Saros 67

Catalog of Solar Eclipses of Saros 67

Fred Espenak

Introduction

A solar eclipse occurs whenever the Moon's shadow passes across Earth's surface. At least two solar eclipses and as many as five occur every year.

The periodicity and recurrence of 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 with the Moon at nearly the same distance from Earth and the same time of year due to a harmonic in three cycles of the Moon's orbit. Thus, the Saros is useful for organizing eclipses into families or series. Each series typically lasts 12 to 13 centuries and contains 70 or more eclipses. Every saros series begins with a number of partial eclipses near one of Earth's polar regions. The series will then produce several dozen central eclipses before ending with a group of partial eclipses near the opposite pole. For more information, see Periodicity of Solar Eclipses.

Catalog of Solar Eclipses of Saros 67

The table below lists the concise characteristics of every solar eclipse belonging to Saros 67 . The date and time of each eclipse is given for the instant of Greatest Eclipse. For eclipses between the years -1999 to 3000, the calendar date links to a web page containing additional details and a map showing the geographic region of eclipse visibility for that eclipse. A description of each parameter in the catalog table can be found in Key to Saros Catalog of Solar Eclipses.

Catalog of Solar Eclipses of Saros 67
Seq Num Rel Num Calendar Date TD of Greatest Eclipse ΔT

s
ΔT Sigma
s
Luna Num Ecl Type QLE Gamma Ecl Mag Lat

°
Long

°
Sun Alt
°
Path Width km Central Dur
1-37 -0709-Mar-0406:55:42 20315 511 -33504 Pb t- 1.5027 0.0608 61N 93E 0 - -
2-36 -0691-Mar-1414:47:34 20026 504 -33281 P t- 1.4598 0.1418 61N 35W 0 - -
3-35 -0673-Mar-2522:32:43 19739 497 -33058 P t- 1.4119 0.2323 61N 162W 0 - -
4-34 -0655-Apr-0506:07:57 19454 490 -32835 P t- 1.3564 0.3373 61N 75E 0 - -
5-33 -0637-Apr-1613:37:58 19171 483 -32612 P t- 1.2972 0.4494 61N 48W 0 - -
6-32 -0619-Apr-2621:00:18 18890 476 -32389 P t- 1.2325 0.5717 61N 168W 0 - -
7-31 -0601-May-0804:18:11 18612 469 -32166 P t- 1.1647 0.6996 62N 72E 0 - -
8-30 -0583-May-1811:31:05 18336 462 -31943 P t- 1.0936 0.8329 62N 46W 0 - -
9-29 -0565-May-2918:41:53 18062 455 -31720 P t- 1.0215 0.9672 63N 165W 0 - -
10-28 -0547-Jun-0901:50:55 17788 448 -31497 T t- 0.9484 1.0266 76N 118E 18 29301m28s
11-27 -0529-Jun-2008:59:20 17520 441 -31274 T p- 0.8757 1.0253 80N 60E 29 18001m30s
12-26 -0511-Jun-3016:09:31 17251 434 -31051 T p- 0.8053 1.0223 77N 9W 36 12901m26s
13-25 -0493-Jul-1123:22:00 16964 428 -30828 T p- 0.7377 1.0183 71N 101W 42 9301m16s
14-24 -0475-Jul-2206:38:35 16652 421 -30605 T p- 0.6742 1.0136 64N 156E 47 6401m00s
15-23 -0457-Aug-0213:59:32 16341 415 -30382 H p- 0.6151 1.0083 57N 48E 52 3700m39s
16-22 -0439-Aug-1221:26:54 16044 408 -30159 H p- 0.5620 1.0026 50N 64W 56 1100m13s
17-21 -0421-Aug-2405:00:44 15755 402 -29936 A p- 0.5153 0.9966 44N 179W 59 1400m18s
18-20 -0403-Sep-0312:40:56 15466 395 -29713 A p- 0.4748 0.9905 37N 64E 61 3800m54s
19-19 -0385-Sep-1420:28:56 15195 389 -29490 A p- 0.4415 0.9845 31N 56W 64 6101m32s
20-18 -0367-Sep-2504:24:19 14926 382 -29267 A n- 0.4151 0.9786 25N 177W 65 8302m14s
21-17 -0349-Oct-0612:26:55 14659 376 -29044 A n- 0.3956 0.9730 19N 60E 67 10502m56s
22-16 -0331-Oct-1620:35:06 14408 370 -28821 A n- 0.3815 0.9677 14N 65W 67 12503m40s
23-15 -0313-Oct-2804:48:41 14157 364 -28598 A n- 0.3729 0.9630 10N 169E 68 14404m22s
24-14 -0295-Nov-0713:06:28 13910 358 -28375 A n- 0.3683 0.9587 6N 43E 68 16105m03s
25-13 -0277-Nov-1821:25:57 13673 351 -28152 A n- 0.3660 0.9551 3N 84W 69 17605m40s
26-12 -0259-Nov-2905:46:55 13435 345 -27929 A n- 0.3655 0.9521 0N 149E 69 18806m12s
27-11 -0241-Dec-1014:06:14 13205 339 -27706 A n- 0.3641 0.9498 2S 23E 69 19806m35s
28-10 -0223-Dec-2022:23:53 12980 334 -27483 A n- 0.3621 0.9481 2S 103W 69 20506m50s
29 -9 -0204-Jan-0106:35:15 12755 328 -27260 A n- 0.3554 0.9471 3S 133E 69 20806m55s
30 -8 -0186-Jan-1114:42:20 12541 322 -27037 A n- 0.3458 0.9465 3S 10E 70 20906m51s
31 -7 -0168-Jan-2222:40:47 12330 316 -26814 A n- 0.3294 0.9465 2S 111W 71 20806m40s
32 -6 -0150-Feb-0206:31:13 12118 310 -26591 A n- 0.3069 0.9469 1S 131E 72 20406m25s
33 -5 -0132-Feb-1314:10:56 11918 305 -26368 A nn 0.2763 0.9476 0N 15E 74 20006m09s
34 -4 -0114-Feb-2321:41:48 11717 299 -26145 A nn 0.2388 0.9485 2N 99W 76 19405m53s
35 -3 -0096-Mar-0605:01:56 11518 294 -25922 A nn 0.1930 0.9495 3N 151E 79 18805m38s
36 -2 -0078-Mar-1712:11:08 11325 288 -25699 A nn 0.1387 0.9506 4N 43E 82 18305m27s
37 -1 -0060-Mar-2719:10:27 11131 283 -25476 Am nn 0.0770 0.9515 6N 62W 86 17805m21s
38 0 -0042-Apr-0802:00:44 10941 277 -25253 A nn 0.0085 0.9522 6N 164W 89 17505m19s
39 1 -0024-Apr-1808:42:28 10755 272 -25030 A nn -0.0664 0.9527 7N 96E 86 17305m22s
40 2 -0006-Apr-2915:16:51 10569 267 -24807 A nn -0.1470 0.9528 6N 3W 82 17405m32s
Catalog of Solar Eclipses of Saros 67
Seq Num Rel Num Calendar Date TD of Greatest Eclipse ΔT

