Saros cycle series 106 for lunar eclipses occurred at the moon's ascending node, 18 years 11 and 1/3 days. It contained 73 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 | ||||||||
06253 | 106 | 1 | 595 Jul 27 | 1:33:13 | Penumbral | 1.5221 | -0.9596 | 90.2 | 0:48:07 | 2:18:19 | |||||||
06301 | 106 | 2 | 613 Aug 06 | 8:29:10 | Penumbral | 1.4514 | -0.8298 | 138.8 | 7:19:46 | 9:38:34 | |||||||
06347 | 106 | 3 | 631 Aug 17 | 15:33:22 | Penumbral | 1.3860 | -0.7097 | 170.3 | 14:08:13 | 16:58:31 | |||||||
06393 | 106 | 4 | 649 Aug 27 | 22:47:19 | Penumbral | 1.3270 | -0.6015 | 193.0 | 21:10:49 | 0:23:49 | |||||||
06438 | 106 | 5 | 667 Sep 08 | 6:11:10 | Penumbral | 1.2749 | -0.5061 | 210.1 | 4:26:07 | 7:56:13 | |||||||
06483 | 106 | 6 | 685 Sep 18 | 13:46:00 | Penumbral | 1.2307 | -0.4250 | 222.9 | 11:54:33 | 15:37:27 | |||||||
06528 | 106 | 7 | 703 Sep 29 | 21:30:42 | Penumbral | 1.1934 | -0.3566 | 232.5 | 19:34:27 | 23:26:57 | |||||||
06572 | 106 | 8 | 721 Oct 10 | 5:25:14 | Penumbral | 1.1632 | -0.3012 | 239.6 | 3:25:26 | 7:25:02 | |||||||
06616 | 106 | 9 | 739 Oct 21 | 13:28:49 | Penumbral | 1.1394 | -0.2574 | 244.6 | 11:26:31 | 15:31:07 | |||||||
06660 | 106 | 10 | 757 Oct 31 | 21:41:14 | Penumbral | 1.1221 | -0.2253 | 247.9 | 19:37:17 | 23:45:11 | |||||||
06704 | 106 | 11 | 775 Nov 12 | 5:59:14 | Penumbral | 1.1088 | -0.2002 | 250.0 | 3:54:14 | 8:04:14 | |||||||
06746 | 106 | 12 | 793 Nov 22 | 14:23:41 | Penumbral | 1.1000 | -0.1832 | 251.0 | 12:18:11 | 16:29:11 | |||||||
06788 | 106 | 13 | 811 Dec 03 | 22:51:00 | Penumbral | 1.0931 | -0.1694 | 251.5 | 20:45:15 | 0:56:45 | |||||||
06828 | 106 | 14 | 829 Dec 14 | 7:21:21 | Penumbral | 1.0879 | -0.1583 | 251.5 | 5:15:36 | 9:27:06 | |||||||
06868 | 106 | 15 | 847 Dec 25 | 15:50:18 | Penumbral | 1.0809 | -0.1436 | 251.9 | 13:44:21 | 17:56:15 | |||||||
06909 | 106 | 16 | 866 Jan 05 | 0:19:44 | Penumbral | 1.0736 | -0.1283 | 252.1 | 22:13:41 | 2:25:47 | |||||||
06950 | 106 | 17 | 884 Jan 16 | 8:45:25 | Penumbral | 1.0630 | -0.1064 | 253.0 | 6:38:55 | 10:51:55 | |||||||
06992 | 106 | 18 | 902 Jan 26 | 17:07:20 | Penumbral | 1.0483 | -0.0769 | 254.6 | 15:00:02 | 19:14:38 | |||||||
07033 | 106 | 19 | 920 Feb 07 | 1:22:57 | Penumbral | 1.0279 | -0.0366 | 257.2 | 23:14:21 | 3:31:33 | |||||||
07074 | 106 | 20 | 938 Feb 17 | 9:33:20 | Partial | 1.0023 | 0.0133 | 260.6 | 26.3 | 7:23:02 | 11:43:38 | 9:20:11 | 9:46:29 | ||||
07115 | 106 | 21 | 956 Feb 28 | 17:36:42 | Partial | 0.9704 | 0.0748 | 264.8 | 61.7 | 15:24:18 | 19:49:06 | 17:05:51 | 18:07:33 | ||||
