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Solar eclipse of June 20, 1974

A total solar eclipse occurred on June 20, 1974. 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.

Solar eclipse of June 20, 1974
Map
Type of eclipse
NatureTotal
Gamma−0.8239
Magnitude1.0592
Maximum eclipse
Duration309 s (5 min 9 s)
Coordinates32°06′S 103°42′E / 32.1°S 103.7°E / -32.1; 103.7
Max. width of band344 km (214 mi)
Times (UTC)
Greatest eclipse4:48:04
References
Saros146 (25 of 76)
Catalog # (SE5000)9452

The path of totality passed over the Indian Ocean, Amsterdam Island, and Western Australia. The partial eclipse was visible from Madagascar, Indonesia, Australia, and the southwestern coast of South Island, New Zealand.[1]

Related eclipses edit

Eclipses in 1974 edit

Solar eclipses of 1971–1974 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.[2]

Note: Partial solar eclipses on February 25, 1971 and August 20, 1971 occur in the next lunar year set.

Solar eclipse series sets from 1971 to 1974
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
116  
1971 July 22
Partial
1.51298 121  
1972 January 16
Annular
−0.93651
126  
1972 July 10
Total
0.68719 131  
1973 January 4
Annular
−0.26441
136  
1973 June 30
Total
−0.07853 141  
1973 December 24
Annular
0.41710
146  
1974 June 20
Total
−0.82388 151  
1974 December 13
Partial
1.07974

Saros 146 edit

It is a part of Saros cycle 146, repeating every 18 years, 11 days, containing 76 events. The series started with partial solar eclipse on September 19, 1541. It contains total eclipses from May 29, 1938 through October 7, 2154, hybrid eclipses from October 17, 2172 through November 20, 2226, and annular eclipses from December 1, 2244 through August 10, 2659. The series ends at member 76 as a partial eclipse on December 29, 2893. The longest duration of totality was 5 minutes, 21 seconds on June 30, 1992.

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).

References edit

  1. ^ Duncombe, Julena S. (June 15, 1973). "Total Solar Eclipse of 20 June 1974". United States Naval Observatory Circular. 144: 2. Bibcode:1973USNOC.144.....D.
  2. ^ 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.

External links edit

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

solar, eclipse, june, 1974, total, solar, eclipse, occurred, june, 1974, solar, eclipse, occurs, when, moon, passes, between, earth, thereby, totally, partly, obscuring, image, viewer, earth, total, solar, eclipse, occurs, when, moon, apparent, diameter, large. A total solar eclipse occurred on June 20 1974 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 Solar eclipse of June 20 1974MapType of eclipseNatureTotalGamma 0 8239Magnitude1 0592Maximum eclipseDuration309 s 5 min 9 s Coordinates32 06 S 103 42 E 32 1 S 103 7 E 32 1 103 7Max width of band344 km 214 mi Times UTC Greatest eclipse4 48 04ReferencesSaros146 25 of 76 Catalog SE5000 9452 The path of totality passed over the Indian Ocean Amsterdam Island and Western Australia The partial eclipse was visible from Madagascar Indonesia Australia and the southwestern coast of South Island New Zealand 1 Contents 1 Related eclipses 1 1 Eclipses in 1974 1 2 Solar eclipses of 1971 1974 1 3 Saros 146 1 4 Metonic series 2 References 3 External linksRelated eclipses editEclipses in 1974 edit A partial lunar eclipse on Tuesday 4 June 1974 A total solar eclipse on Thursday 20 June 1974 A total lunar eclipse on Friday 29 November 1974 A partial solar eclipse on Friday 13 December 1974 Solar eclipses of 1971 1974 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 2 Note Partial solar eclipses on February 25 1971 and August 20 1971 occur in the next lunar year set Solar eclipse series sets from 1971 to 1974 Descending node Ascending node Saros Map Gamma Saros Map Gamma 116 nbsp 1971 July 22Partial 1 51298 121 nbsp 1972 January 16Annular 0 93651 126 nbsp 1972 July 10Total 0 68719 131 nbsp 1973 January 4Annular 0 26441 136 nbsp 1973 June 30Total 0 07853 141 nbsp 1973 December 24Annular 0 41710 146 nbsp 1974 June 20Total 0 82388 151 nbsp 1974 December 13Partial 1 07974 Saros 146 edit It is a part of Saros cycle 146 repeating every 18 years 11 days containing 76 events The series started with partial solar eclipse on September 19 1541 It contains total eclipses from May 29 1938 through October 7 2154 hybrid eclipses from October 17 2172 through November 20 2226 and annular eclipses from December 1 2244 through August 10 2659 The series ends at member 76 as a partial eclipse on December 29 2893 The longest duration of totality was 5 minutes 21 seconds on June 30 1992 Series members 21 37 occur between 1901 and 2200 21 22 23 nbsp May 7 1902 nbsp May 18 1920 nbsp May 29 1938 24 25 26 nbsp June 8 1956 nbsp June 20 1974 nbsp June 30 1992 27 28 29 nbsp July 11 2010 nbsp July 22 2028 nbsp August 2 2046 30 31 32 nbsp August 12 2064 nbsp August 24 2082 nbsp September 4 2100 33 34 35 nbsp September 15 2118 nbsp September 26 2136 nbsp October 7 2154 36 37 nbsp October 17 2172 nbsp October 29 2190 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 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 20 108 114 116 nbsp April 8 1902 nbsp August 31 1913 nbsp June 19 1917 118 120 122 124 126 nbsp April 8 1921 nbsp January 24 1925 nbsp November 12 1928 nbsp August 31 1932 nbsp June 19 1936 128 130 132 134 136 nbsp April 7 1940 nbsp January 25 1944 nbsp November 12 1947 nbsp September 1 1951 nbsp June 20 1955 138 140 142 144 146 nbsp April 8 1959 nbsp January 25 1963 nbsp November 12 1966 nbsp August 31 1970 nbsp June 20 1974 148 150 152 154 nbsp April 7 1978 nbsp January 25 1982 nbsp November 12 1985 nbsp August 31 1989References edit Duncombe Julena S June 15 1973 Total Solar Eclipse of 20 June 1974 United States Naval Observatory Circular 144 2 Bibcode 1973USNOC 144 D 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 External links 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 June 20 1974 amp oldid 1218839666, wikipedia, wiki, book, books, library,

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