Solar Saros 139

Last updated
Historic saros cycle animation Saros139animated.gif
Historic saros cycle animation
January 22, 1898
Series member 23 Solar eclipse 1898Jan22-corona-India-Maunder.png
January 22, 1898
Series member 23
The solar eclipse of March 29, 2006 from Side, Turkey
Series member 29 Diamondring-eclipse-March03-29-2006.jpg
The solar eclipse of March 29, 2006 from Side, Turkey
Series member 29
The solar eclipse of April 8, 2024 from Indianapolis, Indiana
Series member 30 Solar eclipse of April 2024 from Indianapolis.jpg
The solar eclipse of April 8, 2024 from Indianapolis, Indiana
Series member 30

Saros cycle series 139 for solar eclipses occurs at the Moon's ascending node repeating every 18 years and 11 days, containing 71 eclipses, including 55 umbral eclipses, 12 of which will be hybrid and 43 of which will be total. The first eclipse was on 17 May 1501 and the last will be on 3 July 2763. The most recent eclipse was on 8 April 2024, lasting 4 minutes 28 seconds over central North America, entering in Mexico, crossing the United States, and leaving in eastern Canada, and the next will be on 20 April 2042, lasting 4 minutes 51 seconds over the western Pacific Ocean and passing over western Indonesia, eastern Malaysia, Brunei, and the Philippines.

Contents

The first total eclipse occurred on December 21, 1843, over southern Asia and lasted 1 minute and 43 seconds. The last total eclipse will occur on March 26, 2601, over Antarctica and the Southern Ocean, lasting 35 seconds.

This series is currently producing total eclipses over 4 minutes long, with each one gradually increasing in length. It will continue to do so until 16 July 2186, when it will produce the longest total eclipse calculated for the ten millennia from 3999 BCE to 6000 CE. [1] Starting on May 11, 2078, Saros 139 will begin producing the longest total eclipses of any series, surpassing those of Solar Saros 136, whose eclipses are getting slightly shorter. [2]

This solar saros is linked to Lunar Saros 132.

Umbral eclipses

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 139 appears in the following table.

ClassificationNumberPercent
All Umbral eclipses55100.00%
Central (two limits)55100.00%
Central (one limit)00.00%
Non-central (one limit)00.00%

All eclipses

Note: Dates are given in the Julian calendar prior to 15 October 1582, and in the Gregorian calendar after that.

