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![]() 2007 Mar 03 |
Saros cycle series 123 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 130.
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 | ||||||||
07432 | 123 | 1 | 1087 Aug 16 | 21:27:44 | Penumbral | -1.5358 | -0.9548 | 51.8 | 21:01:50 | 21:53:38 | |||||||
07479 | 123 | 2 | 1105 Aug 27 | 5:02:14 | Penumbral | -1.488 | -0.8699 | 98.6 | 4:12:56 | 5:51:32 | |||||||
07525 | 123 | 3 | 1123 Sep 7 | 12:43:57 | Penumbral | -1.4464 | -0.7966 | 125.7 | 11:41:06 | 13:46:48 | |||||||
07571 | 123 | 4 | 1141 Sep 17 | 20:32:05 | Penumbral | -1.4106 | -0.734 | 145.1 | 19:19:32 | 21:44:38 | |||||||
07618 | 123 | 5 | 1159 Sep 29 | 4:27:05 | Penumbral | -1.3809 | -0.6826 | 159.5 | 3:07:20 | 5:46:50 | |||||||
07665 | 123 | 6 | 1177 Oct 9 | 12:29:21 | Penumbral | -1.3577 | -0.6431 | 170.1 | 11:04:18 | 13:54:24 | |||||||
07711 | 123 | 7 | 1195 Oct 20 | 20:38:39 | Penumbral | -1.3406 | -0.6146 | 178 | 19:09:39 | 22:07:39 | |||||||
07757 | 123 | 8 | 1213 Oct 31 | 4:53:28 | Penumbral | -1.3285 | -0.5951 | 183.6 | 3:21:40 | 6:25:16 | |||||||
07803 | 123 | 9 | 1231 Nov 11 | 13:14:04 | Penumbral | -1.3215 | -0.5849 | 187.3 | 11:40:25 | 14:47:43 | |||||||
07848 | 123 | 10 | 1249 Nov 21 | 21:38:08 | Penumbral | -1.3179 | -0.5806 | 189.8 | 20:03:14 | 23:13:02 | |||||||
07892 | 123 | 11 | 1267 Dec 03 | 6:05:09 | Penumbral | -1.3174 | -0.5817 | 191.1 | 4:29:36 | 7:40:42 | |||||||
07937 | 123 | 12 | 1285 Dec 13 | 14:31:36 | Penumbral | -1.3172 | -0.5829 | 192.2 | 12:55:30 | 16:07:42 | |||||||
07982 | 123 | 13 | 1303 Dec 24 | 22:58:34 | Penumbral | -1.3179 | -0.5856 | 192.9 | 21:22:07 | 0:35:01 | |||||||
08025 | 123 | 14 | 1322 Jan 04 | 7:22:09 | Penumbral | -1.3164 | -0.5839 | 194.2 | 5:45:03 | 8:59:15 | |||||||
08067 | 123 | 15 | 1340 Jan 15 | 15:41:50 | Penumbral | -1.3126 | -0.5776 | 196.3 | 14:03:41 | 17:19:59 | |||||||
08109 | 123 | 16 | 1358 Jan 25 | 23:54:42 | Penumbral | -1.3040 | -0.5625 | 199.9 | 22:14:45 | 1:34:39 | |||||||
08150 | 123 | 17 | 1376 Feb 06 | 8:01:19 | Penumbral | -1.2911 | -0.5390 | 204.9 | 6:18:52 | 9:43:46 | |||||||
08191 | 123 | 18 | 1394 Feb 16 | 15:59:20 | Penumbral | -1.2718 | -0.5036 | 211.7 | 14:13:29 | 17:45:11 | |||||||
08232 | 123 | 19 | 1412 Feb 27 | 23:47:40 | Penumbral | -1.2454 | -0.4551 | 220.3 | 21:57:31 | 1:37:49 | |||||||
08274 | 123 | 20 | 1430 Mar 10 | 7:26:31 | Penumbral | -1.2119 | -0.3935 | 230.5 | 5:31:16 | 9:21:46 | |||||||
08316 | 123 | 21 | 1448 Mar 20 | 14:55:10 | Penumbral | -1.1709 | -0.3180 | 242.1 | 12:54:07 | 16:56:13 | |||||||
08357 | 123 | 22 | 1466 Mar 31 | 22:14:13 | Penumbral | -1.1226 | -0.2293 | 254.6 | 20:06:55 | 0:21:31 | |||||||
08397 | 123 | 23 | 1484 Apr 11 | 5:22:47 | Penumbral | -1.0662 | -0.1257 | 267.9 | 3:08:50 | 7:36:44 | |||||||
08437 | 123 | 24 | 1502 Apr 22 | 12:22:44 | Penumbral | -1.0034 | -0.0103 | 281.3 | 10:02:05 | 14:43:23 | |||||||
08477 | 123 | 25 | 1520 May 2 | 19:14:16 | Partial | -0.9344 | 0.1162 | 294.6 | 81.5 | 16:46:58 | 21:41:34 | 18:33:31 | 19:55:01 | ||||