07156 | 106 | 22 | 974 Mar 11 | 1:32:38 | Partial | 0.9317 | 0.1489 | 269.7 | 85.9 | 23:17:47 | 3:47:29 | 0:49:41 | 2:15:35 | ||||
07197 | 106 | 23 | 992 Mar 21 | 9:21:55 | Partial | 0.8867 | 0.2344 | 275.3 | 106.2 | 7:04:16 | 11:39:34 | 8:28:49 | 10:15:01 | ||||
07241 | 106 | 24 | 1010 Apr 01 | 17:04:25 | Partial | 0.8352 | 0.3319 | 281.2 | 124.2 | 14:43:49 | 19:25:01 | 16:02:19 | 18:06:31 | ||||
07286 | 106 | 25 | 1028 Apr 12 | 0:40:17 | Partial | 0.7775 | 0.4405 | 287.3 | 140.4 | 22:16:38 | 3:03:56 | 23:30:05 | 1:50:29 | ||||
07330 | 106 | 26 | 1046 Apr 23 | 8:10:38 | Partial | 0.7145 | 0.5587 | 293.3 | 154.8 | 5:43:59 | 10:37:17 | 6:53:14 | 9:28:02 | ||||
07374 | 106 | 27 | 1064 May 3 | 15:36:35 | Partial | 0.6470 | 0.6850 | 298.9 | 167.5 | 13:07:08 | 18:06:02 | 14:12:50 | 17:00:20 | ||||
07418 | 106 | 28 | 1082 May 14 | 22:59:40 | Partial | 0.5763 | 0.8169 | 304.1 | 178.5 | 20:27:37 | 1:31:43 | 21:30:25 | 0:28:55 | ||||
07464 | 106 | 29 | 1100 May 25 | 6:19:17 | Partial | 0.5017 | 0.9556 | 308.8 | 188.0 | 3:44:53 | 8:53:41 | 4:45:17 | 7:53:17 | ||||
07510 | 106 | 30 | 1118 Jun 5 | 13:39:05 | Total | 0.4266 | 1.095 | 312.7 | 195.7 | 45.5 | 11:02:44 | 16:15:26 | 12:01:14 | 13:16:20 | 14:01:50 | 15:16:56 | |
07556 | 106 | 31 | 1136 Jun 15 | 20:58:24 | Total | 0.35 | 1.2368 | 315.8 | 201.9 | 68.6 | 18:20:30 | 23:36:18 | 19:17:27 | 20:24:06 | 21:32:42 | 22:39:21 | |
07603 | 106 | 32 | 1154 Jun 27 | 4:20:08 | Total | 0.275 | 1.3754 | 318.1 | 206.5 | 82.2 | 1:41:05 | 6:59:11 | 2:36:53 | 3:39:02 | 5:01:14 | 6:03:23 | |
07651 | 106 | 33 | 1172 Jul 7 | 11:43:06 | Total | 0.2002 | 1.5132 | 319.8 | 209.8 | 91.1 | 9:03:12 | 14:23:00 | 9:58:12 | 10:57:33 | 12:28:39 | 13:28:00 | |
07697 | 106 | 34 | 1190 Jul 18 | 19:11:31 | Total | 0.1293 | 1.6436 | 320.6 | 211.8 | 96.3 | 16:31:13 | 21:51:49 | 17:25:37 | 18:23:22 | 19:59:40 | 20:57:25 | |
07743 | 106 | 35 | 1208 Jul 29 | 2:44:05 | Total | 0.0611 | 1.7688 | 320.9 | 212.8 | 99.0 | 0:03:38 | 5:24:32 | 0:57:41 | 1:54:35 | 3:33:35 | 4:30:29 | |
07789 | 106 | 36 | 1226 Aug 09 | 10:22:59 | Total | -0.0021 | 1.8770 | 320.6 | 212.8 | 99.6 | 7:42:41 | 13:03:17 | 8:36:35 | 9:33:11 | 11:12:47 | 12:09:23 | |
07834 | 106 | 37 | 1244 Aug 19 | 18:08:09 | Total | -0.0604 | 1.7694 | 320.0 | 212.0 | 98.7 | 15:28:09 | 20:48:09 | 16:22:09 | 17:18:48 | 18:57:30 | 19:54:09 | |
07879 | 106 | 38 | 1262 Aug 31 | 2:01:40 | Total | -0.1120 | 1.6741 | 319.1 | 210.8 | 96.5 | 23:22:07 | 4:41:13 | 0:16:16 | 1:13:25 | 2:49:55 | 3:47:04 | |
07924 | 106 | 39 | 1280 Sep 10 | 10:02:47 | Total | -0.1577 | 1.5895 | 318.0 | 209.2 | 93.5 | 7:23:47 | 12:41:47 | 8:18:11 | 9:16:02 | 10:49:32 | 11:47:23 | |
