Saros 35

Catalog of Solar Eclipses of Saros 35

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 35

The table below lists the concise characteristics of every solar eclipse belonging to Saros 35 . 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 35
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
1-35 -1870-Jul-2501:47:05 43272 3202 -47859 Pb t- 1.5603 0.0076 67N 152E 0 - -
2-34 -1852-Aug-0408:40:42 42850 3131 -47636 P t- 1.5012 0.1087 68N 35E 0 - -
3-33 -1834-Aug-1515:44:57 42430 3062 -47413 P t- 1.4496 0.1966 69N 84W 0 - -
4-32 -1816-Aug-2522:59:12 42012 2993 -47190 P t- 1.4053 0.2720 70N 153E 0 - -
5-31 -1798-Sep-0606:24:50 41596 2925 -46967 P t- 1.3694 0.3328 71N 27E 0 - -
6-30 -1780-Sep-1614:00:24 41182 2857 -46744 P t- 1.3408 0.3812 71N 102W 0 - -
7-29 -1762-Sep-2721:44:57 40770 2790 -46521 P t- 1.3187 0.4183 72N 126E 0 - -
8-28 -1744-Oct-0805:38:47 40360 2724 -46298 P t- 1.3034 0.4441 72N 8W 0 - -
9-27 -1726-Oct-1913:39:26 39952 2659 -46075 P t- 1.2926 0.4623 72N 144W 0 - -
10-26 -1708-Oct-2921:46:24 39547 2594 -45852 P t- 1.2865 0.4724 71N 78E 0 - -
11-25 -1690-Nov-1005:55:45 39143 2530 -45629 P t- 1.2816 0.4808 71N 59W 0 - -
12-24 -1672-Nov-2014:08:45 38742 2466 -45406 P t- 1.2790 0.4851 70N 163E 0 - -
13-23 -1654-Dec-0122:20:48 38342 2404 -45183 P t- 1.2746 0.4927 69N 26E 0 - -
14-22 -1636-Dec-1206:31:48 37945 2342 -44960 P t- 1.2688 0.5025 68N 110W 0 - -
15-21 -1618-Dec-2314:38:14 37550 2280 -44737 P t- 1.2583 0.5204 67N 116E 0 - -
16-20 -1599-Jan-0222:41:00 37156 2220 -44514 P t- 1.2441 0.5450 66N 17W 0 - -
17-19 -1581-Jan-1406:37:19 36765 2160 -44291 P t- 1.2236 0.5807 64N 148W 0 - -
18-18 -1563-Jan-2414:26:58 36376 2101 -44068 P t- 1.1967 0.6279 64N 84E 0 - -
19-17 -1545-Feb-0422:08:59 35989 2043 -43845 P t- 1.1623 0.6887 63N 43W 0 - -
20-16 -1527-Feb-1505:43:57 35604 1985 -43622 P t- 1.1212 0.7621 62N 167W 0 - -
21-15 -1509-Feb-2613:10:43 35221 1928 -43399 P t- 1.0723 0.8503 61N 70E 0 - -
22-14 -1491-Mar-0820:31:00 34841 1872 -43176 P t- 1.0167 0.9515 61N 50W 0 - -
23-13 -1473-Mar-2003:44:31 34462 1816 -42953 A t- 0.9543 0.9823 54N 140W 17 20801m19s
24-12 -1455-Mar-3010:53:50 34085 1761 -42730 A t- 0.8872 0.9909 50N 118E 27 6700m42s
25-11 -1437-Apr-1017:56:42 33711 1707 -42507 A p- 0.8135 0.9987 48N 16E 35 800m06s
26-10 -1419-Apr-2100:57:55 33338 1654 -42284 H p- 0.7374 1.0056 47N 87W 42 2800m26s
27 -9 -1401-May-0207:55:42 32968 1601 -42061 H p- 0.6574 1.0118 46N 172E 49 5300m55s
28 -8 -1383-May-1214:54:49 32599 1549 -41838 T p- 0.5771 1.0173 45N 70E 55 7201m22s
29 -7 -1365-May-2321:52:32 32233 1498 -41615 T p- 0.4947 1.0220 45N 31W 60 8601m47s
30 -6 -1347-Jun-0304:54:55 31869 1447 -41392 T p- 0.4149 1.0260 43N 134W 65 9702m09s
31 -5 -1329-Jun-1411:59:32 31506 1397 -41169 T p- 0.3363 1.0292 41N 123E 70 10502m30s
32 -4 -1311-Jun-2419:10:27 31146 1348 -40946 T n- 0.2620 1.0317 39N 17E 75 11102m48s
33 -3 -1293-Jul-0602:26:13 30788 1300 -40723 T n- 0.1907 1.0335 35N 91W 79 11503m04s
34 -2 -1275-Jul-1609:50:47 30432 1253 -40500 T nn 0.1258 1.0347 31N 159E 83 11803m16s
35 -1 -1257-Jul-2717:22:48 30078 1206 -40277 T nn 0.0665 1.0352 26N 45E 86 11903m24s
36 0 -1239-Aug-0701:03:39 29726 1160 -40054 T nn 0.0138 1.0354 21N 71W 89 11903m28s
37 1 -1221-Aug-1808:53:57 29377 1114 -39831 T nn -0.0316 1.0351 16N 169E 88 11803m27s
38 2 -1203-Aug-2816:54:00 29029 1070 -39608 T nn -0.0694 1.0347 10N 47E 86 11703m24s
39 3 -1185-Sep-0901:03:44 28683 1026 -39385 T nn -0.0998 1.0341 5N 78W 84 11603m19s
40 4 -1167-Sep-1909:21:52 28340 983 -39162 T nn -0.1237 1.0336 1S 155E 83 11403m14s
Catalog of Solar Eclipses of Saros 35
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 5 -1149-Sep-3017:49:03 27998 941 -38939 T -n -0.1404 1.0331 6S 26E 82 11303m09s