08518 | 123 | 26 | 1538 May 14 | 1:58:00 | Partial | -0.8594 | 0.2535 | 307.5 | 118.3 | 23:24:15 | 4:31:45 | 0:58:51 | 2:57:09 | ||||
08560 | 123 | 27 | 1556 May 24 | 8:36:04 | Partial | -0.7802 | 0.3983 | 319.6 | 145.4 | 5:56:16 | 11:15:52 | 7:23:22 | 9:48:46 | ||||
08603 | 123 | 28 | 1574 Jun 04 | 15:09:13 | Partial | -0.6977 | 0.5492 | 330.8 | 167.1 | 12:23:49 | 17:54:37 | 13:45:40 | 16:32:46 | ||||
08646 | 123 | 29 | 1592 Jun 24 | 21:40:12 | Partial | -0.6135 | 0.7029 | 340.7 | 184.6 | 18:49:51 | 0:30:33 | 20:07:54 | 23:12:30 | ||||
08690 | 123 | 30 | 1610 Jul 06 | 4:08:03 | Partial | -0.5273 | 0.8600 | 349.4 | 199.1 | 1:13:21 | 7:02:45 | 2:28:30 | 5:47:36 | ||||
08735 | 123 | 31 | 1628 Jul 16 | 10:36:57 | Total | -0.4424 | 1.0147 | 356.8 | 210.5 | 19.9 | 7:38:33 | 13:35:21 | 8:51:42 | 10:27:00 | 10:46:54 | 12:22:12 | |
08779 | 123 | 32 | 1646 Jul 27 | 17:06:36 | Total | -0.3586 | 1.1671 | 362.8 | 219.4 | 64.2 | 14:05:12 | 20:08:00 | 15:16:54 | 16:34:30 | 17:38:42 | 18:56:18 | |
08824 | 123 | 33 | 1664 Aug 06 | 23:40:04 | Total | -0.2779 | 1.3135 | 367.6 | 226.0 | 83.5 | 20:36:16 | 2:43:52 | 21:47:04 | 22:58:19 | 0:21:49 | 1:33:04 | |
08870 | 123 | 34 | 1682 Aug 18 | 6:17:12 | Total | -0.2006 | 1.4538 | 371.2 | 230.7 | 95.0 | 3:11:36 | 9:22:48 | 4:21:51 | 5:29:42 | 7:04:42 | 8:12:33 | |
08916 | 123 | 35 | 1700 Aug 29 | 13:01:24 | Total | -0.1291 | 1.5833 | 373.8 | 233.7 | 101.7 | 9:54:30 | 16:08:18 | 11:04:33 | 12:10:33 | 13:52:15 | 14:58:15 | |
08962 | 123 | 36 | 1718 Sep 09 | 19:52:29 | Total | -0.0635 | 1.7017 | 375.5 | 235.3 | 105.0 | 16:44:44 | 23:00:14 | 17:54:50 | 18:59:59 | 20:44:59 | 21:50:08 | |
09009 | 123 | 37 | 1736 Sep 20 | 2:51:00 | Total | -0.0042 | 1.8087 | 376.4 | 235.8 | 106.0 | 23:42:48 | 5:59:12 | 0:53:06 | 1:58:00 | 3:44:00 | 4:48:54 | |
09056 | 123 | 38 | 1754 Oct 01 | 9:58:28 | Total | 0.0478 | 1.7268 | 376.8 | 235.5 | 105.2 | 6:50:04 | 13:06:52 | 8:00:43 | 9:05:52 | 10:51:04 | 11:56:13 | |
09102 | 123 | 39 | 1772 Oct 11 | 17:14:41 | Total | 0.0928 | 1.6425 | 376.9 | 234.7 | 103.3 | 14:06:14 | 20:23:08 | 15:17:20 | 16:23:02 | 18:06:20 | 19:12:02 | |
09147 | 123 | 40 | 1790 Oct 23 | 0:40:41 | Total | 0.1296 | 1.5734 | 376.7 | 233.6 | 100.9 | 21:32:20 | 3:49:02 | 22:43:53 | 23:50:14 | 1:31:08 | 2:37:29 | |
09192 | 123 | 41 | 1808 Nov 03 | 8:13:38 | Total | 0.1607 | 1.5148 | 376.3 | 232.3 | 98.1 | 5:05:29 | 11:21:47 | 6:17:29 | 7:24:35 | 9:02:41 | 10:09:47 | |
09237 | 123 | 42 | 1826 Nov 14 | 15:56:14 | Total | 0.1840 | 1.4709 | 375.9 | 231.2 | 95.6 | 12:48:17 | 19:04:11 | 14:00:38 | 15:08:26 | 16:44:02 | 17:51:50 | |
09284 | 123 | 43 | 1844 Nov 24 | 23:44:52 | Total | 0.2026 | 1.4358 | 375.4 | 230.2 | 93.3 | 20:37:10 | 2:52:34 | 21:49:46 | 22:58:13 | 0:31:31 | 1:39:58 | |
09329 | 123 | 44 | 1862 Dec 06 | 7:40:21 | Total | 0.2157 | 1.4112 | 374.9 | 229.3 | 91.5 | 4:32:54 | 10:47:48 | 5:45:42 | 6:54:36 | 8:26:06 | 9:35:00 | |
09373 | 123 | 45 | 1880 Dec 16 | 15:39:03 | Total | 0.2263 | 1.3914 | 374.4 | 228.6 | 89.9 | 12:31:51 | 18:46:15 | 13:44:45 | 14:54:06 | 16:24:00 | 17:33:21 | |