07969 | 106 | 40 | 1298 Sep 21 | 18:11:08 | Total | -0.1975 | 1.5155 | 316.9 | 207.5 | 90.0 | 15:32:41 | 20:49:35 | 16:27:23 | 17:26:08 | 18:56:08 | 19:54:53 | |
08013 | 106 | 41 | 1316 Oct 02 | 2:28:20 | Total | -0.2301 | 1.4547 | 315.8 | 205.8 | 86.5 | 23:50:26 | 5:06:14 | 0:45:26 | 1:45:05 | 3:11:35 | 4:11:14 | |
08056 | 106 | 42 | 1334 Oct 13 | 10:52:55 | Total | -0.2565 | 1.4053 | 314.9 | 204.2 | 83.1 | 8:15:28 | 13:30:22 | 9:10:49 | 10:11:22 | 11:34:28 | 12:35:01 | |
08098 | 106 | 43 | 1352 Oct 23 | 19:25:34 | Total | -0.2765 | 1.3677 | 314.2 | 202.9 | 80.2 | 16:48:28 | 22:02:40 | 17:44:07 | 18:45:28 | 20:05:40 | 21:07:01 | |
08139 | 106 | 44 | 1370 Nov 04 | 4:03:32 | Total | -0.2920 | 1.3383 | 313.6 | 201.8 | 77.6 | 1:26:44 | 6:40:20 | 2:22:38 | 3:24:44 | 4:42:20 | 5:44:26 | |
08180 | 106 | 45 | 1388 Nov 14 | 12:48:27 | Total | -0.3020 | 1.3193 | 313.2 | 201.1 | 75.9 | 10:11:51 | 15:25:03 | 11:07:54 | 12:10:30 | 13:26:24 | 14:29:00 | |
08221 | 106 | 46 | 1406 Nov 25 | 21:36:51 | Total | -0.3091 | 1.3057 | 313.0 | 200.6 | 74.6 | 19:00:21 | 0:13:21 | 19:56:33 | 20:59:33 | 22:14:09 | 23:17:09 | |
08262 | 106 | 47 | 1424 Dec 06 | 6:28:42 | Total | -0.3134 | 1.2975 | 312.9 | 200.3 | 73.7 | 3:52:15 | 9:05:09 | 4:48:33 | 5:51:51 | 7:05:33 | 8:08:51 | |
08304 | 106 | 48 | 1442 Dec 17 | 15:21:21 | Total | -0.3170 | 1.2906 | 312.8 | 200.0 | 73.1 | 12:44:57 | 17:57:45 | 13:41:21 | 14:44:48 | 15:57:54 | 17:01:21 | |
08345 | 106 | 49 | 1460 Dec 28 | 0:14:45 | Total | -0.3200 | 1.2851 | 312.7 | 199.9 | 72.5 | 21:38:24 | 2:51:06 | 22:34:48 | 23:38:30 | 0:51:00 | 1:54:42 | |
08385 | 106 | 50 | 1479 Jan 08 | 9:05:26 | Total | -0.3253 | 1.2757 | 312.6 | 199.6 | 71.6 | 6:29:08 | 11:41:44 | 7:25:38 | 8:29:38 | 9:41:14 | 10:45:14 | |
08425 | 106 | 51 | 1497 Jan 18 | 17:53:14 | Total | -0.3330 | 1.2619 | 312.3 | 199.2 | 70.2 | 15:17:05 | 20:29:23 | 16:13:38 | 17:18:08 | 18:28:20 | 19:32:50 | |
08465 | 106 | 52 | 1515 Jan 30 | 2:35:56 | Total | -0.3447 | 1.2410 | 311.9 | 198.5 | 67.8 | 23:59:59 | 5:11:53 | 0:56:41 | 2:02:02 | 3:09:50 | 4:15:11 | |
08506 | 106 | 53 | 1533 Feb 09 | 11:13:52 | Total | -0.3602 | 1.2134 | 311.2 | 197.6 | 64.5 | 8:38:16 | 13:49:28 | 9:35:04 | 10:41:37 | 11:46:07 | 12:52:40 | |
08548 | 106 | 54 | 1551 Feb 20 | 19:43:12 | Total | -0.3827 | 1.1729 | 310.3 | 196.0 | 58.9 | 17:08:03 | 22:18:21 | 18:05:12 | 19:13:45 | 20:12:39 | 21:21:12 | |
08592 | 106 | 55 | 1569 Mar 03 | 4:06:08 | Total | -0.4104 | 1.1228 | 308.9 | 193.9 | 50.5 | 1:31:41 | 6:40:35 | 2:29:11 | 3:40:53 | 4:31:23 | 5:43:05 | |
