Solar eclipse of February 5, 2046

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Solar eclipse of February 5, 2046
SE2046Feb05A.png
Map
Type of eclipse
Nature Annular
Gamma 0.3765
Magnitude 0.9232
Maximum eclipse
Duration 9m 42s
Coordinates 4.8N 171.4W
Max. width of band 310 km
Times (UTC)
Greatest eclipse 23:06:26
References
Saros 141 (25 of 70)
Catalog # (SE5000) 9609

An annular solar eclipse will occur on 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.

Images[edit]

SE2046Feb05A.gif
Animated path

Related eclipses[edit]

Solar eclipses of 2044-2047[edit]

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
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 141[edit]

Solar Saros 141 repeats every 18 years, 11 days and contains 70 events. The series started with partial solar eclipse on May 19, 1613. It contains annular eclipses from August 4, 1739 through October 14, 2460. There are no total eclipses in this series. The series ends at member 70 as a partial eclipse on June 13, 2857. [1]

Series members 17-28 occur between 1901 and 2100:

17 18 19
SE1901Nov11A.png
November 11, 1901
SE1919Nov22A.png
November 22, 1919
SE1937Dec02A.png
December 2, 1937
20 21 22
SE1955Dec14A.png
December 14, 1955
SE1973Dec24A.png
December 24, 1973
SE1992Jan04A.png
January 4, 1992
23 24 25
SE2010Jan15A.png
January 15, 2010
SE2028Jan26A.png
January 26, 2028
SE2046Feb05A.png
February 5, 2046
26 27 28
SE2064Feb17A.png
February 17, 2064
SE2082Feb27A.png
February 27, 2082
SE2100Mar10A.png
March 10, 2100

Metonic series[edit]

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, progressing from north to south between July 1, 2000 and July 1, 2076.

July 1-2 April 19-20 February 5-7 November 24-25 September 12-13
117 119 121 123 125
SE2000Jul01P.png
July 1, 2000
SE2004Apr19P.png
April 19, 2004
SE2008Feb07A.png
February 7, 2008
SE2011Nov25P.png
November 25, 2011
SE2015Sep13P.png
September 13, 2015
127 129 131 133 135
SE2019Jul02T.png
July 2, 2019
SE2023Apr20H.png
April 20, 2023
SE2027Feb06A.png
February 6, 2027
SE2030Nov25T.png
November 25, 2030
SE2034Sep12A.png
September 12, 2034
137 139 141 143 145
SE2038Jul02A.png
July 2, 2038
SE2042Apr20T.png
April 20, 2042
SE2046Feb05A.png
February 5, 2046
SE2049Nov25H.png
November 25, 2049
SE2053Sep12T.png
September 12, 2053
147 149 151 153 155
SE2057Jul01A.png
July 1, 2057
SE2061Apr20T.png
April 20, 2061
SE2065Feb05P.png
February 5, 2065
SE2068Nov24P.png
November 24, 2068
SE2072Sep12T.png
September 12, 2072
157
SE2076Jul01P.png
July 1, 2076

Tritos series[edit]

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 synchonization 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.

Series members between 1901 and 2100 are:

SE1904Mar17A.png
March 17, 1904
(Saros 128)
SE1915Feb14A.png
February 14, 1915
(Saros 129)
SE1926Jan14T.png
January 14, 1926
(Saros 130)
SE1936Dec13A.png
December 13, 1936
(Saros 131)
SE1947Nov12A.png
November 12, 1947
(Saros 132)
SE1958Oct12T.png
October 12, 1958
(Saros 133)
SE1969Sep11A.png
September 11, 1969
(Saros 134)
SE1980Aug10A.png
August 10, 1980
(Saros 135)
SE1991Jul11T.png
July 11, 1991
(Saros 136)
SE2002Jun10A.png
June 10, 2002
(Saros 137)
SE2013May10A.png
May 10, 2013
(Saros 138)
SE2024Apr08T.png
April 8, 2024
(Saros 139)
SE2035Mar09A.png
March 9, 2035
(Saros 140)
SE2046Feb05A.png
February 5, 2046
(Saros 141)
SE2057Jan05T.png
January 5, 2057
(Saros 142)
SE2067Dec06H.png
December 6, 2067
(Saros 143)
SE2078Nov04A.png
November 4, 2078
(Saros 144)
SE2089Oct04T.png
October 4, 2089
(Saros 145)
SE2100Sep04T.png
September 4, 2100
(Saros 146)

References[edit]

  1. ^ "NASA - Catalog of Solar Eclipses of Saros 141". Eclipse.gsfc.nasa.gov. Retrieved 2012-03-15. 

External links[edit]