The periodicity and recurrence of lunar (and solar) eclipses is governed by the Saros cycle, a period of approximately 6,585.3 days (18 years 11 days 8 hours). When two eclipses are separated by a period of one Saros, they share a very similar geometry. The two eclipses occur at the same node[1] with the Moon at nearly the same distance from Earth and at the same time of year. Thus, the Saros is useful for organizing eclipses into families or series. Each series typically lasts 12 to 15 centuries and contains 70 or more lunar eclipses.
Lunar eclipses of Saros 67 all occur at the Moons descending node and the Moon moves northward with each eclipse. The series began with a penumbral eclipse near the southern edge of the penumbra on -0660 Jul 11. The series ended with a penumbral eclipse near the northern edge of the penumbra on 0638 Aug 30. The total duration of Saros series 67 is 1298.17 years. In summary:
First Eclipse = -0660 Jul 11 19:40:20 TD Last Eclipse = 0638 Aug 30 09:07:10 TD Duration of Saros 67 = 1298.17 Years
Saros 67 is composed of 73 lunar eclipses as follows:
Lunar Eclipses of Saros 67 | |||
Eclipse Type | Symbol | Number | Percent |
All Eclipses | - | 73 | 100.0% |
Penumbral | N | 29 | 39.7% |
Partial | P | 16 | 21.9% |
Total | T | 28 | 38.4% |
The 73 lunar eclipses in Saros 67 occur in the order of 21N 9P 28T 7P 8N which corresponds to:
21 Penumbral 9 Partial 28 Total 7 Partial 8 Penumbral
The longest and shortest eclipses of Saros 67 are as follows.
Longest Total Lunar Eclipse: 0007 Aug 17 Duration = 01h40m11s Shortest Total Lunar Eclipse: -0119 Jun 02 Duration = 00h16m50s Longest Partial Lunar Eclipse: 0386 Apr 01 Duration = 03h20m55s Shortest Partial Lunar Eclipse: -0281 Feb 25 Duration = 00h19m48s Longest Penumbral Lunar Eclipse: 0512 Jun 15 Duration = 04h36m46s Shortest Penumbral Lunar Eclipse: -0660 Jul 11 Duration = 01h11m43s
The largest and smallest magnitude partial eclipses of Saros 67 are:
Largest Partial Lunar Eclipse: 0386 Apr 01 Magnitude = 0.9881 Smallest Partial Lunar Eclipse: -0281 Feb 25 Magnitude = 0.0083
Local circumstances at greatest eclipse[2] for every lunar eclipse of Saros 67 are presented in the following catalog. For eclipses occurring between the years -1999 to +3000 (2000 BCE to 3000 CE), the sequence number in the first column links to a eclipse geometry diagram and a map from Five Millennium Canon of Lunar Eclipses: -1999 to +3000. A detailed key and additional information about the catalog can be found at: Key to Catalog of Lunar Eclipse Saros Series.
