| Member 40 |
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 2007 Aug 28 |
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. [1]
This lunar saros is linked to Solar Saros 135.
Solar Saros 135 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
Lunar saros series 128, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 57 umbral eclipses (42 partial lunar eclipses and 15 total lunar eclipses). Solar Saros 135 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
| Greatest | First | |||
|---|---|---|---|---|
 The greatest eclipse of the series occurred on 1953 Jul 26, lasting 100.7 minutes. [2] | Penumbral | Partial | Total | Central |
| 1304 Jun 18 | 1430 Sep 2 | 1845 May 21 | 1899 Jun 23 | |
| Last | ||||
| Central | Total | Partial | Penumbral | |
| 2007 Aug 28 | 2097 May 21 | 2440 May 17 | 2566 Aug 2 | |
| 1917 Jul 4 | 1935 Jul 16 | 1953 Jul 26 | |||
 |  |  |  |  |  |
| 1971 Aug 6 | 1989 Aug 17 | 2007 Aug 28 | |||
 |  |  |  |  |  |
| 2025 Sep 7 | 2043 Sep 19 | 2061 Sep 29 | |||
 |  |  |  |  |  |
| 2079 Oct 10 | 2097 Oct 21 | ||||
 |  |  |  | ||
Lunar Saros 128 contains 15 total lunar eclipses between 1845 and 2097 (in years 1845, 1863, 1881, 1899, 1917, 1935, 1953, 1971, 1989, 2007, 2025, 2043, 2061, 2079 and 2097). Solar Saros 135 interleaves with this lunar saros with an event occurring every 9 years 5 days alternating between each saros series.
| 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 | ||||||||
| 07984 | 128 | 1 | 1304 Jun 18 | 9:25:47 | Penumbral | 1.4896 | -0.8572 | 88.5 | 8:41:32 | 10:10:02 | |||||||
| 08027 | 128 | 2 | 1322 Jun 29 | 16:45:29 | Penumbral | 1.4140 | -0.7173 | 132.1 | 15:39:26 | 17:51:32 | |||||||
| 08069 | 128 | 3 | 1340 Jul 10 | 0:06:41 | Penumbral | 1.3388 | -0.5785 | 162.6 | 22:45:23 | 1:27:59 | |||||||
| 08111 | 128 | 4 | 1358 Jul 21 | 7:33:39 | Penumbral | 1.2675 | -0.4473 | 185.5 | 6:00:54 | 9:06:24 | |||||||
| 08152 | 128 | 5 | 1376 Jul 31 | 15:04:49 | Penumbral | 1.1989 | -0.3213 | 204.0 | 13:22:49 | 16:46:49 | |||||||
| 08193 | 128 | 6 | 1394 Aug 11 | 22:42:10 | Penumbral | 1.1347 | -0.2035 | 219.0 | 20:52:40 | 0:31:40 | |||||||
| 08234 | 128 | 7 | 1412 Aug 22 | 6:26:36 | Penumbral | 1.0758 | -0.0957 | 231.2 | 4:31:00 | 8:22:12 | |||||||
| 08276 | 128 | 8 | 1430 Sep 02 | 14:18:56 | Partial | 1.0229 | 0.0008 | 241.1 | 6.3 | 12:18:23 | 16:19:29 | 14:15:47 | 14:22:05 | ||||
| 08317 | 128 | 9 | 1448 Sep 12 | 22:19:32 | Partial | 0.9764 | 0.0854 | 249.0 | 63.3 | 20:15:02 | 0:24:02 | 21:47:53 | 22:51:11 | ||||
| 08358 | 128 | 10 | 1466 Sep 24 | 6:28:03 | Partial | 0.9362 | 0.1585 | 255.4 | 85.3 | 4:20:21 | 8:35:45 | 5:45:24 | 7:10:42 | ||||
| 08398 | 128 | 11 | 1484 Oct 04 | 14:45:35 | Partial | 0.9031 | 0.2185 | 260.3 | 99.2 | 12:35:26 | 16:55:44 | 13:55:59 | 15:35:11 | ||||
