Saros 77

Catalog of Solar Eclipses of Saros 77

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 77

The table below lists the concise characteristics of every solar eclipse belonging to Saros 77 . 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 77
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 -0474-Jul-1114:09:13 16636 421 -30593 Pb t- 1.4889 0.1189 67N 142W 0 - -
2-32 -0456-Jul-2120:56:45 16324 414 -30370 P t- 1.4223 0.2363 68N 103E 0 - -
3-31 -0438-Aug-0203:47:55 16028 408 -30147 P t- 1.3588 0.3472 69N 12W 0 - -
4-30 -0420-Aug-1210:47:19 15739 401 -29924 P t- 1.3024 0.4447 70N 130W 0 - -
5-29 -0402-Aug-2317:52:48 15451 395 -29701 P t- 1.2511 0.5324 71N 110E 0 - -
6-28 -0384-Sep-0301:07:29 15180 388 -29478 P t- 1.2075 0.6064 71N 13W 0 - -
7-27 -0366-Sep-1408:29:16 14911 382 -29255 P t- 1.1699 0.6694 72N 139W 0 - -
8-26 -0348-Sep-2416:00:52 14645 376 -29032 P t- 1.1404 0.7182 72N 93E 0 - -
9-25 -0330-Oct-0523:39:28 14394 370 -28809 P t- 1.1170 0.7564 72N 37W 0 - -
10-24 -0312-Oct-1607:25:04 14143 363 -28586 P t- 1.0996 0.7846 72N 168W 0 - -
11-23 -0294-Oct-2715:16:58 13897 357 -28363 P t- 1.0875 0.8039 71N 59E 0 - -
12-22 -0276-Nov-0623:14:10 13660 351 -28140 P t- 1.0795 0.8164 70N 75W 0 - -
13-21 -0258-Nov-1807:14:35 13422 345 -27917 P t- 1.0746 0.8240 69N 152E 0 - -
14-20 -0240-Nov-2815:16:01 13192 339 -27694 P t- 1.0703 0.8307 68N 19E 0 - -
15-19 -0222-Dec-0923:18:00 12968 333 -27471 P t- 1.0666 0.8368 67N 114W 0 - -
16-18 -0204-Dec-2007:18:15 12743 327 -27248 P t- 1.0612 0.8461 66N 114E 0 - -
17-17 -0186-Dec-3115:14:19 12530 322 -27025 P t- 1.0523 0.8612 65N 16W 0 - -
18-16 -0167-Jan-1023:05:20 12318 316 -26802 P t- 1.0391 0.8838 64N 144W 0 - -
19-15 -0149-Jan-2206:49:33 12107 310 -26579 A+ t- 1.0202 0.9162 63N 90E 0 - -
20-14 -0131-Feb-0114:26:50 11907 304 -26356 An t- 0.9954 0.9121 60N 29W 4 - 07m44s
21-13 -0113-Feb-1221:54:28 11706 299 -26133 A t- 0.9623 0.9179 52N 135W 15 113807m42s
22-12 -0095-Feb-2305:14:12 11508 293 -25910 A p- 0.9224 0.9229 48N 115E 22 73307m19s
23-11 -0077-Mar-0612:24:15 11314 288 -25687 A p- 0.8743 0.9279 45N 8E 29 54006m50s
24-10 -0059-Mar-1619:25:25 11121 282 -25464 A p- 0.8186 0.9329 44N 96W 35 42206m19s
25 -9 -0041-Mar-2802:17:58 10931 277 -25241 A p- 0.7553 0.9377 43N 162E 41 34305m50s
26 -8 -0023-Apr-0709:03:25 10745 272 -25018 A p- 0.6858 0.9425 43N 63E 46 28505m23s
27 -7 -0005-Apr-1815:42:55 10559 266 -24795 A p- 0.6106 0.9470 42N 34W 52 24205m00s
28 -6 0013-Apr-2822:16:00 10379 261 -24572 A p- 0.5295 0.9512 42N 130W 58 20804m41s
29 -5 0031-May-1004:46:34 10202 256 -24349 A p- 0.4458 0.9549 41N 136E 63 18304m26s
30 -4 0049-May-2011:14:10 10025 251 -24126 A p- 0.3590 0.9583 39N 43E 69 16204m15s
31 -3 0067-May-3117:42:07 9851 246 -23903 A pn 0.2716 0.9612 37N 51W 74 14604m08s
32 -2 0085-Jun-1100:09:45 9678 241 -23680 A nn 0.1830 0.9636 34N 146W 79 13404m04s
33 -1 0103-Jun-2206:41:55 9504 236 -23457 A nn 0.0973 0.9654 29N 118E 84 12504m02s
34 0 0121-Jul-0213:17:21 9332 231 -23234 A nn 0.0138 0.9668 24N 19E 89 12004m02s
