Saros 22

Catalog of Solar Eclipses of Saros 22

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 22

The table below lists the concise characteristics of every solar eclipse belonging to Saros 22 . 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 22
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
1-34 -2174-May-2816:18:38 50706 4493 -51621 Pb t- -1.4760 0.1350 69S 178E 0 - -
2-33 -2156-Jun-0722:57:45 50249 4411 -51398 P t- -1.4020 0.2673 69S 65E 0 - -
3-32 -2138-Jun-1905:37:38 49794 4329 -51175 P t- -1.3287 0.3974 68S 49W 0 - -
4-31 -2120-Jun-2912:21:26 49341 4249 -50952 P t- -1.2590 0.5197 67S 163W 0 - -
5-30 -2102-Jul-1019:09:06 48890 4169 -50729 P t- -1.1928 0.6349 66S 83E 0 - -
6-29 -2084-Jul-2102:03:49 48441 4090 -50506 P t- -1.1325 0.7385 65S 33W 0 - -
7-28 -2066-Aug-0109:05:11 47994 4011 -50283 P t- -1.0778 0.8312 64S 150W 0 - -
8-27 -2048-Aug-1116:13:27 47550 3933 -50060 P t- -1.0289 0.9130 63S 92E 0 - -
9-26 -2030-Aug-2223:30:41 47107 3856 -49837 As t- -0.9877 0.9309 56S 17W 8 - 06m04s
10-25 -2012-Sep-0206:56:10 46666 3780 -49614 A p- -0.9535 0.9283 50S 128W 17 88206m37s
11-24 -1994-Sep-1314:30:42 46228 3704 -49391 A p- -0.9269 0.9249 48S 116E 22 73506m57s
12-23 -1976-Sep-2322:11:39 45792 3629 -49168 A p- -0.9057 0.9215 48S 3W 25 67907m10s
13-22 -1958-Oct-0506:01:04 45357 3554 -48945 A p- -0.8918 0.9183 50S 125W 27 66507m16s
14-21 -1940-Oct-1513:55:15 44925 3481 -48722 A p- -0.8820 0.9156 52S 112E 28 66407m17s
15-20 -1922-Oct-2621:54:25 44495 3408 -48499 A p- -0.8768 0.9134 56S 13W 28 67207m15s
16-19 -1904-Nov-0605:55:20 44067 3335 -48276 A p- -0.8732 0.9118 59S 138W 29 68107m10s
17-18 -1886-Nov-1713:58:14 43641 3264 -48053 A p- -0.8714 0.9109 64S 96E 29 68907m03s
18-17 -1868-Nov-2721:59:17 43217 3193 -47830 A p- -0.8682 0.9107 68S 28W 29 68706m55s
19-16 -1850-Dec-0905:57:50 42795 3122 -47607 A p- -0.8631 0.9113 72S 149W 30 67406m47s
20-15 -1832-Dec-1913:51:33 42375 3053 -47384 A p- -0.8543 0.9126 76S 97E 31 64606m40s
21-14 -1814-Dec-3021:40:16 41957 2984 -47161 A p- -0.8417 0.9146 79S 7W 32 60806m34s
22-13 -1795-Jan-1005:20:01 41542 2916 -46938 A p- -0.8216 0.9173 79S 98W 34 55606m29s
23-12 -1777-Jan-2112:52:26 41128 2848 -46715 A p- -0.7953 0.9205 76S 167E 37 50106m26s
24-11 -1759-Jan-3120:14:52 40716 2781 -46492 A p- -0.7608 0.9242 70S 64E 40 44306m25s
25-10 -1741-Feb-1203:29:45 40307 2715 -46269 A p- -0.7200 0.9282 64S 44W 44 39006m24s
26 -9 -1723-Feb-2210:32:44 39899 2650 -46046 A p- -0.6694 0.9324 56S 152W 48 34006m23s
27 -8 -1705-Mar-0517:28:46 39494 2585 -45823 A p- -0.6128 0.9367 48S 101E 52 29706m22s
28 -7 -1687-Mar-1600:14:24 39091 2521 -45600 A p- -0.5471 0.9410 40S 5W 57 26006m20s
29 -6 -1669-Mar-2706:54:30 38690 2458 -45377 A p- -0.4766 0.9451 31S 110W 61 22906m14s
30 -5 -1651-Apr-0613:25:53 38290 2396 -45154 A p- -0.3985 0.9491 22S 147E 66 20306m05s
31 -4 -1633-Apr-1719:54:53 37893 2334 -44931 A p- -0.3179 0.9527 13S 45E 71 18205m53s
32 -3 -1615-Apr-2802:18:39 37498 2273 -44708 A nn -0.2323 0.9559 4S 55W 77 16505m37s
33 -2 -1597-May-0908:41:50 37105 2212 -44485 A nn -0.1456 0.9587 5N 155W 82 15205m18s
34 -1 -1579-May-1915:04:02 36715 2152 -44262 A nn -0.0572 0.9609 13N 105E 87 14204m58s
