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2006 Mar 14 | 2024 Mar 25 |
Saros cycle series 113 for lunar eclipses occurs at the moon's descending node, repeats every 18 years 11 and 1/3 days. It contains 71 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 | ||||||||
06961 | 113 | 1 | 888 Apr 29 | 19:18:38 | Penumbral | -1.5015 | -0.8702 | 72.8 | 18:42:14 | 19:55:02 | |||||||
07003 | 113 | 2 | 906 May 11 | 2:52:46 | Penumbral | -1.4355 | -0.7479 | 115.9 | 1:54:49 | 3:50:43 | |||||||
07043 | 113 | 3 | 924 May 21 | 10:22:51 | Penumbral | -1.3660 | -0.6195 | 146.9 | 9:09:24 | 11:36:18 | |||||||
07084 | 113 | 4 | 942 Jun 01 | 17:51:08 | Penumbral | -1.2946 | -0.4880 | 172.0 | 16:25:08 | 19:17:08 | |||||||
07125 | 113 | 5 | 960 Jun 12 | 1:18:14 | Penumbral | -1.2222 | -0.3550 | 193.0 | 23:41:44 | 2:54:44 | |||||||
07166 | 113 | 6 | 978 Jun 23 | 8:46:20 | Penumbral | -1.1506 | -0.2237 | 210.8 | 7:00:56 | 10:31:44 | |||||||
07208 | 113 | 7 | 996 Jul 03 | 16:14:11 | Penumbral | -1.0788 | -0.0924 | 226.4 | 14:20:59 | 18:07:23 | |||||||
07252 | 113 | 8 | 1014 Jul 14 | 23:45:44 | Partial | -1.0101 | 0.0329 | 239.7 | 39.3 | 21:45:53 | 1:45:35 | 23:26:05 | 0:05:23 | ||||
07296 | 113 | 9 | 1032 Jul 25 | 7:19:48 | Partial | -0.9439 | 0.1534 | 251.2 | 83.6 | 5:14:12 | 9:25:24 | 6:38:00 | 8:01:36 | ||||
07341 | 113 | 10 | 1050 Aug 05 | 14:59:51 | Partial | -0.8826 | 0.2645 | 261.0 | 108.2 | 12:49:21 | 17:10:21 | 14:05:45 | 15:53:57 | ||||
07385 | 113 | 11 | 1068 Aug 15 | 22:43:39 | Partial | -0.8248 | 0.3689 | 269.4 | 125.9 | 20:28:57 | 0:58:21 | 21:40:42 | 23:46:36 | ||||
07429 | 113 | 12 | 1086 Aug 27 | 6:35:39 | Partial | -0.7742 | 0.4600 | 276.3 | 138.8 | 4:17:30 | 8:53:48 | 5:26:15 | 7:45:03 | ||||
07475 | 113 | 13 | 1104 Sep 6 | 14:33:30 | Partial | -0.7288 | 0.5414 | 282.3 | 148.9 | 12:12:21 | 16:54:39 | 13:19:03 | 15:47:57 | ||||
07521 | 113 | 14 | 1122 Sep 17 | 22:39:18 | Partial | -0.6902 | 0.6101 | 287.1 | 156.5 | 20:15:45 | 1:02:51 | 21:21:03 | 23:57:33 | ||||
07567 | 113 | 15 | 1140 Sep 28 | 6:51:51 | Partial | -0.6576 | 0.6678 | 291.2 | 162.4 | 4:26:15 | 9:17:27 | 5:30:39 | 8:13:03 | ||||
07614 | 113 | 16 | 1158 Oct 9 | 15:12:42 | Partial | -0.632 | 0.7127 | 294.5 | 166.8 | 12:45:27 | 17:39:57 | 13:49:18 | 16:36:06 | ||||
07661 | 113 | 17 | 1176 Oct 19 | 23:40:14 | Partial | -0.6126 | 0.7462 | 297.1 | 169.9 | 21:11:41 | 2:08:47 | 22:15:17 | 1:05:11 | ||||
07707 | 113 | 18 | 1194 Oct 31 | 8:13:30 | Partial | -0.5981 | 0.7709 | 299.3 | 172.2 | 5:43:51 | 10:43:09 | 6:47:24 | 9:39:36 | ||||
