Member 57 |
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June 26, 2010 |
Saros cycle series 120 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 83 events. [1]
This lunar saros is linked to Solar Saros 127.
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 | ||||||||
07219 | 120 | 1 | 1000 Oct 16 | 1:35:42 | Penumbral | 1.5463 | -0.9862 | 47.1 | 1:12:09 | 1:59:15 | |||||||
07263 | 120 | 2 | 1018 Oct 27 | 9:53:57 | Penumbral | 1.5341 | -0.9666 | 65.2 | 9:21:21 | 10:26:33 | |||||||
07307 | 120 | 3 | 1036 Nov 06 | 18:16:32 | Penumbral | 1.5260 | -0.9544 | 75.4 | 17:38:50 | 18:54:14 | |||||||
07352 | 120 | 4 | 1054 Nov 18 | 2:44:30 | Penumbral | 1.5231 | -0.9513 | 79.7 | 2:04:39 | 3:24:21 | |||||||
07396 | 120 | 5 | 1072 Nov 28 | 11:14:15 | Penumbral | 1.5223 | -0.9518 | 81.8 | 10:33:21 | 11:55:09 | |||||||
07441 | 120 | 6 | 1090 Dec 09 | 19:45:28 | Penumbral | 1.5233 | -0.9555 | 82.0 | 19:04:28 | 20:26:28 | |||||||
07487 | 120 | 7 | 1108 Dec 20 | 4:16:00 | Penumbral | 1.5246 | -0.9593 | 81.9 | 3:35:03 | 4:56:57 | |||||||
07533 | 120 | 8 | 1126 Dec 31 | 12:45:19 | Penumbral | 1.5261 | -0.9632 | 81.3 | 12:04:40 | 13:25:58 | |||||||
07579 | 120 | 9 | 1145 Jan 10 | 21:09:35 | Penumbral | 1.5241 | -0.9604 | 83.9 | 20:27:38 | 21:51:32 | |||||||
07626 | 120 | 10 | 1163 Jan 22 | 5:29:14 | Penumbral | 1.5192 | -0.952 | 88.8 | 4:44:50 | 6:13:38 | |||||||
07673 | 120 | 11 | 1181 Feb 1 | 13:41:16 | Penumbral | 1.5091 | -0.9337 | 97.6 | 12:52:28 | 14:30:04 | |||||||
07719 | 120 | 12 | 1199 Feb 12 | 21:46:45 | Penumbral | 1.4944 | -0.907 | 108.9 | 20:52:18 | 22:41:12 | |||||||
07765 | 120 | 13 | 1217 Feb 23 | 5:41:09 | Penumbral | 1.4720 | -0.8659 | 123.9 | 4:39:12 | 6:43:06 | |||||||
07811 | 120 | 14 | 1235 Mar 06 | 13:27:40 | Penumbral | 1.4439 | -0.8143 | 140.3 | 12:17:31 | 14:37:49 | |||||||
07856 | 120 | 15 | 1253 Mar 16 | 21:02:30 | Penumbral | 1.4071 | -0.7467 | 158.9 | 19:43:03 | 22:21:57 | |||||||
07900 | 120 | 16 | 1271 Mar 28 | 4:28:45 | Penumbral | 1.3642 | -0.6679 | 177.8 | 2:59:51 | 5:57:39 | |||||||
07945 | 120 | 17 | 1289 Apr 07 | 11:43:12 | Penumbral | 1.3125 | -0.5732 | 197.6 | 10:04:24 | 13:22:00 | |||||||
07990 | 120 | 18 | 1307 Apr 18 | 18:50:03 | Penumbral | 1.2553 | -0.4683 | 216.9 | 17:01:36 | 20:38:30 | |||||||
08033 | 120 | 19 | 1325 Apr 29 | 1:47:03 | Penumbral | 1.1908 | -0.3501 | 236.1 | 23:49:00 | 3:45:06 | |||||||
08075 | 120 | 20 | 1343 May 10 | 8:36:45 | Penumbral | 1.1208 | -0.2221 | 254.5 | 6:29:30 | 10:44:00 | |||||||
08117 | 120 | 21 | 1361 May 20 | 15:19:11 | Penumbral | 1.0453 | -0.0841 | 272.0 | 13:03:11 | 17:35:11 | |||||||
08158 | 120 | 22 | 1379 May 31 | 21:57:14 | Partial | 0.9665 | 0.0597 | 288.2 | 58.8 | 19:33:08 | 0:21:20 | 21:27:50 | 22:26:38 | ||||
