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![]() 2020 Jan 10 |
Saros cycle series 144 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 71 events. [1]
This lunar saros is linked to Solar Saros 151.
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 | ||||||||
09043 | 144 | 1 | 1749 Jul 29 | 16:31:02 | Penumbral | 1.5083 | -0.8842 | 67.7 | 15:57:11 | 17:04:53 | |||||||
09090 | 144 | 2 | 1767 Aug 10 | 0:02:55 | Penumbral | 1.4447 | -0.7690 | 113.2 | 23:06:19 | 0:59:31 | |||||||
09135 | 144 | 3 | 1785 Aug 20 | 7:38:39 | Penumbral | 1.3843 | -0.6598 | 142.9 | 6:27:12 | 8:50:06 | |||||||
09180 | 144 | 4 | 1803 Sep 01 | 15:19:10 | Penumbral | 1.3282 | -0.5589 | 165.1 | 13:56:37 | 16:41:43 | |||||||
09225 | 144 | 5 | 1821 Sep 11 | 23:04:56 | Penumbral | 1.2766 | -0.4666 | 182.9 | 21:33:29 | 0:36:23 | |||||||
09271 | 144 | 6 | 1839 Sep 23 | 6:57:39 | Penumbral | 1.2311 | -0.3855 | 197.0 | 5:19:09 | 8:36:09 | |||||||
09316 | 144 | 7 | 1857 Oct 03 | 14:56:57 | Penumbral | 1.1914 | -0.3150 | 208.4 | 13:12:45 | 16:41:09 | |||||||
09360 | 144 | 8 | 1875 Oct 14 | 23:02:55 | Penumbral | 1.1577 | -0.2558 | 217.7 | 21:14:04 | 0:51:46 | |||||||
09404 | 144 | 9 | 1893 Oct 25 | 7:16:16 | Penumbral | 1.1305 | -0.2084 | 225.0 | 5:23:46 | 9:08:46 | |||||||
09446 | 144 | 10 | 1911 Nov 06 | 15:36:45 | Penumbral | 1.1100 | -0.1733 | 230.6 | 13:41:27 | 17:32:03 | |||||||
09488 | 144 | 11 | 1929 Nov 17 | 0:03:13 | Penumbral | 1.0947 | -0.1474 | 235.0 | 22:05:43 | 2:00:43 | |||||||
09530 | 144 | 12 | 1947 Nov 28 | 8:34:29 | Penumbral | 1.0838 | -0.1297 | 238.3 | 6:35:20 | 10:33:38 | |||||||
09571 | 144 | 13 | 1965 Dec 08 | 17:10:32 | Penumbral | 1.0774 | -0.1201 | 240.7 | 15:10:11 | 19:10:53 | |||||||
09612 | 144 | 14 | 1983 Dec 20 | 1:49:57 | Penumbral | 1.0746 | -0.1167 | 242.3 | 23:48:48 | 3:51:06 | |||||||
09653 | 144 | 15 | 2001 Dec 30 | 10:30:22 | Penumbral | 1.0731 | -0.1155 | 243.5 | 8:28:37 | 12:32:07 | |||||||
09694 | 144 | 16 | 2020 Jan 10 | 19:11:11 | Penumbral | 1.0726 | -0.1160 | 244.6 | 17:08:53 | 21:13:29 | |||||||
09735 | 144 | 17 | 2038 Jan 21 | 3:49:52 | Penumbral | 1.0710 | -0.1140 | 245.8 | 1:46:58 | 5:52:46 | |||||||
09775 | 144 | 18 | 2056 Feb 01 | 12:26:06 | Penumbral | 1.0682 | -0.1096 | 247.2 | 10:22:30 | 14:29:42 | |||||||
09816 | 144 | 19 | 2074 Feb 11 | 20:55:58 | Penumbral | 1.0611 | -0.0972 | 249.5 | 18:51:13 | 23:00:43 | |||||||
09857 | 144 | 20 | 2092 Feb 23 | 5:20:59 | Penumbral | 1.0509 | -0.0789 | 252.4 | 3:14:47 | 7:27:11 | |||||||
09900 | 144 | 21 | 2110 Mar 06 | 13:37:20 | Penumbral | 1.0345 | -0.0491 | 256.4 | 11:29:08 | 15:45:32 | |||||||
