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2015 Sep 28 |
Saros cycle series 137 for lunar eclipses occurs at the moon's descending node, repeats every 18 years 11 and 1/3 days. It contains 78 events. [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 | ||||||||
08582 | 137 | 1 | 1564 Dec 17 | 21:16:37 | Penumbral | -1.5587 | -1.0109 | 23.0 | 21:05:07 | 21:28:07 | |||||||
08625 | 137 | 2 | 1583 Jan 08 | 5:55:04 | Penumbral | -1.5513 | -0.9958 | 38.4 | 5:35:52 | 6:14:16 | |||||||
08668 | 137 | 3 | 1601 Jan 18 | 14:32:25 | Penumbral | -1.5425 | -0.9777 | 50.9 | 14:06:58 | 14:57:52 | |||||||
08713 | 137 | 4 | 1619 Jan 29 | 23:07:09 | Penumbral | -1.5311 | -0.9547 | 63.5 | 22:35:24 | 23:38:54 | |||||||
08757 | 137 | 5 | 1637 Feb 09 | 7:38:45 | Penumbral | -1.5164 | -0.9256 | 76.7 | 7:00:24 | 8:17:06 | |||||||
08801 | 137 | 6 | 1655 Feb 20 | 16:03:56 | Penumbral | -1.4962 | -0.8860 | 91.8 | 15:18:02 | 16:49:50 | |||||||
08846 | 137 | 7 | 1673 Mar 03 | 0:24:02 | Penumbral | -1.4715 | -0.8381 | 107.2 | 23:30:26 | 1:17:38 | |||||||
08892 | 137 | 8 | 1691 Mar 14 | 8:36:44 | Penumbral | -1.4403 | -0.7780 | 123.8 | 7:34:50 | 9:38:38 | |||||||
08938 | 137 | 9 | 1709 Mar 25 | 16:43:34 | Penumbral | -1.4038 | -0.7084 | 140.3 | 15:33:25 | 17:53:43 | |||||||
08985 | 137 | 10 | 1727 Apr 06 | 0:41:54 | Penumbral | -1.3596 | -0.6247 | 157.4 | 23:23:12 | 2:00:36 | |||||||
09031 | 137 | 11 | 1745 Apr 16 | 8:34:55 | Penumbral | -1.3106 | -0.5321 | 173.9 | 7:07:58 | 10:01:52 | |||||||
09078 | 137 | 12 | 1763 Apr 27 | 16:20:38 | Penumbral | -1.2552 | -0.4281 | 190.1 | 14:45:35 | 17:55:41 | |||||||
09124 | 137 | 13 | 1781 May 8 | 0:01:08 | Penumbral | -1.1949 | -0.3152 | 205.6 | 22:18:20 | 1:43:56 | |||||||
09169 | 137 | 14 | 1799 May 19 | 7:36:00 | Penumbral | -1.1294 | -0.1930 | 220.3 | 5:45:51 | 9:26:09 | |||||||
09214 | 137 | 15 | 1817 May 30 | 15:07:30 | Penumbral | -1.0607 | -0.0652 | 233.9 | 13:10:33 | 17:04:27 | |||||||
09260 | 137 | 16 | 1835 Jun 10 | 22:35:53 | Partial | -0.9888 | 0.0681 | 246.4 | 56.8 | 20:32:41 | 0:39:05 | 22:07:29 | 23:04:17 | ||||
09306 | 137 | 17 | 1853 Jun 21 | 6:01:48 | Partial | -0.9146 | 0.2056 | 257.8 | 96.7 | 3:52:54 | 8:10:42 | 5:13:27 | 6:50:09 | ||||
09350 | 137 | 18 | 1871 Jul 02 | 13:27:48 | Partial | -0.8401 | 0.3432 | 267.9 | 122.4 | 11:13:51 | 15:41:45 | 12:26:36 | 14:29:00 | ||||
09393 | 137 | 19 | 1889 Jul 12 | 20:53:52 | Partial | -0.7654 | 0.4807 | 276.8 | 141.7 | 18:35:28 | 23:12:16 | 19:43:01 | 22:04:43 | ||||
09436 | 137 | 20 | 1907 Jul 25 | 4:22:27 | Partial | -0.6924 | 0.6149 | 284.5 | 156.8 | 2:00:12 | 6:44:42 | 3:04:03 | 5:40:51 | ||||
09478 | 137 | 21 | 1925 Aug 04 | 11:52:57 | Partial | -0.6208 | 0.7463 | 291.2 | 168.9 | 9:27:21 | 14:18:33 | 10:28:30 | 13:17:24 | ||||
09520 | 137 | 22 | 1943 Aug 15 | 19:28:46 | Partial | -0.5533 | 0.8697 | 296.7 | 178.4 | 17:00:25 | 21:57:07 | 17:59:34 | 20:57:58 | ||||
