Saros 166

Catalog of Solar Eclipses of Saros 166

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 166

The table below lists the concise characteristics of every solar eclipse belonging to Saros 166 . 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 166
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
1-32 2228-Oct-2900:15:43 309 161 2830 Pb t- -1.5410 0.0477 62S 57E 0 - -
2-31 2246-Nov-0907:47:02 346 182 3053 P t- -1.5082 0.1037 62S 65W 0 - -
3-30 2264-Nov-1915:28:12 386 205 3276 P t- -1.4830 0.1465 63S 171E 0 - -
4-29 2282-Nov-3023:15:22 428 229 3499 P t- -1.4624 0.1813 64S 45E 0 - -
5-28 2300-Dec-1207:09:43 472 254 3722 P t- -1.4472 0.2068 65S 83W 0 - -
6-27 2318-Dec-2315:07:25 520 279 3945 P t- -1.4345 0.2280 66S 148E 0 - -
7-26 2337-Jan-0223:09:43 569 306 4168 P t- -1.4251 0.2435 67S 17E 0 - -
8-25 2355-Jan-1407:12:19 622 333 4391 P t- -1.4157 0.2589 68S 115W 0 - -
9-24 2373-Jan-2415:14:58 677 362 4614 P t- -1.4062 0.2743 69S 113E 0 - -
10-23 2391-Feb-0423:15:05 734 391 4837 P t- -1.3944 0.2934 70S 19W 0 - -
11-22 2409-Feb-1507:12:29 794 421 5060 P t- -1.3802 0.3164 71S 151W 0 - -
12-21 2427-Feb-2615:03:44 857 452 5283 P t- -1.3606 0.3485 72S 78E 0 - -
13-20 2445-Mar-0822:49:33 922 483 5506 P t- -1.3360 0.3892 72S 52W 0 - -
14-19 2463-Mar-2006:27:52 990 516 5729 P t- -1.3050 0.4411 72S 179E 0 - -
15-18 2481-Mar-3014:00:05 1060 549 5952 P t- -1.2684 0.5028 72S 52E 0 - -
16-17 2499-Apr-1021:22:37 1133 584 6175 P t- -1.2232 0.5798 72S 72W 0 - -
17-16 2517-Apr-2204:39:27 1209 619 6398 P t- -1.1726 0.6670 71S 165E 0 - -
18-15 2535-May-0311:47:35 1287 654 6621 P t- -1.1137 0.7692 70S 46E 0 - -
19-14 2553-May-1318:51:19 1367 691 6844 P t- -1.0504 0.8801 70S 72W 0 - -
20-13 2571-May-2501:46:58 1450 729 7067 A t- -0.9794 0.9520 58S 168E 11 92404m21s
21-12 2589-Jun-0408:40:21 1536 767 7290 A t- -0.9054 0.9600 43S 57E 25 34504m10s
22-11 2607-Jun-1615:28:32 1625 806 7513 A p- -0.8257 0.9664 33S 48W 34 21503m47s
23-10 2625-Jun-2622:15:41 1716 846 7736 A p- -0.7443 0.9720 25S 152W 42 15003m16s
24 -9 2643-Jul-0805:00:54 1809 886 7959 A p- -0.6602 0.9768 18S 105E 49 10902m44s
25 -8 2661-Jul-1811:48:05 1905 927 8182 A p- -0.5765 0.9811 13S 3E 55 8102m12s
26 -7 2679-Jul-2918:37:03 2004 969 8405 A p- -0.4932 0.9846 9S 99W 60 6201m44s
27 -6 2697-Aug-0901:29:20 2105 1012 8628 A p- -0.4115 0.9877 7S 159E 66 4701m20s
28 -5 2715-Aug-2108:26:50 2209 1056 8851 A p- -0.3332 0.9901 5S 55E 71 3701m03s
29 -4 2733-Aug-3115:30:14 2315 1100 9074 A n- -0.2586 0.9920 5S 49W 75 2900m49s
30 -3 2751-Sep-1122:41:01 2424 1145 9297 A n- -0.1894 0.9934 5S 156W 79 2400m40s
31 -2 2769-Sep-2205:59:20 2536 1191 9520 A nn -0.1254 0.9944 6S 96E 83 2000m33s
32 -1 2787-Oct-0313:27:26 2650 1238 9743 A nn -0.0684 0.9950 8S 15W 86 1800m29s
33 0 2805-Oct-1321:04:25 2766 1285 9966 A nn -0.0180 0.9954 9S 128W 89 1600m27s
34 1 2823-Oct-2504:50:54 2886 1333 10189 A nn 0.0253 0.9957 11S 116E 89 1500m26s
35 2 2841-Nov-0412:46:57 3007 1382 10412 A nn 0.0615 0.9959 12S 2W 87 1400m25s
36 3 2859-Nov-1520:52:35 3132 1431 10635 A nn 0.0902 0.9962 14S 122W 85 1300m23s
37 4 2877-Nov-2605:06:23 3259 1482 10858 A nn 0.1131 0.9967 15S 115E 84 1200m21s
38 5 2895-Dec-0713:27:17 3388 1533 11081 A nn 0.1307 0.9974 15S 9W 83 900m17s