SarosMemberDateTime
(Greatest)
UTC
TypeLocation
Lat, Long
Gamma Mag. Width
(km)
Duration
(min:sec)
RefQLESun altitude
1391May 17, 15013:27:44Partial63.7N 13.6W1.50020.0905 t-0
1392May 28, 151910:20:09Partial64.6N 126.3W1.41880.2342 t-0
1393June 7, 153717:14:05Partial65.5N 120.2E1.33730.3796 t-0
1394June 19, 15550:07:16Partial66.5N 6.6E1.25420.529 t-0
1395June 29, 15737:03:36Partial67.5N 108.2W1.17240.677 t-0
1396July 20, 159114:02:08Partial68.5N 136E1.09110.8249 t-0
1397July 30, 160921:07:08Partial69.5N 17.9E1.0140.9657 t-0
1398August 11, 16274:17:14Hybrid77.7N 173.3W0.94011.000110m 00s t-19
1399August 21, 164511:34:18Hybrid68.2N 43.7E0.8711.004280m 16s t-29
13910September 1, 166318:59:08Hybrid58.6N 78.9W0.80731.0065380m 29s p-36
13911September 12, 16812:33:12Hybrid49.8N 161.1E0.75041.0083430m 40s p-41
13912September 23, 169910:16:12Hybrid41.8N 40.7E0.69991.0095460m 49s p-45
13913October 4, 171718:08:27Hybrid34.6N 81.1W0.65631.0104470m 56s p-49
13914October 16, 17352:10:34Hybrid28.3N 155.2E0.62021.011481m 02s p-51
13915October 26, 175310:22:01Hybrid22.7N 29.7E0.5911.0115491m 08s p-54
13916November 6, 177118:41:02Hybrid17.9N 97.3W0.56761.012501m 13s p-55
13917November 17, 17893:08:35Hybrid14.1N 133.9E0.55041.0126521m 19s p-57
13918November 29, 180711:42:09Hybrid11.1N 3.9E0.53771.0135551m 26s p-57
13919December 9, 182520:21:45Hybrid [3] 9.2N 127.4W0.52961.0148601m 34s p-58
13920December 21, 18435:03:26Total8N 101E0.52271.0165661m 43s p-58
13921December 31, 186113:49:06Total7.8N 31.6W0.51871.0186741m 55s p-59
13922January 11, 188022:34:25Total8.3N 164.1W0.51361.0212842m 07s p-59
13923 January 22, 1898 7:19:12Total9.5N 63.6E0.50791.0244962m 21s p-59
13924 February 3, 1916 16:00:21Total11.1N 67.7W0.49871.0281082m 36s p-60
13925 February 14, 1934 0:38:41Total13.2N 161.7E0.48681.03211232m 53s p-61
13926 February 25, 1952 9:11:35Total15.6N 32.7E0.46971.03661383m 09s p-62
13927 March 7, 1970 17:38:30Total18.2N 94.7W0.44731.04141533m 28s p-63
13928 March 18, 1988 1:58:56Total20.7N 140E0.41881.04641693m 46s n-65
13929 March 29, 2006 10:12:23Total23.2N 16.7E0.38431.05151844m 07s n-67
13930 April 8, 2024 18:18:29Total25.3N 104.1W0.34311.05661984m 28s n-70
13931 April 20, 2042 2:17:30Total27N 137.3E0.29561.06142104m 51s n-73
13932 April 30, 2060 10:10:00Total28N 20.9E0.24221.0662225m 15s n-76
13933 May 11, 2078 17:56:55Total28.1N 93.7W0.18381.07012325m 40s n-79
13934 May 22, 2096 1:37:14Total27.3N 153.4E0.11961.07372416m 07s nn83
13935 June 3, 2114 9:14:09Total25.4N 41.3E0.05251.07662486m 32s nn87
13936 June 13, 2132 16:46:24Total22.3N 70.1W-0.01861.07882556m 55s nn89
13937 June 25, 2150 0:17:25Total18.3N 178.1E-0.0911.08022607m 14s nn85
13938 July 5, 2168 7:45:23Total13.2N 66.4E-0.1661.08072647m 26s -n81
13939 July 16, 2186 15:14:54Total7.4N 46.5W-0.23961.08052677m 29s -n76
13940July 27, 220422:44:32Total1N 160.1W-0.31291.07932697m 22s -n72
13941August 8, 22226:17:05Total6S 84.9E-0.38371.07742707m 06s -n67
13942August 18, 224013:52:25Total13.3S 31.3W-0.45221.07462706m 40s -p63
13943August 29, 225821:33:05Total20.9S 149.2W-0.51611.07122696m 09s -p59
13944September 9, 22765:18:47Total28.5S 91.2E-0.57551.06712665m 33s -p55
13945September 20, 229413:09:58Total36.2S 29.9W-0.631.06272634m 56s -p51
13946October 1, 231221:08:26Total43.8S 152.9W-0.67831.05782584m 20s -p47
13947October 13, 23305:13:41Total51.2S 82.5E-0.72081.05282513m 46s -p44
13948October 23, 234813:26:56Total58.2S 43.6W-0.75641.04762423m 14s -p41
13949November 3, 236621:46:04Total64.8S 170.2W-0.78681.04262312m 46s -p38
13950November 14, 23846:13:20Total70.9S 63.5E-0.81021.03772172m 22s -p36
13951November 25, 240214:45:41Total76.2S 59.6W-0.82911.03322022m 02s -p34
13952December 5, 242023:23:52Total80.2S 174W-0.84311.0291851m 44s -p32
13953December 17, 24388:05:40Total81.7S 84.3E-0.85391.02541681m 30s -p31
13954December 27, 245616:51:25Total79.8S 22W-0.86141.02221511m 19s -p30
13955January 8, 24751:37:52Total76.2S 141.8W-0.86791.01961361m 10s -p29
13956January 18, 249310:24:30Total72.2S 90.8E-0.87421.01741231m 02s -p29
13957January 30, 251119:09:33Total68.1S 39.5W-0.88161.01571140m 57s -p28
13958February 10, 25293:52:31Total64.3S 170.7W-0.89081.01431080m 53s -p27
13959February 21, 254712:29:30Total61.1S 59.6E-0.90461.01321060m 50s -p25
13960March 3, 256521:01:39Total58.7S 68.8W-0.9221.01211070m 46s -t22
13961March 15, 25835:25:52Total57.4S 166.2E-0.94561.01091150m 42s -t19
13962March 26, 260113:43:55Total58S 45.6E-0.9741.00911420m 35s -t12
13963April 6, 261921:51:02Partial61.2S 60.7W-1.01080.9781 -t0
13964April 17, 26375:51:33Partial61.6S 170.8E-1.05250.9013 -t0
13965April 28, 265513:40:56Partial62S 45.1E-1.10240.8094 -t0
13966May 8, 267321:23:23Partial62.7S 79.1W-1.15740.708 -t0
13967May 20, 26914:55:09Partial63.4S 159.1E-1.22030.5922 -t0
13968May 31, 270912:21:17Partial64.2S 38.6E-1.28690.4697 -t0
13969June 11, 272719:39:01Partial65.2S 80.2W-1.3590.3372 -t0
13970June 22, 27452:51:30Partial66.1S 162E-1.43450.1992 -t0
13971July 3, 27639:58:23Partial67.1S 45.2E-1.51320.0562 -t0