09561 | 137 | 23 | 1961 Aug 26 | 3:08:51 | Partial | -0.4894 | 0.9863 | 301.4 | 186.0 | 0:38:09 | 5:39:33 | 1:35:51 | 4:41:51 | ||||
09602 | 137 | 24 | 1979 Sep 06 | 10:55:02 | Total | -0.4305 | 1.0936 | 305.1 | 191.9 | 44.4 | 8:22:29 | 13:27:35 | 9:19:05 | 10:32:50 | 11:17:14 | 12:30:59 | |
09643 | 137 | 25 | 1997 Sep 16 | 18:47:42 | Total | -0.3768 | 1.1909 | 308.2 | 196.4 | 61.5 | 16:13:36 | 21:21:48 | 17:09:30 | 18:16:57 | 19:18:27 | 20:25:54 | |
09685 | 137 | 26 | 2015 Sep 28 | 2:48:17 | Total | -0.3296 | 1.2764 | 310.7 | 199.9 | 71.9 | 0:12:56 | 5:23:38 | 1:08:20 | 2:12:20 | 3:24:14 | 4:28:14 | |
09726 | 137 | 27 | 2033 Oct 08 | 10:56:23 | Total | -0.2889 | 1.3497 | 312.6 | 202.4 | 78.8 | 8:20:05 | 13:32:41 | 9:15:11 | 10:16:59 | 11:35:47 | 12:37:35 | |
09766 | 137 | 28 | 2051 Oct 19 | 19:11:50 | Total | -0.2542 | 1.4118 | 314.2 | 204.3 | 83.6 | 16:34:44 | 21:48:56 | 17:29:41 | 18:30:02 | 19:53:38 | 20:53:59 | |
09807 | 137 | 29 | 2069 Oct 30 | 3:35:06 | Total | -0.2263 | 1.4616 | 315.4 | 205.6 | 86.8 | 0:57:24 | 6:12:48 | 1:52:18 | 2:51:42 | 4:18:30 | 5:17:54 | |
09848 | 137 | 30 | 2087 Nov 10 | 12:05:33 | Total | -0.2043 | 1.5006 | 316.4 | 206.6 | 88.9 | 9:27:21 | 14:43:45 | 10:22:15 | 11:21:06 | 12:50:00 | 13:48:51 | |
09890 | 137 | 31 | 2105 Nov 21 | 20:42:00 | Total | -0.1874 | 1.5301 | 317.3 | 207.3 | 90.4 | 18:03:21 | 23:20:39 | 18:58:21 | 19:56:48 | 21:27:12 | 22:25:39 | |
09932 | 137 | 32 | 2123 Dec 03 | 5:24:09 | Total | -0.1755 | 1.5507 | 318.0 | 207.7 | 91.4 | 2:45:09 | 8:03:09 | 3:40:18 | 4:38:27 | 6:09:51 | 7:08:00 | |
09975 | 137 | 33 | 2141 Dec 13 | 14:10:16 | Total | -0.1671 | 1.5652 | 318.7 | 208.1 | 92.0 | 11:30:55 | 16:49:37 | 12:26:13 | 13:24:16 | 14:56:16 | 15:54:19 | |
10019 | 137 | 34 | 2159 Dec 24 | 23:00:09 | Total | -0.1619 | 1.5737 | 319.2 | 208.4 | 92.4 | 20:20:33 | 1:39:45 | 21:15:57 | 22:13:57 | 23:46:21 | 0:44:21 | |
10062 | 137 | 35 | 2178 Jan 04 | 7:50:14 | Total | -0.1570 | 1.5820 | 319.8 | 208.8 | 92.8 | 5:10:20 | 10:30:08 | 6:05:50 | 7:03:50 | 8:36:38 | 9:34:38 | |
10105 | 137 | 36 | 2196 Jan 15 | 16:41:55 | Total | -0.1537 | 1.5877 | 320.3 | 209.1 | 93.1 | 14:01:46 | 19:22:04 | 14:57:22 | 15:55:22 | 17:28:28 | 18:26:28 | |
10149 | 137 | 37 | 2214 Jan 27 | 1:30:46 | Total | -0.1480 | 1.5979 | 320.9 | 209.5 | 93.6 | 22:50:19 | 4:11:13 | 23:46:01 | 0:43:58 | 2:17:34 | 3:15:31 | |
10193 | 137 | 38 | 2232 Feb 07 | 10:17:44 | Total | -0.1410 | 1.6106 | 321.5 | 210.0 | 94.1 | 7:36:59 | 12:58:29 | 8:32:44 | 9:30:41 | 11:04:47 | 12:02:44 | |
10239 | 137 | 39 | 2250 Feb 17 | 18:58:32 | Total | -0.1291 | 1.6326 | 322.2 | 210.7 | 95.0 | 16:17:26 | 21:39:38 | 17:13:11 | 18:11:02 | 19:46:02 | 20:43:53 | |
10285 | 137 | 40 | 2268 Feb 29 | 3:35:27 | Total | -0.1142 | 1.6602 | 322.9 | 211.4 | 96.0 | 0:54:00 | 6:16:54 | 1:49:45 | 2:47:27 | 4:23:27 | 5:21:09 | |