07753 | 113 | 19 | 1212 Nov 10 | 16:52:49 | Partial | -0.5890 | 0.7856 | 300.9 | 173.7 | 14:22:22 | 19:23:16 | 15:25:58 | 18:19:40 | ||||
07800 | 113 | 20 | 1230 Nov 22 | 1:36:20 | Partial | -0.5834 | 0.7943 | 302.3 | 174.7 | 23:05:11 | 4:07:29 | 0:08:59 | 3:03:41 | ||||
07845 | 113 | 21 | 1248 Dec 02 | 10:22:46 | Partial | -0.5810 | 0.7974 | 303.4 | 175.3 | 7:51:04 | 12:54:28 | 8:55:07 | 11:50:25 | ||||
07890 | 113 | 22 | 1266 Dec 13 | 19:09:37 | Partial | -0.5792 | 0.7995 | 304.4 | 175.8 | 16:37:25 | 21:41:49 | 17:41:43 | 20:37:31 | ||||
07935 | 113 | 23 | 1284 Dec 24 | 3:56:38 | Partial | -0.5781 | 0.8005 | 305.3 | 176.2 | 1:23:59 | 6:29:17 | 2:28:32 | 5:24:44 | ||||
07980 | 113 | 24 | 1303 Jan 04 | 12:41:28 | Partial | -0.5756 | 0.8044 | 306.4 | 176.9 | 10:08:16 | 15:14:40 | 11:13:01 | 14:09:55 | ||||
08023 | 113 | 25 | 1321 Jan 14 | 21:22:17 | Partial | -0.5704 | 0.8135 | 307.6 | 178.0 | 18:48:29 | 23:56:05 | 19:53:17 | 22:51:17 | ||||
08065 | 113 | 26 | 1339 Jan 26 | 5:58:09 | Partial | -0.5615 | 0.8295 | 309.2 | 179.7 | 3:23:33 | 8:32:45 | 4:28:18 | 7:28:00 | ||||
08107 | 113 | 27 | 1357 Feb 05 | 14:27:27 | Partial | -0.5479 | 0.8542 | 311.1 | 182.1 | 11:51:54 | 17:03:00 | 12:56:24 | 15:58:30 | ||||
08148 | 113 | 28 | 1375 Feb 16 | 22:49:15 | Partial | -0.5287 | 0.8894 | 313.5 | 185.1 | 20:12:30 | 1:26:00 | 21:16:42 | 0:21:48 | ||||
08189 | 113 | 29 | 1393 Feb 27 | 7:02:14 | Partial | -0.5028 | 0.9370 | 316.3 | 188.9 | 4:24:05 | 9:40:23 | 5:27:47 | 8:36:41 | ||||
08230 | 113 | 30 | 1411 Mar 10 | 15:06:37 | Partial | -0.4704 | 0.9965 | 319.5 | 193.3 | 12:26:52 | 17:46:22 | 13:29:58 | 16:43:16 | ||||
08272 | 113 | 31 | 1429 Mar 20 | 23:02:11 | Total | -0.4312 | 1.0683 | 323.0 | 198.1 | 39.5 | 20:20:41 | 1:43:41 | 21:23:08 | 22:42:26 | 23:21:56 | 0:41:14 | |
08314 | 113 | 32 | 1447 Apr 01 | 6:47:26 | Total | -0.3842 | 1.1546 | 326.8 | 203.2 | 58.1 | 4:04:02 | 9:30:50 | 5:05:50 | 6:18:23 | 7:16:29 | 8:29:02 | |
08355 | 113 | 33 | 1465 Apr 11 | 14:24:28 | Total | -0.3312 | 1.2517 | 330.6 | 208.2 | 72.0 | 11:39:10 | 17:09:46 | 12:40:22 | 13:48:28 | 15:00:28 | 16:08:34 | |
08395 | 113 | 34 | 1483 Apr 22 | 21:52:19 | Total | -0.2713 | 1.3612 | 334.4 | 212.9 | 83.2 | 19:05:07 | 0:39:31 | 20:05:52 | 21:10:43 | 22:33:55 | 23:38:46 | |
08435 | 113 | 35 | 1501 May 3 | 5:13:26 | Total | -0.2064 | 1.4797 | 337.8 | 217.0 | 91.9 | 2:24:32 | 8:02:20 | 3:24:56 | 4:27:29 | 5:59:23 | 7:01:56 | |
08475 | 113 | 36 | 1519 May 14 | 12:25:26 | Total | -0.1349 | 1.6101 | 340.8 | 220.4 | 98.3 | 9:35:02 | 15:15:50 | 10:35:14 | 11:36:17 | 13:14:35 | 14:15:38 | |
