Saros cycle series 104 for lunar eclipses occurred at the moon's ascending node, 18 years 11 and 1/3 days. It contained 72 events. [1]
This lunar saros was linked to Solar Saros 111.
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 | ||||||||
05969 | 104 | 1 | 483 Aug 4 | 10:31:02 | Penumbral | 1.492 | -0.8541 | 81.3 | 9:50:23 | 11:11:41 | |||||||
06015 | 104 | 2 | 501 Aug 14 | 18:18:54 | Penumbral | 1.4366 | -0.7533 | 116.4 | 17:20:42 | 19:17:06 | |||||||
06060 | 104 | 3 | 519 Aug 26 | 2:14:07 | Penumbral | 1.3870 | -0.6634 | 139.9 | 1:04:10 | 3:24:04 | |||||||
06105 | 104 | 4 | 537 Sep 05 | 10:16:09 | Penumbral | 1.3429 | -0.5836 | 157.4 | 8:57:27 | 11:34:51 | |||||||
06151 | 104 | 5 | 555 Sep 16 | 18:26:52 | Penumbral | 1.3058 | -0.5171 | 170.4 | 17:01:40 | 19:52:04 | |||||||
06197 | 104 | 6 | 573 Sep 27 | 2:44:59 | Penumbral | 1.2751 | -0.4621 | 180.3 | 1:14:50 | 4:15:08 | |||||||
06243 | 104 | 7 | 591 Oct 08 | 11:11:50 | Penumbral | 1.2514 | -0.4200 | 187.6 | 9:38:02 | 12:45:38 | |||||||
06291 | 104 | 8 | 609 Oct 18 | 19:44:15 | Penumbral | 1.2323 | -0.3863 | 193.2 | 18:07:39 | 21:20:51 | |||||||
06337 | 104 | 9 | 627 Oct 30 | 4:24:39 | Penumbral | 1.2200 | -0.3649 | 196.9 | 2:46:12 | 6:03:06 | |||||||
06383 | 104 | 10 | 645 Nov 09 | 13:09:24 | Penumbral | 1.2114 | -0.3503 | 199.5 | 11:29:39 | 14:49:09 | |||||||
06428 | 104 | 11 | 663 Nov 20 | 21:59:12 | Penumbral | 1.2073 | -0.3437 | 200.9 | 20:18:45 | 23:39:39 | |||||||
06473 | 104 | 12 | 681 Dec 01 | 6:50:31 | Penumbral | 1.2047 | -0.3397 | 201.9 | 5:09:34 | 8:31:28 | |||||||
06519 | 104 | 13 | 699 Dec 12 | 15:43:47 | Penumbral | 1.2041 | -0.3391 | 202.3 | 14:02:38 | 17:24:56 | |||||||
06563 | 104 | 14 | 717 Dec 23 | 0:35:34 | Penumbral | 1.2028 | -0.3370 | 202.9 | 22:54:07 | 2:17:01 | |||||||
06606 | 104 | 15 | 736 Jan 03 | 9:25:09 | Penumbral | 1.2004 | -0.3326 | 203.8 | 7:43:15 | 11:07:03 | |||||||
06651 | 104 | 16 | 754 Jan 13 | 18:10:39 | Penumbral | 1.1951 | -0.3229 | 205.4 | 16:27:57 | 19:53:21 | |||||||
06695 | 104 | 17 | 772 Jan 25 | 2:51:28 | Penumbral | 1.1870 | -0.3076 | 207.6 | 1:07:40 | 4:35:16 | |||||||
06737 | 104 | 18 | 790 Feb 04 | 11:24:47 | Penumbral | 1.1732 | -0.2819 | 211.3 | 9:39:08 | 13:10:26 | |||||||
06779 | 104 | 19 | 808 Feb 15 | 19:51:09 | Penumbral | 1.1543 | -0.2468 | 216.0 | 18:03:09 | 21:39:09 | |||||||
06820 | 104 | 20 | 826 Feb 26 | 4:08:47 | Penumbral | 1.1290 | -0.1999 | 222.1 | 2:17:44 | 5:59:50 | |||||||
06860 | 104 | 21 | 844 Mar 08 | 12:19:11 | Penumbral | 1.0985 | -0.1435 | 229.0 | 10:24:41 | 14:13:41 | |||||||
06901 | 104 | 22 | 862 Mar 19 | 20:18:53 | Penumbral | 1.0598 | -0.0721 | 237.4 | 18:20:11 | 22:17:35 | |||||||
06942 | 104 | 23 | 880 Mar 30 | 4:11:45 | Partial | 1.0161 | 0.0084 | 246.2 | 20.4 | 2:08:39 | 6:14:51 | 4:01:33 | 4:21:57 | ||||
06984 | 104 | 24 | 898 Apr 10 | 11:55:02 | Partial | 0.9647 | 0.1027 | 255.8 | 70.4 | 9:47:08 | 14:02:56 | 11:19:50 | 12:30:14 | ||||
07025 | 104 | 25 | 916 Apr 20 | 19:32:10 | Partial | 0.9090 | 0.2049 | 265.4 | 98.2 | 17:19:28 | 21:44:52 | 18:43:04 | 20:21:16 | ||||
