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Saros cycle series 141 for lunar eclipses occurs at the moon's descending node, repeats every 18 years 11 and 1/3 days. It contains 72 events. [1]
This lunar saros is linked to Solar Saros 148.
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 | ||||||||
08686 | 141 | 1 | 1608 Aug 25 | 19:20:07 | Penumbral | -1.5413 | -0.9471 | 21.1 | 19:09:34 | 19:30:40 | |||||||
08731 | 141 | 2 | 1626 Sep 06 | 3:05:57 | Penumbral | -1.4897 | -0.8544 | 85.7 | 2:23:06 | 3:48:48 | |||||||
08775 | 141 | 3 | 1644 Sep 16 | 10:59:45 | Penumbral | -1.4448 | -0.7742 | 115.0 | 10:02:15 | 11:57:15 | |||||||
08820 | 141 | 4 | 1662 Sep 27 | 18:59:20 | Penumbral | -1.4052 | -0.7037 | 135.6 | 17:51:32 | 20:07:08 | |||||||
08866 | 141 | 5 | 1680 Oct 08 | 3:06:25 | Penumbral | -1.3719 | -0.6450 | 150.6 | 1:51:07 | 4:21:43 | |||||||
08912 | 141 | 6 | 1698 Oct 19 | 11:20:30 | Penumbral | -1.3447 | -0.5973 | 161.9 | 9:59:33 | 12:41:27 | |||||||
08958 | 141 | 7 | 1716 Oct 30 | 19:42:19 | Penumbral | -1.3238 | -0.5613 | 170.2 | 18:17:13 | 21:07:25 | |||||||
09005 | 141 | 8 | 1734 Nov 11 | 4:10:31 | Penumbral | -1.3088 | -0.5360 | 176.2 | 2:42:25 | 5:38:37 | |||||||
09052 | 141 | 9 | 1752 Nov 21 | 12:43:58 | Penumbral | -1.2983 | -0.5189 | 180.5 | 11:13:43 | 14:14:13 | |||||||
09098 | 141 | 10 | 1770 Dec 02 | 21:22:32 | Penumbral | -1.2926 | -0.5104 | 183.2 | 19:50:56 | 22:54:08 | |||||||
09143 | 141 | 11 | 1788 Dec 13 | 6:04:27 | Penumbral | -1.2898 | -0.5069 | 185.0 | 4:31:57 | 7:36:57 | |||||||
09188 | 141 | 12 | 1806 Dec 25 | 14:48:04 | Penumbral | -1.2891 | -0.5071 | 186.0 | 13:15:04 | 16:21:04 | |||||||
09233 | 141 | 13 | 1825 Jan 04 | 23:31:53 | Penumbral | -1.2890 | -0.5081 | 186.8 | 21:58:29 | 1:05:17 | |||||||
09279 | 141 | 14 | 1843 Jan 16 | 8:14:24 | Penumbral | -1.2885 | -0.5083 | 187.7 | 6:40:33 | 9:48:15 | |||||||
09324 | 141 | 15 | 1861 Jan 26 | 16:54:03 | Penumbral | -1.2864 | -0.5052 | 189.0 | 15:19:33 | 18:28:33 | |||||||
09368 | 141 | 16 | 1879 Feb 07 | 1:28:35 | Penumbral | -1.2809 | -0.4956 | 191.4 | 23:52:53 | 3:04:17 | |||||||
09412 | 141 | 17 | 1897 Feb 17 | 9:57:44 | Penumbral | -1.2717 | -0.4790 | 194.8 | 8:20:20 | 11:35:08 | |||||||
09454 | 141 | 18 | 1915 Mar 01 | 18:19:32 | Penumbral | -1.2573 | -0.4528 | 199.8 | 16:39:38 | 19:59:26 | |||||||
09496 | 141 | 19 | 1933 Mar 12 | 2:33:03 | Penumbral | -1.2369 | -0.4154 | 206.3 | 0:49:54 | 4:16:12 | |||||||
09537 | 141 | 20 | 1951 Mar 23 | 10:37:33 | Penumbral | -1.2099 | -0.3661 | 214.3 | 8:50:24 | 12:24:42 | |||||||
09578 | 141 | 21 | 1969 Apr 02 | 18:33:06 | Penumbral | -1.1764 | -0.3047 | 223.7 | 16:41:15 | 20:24:57 | |||||||
