Saros 163

Catalog of Solar Eclipses of Saros 163

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 163

The table below lists the concise characteristics of every solar eclipse belonging to Saros 163 . 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 163
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
1-33 2286-Mar-2520:37:47 436 233 3540 Pb t- 1.5392 0.0473 61N 140E 0 - -
2-32 2304-Apr-0604:00:21 481 258 3763 P t- 1.4956 0.1190 61N 21E 0 - -
3-31 2322-Apr-1711:14:22 529 284 3986 P t- 1.4445 0.2042 62N 96W 0 - -
4-30 2340-Apr-2718:21:32 579 311 4209 P t- 1.3872 0.3006 62N 149E 0 - -
5-29 2358-May-0901:21:14 632 338 4432 P t- 1.3230 0.4098 63N 35E 0 - -
6-28 2376-May-1908:14:43 687 367 4655 P t- 1.2528 0.5305 63N 77W 0 - -
7-27 2394-May-3015:03:02 745 396 4878 P t- 1.1774 0.6610 64N 172E 0 - -
8-26 2412-Jun-0921:48:03 805 426 5101 P t- 1.0987 0.7984 65N 61E 0 - -
9-25 2430-Jun-2104:29:25 869 457 5324 P t- 1.0160 0.9439 66N 49W 0 - -
10-24 2448-Jul-0111:10:15 934 489 5547 A t- 0.9316 0.9620 88N 136W 21 38802m26s
11-23 2466-Jul-1217:50:50 1003 522 5770 A t- 0.8460 0.9676 79N 67W 32 22102m18s
12-22 2484-Jul-2300:34:33 1073 556 5993 A p- 0.7618 0.9720 69N 167W 40 15602m10s
13-21 2502-Aug-0407:19:51 1147 590 6216 A p- 0.6778 0.9756 59N 90E 47 11902m03s
14-20 2520-Aug-1414:11:40 1223 625 6439 A p- 0.5983 0.9784 50N 14W 53 9601m57s
15-19 2538-Aug-2521:08:12 1301 661 6662 A p- 0.5217 0.9806 41N 120W 58 8101m52s
16-18 2556-Sep-0504:13:24 1382 698 6885 A p- 0.4510 0.9823 32N 131E 63 7001m48s
17-17 2574-Sep-1611:24:59 1466 736 7108 A p- 0.3847 0.9835 24N 21E 67 6301m45s
18-16 2592-Sep-2618:46:59 1552 774 7331 A p- 0.3261 0.9844 16N 92W 71 5801m42s
19-15 2610-Oct-0902:17:24 1641 813 7554 A n- 0.2736 0.9849 9N 154E 74 5501m41s
20-14 2628-Oct-1909:57:21 1733 853 7777 A n- 0.2283 0.9854 3N 38E 77 5301m39s
21-13 2646-Oct-3017:46:56 1826 894 8000 A n- 0.1902 0.9857 3S 81W 79 5101m38s
22-12 2664-Nov-1001:46:07 1923 935 8223 A n- 0.1590 0.9861 8S 159E 81 5001m36s
23-11 2682-Nov-2109:54:28 2022 977 8446 A n- 0.1350 0.9866 12S 37E 82 4801m32s
24-10 2700-Dec-0218:09:34 2124 1020 8669 A n- 0.1158 0.9874 15S 86W 83 4501m26s
25 -9 2718-Dec-1402:32:43 2228 1064 8892 A n- 0.1027 0.9885 17S 149E 84 4101m17s
26 -8 2736-Dec-2411:00:54 2335 1108 9115 A n- 0.0926 0.9900 18S 23E 85 3501m06s
27 -7 2755-Jan-0419:33:44 2444 1154 9338 A n- 0.0859 0.9920 18S 104W 85 2800m52s
28 -6 2773-Jan-1504:08:29 2556 1200 9561 A n- 0.0800 0.9945 17S 129E 86 1900m35s
29 -5 2791-Jan-2612:45:13 2671 1246 9784 A nn 0.0750 0.9975 15S 1E 86 900m15s
30 -4 2809-Feb-0521:20:54 2788 1294 10007 H nn 0.0683 1.0011 12S 127W 86 400m06s
31 -3 2827-Feb-1705:54:39 2908 1342 10230 H nn 0.0593 1.0052 9S 105E 87 1800m30s
32 -2 2845-Feb-2714:24:58 3030 1391 10453 H nn 0.0466 1.0098 6S 22W 87 3400m55s
33 -1 2863-Mar-1022:51:03 3155 1441 10676 H nn 0.0298 1.0147 2S 148W 88 5001m21s
34 0 2881-Mar-2107:10:43 3282 1491 10899 T nn 0.0070 1.0201 1N 87E 90 6801m49s
35 1 2899-Apr-0115:24:29 3412 1542 11122 T nn -0.0213 1.0255 4N 35W 89 8702m17s