07065 | 104 | 26 | 934 May 2 | 3:00:10 | Partial | 0.8463 | 0.3196 | 275.4 | 121.0 | 0:42:28 | 5:17:52 | 1:59:40 | 4:00:40 | ||||
07106 | 104 | 27 | 952 May 12 | 10:23:59 | Partial | 0.7807 | 0.4394 | 284.9 | 139.8 | 8:01:32 | 12:46:26 | 9:14:05 | 11:33:53 | ||||
07146 | 104 | 28 | 970 May 23 | 17:41:28 | Partial | 0.7102 | 0.5678 | 294.2 | 156.2 | 15:14:22 | 20:08:34 | 16:23:22 | 18:59:34 | ||||
07187 | 104 | 29 | 988 Jun 03 | 0:55:42 | Partial | 0.6377 | 0.6996 | 302.9 | 170.3 | 22:24:15 | 3:27:09 | 23:30:33 | 2:20:51 | ||||
07231 | 104 | 30 | 1006 Jun 14 | 8:06:25 | Partial | 0.5629 | 0.8354 | 310.9 | 182.4 | 5:30:58 | 10:41:52 | 6:35:13 | 9:37:37 | ||||
07276 | 104 | 31 | 1024 Jun 24 | 15:16:44 | Partial | 0.4885 | 0.9702 | 318.1 | 192.6 | 12:37:41 | 17:55:47 | 13:40:26 | 16:53:02 | ||||
07320 | 104 | 32 | 1042 Jul 05 | 22:26:38 | Total | 0.4145 | 1.1039 | 324.4 | 201.0 | 48.5 | 19:44:26 | 1:08:50 | 20:46:08 | 22:02:23 | 22:50:53 | 0:07:08 | |
07365 | 104 | 33 | 1060 Jul 16 | 5:37:00 | Total | 0.3417 | 1.2352 | 330.0 | 207.8 | 70.2 | 2:52:00 | 8:22:00 | 3:53:06 | 5:01:54 | 6:12:06 | 7:20:54 | |
07409 | 104 | 34 | 1078 Jul 27 | 12:50:23 | Total | 0.2721 | 1.3602 | 334.7 | 213.2 | 83.3 | 10:03:02 | 15:37:44 | 11:03:47 | 12:08:44 | 13:32:02 | 14:36:59 | |
07455 | 104 | 35 | 1096 Aug 06 | 20:07:07 | Total | 0.2060 | 1.4788 | 338.6 | 217.2 | 91.9 | 17:17:49 | 22:56:25 | 18:18:31 | 19:21:10 | 20:53:04 | 21:55:43 | |
07501 | 104 | 36 | 1114 Aug 18 | 3:29:04 | Total | 0.1451 | 1.5875 | 341.9 | 220.1 | 97.3 | 0:38:07 | 6:20:01 | 1:39:01 | 2:40:25 | 4:17:43 | 5:19:07 | |
07547 | 104 | 37 | 1132 Aug 28 | 10:55:54 | Total | 0.089 | 1.6873 | 344.6 | 222.1 | 100.6 | 8:03:36 | 13:48:12 | 9:04:51 | 10:05:36 | 11:46:12 | 12:46:57 | |
07593 | 104 | 38 | 1150 Sep 8 | 18:30:27 | Total | 0.0401 | 1.774 | 346.9 | 223.3 | 102.1 | 15:37:00 | 21:23:54 | 16:38:48 | 17:39:24 | 19:21:30 | 20:22:06 | |
07641 | 104 | 39 | 1168 Sep 19 | 2:11:28 | Total | -0.0028 | 1.8393 | 348.8 | 224 | 102.6 | 23:17:04 | 5:05:52 | 0:19:28 | 1:20:10 | 3:02:46 | 4:03:28 | |
07687 | 104 | 40 | 1186 Sep 30 | 9:59:19 | Total | -0.0392 | 1.7692 | 350.5 | 224.4 | 102.2 | 7:04:04 | 12:54:34 | 8:07:07 | 9:08:13 | 10:50:25 | 11:51:31 | |
07733 | 104 | 41 | 1204 Oct 10 | 17:54:16 | Total | -0.0691 | 1.7113 | 352.0 | 224.5 | 101.4 | 14:58:16 | 20:50:16 | 16:02:01 | 17:03:34 | 18:44:58 | 19:46:31 | |
07779 | 104 | 42 | 1222 Oct 22 | 1:56:29 | Total | -0.0919 | 1.6665 | 353.4 | 224.6 | 100.5 | 22:59:47 | 4:53:11 | 0:04:11 | 1:06:14 | 2:46:44 | 3:48:47 | |
07825 | 104 | 43 | 1240 Nov 01 | 10:04:27 | Total | -0.1096 | 1.6314 | 354.8 | 224.7 | 99.6 | 7:07:03 | 13:01:51 | 8:12:06 | 9:14:39 | 10:54:15 | 11:56:48 | |
07870 | 104 | 44 | 1258 Nov 12 | 18:16:59 | Total | -0.1227 | 1.6049 | 356.2 | 224.8 | 98.9 | 15:18:53 | 21:15:05 | 16:24:35 | 17:27:32 | 19:06:26 | 20:09:23 | |
07915 | 104 | 45 | 1276 Nov 23 | 2:33:30 | Total | -0.1316 | 1.5863 | 357.5 | 225.0 | 98.3 | 23:34:45 | 5:32:15 | 0:41:00 | 1:44:21 | 3:22:39 | 4:26:00 | |
