Saros cycle series 142 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 73 events (72 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 | ||||||||
08940 | 142 | 1 | 1709 Sep 19 | 0:30:48 | Penumbral | 1.5439 | -1.0136 | 78.2 | 23:51:42 | 1:09:54 | |||||||
08987 | 142 | 2 | 1727 Sep 30 | 7:40:13 | Penumbral | 1.4949 | -0.9259 | 121.5 | 6:39:28 | 8:40:58 | |||||||
09033 | 142 | 3 | 1745 Oct 10 | 14:56:57 | Penumbral | 1.4515 | -0.8485 | 149.2 | 13:42:21 | 16:11:33 | |||||||
09080 | 142 | 4 | 1763 Oct 21 | 22:22:45 | Penumbral | 1.4153 | -0.7842 | 168.6 | 20:58:27 | 23:47:03 | |||||||
09125 | 142 | 5 | 1781 Nov 01 | 5:56:11 | Penumbral | 1.3850 | -0.7308 | 183.0 | 4:24:41 | 7:27:41 | |||||||
09170 | 142 | 6 | 1799 Nov 12 | 13:38:20 | Penumbral | 1.3618 | -0.6897 | 193.4 | 12:01:38 | 15:15:02 | |||||||
09215 | 142 | 7 | 1817 Nov 23 | 21:26:57 | Penumbral | 1.3435 | -0.6577 | 201.1 | 19:46:24 | 23:07:30 | |||||||
09261 | 142 | 8 | 1835 Dec 05 | 5:20:19 | Penumbral | 1.3290 | -0.6322 | 206.9 | 3:36:52 | 7:03:46 | |||||||
09307 | 142 | 9 | 1853 Dec 15 | 13:18:43 | Penumbral | 1.3186 | -0.6138 | 211.0 | 11:33:13 | 15:04:13 | |||||||
09351 | 142 | 10 | 1871 Dec 26 | 21:19:33 | Penumbral | 1.3105 | -0.5995 | 213.9 | 19:32:36 | 23:06:30 | |||||||
09394 | 142 | 11 | 1890 Jan 06 | 5:21:26 | Penumbral | 1.3029 | -0.5854 | 216.6 | 3:33:08 | 7:09:44 | |||||||
09437 | 142 | 12 | 1908 Jan 18 | 13:21:36 | Penumbral | 1.2939 | -0.5685 | 219.5 | 11:31:51 | 15:11:21 | |||||||
09479 | 142 | 13 | 1926 Jan 28 | 21:20:24 | Penumbral | 1.2836 | -0.5488 | 222.6 | 19:29:06 | 23:11:42 | |||||||
09521 | 142 | 14 | 1944 Feb 09 | 5:14:57 | Penumbral | 1.2698 | -0.5223 | 226.7 | 3:21:36 | 7:08:18 | |||||||
09562 | 142 | 15 | 1962 Feb 19 | 13:03:42 | Penumbral | 1.2511 | -0.4865 | 231.9 | 11:07:45 | 14:59:39 | |||||||
09603 | 142 | 16 | 1980 Mar 01 | 20:46:03 | Penumbral | 1.2269 | -0.4405 | 238.5 | 18:46:48 | 22:45:18 | |||||||
09644 | 142 | 17 | 1998 Mar 13 | 4:21:08 | Penumbral | 1.1964 | -0.3824 | 246.4 | 2:17:56 | 6:24:20 | |||||||
09686 | 142 | 18 | 2016 Mar 23 | 11:48:21 | Penumbral | 1.1591 | -0.3118 | 255.4 | 9:40:39 | 13:56:03 | |||||||
09727 | 142 | 19 | 2034 Apr 03 | 19:06:59 | Penumbral | 1.1144 | -0.2274 | 265.4 | 16:54:17 | 21:19:41 | |||||||
09767 | 142 | 20 | 2052 Apr 14 | 2:18:06 | Penumbral | 1.0628 | -0.1305 | 276.0 | 0:00:06 | 4:36:06 | |||||||
09808 | 142 | 21 | 2070 Apr 25 | 9:21:24 | Penumbral | 1.0044 | -0.0209 | 286.9 | 6:57:57 | 11:44:51 | |||||||
09849 | 142 | 22 | 2088 May 05 | 16:16:50 | Partial | 0.9387 | 0.1019 | 297.9 | 77.1 | 13:47:53 | 18:45:47 | 15:38:17 | 16:55:23 | ||||
09891 | 142 | 23 | 2106 May 17 | 23:06:43 | Partial | 0.8677 | 0.2345 | 308.4 | 114.5 | 20:32:31 | 1:40:55 | 22:09:28 | 0:03:58 | ||||
09933 | 142 | 24 | 2124 May 28 | 5:50:59 | Partial | 0.7913 | 0.3770 | 318.4 | 141.9 | 3:11:47 | 8:30:11 | 4:40:02 | 7:01:56 | ||||
09976 | 142 | 25 | 2142 Jun 08 | 12:32:42 | Partial | 0.7118 | 0.5247 | 327.2 | 163.2 | 9:49:06 | 15:16:18 | 11:11:06 | 13:54:18 | ||||
