Saros 161

Catalog of Solar Eclipses of Saros 161

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 161

The table below lists the concise characteristics of every solar eclipse belonging to Saros 161 . 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 161
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 2174-Apr-0122:39:09 213 101 2155 Pb t- 1.5106 0.0471 61N 103E 0 - -
2-36 2192-Apr-1206:41:56 243 120 2378 P t- 1.4678 0.1261 61N 26W 0 - -
3-35 2210-Apr-2414:39:19 274 139 2601 P t- 1.4202 0.2149 62N 154W 0 - -
4-34 2228-May-0422:28:44 308 160 2824 P t- 1.3659 0.3174 62N 80E 0 - -
5-33 2246-May-1606:14:10 345 182 3047 P t- 1.3076 0.4285 63N 46W 0 - -
6-32 2264-May-2613:52:06 385 205 3270 P t- 1.2430 0.5527 64N 169W 0 - -
7-31 2282-Jun-0621:28:18 427 228 3493 P t- 1.1764 0.6815 65N 67E 0 - -
8-30 2300-Jun-1804:59:28 471 253 3716 P t- 1.1056 0.8190 66N 55W 0 - -
9-29 2318-Jun-2912:30:21 518 279 3939 P t- 1.0340 0.9583 67N 178W 0 - -
10-28 2336-Jul-0919:58:21 568 305 4162 T t- 0.9598 1.0657 83N 48E 16 79903m18s
11-27 2354-Jul-2103:28:21 620 332 4385 T t- 0.8870 1.0697 81N 171E 27 49903m51s
12-26 2372-Jul-3110:58:29 675 361 4608 T p- 0.8144 1.0717 71N 44E 35 40404m18s
13-25 2390-Aug-1118:31:26 733 390 4831 T p- 0.7440 1.0724 61N 74W 42 35304m41s
14-24 2408-Aug-2202:07:38 793 420 5054 T p- 0.6765 1.0720 52N 169E 47 31705m00s
15-23 2426-Sep-0209:48:46 855 451 5277 T p- 0.6133 1.0709 44N 50E 52 29105m14s
16-22 2444-Sep-1217:35:34 920 483 5500 T p- 0.5548 1.0688 36N 69W 56 26805m24s
17-21 2462-Sep-2401:28:07 988 515 5723 T p- 0.5013 1.0662 28N 170E 60 24905m28s
18-20 2480-Oct-0409:27:57 1058 548 5946 T p- 0.4542 1.0631 21N 48E 63 23105m26s
19-19 2498-Oct-1517:34:43 1131 583 6169 T n- 0.4130 1.0597 15N 76W 66 21505m21s
20-18 2516-Oct-2701:48:44 1206 618 6392 T n- 0.3781 1.0560 9N 159E 68 19905m11s
21-17 2534-Nov-0710:10:05 1284 654 6615 T n- 0.3494 1.0522 4N 33E 70 18404m58s
22-16 2552-Nov-1718:38:44 1365 690 6838 T n- 0.3269 1.0485 0S 95W 71 17004m42s
23-15 2570-Nov-2903:13:42 1448 728 7061 T n- 0.3100 1.0449 3S 136E 72 15804m25s
24-14 2588-Dec-0911:53:26 1534 766 7284 T n- 0.2973 1.0416 6S 6E 73 14604m07s
25-13 2606-Dec-2120:37:54 1622 805 7507 T n- 0.2888 1.0387 7S 125W 73 13503m50s
26-12 2625-Jan-0105:25:24 1713 844 7730 T n- 0.2828 1.0361 7S 103E 74 12603m32s
27-11 2643-Jan-1214:14:03 1806 885 7953 T n- 0.2783 1.0341 6S 28W 74 11903m18s
28-10 2661-Jan-2223:02:20 1902 926 8176 T n- 0.2739 1.0324 4S 160W 74 11303m04s
29 -9 2679-Feb-0307:48:57 2001 968 8399 T n- 0.2684 1.0312 2S 68E 74 10902m54s
30 -8 2697-Feb-1316:33:02 2102 1011 8622 T n- 0.2612 1.0305 1N 63W 75 10602m46s
31 -7 2715-Feb-2601:11:16 2206 1055 8845 T n- 0.2495 1.0302 4N 168E 76 10502m42s
32 -6 2733-Mar-0809:44:47 2312 1099 9068 T n- 0.2342 1.0301 7N 39E 76 10402m39s
33 -5 2751-Mar-1918:10:32 2421 1144 9291 T n- 0.2130 1.0303 10N 87W 78 10502m38s
34 -4 2769-Mar-3002:29:28 2533 1190 9514 T n- 0.1865 1.0307 13N 149E 79 10502m40s
35 -3 2787-Apr-1010:38:54 2647 1236 9737 T nn 0.1524 1.0310 16N 27E 81 10602m43s