Related Research Articles

<span class="mw-page-title-main">Solar eclipse of April 20, 2042</span> Total eclipse

A total solar eclipse will occur on Sunday, April 20, 2042. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. It will be seen significantly in Western Indonesia, Eastern Malaysia, Brunei and the Philippines.

<span class="mw-page-title-main">Solar eclipse of April 30, 2060</span> Total eclipse

A total solar eclipse will occur on Friday, April 30, 2060. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of May 11, 2078</span> Total eclipse

A total solar eclipse will occur on Wednesday, May 11, 2078. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of May 22, 2096</span> Total eclipse

A total solar eclipse will occur on Tuesday, May 22, 2096. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. This will be the first eclipse of saros series 139 to exceed series 136 in length of totality. The length of totality for saros 139 is increasing, while that of Saros 136 is decreasing.

<span class="mw-page-title-main">Solar eclipse of March 18, 1988</span> Total eclipse

A total solar eclipse occurred on March 18, 1988. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Totality was visible in Indonesia and southern Philippines.

<span class="mw-page-title-main">Solar Saros 110</span> Saros cycle series 110 for solar eclipses

Saros cycle series 110 for solar eclipses occurred at the Moon's descending node, repeating every 18 years, 11 days, containing 72 eclipses, 39 of which were umbral, all annular. This series began on 30 August 463 and ended on 17 October 1743. The annular eclipse with the longest duration was 29 December 1274 lasting 11 minutes and 44 seconds.

<span class="mw-page-title-main">Solar Saros 114</span> Saros cycle series 114 for solar eclipses

Saros cycle series 114 for solar eclipses occurred at the Moon's descending node, repeating every 18 years, 11 days, containing 72 eclipses, 46 of which were umbral. The first eclipse was on 23 July 651 and the last was on 12 September 1931. The longest totality was 4 minutes 18 seconds on 21 April 1697, the longest annular was 4 minutes 33 seconds on 13 February 994.

<span class="mw-page-title-main">Solar Saros 116</span> Saros cycle series 116 for solar eclipses

Saros cycle series 116 for solar eclipses occurred at the Moon's descending node, repeating every 18 years, 11 days, containing 70 eclipses, 53 of which were umbral. The first eclipse was on 23 June 727 and the last eclipse was on 22 July 1971, making it the last saros cycle to end.

<span class="mw-page-title-main">Solar Saros 121</span> Saros cycle series 121 for solar eclipses

Saros cycle series 121 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 eclipses. 55 of these are umbral eclipses. The first eclipse in the series was on 25 April 944 and the last will be on 7 June 2206. The most recent eclipse was an annular eclipse on 7 February 2008 and the next will be an annular eclipse on 17 February 2026.

<span class="mw-page-title-main">Solar Saros 122</span> Saros cycle series 122 for solar eclipses

Saros cycle series 122 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 70 eclipses, 42 of which are umbral. The first eclipse was on 17 April 991 and the last will be on 17 May 2235. The most recent eclipse was a partial eclipse on 6 January 2019 and the next will be a partial eclipse on 16 January 2037.

