Saros cycle series 108 for lunar eclipses occurred at the moon's ascending node, 18 years 11 and 1/3 days. It contained 72 events. [1]
This lunar saros was linked to Solar Saros 115.
| 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 | ||||||||
| 06493 | 108 | 1 | 689 Jul 08 | 9:04:39 | Penumbral | 1.5561 | -1.0111 | 37.9 | 8:45:42 | 9:23:36 | |||||||
| 06538 | 108 | 2 | 707 Jul 19 | 15:57:32 | Penumbral | 1.4877 | -0.8881 | 111.6 | 15:01:44 | 16:53:20 | |||||||
| 06582 | 108 | 3 | 725 Jul 29 | 22:53:00 | Penumbral | 1.4218 | -0.7699 | 151.0 | 21:37:30 | 0:08:30 | |||||||
| 06626 | 108 | 4 | 743 Aug 10 | 5:54:17 | Penumbral | 1.3608 | -0.6608 | 179.3 | 4:24:38 | 7:23:56 | |||||||
| 06670 | 108 | 5 | 761 Aug 20 | 12:59:01 | Penumbral | 1.3031 | -0.5578 | 202.0 | 11:18:01 | 14:40:01 | |||||||
| 06713 | 108 | 6 | 779 Aug 31 | 20:12:04 | Penumbral | 1.2523 | -0.4676 | 219.8 | 18:22:10 | 22:01:58 | |||||||
| 06755 | 108 | 7 | 797 Sep 11 | 3:30:50 | Penumbral | 1.2065 | -0.3866 | 234.5 | 1:33:35 | 5:28:05 | |||||||
| 06796 | 108 | 8 | 815 Sep 22 | 10:58:23 | Penumbral | 1.1683 | -0.3194 | 246.1 | 8:55:20 | 13:01:26 | |||||||
| 06837 | 108 | 9 | 833 Oct 02 | 18:32:17 | Penumbral | 1.1356 | -0.2622 | 255.6 | 16:24:29 | 20:40:05 | |||||||
| 06877 | 108 | 10 | 851 Oct 14 | 2:15:28 | Penumbral | 1.1107 | -0.2193 | 262.7 | 0:04:07 | 4:26:49 | |||||||
| 06918 | 108 | 11 | 869 Oct 24 | 10:04:36 | Penumbral | 1.0909 | -0.1854 | 268.4 | 7:50:24 | 12:18:48 | |||||||
| 06959 | 108 | 12 | 887 Nov 04 | 17:59:53 | Penumbral | 1.0765 | -0.1611 | 272.7 | 15:43:32 | 20:16:14 | |||||||
| 07001 | 108 | 13 | 905 Nov 15 | 2:00:01 | Penumbral | 1.0662 | -0.1441 | 275.9 | 23:42:04 | 4:17:58 | |||||||
| 07041 | 108 | 14 | 923 Nov 26 | 10:04:30 | Penumbral | 1.0602 | -0.1346 | 278.0 | 7:45:30 | 12:23:30 | |||||||
| 07082 | 108 | 15 | 941 Dec 06 | 18:10:10 | Penumbral | 1.0551 | -0.1263 | 279.8 | 15:50:16 | 20:30:04 | |||||||
| 07123 | 108 | 16 | 959 Dec 18 | 2:15:57 | Penumbral | 1.0504 | -0.1185 | 281.4 | 23:55:15 | 4:36:39 | |||||||
| 07164 | 108 | 17 | 977 Dec 28 | 10:20:09 | Penumbral | 1.0448 | -0.1086 | 283.0 | 7:58:39 | 12:41:39 | |||||||
| 07206 | 108 | 18 | 996 Jan 08 | 18:21:43 | Penumbral | 1.0376 | -0.0952 | 284.9 | 15:59:16 | 20:44:10 | |||||||
| 07250 | 108 | 19 | 1014 Jan 19 | 2:16:49 | Penumbral | 1.0254 | -0.0726 | 287.5 | 23:53:04 | 4:40:34 | |||||||
| 07295 | 108 | 20 | 1032 Jan 30 | 10:06:26 | Penumbral | 1.0092 | -0.0421 | 290.9 | 7:40:59 | 12:31:53 | |||||||
| 07340 | 108 | 21 | 1050 Feb 09 | 17:47:23 | Partial | 0.9861 | 0.0013 | 295.3 | 8.9 | 15:19:44 | 20:15:02 | 17:42:56 | 17:51:50 | ||||
