| Member 44 | Member 45 |
|---|---|
 2003 Nov 09 |  2021 Nov 19 |
Saros cycle series 126 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 70 member events, with 14 total eclipses, starting in 1769 and ending in 2003. [1]
This lunar saros is linked to Solar Saros 133.
| Cat. | Saros | Mem | Date | Time UT (hr:mn) | Type | Gamma | Magnitude | Duration (min) | Contacts UT (hr:mn) | Chart | |||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Greatest | Pen. | Par. | Tot. | P1 | P4 | U1 | U2 | U3 | U4 | ||||||||
| 07795 | 126 | 1 | 1228 Jul 18 | 18:28:45 | Penumbral | 1.4996 | -0.8858 | 87.1 | 17:45:12 | 19:12:18 | |||||||
| 07840 | 126 | 2 | 1246 Jul 30 | 1:46:44 | Penumbral | 1.4376 | -0.7746 | 128.0 | 0:42:44 | 2:50:44 | |||||||
| 07885 | 126 | 3 | 1264 Aug 09 | 9:08:46 | Penumbral | 1.3792 | -0.6701 | 156.5 | 7:50:31 | 10:27:01 | |||||||
| 07930 | 126 | 4 | 1282 Aug 20 | 16:34:27 | Penumbral | 1.3244 | -0.5725 | 178.9 | 15:05:00 | 18:03:54 | |||||||
| 07975 | 126 | 5 | 1300 Aug 31 | 0:06:34 | Penumbral | 1.2753 | -0.4854 | 196.5 | 22:28:19 | 1:44:49 | |||||||
| 08018 | 126 | 6 | 1318 Sep 11 | 7:44:46 | Penumbral | 1.2321 | -0.4092 | 210.8 | 5:59:22 | 9:30:10 | |||||||
| 08060 | 126 | 7 | 1336 Sep 21 | 15:30:34 | Penumbral | 1.1952 | -0.3447 | 222.3 | 13:39:25 | 17:21:43 | |||||||
| 08102 | 126 | 8 | 1354 Oct 02 | 23:21:57 | Penumbral | 1.1637 | -0.2900 | 231.8 | 21:26:03 | 1:17:51 | |||||||
| 08143 | 126 | 9 | 1372 Oct 13 | 7:21:39 | Penumbral | 1.1395 | -0.2487 | 239.1 | 5:22:06 | 9:21:12 | |||||||
| 08184 | 126 | 10 | 1390 Oct 24 | 15:27:20 | Penumbral | 1.1210 | -0.2176 | 244.9 | 13:24:53 | 17:29:47 | |||||||
| 08225 | 126 | 11 | 1408 Nov 03 | 23:39:10 | Penumbral | 1.1080 | -0.1965 | 249.2 | 21:34:34 | 1:43:46 | |||||||
| 08266 | 126 | 12 | 1426 Nov 15 | 7:55:22 | Penumbral | 1.0992 | -0.1830 | 252.5 | 5:49:07 | 10:01:37 | |||||||
| 08308 | 126 | 13 | 1444 Nov 25 | 16:15:51 | Penumbral | 1.0945 | -0.1764 | 254.8 | 14:08:27 | 18:23:15 | |||||||
| 08349 | 126 | 14 | 1462 Dec 07 | 0:38:21 | Penumbral | 1.0920 | -0.1738 | 256.5 | 22:30:06 | 2:46:36 | |||||||
| 08389 | 126 | 15 | 1480 Dec 17 | 9:00:49 | Penumbral | 1.0903 | -0.1722 | 258.0 | 6:51:49 | 11:09:49 | |||||||
| 08429 | 126 | 16 | 1498 Dec 28 | 17:22:57 | Penumbral | 1.0890 | -0.1710 | 259.3 | 15:13:18 | 19:32:36 | |||||||
| 08469 | 126 | 17 | 1517 Jan 08 | 1:41:58 | Penumbral | 1.0862 | -0.1668 | 260.9 | 23:31:31 | 3:52:25 | |||||||
| 08510 | 126 | 18 | 1535 Jan 19 | 9:56:17 | Penumbral | 1.0800 | -0.1560 | 263.1 | 7:44:44 | 12:07:50 | |||||||