10331 | 137 | 41 | 2286 Mar 11 | 12:04:37 | Total | -0.0929 | 1.6996 | 323.7 | 212.3 | 97.2 | 9:22:46 | 14:46:28 | 10:18:28 | 11:16:01 | 12:53:13 | 13:50:46 | |
10377 | 137 | 42 | 2304 Mar 22 | 20:26:42 | Total | -0.0661 | 1.7491 | 324.6 | 213.1 | 98.4 | 17:44:24 | 23:09:00 | 18:40:09 | 19:37:30 | 21:15:54 | 22:13:15 | |
10423 | 137 | 43 | 2322 Apr 03 | 4:39:45 | Total | -0.0323 | 1.8116 | 325.4 | 213.9 | 99.4 | 1:57:03 | 7:22:27 | 2:52:48 | 3:50:03 | 5:29:27 | 6:26:42 | |
10469 | 137 | 44 | 2340 Apr 13 | 12:45:17 | Total | 0.0074 | 1.8576 | 326.1 | 214.5 | 99.9 | 10:02:14 | 15:28:20 | 10:58:02 | 11:55:20 | 13:35:14 | 14:32:32 | |
10514 | 137 | 45 | 2358 Apr 24 | 20:41:46 | Total | 0.0542 | 1.7720 | 326.7 | 214.8 | 99.5 | 17:58:25 | 23:25:07 | 18:54:22 | 19:52:01 | 21:31:31 | 22:29:10 | |
10559 | 137 | 46 | 2376 May 5 | 4:29:55 | Total | 0.1074 | 1.6744 | 326.9 | 214.4 | 97.8 | 1:46:28 | 7:13:22 | 2:42:43 | 3:41:01 | 5:18:49 | 6:17:07 | |
10603 | 137 | 47 | 2394 May 16 | 12:10:00 | Total | 0.1667 | 1.5656 | 326.6 | 213.3 | 94.3 | 9:26:42 | 14:53:18 | 10:23:21 | 11:22:51 | 12:57:09 | 13:56:39 | |
10649 | 137 | 48 | 2412 May 26 | 19:43:25 | Total | 0.2306 | 1.4479 | 325.8 | 211.1 | 88.2 | 17:00:31 | 22:26:19 | 17:57:52 | 18:59:19 | 20:27:31 | 21:28:58 | |
10693 | 137 | 49 | 2430 Jun 07 | 3:09:30 | Total | 0.3000 | 1.3201 | 324.3 | 207.7 | 78.4 | 0:27:21 | 5:51:39 | 1:25:39 | 2:30:18 | 3:48:42 | 4:53:21 | |
10737 | 137 | 50 | 2448 Jun 17 | 10:30:31 | Total | 0.3730 | 1.1854 | 322.0 | 202.8 | 62.6 | 7:49:31 | 13:11:31 | 8:49:07 | 9:59:13 | 11:01:49 | 12:11:55 | |
10780 | 137 | 51 | 2466 Jun 28 | 17:46:38 | Total | 0.4490 | 1.0448 | 318.7 | 196.2 | 32.2 | 15:07:17 | 20:25:59 | 16:08:32 | 17:30:32 | 18:02:44 | 19:24:44 | |
10822 | 137 | 52 | 2484 Jul 09 | 1:00:42 | Partial | 0.5260 | 0.9021 | 314.5 | 187.6 | 22:23:27 | 3:37:57 | 23:26:54 | 2:34:30 | ||||
10863 | 137 | 53 | 2502 Jul 21 | 8:11:07 | Partial | 0.6051 | 0.7554 | 309.2 | 176.6 | 5:36:31 | 10:45:43 | 6:42:49 | 9:39:25 | ||||
10904 | 137 | 54 | 2520 Jul 31 | 15:22:37 | Partial | 0.6822 | 0.6120 | 303.0 | 163.3 | 12:51:07 | 17:54:07 | 14:00:58 | 16:44:16 | ||||
10944 | 137 | 55 | 2538 Aug 11 | 22:33:32 | Partial | 0.7588 | 0.4693 | 295.7 | 146.7 | 20:05:41 | 1:01:23 | 21:20:11 | 23:46:53 | ||||
10986 | 137 | 56 | 2556 Aug 22 | 5:48:05 | Partial | 0.8315 | 0.3334 | 287.8 | 126.6 | 3:24:11 | 8:11:59 | 4:44:47 | 6:51:23 | ||||
11027 | 137 | 57 | 2574 Sep 02 | 13:03:42 | Partial | 0.9023 | 0.2008 | 278.9 | 100.5 | 10:44:15 | 15:23:09 | 12:13:27 | 13:53:57 | ||||
11067 | 137 | 58 | 2592 Sep 12 | 20:25:19 | Partial | 0.9671 | 0.0791 | 269.7 | 64.3 | 18:10:28 | 22:40:10 | 19:53:10 | 20:57:28 | ||||
11107 | 137 | 59 | 2610 Sep 25 | 3:50:47 | Penumbral | 1.0277 | -0.0350 | 260.2 | 1:40:41 | 6:00:53 | |||||||
11147 | 137 | 60 | 2628 Oct 05 | 11:22:30 | Penumbral | 1.0821 | -0.1379 | 250.7 | 9:17:09 | 13:27:51 | |||||||