| 07384 | 108 | 22 | 1068 Feb 21 | 1:20:57 | Partial | 0.9572 | 0.0555 | 300.5 | 57.8 | 22:50:42 | 3:51:12 | 0:52:03 | 1:49:51 | ||||
| 07428 | 108 | 23 | 1086 Mar 03 | 8:43:45 | Partial | 0.9199 | 0.1254 | 306.9 | 86.1 | 6:10:18 | 11:17:12 | 8:00:42 | 9:26:48 | ||||
| 07474 | 108 | 24 | 1104 Mar 13 | 15:58:54 | Partial | 0.8762 | 0.207 | 313.8 | 109.3 | 13:22:00 | 18:35:48 | 15:04:15 | 16:53:33 | ||||
| 07520 | 108 | 25 | 1122 Mar 24 | 23:03:27 | Partial | 0.824 | 0.3044 | 321.4 | 130.7 | 20:22:45 | 1:44:09 | 21:58:06 | 0:08:48 | ||||
| 07566 | 108 | 26 | 1140 Apr 4 | 5:59:42 | Partial | 0.7647 | 0.4147 | 329.2 | 150 | 3:15:06 | 8:44:18 | 4:44:42 | 7:14:42 | ||||
| 07613 | 108 | 27 | 1158 Apr 15 | 12:47:06 | Partial | 0.6979 | 0.5388 | 337.1 | 167.7 | 9:58:33 | 15:35:39 | 11:23:15 | 14:10:57 | ||||
| 07660 | 108 | 28 | 1176 Apr 25 | 19:28:08 | Partial | 0.6255 | 0.6732 | 344.6 | 183.3 | 16:35:50 | 22:20:26 | 17:56:29 | 20:59:47 | ||||
| 07706 | 108 | 29 | 1194 May 7 | 2:03:17 | Partial | 0.5479 | 0.8169 | 351.5 | 196.8 | 23:07:32 | 4:59:02 | 0:24:53 | 3:41:41 | ||||
| 07752 | 108 | 30 | 1212 May 17 | 8:32:49 | Partial | 0.4652 | 0.9699 | 357.6 | 208.5 | 5:34:01 | 11:31:37 | 6:48:34 | 10:17:04 | ||||
| 07799 | 108 | 31 | 1230 May 28 | 15:00:09 | Total | 0.3801 | 1.1271 | 362.6 | 217.9 | 56.8 | 11:58:51 | 18:01:27 | 13:11:12 | 14:31:45 | 15:28:33 | 16:49:06 | |
| 07844 | 108 | 32 | 1248 Jun 07 | 21:24:58 | Total | 0.2922 | 1.2892 | 366.5 | 225.2 | 81.0 | 18:21:43 | 0:28:13 | 19:32:22 | 20:44:28 | 22:05:28 | 23:17:34 | |
| 07889 | 108 | 33 | 1266 Jun 19 | 3:50:18 | Total | 0.2044 | 1.4511 | 369.2 | 230.3 | 94.8 | 0:45:42 | 6:54:54 | 1:55:09 | 3:02:54 | 4:37:42 | 5:45:27 | |
| 07934 | 108 | 34 | 1284 Jun 29 | 10:16:00 | Total | 0.1164 | 1.6131 | 370.7 | 233.4 | 102.7 | 7:10:39 | 13:21:21 | 8:19:18 | 9:24:39 | 11:07:21 | 12:12:42 | |
| 07979 | 108 | 35 | 1302 Jul 10 | 16:46:06 | Total | 0.0313 | 1.7694 | 371.0 | 234.5 | 105.9 | 13:40:36 | 19:51:36 | 14:48:51 | 15:53:09 | 17:39:03 | 18:43:21 | |
| 08022 | 108 | 36 | 1320 Jul 20 | 23:20:21 | Total | -0.0510 | 1.7335 | 370.2 | 233.9 | 105.3 | 20:15:15 | 2:25:27 | 21:23:24 | 22:27:42 | 0:13:00 | 1:17:18 | |
| 08064 | 108 | 37 | 1338 Aug 01 | 6:00:25 | Total | -0.1292 | 1.5901 | 368.4 | 231.8 | 101.4 | 2:56:13 | 9:04:37 | 4:04:31 | 5:09:43 | 6:51:07 | 7:56:19 | |
| 08106 | 108 | 38 | 1356 Aug 11 | 12:47:57 | Total | -0.2017 | 1.4568 | 365.9 | 228.4 | 94.4 | 9:45:00 | 15:50:54 | 10:53:45 | 12:00:45 | 13:35:09 | 14:42:09 | |
| 08147 | 108 | 39 | 1374 Aug 22 | 19:44:13 | Total | -0.2675 | 1.3358 | 362.9 | 224.2 | 84.8 | 16:42:46 | 22:45:40 | 17:52:07 | 19:01:49 | 20:26:37 | 21:36:19 | |