09620 | 141 | 22 | 1987 Apr 14 | 2:19:50 | Penumbral | -1.1364 | -0.2313 | 234.1 | 0:22:47 | 4:16:53 | |||||||
09661 | 141 | 23 | 2005 Apr 24 | 9:55:55 | Penumbral | -1.0885 | -0.1436 | 245.6 | 7:53:07 | 11:58:43 | |||||||
09702 | 141 | 24 | 2023 May 05 | 17:24:05 | Penumbral | -1.0349 | -0.0457 | 257.5 | 15:15:20 | 19:32:50 | |||||||
09743 | 141 | 25 | 2041 May 16 | 0:43:03 | Partial | -0.9746 | 0.0645 | 269.7 | 58.5 | 22:28:12 | 2:57:54 | 0:13:48 | 1:12:18 | ||||
09783 | 141 | 26 | 2059 May 27 | 7:55:35 | Partial | -0.9097 | 0.1829 | 281.7 | 97.2 | 5:34:44 | 10:16:26 | 7:06:59 | 8:44:11 | ||||
09824 | 141 | 27 | 2077 Jun 06 | 14:59:52 | Partial | -0.8387 | 0.3123 | 293.6 | 125.0 | 12:33:04 | 17:26:40 | 13:57:22 | 16:02:22 | ||||
09865 | 141 | 28 | 2095 Jun 17 | 22:00:11 | Partial | -0.7653 | 0.4459 | 304.7 | 146.9 | 19:27:50 | 0:32:32 | 20:46:44 | 23:13:38 | ||||
09907 | 141 | 29 | 2113 Jun 29 | 4:55:26 | Partial | -0.6887 | 0.5849 | 315.1 | 165.2 | 2:17:53 | 7:32:59 | 3:32:50 | 6:18:02 | ||||
09949 | 141 | 30 | 2131 Jul 10 | 11:47:56 | Partial | -0.6107 | 0.7265 | 324.5 | 180.4 | 9:05:41 | 14:30:11 | 10:17:44 | 13:18:08 | ||||
09993 | 141 | 31 | 2149 Jul 20 | 18:38:11 | Partial | -0.5315 | 0.8700 | 333.1 | 193.2 | 15:51:38 | 21:24:44 | 17:01:35 | 20:14:47 | ||||
10037 | 141 | 32 | 2167 Aug 01 | 1:28:59 | Total | -0.4536 | 1.0108 | 340.5 | 203.6 | 16.6 | 22:38:44 | 4:19:14 | 23:47:11 | 1:20:41 | 1:37:17 | 3:10:47 | |
10080 | 141 | 33 | 2185 Aug 11 | 8:20:59 | Total | -0.3774 | 1.1482 | 346.9 | 212.0 | 59.3 | 5:27:32 | 11:14:26 | 6:34:59 | 7:51:20 | 8:50:38 | 10:06:59 | |
10123 | 141 | 34 | 2203 Aug 23 | 15:15:12 | Total | -0.3039 | 1.2806 | 352.2 | 218.6 | 78.1 | 12:19:06 | 18:11:18 | 13:25:54 | 14:36:09 | 15:54:15 | 17:04:30 | |
10167 | 141 | 35 | 2221 Sep 02 | 22:13:42 | Total | -0.2348 | 1.4048 | 356.6 | 223.5 | 89.7 | 19:15:24 | 1:12:00 | 20:21:57 | 21:28:51 | 22:58:33 | 0:05:27 | |
10212 | 141 | 36 | 2239 Sep 14 | 5:17:34 | Total | -0.1708 | 1.5194 | 360.2 | 227.0 | 97.0 | 2:17:28 | 8:17:40 | 3:24:04 | 4:29:04 | 6:06:04 | 7:11:04 | |
10257 | 141 | 37 | 2257 Sep 24 | 12:27:34 | Total | -0.1123 | 1.6239 | 363.1 | 229.3 | 101.4 | 9:26:01 | 15:29:07 | 10:32:55 | 11:36:52 | 13:18:16 | 14:22:13 | |
10303 | 141 | 38 | 2275 Oct 05 | 19:44:07 | Total | -0.0599 | 1.7172 | 365.3 | 230.8 | 103.7 | 16:41:28 | 22:46:46 | 17:48:43 | 18:52:16 | 20:35:58 | 21:39:31 | |
10350 | 141 | 39 | 2293 Oct 16 | 3:08:18 | Total | -0.0144 | 1.7979 | 367.1 | 231.6 | 104.6 | 0:04:45 | 6:11:51 | 1:12:30 | 2:16:00 | 4:00:36 | 5:04:06 | |