39 6 2913-Dec-1821:55:01 3520 1584 11304 Am nn 0.1431 0.9985 15S 134W 82 500m10s
40 7 2931-Dec-3006:28:18 3655 1637 11527 A nn 0.1512 1.0000 14S 99E 81 000m00s
Catalog of Solar Eclipses of Saros 166
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 8 2950-Jan-0915:04:34 3792 1690 11750 H nn 0.1575 1.0020 13S 29W 81 700m13s
42 9 2968-Jan-2023:43:33 3932 1744 11973 H nn 0.1619 1.0045 11S 158W 81 1600m29s
43 10 2986-Jan-3108:22:32 4074 1799 12196 H -n 0.1670 1.0075 8S 72E 80 2600m48s
44 11 3004-Feb-1217:01:33 4219 1854 12419 H -n 0.1726 1.0110 4S 57W 80 3801m09s
45 12 3022-Feb-2301:36:33 4367 1910 12642 H -n 0.1818 1.0150 0N 174E 80 5201m32s
46 13 3040-Mar-0510:09:33 4517 1967 12865 T -n 0.1934 1.0194 5N 46E 79 6801m56s
47 14 3058-Mar-1618:36:18 4670 2024 13088 T -n 0.2108 1.0242 10N 81W 78 8402m21s
48 15 3076-Mar-2702:58:39 4825 2082 13311 T -n 0.2324 1.0292 16N 152E 76 10202m46s
49 16 3094-Apr-0711:12:59 4983 2141 13534 T -n 0.2615 1.0344 22N 28E 75 12003m10s
50 17 3112-Apr-1819:22:22 5143 2201 13757 T -n 0.2952 1.0396 28N 94W 73 13903m32s
51 18 3130-Apr-3003:23:52 5306 2261 13980 T -n 0.3362 1.0448 34N 146E 70 15803m50s
52 19 3148-May-1011:19:08 5472 2322 14203 T -n 0.3829 1.0497 40N 28E 67 17904m05s
53 20 3166-May-2119:07:34 5640 2384 14426 T -p 0.4360 1.0542 46N 88W 64 19904m15s
54 21 3184-Jun-0102:51:01 5810 2446 14649 T -p 0.4938 1.0583 52N 160E 60 22104m21s
55 22 3202-Jun-1210:29:22 5984 2510 14872 T -p 0.5563 1.0617 57N 51E 56 24504m23s
56 23 3220-Jun-2218:03:20 6160 2573 15095 T -p 0.6228 1.0645 62N 55W 51 27104m20s
57 24 3238-Jul-0401:34:28 6338 2638 15318 T -p 0.6921 1.0664 65N 157W 46 30104m15s
58 25 3256-Jul-1409:04:02 6519 2703 15541 T -p 0.7632 1.0673 67N 105E 40 34104m06s
59 26 3274-Jul-2516:32:12 6702 2769 15764 T -p 0.8357 1.0672 68N 9E 33 40003m55s
60 27 3292-Aug-0500:01:21 6889 2836 15987 T -t 0.9076 1.0657 68N 84W 24 51403m39s
61 28 3310-Aug-1707:31:53 7077 2903 16210 T -t 0.9786 1.0619 66N 170W 11 104203m12s
62 29 3328-Aug-2715:06:22 7269 2971 16433 P -t 1.0466 0.9336 62N 92E 0 - -
63 30 3346-Sep-0722:43:09 7462 3040 16656 P -t 1.1129 0.8050 61N 30W 0 - -
64 31 3364-Sep-1806:26:02 7659 3109 16879 P -t 1.1743 0.6858 61N 153W 0 - -
65 32 3382-Sep-2914:13:27 7858 3180 17102 P -t 1.2321 0.5741 61N 82E 0 - -
66 33 3400-Oct-1022:08:27 8059 3250 17325 P -t 1.2838 0.4744 61N 45W 0 - -
67 34 3418-Oct-2206:08:48 8264 3322 17548 P -t 1.3311 0.3837 62N 173W 0 - -
68 35 3436-Nov-0114:17:48 8470 3394 17771 P -t 1.3716 0.3065 62N 57E 0 - -
69 36 3454-Nov-1222:33:07 8679 3467 17994 P -t 1.4068 0.2398 63N 75W 0 - -
70 37 3472-Nov-2306:56:05 8891 3541 18217 P -t 1.4359 0.1853 64N 151E 0 - -
71 38 3490-Dec-0415:25:16 9106 3615 18440 P -t 1.4600 0.1405 65N 15E 0 - -
72 39 3508-Dec-1600:01:16 9323 3690 18663 P -t 1.4784 0.1066 66N 123W 0 - -
73 40 3526-Dec-2708:42:08 9542 3765 18886 P -t 1.4932 0.0798 67N 97E 0 - -
74 41 3545-Jan-0617:26:42 9765 3842 19109 P -t 1.5049 0.0586 68N 44W 0 - -
75 42 3563-Jan-1802:14:39 9989 3919 19332 P -t 1.5140 0.0424 69N 174E 0 - -
76 43 3581-Jan-2811:04:25 10217 3997 19555 P -t 1.5213 0.0293 70N 31E 0 - -
77 44 3599-Feb-0819:53:56 10446 4075 19778 Pe -t 1.5292 0.0150 71N 113W 0 - -