| 08188 | 108 | 40 | 1392 Sep 02 | 2:49:46 | Total | -0.3265 | 1.2271 | 359.5 | 219.4 | 72.3 | 23:50:01 | 5:49:31 | 1:00:04 | 2:13:37 | 3:25:55 | 4:39:28 | |
| 08229 | 108 | 41 | 1410 Sep 13 | 10:04:27 | Total | -0.3788 | 1.1308 | 355.9 | 214.2 | 56.6 | 7:06:30 | 13:02:24 | 8:17:21 | 9:36:09 | 10:32:45 | 11:51:33 | |
| 08271 | 108 | 42 | 1428 Sep 23 | 17:29:54 | Total | -0.4230 | 1.0492 | 352.5 | 209.1 | 35.6 | 14:33:39 | 20:26:09 | 15:45:21 | 17:12:06 | 17:47:42 | 19:14:27 | |
| 08313 | 108 | 43 | 1446 Oct 05 | 1:05:29 | Partial | -0.4596 | 0.9818 | 349.2 | 204.4 | 22:10:53 | 4:00:05 | 23:23:17 | 2:47:41 | ||||
| 08354 | 108 | 44 | 1464 Oct 15 | 8:50:47 | Partial | -0.4889 | 0.9280 | 346.2 | 200.2 | 5:57:41 | 11:43:53 | 7:10:41 | 10:30:53 | ||||
| 08394 | 108 | 45 | 1482 Oct 26 | 16:45:28 | Partial | -0.5111 | 0.8871 | 343.6 | 196.7 | 13:53:40 | 19:37:16 | 15:07:07 | 18:23:49 | ||||
| 08434 | 108 | 46 | 1500 Nov 06 | 0:48:33 | Partial | -0.5272 | 0.8577 | 341.4 | 193.9 | 21:57:51 | 3:39:15 | 23:11:36 | 2:25:30 | ||||
| 08474 | 108 | 47 | 1518 Nov 17 | 8:59:11 | Partial | -0.5379 | 0.8385 | 339.5 | 191.9 | 6:09:26 | 11:48:56 | 7:23:14 | 10:35:08 | ||||
| 08515 | 108 | 48 | 1536 Nov 27 | 17:14:01 | Partial | -0.5457 | 0.8249 | 337.8 | 190.3 | 14:25:07 | 20:02:55 | 15:38:52 | 18:49:10 | ||||
| 08557 | 108 | 49 | 1554 Dec 09 | 1:34:26 | Partial | -0.5496 | 0.8188 | 336.3 | 189.3 | 22:46:17 | 4:22:35 | 23:59:47 | 3:09:05 | ||||
| 08600 | 108 | 50 | 1572 Dec 19 | 9:56:07 | Partial | -0.5525 | 0.8148 | 334.8 | 188.5 | 7:08:43 | 12:43:31 | 8:21:52 | 11:30:22 | ||||
| 08643 | 108 | 51 | 1591 Jan 09 | 18:19:22 | Partial | -0.5552 | 0.8116 | 333.3 | 187.7 | 15:32:43 | 21:06:01 | 16:45:31 | 19:53:13 | ||||
| 08687 | 108 | 52 | 1609 Jan 20 | 2:39:41 | Partial | -0.5607 | 0.8034 | 331.4 | 186.5 | 23:53:59 | 5:25:23 | 1:06:26 | 4:12:56 | ||||
| 08732 | 108 | 53 | 1627 Jan 31 | 10:59:17 | Partial | -0.5675 | 0.7932 | 329.4 | 185.2 | 8:14:35 | 13:43:59 | 9:26:41 | 12:31:53 | ||||
| 08776 | 108 | 54 | 1645 Feb 10 | 19:13:47 | Partial | -0.5789 | 0.7748 | 326.8 | 183.1 | 16:30:23 | 21:57:11 | 17:42:14 | 20:45:20 | ||||
| 08821 | 108 | 55 | 1663 Feb 22 | 3:23:34 | Partial | -0.5950 | 0.7481 | 323.8 | 180.2 | 0:41:40 | 6:05:28 | 1:53:28 | 4:53:40 | ||||
| 08867 | 108 | 56 | 1681 Mar 04 | 11:26:33 | Partial | -0.6173 | 0.7101 | 320.1 | 176.2 | 8:46:30 | 14:06:36 | 9:58:27 | 12:54:39 | ||||
| 08913 | 108 | 57 | 1699 Mar 15 | 19:23:52 | Partial | -0.6453 | 0.6619 | 315.7 | 171.0 | 16:46:01 | 22:01:43 | 17:58:22 | 20:49:22 | ||||
| 08959 | 108 | 58 | 1717 Mar 27 | 3:13:41 | Partial | -0.6800 | 0.6013 | 310.4 | 164.1 | 0:38:29 | 5:48:53 | 1:51:38 | 4:35:44 | ||||