11188 | 137 | 61 | 2646 Oct 16 | 19:00:12 | Penumbral | 1.1308 | -0.2304 | 241.4 | 16:59:30 | 21:00:54 | |||||||
11230 | 137 | 62 | 2664 Oct 27 | 2:45:20 | Penumbral | 1.1726 | -0.3102 | 232.7 | 0:48:59 | 4:41:41 | |||||||
11273 | 137 | 63 | 2682 Nov 07 | 10:37:27 | Penumbral | 1.2077 | -0.3776 | 225.0 | 8:44:57 | 12:29:57 | |||||||
11315 | 137 | 64 | 2700 Nov 18 | 18:35:06 | Penumbral | 1.2375 | -0.4352 | 218.0 | 16:46:06 | 20:24:06 | |||||||
11358 | 137 | 65 | 2718 Nov 30 | 2:39:40 | Penumbral | 1.2608 | -0.4808 | 212.5 | 0:53:25 | 4:25:55 | |||||||
11400 | 137 | 66 | 2736 Dec 10 | 10:49:08 | Penumbral | 1.2799 | -0.5183 | 207.8 | 9:05:14 | 12:33:02 | |||||||
11443 | 137 | 67 | 2754 Dec 21 | 19:03:15 | Penumbral | 1.2944 | -0.5472 | 204.3 | 17:21:06 | 20:45:24 | |||||||
11487 | 137 | 68 | 2773 Jan 01 | 3:19:29 | Penumbral | 1.3067 | -0.5717 | 201.3 | 1:38:50 | 5:00:08 | |||||||
11532 | 137 | 69 | 2791 Jan 12 | 11:38:09 | Penumbral | 1.3165 | -0.5914 | 198.9 | 9:58:42 | 13:17:36 | |||||||
11578 | 137 | 70 | 2809 Jan 22 | 19:56:13 | Penumbral | 1.3263 | -0.6107 | 196.3 | 18:18:04 | 21:34:22 | |||||||
11625 | 137 | 71 | 2827 Feb 03 | 4:12:29 | Penumbral | 1.3371 | -0.6314 | 193.2 | 2:35:53 | 5:49:05 | |||||||
11672 | 137 | 72 | 2845 Feb 13 | 12:25:13 | Penumbral | 1.3502 | -0.6561 | 188.9 | 10:50:46 | 13:59:40 | |||||||
11718 | 137 | 73 | 2863 Feb 24 | 20:33:14 | Penumbral | 1.3665 | -0.6864 | 183.1 | 19:01:41 | 22:04:47 | |||||||
11764 | 137 | 74 | 2881 Mar 07 | 4:34:07 | Penumbral | 1.3878 | -0.7256 | 174.7 | 3:06:46 | 6:01:28 | |||||||
11810 | 137 | 75 | 2899 Mar 18 | 12:27:24 | Penumbral | 1.4146 | -0.7748 | 163.0 | 11:05:54 | 13:48:54 | |||||||
11855 | 137 | 76 | 2917 Mar 29 | 20:11:52 | Penumbral | 1.4477 | -0.8350 | 146.6 | 18:58:34 | 21:25:10 | |||||||
11900 | 137 | 77 | 2935 Apr 10 | 3:47:50 | Penumbral | 1.4869 | -0.9066 | 123.4 | 2:46:08 | 4:49:32 | |||||||
11945 | 137 | 78 | 2953 Apr 20 | 11:12:26 | Penumbral | 1.5341 | -0.9928 | 86.0 | 10:29:26 | 11:55:26 |
A total lunar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, June 15, 2011, with an umbral magnitude of 1.7014. 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 4.1 days after perigee, the Moon's apparent diameter was larger.
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 ascending node of orbit on Tuesday, June 26, 2029, with an umbral magnitude of 1.8452. 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 3.7 days before perigee, the Moon's apparent diameter will be larger.
A total lunar eclipse took place on Friday, June 4, 1993, the first of two total lunar eclipses in 1993, the second being on Monday, November 29. The Moon was plunged into darkness for 1 hour and 36 minutes, in a deep total eclipse which saw the Moon 56% 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 and 38 minutes in total. The moon passed through the center of the Earth's shadow.