35 0 -1561-May-3021:28:58 36326 2093 -44039 A nn 0.0297 0.9628 21N 6E 88 13504m37s
36 1 -1543-Jun-1003:56:49 35939 2035 -43816 Am nn 0.1150 0.9641 28N 93W 83 13104m16s
37 2 -1525-Jun-2110:29:15 35554 1977 -43593 A nn 0.1973 0.9649 34N 168E 78 12903m58s
38 3 -1507-Jul-0117:08:42 35172 1920 -43370 A nn 0.2747 0.9653 40N 69E 74 13103m43s
39 4 -1489-Jul-1223:55:42 34791 1864 -43147 A -n 0.3470 0.9653 44N 31W 69 13403m31s
40 5 -1471-Jul-2306:51:42 34413 1809 -42924 A -p 0.4126 0.9650 47N 132W 65 13903m23s
Catalog of Solar Eclipses of Saros 22
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 6 -1453-Aug-0313:57:07 34036 1754 -42701 A -p 0.4711 0.9644 48N 125E 62 14503m18s
42 7 -1435-Aug-1321:13:34 33662 1700 -42478 A -p 0.5215 0.9637 48N 18E 58 15303m16s
43 8 -1417-Aug-2504:40:22 33290 1647 -42255 A -p 0.5643 0.9630 46N 91W 55 16103m16s
44 9 -1399-Sep-0412:17:15 32920 1594 -42032 A -p 0.5997 0.9624 44N 155E 53 16803m18s
45 10 -1381-Sep-1520:04:57 32551 1542 -41809 A -p 0.6269 0.9620 41N 38E 51 17403m21s
46 11 -1363-Sep-2604:02:45 32185 1491 -41586 A -p 0.6464 0.9619 38N 84W 50 17703m25s
47 12 -1345-Oct-0712:09:30 31821 1441 -41363 A -p 0.6596 0.9623 35N 152E 49 17703m27s
48 13 -1327-Oct-1720:23:39 31459 1391 -41140 A -p 0.6676 0.9631 31N 25E 48 17503m29s
49 14 -1309-Oct-2904:44:39 31100 1342 -40917 A -p 0.6708 0.9645 28N 103W 48 16903m28s
50 15 -1291-Nov-0813:10:41 30742 1294 -40694 A -p 0.6706 0.9665 25N 126E 48 15903m23s
51 16 -1273-Nov-1921:39:06 30386 1246 -40471 A -p 0.6693 0.9691 22N 4W 48 14703m13s
52 17 -1255-Nov-3006:09:20 30032 1200 -40248 A -p 0.6673 0.9723 20N 136W 48 13102m59s
53 18 -1237-Dec-1114:38:21 29681 1154 -40025 A -p 0.6671 0.9762 19N 94E 48 11302m37s
54 19 -1219-Dec-2123:06:03 29331 1109 -39802 A -p 0.6688 0.9806 18N 37W 48 9302m10s
55 20 -1200-Jan-0207:28:27 28984 1064 -39579 A -p 0.6755 0.9855 19N 166W 47 6901m37s
56 21 -1182-Jan-1215:47:17 28639 1020 -39356 A -p 0.6860 0.9908 20N 66E 47 4501m00s
57 22 -1164-Jan-2323:58:49 28295 977 -39133 A -p 0.7029 0.9964 23N 61W 45 1800m23s
58 23 -1146-Feb-0308:03:59 27954 935 -38910 H -p 0.7260 1.0022 27N 173E 43 1100m13s
59 24 -1128-Feb-1416:00:48 27615 894 -38687 H -p 0.7567 1.0080 32N 49E 41 4200m46s
60 25 -1110-Feb-2423:51:21 27278 853 -38464 T -p 0.7932 1.0136 38N 74W 37 7601m13s
61 26 -1092-Mar-0707:34:27 26943 813 -38241 T -p 0.8365 1.0189 45N 163E 33 11701m33s
62 27 -1074-Mar-1815:10:34 26610 774 -38018 T -p 0.8862 1.0236 53N 39E 27 17301m46s
63 28 -1056-Mar-2822:40:37 26279 736 -37795 T -t 0.9418 1.0272 63N 89W 19 27801m49s
64 29 -1038-Apr-0906:05:48 25950 698 -37572 T+ -t 1.0021 1.0038 72N 97E 0 - -
65 30 -1020-Apr-1913:27:02 25623 661 -37349 P -t 1.0664 0.8849 71N 28W 0 - -
66 31 -1002-Apr-3020:45:02 25299 625 -37126 P -t 1.1338 0.7586 71N 152W 0 - -
67 32 -0984-May-1104:02:05 24976 616 -36903 P -t 1.2028 0.6282 70N 84E 0 - -
68 33 -0966-May-2211:18:57 24655 609 -36680 P -t 1.2727 0.4951 69N 39W 0 - -
69 34 -0948-Jun-0118:36:23 24337 602 -36457 P -t 1.3427 0.3611 68N 161W 0 - -
70 35 -0930-Jun-1301:56:21 24021 595 -36234 P -t 1.4111 0.2297 67N 76E 0 - -
71 36 -0912-Jun-2309:19:23 23706 588 -36011 Pe -t 1.4775 0.1021 66N 47W 0 - -