<span class="mw-page-title-main">Solar Saros 123</span> Saros cycle series 123 for solar eclipses

Saros cycle series 123 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 70 eclipses, 44 of which are umbral. The first eclipse in the series was on 29 April 1074 and the last will be on 31 May 2318. The most recent eclipse was a partial eclipse on 25 November 2011 and the next will be a partial eclipse on 5 December 2029.

<span class="mw-page-title-main">Solar Saros 126</span> Saros cycle series 126 for solar eclipses

Saros cycle series 126 for solar eclipses occurs at the Moon's descending node, repeating every 18 years and 11 days, containing 72 eclipses, 41 of which are umbral. The first eclipse was on 10 March 1179 and the last will be on 3 May 2459, lasting 1,280 years. The most recent eclipse was a total eclipse on 1 August 2008 and the next will be a total eclipse on 12 August 2026.

<span class="mw-page-title-main">Solar Saros 129</span> Saros cycle series 129 for solar eclipses

Saros cycle series 129 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 80 eclipses, 41 of which are umbral. The first eclipse in the series was on 3 October 1103 and the last will be on 21 February 2528. The most recent eclipse was a hybrid eclipse on 20 April 2023 and the next will be a total eclipse on 30 April 2041.

<span class="mw-page-title-main">Solar Saros 132</span> Saros cycle series 132 for solar eclipses

Saros cycle series 132 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 eclipses, 42 of which are umbral. The first eclipse in the series was on 13 August 1208 and the last eclipse will be on 25 September 2470. The most recent eclipse was an annular eclipse on 26 December 2019 and the next will be an annular eclipse on 5 January 2038.

<span class="mw-page-title-main">Solar Saros 133</span> Saros cycle series 133 for solar eclipses

Saros cycle series 133 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 72 eclipses, 53 of which are umbral. The first eclipse in the series was on 13 July 1219 and the last will be on 5 September 2499. The most recent eclipse was a total eclipse on 13 November 2012 and the next will be a total eclipse on 25 November 2030.

<span class="mw-page-title-main">Solar Saros 135</span> Series of solar eclipses

Saros cycle series 135 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 eclipses, including 53 umbral eclipses. The longest duration of totality will be 2 minutes, 27 seconds on May 12, 2431 while the longest annular was 10 minutes 14 seconds on 24 December 1601.

<span class="mw-page-title-main">Solar Saros 136</span> Saros cycle series 136 for solar eclipses

Saros cycle series 136 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 eclipses, 56 of which are umbral. The first eclipse in the series was on 14 June 1360 and the last will be on 30 July 2622. The most recent eclipse was a total eclipse on 22 July 2009 and the next will be a total eclipse on 2 August 2027.

<span class="mw-page-title-main">Solar Saros 137</span> Series of solar eclipses

Saros cycle series 137 for solar eclipses occurs at the Moon's ascending node. It repeats every 18 years, 11 days, and contains 70 eclipses, 55 of which are umbral eclipses. The first eclipse in the series was on 25 May 1389 and the last will be on 28 June 2633. The most recent eclipse was an annular eclipse on 21 June 2020 and the next will be an annular eclipse on 2 July 2038. The longest duration of totality was 2 minutes, 55 seconds on September 10, 1569 and the longest annular eclipse will be 7 minutes 5 seconds on 28 February 2435. This series has an unusual order of umbral eclipses, with 10 total eclipses followed by 6 hybrid eclipses, 4 annular eclipses, 3 more hybrid eclipses, and then finally 32 annular eclipses.

<span class="mw-page-title-main">Solar Saros 138</span> Saros cycle series 138 for solar eclipses

Saros cycle series 138 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 70 eclipses, 54 of which are umbral. The first eclipse of the series was on 6 June 1472 and the last will be on 11 July 2716. The most recent eclipse was an annular eclipse on 10 May 2013 and the next will be an annular eclipse on 21 May 2031.

<span class="mw-page-title-main">Solar Saros 140</span> Saros cycle series 140 for solar eclipses

Saros cycle series 140 for solar eclipses occurs at the Moon's descending node, repeating every 18 years, 11 days, containing 71 eclipses, including 47 umbral eclipses. The first eclipse in this series was on 16 April 1512 and the last will be on 1 June 2774. The most recent eclipse was an annular eclipse on 26 February 2017 and the next will be an annular eclipse on 9 March 2035.

References