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Solar eclipse of September 1, 1951

An annular solar eclipse occurred on September 1, 1951. 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. Annularity was visible from the United States, Spanish Sahara (today's West Sahara), French West Africa (the parts now belonging to Mauritania, Mali, Burkina Faso and Ivory Coast), British Gold Coast (today's Ghana), southern tip of French Equatorial Africa (the part now belonging to R. Congo), Belgian Congo (today's DR Congo), Northern Rhodesia (today's Zambia), Portuguese Mozambique (today's Mozambique), Nyasaland (today's Malawi), and French Madagascar (today's Madagascar).

Solar eclipse of September 1, 1951
Map
Type of eclipse
NatureAnnular
Gamma0.1557
Magnitude0.9747
Maximum eclipse
Duration156 sec (2 m 36 s)
Coordinates16°30′N 8°30′W / 16.5°N 8.5°W / 16.5; -8.5
Max. width of band91 km (57 mi)
Times (UTC)
Greatest eclipse12:51:51
References
Saros134 (40 of 71)
Catalog # (SE5000)9401

Related eclipses edit

Solar eclipses of 1950–1953 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]

Solar eclipse series sets from 1950–1953
Ascending node   Descending node
Saros Map Saros Map
119  
1950 March 18
Annular (non-central)
124  
1950 September 12
Total
129  
1951 March 7
Annular
134  
1951 September 1
Annular
139  
1952 February 25
Total
144  
1952 August 20
Annular
149  
1953 February 14
Partial
154  
1953 August 9
Partial
Solar eclipse of July 11, 1953 belongs to the next lunar year set

Saros 134 edit

It is a part of Saros cycle 134, repeating every 18 years, 11 days, containing 71 events. The series started with a partial solar eclipse on June 22, 1248. It contains total eclipses from October 9, 1428 through December 24, 1554 and hybrid eclipses from January 3, 1573 through June 27, 1843, and annular eclipses from July 8, 1861 through May 21, 2384. The series ends at member 71 as a partial eclipse on August 6, 2510. The longest duration of totality was 1 minutes, 30 seconds on October 9, 1428. All eclipses in this series occur at the Moon’s descending node.[2]

Series members 32–48 occur between 1801 and 2100:
32 33 34
 
June 6, 1807
 
June 16, 1825
 
June 27, 1843
35 36 37
 
July 8, 1861
 
July 19, 1879
 
July 29, 1897
38 39 40
 
August 10, 1915
 
August 21, 1933
 
September 1, 1951
41 42 43
 
September 11, 1969
 
September 23, 1987
 
October 3, 2005
44 45 46
 
October 14, 2023
 
October 25, 2041
 
November 5, 2059
47 48
 
November 15, 2077
 
November 27, 2095

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).

Notes edit

  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. ^ "NASA - Catalog of Solar Eclipses of Saros 134". eclipse.gsfc.nasa.gov.

References edit

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

solar, eclipse, september, 1951, annular, solar, eclipse, occurred, september, 1951, solar, eclipse, occurs, when, moon, passes, between, earth, thereby, totally, partly, obscuring, image, viewer, earth, annular, solar, eclipse, occurs, when, moon, apparent, d. An annular solar eclipse occurred on September 1 1951 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 Annularity was visible from the United States Spanish Sahara today s West Sahara French West Africa the parts now belonging to Mauritania Mali Burkina Faso and Ivory Coast British Gold Coast today s Ghana southern tip of French Equatorial Africa the part now belonging to R Congo Belgian Congo today s DR Congo Northern Rhodesia today s Zambia Portuguese Mozambique today s Mozambique Nyasaland today s Malawi and French Madagascar today s Madagascar Solar eclipse of September 1 1951MapType of eclipseNatureAnnularGamma0 1557Magnitude0 9747Maximum eclipseDuration156 sec 2 m 36 s Coordinates16 30 N 8 30 W 16 5 N 8 5 W 16 5 8 5Max width of band91 km 57 mi Times UTC Greatest eclipse12 51 51ReferencesSaros134 40 of 71 Catalog SE5000 9401 Contents 1 Related eclipses 1 1 Solar eclipses of 1950 1953 1 2 Saros 134 1 3 Metonic series 2 Notes 3 ReferencesRelated eclipses editSolar eclipses of 1950 1953 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 Solar eclipse series sets from 1950 1953Ascending node Descending nodeSaros Map Saros Map119 nbsp 1950 March 18Annular non central 124 nbsp 1950 September 12Total129 nbsp 1951 March 7Annular 134 nbsp 1951 September 1Annular139 nbsp 1952 February 25Total 144 nbsp 1952 August 20Annular149 nbsp 1953 February 14Partial 154 nbsp 1953 August 9PartialSolar eclipse of July 11 1953 belongs to the next lunar year setSaros 134 edit It is a part of Saros cycle 134 repeating every 18 years 11 days containing 71 events The series started with a partial solar eclipse on June 22 1248 It contains total eclipses from October 9 1428 through December 24 1554 and hybrid eclipses from January 3 1573 through June 27 1843 and annular eclipses from July 8 1861 through May 21 2384 The series ends at member 71 as a partial eclipse on August 6 2510 The longest duration of totality was 1 minutes 30 seconds on October 9 1428 All eclipses in this series occur at the Moon s descending node 2 Series members 32 48 occur between 1801 and 2100 32 33 34 nbsp June 6 1807 nbsp June 16 1825 nbsp June 27 184335 36 37 nbsp July 8 1861 nbsp July 19 1879 nbsp July 29 189738 39 40 nbsp August 10 1915 nbsp August 21 1933 nbsp September 1 195141 42 43 nbsp September 11 1969 nbsp September 23 1987 nbsp October 3 200544 45 46 nbsp October 14 2023 nbsp October 25 2041 nbsp November 5 205947 48 nbsp November 15 2077 nbsp November 27 2095Metonic 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 nbsp April 8 1902 nbsp August 31 1913 nbsp June 19 1917118 120 122 124 126 nbsp April 8 1921 nbsp January 24 1925 nbsp November 12 1928 nbsp August 31 1932 nbsp June 19 1936128 130 132 134 136 nbsp April 7 1940 nbsp January 25 1944 nbsp November 12 1947 nbsp September 1 1951 nbsp June 20 1955138 140 142 144 146 nbsp April 8 1959 nbsp January 25 1963 nbsp November 12 1966 nbsp August 31 1970 nbsp June 20 1974148 150 152 154 nbsp April 7 1978 nbsp January 25 1982 nbsp November 12 1985 nbsp 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 NASA Catalog of Solar Eclipses of Saros 134 eclipse gsfc nasa gov References editEarth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak NASA GSFC Google interactive map Besselian elements nbsp 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 September 1 1951 amp oldid 1047607045, wikipedia, wiki, book, books, library,

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