TD of Phase Seq. Rel. Calendar Greatest Luna Ecl. Pen. Um. ---- Durations ---- Num. Num. Date Eclipse ΔT Num Type QSE Gamma Mag. Mag. Pen. Par. Total s m m m 01 -37 -0660 Jul 11 19:40:20 19564 -32894 Nb a- -1.5130 0.0681 -0.9050 71.7 - - 02 -36 -0642 Jul 23 03:09:50 19281 -32671 N a- -1.4476 0.1880 -0.7847 117.5 - - 03 -35 -0624 Aug 02 10:47:04 18999 -32448 N a- -1.3878 0.2975 -0.6750 145.9 - - 04 -34 -0606 Aug 13 18:32:09 18719 -32225 N a- -1.3340 0.3965 -0.5763 166.5 - - 05 -33 -0588 Aug 24 02:26:30 18441 -32002 N a- -1.2871 0.4828 -0.4906 181.8 - - 06 -32 -0570 Sep 04 10:30:12 18166 -31779 N a- -1.2473 0.5561 -0.4180 193.3 - - 07 -31 -0552 Sep 14 18:43:09 17892 -31556 N a- -1.2149 0.6161 -0.3589 201.9 - - 08 -30 -0534 Sep 26 03:04:05 17621 -31333 N a- -1.1886 0.6648 -0.3111 208.3 - - 09 -29 -0516 Oct 06 11:33:32 17352 -31110 N a- -1.1692 0.7009 -0.2759 212.8 - - 10 -28 -0498 Oct 17 20:10:28 17075 -30887 N a- -1.1554 0.7264 -0.2510 215.7 - - 11 -27 -0480 Oct 28 04:53:04 16757 -30664 N a- -1.1461 0.7437 -0.2339 217.6 - - 12 -26 -0462 Nov 08 13:41:02 16447 -30441 N a- -1.1409 0.7532 -0.2244 218.4 - - 13 -25 -0444 Nov 18 22:31:49 16147 -30218 N a- -1.1376 0.7589 -0.2181 218.8 - - 14 -24 -0426 Nov 30 07:25:15 15854 -29995 N a- -1.1366 0.7604 -0.2158 218.7 - - 15 -23 -0408 Dec 10 16:17:01 15569 -29772 N a- -1.1340 0.7644 -0.2102 218.9 - - 16 -22 -0390 Dec 22 01:08:45 15291 -29549 N a- -1.1313 0.7684 -0.2044 219.1 - - 17 -21 -0371 Jan 01 09:56:06 15020 -29326 N a- -1.1247 0.7794 -0.1912 220.2 - - 18 -20 -0353 Jan 12 18:39:29 14755 -29103 N a- -1.1151 0.7956 -0.1724 221.8 - - 19 -19 -0335 Jan 23 03:15:31 14497 -28880 N a- -1.0996 0.8226 -0.1425 224.7 - - 20 -18 -0317 Feb 03 11:46:02 14244 -28657 N a- -1.0797 0.8576 -0.1045 228.4 - - 21 -17 -0299 Feb 13 20:08:15 13997 -28434 N a- -1.0530 0.9051 -0.0540 233.3 - - 22 -16 -0281 Feb 25 04:22:31 13756 -28211 P a- -1.0199 0.9643 0.0083 239.1 19.8 - 23 -15 -0263 Mar 07 12:28:13 13519 -27988 P a- -0.9799 1.0363 0.0831 245.9 62.1 - 24 -14 -0245 Mar 18 20:26:41 13287 -27765 P a- -0.9340 1.1192 0.1686 253.1 87.4 - 25 -13 -0227 Mar 29 04:17:04 13061 -27542 P a- -0.8816 1.2142 0.2659 260.9 108.3 - 26 -12 -0209 Apr 09 12:00:38 12838 -27319 P a- -0.8234 1.3201 0.3735 268.8 126.5 - 27 -11 -0191 Apr 19 19:38:06 12620 -27096 P a- -0.7603 1.4352 0.4899 276.7 142.5 - 28 -10 -0173 May 01 03:10:54 12406 -26873 P a- -0.6935 1.5575 0.6128 284.3 156.5 - 29 -09 -0155 May 11 10:38:15 12196 -26650 P a- -0.6223 1.6880 0.7435 291.6 169.0 - 30 -08 -0137 May 22 18:03:37 11990 -26427 P a- -0.5496 1.8219 0.8767 298.2 179.6 - 31 -07 -0119 Jun 02 01:26:17 11788 -26204 T a- -0.4751 1.9591 1.0126 304.2 188.7 16.8 32 -06 -0101 Jun 13 08:49:48 11589 -25981 T a- -0.4015 2.0951 1.1468 309.4 196.2 55.2 33 -05 -0083 Jun 23 16:11:50 11393 -25758 T p- -0.3273 2.2327 1.2817 314.0 202.3 73.3 34 -04 -0065 Jul 04 23:37:55 11201 -25535 T- p- -0.2570 2.3632 1.4090 317.7 