07960 | 104 | 46 | 1294 Dec 04 | 10:52:56 | Total | -0.1372 | 1.5741 | 358.8 | 225.3 | 98.0 | 7:53:32 | 13:52:20 | 9:00:17 | 10:03:56 | 11:41:56 | 12:45:35 | |
08005 | 104 | 47 | 1312 Dec 14 | 19:11:58 | Total | -0.1424 | 1.5630 | 360.0 | 225.7 | 97.7 | 16:11:58 | 22:11:58 | 17:19:07 | 18:23:07 | 20:00:49 | 21:04:49 | |
08048 | 104 | 48 | 1330 Dec 26 | 3:30:41 | Total | -0.1471 | 1.5532 | 361.1 | 226.0 | 97.5 | 0:30:08 | 6:31:14 | 1:37:41 | 2:41:56 | 4:19:26 | 5:23:41 | |
08089 | 104 | 49 | 1349 Jan 05 | 11:45:40 | Total | -0.1541 | 1.5395 | 362.1 | 226.3 | 97.1 | 8:44:37 | 14:46:43 | 9:52:31 | 10:57:07 | 12:34:13 | 13:38:49 | |
08130 | 104 | 50 | 1367 Jan 16 | 19:57:34 | Total | -0.1629 | 1.5227 | 362.9 | 226.5 | 96.5 | 16:56:07 | 22:59:01 | 18:04:19 | 19:09:19 | 20:45:49 | 21:50:49 | |
08171 | 104 | 51 | 1385 Jan 27 | 4:01:25 | Total | -0.1775 | 1.4957 | 363.5 | 226.5 | 95.3 | 0:59:40 | 7:03:10 | 2:08:10 | 3:13:46 | 4:49:04 | 5:54:40 | |
08212 | 104 | 52 | 1403 Feb 07 | 12:00:03 | Total | -0.1958 | 1.4622 | 363.8 | 226.2 | 93.6 | 8:58:09 | 15:01:57 | 10:06:57 | 11:13:15 | 12:46:51 | 13:53:09 | |
08253 | 104 | 53 | 1421 Feb 17 | 19:48:27 | Total | -0.2216 | 1.4150 | 363.8 | 225.4 | 90.6 | 16:46:33 | 22:50:21 | 17:55:45 | 19:03:09 | 20:33:45 | 21:41:09 | |
08295 | 104 | 54 | 1439 Mar 01 | 3:28:54 | Total | -0.2536 | 1.3568 | 363.4 | 224.1 | 86.2 | 0:27:12 | 6:30:36 | 1:36:51 | 2:45:48 | 4:12:00 | 5:20:57 | |
08336 | 104 | 55 | 1457 Mar 11 | 10:57:52 | Total | -0.2944 | 1.2823 | 362.4 | 221.9 | 79.1 | 7:56:40 | 13:59:04 | 9:06:55 | 10:18:19 | 11:37:25 | 12:48:49 | |
08377 | 104 | 56 | 1475 Mar 22 | 18:18:39 | Total | -0.3413 | 1.1969 | 360.8 | 218.7 | 68.2 | 15:18:15 | 21:19:03 | 16:29:18 | 17:44:33 | 18:52:45 | 20:08:00 | |
08417 | 104 | 57 | 1493 Apr 02 | 1:28:34 | Total | -0.3964 | 1.0963 | 358.3 | 214.0 | 49.5 | 22:29:25 | 4:27:43 | 23:41:34 | 1:03:49 | 1:53:19 | 3:15:34 | |
08457 | 104 | 58 | 1511 Apr 13 | 8:29:06 | Partial | -0.4585 | 0.9828 | 354.7 | 207.5 | 5:31:45 | 11:26:27 | 6:45:21 | 10:12:51 | ||||
08498 | 104 | 59 | 1529 Apr 23 | 15:20:28 | Partial | -0.5277 | 0.8563 | 349.9 | 198.6 | 12:25:31 | 18:15:25 | 13:41:10 | 16:59:46 | ||||
08539 | 104 | 60 | 1547 May 4 | 22:04:32 | Partial | -0.6022 | 0.7198 | 343.7 | 186.8 | 19:12:41 | 0:56:23 | 20:31:08 | 23:37:56 | ||||
08583 | 104 | 61 | 1565 May 15 | 4:41:16 | Partial | -0.6820 | 0.5736 | 335.7 | 171.1 | 1:53:25 | 7:29:07 | 3:15:43 | 6:06:49 | ||||
08626 | 104 | 62 | 1583 Jun 05 | 11:12:22 | Partial | -0.7655 | 0.4203 | 325.9 | 150.3 | 8:29:25 | 13:55:19 | 9:57:13 | 12:27:31 | ||||
08669 | 104 | 63 | 1601 Jun 15 | 17:39:34 | Partial | -0.8517 | 0.2621 | 314.1 | 121.7 | 15:02:31 | 20:16:37 | 16:38:43 | 18:40:25 | ||||
08714 | 104 | 64 | 1619 Jun 27 | 0:04:48 | Partial | -0.9389 | 0.1017 | 300.2 | 77.7 | 21:34:42 | 2:34:54 | 23:25:57 | 0:43:39 | ||||
08758 | 104 | 65 | 1637 Jul 07 | 6:28:09 | Penumbral | -1.0270 | -0.0604 | 283.9 | 4:06:12 | 8:50:06 | |||||||