36 2 2917-Apr-1223:31:10 3545 1594 11345 T nn -0.0561 1.0312 6N 156W 87 10602m48s
37 3 2935-Apr-2407:32:08 3680 1647 11568 Tm nn -0.0965 1.0368 8N 84E 85 12403m20s
38 4 2953-May-0415:24:29 3818 1700 11791 T nn -0.1444 1.0424 9N 33W 82 14303m54s
39 5 2971-May-1523:12:06 3958 1754 12014 T -n -0.1968 1.0476 8N 148W 79 16104m27s
40 6 2989-May-2606:52:39 4101 1809 12237 T -n -0.2556 1.0525 7N 98E 75 17905m00s
Catalog of Solar Eclipses of Saros 163
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 7 3007-Jun-0714:29:51 4246 1864 12460 T -n -0.3178 1.0568 4N 16W 71 19705m30s
42 8 3025-Jun-1722:01:08 4394 1920 12683 T -n -0.3856 1.0606 1N 129W 67 21605m56s
43 9 3043-Jun-2905:31:30 4545 1977 12906 T -p -0.4546 1.0636 4S 119E 63 23406m13s
44 10 3061-Jul-0912:58:51 4698 2035 13129 T -p -0.5263 1.0659 10S 6E 58 25306m20s
45 11 3079-Jul-2020:26:17 4854 2093 13352 T -p -0.5985 1.0673 16S 108W 53 27406m16s
46 12 3097-Jul-3103:53:03 5012 2152 13575 T -p -0.6718 1.0678 24S 138E 48 29806m02s
47 13 3115-Aug-1211:22:42 5173 2212 13798 T -p -0.7427 1.0674 32S 22E 42 32705m38s
48 14 3133-Aug-2218:54:37 5336 2272 14021 T -p -0.8121 1.0661 41S 96W 35 36805m07s
49 15 3151-Sep-0302:30:11 5502 2334 14244 T -p -0.8785 1.0637 51S 142E 28 43504m30s
50 16 3169-Sep-1310:10:42 5671 2395 14467 T -t -0.9409 1.0600 62S 14E 19 58903m49s
51 17 3187-Sep-2417:57:04 5842 2458 14690 T- -t -0.9985 1.0232 72S 159W 0 - -
52 18 3205-Oct-0501:49:45 6016 2521 14913 P -t -1.0511 0.9210 72S 70E 0 - -
53 19 3223-Oct-1609:48:49 6192 2585 15136 P -t -1.0984 0.8293 72S 63W 0 - -
54 20 3241-Oct-2617:55:35 6371 2650 15359 P -t -1.1396 0.7498 71S 162E 0 - -
55 21 3259-Nov-0702:09:52 6552 2715 15582 P -t -1.1746 0.6823 70S 27E 0 - -
56 22 3277-Nov-1710:30:43 6736 2781 15805 P -t -1.2045 0.6250 69S 110W 0 - -
57 23 3295-Nov-2818:59:24 6923 2848 16028 P -t -1.2282 0.5797 68S 112E 0 - -
58 24 3313-Dec-1003:34:23 7112 2916 16251 P -t -1.2473 0.5434 67S 27W 0 - -
59 25 3331-Dec-2112:15:45 7304 2984 16474 P -t -1.2612 0.5171 66S 167W 0 - -
60 26 3349-Dec-3121:00:07 7498 3053 16697 P -t -1.2729 0.4951 65S 52E 0 - -
61 27 3368-Jan-1205:49:14 7695 3122 16920 P -t -1.2810 0.4799 64S 89W 0 - -
62 28 3386-Jan-2214:39:37 7895 3192 17143 P -t -1.2886 0.4657 63S 130E 0 - -
63 29 3404-Feb-0323:30:51 8097 3263 17366 P -t -1.2955 0.4529 63S 11W 0 - -
64 30 3422-Feb-1408:20:10 8301 3335 17589 P -t -1.3041 0.4368 62S 152W 0 - -
65 31 3440-Feb-2517:07:43 8509 3407 17812 P -t -1.3141 0.4180 62S 69E 0 - -
66 32 3458-Mar-0801:50:53 8718 3480 18035 P -t -1.3278 0.3924 61S 70W 0 - -
67 33 3476-Mar-1810:28:31 8931 3554 18258 P -t -1.3458 0.3584 61S 153E 0 - -
68 34 3494-Mar-2919:00:06 9145 3629 18481 P -t -1.3688 0.3150 61S 17E 0 - -
69 35 3512-Apr-1003:24:42 9363 3704 18704 P -t -1.3971 0.2616 62S 117W 0 - -
70 36 3530-Apr-2111:41:10 9583 3779 18927 P -t -1.4319 0.1957 62S 111E 0 - -
71 37 3548-May-0119:49:45 9806 3856 19150 P -t -1.4727 0.1183 62S 19W 0 - -
72 38 3566-May-1303:50:15 10031 3933 19373 Pe -t -1.5198 0.0291 63S 147W 0 - -