08199 | 120 | 23 | 1397 Jun 11 | 4:31:36 | Partial | 0.8850 | 0.2082 | 303.0 | 107.8 | 2:00:06 | 7:03:06 | 3:37:42 | 5:25:30 | ||||
08240 | 120 | 24 | 1415 Jun 22 | 11:03:06 | Partial | 0.8015 | 0.3602 | 316.4 | 139.0 | 8:24:54 | 13:41:18 | 9:53:36 | 12:12:36 | ||||
08282 | 120 | 25 | 1433 Jul 02 | 17:34:56 | Partial | 0.7183 | 0.5115 | 328.2 | 162.2 | 14:50:50 | 20:19:02 | 16:13:50 | 18:56:02 | ||||
08323 | 120 | 26 | 1451 Jul 14 | 0:07:29 | Partial | 0.6357 | 0.6615 | 338.5 | 180.3 | 21:18:14 | 2:56:44 | 22:37:20 | 1:37:38 | ||||
08364 | 120 | 27 | 1469 Jul 24 | 6:42:46 | Partial | 0.5556 | 0.8066 | 347.3 | 194.6 | 3:49:07 | 9:36:25 | 5:05:28 | 8:20:04 | ||||
08404 | 120 | 28 | 1487 Aug 04 | 13:21:13 | Partial | 0.4783 | 0.9466 | 354.6 | 205.8 | 10:23:55 | 16:18:31 | 11:38:19 | 15:04:07 | ||||
08444 | 120 | 29 | 1505 Aug 14 | 20:05:59 | Total | 0.4063 | 1.0766 | 360.6 | 214.4 | 44.7 | 17:05:41 | 23:06:17 | 18:18:47 | 19:43:38 | 20:28:20 | 21:53:11 | |
08485 | 120 | 30 | 1523 Aug 26 | 2:57:01 | Total | 0.3395 | 1.1971 | 365.5 | 221.0 | 68.9 | 23:54:16 | 5:59:46 | 1:06:31 | 2:22:34 | 3:31:28 | 4:47:31 | |
08526 | 120 | 31 | 1541 Sep 05 | 9:54:46 | Total | 0.2784 | 1.3072 | 369.3 | 225.8 | 82.7 | 6:50:07 | 12:59:25 | 8:01:52 | 9:13:25 | 10:36:07 | 11:47:40 | |
08569 | 120 | 32 | 1559 Sep 16 | 17:01:00 | Total | 0.2244 | 1.4041 | 372.2 | 229.3 | 91.3 | 13:54:54 | 20:07:06 | 15:06:21 | 16:15:21 | 17:46:39 | 18:55:39 | |
08612 | 120 | 33 | 1577 Sep 27 | 0:16:07 | Total | 0.1781 | 1.4869 | 374.4 | 231.6 | 96.7 | 21:08:55 | 3:23:19 | 22:20:19 | 23:27:46 | 1:04:28 | 2:11:55 | |
08655 | 120 | 34 | 1595 Oct 18 | 7:40:06 | Total | 0.1391 | 1.5567 | 376.0 | 233.1 | 100.2 | 4:32:06 | 10:48:06 | 5:43:33 | 6:50:00 | 8:30:12 | 9:36:39 | |
08699 | 120 | 35 | 1613 Oct 28 | 15:11:40 | Total | 0.1064 | 1.6149 | 377.2 | 234.1 | 102.3 | 12:03:04 | 18:20:16 | 13:14:37 | 14:20:31 | 16:02:49 | 17:08:43 | |
08743 | 120 | 36 | 1631 Nov 08 | 22:51:38 | Total | 0.0805 | 1.6608 | 378.1 | 234.7 | 103.5 | 19:42:35 | 2:00:41 | 20:54:17 | 21:59:53 | 23:43:23 | 0:48:59 | |
08787 | 120 | 37 | 1649 Nov 19 | 6:38:54 | Total | 0.0608 | 1.6957 | 378.6 | 234.9 | 104.1 | 3:29:36 | 9:48:12 | 4:41:27 | 5:46:51 | 7:30:57 | 8:36:21 | |
08832 | 120 | 38 | 1667 Nov 30 | 14:31:26 | Total | 0.0455 | 1.7228 | 379.0 | 235.1 | 104.5 | 11:21:56 | 17:40:56 | 12:33:53 | 13:39:11 | 15:23:41 | 16:28:59 | |
08878 | 120 | 39 | 1685 Dec 10 | 22:29:22 | Total | 0.0346 | 1.7422 | 379.1 | 235.1 | 104.7 | 19:19:49 | 1:38:55 | 20:31:49 | 21:37:01 | 23:21:43 | 0:26:55 | |
08924 | 120 | 40 | 1703 Dec 23 | 6:29:54 | Total | 0.0258 | 1.7582 | 379.1 | 235.1 | 104.7 | 3:20:21 | 9:39:27 | 4:32:21 | 5:37:33 | 7:22:15 | 8:27:27 | |