08802 | 104 | 66 | 1655 Jul 18 | 12:53:09 | Penumbral | -1.1131 | -0.2192 | 265.4 | 10:40:27 | 15:05:51 | |||||||
08847 | 104 | 67 | 1673 Jul 28 | 19:20:13 | Penumbral | -1.1971 | -0.3740 | 244.2 | 17:18:07 | 21:22:19 | |||||||
08893 | 104 | 68 | 1691 Aug 09 | 1:52:19 | Penumbral | -1.2766 | -0.5210 | 220.6 | 0:02:01 | 3:42:37 | |||||||
08939 | 104 | 69 | 1709 Aug 20 | 8:27:54 | Penumbral | -1.3529 | -0.6622 | 193.5 | 6:51:09 | 10:04:39 | |||||||
08986 | 104 | 70 | 1727 Aug 31 | 15:12:00 | Penumbral | -1.4223 | -0.7907 | 163.4 | 13:50:18 | 16:33:42 | |||||||
09032 | 104 | 71 | 1745 Sep 10 | 22:02:28 | Penumbral | -1.4863 | -0.9095 | 127.5 | 20:58:43 | 23:06:13 | |||||||
09079 | 104 | 72 | 1763 Sep 22 | 5:02:59 | Penumbral | -1.5421 | -1.0131 | 82.5 | 4:21:44 | 5:44:14 |
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 total lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, October 28, 2004, with an umbral magnitude of 1.3100. 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 5.4 days before apogee, the Moon's apparent diameter was smaller.
A total lunar eclipse took place on Friday, September 27, 1996, the second of two lunar eclipses in 1996, the first being on Thursday, April 4. This is the 41st member of Lunar Saros 127. The previous event is the September 1978 lunar eclipse. The next event is the October 2014 lunar eclipse.
Saros cycle series 121 for lunar eclipses occurs at the moon's descending node. It began in 1029 and will end in 2526. It contains 84 member lunar eclipses, each separated by 18 years 11 and 1/3 days, and will last 1496.5 years.
A penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Thursday, August 18, 2016, with an umbral magnitude of −0.9925. 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 3.4 days before perigee, the Moon's apparent diameter was larger.
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 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 penumbral lunar eclipse took place on Friday, July 26, 1991, the third of four lunar eclipses in 1991. This was the second member of Lunar Saros 148. The previous event was on 15 July 1973, and the first eclipse of the series. The next event was on 6 August 2009.
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 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 penumbral lunar eclipse is a lunar eclipse that occurs when the Moon becomes completely immersed in the penumbral cone of the Earth without touching the umbra.
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 100 for lunar eclipses occurred at the moon's ascending node, 18 years 11 and 1/3 days. It contained 72 events.
Saros cycle series 101 for lunar eclipses occurred at the moon's descending node, 18 years 11 and 1/3 days. It contained 72 events.
Saros cycle series 102 for lunar eclipses occurred at the moon's ascending node, 18 years 11 and 1/3 days. It contained 84 events.
Saros cycle series 103 for lunar eclipses occurred at the moon's descending node, 18 years 11 and 1/3 days. It contained at least 82 events.