207.0 84.6 35 -03 -0047 Jul 15 07:05:20 11011 -25312 T- p- -0.1887 2.4905 1.5325 320.9 210.5 92.1 36 -02 -0029 Jul 26 14:38:10 10824 -25089 T- pp -0.1254 2.6089 1.6465 323.3 212.9 96.7 37 -01 -0011 Aug 05 22:14:21 10640 -24866 T- pp -0.0656 2.7210 1.7539 325.3 214.4 99.3 38 00 0007 Aug 17 05:58:18 10457 -24643 T- pp -0.0129 2.8203 1.8479 326.9 215.2 100.2 39 01 0025 Aug 27 13:47:51 10277 -24420 T+ pp 0.0341 2.7841 1.8063 328.2 215.4 100.0 40 02 0043 Sep 07 21:44:44 10099 -24197 T+ pp 0.0744 2.7130 1.7296 329.3 215.3 99.0
TD of Phase Seq. Rel. Calendar Greatest Luna Ecl. Pen. Um. ---- Durations ---- Num. Num. Date Eclipse ΔT Num Type QSE Gamma Mag. Mag. Pen. Par. Total s m m m 41 03 0061 Sep 18 05:48:54 9923 -23974 T+ -p 0.1081 2.6542 1.6650 330.3 215.1 97.5 42 04 0079 Sep 29 14:01:11 9748 -23751 T+ -p 0.1346 2.6084 1.6136 331.3 214.8 96.0 43 05 0097 Oct 09 22:20:04 9574 -23528 T+ -p 0.1548 2.5741 1.5739 332.3 214.5 94.6 44 06 0115 Oct 21 06:44:43 9401 -23305 T+ -p 0.1697 2.5494 1.5439 333.4 214.4 93.4 45 07 0133 Oct 31 15:15:03 9229 -23082 T+ -p 0.1791 2.5346 1.5243 334.6 214.5 92.6 46 08 0151 Nov 11 23:49:40 9057 -22859 T+ -p 0.1847 2.5265 1.5118 335.8 214.7 92.1 47 09 0169 Nov 22 08:26:30 8886 -22636 T+ -p 0.1877 2.5229 1.5044 337.0 215.1 91.9 48 10 0187 Dec 03 17:04:34 8715 -22413 T+ -p 0.1893 2.5217 1.4999 338.3 215.5 91.8 49 11 0205 Dec 14 01:41:42 8544 -22190 T+ -p 0.1909 2.5200 1.4955 339.5 216.0 91.8 50 12 0223 Dec 25 10:16:37 8373 -21967 T+ -p 0.1937 2.5160 1.4894 340.6 216.4 91.6 51 13 0242 Jan 04 18:46:22 8202 -21744 T+ -p 0.2001 2.5051 1.4769 341.6 216.8 91.2 52 14 0260 Jan 16 03:11:11 8030 -21521 T+ -p 0.2100 2.4875 1.4582 342.5 216.9 90.3 53 15 0278 Jan 26 11:28:31 7857 -21298 T+ -p 0.2255 2.4594 1.4294 343.2 216.8 88.7 54 16 0296 Feb 06 19:37:21 7683 -21075 T+ -p 0.2472 2.4196 1.3892 343.5 216.3 86.0 55 17 0314 Feb 17 03:36:44 7509 -20852 T -p 0.2761 2.3669 1.3362 343.6 215.2 81.8 56 18 0332 Feb 28 11:26:32 7334 -20629 T -a 0.3121 2.3008 1.2701 343.1 213.5 75.4 57 19 0350 Mar 10 19:06:45 7158 -20406 T -a 0.3554 2.2213 1.1905 342.1 210.7 65.2 58 20 0368 Mar 21 02:35:36 6981 -20183 T -a 0.4073 2.1262 1.0953 340.3 206.6 47.7 59 21 0386 Apr 01 09:55:38 6804 -19960 P -h 0.4656 2.0195 0.9881 337.7 200.9 - 60 22 0404 Apr 11 17:05:42 6626 -19737 P -t 0.5310 1.8997 0.8678 333.9 193.1 - 61 23 0422 Apr 23 00:08:11 6447 -19514 P -t 0.6018 1.7703 0.7374 328.8 182.6 - 62 24 0440 May 03 07:01:41 6269 -19291 P -t 0.6790 1.6292 0.5951 322.1 168.5 - 63 25 0458 May 14 13:50:08 6091 -19068 P -t 0.7592 1.4830 0.4471 313.9 150.0 - 64 26 0476 May 24 20:32:20 5913 -18845 P -t 0.8431 1.3302 0.2921 303.6 124.5 - 65 27 0494 Jun 05 03:11:03 5737 -18622 P -t 0.9285 1.1747 0.1340 291.4 86.5 - 66 28 0512 Jun 15 09:47:02 5560 -18399 Nx -t 1.0151 1.0175 -0.0264 276.8 - - 67 29 0530 Jun 26 16:23:02 5384 -18176 N -t 1.1001 0.8632 -0.1842 260.0 - - 68 30 0548 Jul 06 22:59:59 5208 -17953 N -t 1.1833 0.7126 -0.3387 240.7 - - 69 31 0566 Jul 18 05:38:45 5035 -17730 N -t 1.2637 0.5673 -0.4884 218.6 - - 70 32 0584 Jul 28 12:22:13 4862 -17507 N -t 1.3390 0.4314 -0.6290 193.7 - - 71 33 0602 Aug 08 19:10:29 4691 -17284 N -t 1.4094 0.3048 -0.7605 165.3 - - 72 34 0620 Aug 19 02:05:18 4521 -17061 N -t 1.4737 0.1893 -0.8809 132.1 - - 73 35 0638 Aug 30 09:07:10 4353 -16838 N -t 1.5314 0.0859 -0.9895 90.1 - -