| 09006 | 108 | 59 | 1735 Apr 07 | 10:56:51 | Partial | -0.7210 | 0.5292 | 304.2 | 155.3 | 8:24:45 | 13:28:57 | 9:39:12 | 12:14:30 | ||||
| 09053 | 108 | 60 | 1753 Apr 17 | 18:33:18 | Partial | -0.7683 | 0.4454 | 297.0 | 143.9 | 16:04:48 | 21:01:48 | 17:21:21 | 19:45:15 | ||||
| 09099 | 108 | 61 | 1771 Apr 29 | 2:04:10 | Partial | -0.8211 | 0.3515 | 288.5 | 129.3 | 23:39:55 | 4:28:25 | 0:59:31 | 3:08:49 | ||||
| 09144 | 108 | 62 | 1789 May 9 | 9:28:39 | Partial | -0.8799 | 0.2465 | 278.7 | 109.6 | 7:09:18 | 11:48:00 | 8:33:51 | 10:23:27 | ||||
| 09189 | 108 | 63 | 1807 May 21 | 16:49:32 | Partial | -0.9423 | 0.1346 | 267.4 | 82.0 | 14:35:50 | 19:03:14 | 16:08:32 | 17:30:32 | ||||
| 09234 | 108 | 64 | 1825 Jun 01 | 0:06:18 | Partial | -1.0089 | 0.0149 | 254.4 | 27.6 | 21:59:06 | 2:13:30 | 23:52:30 | 0:20:06 | ||||
| 09280 | 108 | 65 | 1843 Jun 12 | 7:22:16 | Penumbral | -1.0767 | -0.1073 | 240.0 | 5:22:16 | 9:22:16 | |||||||
| 09325 | 108 | 66 | 1861 Jun 22 | 14:35:14 | Penumbral | -1.1476 | -0.2355 | 223.2 | 12:43:38 | 16:26:50 | |||||||
| 09369 | 108 | 67 | 1879 Jul 03 | 21:50:28 | Penumbral | -1.2172 | -0.3618 | 204.6 | 20:08:10 | 23:32:46 | |||||||
| 09413 | 108 | 68 | 1897 Jul 14 | 5:05:19 | Penumbral | -1.2879 | -0.4902 | 183.0 | 3:33:49 | 6:36:49 | |||||||
| 09455 | 108 | 69 | 1915 Jul 26 | 12:24:39 | Penumbral | -1.3553 | -0.6129 | 158.7 | 11:05:18 | 13:44:00 | |||||||
| 09497 | 108 | 70 | 1933 Aug 05 | 19:46:05 | Penumbral | -1.4216 | -0.7338 | 129.5 | 18:41:20 | 20:50:50 | |||||||
| 09538 | 108 | 71 | 1951 Aug 17 | 3:14:39 | Penumbral | -1.4828 | -0.8456 | 93.6 | 2:27:51 | 4:01:27 | |||||||
| 09579 | 108 | 72 | 1969 Aug 27 | 10:48:15 | Penumbral | -1.5407 | -0.9516 | 31.3 | 10:32:36 | 11:03:54 | |||||||
The saros is a period of exactly 223 synodic months, approximately 6585.321 days, or 18 years plus 10, 11, or 12 days, and 8 hours, that can be used to predict eclipses of the Sun and Moon. One saros period after an eclipse, the Sun, Earth, and Moon return to approximately the same relative geometry, a near straight line, and a nearly identical eclipse will occur, in what is referred to as an eclipse cycle. A sar is one half of a saros.
A total lunar eclipse occurred at the Moon’s descending node of orbit on Tuesday, May 4, 2004, with an umbral magnitude of 1.3035. 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 perigee, the Moon's apparent diameter was larger.
A total lunar eclipse took place on Friday, February 9, 1990, the first of two lunar eclipses in 1990.
A total lunar eclipse took place at 0308 UT (GMT) on Thursday, August 17, 1989, the second of two total lunar eclipses in 1989.
