Solar eclipse of February 5, 2046

Solar eclipse of February 5, 2046
Map
Type of eclipse
Nature Annular
Gamma 0.3765
Magnitude 0.9232
Maximum eclipse
Duration 582 sec (9 m 42 s)
Coordinates 4°48′N 171°24′W / 4.8°N 171.4°W
Max. width of band 310 km (190 mi)
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


Animated path

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
121February 28, 2044

Annular
126August 23, 2044

Total
131February 16, 2045

Annular
136August 12, 2045

Total
141February 5, 2046

Annular
146August 2, 2046

Total
151January 26, 2047

Partial
156July 22, 2047

Partial
Partial solar eclipses on June 23, 2047 and December 16, 2047 occur on the next lunar year eclipse set.

Saros 141

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

November 11, 1901

November 22, 1919

December 2, 1937
20 21 22

December 14, 1955

December 24, 1973

January 4, 1992
23 24 25

January 15, 2010

January 26, 2028

February 5, 2046
26 27 28

February 17, 2064

February 27, 2082

March 10, 2100

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, 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

July 1, 2000

April 19, 2004

February 7, 2008

November 25, 2011

September 13, 2015
127 129 131 133 135

July 2, 2019

April 20, 2023

February 6, 2027

November 25, 2030

September 12, 2034
137 139 141 143 145

July 2, 2038

April 20, 2042

February 5, 2046

November 25, 2049

September 12, 2053
147 149 151 153 155

July 1, 2057

April 20, 2061

February 5, 2065

November 24, 2068

September 12, 2072
157

July 1, 2076

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.

Series members between 1901 and 2100 are:


March 17, 1904
(Saros 128)

February 14, 1915
(Saros 129)

January 14, 1926
(Saros 130)

December 13, 1936
(Saros 131)

November 12, 1947
(Saros 132)

October 12, 1958
(Saros 133)

September 11, 1969
(Saros 134)

August 10, 1980
(Saros 135)

July 11, 1991
(Saros 136)

June 10, 2002
(Saros 137)

May 10, 2013
(Saros 138)

April 8, 2024
(Saros 139)

March 9, 2035
(Saros 140)

February 5, 2046
(Saros 141)

January 5, 2057
(Saros 142)

December 6, 2067
(Saros 143)

November 4, 2078
(Saros 144)

October 4, 2089
(Saros 145)

September 4, 2100
(Saros 146)

References

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