36 -2 2805-Apr-2018:41:05 2763 1284 9960 T nn 0.1129 1.0313 18N 92W 83 10602m46s
37 -1 2823-May-0202:34:01 2882 1332 10183 Tm nn 0.0661 1.0314 19N 151E 86 10602m51s
38 0 2841-May-1210:18:30 3004 1381 10406 T nn 0.0128 1.0312 19N 37E 89 10502m55s
39 1 2859-May-2317:54:30 3128 1430 10629 T nn -0.0468 1.0305 18N 75W 87 10302m58s
40 2 2877-Jun-0301:23:29 3255 1480 10852 T nn -0.1115 1.0294 16N 174E 84 10002m58s
Catalog of Solar Eclipses of Saros 161
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 2895-Jun-1408:45:45 3385 1531 11075 T -n -0.1812 1.0278 13N 65E 80 9602m55s
42 4 2913-Jun-2516:01:33 3517 1583 11298 T -n -0.2552 1.0255 9N 44W 75 9002m46s
43 5 2931-Jul-0623:13:19 3651 1636 11521 T -p -0.3317 1.0226 3N 152W 71 8102m30s
44 6 2949-Jul-1706:21:22 3788 1689 11744 T -p -0.4100 1.0189 3S 101E 66 7102m06s
45 7 2967-Jul-2813:27:17 3928 1743 11967 H3 -p -0.4893 1.0147 10S 8W 61 5801m37s
46 8 2985-Aug-0720:31:45 4071 1797 12190 H -p -0.5687 1.0097 18S 116W 55 4101m02s
47 9 3003-Aug-2003:37:03 4215 1852 12413 H -p -0.6464 1.0042 27S 134E 50 1900m26s
48 10 3021-Aug-3010:44:23 4363 1908 12636 A -p -0.7211 0.9980 36S 23E 44 1000m11s
49 11 3039-Sep-1017:53:31 4513 1965 12859 A -p -0.7933 0.9914 45S 89W 37 4900m46s
50 12 3057-Sep-2101:07:52 4666 2023 13082 A -t -0.8602 0.9842 55S 154E 30 10901m17s
51 13 3075-Oct-0208:26:33 4821 2081 13305 A -t -0.9226 0.9765 65S 30E 22 21901m44s
52 14 3093-Oct-1215:52:42 4978 2140 13528 A -t -0.9780 0.9678 74S 118W 11 59402m06s
53 15 3111-Oct-2423:23:20 5139 2199 13751 P -t -1.0287 0.9239 71S 79E 0 - -
54 16 3129-Nov-0407:02:31 5302 2260 13974 P -t -1.0715 0.8467 71S 48W 0 - -
55 17 3147-Nov-1514:47:06 5467 2321 14197 P -t -1.1091 0.7795 70S 176W 0 - -
56 18 3165-Nov-2522:39:22 5635 2382 14420 P -t -1.1398 0.7252 69S 55E 0 - -
57 19 3183-Dec-0706:36:40 5806 2445 14643 P -t -1.1655 0.6799 68S 75W 0 - -
58 20 3201-Dec-1714:40:41 5979 2508 14866 P -t -1.1853 0.6454 67S 154E 0 - -
59 21 3219-Dec-2822:48:07 6155 2572 15089 P -t -1.2014 0.6174 65S 22E 0 - -
60 22 3238-Jan-0806:58:45 6333 2636 15312 P -t -1.2144 0.5950 64S 109W 0 - -
61 23 3256-Jan-1915:10:29 6514 2701 15535 P -t -1.2259 0.5755 64S 119E 0 - -
62 24 3274-Jan-2923:23:12 6697 2767 15758 P -t -1.2363 0.5578 63S 12W 0 - -
63 25 3292-Feb-1007:33:04 6884 2834 15981 P -t -1.2483 0.5375 62S 143W 0 - -
64 26 3310-Feb-2115:40:15 7072 2901 16204 P -t -1.2620 0.5145 62S 87E 0 - -
65 27 3328-Mar-0323:41:59 7263 2969 16427 P -t -1.2796 0.4847 61S 41W 0 - -
66 28 3346-Mar-1507:39:03 7457 3038 16650 P -t -1.3007 0.4493 61S 168W 0 - -
67 29 3364-Mar-2515:26:36 7654 3108 16873 P -t -1.3289 0.4017 61S 67E 0 - -
68 30 3382-Apr-0523:07:41 7852 3178 17096 P -t -1.3617 0.3462 61S 56W 0 - -
69 31 3400-Apr-1706:38:19 8054 3248 17319 P -t -1.4022 0.2775 62S 176W 0 - -
70 32 3418-Apr-2814:01:18 8258 3320 17542 P -t -1.4482 0.1992 62S 65E 0 - -
71 33 3436-May-0821:12:59 8465 3392 17765 P -t -1.5028 0.1062 63S 51W 0 - -
72 34 3454-May-2004:17:39 8674 3465 17988 Pe -t -1.5620 0.0048 64S 165W 0 - -