09942 | 144 | 22 | 2128 Mar 16 | 21:46:08 | Penumbral | 1.0128 | -0.0093 | 261.3 | 19:35:29 | 23:56:47 | |||||||
09985 | 144 | 23 | 2146 Mar 28 | 5:44:28 | Partial | 0.9832 | 0.0448 | 267.6 | 48.6 | 3:30:40 | 7:58:16 | 5:20:10 | 6:08:46 | ||||
10029 | 144 | 24 | 2164 Apr 07 | 13:34:34 | Partial | 0.9479 | 0.1095 | 274.6 | 75.5 | 11:17:16 | 15:51:52 | 12:56:49 | 14:12:19 | ||||
10072 | 144 | 25 | 2182 Apr 18 | 21:14:14 | Partial | 0.9049 | 0.1883 | 282.5 | 98.3 | 18:52:59 | 23:35:29 | 20:25:05 | 22:03:23 | ||||
10115 | 144 | 26 | 2200 Apr 30 | 4:44:34 | Partial | 0.8550 | 0.2797 | 291.1 | 118.6 | 2:19:01 | 7:10:07 | 3:45:16 | 5:43:52 | ||||
10159 | 144 | 27 | 2218 May 11 | 12:05:34 | Partial | 0.7980 | 0.3839 | 300.0 | 137.2 | 9:35:34 | 14:35:34 | 10:56:58 | 13:14:10 | ||||
10203 | 144 | 28 | 2236 May 21 | 19:18:51 | Partial | 0.7352 | 0.4987 | 309.1 | 154.2 | 16:44:18 | 21:53:24 | 18:01:45 | 20:35:57 | ||||
10248 | 144 | 29 | 2254 Jun 02 | 2:24:40 | Partial | 0.6670 | 0.6231 | 317.9 | 169.5 | 23:45:43 | 5:03:37 | 0:59:55 | 3:49:25 | ||||
10294 | 144 | 30 | 2272 Jun 12 | 9:23:36 | Partial | 0.5938 | 0.7565 | 326.5 | 183.3 | 6:40:21 | 12:06:51 | 7:51:57 | 10:55:15 | ||||
10341 | 144 | 31 | 2290 Jun 23 | 16:17:39 | Partial | 0.5172 | 0.8959 | 334.4 | 195.3 | 13:30:27 | 19:04:51 | 14:40:00 | 17:55:18 | ||||
10388 | 144 | 32 | 2308 Jul 04 | 23:07:47 | Total | 0.4377 | 1.0404 | 341.6 | 205.5 | 31.9 | 20:16:59 | 1:58:35 | 21:25:02 | 22:51:50 | 23:23:44 | 0:50:32 | |
10434 | 144 | 33 | 2326 Jul 16 | 5:54:47 | Total | 0.3565 | 1.1878 | 347.8 | 214.0 | 65.9 | 3:00:53 | 8:48:41 | 4:07:47 | 5:21:50 | 6:27:44 | 7:41:47 | |
10480 | 144 | 34 | 2344 Jul 26 | 12:40:59 | Total | 0.2752 | 1.3351 | 353.2 | 220.7 | 83.8 | 9:44:23 | 15:37:35 | 10:50:38 | 11:59:05 | 13:22:53 | 14:31:20 | |
10525 | 144 | 35 | 2362 Aug 06 | 19:27:11 | Total | 0.1948 | 1.4807 | 357.5 | 225.7 | 94.9 | 16:28:26 | 22:25:56 | 17:34:20 | 18:39:44 | 20:14:38 | 21:20:02 | |
10570 | 144 | 36 | 2380 Aug 17 | 2:16:10 | Total | 0.1172 | 1.6209 | 360.8 | 229.1 | 101.5 | 23:15:46 | 5:16:34 | 0:21:37 | 1:25:25 | 3:06:55 | 4:10:43 | |
10614 | 144 | 37 | 2398 Aug 28 | 9:06:27 | Total | 0.0414 | 1.7575 | 363.3 | 230.9 | 104.6 | 6:04:48 | 12:08:06 | 7:11:00 | 8:14:09 | 9:58:45 | 11:01:54 | |
10659 | 144 | 38 | 2416 Sep 07 | 16:02:33 | Total | -0.0288 | 1.7780 | 364.9 | 231.5 | 104.9 | 13:00:06 | 19:05:00 | 14:06:48 | 15:10:06 | 16:55:00 | 17:58:18 | |
10703 | 144 | 39 | 2434 Sep 18 | 23:02:35 | Total | -0.0951 | 1.6538 | 365.8 | 230.9 | 102.8 | 19:59:41 | 2:05:29 | 21:07:08 | 22:11:11 | 23:53:59 | 0:58:02 | |