10020 | 142 | 26 | 2160 Jun 18 | 19:10:10 | Partial | 0.6280 | 0.6804 | 335.2 | 180.8 | 16:22:34 | 21:57:46 | 17:39:46 | 20:40:34 | ||||
10063 | 142 | 27 | 2178 Jun 30 | 1:48:39 | Partial | 0.5438 | 0.8364 | 341.8 | 194.6 | 22:57:45 | 4:39:33 | 0:11:21 | 3:25:57 | ||||
10106 | 142 | 28 | 2196 Jul 10 | 8:26:05 | Partial | 0.4577 | 0.9960 | 347.3 | 205.8 | 5:32:26 | 11:19:44 | 6:43:11 | 10:08:59 | ||||
10150 | 142 | 29 | 2214 Jul 22 | 15:06:54 | Total | 0.3734 | 1.1518 | 351.4 | 214.2 | 60.4 | 12:11:12 | 18:02:36 | 13:19:48 | 14:36:42 | 15:37:06 | 16:54:00 | |
10194 | 142 | 30 | 2232 Aug 01 | 21:49:49 | Total | 0.2898 | 1.3061 | 354.3 | 220.4 | 81.1 | 18:52:40 | 0:46:58 | 19:59:37 | 21:09:16 | 22:30:22 | 23:40:01 | |
10240 | 142 | 31 | 2250 Aug 13 | 4:39:38 | Total | 0.2108 | 1.4520 | 356.0 | 224.5 | 92.9 | 1:41:38 | 7:37:38 | 2:47:23 | 3:53:11 | 5:26:05 | 6:31:53 | |
10286 | 142 | 32 | 2268 Aug 23 | 11:34:51 | Total | 0.1351 | 1.5915 | 356.7 | 226.9 | 99.8 | 8:36:30 | 14:33:12 | 9:41:24 | 10:44:57 | 12:24:45 | 13:28:18 | |
10332 | 142 | 33 | 2286 Sep 03 | 18:37:54 | Total | 0.0648 | 1.7209 | 356.6 | 227.8 | 103.2 | 15:39:36 | 21:36:12 | 16:44:00 | 17:46:18 | 19:29:30 | 20:31:48 | |
10378 | 142 | 34 | 2304 Sep 15 | 1:48:59 | Total | 0.0003 | 1.8394 | 355.7 | 227.6 | 103.9 | 22:51:08 | 4:46:50 | 23:55:11 | 0:57:02 | 2:40:56 | 3:42:47 | |
10424 | 142 | 35 | 2322 Sep 26 | 9:09:54 | Total | -0.0568 | 1.7360 | 354.3 | 226.5 | 102.8 | 6:12:45 | 12:07:03 | 7:16:39 | 8:18:30 | 10:01:18 | 11:03:09 | |
10470 | 142 | 36 | 2340 Oct 06 | 16:39:55 | Total | -0.1074 | 1.6431 | 352.6 | 224.9 | 100.4 | 13:43:37 | 19:36:13 | 14:47:28 | 15:49:43 | 17:30:07 | 18:32:22 | |
10515 | 142 | 37 | 2358 Oct 18 | 0:19:34 | Total | -0.1509 | 1.5634 | 350.7 | 222.9 | 97.2 | 21:24:13 | 3:14:55 | 22:28:07 | 23:30:58 | 1:08:10 | 2:11:01 | |
10560 | 142 | 38 | 2376 Oct 28 | 8:09:00 | Total | -0.1871 | 1.4971 | 348.7 | 220.9 | 93.7 | 5:14:39 | 11:03:21 | 6:18:33 | 7:22:09 | 8:55:51 | 9:59:27 | |
10604 | 142 | 39 | 2394 Nov 08 | 16:08:09 | Total | -0.2159 | 1.4443 | 346.8 | 218.9 | 90.3 | 13:14:45 | 19:01:33 | 14:18:42 | 15:23:00 | 16:53:18 | 17:57:36 | |
10650 | 142 | 40 | 2412 Nov 19 | 0:15:25 | Total | -0.2386 | 1.4030 | 345.0 | 217.1 | 87.1 | 21:22:55 | 3:07:55 | 22:26:52 | 23:31:52 | 0:58:58 | 2:03:58 | |
10694 | 142 | 41 | 2430 Nov 30 | 8:31:15 | Total | -0.2548 | 1.3735 | 343.3 | 215.5 | 84.6 | 5:39:36 | 11:22:54 | 6:43:30 | 7:48:57 | 9:13:33 | 10:19:00 | |
10738 | 142 | 42 | 2448 Dec 10 | 16:53:19 | Total | -0.2667 | 1.3524 | 341.7 | 214.2 | 82.6 | 14:02:28 | 19:44:10 | 15:06:13 | 16:12:01 | 17:34:37 | 18:40:25 | |
10781 | 142 | 43 | 2466 Dec 22 | 1:21:41 | Total | -0.2740 | 1.3398 | 340.3 | 213.2 | 81.3 | 22:31:32 | 4:11:50 | 23:35:05 | 0:41:02 | 2:02:20 | 3:08:17 | |
10823 | 142 | 44 | 2485 Jan 01 | 9:52:20 | Total | -0.2800 | 1.3298 | 338.8 | 212.3 | 80.2 | 7:02:56 | 12:41:44 | 8:06:11 | 9:12:14 | 10:32:26 | 11:38:29 | |
