Solar eclipse of August 12, 2045

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Solar eclipse of August 12, 2045
SE2045Aug12T.png
Map
Type of eclipse
Nature Total
Gamma 0.2116
Magnitude 1.0774
Maximum eclipse
Duration 366 sec (6 m 6 s)
Coordinates Lua error in package.lua at line 80: module 'strict' not found.
Max. width of band 256 km (159 mi)
Times (UTC)
Greatest eclipse 17:42:39
References
Saros 136 (39 of 71)
Catalog # (SE5000) 9608

A total solar eclipse will occur on August 12, 2045. It will be the fourth longest eclipse of the 21st century with a magnitude of 1.0774 occurring just one hour before 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, Arkansas, Mississippi, Alabama, and Florida. The total eclipse will be greatest over the Bahamas, before continuing over the Virgin Islands, Hispaniola, Venezuela, 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, Fort Lauderdale, Miami, Orlando, St. Petersburg, Tampa, Nassau, and Santo Domingo.[2] It will also be the second total eclipse visible from Little Rock in about 21 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 Lua error in package.lua at line 80: module 'strict' not found., which is over the Atlantic Ocean east of Fort Lauderdale and south of Freeport, Bahamas.[2]

The Solar eclipse of August 21, 2017 will have a very similar path of totality over the USA, about 250 miles to the northeast, also crossing the USA's Pacific coast and Atlantic coast.[3]

Images

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

Related eclipses

Solar eclipses of 2044–2047

Each member 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.

Solar eclipse series sets from 2044-2047
Ascending node   Descending node
121 February 28, 2044
150px
Annular
126 August 23, 2044
150px
Total
131 February 16, 2045
150px
Annular
136 August 12, 2045
SE2045Aug12T.png
Total
141 February 5, 2046
SE2046Feb05A.png
Annular
146 August 2, 2046
150px
Total
151 January 26, 2047
150px
Partial
156 July 22, 2047
150px
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 Jun 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, 8 seconds.[4]

Series members 29–43 occur between 1865 and 2117:

29 30 31
SE1865Apr25T.gif
April 25, 1865
SE1883May06T.png
May 6, 1883
SE1901May18T.png
May 18, 1901
32 33 34
SE1919May29T.png
May 29, 1919
SE1937Jun08T.png
Jun 8, 1937
SE1955Jun20T.png
Jun 20, 1955
35 36 37
SE1973Jun30T.png
Jun 30, 1973
SE1991Jul11T.png
Jul 11, 1991
SE2009Jul22T.png
Jul 22, 2009
38 39 40
SE2027Aug02T.png
Aug 2, 2027
SE2045Aug12T.png
Aug 12, 2045
SE2063Aug24T.png
Aug. 24, 2063
41 42 43
SE2081Sep03T.png
Sep. 3, 2081
SE2099Sep14T.png
Sep. 14, 2099
SE2117Sep26T.png
Sep. 26, 2117

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).

This series has 21 eclipse events between June 1, 2011 and June 1, 2087.

May 31 – June 1 March 19–20 January 5–6 October 24–25 August 12–13
118 119 121 123 125
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
128 129 131 133 135
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
138 139 141 143 145
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
148 149 151 153 155
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
157
SE2087Jun01P.png
June 1, 2087

References

  1. http://www.fourmilab.ch/earthview/pacalc.html
  2. 2.0 2.1 2.2 Lua error in package.lua at line 80: module 'strict' not found.
  3. Google Earth Gallery for Solar and Lunar Eclipses, Xavier M. Jubier, 2011
  4. SEsaros136 at NASA.gov

External links