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2005 Apr 24 | 2023 May 05 |
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 total lunar eclipse took place on May 4, 2004, the first of two total lunar eclipses in 2004, the second being on October 28, 2004.
A penumbral lunar eclipse took place on April 24, 2005, the first of two lunar eclipses in 2005. At maximum eclipse, 86.5% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours and 6 minutes overall, and was visible from east Asia, Australia, and the Americas.
A total lunar eclipse took place on Tuesday 9 January 2001, the first of three lunar eclipses in 2001. A shallow total eclipse saw the Moon in relative darkness for 1 hour 1 minute and 2 seconds. The Moon was 18.89% of its diameter into the Earth's umbral shadow, and totality was observed in all of Europe, Africa, and Asia. The partial eclipse lasted for 3 hours 16 minutes and 19 seconds and was visible in parts of north-eastern North America and Australia. It is the only total eclipse of 2001. It was visible over Asia and Western Australia with the Middle East getting mid eclipse at midnight.
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.
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 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 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 penumbral lunar eclipse occured on Friday, May 5, 2023, the first of two lunar eclipses in 2023. The moon's apparent diameter was 0.1% larger than average because it occured 5.5 days before perigee. This was the deepest penumbral eclipse since February 2017 and until September 2042.
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 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 solar eclipse will occur on May 20, 2050. 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. This eclipse is a hybrid eclipse, starting and ending as an annular solar eclipse.
Saros cycle series 141 for solar eclipses occurs at the Moon's ascending node, repeats every 18 years, 11 days and contains 70 events. The series started with a partial solar eclipse on May 19, 1613. It contains 41 annular eclipses from August 4, 1739 through October 14, 2460. There are no total eclipses in this series. The series ends at member 70 as a partial eclipse on June 13, 2857. All eclipses in this series occurs at the Moon's ascending node.
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.
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.