Saros 153

Catalog of Solar Eclipses of Saros 153

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 153

The table below lists the concise characteristics of every solar eclipse belonging to Saros 153 . 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 153
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
1-34 1870-Jul-2811:02:31 1 0 -1601 Pb t- 1.5044 0.0742 69N 171E 0 - -
2-33 1888-Aug-0718:05:46 -6 0 -1378 P t- 1.4369 0.1983 70N 53E 0 - -
3-32 1906-Aug-2001:12:50 6 0 -1155 P t- 1.3731 0.3147 71N 66W 0 - -
4-31 1924-Aug-3008:23:00 24 0 -932 P t- 1.3123 0.4245 71N 173E 0 - -
5-30 1942-Sep-1015:39:32 26 0 -709 P t- 1.2571 0.5231 72N 50E 0 - -
6-29 1960-Sep-2022:59:56 33 0 -486 P t- 1.2057 0.6139 72N 74W 0 - -
7-28 1978-Oct-0206:28:43 49 0 -263 P t- 1.1616 0.6905 72N 160E 0 - -
8-27 1996-Oct-1214:03:04 62 0 -40 P t- 1.1227 0.7575 72N 32E 0 - -
9-26 2014-Oct-2321:45:39 68 0 183 P t- 1.0908 0.8114 71N 97W 0 - -
10-25 2032-Nov-0305:34:13 74 3 406 P t- 1.0643 0.8554 70N 133E 0 - -
11-24 2050-Nov-1413:30:53 83 9 629 P t- 1.0447 0.8874 70N 1E 0 - -
12-23 2068-Nov-2421:32:30 95 18 852 P t- 1.0299 0.9109 69N 131W 0 - -
13-22 2086-Dec-0605:38:55 109 29 1075 P p- 1.0194 0.9271 67N 96E 0 - -
14-21 2104-Dec-1713:48:27 125 41 1298 A+ p- 1.0120 0.9381 66N 37W 0 - -
15-20 2122-Dec-2822:00:56 145 55 1521 A+ p- 1.0072 0.9451 65N 170W 0 - -
16-19 2141-Jan-0806:12:38 166 70 1744 A+ p- 1.0024 0.9522 64N 57E 0 - -
17-18 2159-Jan-1914:23:26 191 86 1967 A+ p- 0.9974 0.9600 63N 75W 0 - -
18-17 2177-Jan-2922:30:30 218 104 2190 An p- 0.9897 0.9212 58N 164E 7 - 06m55s
19-16 2195-Feb-1006:34:27 247 123 2413 An p- 0.9797 0.9218 55N 41E 11 - 06m52s
20-15 2213-Feb-2114:30:14 279 143 2636 A p- 0.9635 0.9230 53N 79W 15 108006m44s
21-14 2231-Mar-0422:20:23 314 163 2859 A p- 0.9430 0.9246 52N 162E 19 83706m32s
22-13 2249-Mar-1506:00:45 351 185 3082 A p- 0.9149 0.9266 52N 47E 23 66606m18s
23-12 2267-Mar-2613:33:45 391 208 3305 A p- 0.8810 0.9290 52N 65W 28 54906m03s
24-11 2285-Apr-0520:55:22 433 232 3528 A p- 0.8378 0.9315 53N 172W 33 45905m50s
25-10 2303-Apr-1804:09:26 478 257 3751 A p- 0.7888 0.9341 54N 83E 38 39305m38s
26 -9 2321-Apr-2811:12:58 526 283 3974 A p- 0.7314 0.9367 54N 18W 43 34105m30s
27 -8 2339-May-0918:08:03 576 309 4197 A p- 0.6672 0.9392 55N 116W 48 30005m24s
28 -7 2357-May-2000:54:22 629 337 4420 A p- 0.5960 0.9415 54N 150E 53 26805m24s
29 -6 2375-May-3107:34:32 684 365 4643 A p- 0.5200 0.9436 52N 57E 58 24305m26s
30 -5 2393-Jun-1014:08:40 742 395 4866 A p- 0.4389 0.9453 49N 36W 64 22405m34s
31 -4 2411-Jun-2120:37:42 802 425 5089 A pn 0.3537 0.9467 44N 128W 69 21005m46s
32 -3 2429-Jul-0203:04:28 865 456 5312 A pn 0.2668 0.9476 39N 138E 74 20006m01s
33 -2 2447-Jul-1309:29:34 931 488 5535 A nn 0.1786 0.9481 32N 44E 80 19406m18s
34 -1 2465-Jul-2315:54:46 999 520 5758 A nn 0.0903 0.9482 25N 52W 85 19106m35s
35 0 2483-Aug-0322:21:16 1069 554 5981 A nn 0.0029 0.9479 17N 149W 90 19206m50s
36 1 2501-Aug-1504:52:07 1143 588 6204 Am nn -0.0811 0.9471 9N 112E 85 19507m01s
37 2 2519-Aug-2611:27:48 1219 623 6427 A nn -0.1611 0.9460 1N 11E 81 20107m08s
38 3 2537-Sep-0518:08:58 1297 659 6650 A nn -0.2368 0.9446 7S 91W 76 21007m11s
39 4 2555-Sep-1700:58:16 1378 696 6873 A nn -0.3062 0.9429 15S 165E 72 22107m10s
40 5 2573-Sep-2707:55:48 1461 733 7096 A -p -0.3691 0.9411 23S 58E 68 23307m06s
Catalog of Solar Eclipses of Saros 153
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 6 2591-Oct-0815:02:46 1548 772 7319 A -p -0.4245 0.9393 30S 50W 65 24707m00s
42 7 2609-Oct-1922:18:03 1636 811 7542 A -p -0.4735 0.9375 37S 161W 62 26306m53s
43 8 2627-Oct-3105:43:48 1728 851 7765 A -p -0.5141 0.9358 44S 88E 59 27806m44s
44 9 2645-Nov-1013:18:33 1821 891 7988 A -p -0.5477 0.9344 50S 25W 57 29306m35s
45 10 2663-Nov-2121:01:58 1918 933 8211 A -p -0.5748 0.9333 55S 138W 55 30506m26s
46 11 2681-Dec-0204:53:52 2017 975 8434 A -p -0.5952 0.9326 59S 109E 53 31406m18s
47 12 2699-Dec-1312:52:47 2118 1018 8657 A -p -0.6106 0.9325 61S 4W 52 32006m08s
48 13 2717-Dec-2420:58:03 2222 1062 8880 A -p -0.6211 0.9329 62S 117W 51 32106m00s
49 14 2736-Jan-0505:06:09 2329 1106 9103 A -p -0.6301 0.9340 61S 129E 51 31805m50s
50 15 2754-Jan-1513:18:41 2438 1151 9326 A -p -0.6359 0.9356 58S 12E 50 31005m39s
51 16 2772-Jan-2621:31:15 2550 1197 9549 A -p -0.6427 0.9378 55S 107W 50 30005m26s
52 17 2790-Feb-0605:44:11 2665 1244 9772 A -p -0.6496 0.9407 52S 132E 49 28605m12s
53 18 2808-Feb-1713:53:33 2782 1291 9995 A -p -0.6602 0.9441 48S 12E 48 27104m56s
54 19 2826-Feb-2722:00:56 2901 1339 10218 A -p -0.6730 0.9480 44S 110W 47 25404m38s
55 20 2844-Mar-1006:02:45 3023 1388 10441 A -p -0.6914 0.9523 41S 130E 46 23604m18s
56 21 2862-Mar-2113:59:03 3148 1438 10664 A -p -0.7149 0.9570 38S 11E 44 21803m55s
57 22 2880-Mar-3121:48:24 3275 1488 10887 A -p -0.7448 0.9619 37S 106W 42 20103m31s
58 23 2898-Apr-1205:31:36 3405 1539 11110 A -p -0.7802 0.9669 36S 138E 38 18503m06s
59 24 2916-Apr-2313:07:17 3538 1591 11333 A -p -0.8224 0.9718 37S 24E 34 17302m39s
60 25 2934-May-0420:36:32 3673 1644 11556 A -p -0.8707 0.9764 40S 89W 29 16802m12s
61 26 2952-May-1503:59:06 3810 1697 11779 A -p -0.9250 0.9803 45S 161E 22 18201m46s
62 27 2970-May-2611:17:01 3950 1751 12002 A -t -0.9835 0.9826 56S 55E 10 36401m26s
63 28 2988-Jun-0518:28:48 4093 1806 12225 P -t -1.0477 0.9016 65S 53W 0 - -
64 29 3006-Jun-1801:38:16 4238 1861 12448 P -t -1.1144 0.7827 66S 169W 0 - -
65 30 3024-Jun-2808:44:24 4386 1917 12671 P -t -1.1842 0.6568 67S 74E 0 - -
66 31 3042-Jul-0915:51:07 4537 1974 12894 P -t -1.2543 0.5291 68S 43W 0 - -
67 32 3060-Jul-1922:55:59 4690 2032 13117 P -t -1.3263 0.3969 69S 159W 0 - -
68 33 3078-Jul-3106:04:32 4845 2090 13340 P -t -1.3959 0.2683 70S 82E 0 - -
69 34 3096-Aug-1013:14:04 5003 2149 13563 P -t -1.4651 0.1397 70S 37W 0 - -
70 35 3114-Aug-2220:29:03 5164 2209 13786 Pe -t -1.5305 0.0176 71S 158W 0 - -

