Solar eclipse of March 20, 2034

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Solar eclipse of March 20, 2034
SE2034Mar20T.png
Map
Type of eclipse
NatureTotal
Gamma0.2894
Magnitude1.0458
Maximum eclipse
Duration249 sec (4 m 9 s)
Coordinates16°06′N 22°12′E / 16.1°N 22.2°E / 16.1; 22.2
Max. width of band159 km (99 mi)
Times (UTC)
Greatest eclipse10:18:45
References
Saros130 (53 of 73)
Catalog # (SE5000)9583

A total solar eclipse will occur on March 20, 2034. 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.

Images[]

SE2034Mar20T.gif
Animated path

Related eclipses[]

Solar eclipses of 2033–2036[]

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.[1]

Solar eclipse series sets from 2033–2036
Descending node   Ascending node
120 March 30, 2033
SE2033Mar30T.png
Total
125 September 23, 2033
SE2033Sep23P.png
Partial
130 March 20, 2034
SE2034Mar20T.png
Total
135 September 12, 2034
SE2034Sep12A.png
Annular
140 March 9, 2035
SE2035Mar09A.png
Annular
145 September 2, 2035
SE2035Sep02T.png
Total
150 February 27, 2036
SE2036Feb27P.png
Partial
155 August 21, 2036
SE2036Aug21P.png
Partial
A partial solar eclipse on July 23, 2036 occurs in the next lunar year eclipse set.

Saros 130[]

This eclipse is a part of Saros cycle 130, repeating every 18 years, 11 days, containing 73 events. The series started with partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. There are no annular eclipses in the series. The series ends at member 73 as a partial eclipse on October 25, 2394. The longest duration of totality was 6 minutes, 41 seconds on July 11, 1619. All eclipses in this series occurs at the Moon’s descending node.[2]

Series members 43–56 between 1853 and 2300
43 44 45
SE1853Nov30T.png
November 30, 1853
SE1871Dec12T.png
December 12, 1871
SE1889Dec22T.png
December 22, 1889
46 47 48
SE1908Jan03T.png
January 3, 1908
SE1926Jan14T.png
January 14, 1926
SE1944Jan25T.png
January 25, 1944
49 50 51
SE1962Feb05T.png
February 5, 1962
SE1980Feb16T.png
February 16, 1980
SE1998Feb26T.png
February 26, 1998
52 53 54
SE2016Mar09T.png
March 9, 2016
SE2034Mar20T.png
March 20, 2034
SE2052Mar30T.png
March 30, 2052
55 56 57
SE2070Apr11T.png
April 11, 2070
SE2088Apr21T.png
April 21, 2088
SE2106May03T.png
May 3, 2106
58 59 60
SE2124May14T.png
May 14, 2124
SE2142May25T.png
May 25, 2142
SE2160Jun04T.png
June 4, 2160
61 62 63
SE2178Jun16T.png
June 16, 2178
SE2196Jun26T.png
June 26, 2196
SE2214Jul08T.png
July 8, 2214
64 65 66
SE2232Jul18T.png
July 18, 2232
SE2250Jul30P.png
July 30, 2250
SE2268Aug09P.png
August 9, 2268
67
SE2286Aug20P.png
August 20, 2286

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 1 March 19–20 January 5–6 October 24–25 August 12–13
118 120 122 124 126
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
128 130 132 134 136
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
138 140 142 144 146
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
148 150 152 154 156
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
158 160 162 164 166
SE2087Jun01P.png
June 1, 2087
SE2098Oct24P.png
October 24, 2098

References[]

  1. ^ 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.
  2. ^ "Saros Series catalog of solar eclipses". NASA.

External links[]

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