42 6 -1131-Oct-1102:23:24 27659 899 -38716 T -n -0.1516 1.0329 11S 105W 81 11203m05s
43 7 -1113-Oct-2211:03:57 27321 858 -38493 Tm -n -0.1581 1.0330 16S 123E 81 11303m04s
44 8 -1095-Nov-0119:49:40 26986 818 -38270 T -n -0.1607 1.0335 21S 10W 81 11403m05s
45 9 -1077-Nov-1304:39:05 26653 779 -38047 T -n -0.1608 1.0345 25S 144W 81 11803m08s
46 10 -1059-Nov-2313:30:06 26322 741 -37824 T -n -0.1598 1.0360 28S 83E 81 12303m15s
47 11 -1041-Dec-0422:20:52 25993 703 -37601 T -n -0.1595 1.0380 30S 49W 81 12903m23s
48 12 -1023-Dec-1507:10:34 25666 666 -37378 T -n -0.1605 1.0405 32S 179E 81 13703m34s
49 13 -1005-Dec-2615:57:28 25341 630 -37155 T -n -0.1645 1.0434 33S 48E 80 14703m46s
50 14 -0986-Jan-0600:39:08 25018 617 -36932 T -n -0.1732 1.0467 34S 81W 80 15803m59s
51 15 -0968-Jan-1709:15:20 24697 610 -36709 T -n -0.1869 1.0503 33S 150E 79 17004m12s
52 16 -0950-Jan-2717:44:30 24378 603 -36486 T -n -0.2069 1.0541 32S 24E 78 18304m25s
53 17 -0932-Feb-0802:07:10 24062 596 -36263 T -n -0.2327 1.0579 31S 101W 76 19604m38s
54 18 -0914-Feb-1810:20:30 23747 589 -36040 T -n -0.2666 1.0617 29S 136E 74 21004m51s
55 19 -0896-Feb-2918:27:12 23434 582 -35817 T -n -0.3065 1.0652 27S 14E 72 22305m04s
56 20 -0878-Mar-1202:24:49 23124 576 -35594 T -n -0.3540 1.0685 25S 106W 69 23705m16s
57 21 -0860-Mar-2210:15:59 22816 569 -35371 T -n -0.4071 1.0712 24S 136E 66 25105m28s
58 22 -0842-Apr-0217:59:02 22509 562 -35148 T -p -0.4672 1.0733 23S 20E 62 26605m39s
59 23 -0824-Apr-1301:37:13 22205 555 -34925 T -p -0.5312 1.0747 22S 95W 58 28205m49s
60 24 -0806-Apr-2409:09:52 21903 548 -34702 T -p -0.5999 1.0752 23S 151E 53 30005m56s
61 25 -0788-May-0416:38:07 21603 541 -34479 T -p -0.6722 1.0747 25S 38E 48 32205m59s
62 26 -0770-May-1600:03:28 21305 534 -34256 T -p -0.7466 1.0732 28S 75W 42 35105m54s
63 27 -0752-May-2607:27:18 21009 528 -34033 T -p -0.8219 1.0705 33S 172E 34 39805m40s
64 28 -0734-Jun-0614:51:02 20715 521 -33810 T -t -0.8973 1.0665 40S 60E 26 49005m12s
65 29 -0716-Jun-1622:14:52 20423 514 -33587 T -t -0.9720 1.0601 52S 52W 13 87004m21s
66 30 -0698-Jun-2805:41:34 20133 507 -33364 P -t -1.0440 0.9362 65S 166W 0 - -
67 31 -0680-Jul-0813:11:32 19845 500 -33141 P -t -1.1126 0.8029 66S 70E 0 - -
68 32 -0662-Jul-1920:45:36 19560 493 -32918 P -t -1.1773 0.6777 67S 56W 0 - -
69 33 -0644-Jul-3004:24:46 19276 485 -32695 P -t -1.2373 0.5626 68S 177E 0 - -
70 34 -0626-Aug-1012:10:23 18995 478 -32472 P -t -1.2915 0.4595 69S 47E 0 - -
71 35 -0608-Aug-2020:03:11 18715 471 -32249 P -t -1.3390 0.3701 70S 85W 0 - -
72 36 -0590-Sep-0104:01:56 18439 464 -32026 P -t -1.3810 0.2919 71S 141E 0 - -
73 37 -0572-Sep-1112:09:16 18164 457 -31803 P -t -1.4155 0.2288 71S 5E 0 - -
74 38 -0554-Sep-2220:23:22 17890 451 -31580 P -t -1.4440 0.1773 72S 134W 0 - -
75 39 -0536-Oct-0304:45:34 17620 444 -31357 P -t -1.4656 0.1392 72S 85E 0 - -
76 40 -0518-Oct-1413:12:21 17351 437 -31134 P -t -1.4829 0.1093 72S 57W 0 - -
77 41 -0500-Oct-2421:46:06 17080 430 -30911 P -t -1.4941 0.0906 71S 160E 0 - -
78 42 -0482-Nov-0506:22:59 16768 424 -30688 P -t -1.5025 0.0771 70S 16E 0 - -
79 43 -0464-Nov-1515:03:19 16457 417 -30465 P -t -1.5078 0.0691 69S 128W 0 - -
80 44 -0446-Nov-2623:44:12 16151 410 -30242 P -t -1.5124 0.0622 69S 88E 0 - -
Catalog of Solar Eclipses of Saros 35
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
81 45 -0428-Dec-0708:25:39 15862 404 -30019 P -t -1.5163 0.0563 67S 55W 0 - -
82 46 -0410-Dec-1817:03:51 15574 397 -29796 P -t -1.5223 0.0466 66S 164E 0 - -
83 47 -0392-Dec-2901:38:16 15295 391 -29573 P -t -1.5309 0.0319 65S 24E 0 - -
84 48 -0373-Jan-0910:06:56 15026 385 -29350 Pe -t -1.5436 0.0096 64S 115W 0 - -