10864 | 142 | 45 | 2503 Jan 13 | 18:27:08 | Total | -0.2833 | 1.3250 | 337.4 | 211.6 | 79.6 | 15:38:26 | 21:15:50 | 16:41:20 | 17:47:20 | 19:06:56 | 20:12:56 | |
10905 | 142 | 46 | 2521 Jan 24 | 3:01:30 | Total | -0.2872 | 1.3195 | 336.0 | 210.8 | 78.9 | 0:13:30 | 5:49:30 | 1:16:06 | 2:22:03 | 3:40:57 | 4:46:54 | |
10945 | 142 | 47 | 2539 Feb 04 | 11:35:58 | Total | -0.2921 | 1.3124 | 334.5 | 210.1 | 78.1 | 8:48:43 | 14:23:13 | 9:50:55 | 10:56:55 | 12:15:01 | 13:21:01 | |
10987 | 142 | 48 | 2557 Feb 14 | 20:06:30 | Total | -0.3008 | 1.2986 | 332.7 | 209.0 | 76.6 | 17:20:09 | 22:52:51 | 18:22:00 | 19:28:12 | 20:44:48 | 21:51:00 | |
11028 | 142 | 49 | 2575 Feb 26 | 4:34:54 | Total | -0.3120 | 1.2805 | 330.8 | 207.9 | 74.6 | 1:49:30 | 7:20:18 | 2:50:57 | 3:57:36 | 5:12:12 | 6:18:51 | |
11068 | 142 | 50 | 2593 Mar 08 | 12:57:32 | Total | -0.3284 | 1.2528 | 328.7 | 206.3 | 71.4 | 10:13:11 | 15:41:53 | 11:14:23 | 12:21:50 | 13:33:14 | 14:40:41 | |
11108 | 142 | 51 | 2611 Mar 20 | 21:14:33 | Total | -0.3502 | 1.2156 | 326.2 | 204.3 | 66.6 | 18:31:27 | 23:57:39 | 19:32:24 | 20:41:15 | 21:47:51 | 22:56:42 | |
11148 | 142 | 52 | 2629 Mar 31 | 5:24:37 | Total | -0.3783 | 1.1668 | 323.3 | 201.6 | 59.5 | 2:42:58 | 8:06:16 | 3:43:49 | 4:54:52 | 5:54:22 | 7:05:25 | |
11189 | 142 | 53 | 2647 Apr 11 | 13:28:29 | Total | -0.4123 | 1.1071 | 320.0 | 198.2 | 48.5 | 10:48:29 | 16:08:29 | 11:49:23 | 13:04:14 | 13:52:44 | 15:07:35 | |
11231 | 142 | 54 | 2665 Apr 21 | 21:25:02 | Total | -0.4528 | 1.0355 | 316.1 | 193.8 | 28.5 | 18:46:59 | 0:03:05 | 19:48:08 | 21:10:47 | 21:39:17 | 23:01:56 | |
11274 | 142 | 55 | 2683 May 3 | 5:14:46 | Partial | -0.4996 | 0.9523 | 311.5 | 188.3 | 2:39:01 | 7:50:31 | 3:40:37 | 6:48:55 | ||||
11316 | 142 | 56 | 2701 May 14 | 12:58:21 | Partial | -0.5522 | 0.8584 | 306.2 | 181.4 | 10:25:15 | 15:31:27 | 11:27:39 | 14:29:03 | ||||
11359 | 142 | 57 | 2719 May 25 | 20:36:44 | Partial | -0.6097 | 0.7552 | 300.1 | 172.7 | 18:06:41 | 23:06:47 | 19:10:23 | 22:03:05 | ||||
11401 | 142 | 58 | 2737 Jun 05 | 4:09:30 | Partial | -0.6726 | 0.6421 | 292.9 | 161.9 | 1:43:03 | 6:35:57 | 2:48:33 | 5:30:27 | ||||
11444 | 142 | 59 | 2755 Jun 16 | 11:39:21 | Partial | -0.7384 | 0.5233 | 284.8 | 148.6 | 9:16:57 | 14:01:45 | 10:25:03 | 12:53:39 | ||||
11488 | 142 | 60 | 2773 Jun 26 | 19:05:54 | Partial | -0.8076 | 0.3979 | 275.5 | 131.8 | 16:48:09 | 21:23:39 | 18:00:00 | 20:11:48 | ||||
11534 | 142 | 61 | 2791 Jul 08 | 2:32:22 | Partial | -0.8773 | 0.2713 | 265.2 | 110.6 | 0:19:46 | 4:44:58 | 1:37:04 | 3:27:40 | ||||
11580 | 142 | 62 | 2809 Jul 18 | 9:56:45 | Partial | -0.9494 | 0.1402 | 253.5 | 80.9 | 7:50:00 | 12:03:30 | 9:16:18 | 10:37:12 | ||||
11627 | 142 | 63 | 2827 Jul 29 | 17:23:45 | Partial | -1.0197 | 0.0119 | 240.7 | 23.9 | 15:23:24 | 19:24:06 | 17:11:48 | 17:35:42 | ||||
11674 | 142 | 64 | 2845 Aug 09 | 0:51:23 | Penumbral | -1.0901 | -0.1169 | 226.6 | 22:58:05 | 2:44:41 | |||||||
