Solar eclipse of August 12, 2045

Last updated
Solar eclipse of August 12, 2045
SE2045Aug12T.png
Map
Type of eclipse
NatureTotal
Gamma 0.2116
Magnitude 1.0774
Maximum eclipse
Duration366 s (6 min 6 s)
Coordinates 25°54′N78°30′W / 25.9°N 78.5°W / 25.9; -78.5
Max. width of band256 km (159 mi)
Times (UTC)
Greatest eclipse17:42:39
References
Saros 136 (39 of 71)
Catalog # (SE5000) 9608

A total solar eclipse will occur on Saturday, August 12, 2045, 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.

Contents

It will be the fourth longest eclipse of the 21st century with a magnitude of 1.0774 occurring just one hour after perigee. [1] It will be visible throughout much of the continental United States, with a path of totality running through northern California, Nevada, Utah, Colorado, Kansas, Oklahoma, Texas, Arkansas, Mississippi, Alabama, and Florida. The total eclipse will be greatest over the Bahamas, before continuing over the Turks and Caicos Islands, Cuba, Dominican Republic, Haiti, Venezuela, Trinidad and Tobago, Guyana, Suriname, French Guiana, and Brazil.

The path of totality of this eclipse will be seen over many major cities, including Reno, Salt Lake City, Colorado Springs, Oklahoma City, Tulsa, Jackson, Montgomery, Tallahassee, Tampa, Orlando, Fort Lauderdale, Miami, Nassau, Santo Domingo, Porlamar, Port of Spain, Georgetown, Paramaribo, Belém, São Luís, Joāo Pessoa and Recife. [2] It will also be the second total eclipse visible from Little Rock in 21.3 years. [2] Totality will last for at least 6 minutes along the part of the path that starts at Camden, Alabama, crossing Florida and ending near the southernmost Bahama Islands. The longest duration of totality will be 6 minutes 5.5 seconds at 25°54.594′N78°32.19′W / 25.909900°N 78.53650°W / 25.909900; -78.53650 , which is over the Atlantic Ocean east of Fort Lauderdale and south of Freeport, Bahamas. [2]

The solar eclipse of August 21, 2017 had a very similar path of totality over the U.S., about 250 miles (400 km) to the northeast, also crossing the Pacific coast and Atlantic coast of the country. This is because when a solar eclipse crosses the U.S. in mid-August at an ascending node (i.e. moves from south to north during odd-numbered saros), the path of the eclipse tracks from coast to coast. When a solar eclipse crosses the U.S. in mid-August at descending node (even numbered saros), the path tracks a large distance southward. [3]

Details of the totality in some places or cities

Solar Eclipse of August 12, 2045
Country or TerritoryCity or TownStart

of
partial
eclipse
(Local Time)

