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Solar eclipse of January 25, 1944

A total solar eclipse occurred on January 25, 1944. 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 Peru, Brazil, British Sierra Leone (today's Sierra Leone), and French West Africa (the parts now belonging to Guinea, Mali, Burkina Faso and Niger, including Guinean capital Conakry). At greatest eclipse, the Sun was 78 degrees above horizon (just 12 degrees from zenith).

Solar eclipse of January 25, 1944
Map
Type of eclipse
NatureTotal
Gamma0.2025
Magnitude1.0428
Maximum eclipse
Duration249 sec (4 m 9 s)
Coordinates7°36′S 50°12′W / 7.6°S 50.2°W / -7.6; -50.2
Max. width of band146 km (91 mi)
Times (UTC)
Greatest eclipse15:26:42
References
Saros130 (48 of 73)
Catalog # (SE5000)9384

Related eclipses

Solar eclipses 1942–1946

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]

Note: The partial solar eclipse on September 10, 1942 occurs in the previous lunar year eclipse set.

Solar eclipse series sets from 1942–1946
Ascending node   Descending node
115 August 12, 1942
 
Partial
120 February 4, 1943
 
Total
125 August 1, 1943
 
Annular
130 January 25, 1944
 
Total
135 July 20, 1944
 
Annular
140 January 14, 1945
 
Annular
145 July 9, 1945
 
Total
150 January 3, 1946
 
Partial
155 June 29, 1946
 
Partial

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
 
November 30, 1853
 
December 12, 1871
 
December 22, 1889
46 47 48
 
January 3, 1908
 
January 14, 1926
 
January 25, 1944
49 50 51
 
February 5, 1962
 
February 16, 1980
 
February 26, 1998
52 53 54
 
March 9, 2016
 
March 20, 2034
 
March 30, 2052
55 56 57
 
April 11, 2070
 
April 21, 2088
 
May 3, 2106
58 59 60
 
May 14, 2124
 
May 25, 2142
 
June 4, 2160
61 62 63
 
June 16, 2178
 
June 26, 2196
 
July 8, 2214
64 65 66
 
July 18, 2232
 
July 30, 2250
 
August 9, 2268
67
 
August 20, 2286

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).

Notes

  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.

References

  • Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
    • Google interactive map
    • Besselian elements

solar, eclipse, january, 1944, total, solar, eclipse, occurred, january, 1944, solar, eclipse, occurs, when, moon, passes, between, earth, thereby, totally, partly, obscuring, image, viewer, earth, total, solar, eclipse, occurs, when, moon, apparent, diameter,. A total solar eclipse occurred on January 25 1944 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 Peru Brazil British Sierra Leone today s Sierra Leone and French West Africa the parts now belonging to Guinea Mali Burkina Faso and Niger including Guinean capital Conakry At greatest eclipse the Sun was 78 degrees above horizon just 12 degrees from zenith Solar eclipse of January 25 1944MapType of eclipseNatureTotalGamma0 2025Magnitude1 0428Maximum eclipseDuration249 sec 4 m 9 s Coordinates7 36 S 50 12 W 7 6 S 50 2 W 7 6 50 2Max width of band146 km 91 mi Times UTC Greatest eclipse15 26 42ReferencesSaros130 48 of 73 Catalog SE5000 9384 Contents 1 Related eclipses 1 1 Solar eclipses 1942 1946 1 2 Saros 130 1 3 Metonic series 2 Notes 3 ReferencesRelated eclipses EditSolar eclipses 1942 1946 Edit 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 Note The partial solar eclipse on September 10 1942 occurs in the previous lunar year eclipse set Solar eclipse series sets from 1942 1946Ascending node Descending node115 August 12 1942 Partial 120 February 4 1943 Total125 August 1 1943 Annular 130 January 25 1944 Total135 July 20 1944 Annular 140 January 14 1945 Annular145 July 9 1945 Total 150 January 3 1946 Partial155 June 29 1946 PartialSaros 130 Edit 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 230043 44 45 November 30 1853 December 12 1871 December 22 188946 47 48 January 3 1908 January 14 1926 January 25 194449 50 51 February 5 1962 February 16 1980 February 26 199852 53 54 March 9 2016 March 20 2034 March 30 205255 56 57 April 11 2070 April 21 2088 May 3 210658 59 60 May 14 2124 May 25 2142 June 4 216061 62 63 June 16 2178 June 26 2196 July 8 221464 65 66 July 18 2232 July 30 2250 August 9 226867 August 20 2286Metonic 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 22 eclipse events progressing from north to south between April 8 1902 and August 31 1989 April 7 8 January 24 25 November 12 August 31 September 1 June 19 20108 114 116 April 8 1902 August 31 1913 June 19 1917118 120 122 124 126 April 8 1921 January 24 1925 November 12 1928 August 31 1932 June 19 1936128 130 132 134 136 April 7 1940 January 25 1944 November 12 1947 September 1 1951 June 20 1955138 140 142 144 146 April 8 1959 January 25 1963 November 12 1966 August 31 1970 June 20 1974148 150 152 154 April 7 1978 January 25 1982 November 12 1985 August 31 1989Notes Edit 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 Saros Series catalog of solar eclipses NASA References EditEarth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak NASA GSFC Google interactive map Besselian elements This solar eclipse related article is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title Solar eclipse of January 25 1944 amp oldid 1047605087, wikipedia, wiki, book, books, library,

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