08971 | 120 | 41 | 1722 Jan 02 | 14:32:53 | Total | 0.0187 | 1.7714 | 378.9 | 235.0 | 104.8 | 11:23:26 | 17:42:20 | 12:35:23 | 13:40:29 | 15:25:17 | 16:30:23 | |
09018 | 120 | 42 | 1740 Jan 13 | 22:33:33 | Total | 0.0096 | 1.7887 | 378.5 | 235.0 | 104.9 | 19:24:18 | 1:42:48 | 20:36:03 | 21:41:06 | 23:26:00 | 0:31:03 | |
09065 | 120 | 43 | 1758 Jan 24 | 6:34:14 | Total | 0.0003 | 1.8067 | 378.0 | 234.9 | 104.9 | 3:25:14 | 9:43:14 | 4:36:47 | 5:41:47 | 7:26:41 | 8:31:41 | |
09111 | 120 | 44 | 1776 Feb 04 | 14:29:50 | Total | -0.0128 | 1.7851 | 377.4 | 234.7 | 104.9 | 11:21:08 | 17:38:32 | 12:32:29 | 13:37:23 | 15:22:17 | 16:27:11 | |
09156 | 120 | 45 | 1794 Feb 14 | 22:21:16 | Total | -0.0300 | 1.7553 | 376.5 | 234.5 | 104.8 | 19:13:01 | 1:29:31 | 20:24:01 | 21:28:52 | 23:13:40 | 0:18:31 | |
09201 | 120 | 46 | 1812 Feb 27 | 6:04:51 | Total | -0.0538 | 1.7135 | 375.5 | 234.1 | 104.3 | 2:57:06 | 9:12:36 | 4:07:48 | 5:12:42 | 6:57:00 | 8:01:54 | |
09246 | 120 | 47 | 1830 Mar 09 | 13:42:57 | Total | -0.0824 | 1.6632 | 374.2 | 233.4 | 103.3 | 10:35:51 | 16:50:03 | 11:46:15 | 12:51:18 | 14:34:36 | 15:39:39 | |
09293 | 120 | 48 | 1848 Mar 19 | 21:12:12 | Total | -0.1186 | 1.5993 | 372.5 | 232.4 | 101.4 | 18:05:57 | 0:18:27 | 19:16:00 | 20:21:30 | 22:02:54 | 23:08:24 | |
09337 | 120 | 49 | 1866 Mar 31 | 4:33:35 | Total | -0.1614 | 1.5232 | 370.4 | 230.7 | 98.2 | 1:28:23 | 7:38:47 | 2:38:14 | 3:44:29 | 5:22:41 | 6:28:56 | |
09380 | 120 | 50 | 1884 Apr 10 | 11:46:34 | Total | -0.2116 | 1.4337 | 367.7 | 228.2 | 92.9 | 8:42:43 | 14:50:25 | 9:52:28 | 11:00:07 | 12:33:01 | 13:40:40 | |
09424 | 120 | 51 | 1902 Apr 22 | 18:52:40 | Total | -0.2680 | 1.3327 | 364.3 | 224.6 | 84.6 | 15:50:31 | 21:54:49 | 17:00:22 | 18:10:22 | 19:34:58 | 20:44:58 | |
09466 | 120 | 52 | 1920 May 03 | 1:51:08 | Total | -0.3312 | 1.2194 | 360.1 | 219.7 | 71.5 | 22:51:05 | 4:51:11 | 0:01:17 | 1:15:23 | 2:26:53 | 3:40:59 | |
09508 | 120 | 53 | 1938 May 14 | 8:44:00 | Total | -0.3994 | 1.0966 | 354.9 | 213.1 | 49.4 | 5:46:33 | 11:41:27 | 6:57:27 | 8:19:18 | 9:08:42 | 10:30:33 | |
09549 | 120 | 54 | 1956 May 24 | 15:31:52 | Partial | -0.4726 | 0.9647 | 348.5 | 204.5 | 12:37:37 | 18:26:07 | 13:49:37 | 17:14:07 | ||||
09591 | 120 | 55 | 1974 Jun 04 | 22:16:44 | Partial | -0.5488 | 0.8269 | 341.0 | 193.6 | 19:26:14 | 1:07:14 | 20:39:56 | 23:53:32 | ||||
09632 | 120 | 56 | 1992 Jun 15 | 4:57:57 | Partial | -0.6288 | 0.6822 | 332.2 | 179.8 | 2:11:51 | 7:44:03 | 3:28:03 | 6:27:51 | ||||
09673 | 120 | 57 | 2010 Jun 26 | 11:39:34 | Partial | -0.7091 | 0.5368 | 322.1 | 162.9 | 8:58:31 | 14:20:37 | 10:18:07 | 13:01:01 | ||||