s
ΔT Sigma
s
Luna Num Ecl Type QLE Gamma Ecl Mag Lat

°
Long

°
Sun Alt
°
Path Width km Central Dur
41 3 0012-May-0921:45:41 10389 261 -24584 A nn -0.2316 0.9525 5N 100W 77 17805m48s
42 4 0030-May-2104:10:41 10212 256 -24361 A np -0.3186 0.9518 2N 164E 71 18506m09s
43 5 0048-May-3110:31:52 10034 251 -24138 A -p -0.4083 0.9506 2S 68E 66 19706m33s
44 6 0066-Jun-1116:52:51 9861 246 -23915 A -p -0.4977 0.9488 6S 28W 60 21606m58s
45 7 0084-Jun-2123:13:50 9687 241 -23692 A -p -0.5865 0.9466 12S 125W 54 24207m19s
46 8 0102-Jul-0305:38:37 9513 236 -23469 A -p -0.6718 0.9439 19S 136E 48 28007m33s
47 9 0120-Jul-1312:05:21 9342 231 -23246 A -p -0.7552 0.9407 27S 36E 41 33507m36s
48 10 0138-Jul-2418:39:41 9170 226 -23023 A -p -0.8318 0.9370 36S 68W 33 42207m29s
49 11 0156-Aug-0401:19:09 8998 221 -22800 A -p -0.9038 0.9328 46S 175W 25 58807m11s
50 12 0174-Aug-1508:08:04 8826 217 -22577 A -t -0.9679 0.9278 59S 71E 14 111206m42s
51 13 0192-Aug-2515:03:49 8654 212 -22354 P -t -1.0263 0.9115 71S 64W 0 - -
52 14 0210-Sep-0522:10:47 8482 207 -22131 P -t -1.0754 0.8277 72S 174E 0 - -
53 15 0228-Sep-1605:26:11 8310 203 -21908 P -t -1.1175 0.7563 72S 51E 0 - -
54 16 0246-Sep-2712:51:27 8138 198 -21685 P -t -1.1515 0.6987 72S 76W 0 - -
55 17 0264-Oct-0720:25:40 7966 193 -21462 P -t -1.1784 0.6533 72S 156E 0 - -
56 18 0282-Oct-1904:09:32 7794 189 -21239 P -t -1.1980 0.6204 71S 25E 0 - -
57 19 0300-Oct-2912:00:42 7622 185 -21016 P -t -1.2117 0.5975 71S 106W 0 - -
58 20 0318-Nov-0919:58:08 7448 180 -20793 P -t -1.2208 0.5824 70S 121E 0 - -
59 21 0336-Nov-2004:00:27 7274 176 -20570 P -t -1.2262 0.5735 69S 13W 0 - -
60 22 0354-Dec-0112:06:54 7100 172 -20347 P -t -1.2290 0.5689 68S 146W 0 - -
61 23 0372-Dec-1120:13:48 6922 168 -20124 P -t -1.2319 0.5643 67S 80E 0 - -
62 24 0390-Dec-2304:21:22 6745 163 -19901 P -t -1.2348 0.5597 65S 53W 0 - -
63 25 0409-Jan-0212:26:00 6566 159 -19678 P -t -1.2406 0.5501 64S 175E 0 - -
64 26 0427-Jan-1320:28:26 6387 155 -19455 P -t -1.2486 0.5368 64S 44E 0 - -
65 27 0445-Jan-2404:23:58 6208 151 -19232 P -t -1.2629 0.5129 63S 84W 0 - -
66 28 0463-Feb-0412:15:08 6031 147 -19009 P -t -1.2812 0.4818 62S 148E 0 - -
67 29 0481-Feb-1419:58:08 5855 143 -18786 P -t -1.3066 0.4382 62S 23E 0 - -
68 30 0499-Feb-2603:34:12 5680 140 -18563 P -t -1.3380 0.3837 61S 101W 0 - -
69 31 0517-Mar-0811:01:41 5504 136 -18340 P -t -1.3768 0.3158 61S 138E 0 - -
70 32 0535-Mar-1918:22:45 5328 132 -18117 P -t -1.4211 0.2374 61S 18E 0 - -
71 33 0553-Mar-3001:36:42 5153 128 -17894 P -t -1.4719 0.1468 61S 100W 0 - -
72 34 0571-Apr-1008:43:33 4981 125 -17671 Pe -t -1.5287 0.0444 61S 144E 0 - -