09417 | 123 | 46 | 1898 Dec 27 | 23:41:52 | Total | 0.2339 | 1.3777 | 373.8 | 228.0 | 88.8 | 20:34:58 | 2:48:46 | 21:47:52 | 22:57:28 | 0:26:16 | 1:35:52 | |
09459 | 123 | 47 | 1917 Jan 08 | 7:44:48 | Total | 0.2415 | 1.3642 | 373.1 | 227.3 | 87.6 | 4:38:15 | 10:51:21 | 5:51:09 | 7:01:00 | 8:28:36 | 9:38:27 | |
09501 | 123 | 48 | 1935 Jan 19 | 15:47:35 | Total | 0.2498 | 1.3499 | 372.1 | 226.7 | 86.3 | 12:41:32 | 18:53:38 | 13:54:14 | 15:04:26 | 16:30:44 | 17:40:56 | |
09542 | 123 | 49 | 1953 Jan 29 | 23:47:49 | Total | 0.2606 | 1.3314 | 371.0 | 225.8 | 84.5 | 20:42:19 | 2:53:19 | 21:54:55 | 23:05:34 | 0:30:04 | 1:40:43 | |
09583 | 123 | 50 | 1971 Feb 10 | 7:45:21 | Total | 0.2741 | 1.3082 | 369.5 | 224.7 | 82.2 | 4:40:36 | 10:50:06 | 5:53:00 | 7:04:15 | 8:26:27 | 9:37:42 | |
09624 | 123 | 51 | 1989 Feb 20 | 15:36:18 | Total | 0.2934 | 1.2747 | 367.7 | 223.1 | 78.5 | 12:32:27 | 18:40:09 | 13:44:45 | 14:57:03 | 16:15:33 | 17:27:51 | |
09665 | 123 | 52 | 2007 Mar 03 | 23:21:59 | Total | 0.3175 | 1.2328 | 365.4 | 221.1 | 73.4 | 20:19:17 | 2:24:41 | 21:31:26 | 22:45:17 | 23:58:41 | 1:12:32 | |
09706 | 123 | 53 | 2025 Mar 14 | 6:59:56 | Total | 0.3484 | 1.1784 | 362.6 | 218.3 | 65.4 | 3:58:38 | 10:01:14 | 5:10:47 | 6:27:14 | 7:32:38 | 8:49:05 | |
09747 | 123 | 54 | 2043 Mar 25 | 14:32:04 | Total | 0.3849 | 1.1142 | 359.3 | 214.6 | 53.4 | 11:32:25 | 17:31:43 | 12:44:46 | 14:05:22 | 14:58:46 | 16:19:22 | |
09788 | 123 | 55 | 2061 Apr 04 | 21:54:05 | Total | 0.4300 | 1.0341 | 355.0 | 209.6 | 29.9 | 18:56:35 | 0:51:35 | 20:09:17 | 21:39:08 | 22:09:02 | 23:38:53 | |
09829 | 123 | 56 | 2079 Apr 16 | 5:10:45 | Partial | 0.4799 | 0.9451 | 350.1 | 203.4 | 2:15:42 | 8:05:48 | 3:29:03 | 6:52:27 | ||||
09871 | 123 | 57 | 2097 Apr 26 | 12:18:17 | Partial | 0.5377 | 0.8420 | 344.0 | 195.2 | 9:26:17 | 15:10:17 | 10:40:41 | 13:55:53 | ||||
09913 | 123 | 58 | 2115 May 08 | 19:21:24 | Partial | 0.5996 | 0.7311 | 336.9 | 185.0 | 16:32:57 | 22:09:51 | 17:48:54 | 20:53:54 | ||||
09955 | 123 | 59 | 2133 May 19 | 2:16:19 | Partial | 0.6688 | 0.6067 | 328.4 | 171.6 | 23:32:07 | 5:00:31 | 0:50:31 | 3:42:07 | ||||
09999 | 123 | 60 | 2151 May 30 | 9:09:10 | Partial | 0.7403 | 0.4780 | 318.6 | 155.1 | 6:29:52 | 11:48:28 | 7:51:37 | 10:26:43 | ||||
10042 | 123 | 61 | 2169 Jun 09 | 15:57:06 | Partial | 0.8158 | 0.3416 | 307.2 | 133.5 | 13:23:30 | 18:30:42 | 14:50:21 | 17:03:51 | ||||
10085 | 123 | 62 | 2187 Jun 20 | 22:44:13 | Partial | 0.8928 | 0.2025 | 294.4 | 104.6 | 20:17:01 | 1:11:25 | 21:51:55 | 23:36:31 | ||||
10128 | 123 | 63 | 2205 Jul 02 | 5:29:54 | Partial | 0.9713 | 0.0603 | 279.8 | 58.0 | 3:10:00 | 7:49:48 | 5:00:54 | 5:58:54 | ||||
10172 | 123 | 64 | 2223 Jul 13 | 12:17:52 | Penumbral | 1.0485 | -0.0797 | 263.7 | 10:06:01 | 14:29:43 | |||||||
10217 | 123 | 65 | 2241 Jul 23 | 19:08:10 | Penumbral | 1.1245 | -0.2177 | 245.9 | 17:05:13 | 21:11:07 | |||||||
10262 | 123 | 66 | 2259 Aug 04 | 2:02:00 | Penumbral | 1.1981 | -0.3516 | 226.3 | 0:08:51 | 3:55:09 | |||||||
10308 | 123 | 67 | 2277 Aug 14 | 9:01:20 | Penumbral | 1.2678 | -0.4785 | 205.3 | 7:18:41 | 10:43:59 | |||||||