10747 | 144 | 40 | 2452 Sep 29 | 6:10:28 | Total | -0.1542 | 1.5426 | 366.2 | 229.6 | 98.7 | 3:07:22 | 9:13:34 | 4:15:40 | 5:21:07 | 6:59:49 | 8:05:16 | |
10789 | 144 | 41 | 2470 Oct 10 | 13:23:39 | Total | -0.2084 | 1.4405 | 366.2 | 227.5 | 93.0 | 10:20:33 | 16:26:45 | 11:29:54 | 12:37:09 | 14:10:09 | 15:17:24 | |
10831 | 144 | 42 | 2488 Oct 20 | 20:46:19 | Total | -0.2544 | 1.3535 | 365.9 | 225.2 | 86.4 | 17:43:22 | 23:49:16 | 18:53:43 | 20:03:07 | 21:29:31 | 22:38:55 | |
10872 | 144 | 43 | 2506 Nov 02 | 4:15:24 | Total | -0.2945 | 1.2773 | 365.6 | 222.8 | 78.8 | 1:12:36 | 7:18:12 | 2:24:00 | 3:36:00 | 4:54:48 | 6:06:48 | |
10913 | 144 | 44 | 2524 Nov 12 | 11:52:58 | Total | -0.3270 | 1.2152 | 365.2 | 220.4 | 71.0 | 8:50:22 | 14:55:34 | 10:02:46 | 11:17:28 | 12:28:28 | 13:43:10 | |
10954 | 144 | 45 | 2542 Nov 23 | 19:37:00 | Total | -0.3540 | 1.1635 | 364.9 | 218.3 | 63.1 | 16:34:33 | 22:39:27 | 17:47:51 | 19:05:27 | 20:08:33 | 21:26:09 | |
10996 | 144 | 46 | 2560 Dec 04 | 3:28:39 | Total | -0.3739 | 1.1250 | 364.8 | 216.6 | 55.9 | 0:26:15 | 6:31:03 | 1:40:21 | 3:00:42 | 3:56:36 | 5:16:57 | |
11037 | 144 | 47 | 2578 Dec 15 | 11:24:39 | Total | -0.3903 | 1.0933 | 364.7 | 215.1 | 48.8 | 8:22:18 | 14:27:00 | 9:37:06 | 11:00:15 | 11:49:03 | 13:12:12 | |
11077 | 144 | 48 | 2596 Dec 25 | 19:24:44 | Total | -0.4030 | 1.0688 | 364.6 | 213.9 | 42.3 | 16:22:26 | 22:27:02 | 17:37:47 | 19:03:35 | 19:45:53 | 21:11:41 | |
11117 | 144 | 49 | 2615 Jan 07 | 3:27:06 | Total | -0.4133 | 1.0490 | 364.6 | 213.0 | 36.0 | 0:24:48 | 6:29:24 | 1:40:36 | 3:09:06 | 3:45:06 | 5:13:36 | |
11156 | 144 | 50 | 2633 Jan 17 | 11:31:11 | Total | -0.4215 | 1.0334 | 364.5 | 212.2 | 29.9 | 8:28:56 | 14:33:26 | 9:45:05 | 11:16:14 | 11:46:08 | 13:17:17 | |
11197 | 144 | 51 | 2651 Jan 28 | 19:32:59 | Total | -0.4314 | 1.0151 | 364.1 | 211.2 | 20.2 | 16:30:56 | 22:35:02 | 17:47:23 | 19:22:53 | 19:43:05 | 21:18:35 | |
11239 | 144 | 52 | 2669 Feb 08 | 3:33:04 | Partial | -0.4424 | 0.9951 | 363.5 | 210.0 | 0:31:19 | 6:34:49 | 1:48:04 | 5:18:04 | ||||
11282 | 144 | 53 | 2687 Feb 19 | 11:28:02 | Partial | -0.4574 | 0.9682 | 362.5 | 208.3 | 8:26:47 | 14:29:17 | 9:43:53 | 13:12:11 | ||||
11325 | 144 | 54 | 2705 Mar 02 | 19:18:45 | Partial | -0.4756 | 0.9357 | 361.1 | 206.2 | 16:18:12 | 22:19:18 | 17:35:39 | 21:01:51 | ||||
11368 | 144 | 55 | 2723 Mar 14 | 3:00:48 | Partial | -0.5004 | 0.8913 | 358.9 | 202.9 | 0:01:21 | 6:00:15 | 1:19:21 | 4:42:15 | ||||
11410 | 144 | 56 | 2741 Mar 24 | 10:36:55 | Partial | -0.5301 | 0.8383 | 356.2 | 198.7 | 7:38:49 | 13:35:01 | 8:57:34 | 12:16:16 | ||||