| 08552 | 126 | 19 | 1553 Jan 29 | 18:03:50 | Penumbral | 1.0690 | -0.1363 | 266.2 | 15:50:44 | 20:16:56 | |||||||
| 08596 | 126 | 20 | 1571 Feb 10 | 2:04:37 | Penumbral | 1.0535 | -0.1079 | 270.2 | 23:49:31 | 4:19:43 | |||||||
| 08639 | 126 | 21 | 1589 Mar 02 | 9:56:49 | Penumbral | 1.0319 | -0.0681 | 275.3 | 7:39:10 | 12:14:28 | |||||||
| 08682 | 126 | 22 | 1607 Mar 13 | 17:38:53 | Penumbral | 1.0028 | -0.0145 | 281.6 | 15:18:05 | 19:59:41 | |||||||
| 08727 | 126 | 23 | 1625 Mar 24 | 1:11:28 | Partial | 0.9665 | 0.0524 | 289.0 | 55.0 | 22:46:58 | 3:35:58 | 0:43:58 | 1:38:58 | ||||
| 08771 | 126 | 24 | 1643 Apr 04 | 8:33:34 | Partial | 0.9222 | 0.1341 | 297.3 | 87.2 | 6:04:55 | 11:02:13 | 7:49:58 | 9:17:10 | ||||
| 08816 | 126 | 25 | 1661 Apr 14 | 15:46:19 | Partial | 0.8708 | 0.2286 | 306.2 | 112.5 | 13:13:13 | 18:19:25 | 14:50:04 | 16:42:34 | ||||
| 08861 | 126 | 26 | 1679 Apr 25 | 22:48:29 | Partial | 0.8115 | 0.3379 | 315.6 | 134.9 | 20:10:41 | 1:26:17 | 21:41:02 | 23:55:56 | ||||
| 08907 | 126 | 27 | 1697 May 6 | 5:42:53 | Partial | 0.7461 | 0.4581 | 324.9 | 154.5 | 3:00:26 | 8:25:20 | 4:25:38 | 7:00:08 | ||||
| 08953 | 126 | 28 | 1715 May 18 | 12:28:52 | Partial | 0.6739 | 0.5906 | 334.1 | 172.1 | 9:41:49 | 15:15:55 | 11:02:49 | 13:54:55 | ||||
| 09000 | 126 | 29 | 1733 May 28 | 19:08:10 | Partial | 0.5966 | 0.7324 | 342.8 | 187.6 | 16:16:46 | 21:59:34 | 17:34:22 | 20:41:58 | ||||
| 09047 | 126 | 30 | 1751 Jun 09 | 1:41:59 | Partial | 0.5150 | 0.8819 | 350.7 | 200.8 | 22:46:38 | 4:37:20 | 0:01:35 | 3:22:23 | ||||
| 09094 | 126 | 31 | 1769 Jun 19 | 8:11:40 | Total | 0.4302 | 1.0372 | 357.6 | 211.9 | 31.5 | 5:12:52 | 11:10:28 | 6:25:43 | 7:55:55 | 8:27:25 | 9:57:37 | |
| 09139 | 126 | 32 | 1787 Jun 30 | 14:39:32 | Total | 0.3440 | 1.1947 | 363.5 | 220.8 | 68.6 | 11:37:47 | 17:41:17 | 12:49:08 | 14:05:14 | 15:13:50 | 16:29:56 | |
| 09184 | 126 | 33 | 1805 Jul 11 | 21:04:52 | Total | 0.2561 | 1.3554 | 368.1 | 227.6 | 87.6 | 18:00:49 | 0:08:55 | 19:11:04 | 20:21:04 | 21:48:40 | 22:58:40 | |
| 09229 | 126 | 34 | 1823 Jul 23 | 3:32:23 | Total | 0.1699 | 1.5124 | 371.6 | 232.3 | 98.6 | 0:26:35 | 6:38:11 | 1:36:14 | 2:43:05 | 4:21:41 | 5:28:32 | |
| 09275 | 126 | 35 | 1841 Aug 02 | 10:00:51 | Total | 0.0846 | 1.6678 | 373.8 | 235.0 | 104.6 | 6:53:57 | 13:07:45 | 8:03:21 | 9:08:33 | 10:53:09 | 11:58:21 | |
| 09320 | 126 | 36 | 1859 Aug 13 | 16:34:26 | Total | 0.0038 | 1.8148 | 374.9 | 236.0 | 106.5 | 13:26:59 | 19:41:53 | 14:36:26 | 15:41:11 | 17:27:41 | 18:32:26 | |