08635 | 106 | 56 | 1587 Mar 24 | 12:19:48 | Total | -0.4456 | 1.0591 | 307.1 | 190.8 | 35.7 | 9:46:15 | 14:53:21 | 10:44:24 | 12:01:57 | 12:37:39 | 13:55:12 | |
08678 | 106 | 57 | 1605 Apr 03 | 20:27:02 | Partial | -0.4858 | 0.9861 | 304.8 | 186.9 | 17:54:38 | 22:59:26 | 18:53:35 | 22:00:29 | ||||
08723 | 106 | 58 | 1623 Apr 15 | 4:23:33 | Partial | -0.5345 | 0.8972 | 301.6 | 181.4 | 1:52:45 | 6:54:21 | 2:52:51 | 5:54:15 | ||||
08767 | 106 | 59 | 1641 Apr 25 | 12:14:36 | Partial | -0.5876 | 0.8003 | 297.8 | 174.6 | 9:45:42 | 14:43:30 | 10:47:18 | 13:41:54 | ||||
08812 | 106 | 60 | 1659 May 6 | 19:56:13 | Partial | -0.6484 | 0.6890 | 292.8 | 165.3 | 17:29:49 | 22:22:37 | 18:33:34 | 21:18:52 | ||||
08857 | 106 | 61 | 1677 May 17 | 3:32:58 | Partial | -0.7127 | 0.5710 | 286.8 | 153.7 | 1:09:34 | 5:56:22 | 2:16:07 | 4:49:49 | ||||
08903 | 106 | 62 | 1695 May 28 | 11:01:57 | Partial | -0.7830 | 0.4417 | 279.3 | 138.2 | 8:42:18 | 13:21:36 | 9:52:51 | 12:11:03 | ||||
08949 | 106 | 63 | 1713 Jun 08 | 18:28:15 | Partial | -0.8551 | 0.3089 | 270.6 | 118.1 | 16:12:57 | 20:43:33 | 17:29:12 | 19:27:18 | ||||
08996 | 106 | 64 | 1731 Jun 20 | 1:49:42 | Partial | -0.9307 | 0.1692 | 260.2 | 89.4 | 23:39:36 | 3:59:48 | 1:05:00 | 2:34:24 | ||||
09042 | 106 | 65 | 1749 Jun 30 | 9:09:16 | Partial | -1.0073 | 0.0276 | 248.2 | 36.9 | 7:05:10 | 11:13:22 | 8:50:49 | 9:27:43 | ||||
09089 | 106 | 66 | 1767 Jul 11 | 16:27:13 | Penumbral | -1.0845 | -0.1155 | 234.2 | 14:30:07 | 18:24:19 | |||||||
09134 | 106 | 67 | 1785 Jul 21 | 23:45:46 | Penumbral | -1.1605 | -0.2568 | 218.2 | 21:56:40 | 1:34:52 | |||||||
09179 | 106 | 68 | 1803 Aug 03 | 7:05:09 | Penumbral | -1.2349 | -0.3953 | 200.0 | 5:25:09 | 8:45:09 | |||||||
09224 | 106 | 69 | 1821 Aug 13 | 14:26:43 | Penumbral | -1.3066 | -0.5292 | 179.2 | 12:57:07 | 15:56:19 | |||||||
09270 | 106 | 70 | 1839 Aug 24 | 21:52:11 | Penumbral | -1.3743 | -0.6560 | 155.5 | 20:34:26 | 23:09:56 | |||||||
09315 | 106 | 71 | 1857 Sep 04 | 5:22:14 | Penumbral | -1.4376 | -0.7748 | 127.6 | 4:18:26 | 6:26:02 | |||||||
09359 | 106 | 72 | 1875 Sep 15 | 12:57:27 | Penumbral | -1.4955 | -0.8839 | 93.2 | 12:10:51 | 13:44:03 | |||||||
09403 | 106 | 73 | 1893 Sep 25 | 20:39:00 | Penumbral | -1.5476 | -0.9825 | 38.9 | 20:19:33 | 20:58:27 |
A total lunar eclipse occurred at the Moon’s descending node of orbit on Sunday, July 16, 2000, with an umbral magnitude of 1.7684. 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 1.1 days after apogee, the Moon's apparent diameter was smaller.