Statistics for Solar Eclipses of Saros 163

Solar eclipses of Saros 163 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 2286 Mar 25. The series will end with a partial eclipse in the southern hemisphere on 3566 May 13. The total duration of Saros series 163 is 1280.14 years.

Summary of Saros 163
First Eclipse 2286 Mar 25
Last Eclipse 3566 May 13
Series Duration 1280.14 Years
No. of Eclipses 72
Sequence 9P 20A 4H 18T 21P

Saros 163 is composed of 72 solar eclipses as follows:

Solar Eclipses of Saros 163
Eclipse Type Symbol Number Percent
All Eclipses - 72100.0%
PartialP 30 41.7%
AnnularA 20 27.8%
TotalT 18 25.0%
HybridH 4 5.6%

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 163 appears in the following table.

Umbral Eclipses of Saros 163
Classification Number Percent
All Umbral Eclipses 42100.0%
Central (two limits) 41 97.6%
Central (one limit) 0 0.0%
Non-Central (one limit) 1 2.4%

The 72 eclipses in Saros 163 occur in the following order : 9P 20A 4H 18T 21P

The longest and shortest central eclipses of Saros 163 as well as largest and smallest partial eclipses appear below.

Extreme Durations and Magnitudes of Solar Eclipses of Saros 163
Extrema Type Date Duration Magnitude
Longest Annular Solar Eclipse 2448 Jul 0102m26s -
Shortest Annular Solar Eclipse 2791 Jan 2600m15s -
Longest Total Solar Eclipse 3061 Jul 0906m20s -
Shortest Total Solar Eclipse 2881 Mar 2101m49s -
Longest Hybrid Solar Eclipse 2863 Mar 1001m21s -
Shortest Hybrid Solar Eclipse 2809 Feb 0500m06s -
Largest Partial Solar Eclipse 2430 Jun 21 - 0.94393
Smallest Partial Solar Eclipse 3566 May 13 - 0.02910

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.