| 09364 | 126 | 37 | 1877 Aug 23 | 23:11:35 | Total | -0.0739 | 1.6849 | 375.0 | 235.4 | 104.9 | 20:04:05 | 2:19:05 | 21:13:53 | 22:19:08 | 0:04:02 | 1:09:17 | |
| 09408 | 126 | 38 | 1895 Sep 04 | 5:56:52 | Total | -0.1449 | 1.5530 | 374.4 | 233.5 | 100.5 | 2:49:40 | 9:04:04 | 4:00:07 | 5:06:37 | 6:47:07 | 7:53:37 | |
| 09450 | 126 | 39 | 1913 Sep 15 | 12:48:19 | Total | -0.2109 | 1.4304 | 373.0 | 230.5 | 93.5 | 9:41:49 | 15:54:49 | 10:53:04 | 12:01:34 | 13:35:04 | 14:43:34 | [ dead link ] |
| 09492 | 126 | 40 | 1931 Sep 26 | 19:48:29 | Total | -0.2698 | 1.3208 | 371.2 | 226.9 | 84.2 | 16:42:53 | 22:54:05 | 17:55:02 | 19:06:23 | 20:30:35 | 21:41:56 | |
| 09534 | 126 | 41 | 1949 Oct 07 | 2:56:55 | Total | -0.3219 | 1.2236 | 369.2 | 222.9 | 72.8 | 23:52:19 | 6:01:31 | 1:05:28 | 2:20:31 | 3:33:19 | 4:48:22 | |
| 09575 | 126 | 42 | 1967 Oct 18 | 10:15:48 | Total | -0.3653 | 1.1426 | 367.1 | 218.9 | 59.8 | 7:12:15 | 13:19:21 | 8:26:21 | 9:45:54 | 10:45:42 | 12:05:15 | |
| 09617 | 126 | 43 | 1985 Oct 28 | 17:43:17 | Total | -0.4022 | 1.0736 | 365.1 | 214.9 | 43.9 | 14:40:44 | 20:45:50 | 15:55:50 | 17:21:20 | 18:05:14 | 19:30:44 | |
| 09658 | 126 | 44 | 2003 Nov 09 | 1:19:38 | Total | -0.4319 | 1.0178 | 363.2 | 211.4 | 22.0 | 22:18:02 | 4:21:14 | 23:33:56 | 1:08:38 | 1:30:38 | 3:05:20 | |
| 09699 | 126 | 45 | 2021 Nov 19 | 9:04:06 | Partial | -0.4552 | 0.9742 | 361.5 | 208.4 | 6:03:21 | 12:04:51 | 7:19:54 | 10:48:18 | ||||
| 09740 | 126 | 46 | 2039 Nov 30 | 16:56:28 | Partial | -0.4721 | 0.9426 | 360.1 | 206.0 | 13:56:25 | 19:56:31 | 15:13:28 | 18:39:28 | ||||
| 09780 | 126 | 47 | 2057 Dec 11 | 0:53:38 | Partial | -0.4853 | 0.9181 | 358.8 | 204.0 | 21:54:14 | 3:53:02 | 23:11:38 | 2:35:38 | ||||
| 09821 | 126 | 48 | 2075 Dec 22 | 8:55:55 | Partial | -0.4945 | 0.9013 | 357.6 | 202.5 | 5:57:07 | 11:54:43 | 7:14:40 | 10:37:10 | ||||
| 09862 | 126 | 49 | 2094 Jan 01 | 17:00:06 | Partial | -0.5024 | 0.8871 | 356.5 | 201.2 | 14:01:51 | 19:58:21 | 15:19:30 | 18:40:42 | ||||
| 09904 | 126 | 50 | 2112 Jan 14 | 1:06:36 | Partial | -0.5087 | 0.8764 | 355.3 | 200.1 | 22:08:57 | 4:04:15 | 23:26:33 | 2:46:39 | ||||
| 09946 | 126 | 51 | 2130 Jan 24 | 9:10:19 | Partial | -0.5173 | 0.8619 | 353.7 | 198.7 | 6:13:28 | 12:07:10 | 7:30:58 | 10:49:40 | ||||
| 09990 | 126 | 52 | 2148 Feb 04 | 17:13:45 | Partial | -0.5265 | 0.8465 | 352.0 | 197.2 | 14:17:45 | 20:09:45 | 15:35:09 | 18:52:21 | ||||
| 10034 | 126 | 53 | 2166 Feb 15 | 1:11:40 | Partial | -0.5402 | 0.8233 | 349.8 | 194.9 | 22:16:46 | 4:06:34 | 23:34:13 | 2:49:07 | ||||