10396 | 141 | 40 | 2311 Oct 28 | 10:40:16 | Total | 0.0241 | 1.7773 | 368.6 | 231.9 | 104.5 | 7:35:58 | 13:44:34 | 8:44:19 | 9:48:01 | 11:32:31 | 12:36:13 | |
10442 | 141 | 41 | 2329 Nov 07 | 18:18:33 | Total | 0.0568 | 1.7146 | 369.8 | 231.9 | 103.7 | 15:13:39 | 21:23:27 | 16:22:36 | 17:26:42 | 19:10:24 | 20:14:30 | |
10488 | 141 | 42 | 2347 Nov 19 | 2:04:59 | Total | 0.0825 | 1.6651 | 370.8 | 231.8 | 102.7 | 22:59:35 | 5:10:23 | 0:09:05 | 1:13:38 | 2:56:20 | 4:00:53 | |
10533 | 141 | 43 | 2365 Nov 29 | 9:57:07 | Total | 0.1031 | 1.6251 | 371.8 | 231.6 | 101.7 | 6:51:13 | 13:03:01 | 8:01:19 | 9:06:16 | 10:47:58 | 11:52:55 | |
10578 | 141 | 44 | 2383 Dec 10 | 17:55:40 | Total | 0.1179 | 1.5961 | 372.6 | 231.5 | 100.8 | 14:49:22 | 21:01:58 | 15:59:55 | 17:05:16 | 18:46:04 | 19:51:25 | |
10623 | 141 | 45 | 2401 Dec 21 | 1:56:07 | Total | 0.1306 | 1.5711 | 373.3 | 231.4 | 99.9 | 22:49:28 | 5:02:46 | 0:00:25 | 1:06:10 | 2:46:04 | 3:51:49 | |
10668 | 141 | 46 | 2420 Jan 01 | 10:00:56 | Total | 0.1394 | 1.5539 | 374.0 | 231.4 | 99.2 | 6:53:56 | 13:07:56 | 8:05:14 | 9:11:20 | 10:50:32 | 11:56:38 | |
10712 | 141 | 47 | 2438 Jan 11 | 18:05:30 | Total | 0.1483 | 1.5366 | 374.5 | 231.3 | 98.5 | 14:58:15 | 21:12:45 | 16:09:51 | 17:16:15 | 18:54:45 | 20:01:09 | |
10756 | 141 | 48 | 2456 Jan 23 | 2:10:08 | Total | 0.1568 | 1.5206 | 374.9 | 231.3 | 97.9 | 23:02:41 | 5:17:35 | 0:14:29 | 1:21:11 | 2:59:05 | 4:05:47 | |
10798 | 141 | 49 | 2474 Feb 02 | 10:11:05 | Total | 0.1681 | 1.4998 | 375.0 | 231.1 | 96.9 | 7:03:35 | 13:18:35 | 8:15:32 | 9:22:38 | 10:59:32 | 12:06:38 | |
10839 | 141 | 50 | 2492 Feb 13 | 18:09:20 | Total | 0.1814 | 1.4757 | 375.0 | 230.7 | 95.6 | 15:01:50 | 21:16:50 | 16:13:59 | 17:21:32 | 18:57:08 | 20:04:41 | |
10880 | 141 | 51 | 2510 Feb 25 | 2:01:15 | Total | 0.1998 | 1.4426 | 374.6 | 230.1 | 93.7 | 22:53:57 | 5:08:33 | 0:06:12 | 1:14:24 | 2:48:06 | 3:56:18 | |
10920 | 141 | 52 | 2528 Mar 07 | 9:46:47 | Total | 0.2233 | 1.4003 | 373.9 | 229.1 | 90.8 | 6:39:50 | 12:53:44 | 7:52:14 | 9:01:23 | 10:32:11 | 11:41:20 | |
10961 | 141 | 53 | 2546 Mar 18 | 17:24:17 | Total | 0.2534 | 1.3462 | 372.7 | 227.5 | 86.4 | 14:17:56 | 20:30:38 | 15:30:32 | 16:41:05 | 18:07:29 | 19:18:02 | |
11003 | 141 | 54 | 2564 Mar 29 | 0:54:06 | Total | 0.2895 | 1.2813 | 371.1 | 225.2 | 79.9 | 21:48:33 | 3:59:39 | 23:01:30 | 0:14:09 | 1:34:03 | 2:46:42 | |
11044 | 141 | 55 | 2582 Apr 09 | 8:13:59 | Total | 0.3337 | 1.2017 | 368.7 | 221.9 | 69.7 | 5:09:38 | 11:18:20 | 6:23:02 | 7:39:08 | 8:48:50 | 10:04:56 | |
11084 | 141 | 56 | 2600 Apr 20 | 15:25:41 | Total | 0.3845 | 1.1101 | 365.5 | 217.3 | 53.2 | 12:22:56 | 18:28:26 | 13:37:02 | 14:59:05 | 15:52:17 | 17:14:20 | |