A total lunar eclipse took place on Monday, February 20, 1989, the first of two total lunar eclipses in 1989.
A total lunar eclipse will occur at the Moon’s descending node of orbit on Thursday, August 7, 2036, with an umbral magnitude of 1.4556. 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 11 hours after apogee, the Moon's apparent diameter will be smaller.
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 at the Moon's descending node of the orbit on Wednesday, February 10, 1971, the first of two total lunar eclipses in 1971. It had an umbral magnitude of 1.30819. The Moon narrowly missed the center of the Earth's shadow due its gamma being >0.2725 at 0.27413. The Moon was plunged into darkness for 1 hour, 22 minutes and 11.4 seconds, in a deep total eclipse which saw the Moon 30.819% 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, 44 minutes and 42.9 seconds and in total. Occurring only 2.7 days before apogee, the Moon's apparent diameter was 5.9% smaller than average.
A total lunar eclipse took place on Monday, October 28, 1985, the second of two total lunar eclipses in 1985, the first being on May 4, 1985.
A penumbral lunar eclipse took place on Tuesday, May 15, 1984, the first of three lunar eclipses in 1984. This was a deep penumbral eclipse, with the southern limb of the Moon close to the Earth's shadow.
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 total lunar eclipse took place on Wednesday, October 18, 1967, the second of two total lunar eclipses in 1967, the first being on April 24, 1967.
A penumbral lunar eclipse took place on Wednesday, May 4, 1966, the first of two penumbral lunar eclipses in 1966. It was visible from South America, Europe, Africa, Asia, Australia and Antarctica.
A total lunar eclipse occurred at the Moon’s ascending node of orbit on Sunday, July 26, 1953, with an umbral magnitude of 1.8629. 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 2.1 days before perigee, the Moon's apparent diameter was larger.
A total lunar eclipse occurred at the Moon’s ascending node of orbit on Monday, September 15, 1913, with an umbral magnitude of 1.4304. 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 apogee, the Moon's apparent diameter was smaller.
A total lunar eclipse occurred at the Moon’s descending node of orbit on Tuesday, May 24, 1910, with an umbral magnitude of 1.0950. 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 2.4 days after apogee, the Moon's apparent diameter was smaller.
A total lunar eclipse will occur at the Moon’s descending node of orbit on Sunday, August 28, 2072, with an umbral magnitude of 1.1673. 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 4.5 hours before apogee, the Moon's apparent diameter will be smaller.
A total lunar eclipse will occur at the Moon’s descending node of orbit on Friday, September 8, 2090, with an umbral magnitude of 1.0387. 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 12 hours before apogee, the Moon's apparent diameter will be smaller.
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 111 for lunar eclipses occurs at the moon's descending node, repeats every 18 years 11 and 1/3 days. It contains 71 events.
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.
A total lunar eclipse will occur at the Moon’s ascending node of orbit on Wednesday, June 9, 2123, with an umbral magnitude of 1.7488. 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 after apogee, the Moon's apparent diameter will be smaller.