Saros cycle series 157 for lunar eclipses occurs at the moon's descending node, repeats every 18 years 11 and 1/3 days. It contains 73 events (39 events listed before 3000). [1]
| 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 | ||||||||
| 10382 | 157 | 1 | 2306 Mar 01 | 13:42:55 | Penumbral | -1.5675 | -1.0597 | 47.5 | 13:19:10 | 14:06:40 | |||||||
| 10428 | 157 | 2 | 2324 Mar 11 | 21:29:30 | Penumbral | -1.5451 | -1.0182 | 78.0 | 20:50:30 | 22:08:30 | |||||||
| 10474 | 157 | 3 | 2342 Mar 23 | 5:08:18 | Penumbral | -1.5166 | -0.9654 | 104.3 | 4:16:09 | 6:00:27 | |||||||
| 10519 | 157 | 4 | 2360 Apr 02 | 12:35:50 | Penumbral | -1.4797 | -0.8970 | 130.4 | 11:30:38 | 13:41:02 | |||||||
| 10564 | 157 | 5 | 2378 Apr 13 | 19:55:16 | Penumbral | -1.4366 | -0.8170 | 154.9 | 18:37:49 | 21:12:43 | |||||||
| 10608 | 157 | 6 | 2396 Apr 24 | 3:03:43 | Penumbral | -1.3852 | -0.7219 | 179.1 | 1:34:10 | 4:33:16 | |||||||
| 10653 | 157 | 7 | 2414 May 5 | 10:04:13 | Penumbral | -1.3275 | -0.6152 | 202.2 | 8:23:07 | 11:45:19 | |||||||
| 10697 | 157 | 8 | 2432 May 15 | 16:54:29 | Penumbral | -1.2616 | -0.4934 | 224.6 | 15:02:11 | 18:46:47 | |||||||
| 10741 | 157 | 9 | 2450 May 26 | 23:38:32 | Penumbral | -1.1906 | -0.3626 | 245.5 | 21:35:47 | 1:41:17 | |||||||
| 10784 | 157 | 10 | 2468 Jun 06 | 6:15:13 | Penumbral | -1.1139 | -0.2213 | 265.1 | 4:02:40 | 8:27:46 | |||||||
| 10826 | 157 | 11 | 2486 Jun 17 | 12:46:55 | Penumbral | -1.0329 | -0.0722 | 283.1 | 10:25:22 | 15:08:28 | |||||||
| 10867 | 157 | 12 | 2504 Jun 28 | 19:14:33 | Partial | -0.9484 | 0.0831 | 299.4 | 70.5 | 16:44:51 | 21:44:15 | 18:39:18 | 19:49:48 | ||||
| 10908 | 157 | 13 | 2522 Jul 10 | 1:40:39 | Partial | -0.8624 | 0.2409 | 313.8 | 117.4 | 23:03:45 | 4:17:33 | 0:41:57 | 2:39:21 | ||||
| 10948 | 157 | 14 | 2540 Jul 20 | 8:06:21 | Partial | -0.7756 | 0.4001 | 326.4 | 147.7 | 5:23:09 | 10:49:33 | 6:52:30 | 9:20:12 | ||||
| 10990 | 157 | 15 | 2558 Jul 31 | 14:32:26 | Partial | -0.6888 | 0.5590 | 337.3 | 170.3 | 11:43:47 | 17:21:05 | 13:07:17 | 15:57:35 | ||||
| 11031 | 157 | 16 | 2576 Aug 10 | 21:01:26 | Partial | -0.6042 | 0.7139 | 346.4 | 187.5 | 18:08:14 | 23:54:38 | 19:27:41 | 22:35:11 | ||||
| 11071 | 157 | 17 | 2594 Aug 22 | 3:34:22 | Partial | -0.5225 | 0.8632 | 353.8 | 200.7 | 0:37:28 | 6:31:16 | 1:54:01 | 5:14:43 | ||||
| 11111 | 157 | 18 | 2612 Sep 02 | 10:12:37 | Total | -0.4447 | 1.0052 | 359.8 | 210.9 | 12.0 | 7:12:43 | 13:12:31 | 8:27:10 | 10:06:37 | 10:18:37 | 11:58:04 | |
| 11151 | 157 | 19 | 2630 Sep 13 | 16:57:18 | Total | -0.3718 | 1.1381 | 364.3 | 218.5 | 59.0 | 13:55:09 | 19:59:27 | 15:08:03 | 16:27:48 | 17:26:48 | 18:46:33 | |