11124 | 141 | 57 | 2618 May 1 | 22:28:05 | Total | 0.4426 | 1.0049 | 361.4 | 211.1 | 11.6 | 19:27:23 | 1:28:47 | 20:42:32 | 22:22:17 | 22:33:53 | 0:13:38 | |
11165 | 141 | 58 | 2636 May 12 | 5:23:36 | Partial | 0.5064 | 0.8894 | 356.1 | 202.9 | 2:25:33 | 8:21:39 | 3:42:09 | 7:05:03 | ||||
11206 | 141 | 59 | 2654 May 23 | 12:09:21 | Partial | 0.5779 | 0.7597 | 349.4 | 191.8 | 9:14:39 | 15:04:03 | 10:33:27 | 13:45:15 | ||||
11248 | 141 | 60 | 2672 Jun 02 | 18:50:39 | Partial | 0.6528 | 0.6238 | 341.3 | 177.8 | 16:00:00 | 21:41:18 | 17:21:45 | 20:19:33 | ||||
11291 | 141 | 61 | 2690 Jun 14 | 1:25:03 | Partial | 0.7329 | 0.4780 | 331.4 | 159.2 | 22:39:21 | 4:10:45 | 0:05:27 | 2:44:39 | ||||
11334 | 141 | 62 | 2708 Jun 25 | 7:57:36 | Partial | 0.8147 | 0.3292 | 319.9 | 135.1 | 5:17:39 | 10:37:33 | 6:50:03 | 9:05:09 | ||||
11376 | 141 | 63 | 2726 Jul 06 | 14:25:33 | Partial | 0.9000 | 0.1736 | 306.2 | 100.2 | 11:52:27 | 16:58:39 | 13:35:27 | 15:15:39 | ||||
11418 | 141 | 64 | 2744 Jul 16 | 20:55:09 | Partial | 0.9841 | 0.0202 | 290.8 | 34.9 | 18:29:45 | 23:20:33 | 20:37:42 | 21:12:36 | ||||
11462 | 141 | 65 | 2762 Jul 28 | 3:24:16 | Penumbral | 1.0681 | -0.1333 | 273.2 | 1:07:40 | 5:40:52 | |||||||
11506 | 141 | 66 | 2780 Aug 07 | 9:56:19 | Penumbral | 1.1498 | -0.2829 | 253.5 | 7:49:34 | 12:03:04 | |||||||
11552 | 141 | 67 | 2798 Aug 18 | 16:31:28 | Penumbral | 1.2293 | -0.4284 | 231.4 | 14:35:46 | 18:27:10 | |||||||
11598 | 141 | 68 | 2816 Aug 28 | 23:13:01 | Penumbral | 1.3037 | -0.5648 | 207.2 | 21:29:25 | 0:56:37 | |||||||
11646 | 141 | 69 | 2834 Sep 09 | 6:01:06 | Penumbral | 1.3730 | -0.6920 | 180.6 | 4:30:48 | 7:31:24 | |||||||
11692 | 141 | 70 | 2852 Sep 19 | 12:56:17 | Penumbral | 1.4368 | -0.8093 | 150.6 | 11:40:59 | 14:11:35 | |||||||
11738 | 141 | 71 | 2870 Sep 30 | 20:00:43 | Penumbral | 1.4935 | -0.9136 | 116.5 | 19:02:28 | 20:58:58 | |||||||
11784 | 141 | 72 | 2888 Oct 11 | 3:14:10 | Penumbral | 1.5434 | -1.0055 | 72.9 | 2:37:43 | 3:50:37 |
The inex is an eclipse cycle of 10,571.95 days. The cycle was first described in modern times by Crommelin in 1901, but was named by George van den Bergh who studied it in detail half a century later. It has been suggested that the cycle was known to Hipparchos. One inex after an eclipse of a particular saros series there will be an eclipse in the next saros series, unless the latter saros series has come to an end.
A penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Sunday, April 24, 2005, with an umbral magnitude of −0.1417. 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 4.9 days before perigee, the Moon's apparent diameter was larger.