08516 | 113 | 37 | 1537 May 24 | 19:33:13 | Total | -0.0608 | 1.7451 | 343.3 | 222.7 | 102.1 | 16:41:34 | 22:24:52 | 17:41:52 | 18:42:10 | 20:24:16 | 21:24:34 | |
08558 | 113 | 38 | 1555 Jun 05 | 2:34:54 | Total | 0.0172 | 1.8238 | 345.0 | 223.7 | 103.1 | 23:42:24 | 5:27:24 | 0:43:03 | 1:43:21 | 3:26:27 | 4:26:45 | |
08601 | 113 | 39 | 1573 Jun 15 | 9:34:00 | Total | 0.0964 | 1.6770 | 345.9 | 223.4 | 101.1 | 6:41:03 | 12:26:57 | 7:42:18 | 8:43:27 | 10:24:33 | 11:25:42 | |
08644 | 113 | 40 | 1591 Jul 06 | 16:29:29 | Total | 0.1776 | 1.5260 | 345.9 | 221.6 | 95.7 | 13:36:32 | 19:22:26 | 14:38:41 | 15:41:38 | 17:17:20 | 18:20:17 | |
08688 | 113 | 41 | 1609 Jul 16 | 23:25:49 | Total | 0.2570 | 1.3783 | 345.0 | 218.3 | 86.3 | 20:33:19 | 2:18:19 | 21:36:40 | 22:42:40 | 0:08:58 | 1:14:58 | |
08733 | 113 | 42 | 1627 Jul 28 | 6:21:40 | Total | 0.3356 | 1.2317 | 343.3 | 213.5 | 71.4 | 3:30:01 | 9:13:19 | 4:34:55 | 5:45:58 | 6:57:22 | 8:08:25 | |
08777 | 113 | 43 | 1645 Aug 07 | 13:19:26 | Total | 0.4115 | 1.0899 | 340.8 | 207.1 | 46.7 | 10:29:02 | 16:09:50 | 11:35:53 | 12:56:05 | 13:42:47 | 15:02:59 | |
08822 | 113 | 44 | 1663 Aug 18 | 20:20:08 | Partial | 0.4840 | 0.9543 | 337.6 | 199.4 | 17:31:20 | 23:08:56 | 18:40:26 | 21:59:50 | ||||
08868 | 113 | 45 | 1681 Aug 29 | 3:25:58 | Partial | 0.5511 | 0.8282 | 334.0 | 190.6 | 0:38:58 | 6:12:58 | 1:50:40 | 5:01:16 | ||||
08914 | 113 | 46 | 1699 Sep 09 | 10:37:10 | Partial | 0.6130 | 0.7117 | 330.0 | 180.7 | 7:52:10 | 13:22:10 | 9:06:49 | 12:07:31 | ||||
08960 | 113 | 47 | 1717 Sep 20 | 17:54:25 | Partial | 0.6690 | 0.6059 | 325.9 | 170.2 | 15:11:28 | 20:37:22 | 16:29:19 | 19:19:31 | ||||
09007 | 113 | 48 | 1735 Oct 02 | 1:19:13 | Partial | 0.7178 | 0.5134 | 322.1 | 159.4 | 22:38:10 | 4:00:16 | 23:59:31 | 2:38:55 | ||||
09054 | 113 | 49 | 1753 Oct 12 | 8:51:29 | Partial | 0.7597 | 0.4333 | 318.5 | 148.7 | 6:12:14 | 11:30:44 | 7:37:08 | 10:05:50 | ||||
09100 | 113 | 50 | 1771 Oct 23 | 16:30:23 | Partial | 0.7955 | 0.3649 | 315.3 | 138.3 | 13:52:44 | 19:08:02 | 15:21:14 | 17:39:32 | ||||
09145 | 113 | 51 | 1789 Nov 03 | 0:17:06 | Partial | 0.8242 | 0.3094 | 312.7 | 128.7 | 21:40:45 | 2:53:27 | 23:12:45 | 1:21:27 | ||||
09190 | 113 | 52 | 1807 Nov 15 | 8:09:59 | Partial | 0.8473 | 0.2646 | 310.7 | 120.1 | 5:34:38 | 10:45:20 | 7:09:56 | 9:10:02 | ||||
09235 | 113 | 53 | 1825 Nov 25 | 16:09:25 | Partial | 0.8643 | 0.2311 | 309.4 | 113.0 | 13:34:43 | 18:44:07 | 15:12:55 | 17:05:55 | ||||