| 08438 | 128 | 12 | 1502 Oct 15 | 23:10:40 | Partial | 0.8759 | 0.2675 | 264.1 | 108.8 | 20:58:37 | 1:22:43 | 22:16:16 | 0:05:04 | ||||
| 08478 | 128 | 13 | 1520 Oct 26 | 7:43:02 | Partial | 0.8549 | 0.3053 | 266.9 | 115.5 | 5:29:35 | 9:56:29 | 6:45:17 | 8:40:47 | ||||
| 08519 | 128 | 14 | 1538 Nov 06 | 16:22:02 | Partial | 0.8392 | 0.3334 | 268.9 | 120.1 | 14:07:35 | 18:36:29 | 15:21:59 | 17:22:05 | ||||
| 08561 | 128 | 15 | 1556 Nov 17 | 1:06:54 | Partial | 0.8286 | 0.3523 | 270.2 | 123.0 | 22:51:48 | 3:22:00 | 0:05:24 | 2:08:24 | ||||
| 08604 | 128 | 16 | 1574 Nov 28 | 9:55:43 | Partial | 0.8213 | 0.3655 | 271.1 | 125.0 | 7:40:10 | 12:11:16 | 8:53:13 | 10:58:13 | ||||
| 08647 | 128 | 17 | 1592 Dec 18 | 18:46:58 | Partial | 0.8160 | 0.3749 | 271.7 | 126.4 | 16:31:07 | 21:02:49 | 17:43:46 | 19:50:10 | ||||
| 08691 | 128 | 18 | 1610 Dec 30 | 3:39:54 | Partial | 0.8124 | 0.3817 | 272.1 | 127.3 | 1:23:51 | 5:55:57 | 2:36:15 | 4:43:33 | ||||
| 08736 | 128 | 19 | 1629 Jan 09 | 12:32:47 | Partial | 0.8092 | 0.3877 | 272.4 | 128.2 | 10:16:35 | 14:48:59 | 11:28:41 | 13:36:53 | ||||
| 08780 | 128 | 20 | 1647 Jan 20 | 21:23:09 | Partial | 0.8039 | 0.3979 | 273.0 | 129.7 | 19:06:39 | 23:39:39 | 20:18:18 | 22:28:00 | ||||
| 08825 | 128 | 21 | 1665 Jan 31 | 6:10:20 | Partial | 0.7963 | 0.4124 | 273.9 | 131.8 | 3:53:23 | 8:27:17 | 5:04:26 | 7:16:14 | ||||
| 08871 | 128 | 22 | 1683 Feb 11 | 14:52:35 | Partial | 0.7848 | 0.4345 | 275.2 | 134.9 | 12:34:59 | 17:10:11 | 13:45:08 | 16:00:02 | ||||
| 08917 | 128 | 23 | 1701 Feb 22 | 23:29:56 | Partial | 0.7695 | 0.4634 | 277.0 | 138.8 | 21:11:26 | 1:48:26 | 22:20:32 | 0:39:20 | ||||
| 08963 | 128 | 24 | 1719 Mar 06 | 7:59:13 | Partial | 0.7478 | 0.5043 | 279.5 | 143.9 | 5:39:28 | 10:18:58 | 6:47:16 | 9:11:10 | ||||
| 09010 | 128 | 25 | 1737 Mar 16 | 16:22:12 | Partial | 0.7211 | 0.5542 | 282.5 | 149.9 | 14:00:57 | 18:43:27 | 15:07:15 | 17:37:09 | ||||
| 09057 | 128 | 26 | 1755 Mar 28 | 0:36:25 | Partial | 0.6871 | 0.6176 | 286.2 | 156.8 | 22:13:19 | 2:59:31 | 23:18:01 | 1:54:49 | ||||
| 09103 | 128 | 27 | 1773 Apr 07 | 8:43:30 | Partial | 0.6476 | 0.6909 | 290.2 | 164.1 | 6:18:24 | 11:08:36 | 7:21:27 | 10:05:33 | ||||
| 09148 | 128 | 28 | 1791 Apr 18 | 16:41:28 | Partial | 0.6008 | 0.7776 | 294.7 | 171.8 | 14:14:07 | 19:08:49 | 15:15:34 | 18:07:22 | ||||
| 09193 | 128 | 29 | 1809 Apr 30 | 0:33:02 | Partial | 0.5490 | 0.8733 | 299.3 | 179.4 | 22:03:23 | 3:02:41 | 23:03:20 | 2:02:44 | ||||
| 09238 | 128 | 30 | 1827 May 11 | 8:16:57 | Partial | 0.4910 | 0.9801 | 304.0 | 186.8 | 5:44:57 | 10:48:57 | 6:43:33 | 9:50:21 | ||||
| 09285 | 128 | 31 | 1845 May 21 | 15:54:30 | Total | 0.4281 | 1.0957 | 308.6 | 193.7 | 45.3 | 13:20:12 | 18:28:48 | 14:17:39 | 15:31:51 | 16:17:09 | 17:31:21 | |