A total lunar eclipse will occur at the Moon’s ascending node of orbit on Sunday, July 7, 2047, with an umbral magnitude of 1.7529. 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 3.4 days after perigee, the Moon's apparent diameter will be larger.
A total lunar eclipse took place on Saturday, May 24 and Sunday, May 25, 1975, the first of two total lunar eclipses in 1975. The Moon was plunged into darkness for 1 hour and 28 minutes in a deep total eclipse which saw the Moon 43% of its diameter inside the Earth's umbral shadow. The visual effect of an eclipse 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 and 35 minutes in total. Occurring only 4.4 days after perigee, the Moon's apparent diameter was 0.7% larger than average. The moon was 377,010 km from 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, 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 total lunar eclipse occurred at the Moon’s ascending node of orbit on Monday, May 13, 1957, with an umbral magnitude of 1.2982. 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 3.25 days after perigee, the Moon's apparent diameter was larger.
A total lunar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, May 3, 1939, with an umbral magnitude of 1.1765. 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 5.2 days after perigee, the Moon's apparent diameter was larger.
A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Sunday, April 12, 1903, with an umbral magnitude of 0.9677. 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. The Moon's apparent diameter was near the average diameter because it occurred 6.2 days after perigee and 7.1 days before apogee.
A total lunar eclipse will occur at the Moon’s ascending node of orbit on Thursday, July 29, 2083, with an umbral magnitude of 1.4791. 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 2.9 days after perigee, the Moon's apparent diameter will be larger.
A total lunar eclipse will occur at the Moon’s ascending node of orbit on Friday, July 17, 2065, 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 4.2 days after perigee, the Moon's apparent diameter will be 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 137 for solar eclipses occurs at the Moon's ascending node. It repeats every 18 years, 11 days, and contains 70 eclipses, 55 of which are umbral eclipses. The first eclipse in the series was on 25 May 1389 and the last will be on 28 June 2633. The most recent eclipse was an annular eclipse on 21 June 2020 and the next will be an annular eclipse on 2 July 2038. The longest duration of totality was 2 minutes, 55 seconds on September 10, 1569 and the longest annular eclipse will be 7 minutes 5 seconds on 28 February 2435. This series has an unusual order of umbral eclipses, with 10 total eclipses followed by 6 hybrid eclipses, 4 annular eclipses, 3 more hybrid eclipses, and then finally 32 annular eclipses.
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.