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![]() 2020 Jun 05 |
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. [1]
The first total lunar eclipse of this series was on April 19, 1353, and last was on August 4, 1533. The longest occurrence of this series was on June 12, 1443 when the totality lasted 106 minutes.
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 | ||||||||
06830 | 111 | 1 | 830 Jun 10 | 6:33:54 | Penumbral | -1.5398 | -0.9806 | 63.1 | 6:02:21 | 7:05:27 | |||||||
06870 | 111 | 2 | 848 Jun 20 | 13:19:57 | Penumbral | -1.4660 | -0.8468 | 125.2 | 12:17:21 | 14:22:33 | |||||||
06911 | 111 | 3 | 866 Jul 01 | 20:03:56 | Penumbral | -1.3912 | -0.7116 | 164.7 | 18:41:35 | 21:26:17 | |||||||
06952 | 111 | 4 | 884 Jul 12 | 2:49:55 | Penumbral | -1.3183 | -0.5801 | 194.7 | 1:12:34 | 4:27:16 | |||||||
06994 | 111 | 5 | 902 Jul 23 | 9:37:09 | Penumbral | -1.2466 | -0.4510 | 219.5 | 7:47:24 | 11:26:54 | |||||||
07034 | 111 | 6 | 920 Aug 02 | 16:29:26 | Penumbral | -1.1794 | -0.3302 | 239.7 | 14:29:35 | 18:29:17 | |||||||
07075 | 111 | 7 | 938 Aug 13 | 23:26:21 | Penumbral | -1.1163 | -0.2172 | 256.7 | 21:18:00 | 1:34:42 | |||||||
07116 | 111 | 8 | 956 Aug 24 | 6:28:59 | Penumbral | -1.0582 | -0.1135 | 271.0 | 4:13:29 | 8:44:29 | |||||||
07157 | 111 | 9 | 974 Sep 04 | 13:38:51 | Penumbral | -1.0065 | -0.0215 | 282.8 | 11:17:27 | 16:00:15 | |||||||
07198 | 111 | 10 | 992 Sep 14 | 20:56:23 | Partial | -0.9615 | 0.0584 | 292.6 | 58.4 | 18:30:05 | 23:22:41 | 20:27:11 | 21:25:35 | ||||
07242 | 111 | 11 | 1010 Sep 26 | 4:21:48 | Partial | -0.9230 | 0.1262 | 300.6 | 85.2 | 1:51:30 | 6:52:06 | 3:39:12 | 5:04:24 | ||||
07287 | 111 | 12 | 1028 Oct 06 | 11:54:42 | Partial | -0.8911 | 0.1821 | 307.1 | 101.7 | 9:21:09 | 14:28:15 | 11:03:51 | 12:45:33 | ||||
07331 | 111 | 13 | 1046 Oct 17 | 19:35:27 | Partial | -0.8660 | 0.2258 | 312.2 | 112.7 | 16:59:21 | 22:11:33 | 18:39:06 | 20:31:48 | ||||
07375 | 111 | 14 | 1064 Oct 28 | 3:23:09 | Partial | -0.8469 | 0.2587 | 316.2 | 120.3 | 0:45:03 | 6:01:15 | 2:23:00 | 4:23:18 | ||||
07419 | 111 | 15 | 1082 Nov 08 | 11:16:05 | Partial | -0.8323 | 0.2835 | 319.3 | 125.6 | 8:36:26 | 13:55:44 | 10:13:17 | 12:18:53 | ||||
07465 | 111 | 16 | 1100 Nov 18 | 19:14:28 | Partial | -0.8223 | 0.3003 | 321.6 | 129.2 | 16:33:40 | 21:55:16 | 18:09:52 | 20:19:04 | ||||
07511 | 111 | 17 | 1118 Nov 30 | 3:16:19 | Partial | -0.815 | 0.3124 | 323.3 | 131.6 | 0:34:40 | 5:57:58 | 2:10:31 | 4:22:07 | ||||
07557 | 111 | 18 | 1136 Dec 10 | 11:19:58 | Partial | -0.8096 | 0.3216 | 324.6 | 133.5 | 8:37:40 | 14:02:16 | 10:13:13 | 12:26:43 | ||||
07604 | 111 | 19 | 1154 Dec 21 | 19:22:51 | Partial | -0.8036 | 0.3322 | 325.9 | 135.6 | 16:39:54 | 22:05:48 | 18:15:03 | 20:30:39 | ||||
07652 | 111 | 20 | 1173 Jan 1 | 3:24:43 | Partial | -0.7967 | 0.3448 | 327.1 | 138 | 0:41:10 | 6:08:16 | 2:15:43 | 4:33:43 | ||||