Statistics for Solar Eclipses of Saros 67

Solar eclipses of Saros 67 all occur at the Moon’s ascending node and the Moon moves southward with each eclipse. The series began with a partial eclipse in the northern hemisphere on -0709 Mar 04. The series ended with a partial eclipse in the southern hemisphere on 0571 Apr 10. The total duration of Saros series 67 is 1280.14 years.

Summary of Saros 67
First Eclipse -0709 Mar 04
Last Eclipse 0571 Apr 10
Series Duration 1280.14 Years
No. of Eclipses 72
Sequence 9P 5T 2H 34A 22P

Saros 67 is composed of 72 solar eclipses as follows:

Solar Eclipses of Saros 67
Eclipse Type Symbol Number Percent
All Eclipses - 72100.0%
PartialP 31 43.1%
AnnularA 34 47.2%
TotalT 5 6.9%
HybridH 2 2.8%

Umbral eclipses (annular, total and hybrid) can be further classified as either: 1) Central (two limits), 2) Central (one limit) or 3) Non-Central (one limit). The statistical distribution of these classes in Saros series 67 appears in the following table.

Umbral Eclipses of Saros 67
Classification Number Percent
All Umbral Eclipses 41100.0%
Central (two limits) 41100.0%
Central (one limit) 0 0.0%
Non-Central (one limit) 0 0.0%

The 72 eclipses in Saros 67 occur in the following order : 9P 5T 2H 34A 22P

The longest and shortest central eclipses of Saros 67 as well as largest and smallest partial eclipses appear below.

Extreme Durations and Magnitudes of Solar Eclipses of Saros 67
Extrema Type Date Duration Magnitude
Longest Annular Solar Eclipse 0120 Jul 1307m36s -
Shortest Annular Solar Eclipse -0421 Aug 2400m18s -
Longest Total Solar Eclipse -0529 Jun 2001m30s -
Shortest Total Solar Eclipse -0475 Jul 2201m00s -
Longest Hybrid Solar Eclipse -0457 Aug 0200m39s -
Shortest Hybrid Solar Eclipse -0439 Aug 1200m13s -
Largest Partial Solar Eclipse -0565 May 29 - 0.96720
Smallest Partial Solar Eclipse 0571 Apr 10 - 0.04445

Eclipse Publications

by Fred Espenak

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Calendar

The Gregorian calendar (also called the Western calendar) is internationally the most widely used civil calendar. It is named for Pope Gregory XIII, who introduced it in 1582. On this website, the Gregorian calendar is used for all calendar 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..

Eclipse Predictions

The eclipse predictions presented here were generated using the JPL DE406 solar and lunar ephemerides. The lunar coordinates have been calculated with respect to the Moon's Center of Mass.

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:

  1. pre-1950's: ΔT calculated from empirical fits to historical records derived by Morrison and Stephenson (2004)
  2. 1955-present: ΔT obtained from published observations
  3. future: ΔT is extrapolated from current values weighted by the long term trend from tidal effects

A series of polynomial expressions have been derived to simplify the evaluation of ΔT for any time from -2999 to +3000. The uncertainty in ΔT over this period can be estimated from scatter in the measurements.

Acknowledgments

Some of the content on this web site is based on the books Five Millennium Canon of Solar Eclipses: -1999 to +3000 and Thousand Year Canon of Solar Eclipses 1501 to 2500. All eclipse calculations are by Fred Espenak, and he assumes full responsibility for their accuracy.

Permission is granted to reproduce eclipse data when accompanied by a link to this page and an acknowledgment:

"Eclipse Predictions by Fred Espenak, www.EclipseWise.com"

The use of diagrams and maps is permitted provided that they are NOT altered (except for re-sizing) and the embedded credit line is NOT removed or covered.