09282 | 113 | 54 | 1843 Dec 07 | 0:11:31 | Partial | 0.8785 | 0.2031 | 308.3 | 106.6 | 21:37:22 | 2:45:40 | 23:18:13 | 1:04:49 | ||||
09327 | 113 | 55 | 1861 Dec 17 | 8:18:43 | Partial | 0.8880 | 0.1840 | 307.8 | 101.9 | 5:44:49 | 10:52:37 | 7:27:46 | 9:09:40 | ||||
09371 | 113 | 56 | 1879 Dec 28 | 16:26:22 | Partial | 0.8969 | 0.1664 | 307.2 | 97.4 | 13:52:46 | 18:59:58 | 15:37:40 | 17:15:04 | ||||
09415 | 113 | 57 | 1898 Jan 08 | 0:34:46 | Partial | 0.9046 | 0.1515 | 306.7 | 93.3 | 22:01:25 | 3:08:07 | 23:48:07 | 1:21:25 | ||||
09457 | 113 | 58 | 1916 Jan 20 | 8:39:41 | Partial | 0.9146 | 0.1327 | 305.7 | 87.7 | 6:06:50 | 11:12:32 | 7:55:50 | 9:23:32 | ||||
09499 | 113 | 59 | 1934 Jan 30 | 16:42:42 | Partial | 0.9258 | 0.1120 | 304.3 | 80.9 | 14:10:33 | 19:14:51 | 16:02:15 | 17:23:09 | ||||
09540 | 113 | 60 | 1952 Feb 11 | 0:39:48 | Partial | 0.9416 | 0.0832 | 301.9 | 70.1 | 22:08:51 | 3:10:45 | 0:04:45 | 1:14:51 | ||||
09581 | 113 | 61 | 1970 Feb 21 | 8:30:43 | Partial | 0.9619 | 0.0463 | 298.5 | 52.7 | 6:01:28 | 10:59:58 | 8:04:22 | 8:57:04 | ||||
09622 | 113 | 62 | 1988 Mar 03 | 16:13:41 | Penumbral | 0.9885 | -0.0017 | 293.8 | 13:46:47 | 18:40:35 | |||||||
09663 | 113 | 63 | 2006 Mar 14 | 23:48:34 | Penumbral | 1.0210 | -0.0604 | 287.5 | 21:24:49 | 2:12:19 | |||||||
09704 | 113 | 64 | 2024 Mar 25 | 7:13:59 | Penumbral | 1.0609 | -0.1325 | 279.1 | 4:54:26 | 9:33:32 | |||||||
09745 | 113 | 65 | 2042 Apr 05 | 14:30:11 | Penumbral | 1.1080 | -0.2176 | 268.4 | 12:15:59 | 16:44:23 | |||||||
09785 | 113 | 66 | 2060 Apr 15 | 21:37:04 | Penumbral | 1.1621 | -0.3156 | 255.0 | 19:29:34 | 23:44:34 | |||||||
09826 | 113 | 67 | 2078 Apr 27 | 4:35:44 | Penumbral | 1.2222 | -0.4246 | 238.2 | 2:36:38 | 6:34:50 | |||||||
09867 | 113 | 68 | 2096 May 07 | 11:24:42 | Penumbral | 1.2896 | -0.5469 | 216.9 | 9:36:15 | 13:13:09 | |||||||
09909 | 113 | 69 | 2114 May 19 | 18:07:33 | Penumbral | 1.3611 | -0.6770 | 190.1 | 16:32:30 | 19:42:36 | |||||||
09951 | 113 | 70 | 2132 May 30 | 0:42:50 | Penumbral | 1.4380 | -0.8169 | 154.4 | 23:25:38 | 2:00:02 | |||||||
09995 | 113 | 71 | 2150 Jun 10 | 7:14:48 | Penumbral | 1.5171 | -0.9612 | 102.4 | 6:23:36 | 8:06:00 |
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 take place on May 26, 2040. The northern limb of the Moon will pass through the center of the Earth's shadow. This is the second central lunar eclipse of Saros series 131. This lunar event will occur near perigee, as a result, it will be referred to as a "super flower blood moon" or "super blood moon", though not quite as close to Earth as the eclipse of May 26, 2021.