07698 | 111 | 21 | 1191 Jan 12 | 11:23:18 | Partial | -0.7869 | 0.3631 | 328.6 | 141.3 | 8:39:00 | 14:07:36 | 10:12:39 | 12:33:57 | ||||
07744 | 111 | 22 | 1209 Jan 22 | 19:16:05 | Partial | -0.7725 | 0.3903 | 330.5 | 146.0 | 16:30:50 | 22:01:20 | 18:03:05 | 20:29:05 | ||||
07790 | 111 | 23 | 1227 Feb 03 | 3:02:49 | Partial | -0.7531 | 0.4269 | 333.0 | 151.9 | 0:16:19 | 5:49:19 | 1:46:52 | 4:18:46 | ||||
07835 | 111 | 24 | 1245 Feb 13 | 10:41:36 | Partial | -0.7272 | 0.4757 | 336.0 | 159.1 | 7:53:36 | 13:29:36 | 9:22:03 | 12:01:09 | ||||
07880 | 111 | 25 | 1263 Feb 24 | 18:12:42 | Partial | -0.6950 | 0.5364 | 339.5 | 167.4 | 15:22:57 | 21:02:27 | 16:49:00 | 19:36:24 | ||||
07925 | 111 | 26 | 1281 Mar 07 | 1:33:37 | Partial | -0.6542 | 0.6128 | 343.6 | 176.7 | 22:41:49 | 4:25:25 | 0:05:16 | 3:01:58 | ||||
07970 | 111 | 27 | 1299 Mar 18 | 8:46:35 | Partial | -0.6068 | 0.7016 | 348.0 | 186.2 | 5:52:35 | 11:40:35 | 7:13:29 | 10:19:41 | ||||
08014 | 111 | 28 | 1317 Mar 28 | 15:49:55 | Partial | -0.5516 | 0.8048 | 352.6 | 195.8 | 12:53:37 | 18:46:13 | 14:12:01 | 17:27:49 | ||||
08057 | 111 | 29 | 1335 Apr 08 | 22:45:02 | Partial | -0.4893 | 0.9209 | 357.1 | 205.0 | 19:46:29 | 1:43:35 | 21:02:32 | 0:27:32 | ||||
08099 | 111 | 30 | 1353 Apr 19 | 5:32:00 | Total | -0.4201 | 1.0498 | 361.4 | 213.5 | 36.4 | 2:31:18 | 8:32:42 | 3:45:15 | 5:13:48 | 5:50:12 | 7:18:45 | |
08140 | 111 | 31 | 1371 Apr 30 | 12:13:03 | Total | -0.3457 | 1.1879 | 365.0 | 220.9 | 67.6 | 9:10:33 | 15:15:33 | 10:22:36 | 11:39:15 | 12:46:51 | 14:03:30 | |
08181 | 111 | 32 | 1389 May 10 | 18:48:43 | Total | -0.2665 | 1.3350 | 367.9 | 226.8 | 85.6 | 15:44:46 | 21:52:40 | 16:55:19 | 18:05:55 | 19:31:31 | 20:42:07 | |
08222 | 111 | 33 | 1407 May 22 | 1:19:29 | Total | -0.1827 | 1.4902 | 369.9 | 231.2 | 97.2 | 22:14:32 | 4:24:26 | 23:23:53 | 0:30:53 | 2:08:05 | 3:15:05 | |
08263 | 111 | 34 | 1425 Jun 01 | 7:48:18 | Total | -0.0970 | 1.6488 | 370.9 | 233.8 | 103.8 | 4:42:51 | 10:53:45 | 5:51:24 | 6:56:24 | 8:40:12 | 9:45:12 | |
08305 | 111 | 35 | 1443 Jun 12 | 14:15:52 | Total | -0.0098 | 1.8097 | 370.7 | 234.6 | 106.2 | 11:10:31 | 17:21:13 | 12:18:34 | 13:22:46 | 15:08:58 | 16:13:10 | |
08346 | 111 | 36 | 1461 Jun 22 | 20:44:43 | Total | 0.0770 | 1.6874 | 369.4 | 233.5 | 104.6 | 17:40:01 | 23:49:25 | 18:47:58 | 19:52:25 | 21:37:01 | 22:41:28 | |
08386 | 111 | 37 | 1479 Jul 04 | 3:14:45 | Total | 0.1634 | 1.5297 | 366.9 | 230.6 | 98.8 | 0:11:18 | 6:18:12 | 1:19:27 | 2:25:21 | 4:04:09 | 5:10:03 | |
08426 | 111 | 38 | 1497 Jul 14 | 9:49:55 | Total | 0.2462 | 1.3783 | 363.5 | 226.1 | 88.8 | 6:48:10 | 12:51:40 | 7:56:52 | 9:05:31 | 10:34:19 | 11:42:58 | |
08466 | 111 | 39 | 1515 Jul 25 | 16:29:57 | Total | 0.3252 | 1.2336 | 359.2 | 220.1 | 73.4 | 13:30:21 | 19:29:33 | 14:39:54 | 15:53:15 | 17:06:39 | 18:20:00 | |
08507 | 111 | 40 | 1533 Aug 04 | 23:16:00 | Total | 0.3999 | 1.0967 | 354.1 | 212.8 | 49.4 | 20:18:57 | 2:13:03 | 21:29:36 | 22:51:18 | 23:40:42 | 1:02:24 | |