Start of
total
eclipse (Local Time)
End of
total
eclipse (Local Time)
Duration of
total
eclipse
End of
partial
eclipse (Local Time)
Magnitude
Flag of the United States (23px).png  United States Eureka, California 07:13:0208:14:2108:18:284 min 07s09:25:231,069
Flag of the United States (23px).png  United States Redding, California 07:13:4508:15:4308:20:074 min 25 s09:27:431,069
Flag of the United States (23px).png  United States Reno, Nevada 07:14:4108:18:4308:21:302 min 46 s09:31:211,070
Flag of the United States (23px).png  United States Salt Lake City, Utah 08:20:5409:28:1509:30:322 min 17 s10:43:031,072
Flag of the United States (23px).png  United States Colorado Springs, Colorado 08:27:1409:36:4809:41:545 min 06 s10:55:581,073
Flag of the United States (23px).png  United States Oklahoma City, Oklahoma 09:36:3710:51:1310:54:393 min 26 s12:12:221,075
Flag of the United States (23px).png  United States Tulsa, Oklahoma 09:38:3910:52:2210:57:585 min 36 s12:14:221,075
Flag of the United States (23px).png  United States Little Rock, Arkansas 09:44:4011:00:0511:05:435 min 38 s12:22:421,076
Flag of the United States (23px).png  United States Jackson, Mississippi 09:49:3111:07:4411:11:073 min 23 s12:30:051,076
Flag of the United States (23px).png  United States Montgomery, Alabama 09:56:1111:14:2811:18:514 min 23 s12:36:401,077
Flag of the United States (23px).png  United States Tallahassee, Florida 11:01:3512:20:1212:26:075 min 55 s13:43:201,077
Flag of the United States (23px).png  United States Tampa, Florida 11:07:4512:27:5612:32:534 min 57s13:50:401,077
Flag of the United States (23px).png  United States Orlando, Florida 11:09:0912:28:3812:34:245 min 46 s13:51:171,077
Flag of the United States (23px).png  United States Miami, Florida 11:14:5412:36:4312:39:433 min 00 s13:58:031,077
Flag of the United States (23px).png  United States Jensen Beach, Florida 11:12:5912:32:4512:38:516 min 6 s13:55:271,077
Flag of the Bahamas.svg  Bahamas Freeport 11:17:0512:37:0812:42:495 min 41 s13:59:071,077
Flag of the Bahamas.svg  Bahamas Nassau 11:21:4812:41:5812:48:026 min 04 s14:03:501,077
Flag of the Turks and Caicos Islands.svg  Turks and Caicos Islands Providenciales 11:37:3012:58:4813:01:212 min 34 s14:16:381,077
Flag of Haiti.svg  Haiti Cap-Haïtien 11:41:0113:01:0213:06:445 min 32 s14:20:321,077
Flag of the Dominican Republic.svg  Dominican Republic Santo Domingo 12:47:5414:07:1514:13:015 min 47 s15:25:311,077
Flag of Venezuela.svg  Venezuela Porlamar 13:14:0014:31:3114:34:473 min 16 s15:44:201,075
Flag of Trinidad and Tobago.svg  Trinidad and Tobago Port of Spain 13:18:4814:34:1314:39:094 min 57 s15:46:071,074
Flag of Venezuela.svg  Venezuela Tucupita 13:20:5214:38:0814:39:291 min 21 s15:48:421,074
Flag of Guyana.svg  Guyana Georgetown 13:31:3714:44:3714:49:334 min 56 s15:54:351,073
Flag of Suriname.svg  Suriname Paramaribo 13:38:0814:50:1414:53:133 min 00 s15:57:031,072
Flag of France.svg  French Guiana Apatou 13:40:2814:52:0414:54:532 min 49 s15:58:461,071
Flag of Brazil.svg  Brazil Belem, Para 14:58:2516:05:5316:07:562 min 03 s117:08:201,069
Flag of Brazil.svg  Brazil Sāo Luis, Maranhāo 15:04:3416:08:4116:12:414 min 00 s17:10:101,067
Flag of Brazil.svg  Brazil Joāo Pessoa, Paraíba 15:17:2916:16:3716:20:023 min 26 s17:13:361,063
Flag of Brazil.svg  Brazil Recife, Pernambuco 15:18:2216:17:4216:20:262 min 44 s17:14:151,063

Images

Solar eclipse aug12 2045 spaceview.gif
Animated path: Small dark circle represents umbra, much larger grey circle represents penumbra.

Solar eclipses of 2044–2047

This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit. [4]

Solar eclipse series sets from 2044 to 2047
Ascending node Descending node
121 February 28, 2044
SE2044Feb28A.png
Annular
126 August 23, 2044
SE2044Aug23T.png
Total
131 February 16, 2045
SE2045Feb16A.png
Annular
136 August 12, 2045
SE2045Aug12T.png
Total
141 February 5, 2046
SE2046Feb05A.png
Annular
146 August 2, 2046
SE2046Aug02T.png
Total
151 January 26, 2047
SE2047Jan26P.png
Partial
156 July 22, 2047
SE2047Jul22P.png
Partial
Partial solar eclipses on June 23, 2047 and December 16, 2047 occur on the next lunar year eclipse set.