35 1 0139-Jul-1319:59:05 9160 226 -23011 A nn -0.0653 0.9678 19N 81W 86 11604m02s
36 2 0157-Jul-2402:47:20 8989 221 -22788 Am nn -0.1399 0.9683 13N 175E 82 11504m01s
37 3 0175-Aug-0409:44:43 8817 216 -22565 A nn -0.2077 0.9684 6N 69E 78 11603m59s
38 4 0193-Aug-1416:50:41 8645 212 -22342 A nn -0.2690 0.9683 0S 39W 74 11803m56s
39 5 0211-Aug-2600:06:04 8473 207 -22119 A -n -0.3233 0.9680 7S 151W 71 12203m51s
40 6 0229-Sep-0507:31:55 8301 202 -21896 A -n -0.3694 0.9676 14S 95E 68 12503m46s
Catalog of Solar Eclipses of Saros 77
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 0247-Sep-1615:08:14 8129 198 -21673 A -n -0.4077 0.9671 20S 22W 66 12903m40s
42 8 0265-Sep-2622:54:30 7957 193 -21450 A -p -0.4385 0.9669 26S 141W 64 13203m32s
43 9 0283-Oct-0806:50:49 7785 189 -21227 A -p -0.4619 0.9669 32S 98E 62 13403m24s
44 10 0301-Oct-1814:56:09 7613 184 -21004 A -p -0.4785 0.9672 37S 25W 61 13403m15s
45 11 0319-Oct-2923:09:56 7439 180 -20781 A -p -0.4891 0.9679 42S 149W 60 13203m04s
46 12 0337-Nov-0907:29:07 7265 176 -20558 A -p -0.4959 0.9691 47S 87E 60 12802m52s
47 13 0355-Nov-2015:55:03 7090 171 -20335 A -p -0.4982 0.9709 50S 37W 60 12102m38s
48 14 0373-Dec-0100:23:32 6913 167 -20112 A -p -0.4995 0.9732 52S 161W 60 11102m22s
49 15 0391-Dec-1208:54:56 6735 163 -19889 A -p -0.4990 0.9762 54S 75E 60 9802m04s
50 16 0409-Dec-2217:24:38 6557 159 -19666 A -p -0.5008 0.9797 54S 47W 60 8401m44s
51 17 0428-Jan-0301:54:37 6377 155 -19443 A -p -0.5032 0.9838 52S 170W 60 6601m22s
52 18 0446-Jan-1310:20:11 6198 151 -19220 A -p -0.5104 0.9884 51S 67E 59 4700m58s
53 19 0464-Jan-2418:41:51 6022 147 -18997 A -p -0.5214 0.9935 48S 56W 58 2600m32s
54 20 0482-Feb-0402:56:48 5846 143 -18774 A -p -0.5388 0.9989 45S 178W 57 400m05s
55 21 0500-Feb-1511:06:13 5670 139 -18551 H -p -0.5614 1.0046 42S 61E 56 1900m22s
56 22 0518-Feb-2519:08:12 5494 136 -18328 H -p -0.5911 1.0104 40S 60W 54 4400m50s
57 23 0536-Mar-0803:03:03 5319 132 -18105 T -p -0.6274 1.0162 37S 178W 51 7001m18s
58 24 0554-Mar-1910:50:37 5144 128 -17882 T -p -0.6707 1.0217 36S 65E 48 9801m44s
59 25 0572-Mar-2918:32:00 4972 125 -17659 T -p -0.7196 1.0270 35S 51W 44 12902m10s
60 26 0590-Apr-1002:06:31 4799 121 -17436 T -p -0.7750 1.0318 36S 165W 39 16602m33s
61 27 0608-Apr-2009:36:28 4629 117 -17213 T -p -0.8351 1.0358 38S 82E 33 21402m51s
62 28 0626-May-0117:01:37 4460 114 -16990 T -p -0.8996 1.0389 43S 29W 26 29403m02s
63 29 0644-May-1200:24:58 4292 111 -16767 T -t -0.9665 1.0400 52S 138W 14 53002m56s
64 30 0662-May-2307:44:32 4126 107 -16544 P -t -1.0370 0.9442 64S 119E 0 - -
65 31 0680-Jun-0215:04:49 3961 104 -16321 P -t -1.1074 0.8111 64S 2W 0 - -
66 32 0698-Jun-1322:24:13 3796 101 -16098 P -t -1.1787 0.6752 65S 122W 0 - -
67 33 0716-Jun-2405:46:42 3639 97 -15875 P -t -1.2482 0.5422 66S 116E 0 - -
68 34 0734-Jul-0513:10:10 3483 94 -15652 P -t -1.3171 0.4100 67S 6W 0 - -
69 35 0752-Jul-1520:39:31 3328 91 -15429 P -t -1.3815 0.2861 68S 130W 0 - -
70 36 0770-Jul-2704:12:45 3179 88 -15206 P -t -1.4427 0.1684 69S 104E 0 - -
71 37 0788-Aug-0611:52:45 3030 85 -14983 Pe -t -1.4988 0.0609 70S 24W 0 - -