| 10077 | 126 | 54 | 2184 Feb 26 | 9:05:35 | Partial | -0.5579 | 0.7930 | 347.1 | 192.0 | 6:12:02 | 11:59:08 | 7:29:35 | 10:41:35 | ||||
| 10120 | 126 | 55 | 2202 Mar 09 | 16:51:36 | Partial | -0.5824 | 0.7505 | 343.6 | 187.8 | 13:59:48 | 19:43:24 | 15:17:42 | 18:25:30 | ||||
| 10164 | 126 | 56 | 2220 Mar 20 | 0:32:40 | Partial | -0.6114 | 0.6999 | 339.4 | 182.6 | 21:42:58 | 3:22:22 | 23:01:22 | 2:03:58 | ||||
| 10209 | 126 | 57 | 2238 Mar 31 | 8:05:25 | Partial | -0.6477 | 0.6362 | 334.3 | 175.6 | 5:18:16 | 10:52:34 | 6:37:37 | 9:33:13 | ||||
| 10254 | 126 | 58 | 2256 Apr 10 | 15:31:04 | Partial | -0.6904 | 0.5606 | 328.1 | 166.5 | 12:47:01 | 18:15:07 | 14:07:49 | 16:54:19 | ||||
| 10300 | 126 | 59 | 2274 Apr 21 | 22:48:59 | Partial | -0.7401 | 0.4723 | 320.8 | 154.6 | 20:08:35 | 1:29:23 | 21:31:41 | 0:06:17 | ||||
| 10347 | 126 | 60 | 2292 May 2 | 6:00:52 | Partial | -0.7956 | 0.3735 | 312.0 | 139.2 | 3:24:52 | 8:36:52 | 4:51:16 | 7:10:28 | ||||
| 10393 | 126 | 61 | 2310 May 14 | 13:06:26 | Partial | -0.8566 | 0.2643 | 301.8 | 118.7 | 10:35:32 | 15:37:20 | 12:07:05 | 14:05:47 | ||||
| 10439 | 126 | 62 | 2328 May 24 | 20:06:39 | Partial | -0.9225 | 0.1460 | 289.9 | 89.5 | 17:41:42 | 22:31:36 | 19:21:54 | 20:51:24 | ||||
| 10485 | 126 | 63 | 2346 Jun 05 | 3:03:17 | Partial | -0.9921 | 0.0209 | 276.2 | 34.4 | 0:45:11 | 5:21:23 | 2:46:05 | 3:20:29 | ||||
| 10530 | 126 | 64 | 2364 Jun 15 | 9:57:15 | Penumbral | -1.0645 | -0.1097 | 260.4 | 7:47:03 | 12:07:27 | |||||||
| 10575 | 126 | 65 | 2382 Jun 26 | 16:49:14 | Penumbral | -1.1391 | -0.2444 | 242.3 | 14:48:05 | 18:50:23 | |||||||
| 10619 | 126 | 66 | 2400 Jul 06 | 23:41:22 | Penumbral | -1.2140 | -0.3798 | 221.8 | 21:50:28 | 1:32:16 | |||||||
| 10664 | 126 | 67 | 2418 Jul 18 | 6:34:23 | Penumbral | -1.2887 | -0.5153 | 198.1 | 4:55:20 | 8:13:26 | |||||||
| 10708 | 126 | 68 | 2436 Jul 28 | 13:31:07 | Penumbral | -1.3610 | -0.6466 | 171.1 | 12:05:34 | 14:56:40 | |||||||
| 10752 | 126 | 69 | 2454 Aug 08 | 20:30:20 | Penumbral | -1.4320 | -0.7757 | 138.2 | 19:21:14 | 21:39:26 | |||||||
| 10794 | 126 | 70 | 2472 Aug 19 | 3:36:26 | Penumbral | -1.4981 | -0.8961 | 96.8 | 2:48:02 | 4:24:50 | |||||||
The inex is an eclipse cycle of 10,571.95 days. The cycle was first described in modern times by Crommelin in 1901, but was named by George van den Bergh who studied it in detail half a century later. One inex after an eclipse of a particular saros series there will be an eclipse in the next saros series, unless the latter saros series has come to an end.