| 11192 | 157 | 20 | 2648 Sep 23 | 23:50:09 | Total | -0.3051 | 1.2595 | 367.7 | 223.9 | 77.4 | 20:46:18 | 2:54:00 | 21:58:12 | 23:11:27 | 0:28:51 | 1:42:06 | |
| 11234 | 157 | 21 | 2666 Oct 05 | 6:52:02 | Total | -0.2457 | 1.3675 | 370.1 | 227.7 | 88.3 | 3:46:59 | 9:57:05 | 4:58:11 | 6:07:53 | 7:36:11 | 8:45:53 | |
| 11277 | 157 | 22 | 2684 Oct 15 | 14:01:43 | Total | -0.1924 | 1.4645 | 371.6 | 230.3 | 95.2 | 10:55:55 | 17:07:31 | 12:06:34 | 13:14:07 | 14:49:19 | 15:56:52 | |
| 11319 | 157 | 23 | 2702 Oct 27 | 21:21:47 | Total | -0.1470 | 1.5467 | 372.5 | 231.8 | 99.4 | 18:15:32 | 0:28:02 | 19:25:53 | 20:32:05 | 22:11:29 | 23:17:41 | |
| 11362 | 157 | 24 | 2720 Nov 07 | 4:50:33 | Total | -0.1083 | 1.6171 | 372.9 | 232.6 | 102.0 | 1:44:06 | 7:57:00 | 2:54:15 | 3:59:33 | 5:41:33 | 6:46:51 | |
| 11404 | 157 | 25 | 2738 Nov 18 | 12:29:42 | Total | -0.0776 | 1.6726 | 372.9 | 232.9 | 103.3 | 9:23:15 | 15:36:09 | 10:33:15 | 11:38:03 | 13:21:21 | 14:26:09 | |
| 11447 | 157 | 26 | 2756 Nov 28 | 20:15:29 | Total | -0.0519 | 1.7193 | 372.7 | 232.8 | 104.0 | 17:09:08 | 23:21:50 | 18:19:05 | 19:23:29 | 21:07:29 | 22:11:53 | |
| 11491 | 157 | 27 | 2774 Dec 10 | 4:10:47 | Total | -0.0334 | 1.7531 | 372.2 | 232.6 | 104.2 | 1:04:41 | 7:16:53 | 2:14:29 | 3:18:41 | 5:02:53 | 6:07:05 | |
| 11537 | 157 | 28 | 2792 Dec 20 | 12:11:32 | Total | -0.0186 | 1.7803 | 371.6 | 232.3 | 104.2 | 9:05:44 | 15:17:20 | 10:15:23 | 11:19:26 | 13:03:38 | 14:07:41 | |
| 11583 | 157 | 29 | 2810 Dec 31 | 20:18:19 | Total | -0.0081 | 1.8000 | 370.8 | 231.9 | 104.1 | 17:12:55 | 23:23:43 | 18:22:22 | 19:26:16 | 21:10:22 | 22:14:16 | |
| 11631 | 157 | 30 | 2829 Jan 11 | 4:27:25 | Total | 0.0011 | 1.8136 | 369.9 | 231.5 | 104.0 | 1:22:28 | 7:32:22 | 2:31:40 | 3:35:25 | 5:19:25 | 6:23:10 | |
| 11678 | 157 | 31 | 2847 Jan 22 | 12:39:37 | Total | 0.0084 | 1.8011 | 368.8 | 231.1 | 103.9 | 9:35:13 | 15:44:01 | 10:44:04 | 11:47:40 | 13:31:34 | 14:35:10 | |
| 11724 | 157 | 32 | 2865 Feb 01 | 20:51:00 | Total | 0.0170 | 1.7868 | 367.7 | 230.6 | 103.7 | 17:47:09 | 23:54:51 | 18:55:42 | 19:59:09 | 21:42:51 | 22:46:18 | |
| 11770 | 157 | 33 | 2883 Feb 13 | 5:01:07 | Total | 0.0274 | 1.7695 | 366.4 | 230.2 | 103.5 | 1:57:55 | 8:04:19 | 3:06:01 | 4:09:22 | 5:52:52 | 6:56:13 | |
| 11816 | 157 | 34 | 2901 Feb 24 | 13:07:56 | Total | 0.0412 | 1.7463 | 365.0 | 229.6 | 103.2 | 10:05:26 | 16:10:26 | 11:13:08 | 12:16:20 | 13:59:32 | 15:02:44 | |
| 11861 | 157 | 35 | 2919 Mar 07 | 21:11:15 | Total | 0.0585 | 1.7170 | 363.4 | 229.0 | 102.8 | 18:09:33 | 0:12:57 | 19:16:45 | 20:19:51 | 22:02:39 | 23:05:45 | |
| 11906 | 157 | 36 | 2937 Mar 18 | 5:07:34 | Total | 0.0821 | 1.6762 | 361.6 | 228.2 | 101.9 | 2:06:46 | 8:08:22 | 3:13:28 | 4:16:37 | 5:58:31 | 7:01:40 | |