Statistics for Solar Eclipses of Saros 153

Solar eclipses of Saros 153 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 28. The series will end with a partial eclipse in the southern hemisphere on 3114 Aug 22. The total duration of Saros series 153 is 1244.08 years.

Summary of Saros 153
First Eclipse 1870 Jul 28
Last Eclipse 3114 Aug 22
Series Duration 1244.08 Years
No. of Eclipses 70
Sequence 13P 49A 8P

Saros 153 is composed of 70 solar eclipses as follows:

Solar Eclipses of Saros 153
Eclipse Type Symbol Number Percent
All Eclipses - 70100.0%
PartialP 21 30.0%
AnnularA 49 70.0%
TotalT 0 0.0%
HybridH 0 0.0%

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 153 appears in the following table.

Umbral Eclipses of Saros 153
Classification Number Percent
All Umbral Eclipses 49100.0%
Central (two limits) 43 87.8%
Central (one limit) 2 4.1%
Non-Central (one limit) 4 8.2%

The 70 eclipses in Saros 153 occur in the following order : 13P 49A 8P

The longest and shortest central eclipses of Saros 153 as well as largest and smallest partial eclipses appear below.

Extreme Durations and Magnitudes of Solar Eclipses of Saros 153
Extrema Type Date Duration Magnitude
Longest Annular Solar Eclipse 2537 Sep 0507m11s -
Shortest Annular Solar Eclipse 2970 May 2601m26s -
Largest Partial Solar Eclipse 2086 Dec 06 - 0.92712
Smallest Partial Solar Eclipse 3114 Aug 22 - 0.01761

Eclipse Publications

by Fred Espenak

jpeg jpeg
jpeg jpeg
jpeg jpeg

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.