411 | 0.9159 | 597 | 6m 45s | |
119 | 52 | November 28, 1769 | 8:18:40 | Annular | 80S 32E | -0.8559 | 0.9144 | 638 | 6m 38s | |
119 | 53 | December 9, 1787 | 16:15:38 | Annular | 83.4S 62.7W | -0.8675 | 0.9136 | 672 | 6m 32s | |
119 | 54 | December 21, 1805 | 0:17:38 | Annular | 83.1S 143.8W | -0.8751 | 0.9134 | 692 | 6m 27s | |
119 | 55 | January 1, 1824 | 8:21:09 | Annular | 79.9S 116.2E | -0.8821 | 0.9139 | 705 | 6m 21s | |
119 | 56 | January 11, 1842 | 16:25:41 | Annular | 75.8S 1.4E | -0.8882 | 0.9151 | 710 | 6m 15s | |
119 | 57 | January 23, 1860 | 0:27:31 | Annular | 71.8S 117.2W | -0.8969 | 0.9168 | 719 | 6m 7s | |
119 | 58 | February 2, 1878 | 8:27:52 | Annular | 67.9S 122.4E | -0.9071 | 0.9191 | 729 | 5m 59s | |
119 | 59 | February 13, 1896 | 16:23:13 | Annular | 64.6S 3.5E | -0.922 | 0.9218 | 761 | 5m 48s | |
119 | 60 | February 25, 1914 | 0:13:01 | Annular | 62.1S 113.3W | -0.9416 | 0.9248 | 839 | 5m 35s | |
119 | 61 | March 7, 1932 | 7:55:50 | Annular | 60.7S 134.4E | -0.9673 | 0.9277 | 1083 | 5m 19s | |
119 | 62 | March 18, 1950 | 15:32:01 | Annular | 60.9S 40.9E | 0.9988 | 0.962 | - | - | |
119 | 63 | March 28, 1968 | 23:00:30 | Partial | 61S 79.8W | -1.037 | 0.899 | |||
119 | 64 | April 9, 1986 | 6:21:22 | Partial | 61.2S 161.4E | -1.0822 | 0.8236 | |||
119 | 65 | April 19, 2004 | 13:35:05 | Partial | 61.6S 44.3E | -1.1335 | 0.7367 | |||
119 | 66 | April 30, 2022 | 20:42:36 | Partial | 62.1S 71.5W | -1.1901 | 0.6396 | |||
119 | 67 | May 11, 2040 | 3:43:02 | Partial | 62.8S 174.4E | -1.2529 | 0.5306 | |||
119 | 68 | May 22, 2058 | 10:39:25 | Partial | 63.5S 61.1E | -1.3194 | 0.4141 | |||
119 | 69 | June 1, 2076 | 17:31:22 | Partial | 64.4S 51.2W | -1.3897 | 0.2897 | |||
119 | 70 | June 13, 2094 | 0:22:11 | Partial | 65.3S 163.6W | -1.4613 | 0.1618 | |||
119 | 71 | June 24, 2112 | 7:09:53 | Partial | 66.3S 84.4E | -1.5356 | 0.0282 |
A partial solar eclipse took place on 19 April 2004. 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. It was largely visible over the south Atlantic Ocean and north shores of Antarctica, most prominently the Antarctic Peninsula.
A partial solar eclipse will occur on Saturday, April 30, 2022. 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 on April 9, 1986. 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 on March 28, 1968. 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 March 18, 1950. 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.
A partial solar eclipse will occur on Friday, May 11, 2040. 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 will occur on Wednesday, May 22, 2058. 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 will occur on Monday, June 1, 2076. 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 will occur on June 12–13, 2094. 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. In the West of International Date Line it is June 12 local time.
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 occurs 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 occurs 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 occurs 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 occurs at the Moon's ascending 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 occurs 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 occurs at the Moon's descending node.
Saros cycle series 145 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 77 events. It is currently a young cycle producing total eclipses less than 3 minutes in length. The series started with a partial solar eclipse on January 4, 1639, and reached a first annular eclipse on June 6, 1891. It was a hybrid event on June 17, 1909, and total eclipses from June 29, 1927, through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. The longest duration eclipse in the cycle will be member 50 at 7 minutes and 12 seconds in length on June 25, 2522, after which the durations of eclipses will decrease until the end of the cycle. In its central phase it will produce mainly total eclipses. 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 occurs at the Moon's descending node.
Saros cycle series 155 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days. Saros 155 contains 71 events in which of 15 will be partial solar eclipses and other 56 are umbral. There are 60 solar eclipses before 3000 AD. All eclipses in this series occurs at the Moon's ascending node.
An annular solar eclipse occurred on March 7, 1932. 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 February 25, 1914. 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.