A total lunar eclipse will occur at the Moon’s descending node of orbit on Saturday, May 26, 2040, with an umbral magnitude of 1.5365. 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 1.4 days before perigee, the Moon's apparent diameter will be larger.
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 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 will occur at the Moon’s descending node of orbit on Thursday, June 6, 2058, with an umbral magnitude of 1.6628. 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 1.6 days before perigee, the Moon's apparent diameter will be larger.
A total lunar eclipse will occur at the Moon’s descending node of orbit on Wednesday, June 17, 2076, with an umbral magnitude of 1.7959. 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 1.9 days before perigee, the Moon's apparent diameter will be larger.
A total lunar eclipse will occur at the Moon’s descending node of orbit on Monday, June 28, 2094, with an umbral magnitude of 1.8249. 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 1.9 days before perigee, the Moon's apparent diameter will be larger.
A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, March 12, 1914, with an umbral magnitude of 0.9111. 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 18 hours before perigee, the Moon's apparent diameter was larger.
A penumbral lunar eclipse took place on Wednesday, August 27, 1969, the second of three penumbral lunar eclipses in 1969, the first being on Wednesday, April 2, and the last being on Thursday, September 25. This is the last lunar eclipse of Saros 108.
A partial solar eclipse occurred at the Moon's descending node of orbit on Tuesday, April 8, 1902, with a magnitude of 0.0643. 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.
Saros cycle series 112 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 72 events, with 15 total eclipses, starting in 1364 and ending in 1616. Solar Saros 119 interleaves with this lunar Saros with an event occurring every 9 years 5 days alternating between each saros series.
Saros cycle series 114 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 71 member events, with 13 total eclipses, starting in 1458 and ending in 1674. Solar saros 121 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
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 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.
Saros cycle series 129 for lunar eclipses occurs at the moon's descending node, repeats every 18 years 11+1/3 days. The 129th lunar saros is associated with Solar Saros 136.
Saros cycle series 101 for lunar eclipses occurred at the moon's descending node, 18 years 11 and 1/3 days. It contained 72 events.