Statistics for Solar Eclipses of Saros 77

Solar eclipses of Saros 77 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 -0474 Jul 11. The series ended with a partial eclipse in the southern hemisphere on 0788 Aug 06. The total duration of Saros series 77 is 1262.11 years.

Summary of Saros 77
First Eclipse -0474 Jul 11
Last Eclipse 0788 Aug 06
Series Duration 1262.11 Years
No. of Eclipses 71
Sequence 18P 36A 2H 7T 8P

Saros 77 is composed of 71 solar eclipses as follows:

Solar Eclipses of Saros 77
Eclipse Type Symbol Number Percent
All Eclipses - 71100.0%
PartialP 26 36.6%
AnnularA 36 50.7%
TotalT 7 9.9%
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 77 appears in the following table.

Umbral Eclipses of Saros 77
Classification Number Percent
All Umbral Eclipses 45100.0%
Central (two limits) 43 95.6%
Central (one limit) 1 2.2%
Non-Central (one limit) 1 2.2%

The 71 eclipses in Saros 77 occur in the following order : 18P 36A 2H 7T 8P

The longest and shortest central eclipses of Saros 77 as well as largest and smallest partial eclipses appear below.

Extreme Durations and Magnitudes of Solar Eclipses of Saros 77
Extrema Type Date Duration Magnitude
Longest Annular Solar Eclipse -0131 Feb 0107m44s -
Shortest Annular Solar Eclipse 0482 Feb 0400m05s -
Longest Total Solar Eclipse 0626 May 0103m02s -
Shortest Total Solar Eclipse 0536 Mar 0801m18s -
Longest Hybrid Solar Eclipse 0518 Feb 2500m50s -
Shortest Hybrid Solar Eclipse 0500 Feb 1500m22s -
Largest Partial Solar Eclipse 0662 May 23 - 0.94422
Smallest Partial Solar Eclipse 0788 Aug 06 - 0.06090

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.