08549 | 111 | 41 | 1551 Aug 16 | 6:09:51 | Partial | 0.4688 | 0.9702 | 348.7 | 204.5 | 3:15:30 | 9:04:12 | 4:27:36 | 7:52:06 | ||||
08593 | 111 | 42 | 1569 Aug 26 | 13:12:21 | Partial | 0.5313 | 0.8556 | 342.9 | 195.6 | 10:20:54 | 16:03:48 | 11:34:33 | 14:50:09 | ||||
08636 | 111 | 43 | 1587 Sep 16 | 20:25:05 | Partial | 0.5857 | 0.7555 | 337.3 | 186.6 | 17:36:26 | 23:13:44 | 18:51:47 | 21:58:23 | ||||
08679 | 111 | 44 | 1605 Sep 27 | 3:46:02 | Partial | 0.6341 | 0.6666 | 331.8 | 177.4 | 1:00:08 | 6:31:56 | 2:17:20 | 5:14:44 | ||||
08724 | 111 | 45 | 1623 Oct 08 | 11:18:42 | Partial | 0.6734 | 0.5941 | 326.8 | 169.1 | 8:35:18 | 14:02:06 | 9:54:09 | 12:43:15 | ||||
08768 | 111 | 46 | 1641 Oct 18 | 19:00:25 | Partial | 0.7062 | 0.5340 | 322.2 | 161.4 | 16:19:19 | 21:41:31 | 17:39:43 | 20:21:07 | ||||
08813 | 111 | 47 | 1659 Oct 30 | 2:52:52 | Partial | 0.7310 | 0.4885 | 318.4 | 155.1 | 0:13:40 | 5:32:04 | 1:35:19 | 4:10:25 | ||||
08858 | 111 | 48 | 1677 Nov 09 | 10:52:40 | Partial | 0.7504 | 0.4529 | 315.1 | 149.7 | 8:15:07 | 13:30:13 | 9:37:49 | 12:07:31 | ||||
08904 | 111 | 49 | 1695 Nov 20 | 19:02:06 | Partial | 0.7629 | 0.4303 | 312.6 | 146.0 | 16:25:48 | 21:38:24 | 17:49:06 | 20:15:06 | ||||
08950 | 111 | 50 | 1713 Dec 02 | 3:17:09 | Partial | 0.7716 | 0.4149 | 310.5 | 143.4 | 0:41:54 | 5:52:24 | 2:05:27 | 4:28:51 | ||||
08997 | 111 | 51 | 1731 Dec 13 | 11:38:06 | Partial | 0.7764 | 0.4069 | 308.8 | 141.7 | 9:03:42 | 14:12:30 | 10:27:15 | 12:48:57 | ||||
09044 | 111 | 52 | 1749 Dec 23 | 20:02:11 | Partial | 0.7796 | 0.4023 | 307.3 | 140.6 | 17:28:32 | 22:35:50 | 18:51:53 | 21:12:29 | ||||
09091 | 111 | 53 | 1768 Jan 04 | 4:29:31 | Partial | 0.7810 | 0.4011 | 305.9 | 140.1 | 1:56:34 | 7:02:28 | 3:19:28 | 5:39:34 | ||||
09136 | 111 | 54 | 1786 Jan 14 | 12:55:56 | Partial | 0.7838 | 0.3978 | 304.2 | 139.1 | 10:23:50 | 15:28:02 | 11:46:23 | 14:05:29 | ||||
09181 | 111 | 55 | 1804 Jan 26 | 21:21:21 | Partial | 0.7882 | 0.3918 | 302.3 | 137.8 | 18:50:12 | 23:52:30 | 20:12:27 | 22:30:15 | ||||
09226 | 111 | 56 | 1822 Feb 06 | 5:43:26 | Partial | 0.7961 | 0.3797 | 299.9 | 135.6 | 3:13:29 | 8:13:23 | 4:35:38 | 6:51:14 | ||||
09272 | 111 | 57 | 1840 Feb 17 | 14:02:34 | Partial | 0.8074 | 0.3615 | 297.0 | 132.3 | 11:34:04 | 16:31:04 | 12:56:25 | 15:08:43 | ||||
09317 | 111 | 58 | 1858 Feb 27 | 22:14:20 | Partial | 0.8252 | 0.3316 | 293.0 | 126.9 | 19:47:50 | 0:40:50 | 21:10:53 | 23:17:47 | ||||
09361 | 111 | 59 | 1876 Mar 10 | 6:21:31 | Partial | 0.8474 | 0.2937 | 288.4 | 119.7 | 3:57:19 | 8:45:43 | 5:21:40 | 7:21:22 | ||||
09405 | 111 | 60 | 1894 Mar 21 | 14:20:27 | Partial | 0.8770 | 0.2424 | 282.6 | 109.3 | 11:59:09 | 16:41:45 | 13:25:48 | 15:15:06 | ||||
09447 | 111 | 61 | 1912 Apr 01 | 22:14:16 | Partial | 0.9116 | 0.1820 | 275.8 | 95.2 | 19:56:22 | 0:32:10 | 21:26:40 | 23:01:52 | ||||