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, December 30, 1982. A shallow total eclipse saw the Moon in relative darkness for 1 hour 3 seconds. The Moon was 18% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 16 minutes in total. This was a supermoon since perigee was on the same day. It was also a blue moon, the second full moon of December for the eastern hemisphere where the previous full moon was on December 1. Since total lunar eclipses are also known as blood moons, this combination is known as a super blue blood moon.
A penumbral lunar eclipse took place on Tuesday, April 14, 1987, the first of two lunar eclipses in 1987, the second being on October 7, 1987. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 77.703% of the Moon's disc was partially shaded by the Earth, which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours, 54 minutes and 12.8 seconds. The Moon was just 4.6 days before perigee, making it 0.5% larger than average.
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 will take place on May 16, 2041.
A penumbral lunar eclipse took place on Wednesday, April 2, 1969, the first of three penumbral lunar eclipses in 1969, the second being on Wednesday, August 27, and the last being on Thursday, September 25. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 70.337% of the Moon's disc was partially shaded by the Earth, which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours, 43 minutes and 46.9 seconds. Occurring only 4.2 days before perigee, the Moon's apparent diameter was 0.9% larger than average.
A total lunar eclipse will take place on September 19, 2043.
Saros cycle series 141 for solar eclipses occurs at the Moon's ascending node, repeats every 18 years, 11 days containing 70 eclipses, 41 of which are umbral. The first eclipse in this series was on 19 May 1613 and the last will be on 23 June 2857. The most recent eclipse was an annular eclipse on 15 January 2010 and the next will be an annular eclipse on 26 January 2028. This series contains only annular eclipses from 4 August 1739 through 14 October 2460, with no total or hybrid eclipses.
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 134 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 72 events.
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 penumbral lunar eclipse took place on Friday, March 23, 1951. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 64% of the Moon's disc was partially shaded by the Earth, which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours and 34 minutes.