Saros 136

Solar Saros 136, repeating every 18 years, 11 days, contains 71 events. The series started with partial solar eclipse on June 14, 1360, and reached a first annular eclipse on September 8, 1504. It was a hybrid event from November 22, 1612, through January 17, 1703, and total eclipses from January 27, 1721, through May 13, 2496. The series ends at member 71 as a partial eclipse on July 30, 2622, with the entire series lasting 1262 years. The longest eclipse occurred on June 20, 1955, with a maximum duration of totality at 7 minutes, 7.74 seconds. All eclipses in this series occurs at the Moon's descending node. [5]

Series members 29–43 occur between 1865 and 2117
293031
SE1865Apr25T.gif
Apr 25, 1865
SE1883May06T.png
May 6, 1883
SE1901May18T.png
May 18, 1901
323334
SE1919May29T.png
May 29, 1919
SE1937Jun08T.png
Jun 8, 1937
SE1955Jun20T.png
Jun 20, 1955
353637
SE1973Jun30T.png
Jun 30, 1973
SE1991Jul11T.png
Jul 11, 1991
SE2009Jul22T.png
Jul 22, 2009
383940
SE2027Aug02T.png
Aug 2, 2027
SE2045Aug12T.png
Aug 12, 2045
SE2063Aug24T.png
Aug 24, 2063
414243
SE2081Sep03T.png
Sep 3, 2081
SE2099Sep14T.png
Sep 14, 2099
SE2117Sep26T.png
Sep 26, 2117

Tritos series

This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.

21 eclipse events between June 1, 2011 and June 1, 2087
May 31 – June 1March 19–20January 5–6October 24–25August 12–13
118120122124126
SE2011Jun01P.png
June 1, 2011
SE2015Mar20T.png
March 20, 2015
SE2019Jan06P.png
January 6, 2019
SE2022Oct25P.png
October 25, 2022
SE2026Aug12T.png
August 12, 2026
128130132134136
SE2030Jun01A.png
June 1, 2030
SE2034Mar20T.png
March 20, 2034
SE2038Jan05A.png
January 5, 2038
SE2041Oct25A.png
October 25, 2041
SE2045Aug12T.png
August 12, 2045
138140142144146
SE2049May31A.png
May 31, 2049
SE2053Mar20A.png
March 20, 2053
SE2057Jan05T.png
January 5, 2057
SE2060Oct24A.png
October 24, 2060
SE2064Aug12T.png
August 12, 2064
148150152154156
SE2068May31T.png
May 31, 2068
SE2072Mar19P.png
March 19, 2072
SE2076Jan06T.png
January 6, 2076
SE2079Oct24A.png
October 24, 2079
SE2083Aug13P.png
August 13, 2083
158160162164166
SE2087Jun01P.png
June 1, 2087
SE2098Oct24P.png
October 24, 2098

See also

Related Research Articles

<span class="mw-page-title-main">Solar eclipse of May 10, 2013</span> 21st-century annular solar eclipse

An annular solar eclipse took place at the Moon's descending node of the orbit on May 9–10 (UTC), 2013, with a magnitude of 0.9544. 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 eclipse of November 3, 2013</span> Total eclipse

A total solar eclipse occurred at the Moon's ascending node on 3 November 2013. It was a hybrid eclipse of the Sun with a magnitude of 1.0159, with a small portion over the western Atlantic Ocean at sunrise as an annular eclipse, and the rest of the path as a narrow total solar eclipse. 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 hybrid solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's in sunrise and sunset, but at Greatest Eclipse the Moon's apparent diameter is larger than the Sun's.

<span class="mw-page-title-main">Solar eclipse of March 20, 2034</span> Total eclipse

A total solar eclipse will occur on Monday, March 20, 2034. Totality will be visible in 13 countries: from east to west, Benin, Nigeria, Cameroon, Chad, Sudan, Egypt, Saudi Arabia, Kuwait, Iran, Afghanistan, Pakistan, India, and China.

