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 events. It has 16 partial solar eclipses, 12 will be hybrid and 43 will be total. 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.

Contents

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 July 16, 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] The latest eclipse in this series to occur was a total eclipse on April 8, 2024, lasting 4 minutes 28 seconds over central North America, entering in Mexico, crossing the United States, and leaving in eastern Canada. The next eclipse will occur on April 20, 2042, lasting 4 minutes 51 seconds over the western Pacific Ocean and passing over western Indonesia, eastern Malaysia, Brunei, and the Philippines. All eclipses in this series occurs at the Moon's ascending node.

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%

Events

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, 182520:21:45Hybrid9.2N 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 March 29, 2006</span> Total eclipse

A total solar eclipse occurred on March 29, 2006. 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 was visible from a narrow corridor which traversed half the Earth. The magnitude, that is, the ratio between the apparent sizes of the Moon and that of the Sun, was 1.052, and it was part of Saros 139.

<span class="mw-page-title-main">July 2000 lunar eclipse</span> Central lunar eclipse

A total lunar eclipse took place on Sunday 16 July 2000, the second of two total lunar eclipses in 2000.

<span class="mw-page-title-main">Solar eclipse of April 20, 2042</span> Future total solar 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> Future total solar 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> Future total solar 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> Future total solar 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 eclipse of March 7, 1970</span> Total eclipse

A total solar eclipse occurred on Saturday, March 7, 1970, visible across most of North America and Central America.

<span class="mw-page-title-main">Solar eclipse of February 25, 1952</span> Total eclipse

A total solar eclipse occurred on February 25, 1952. 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. The path of totality crossed Africa, the Middle East, and Asia.

<span class="mw-page-title-main">Solar eclipse of February 14, 1934</span> Total eclipse

A total solar eclipse occurred on February 14, 1934. 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 from the Dutch East Indies, North Borneo, and the South Seas Mandate of Japan.

<span class="mw-page-title-main">Solar eclipse of February 3, 1916</span> Total eclipse

A total solar eclipse occurred on February 3, 1916. 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 Colombia, Venezuela, and the whole Guadeloupe except Marie-Galante, Saint Martin and Saint Barthélemy.

<span class="mw-page-title-main">Solar eclipse of March 29, 1987</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node of the orbit on March 29, 1987. It was a hybrid eclipse, with only a small portion of the central path as total, lasting a maximum of only 7.57 seconds. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Totality of this eclipse was not visible on any land, while annularity was visible in southern Argentina, Gabon, Equatorial Guinea, Cameroon, Central African Republic, Sudan, Ethiopia, Djibouti and Somaliland.

<span class="mw-page-title-main">Solar eclipse of July 16, 2186</span> Astronomical event

A total solar eclipse will occur on July 16, 2186. 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 December 24, 1973</span> 20th-century annular solar eclipse

An annular solar eclipse occurred on December 24, 1973. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Annularity was visible from southern Mexico, southwestern Nicaragua, Costa Rica including the capital city San José, Panama, Colombia including the capital city Bogotá, southern Venezuela, Brazil, southern Guyana, southern Dutch Guiana, southern French Guiana, Portuguese Cape Verde including the capital city Praia, Mauritania including the capital city Nouakchott, Spanish Sahara, Mali, and Algeria.

<span class="mw-page-title-main">Solar eclipse of December 14, 1955</span> 20th-century annular solar eclipse

An annular solar eclipse occurred on December 14, 1955. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide.

<span class="mw-page-title-main">Solar Saros 119</span> Saros cycle series 119 for solar eclipses

Saros cycle series 119 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 71 events. All eclipses in this series occurs at the Moon's ascending node.

<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 events. All eclipses in this series occur at the Moon's ascending node.

<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 events. All eclipses in this series occurs at the Moon's descending node.

<span class="mw-page-title-main">Solar Saros 145</span> Series of solar eclipses

Saros cycle series 145 for solar eclipses occurs at the Moon's ascending node, repeating every 18 years, 11 days, containing 77 events. It is currently a young cycle producing total eclipses less than 3 minutes in length. The series started with a partial solar eclipse on January 4, 1639, and reached a first annular eclipse on June 6, 1891. It was a hybrid event on June 17, 1909, and total eclipses from June 29, 1927, through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. The longest duration eclipse in the cycle will be member 50 at 7 minutes and 12 seconds in length on June 25, 2522, after which the durations of eclipses will decrease until the end of the cycle. In its central phase it will produce mainly total eclipses. All eclipses in this series occur at the Moon's ascending node.

<span class="mw-page-title-main">Solar eclipse of December 2, 1937</span> 20th-century annular solar eclipse

An annular solar eclipse occurred on December 2, 1937. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Annularity was visible from Ogasawara, Tokyo and South Seas Mandate in Japan, and Gilbert and Ellice Islands.

References