11720 | 142 | 65 | 2863 Aug 20 | 8:23:18 | Penumbral | -1.1571 | -0.2396 | 211.5 | 6:37:33 | 10:09:03 | |||||||
11766 | 142 | 66 | 2881 Aug 30 | 15:58:08 | Penumbral | -1.2220 | -0.3589 | 194.9 | 14:20:41 | 17:35:35 | |||||||
11812 | 142 | 67 | 2899 Sep 10 | 23:39:29 | Penumbral | -1.2819 | -0.4692 | 177.6 | 22:10:41 | 1:08:17 | |||||||
11857 | 142 | 68 | 2917 Sep 22 | 7:26:14 | Penumbral | -1.3377 | -0.5721 | 159.1 | 6:06:41 | 8:45:47 | |||||||
11902 | 142 | 69 | 2935 Oct 03 | 15:19:37 | Penumbral | -1.3883 | -0.6658 | 139.6 | 14:09:49 | 16:29:25 | |||||||
11947 | 142 | 70 | 2953 Oct 13 | 23:20:11 | Penumbral | -1.4331 | -0.7492 | 119.0 | 22:20:41 | 0:19:41 | |||||||
11993 | 142 | 71 | 2971 Oct 25 | 7:28:21 | Penumbral | -1.4719 | -0.8214 | 97.2 | 6:39:45 | 8:16:57 | |||||||
12037 | 142 | 72 | 2989 Nov 04 | 15:44:27 | Penumbral | -1.5048 | -0.8830 | 73.3 | 15:07:48 | 16:21:06 | |||||||
– | 142 | 73 | 3007 Nov 17 | 00:06:57 | Penumbral | -1.5328 | -0.9354 | 43.0 |
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.
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 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 at 0308 UT (GMT) on Thursday, August 17, 1989, the second of two total lunar eclipses in 1989.
A total lunar eclipse took place on Monday, November 29, 1993, the second of two total lunar eclipses in 1993, the first was on Friday, June 4.
A penumbral lunar eclipse took place on Friday, March 13, 1998, the first of three lunar eclipses in 1998.
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 Saturday, March 1, 1980, the first of three penumbral lunar eclipses in 1980. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 65.455% of the Moon's disc was partially shaded by the Earth, which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours, 58 minutes and 33.3 seconds.
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 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 total lunar eclipse took place on Tuesday, November 18, 1975, the second of two total lunar eclipses in 1975. A shallow total eclipse saw the Moon in relative darkness for 40 minutes and 11.1 seconds. The Moon was 6.421% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours, 29 minutes and 2.1 seconds in total. Occurring only 4.9 days after apogee, the Moon's apparent diameter was 4% smaller than average.
A total lunar eclipse will occur at the Moon’s descending node of orbit on Saturday, January 22, 2084, with an umbral magnitude of 1.1531. 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 4 days after apogee, the Moon's apparent diameter will be smaller.
Saros cycle series 142 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 72 eclipses, 44 of which are umbral, of which all but one are total. The first eclipse in the series was on 17 April 1624 and the final eclipse will be on 5 June 2904.
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 135 for lunar eclipses occurs at the moon's descending node, repeats every 18 years 11 and 1/3 days. It contains 71 events.