| 09330 | 128 | 32 | 1863 Jun 01 | 23:26:14 | Total | 0.3605 | 1.2195 | 312.9 | 199.9 | 66.1 | 20:49:47 | 2:02:41 | 21:46:17 | 22:53:11 | 23:59:17 | 1:06:11 | |
| 09374 | 128 | 33 | 1881 Jun 12 | 6:53:44 | Total | 0.2898 | 1.3488 | 316.8 | 205.2 | 79.9 | 4:15:20 | 9:32:08 | 5:11:08 | 6:13:47 | 7:33:41 | 8:36:20 | |
| 09418 | 128 | 34 | 1899 Jun 23 | 14:17:53 | Total | 0.2169 | 1.4820 | 320.1 | 209.5 | 89.5 | 11:37:50 | 16:57:56 | 12:33:08 | 13:33:08 | 15:02:38 | 16:02:38 | |
| 09460 | 128 | 35 | 1917 Jul 04 | 21:39:04 | Total | 0.1419 | 1.6185 | 322.9 | 212.8 | 96.0 | 18:57:37 | 0:20:31 | 19:52:40 | 20:51:04 | 22:27:04 | 23:25:28 | |
| 09502 | 128 | 36 | 1935 Jul 16 | 5:00:05 | Total | 0.0672 | 1.7542 | 325.0 | 214.8 | 99.6 | 2:17:35 | 7:42:35 | 3:12:41 | 4:10:17 | 5:49:53 | 6:47:29 | |
| 09543 | 128 | 37 | 1953 Jul 26 | 12:21:10 | Total | -0.0071 | 1.8628 | 326.5 | 215.7 | 100.7 | 9:37:55 | 15:04:25 | 10:33:19 | 11:30:49 | 13:11:31 | 14:09:01 | |
| 09584 | 128 | 38 | 1971 Aug 06 | 19:43:52 | Total | -0.0794 | 1.7283 | 327.3 | 215.5 | 99.4 | 17:00:13 | 22:27:31 | 17:56:07 | 18:54:10 | 20:33:34 | 21:31:37 | |
| 09625 | 128 | 39 | 1989 Aug 17 | 3:09:07 | Total | -0.1490 | 1.5984 | 327.5 | 214.3 | 95.8 | 0:25:22 | 5:52:52 | 1:21:58 | 2:21:13 | 3:57:01 | 4:56:16 | |
| 09666 | 128 | 40 | 2007 Aug 28 | 10:38:27 | Total | -0.2145 | 1.4758 | 327.3 | 212.2 | 90.0 | 7:54:48 | 13:22:06 | 8:52:21 | 9:53:27 | 11:23:27 | 12:24:33 | |
| 09707 | 128 | 41 | 2025 Sep 07 | 18:12:58 | Total | -0.2752 | 1.3619 | 326.7 | 209.4 | 82.1 | 15:29:37 | 20:56:19 | 16:28:16 | 17:31:55 | 18:54:01 | 19:57:40 | |
| 09748 | 128 | 42 | 2043 Sep 19 | 1:51:50 | Total | -0.3316 | 1.2556 | 325.8 | 206.0 | 71.7 | 23:08:56 | 4:34:44 | 0:08:50 | 1:15:59 | 2:27:41 | 3:34:50 | |
| 09789 | 128 | 43 | 2061 Sep 29 | 9:38:13 | Total | -0.3810 | 1.1621 | 324.8 | 202.4 | 59.0 | 6:55:49 | 12:20:37 | 7:57:01 | 9:08:43 | 10:07:43 | 11:19:25 | |
| 09830 | 128 | 44 | 2079 Oct 10 | 17:30:30 | Total | -0.4246 | 1.0791 | 323.8 | 198.7 | 42.4 | 14:48:36 | 20:12:24 | 15:51:09 | 17:09:18 | 17:51:42 | 19:09:51 | |
| 09872 | 128 | 45 | 2097 Oct 21 | 1:30:55 | Total | -0.4608 | 1.0097 | 323.1 | 195.2 | 15.2 | 22:49:22 | 4:12:28 | 23:53:19 | 1:23:19 | 1:38:31 | 3:08:31 | |
| 09914 | 128 | 46 | 2115 Nov 02 | 9:36:34 | Partial | -0.4919 | 0.9498 | 322.4 | 191.9 | 6:55:22 | 12:17:46 | 8:00:37 | 11:12:31 | ||||
| 09956 | 128 | 47 | 2133 Nov 12 | 17:50:08 | Partial | -0.5157 | 0.9033 | 322.2 | 189.3 | 15:09:02 | 20:31:14 | 16:15:29 | 19:24:47 | ||||
| 10000 | 128 | 48 | 2151 Nov 24 | 2:08:13 | Partial | -0.5350 | 0.8651 | 322.2 | 187.0 | 23:27:07 | 4:49:19 | 0:34:43 | 3:41:43 | ||||