Statistics for Solar Eclipses of Saros 22

Solar eclipses of Saros 22 all occur at the Moon’s descending node and the Moon moves northward with each eclipse. The series began with a partial eclipse in the southern hemisphere on -2174 May 28. The series ended with a partial eclipse in the northern hemisphere on -0912 Jun 23. The total duration of Saros series 22 is 1262.11 years.

Summary of Saros 22
First Eclipse -2174 May 28
Last Eclipse -0912 Jun 23
Series Duration 1262.11 Years
No. of Eclipses 71
Sequence 8P 49A 2H 5T 7P

Saros 22 is composed of 71 solar eclipses as follows:

Solar Eclipses of Saros 22
Eclipse Type Symbol Number Percent
All Eclipses - 71100.0%
PartialP 15 21.1%
AnnularA 49 69.0%
TotalT 5 7.0%
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 22 appears in the following table.

Umbral Eclipses of Saros 22
Classification Number Percent
All Umbral Eclipses 56100.0%
Central (two limits) 54 96.4%
Central (one limit) 1 1.8%
Non-Central (one limit) 1 1.8%

The 71 eclipses in Saros 22 occur in the following order : 8P 49A 2H 5T 7P

The longest and shortest central eclipses of Saros 22 as well as largest and smallest partial eclipses appear below.

Extreme Durations and Magnitudes of Solar Eclipses of Saros 22
Extrema Type Date Duration Magnitude
Longest Annular Solar Eclipse -1940 Oct 1507m17s -
Shortest Annular Solar Eclipse -1164 Jan 2300m23s -
Longest Total Solar Eclipse -1056 Mar 2801m49s -
Shortest Total Solar Eclipse -1110 Feb 2401m13s -
Longest Hybrid Solar Eclipse -1128 Feb 1400m46s -
Shortest Hybrid Solar Eclipse -1146 Feb 0300m13s -
Largest Partial Solar Eclipse -2048 Aug 11 - 0.91298
Smallest Partial Solar Eclipse -0912 Jun 23 - 0.10205

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.