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Solar eclipse of August 21, 1933

An annular solar eclipse occurred on August 21, 1933. 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 Italian Libya (today's Libya), Egypt, Mandatory Palestine (today's Israel, Palestine and Jordan) including Jerusalem and Amman, French Mandate for Syria and the Lebanon (the part now belonging to Syria), Iraq including Baghdad, Persia, Afghanistan, British Raj (the parts now belonging to Pakistan, India, Bangladesh and Myanmar), Siam (name changed to Thailand later), Dutch East Indies (today's Indonesia), North Borneo (now belonging to Malaysia), and Australia.

Solar eclipse of August 21, 1933
Map
Type of eclipse
NatureAnnular
Gamma0.0869
Magnitude0.9801
Maximum eclipse
Duration124 s (2 min 4 s)
Coordinates16°54′N 95°54′E / 16.9°N 95.9°E / 16.9; 95.9
Max. width of band71 km (44 mi)
Times (UTC)
Greatest eclipse5:49:11
References
Saros134 (39 of 71)
Catalog # (SE5000)9359

Related eclipses edit

Solar eclipses 1931–1935 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 1931 to 1935
Descending node   Ascending node
114 September 12, 1931
 
Partial
119 March 7, 1932
 
Annular
124 August 31, 1932
 
Total
129 February 24, 1933
 
Annular
134 August 21, 1933
 
Annular
139 February 14, 1934
 
Total
144 August 10, 1934
 
Annular
149 February 3, 1935
 
Partial
154 July 30, 1935
 
Partial

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

Inex series edit

This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings. In the 18th century:

  • Solar Saros 127: Total Solar Eclipse of 1731 Jan 08
  • Solar Saros 128: Annular Solar Eclipse of 1759 Dec 19
  • Solar Saros 129: Annular Solar Eclipse of 1788 Nov 27
Inex series members between 1801 and 2200:
Near lunar perigee After lunar apogee
Before lunar perigee
Before lunar apogee
After lunar perigee
 
November 9, 1817
(Saros 130)
 
October 20, 1846
(Saros 131)
 
September 29, 1875
(Saros 132)
 
September 9, 1904
(Saros 133)
 
August 21, 1933
(Saros 134)
 
July 31, 1962
(Saros 135)
 
July 11, 1991
(Saros 136)
 
June 21, 2020
(Saros 137)
 
May 31, 2049
(Saros 138)
 
May 11, 2078
(Saros 139)
 
April 23, 2107
(Saros 140)
 
April 1, 2136
(Saros 141)
 
March 12, 2165
(Saros 142)
 
February 21, 2194
(Saros 143)

In the 23rd century:

  • Solar Saros 144: Annular Solar Eclipse of 2223 Feb 01
  • Solar Saros 145: Total Solar Eclipse of 2252 Jan 12
  • Solar Saros 146: Annular Solar Eclipse of 2280 Dec 22

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, august, 1933, annular, solar, eclipse, occurred, august, 1933, solar, eclipse, occurs, when, moon, passes, between, earth, thereby, totally, partly, obscuring, image, viewer, earth, annular, solar, eclipse, occurs, when, moon, apparent, diamete. An annular solar eclipse occurred on August 21 1933 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 Italian Libya today s Libya Egypt Mandatory Palestine today s Israel Palestine and Jordan including Jerusalem and Amman French Mandate for Syria and the Lebanon the part now belonging to Syria Iraq including Baghdad Persia Afghanistan British Raj the parts now belonging to Pakistan India Bangladesh and Myanmar Siam name changed to Thailand later Dutch East Indies today s Indonesia North Borneo now belonging to Malaysia and Australia Solar eclipse of August 21 1933MapType of eclipseNatureAnnularGamma0 0869Magnitude0 9801Maximum eclipseDuration124 s 2 min 4 s Coordinates16 54 N 95 54 E 16 9 N 95 9 E 16 9 95 9Max width of band71 km 44 mi Times UTC Greatest eclipse5 49 11ReferencesSaros134 39 of 71 Catalog SE5000 9359 Contents 1 Related eclipses 1 1 Solar eclipses 1931 1935 1 2 Saros 134 1 3 Inex series 2 Notes 3 ReferencesRelated eclipses editSolar eclipses 1931 1935 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 1931 to 1935Descending node Ascending node114 September 12 1931 nbsp Partial 119 March 7 1932 nbsp Annular124 August 31 1932 nbsp Total 129 February 24 1933 nbsp Annular134 August 21 1933 nbsp Annular 139 February 14 1934 nbsp Total144 August 10 1934 nbsp Annular 149 February 3 1935 nbsp Partial154 July 30 1935 nbsp PartialSaros 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 2095Inex series edit This eclipse is a part of the long period inex cycle repeating at alternating nodes every 358 synodic months 10 571 95 days or 29 years minus 20 days Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month period of perigee However groupings of 3 inex cycles 87 years minus 2 months comes close 1 151 02 anomalistic months so eclipses are similar in these groupings In the 18th century Solar Saros 127 Total Solar Eclipse of 1731 Jan 08 Solar Saros 128 Annular Solar Eclipse of 1759 Dec 19 Solar Saros 129 Annular Solar Eclipse of 1788 Nov 27Inex series members between 1801 and 2200 Near lunar perigee After lunar apogeeBefore lunar perigee Before lunar apogeeAfter lunar perigee nbsp November 9 1817 Saros 130 nbsp October 20 1846 Saros 131 nbsp September 29 1875 Saros 132 nbsp September 9 1904 Saros 133 nbsp August 21 1933 Saros 134 nbsp July 31 1962 Saros 135 nbsp July 11 1991 Saros 136 nbsp June 21 2020 Saros 137 nbsp May 31 2049 Saros 138 nbsp May 11 2078 Saros 139 nbsp April 23 2107 Saros 140 nbsp April 1 2136 Saros 141 nbsp March 12 2165 Saros 142 nbsp February 21 2194 Saros 143 In the 23rd century Solar Saros 144 Annular Solar Eclipse of 2223 Feb 01 Solar Saros 145 Total Solar Eclipse of 2252 Jan 12 Solar Saros 146 Annular Solar Eclipse of 2280 Dec 22Notes 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 August 21 1933 amp oldid 989831510, wikipedia, wiki, book, books, library,

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