09714 | 120 | 58 | 2028 Jul 06 | 18:20:57 | Partial | -0.7903 | 0.3892 | 310.6 | 141.5 | 15:45:39 | 20:56:15 | 17:10:12 | 19:31:42 | ||||
09754 | 120 | 59 | 2046 Jul 18 | 1:06:05 | Partial | -0.8691 | 0.2461 | 298.1 | 114.6 | 22:37:02 | 3:35:08 | 0:08:47 | 2:03:23 | ||||
09795 | 120 | 60 | 2064 Jul 28 | 7:52:48 | Partial | -0.9473 | 0.1038 | 284.3 | 75.7 | 5:30:39 | 10:14:57 | 7:14:57 | 8:30:39 | ||||
09836 | 120 | 61 | 2082 Aug 08 | 14:46:42 | Penumbral | -1.0203 | -0.0294 | 269.8 | 12:31:48 | 17:01:36 | |||||||
09878 | 120 | 62 | 2100 Aug 19 | 21:44:58 | Penumbral | -1.0905 | -0.1575 | 254.2 | 19:37:52 | 23:52:04 | |||||||
09920 | 120 | 63 | 2118 Aug 31 | 4:51:45 | Penumbral | -1.1543 | -0.2740 | 238.5 | 2:52:30 | 6:51:00 | |||||||
09963 | 120 | 64 | 2136 Sep 10 | 12:05:06 | Penumbral | -1.2134 | -0.3821 | 222.2 | 10:14:00 | 13:56:12 | |||||||
10007 | 120 | 65 | 2154 Sep 21 | 19:29:06 | Penumbral | -1.2646 | -0.4759 | 206.5 | 17:45:51 | 21:12:21 | |||||||
10050 | 120 | 66 | 2172 Oct 02 | 3:01:41 | Penumbral | -1.3098 | -0.5586 | 191.3 | 1:26:02 | 4:37:20 | |||||||
10093 | 120 | 67 | 2190 Oct 13 | 10:43:55 | Penumbral | -1.3479 | -0.6285 | 176.9 | 9:15:28 | 12:12:22 | |||||||
10136 | 120 | 68 | 2208 Oct 24 | 18:36:02 | Penumbral | -1.3789 | -0.6853 | 164.2 | 17:13:56 | 19:58:08 | |||||||
10180 | 120 | 69 | 2226 Nov 05 | 2:38:01 | Penumbral | -1.4024 | -0.7283 | 153.5 | 1:21:16 | 3:54:46 | |||||||
10225 | 120 | 70 | 2244 Nov 15 | 10:48:54 | Penumbral | -1.4201 | -0.7605 | 144.8 | 9:36:30 | 12:01:18 | |||||||
10271 | 120 | 71 | 2262 Nov 26 | 19:06:54 | Penumbral | -1.4327 | -0.7833 | 138.1 | 17:57:51 | 20:15:57 | |||||||
10317 | 120 | 72 | 2280 Dec 07 | 3:32:38 | Penumbral | -1.4402 | -0.7964 | 133.7 | 2:25:47 | 4:39:29 | |||||||
10363 | 120 | 73 | 2298 Dec 18 | 12:03:40 | Penumbral | -1.4439 | -0.8025 | 131.1 | 10:58:07 | 13:09:13 | |||||||
10409 | 120 | 74 | 2316 Dec 29 | 20:38:45 | Penumbral | -1.4452 | -0.8039 | 129.7 | 19:33:54 | 21:43:36 | |||||||
10455 | 120 | 75 | 2335 Jan 10 | 5:16:00 | Penumbral | -1.4453 | -0.8029 | 128.9 | 4:11:33 | 6:20:27 | |||||||
10501 | 120 | 76 | 2353 Jan 20 | 13:54:28 | Penumbral | -1.4453 | -0.8012 | 128.0 | 12:50:28 | 14:58:28 | |||||||
10546 | 120 | 77 | 2371 Jan 31 | 22:31:48 | Penumbral | -1.4466 | -0.8019 | 126.3 | 21:28:39 | 23:34:57 | |||||||
10590 | 120 | 78 | 2389 Feb 11 | 7:06:06 | Penumbral | -1.4510 | -0.8078 | 122.9 | 6:04:39 | 8:07:33 | |||||||
10635 | 120 | 79 | 2407 Feb 22 | 15:37:08 | Penumbral | -1.4584 | -0.8192 | 117.6 | 14:38:20 | 16:35:56 | |||||||
10679 | 120 | 80 | 2425 Mar 05 | 0:03:15 | Penumbral | -1.4701 | -0.8383 | 109.5 | 23:08:30 | 0:58:00 | |||||||