Statistics for Solar Eclipses of Saros 166

Solar eclipses of Saros 166 all occur at the Moon’s descending node and the Moon moves northward with each eclipse. The series will begin with a partial eclipse in the southern hemisphere on 2228 Oct 29. The series will end with a partial eclipse in the northern hemisphere on 3599 Feb 08. The total duration of Saros series 166 is 1370.29 years.

Summary of Saros 166
First Eclipse 2228 Oct 29
Last Eclipse 3599 Feb 08
Series Duration 1370.29 Years
No. of Eclipses 77
Sequence 19P 21A 5H 16T 16P

Saros 166 is composed of 77 solar eclipses as follows:

Solar Eclipses of Saros 166
Eclipse Type Symbol Number Percent
All Eclipses - 77100.0%
PartialP 35 45.5%
AnnularA 21 27.3%
TotalT 16 20.8%
HybridH 5 6.5%

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 166 appears in the following table.

Umbral Eclipses of Saros 166
Classification Number Percent
All Umbral Eclipses 42100.0%
Central (two limits) 42100.0%
Central (one limit) 0 0.0%
Non-Central (one limit) 0 0.0%

The 77 eclipses in Saros 166 occur in the following order : 19P 21A 5H 16T 16P

The longest and shortest central eclipses of Saros 166 as well as largest and smallest partial eclipses appear below.

Extreme Durations and Magnitudes of Solar Eclipses of Saros 166
Extrema Type Date Duration Magnitude
Longest Annular Solar Eclipse 2571 May 2504m21s -
Shortest Annular Solar Eclipse 2931 Dec 3000m00s -
Longest Total Solar Eclipse 3202 Jun 1204m23s -
Shortest Total Solar Eclipse 3040 Mar 0501m56s -
Longest Hybrid Solar Eclipse 3022 Feb 2301m32s -
Shortest Hybrid Solar Eclipse 2950 Jan 0900m13s -
Largest Partial Solar Eclipse 3328 Aug 27 - 0.93362
Smallest Partial Solar Eclipse 3599 Feb 08 - 0.01502

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.