<span class="mw-page-title-main">Solar eclipse of July 22, 1990</span> Total eclipse

A total solar eclipse occurred on Sunday, July 22, 1990. 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 southern Finland including its capital city Helsinki, the Soviet Union, and eastern Andreanof Islands and Amukta of Alaska.

<span class="mw-page-title-main">Solar eclipse of September 14, 2099</span> Total eclipse

A total solar eclipse will occur on Monday, September 14, 2099. 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 November 22, 1984</span> Total eclipse

A total solar eclipse occurred on November 22, 1984. 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, Papua New Guinea and southern Pacific Ocean. West of the International Date Line the eclipse took place on November 23, including all land in the path of totality. Occurring only 2.1 days after perigee, the Moon's apparent diameter was fairly larger.

<span class="mw-page-title-main">Solar eclipse of June 30, 1992</span> Total eclipse

A total solar eclipse occurred on Tuesday, June 30, 1992. 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 southeastern Uruguay and southern tip of Rio Grande do Sul, Brazil.

<span class="mw-page-title-main">Solar eclipse of January 24, 1925</span> Total eclipse

A total solar eclipse occurred on January 24, 1925. 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 southwestern and southeastern Quebec in Canada, and the United States, including Toronto, Niagara Falls and the northern part of New York City.

<span class="mw-page-title-main">Solar eclipse of March 9, 2035</span> Future annular solar eclipse

An annular solar eclipse will occur on March 9, 2035. 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 eclipse of September 2, 2035</span> Total eclipse

A total solar eclipse will occur on Sunday, September 2, 2035. 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 February 27, 2036</span> Future partial solar eclipse

A partial solar eclipse will occur on Wednesday, February 27, 2036. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

<span class="mw-page-title-main">Solar eclipse of February 5, 2046</span> Future annular solar eclipse

An annular solar eclipse will occur on Monday, February 5, 2046. 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 eclipse of February 4, 1981</span> 20th-century annular solar eclipse

An annular solar eclipse occurred at the Moon's descending node of the orbit on February 4–5, 1981. 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. This annular solar eclipse was large because the Moon covered 99.4% of the Sun, with a path width of only 25 km . It was visible in Australia, crossing over Tasmania and southern Stewart Island of New Zealand near sunrise on February 5 (Thursday), and ended at sunset over western South America on February 4 (Wednesday). Occurring only 4 days before perigee, the moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of August 2, 2046</span> Total eclipse

A total solar eclipse will occur on Thursday, August 2, 2046. 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 greater than the Sun's, blocking all direct sunlight. 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 January 5, 2057</span> Total eclipse

A total solar eclipse will occur on January 5, 2057. 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 November 1, 1948</span> Total eclipse

A total solar eclipse occurred on November 1, 1948. 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 Belgian Congo, Uganda Protectorate including the capital city Kampala, British Kenya including the capital city Nairobi, British Seychelles, and British Mauritius . During this eclipse, comet C/1948 V1, also known as the Eclipse Comet of 1948, was discovered shining near the Sun.

<span class="mw-page-title-main">Solar eclipse of August 10, 1915</span> 20th-century annular solar eclipse

An annular solar eclipse occurred on August 10, 1915. 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 the Pacific Ocean, with the only land being Haha-jima Group in Japan, where the eclipse occurred on August 11 because it is west of International Date Line.

<span class="mw-page-title-main">Solar eclipse of September 4, 2100</span> Total eclipse

A total solar eclipse is forecast to occur on Saturday, September 4, 2100. 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 26, 2057</span> Total eclipse

A total solar eclipse will occur on December 26, 2057. 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 31, 2068</span> Total eclipse

A total solar eclipse will occur on May 31, 2068. 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.

References

  1. Walker, John. "Lunar Perigee and Apogee Calculator". www.fourmilab.ch.
  2. 1 2 3 "TOTAL SOLAR ECLIPSE OF 2045 AUG 12".
  3. Google Earth Gallery for Solar and Lunar Eclipses, Xavier M. Jubier, 2011
  4. van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  5. SEsaros136 at NASA.gov