11454 | 144 | 57 | 2759 Apr 04 | 18:03:23 | Partial | -0.5676 | 0.7710 | 352.5 | 192.9 | 15:07:08 | 20:59:38 | 16:26:56 | 19:39:50 | ||||
11498 | 144 | 58 | 2777 Apr 15 | 1:22:23 | Partial | -0.6112 | 0.6927 | 347.8 | 185.3 | 22:28:29 | 4:16:17 | 23:49:44 | 2:55:02 | ||||
11544 | 144 | 59 | 2795 Apr 26 | 8:31:28 | Partial | -0.6630 | 0.5996 | 341.7 | 175.0 | 5:40:37 | 11:22:19 | 7:03:58 | 9:58:58 | ||||
11590 | 144 | 60 | 2813 May 6 | 15:33:47 | Partial | -0.7203 | 0.4963 | 334.4 | 161.9 | 12:46:35 | 18:20:59 | 14:12:50 | 16:54:44 | ||||
11638 | 144 | 61 | 2831 May 17 | 22:27:44 | Partial | -0.7844 | 0.3804 | 325.5 | 144.2 | 19:44:59 | 1:10:29 | 21:15:38 | 23:39:50 | ||||
11684 | 144 | 62 | 2849 May 28 | 5:14:53 | Partial | -0.8542 | 0.2543 | 314.7 | 120.0 | 2:37:32 | 7:52:14 | 4:14:53 | 6:14:53 | ||||
11730 | 144 | 63 | 2867 Jun 08 | 11:56:08 | Partial | -0.9288 | 0.1189 | 301.8 | 83.6 | 9:25:14 | 14:27:02 | 11:14:20 | 12:37:56 | ||||
11776 | 144 | 64 | 2885 Jun 18 | 18:33:10 | Penumbral | -1.0070 | -0.0230 | 286.6 | 16:09:52 | 20:56:28 | |||||||
11822 | 144 | 65 | 2903 Jul 01 | 1:07:21 | Penumbral | -1.0874 | -0.1692 | 269.0 | 22:52:51 | 3:21:51 | |||||||
11867 | 144 | 66 | 2921 Jul 11 | 7:38:47 | Penumbral | -1.1700 | -0.3194 | 248.2 | 5:34:41 | 9:42:53 | |||||||
11912 | 144 | 67 | 2939 Jul 22 | 14:10:52 | Penumbral | -1.2522 | -0.4692 | 224.2 | 12:18:46 | 16:02:58 | |||||||
11957 | 144 | 68 | 2957 Aug 01 | 20:43:50 | Penumbral | -1.3338 | -0.6182 | 195.8 | 19:05:56 | 22:21:44 | |||||||
12003 | 144 | 69 | 2975 Aug 13 | 3:19:41 | Penumbral | -1.4131 | -0.7631 | 161.8 | 1:58:47 | 4:40:35 | |||||||
12047 | 144 | 70 | 2993 Aug 23 | 9:59:37 | Penumbral | -1.4893 | -0.9024 | 118.1 | 9:00:34 | 10:58:40 |
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 penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Sunday, December 30, 2001, with an umbral magnitude of −0.1141. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into 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 3.7 days before perigee, the Moon's apparent diameter was larger.
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 took place at the Moon's descending node of the orbit on Tuesday, September 16, 1997, the second of two lunar eclipses in 1997. A shallow total eclipse saw the Moon in relative darkness for 1 hour, 1 minute and 30.8 seconds. The Moon was 19.094% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours, 16 minutes and 28.2 seconds in total. The penumbral eclipse lasted for 5 hours, 8 minutes and 20.1 seconds. The partial eclipse lasted for 3 hours, 16 minutes and 28.2 seconds. The total eclipse lasted for 1 hour, 1 minute and 30.8 seconds. Maximum eclipse was at 18:46:39.1 UTC. The moon's apparent diameter was extremely large because occurred only 3 hours and 21 minutes past perigee. The Moon was only 356,986 km of the Earth at greatest eclipse.