[1] The Moon's orbit is inclined about 5 degrees to Earth's orbit around the Sun. The points where the lunar orbit intersects the plane of Earth's orbit are known as the nodes. The Moon moves from south to north of Earth's orbit at the ascending node, and from north to south at the descending node.
[2]Greatest eclipse is defined as the instant when Moon passes closest to the axis of Earth's shadow.
The Gregorian calendar is used for all dates from 1582 Oct 15 onwards. Before that date, the Julian calendar is used. For more information on this topic, see Calendar Dates. The Julian calendar does not include the year 0. Thus the year 1 BCE is followed by the year 1 CE (See: BCE/CE Dating Conventions ). This is awkward for arithmetic calculations. Years in this catalog are numbered astronomically and include the year 0. Historians should note there is a difference of one year between astronomical dates and BCE dates. Thus, the astronomical year 0 corresponds to 1 BCE, and astronomical year -1 corresponds to 2 BCE, etc..
The coordinates of the Sun used in these predictions are based on the VSOP87 theory [Bretagnon and Francou, 1988]. The Moon's coordinates are based on the ELP-2000/82 theory [Chapront-Touze and Chapront, 1983]. For more information, see: Solar and Lunar Ephemerides. The revised value used for the Moon's secular acceleration is n-dot = -25.858 arc-sec/cy*cy, as deduced from the Apollo lunar laser ranging experiment (Chapront, Chapront-Touze, and Francou, 2002).
The largest uncertainty in the eclipse predictions is caused by fluctuations in Earth's rotation due primarily to tidal friction of the Moon. The resultant drift in apparent clock time is expressed as ΔT and is determined as follows:
A series of polynomial expressions have been derived to simplify the evaluation of ΔT for any time from -1999 to +3000. The uncertainty in ΔT over this period can be estimated from scatter in the measurements.
The Besselian elements used in the predictions were kindly provided by Jean Meeus. All eclipse calculations are by Fred Espenak, and he assumes full responsibility for their accuracy. Some of the information presented on this web site is based on data originally published in Five Millennium Canon of Lunar Eclipses: -1999 to +3000 and Five Millennium Catalog of Lunar Eclipses: -1999 to +3000.
Permission is freely granted to reproduce this data when accompanied by an acknowledgment:
"Eclipse Predictions by Fred Espenak and Jean Meeus (NASA's GSFC)"