10355 | 123 | 68 | 2295 Aug 25 | 16:07:04 | Penumbral | 1.3328 | -0.5971 | 182.5 | 14:35:49 | 17:38:19 | |||||||
10401 | 123 | 69 | 2313 Sep 05 | 23:20:24 | Penumbral | 1.3925 | -0.7061 | 158.0 | 22:01:24 | 0:39:24 | |||||||
10447 | 123 | 70 | 2331 Sep 17 | 6:41:33 | Penumbral | 1.4465 | -0.8048 | 131.1 | 5:36:00 | 7:47:06 | |||||||
10493 | 123 | 71 | 2349 Sep 27 | 14:12:31 | Penumbral | 1.4935 | -0.8907 | 101.4 | 13:21:49 | 15:03:13 | |||||||
10538 | 123 | 72 | 2367 Oct 08 | 21:52:39 | Penumbral | 1.5336 | -0.9642 | 65.4 | 21:19:57 | 22:25:21 |
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.
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. 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 occurred at the Moon’s descending node of orbit on Saturday, March 3, 2007, with an umbral magnitude of 1.2347. 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 2.9 days before apogee, the Moon's apparent diameter was smaller.
A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, November 20, 2002, with an umbral magnitude of −0.2246. 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 3.8 days after apogee, the Moon's apparent diameter was smaller.
A total lunar eclipse took place on Monday, February 20, 1989, the first of two total lunar eclipses in 1989.
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 took place at the Moon's descending node of the orbit on Wednesday, February 10, 1971, the first of two total lunar eclipses in 1971. It had an umbral magnitude of 1.30819. The Moon narrowly missed the center of the Earth's shadow due its gamma being >0.2725 at 0.27413. The Moon was plunged into darkness for 1 hour, 22 minutes and 11.4 seconds, in a deep total eclipse which saw the Moon 30.819% 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, 44 minutes and 42.9 seconds and in total. Occurring only 2.7 days before apogee, the Moon's apparent diameter was 5.9% smaller than average.
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, November 8, 1984, the last of three lunar eclipses in 1984. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 90% 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 4 hours and 28 minutes.
A total lunar eclipse will occur at the Moon’s descending node of orbit on Friday, March 14, 2025, with an umbral magnitude of 1.1804. 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 3.3 days before apogee, the Moon's apparent diameter will be smaller.
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 penumbral lunar eclipse took place on Saturday, October 29, 1966, the second of two lunar eclipses in 1966. This was a deep penumbral eclipse, with over 90% within Penumbral Shadow.
Saros cycle series 123 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 70 eclipses, 44 of which are umbral. The first eclipse in the series was on 29 April 1074 and the last will be on 31 May 2318. The most recent eclipse was a partial eclipse on 25 November 2011 and the next will be a partial eclipse on 5 December 2029.
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 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.