| 10043 | 128 | 49 | 2169 Dec 04 | 10:31:58 | Partial | -0.5488 | 0.8375 | 322.5 | 185.3 | 7:50:43 | 13:13:13 | 8:59:19 | 12:04:37 | ||||
| 10086 | 128 | 50 | 2187 Dec 15 | 18:58:37 | Partial | -0.5595 | 0.8156 | 323.0 | 184.1 | 16:17:07 | 21:40:07 | 17:26:34 | 20:30:40 | ||||
| 10129 | 128 | 51 | 2205 Dec 27 | 3:28:47 | Partial | -0.5665 | 0.8008 | 323.8 | 183.4 | 0:46:53 | 6:10:41 | 1:57:05 | 5:00:29 | ||||
| 10173 | 128 | 52 | 2224 Jan 07 | 11:58:46 | Partial | -0.5731 | 0.7870 | 324.5 | 182.7 | 9:16:31 | 14:41:01 | 10:27:25 | 13:30:07 | ||||
| 10218 | 128 | 53 | 2242 Jan 17 | 20:28:26 | Partial | -0.5794 | 0.7742 | 325.2 | 182.2 | 17:45:50 | 23:11:02 | 18:57:20 | 21:59:32 | ||||
| 10264 | 128 | 54 | 2260 Jan 29 | 4:55:22 | Partial | -0.5871 | 0.7589 | 325.7 | 181.3 | 2:12:31 | 7:38:13 | 3:24:43 | 6:26:01 | ||||
| 10310 | 128 | 55 | 2278 Feb 08 | 13:19:10 | Partial | -0.5965 | 0.7409 | 326.0 | 180.2 | 10:36:10 | 16:02:10 | 11:49:04 | 14:49:16 | ||||
| 10357 | 128 | 56 | 2296 Feb 19 | 21:35:59 | Partial | -0.6112 | 0.7135 | 325.6 | 178.2 | 18:53:11 | 0:18:47 | 20:06:53 | 23:05:05 | ||||
| 10403 | 128 | 57 | 2314 Mar 03 | 5:46:48 | Partial | -0.6301 | 0.6784 | 324.8 | 175.3 | 3:04:24 | 8:29:12 | 4:19:09 | 7:14:27 | ||||
| 10449 | 128 | 58 | 2332 Mar 13 | 13:48:34 | Partial | -0.6557 | 0.6313 | 323.2 | 170.9 | 11:06:58 | 16:30:10 | 12:23:07 | 15:14:01 | ||||
| 10495 | 128 | 59 | 2350 Mar 24 | 21:42:58 | Partial | -0.6865 | 0.5747 | 320.9 | 165.1 | 19:02:31 | 0:23:25 | 20:20:25 | 23:05:31 | ||||
| 10540 | 128 | 60 | 2368 Apr 04 | 5:25:31 | Partial | -0.7261 | 0.5021 | 317.3 | 156.6 | 2:46:52 | 8:04:10 | 4:07:13 | 6:43:49 | ||||
| 10584 | 128 | 61 | 2386 Apr 15 | 12:59:59 | Partial | -0.7715 | 0.4189 | 312.6 | 145.3 | 10:23:41 | 15:36:17 | 11:47:20 | 14:12:38 | ||||
| 10629 | 128 | 62 | 2404 Apr 25 | 20:22:55 | Partial | -0.8255 | 0.3197 | 306.1 | 129.2 | 17:49:52 | 22:55:58 | 19:18:19 | 21:27:31 | ||||
| 10673 | 128 | 63 | 2422 May 7 | 3:37:48 | Partial | -0.8852 | 0.2103 | 298.1 | 106.8 | 1:08:45 | 6:06:51 | 2:44:24 | 4:31:12 | ||||
| 10717 | 128 | 64 | 2440 May 17 | 10:41:49 | Partial | -0.9527 | 0.0862 | 287.8 | 69.8 | 8:17:55 | 13:05:43 | 10:06:55 | 11:16:43 | ||||
| 10761 | 128 | 65 | 2458 May 28 | 17:39:26 | Penumbral | -1.0244 | -0.0456 | 275.2 | 15:21:50 | 19:57:02 | |||||||
| 10803 | 128 | 66 | 2476 Jun 08 | 0:28:51 | Penumbral | -1.1019 | -0.1884 | 259.5 | 22:19:06 | 2:38:36 | |||||||
| 10844 | 128 | 67 | 2494 Jun 19 | 7:12:41 | Penumbral | -1.1829 | -0.3375 | 240.4 | 5:12:29 | 9:12:53 | |||||||
| 10885 | 128 | 68 | 2512 Jun 30 | 13:51:10 | Penumbral | -1.2672 | -0.4931 | 216.7 | 12:02:49 | 15:39:31 | |||||||
| 10925 | 128 | 69 | 2530 Jul 11 | 20:27:10 | Penumbral | -1.3526 | -0.6507 | 187.3 | 18:53:31 | 22:00:49 | |||||||