A total lunar eclipse will occur at the Moon’s descending node of orbit on Thursday, October 19, 2051, with an umbral magnitude of 1.4130. 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 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 penumbral lunar eclipse took place on Tuesday, December 20, 1983, the second of two lunar eclipses in 1983. At the maximum eclipse, 89% of the Moon's disk was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours and 2 minutes overall.
A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Friday, January 10, 2020, with an umbral magnitude of −0.1146. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into 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 2.8 days before perigee, the Moon's apparent diameter was larger.
A total lunar eclipse took place on Thursday, September 6, 1979, the second of two lunar eclipses in 1979. A shallow total eclipse saw the Moon in relative darkness for 44 minutes and 24.7 seconds. The Moon was 9.358% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours, 11 minutes and 54.1 seconds in total.
A total lunar eclipse will occur at the Moon’s descending node of orbit on Saturday, October 8, 2033, with an umbral magnitude of 1.3508. 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 3 hours after perigee, the Moon's apparent diameter will be larger.
A penumbral lunar eclipse will occur at the Moon’s ascending node of orbit on Thursday, January 21, 2038, with an umbral magnitude of −0.1127. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into 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 3.1 days before perigee, the Moon's apparent diameter will be larger.
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 penumbral lunar eclipse will occur at the Moon’s ascending node of orbit on Wednesday, December 8, 1965, with an umbral magnitude of −0.1200. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into 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 2.5 days before perigee, the Moon's apparent diameter was larger.
A partial lunar eclipse occurred at the Moon’s descending node of orbit on Saturday, August 26, 1961, with an umbral magnitude of 0.9863. 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 7.5 hours after perigee, the Moon's apparent diameter was larger.
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.