| 11951 | 157 | 37 | 2955 Mar 29 | 12:58:25 | Total | 0.1108 | 1.6265 | 359.6 | 227.1 | 100.5 | 9:58:37 | 15:58:13 | 11:04:52 | 12:08:10 | 13:48:40 | 14:51:58 | |
| 11997 | 157 | 38 | 2973 Apr 08 | 20:41:47 | Total | 0.1463 | 1.5642 | 357.3 | 225.6 | 98.1 | 17:43:08 | 23:40:26 | 18:48:59 | 19:52:44 | 21:30:50 | 22:34:35 | |
| 12041 | 157 | 39 | 2991 Apr 20 | 4:19:45 | Total | 0.1872 | 1.4921 | 354.6 | 223.6 | 94.5 | 1:22:27 | 7:17:03 | 2:27:57 | 3:32:30 | 5:07:00 | 6:11:33 | |
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 penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Saturday, May 25, 2013, with an umbral magnitude of −0.9322. 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 only about 18 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 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 Tuesday, 6 July 1982, the second of three total lunar eclipses in 1982, and the only one that was in the descending node. A dramatic total eclipse lasting 1 hour and 46 minutes plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours and 56 minutes in total.
A total lunar eclipse took place on Friday, August 6, 1971, the second of two total lunar eclipses in 1971. A dramatic total eclipse lasting 1 hour, 39 minutes and 24.8 seconds plunged the full Moon into deep darkness, as it passed right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may have been stained a deep orange or red colour at maximum eclipse. This was a great spectacle for everyone who saw it. The partial eclipse lasted for 3 hours, 35 minutes and 31.9 seconds in total. Occurring only 2.2 days before perigee, the Moon's apparent diameter was 3.6% larger than average and the moon passed through the center of the Earth's shadow.
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 took place on Saturday, September 16, 1978, the second of two total lunar eclipses in 1978. The Moon was plunged into darkness for 1 hour, 18 minutes and 39 seconds, in a deep total eclipse which saw the Moon 32.683% 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 3 hours, 27 minutes and 11.6 seconds in total.
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 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 partial solar eclipse will occur at the Moon's ascending node of orbit between Thursday, June 20 and Friday, June 21, 2058, with a magnitude of 0.126. 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 136 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 72 events. Solar saros 143 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
Saros cycle series 150 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 71 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.
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.