| 10966 | 128 | 70 | 2548 Jul 22 | 3:01:34 | Penumbral | -1.4381 | -0.8088 | 149.3 | 1:46:55 | 4:16:13 | |||||||
| 11008 | 128 | 71 | 2566 Aug 02 | 9:35:06 | Penumbral | -1.5233 | -0.9665 | 92.9 | 8:48:39 | 10:21:33 | |||||||
A total lunar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, August 28, 2007, with an umbral magnitude of 1.4777. 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 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 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 will occur at the Moon’s ascending node of orbit on Sunday, September 7, 2025, with an umbral magnitude of 1.3638. 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 2.6 days after perigee, the Moon's apparent diameter will be larger.
A total lunar eclipse took place on Saturday, April 13, 1968, the first of two total eclipses in 1968, the second being on October 6, 1968.
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 partial lunar eclipse occurred at the Moon’s descending node of orbit on Tuesday, March 22, 1932, with an umbral magnitude of 0.9666. 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 21 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 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 will occur at the Moon’s ascending node of orbit on Saturday, September 19, 2043, with an umbral magnitude of 1.2575. 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 2.8 days before perigee, the Moon's apparent diameter will be larger.
An annular solar eclipse will occur at the Moon's descending node of orbit between Sunday, November 3 and Monday, November 4, 2097, with a magnitude of 0.9494. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 5.4 days before apogee, the Moon's apparent diameter will be smaller.
A total solar eclipse will occur at the Moon's ascending node of orbit on Saturday, May 11, 2097, with a magnitude of 1.0538. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.3 days before perigee, the Moon's apparent diameter will be larger.
An annular solar eclipse will occur at the Moon's ascending node of orbit on Thursday, October 14, 2088, with a magnitude of 0.9727. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 6.3 days before apogee, the Moon's apparent diameter will be smaller.
A partial solar eclipse will occur at the Moon's descending node of orbit on Friday, March 31, 2090, with a magnitude of 0.7843. 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 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 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.
A total lunar eclipse occurred at the Moon’s ascending node of orbit on Tuesday, July 16, 1935, with an umbral magnitude of 1.7542. 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 was larger.