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 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 penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Monday, March 25, 2024, with an umbral magnitude of −0.1304. 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 before apogee, the Moon's apparent diameter was smaller.
A total lunar eclipse took place on Sunday, April 2, 1950. This was the first total lunar eclipse of Saros cycle 131.
A total lunar eclipse will take place on June 6, 2058. The Moon will pass through the center of the Earth's shadow.
A total lunar eclipse will take place on June 17, 2076. The moon will pass through the center of the Earth's shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red color at maximum eclipse. With a gamma value of only −0.0452 and an umbral eclipse magnitude of 1.7943, this is the second greatest eclipse in Saros series 131 as well as the largest and darkest lunar eclipse between June 26, 2029 and June 28, 2094. Overall, it will be the third largest and darkest lunar eclipse of the 21st century. While it will have similar values to the lunar eclipse of July 16, 2000, totality will not last over 106 minutes due to the moon's relatively large apparent size as seen from Earth and greater speed in its elliptical orbit. Totality's expected to last 100 minutes 34 seconds from 9:11:39 to 10:52:15 with the greatest point at 10:01:57 UTC.
A total lunar eclipse will take place on June 28, 2094. The Moon will pass through the center of the Earth's shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red color at maximum eclipse. With a gamma value of only 0.0288 and an umbral eclipse magnitude of 1.8234, this is the greatest eclipse in Saros series 131 as well as the second largest and darkest lunar eclipse of the 21st century.
A partial lunar eclipse took place on Thursday, March 12, 1914.
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 total lunar eclipse took place on Sunday, March 13, 1960. The moon passed through the center of the Earth's shadow.
A total lunar eclipse will take place on September 19, 2043.
Saros cycle series 113 for solar eclipses occurred at the Moon's ascending node, repeating every 18 years, 11 days, contained 71 eclipses, 40 of which were umbral, all annular. The first eclipse was on 22 July 586 and the last was on 28 August 1848. The eclipse with the longest duration was 9 minutes 32 seconds on 20 November 1397.
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 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.