09489 | 111 | 62 | 1930 Apr 13 | 5:58:54 | Partial | 0.9545 | 0.1064 | 267.3 | 73.4 | 3:45:15 | 8:12:33 | 5:22:12 | 6:35:36 | ||||
09531 | 111 | 63 | 1948 Apr 23 | 13:39:18 | Partial | 1.0016 | 0.0229 | 257.6 | 34.3 | 11:30:30 | 15:48:06 | 13:22:09 | 13:56:27 | ||||
09572 | 111 | 64 | 1966 May 04 | 21:12:06 | Penumbral | 1.0553 | -0.0728 | 246.0 | 19:09:06 | 23:15:06 | |||||||
09613 | 111 | 65 | 1984 May 15 | 4:41:03 | Penumbral | 1.1130 | -0.1760 | 232.5 | 2:44:48 | 6:37:18 | |||||||
09654 | 111 | 66 | 2002 May 26 | 12:04:26 | Penumbral | 1.1758 | -0.2888 | 216.6 | 10:16:08 | 13:52:44 | |||||||
09695 | 111 | 67 | 2020 Jun 05 | 19:26:14 | Penumbral | 1.2406 | -0.4053 | 198.2 | 17:47:08 | 21:05:20 | |||||||
09736 | 111 | 68 | 2038 Jun 17 | 2:45:02 | Penumbral | 1.3082 | -0.5275 | 176.3 | 1:16:53 | 4:13:11 | |||||||
09776 | 111 | 69 | 2056 Jun 27 | 10:03:09 | Penumbral | 1.3769 | -0.6519 | 149.9 | 8:48:12 | 11:18:06 | |||||||
09817 | 111 | 70 | 2074 Jul 08 | 17:21:38 | Penumbral | 1.4456 | -0.7765 | 116.6 | 16:23:20 | 18:19:56 | |||||||
09858 | 111 | 71 | 2092 Jul 19 | 0:41:58 | Penumbral | 1.5131 | -0.8992 | 67.7 | 0:08:07 | 1:15:49 |
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 took place on Friday, February 9, 1990, the first of two lunar eclipses in 1990.
A penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Sunday, May 26, 2002, with an umbral magnitude of −0.2871. 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 3.1 days after perigee, the Moon's apparent diameter was larger.
A total lunar eclipse took place on Monday, February 20, 1989, the first of two total lunar eclipses in 1989.
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 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 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 penumbral lunar eclipse will occur at the Moon’s descending node of orbit on Thursday, June 17, 2038, with an umbral magnitude of −0.5259. 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 2.7 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 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 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 will occur at the Moon’s descending node of orbit on Monday, June 28, 2094, with an umbral magnitude of 1.8249. 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.
Saros cycle series 111 for solar eclipses occurred at the Moon's ascending node, repeating every 18 years and 11 days, containing 79 eclipses, 42 of which were umbral. The first eclipse was on 30 August 528 and the last was on 5 Jan 1935. The longest totality was 6 minutes 11 seconds on 9 June 1592 and the longest annular eclipse was 3 minutes 4 seconds on 15 April 907.
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 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 104 for lunar eclipses occurred at the moon's ascending node, 18 years 11 and 1/3 days. It contained 72 events.