A total lunar eclipse occurred at the Moon’s ascending node of orbit on Sunday, November 9, 2003, with an umbral magnitude of 1.0197. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 1.2 days before apogee, the Moon's apparent diameter was smaller.
A partial lunar eclipse took place on Wednesday, July 28, 1999, the second of two lunar eclipses in 1999.
A partial lunar eclipse took place on Friday, July 17, 1981, the second of two lunar eclipses in 1981. The Earth's shadow on the Moon was clearly visible in this eclipse, with 55% of the Moon in shadow; the partial eclipse lasted for 2 hours and 43 minutes.
A total lunar eclipse took place on Monday, October 28, 1985, the second of two total lunar eclipses in 1985, the first being on May 4, 1985.
A total lunar eclipse took place on Thursday, April 24, 1986, the first of two total lunar eclipses in 1986, the second being on October 17, 1986. The Moon was plunged into darkness for 1 hour, 3 minutes and 34.8 seconds, in a deep total eclipse which saw the Moon 20.217% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may have been stained a deep red colour. The partial eclipse lasted for 3 hours, 18 minutes and 46.8 seconds in total. The Moon was just 1.2 days before perigee, making it 5.3% larger than average.
A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Friday, November 19, 2021, with an umbral magnitude of 0.9760. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring only about 12 hours before apogee, the Moon's apparent diameter was smaller.
A partial lunar eclipse will occur at the Moon’s ascending node of orbit on Wednesday, November 30, 2039, with an umbral magnitude of 0.9443. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 1.8 days before apogee, the Moon's apparent diameter will be smaller.
A total lunar eclipse occurred at the Moon’s descending node of orbit on Sunday, April 2, 1950, with an umbral magnitude of 1.0329. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring only about 23 hours before perigee, the Moon's apparent diameter was larger.
A total lunar eclipse took place on Wednesday, October 18, 1967, the second of two total lunar eclipses in 1967, the first being on April 24, 1967.
A total lunar eclipse occurred at the Moon’s ascending node of orbit on Monday, September 15, 1913, with an umbral magnitude of 1.4304. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring only about 30 minutes after apogee, the Moon's apparent diameter was smaller.
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 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 128 for lunar eclipses occurs at the moon's ascending node, repeating every 18 years 11 and 1/3 days. It contains 71 events. Solar saros 135 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
Saros cycle series 130 for lunar eclipses occurs at the moon's ascending node, repeats every 18 years 11+1/3 days. The 130th lunar saros is associated with Solar Saros 137.
Saros cycle series 119 for lunar eclipses occurs at the moon's descending node, repeats every 18 years 11 and 1/3 days. It contains 82 events.
Saros cycle series 127 for lunar eclipses occurs at the moon's descending node, repeats every 18 years 11 and 1/3 days. It contains 72 events. Solar saros 134 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series. It consisted with 10 penumbral eclipses, 21 partial eclipses, 11 total eclipses, 21 partial eclipses, and ends with 8 penumbral eclipses.
A total lunar eclipse occurred at the Moon’s ascending node of orbit on Friday, October 7, 1949, with an umbral magnitude of 1.2236. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring only about 15 hours before apogee, the Moon's apparent diameter was smaller.
A total lunar eclipse occurred at the Moon’s ascending node of orbit on Saturday, September 26, 1931, with an umbral magnitude of 1.3208. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring only about 8 hours before apogee, the Moon's apparent diameter was smaller.