10723 | 120 | 81 | 2443 Mar 16 | 8:22:54 | Penumbral | -1.4877 | -0.8680 | 96.7 | 7:34:33 | 9:11:15 | |||||||
10767 | 120 | 82 | 2461 Mar 26 | 16:36:11 | Penumbral | -1.5110 | -0.9080 | 77.1 | 15:57:38 | 17:14:44 | |||||||
10809 | 120 | 83 | 2479 Apr 07 | 0:42:37 | Penumbral | -1.5402 | -0.9591 | 41.1 | 0:22:04 | 1:03:10 |
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 penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Tuesday, March 14, 2006, with an umbral magnitude of −0.0584. It was a relatively rare total penumbral lunar eclipse, with the Moon passing entirely within the penumbral shadow without entering the darker umbral shadow. 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 2.2 days after apogee, the Moon's apparent diameter was smaller.
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 partial lunar eclipse took place on Monday, June 15, 1992, the first of two lunar eclipses in 1992, the second being with a total lunar eclipse on Wednesday, December 9.
A penumbral lunar eclipse took place on Thursday, March 3, 1988, the first of two lunar eclipses in 1988, the second being on August 27, 1988. Earlier sources compute this as a 0.3% partial eclipse lasting under 14 minutes, and newest calculations list it as a penumbral eclipse that never enters the umbral shadow. In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth, and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours, 53 minutes and 50.6 seconds in all, though for most of it, the eclipse was extremely difficult or impossible to see. The Moon was 2.2 days after apogee, making it 6.1% smaller 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 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 lunar eclipse took place on Tuesday, June 4, 1974, the first of two lunar eclipses in 1974. The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours and 14 minutes, with 82.695% of the Moon in darkness at maximum. Occurring 4.5 days before apogee, the Moon's apparent diameter was 4.4% smaller than average.
A partial lunar eclipse took place on Saturday, February 21, 1970. It was the first of two partial lunar eclipses in 1970, the other being on August 17 of the same year. A tiny bite out of the Moon may have been visible at maximum, though just 5% of the Moon was shadowed in a partial eclipse which lasted for 52 minutes and 42 seconds. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.
A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, May 24, 1956, with an umbral magnitude of 0.9647. 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 about 4.3 days before apogee, the Moon's apparent diameter was smaller.
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.