Statistics for Solar Eclipses of Saros 35

Solar eclipses of Saros 35 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 -1870 Jul 25. The series ended with a partial eclipse in the southern hemisphere on -0373 Jan 09. The total duration of Saros series 35 is 1496.50 years.

Summary of Saros 35
First Eclipse -1870 Jul 25
Last Eclipse -0373 Jan 09
Series Duration 1496.50 Years
No. of Eclipses 84
Sequence 22P 3A 2H 38T 19P

Saros 35 is composed of 84 solar eclipses as follows:

Solar Eclipses of Saros 35
Eclipse Type Symbol Number Percent
All Eclipses - 84100.0%
PartialP 41 48.8%
AnnularA 3 3.6%
TotalT 38 45.2%
HybridH 2 2.4%

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 35 appears in the following table.

Umbral Eclipses of Saros 35
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 84 eclipses in Saros 35 occur in the following order : 22P 3A 2H 38T 19P

The longest and shortest central eclipses of Saros 35 as well as largest and smallest partial eclipses appear below.

Extreme Durations and Magnitudes of Solar Eclipses of Saros 35
Extrema Type Date Duration Magnitude
Longest Annular Solar Eclipse -1473 Mar 2001m19s -
Shortest Annular Solar Eclipse -1437 Apr 1000m06s -
Longest Total Solar Eclipse -0788 May 0405m59s -
Shortest Total Solar Eclipse -1383 May 1201m22s -
Longest Hybrid Solar Eclipse -1401 May 0200m55s -
Shortest Hybrid Solar Eclipse -1419 Apr 2100m26s -
Largest Partial Solar Eclipse -1491 Mar 08 - 0.95150
Smallest Partial Solar Eclipse -1870 Jul 25 - 0.00761

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.