Statistics for Solar Eclipses of Saros 161

Solar eclipses of Saros 161 all occur at the Moon’s ascending node and the Moon moves southward with each eclipse. The series will begin with a partial eclipse in the northern hemisphere on 2174 Apr 01. The series will end with a partial eclipse in the southern hemisphere on 3454 May 20. The total duration of Saros series 161 is 1280.14 years.

Summary of Saros 161
First Eclipse 2174 Apr 01
Last Eclipse 3454 May 20
Series Duration 1280.14 Years
No. of Eclipses 72
Sequence 9P 35T 3H 5A 20P

Saros 161 is composed of 72 solar eclipses as follows:

Solar Eclipses of Saros 161
Eclipse Type Symbol Number Percent
All Eclipses - 72100.0%
PartialP 29 40.3%
AnnularA 5 6.9%
TotalT 35 48.6%
HybridH 3 4.2%

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 161 appears in the following table.

Umbral Eclipses of Saros 161
Classification Number Percent
All Umbral Eclipses 43100.0%
Central (two limits) 43100.0%
Central (one limit) 0 0.0%
Non-Central (one limit) 0 0.0%

The 72 eclipses in Saros 161 occur in the following order : 9P 35T 3H 5A 20P

The longest and shortest central eclipses of Saros 161 as well as largest and smallest partial eclipses appear below.

Extreme Durations and Magnitudes of Solar Eclipses of Saros 161
Extrema Type Date Duration Magnitude
Longest Annular Solar Eclipse 3093 Oct 1202m06s -
Shortest Annular Solar Eclipse 3021 Aug 3000m11s -
Longest Total Solar Eclipse 2462 Sep 2405m28s -
Shortest Total Solar Eclipse 2949 Jul 1702m06s -
Longest Hybrid Solar Eclipse 2967 Jul 2801m37s -
Shortest Hybrid Solar Eclipse 3003 Aug 2000m26s -
Largest Partial Solar Eclipse 2318 Jun 29 - 0.95834
Smallest Partial Solar Eclipse 3454 May 20 - 0.00485

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.