Solar eclipse of April 6, 1913

Last updated
Solar eclipse of April 6, 1913
SE1913Apr06P.png
Map
Type of eclipse
NaturePartial
Gamma 1.3147
Magnitude 0.4244
Maximum eclipse
Coordinates 61°12′N175°42′E / 61.2°N 175.7°E / 61.2; 175.7
Times (UTC)
Greatest eclipse17:33:07
References
Saros 147 (17 of 80)
Catalog # (SE5000) 9310

A partial solar eclipse occurred at the Moon's ascending node of orbit on Sunday, April 6, 1913, [1] [2] [3] with a magnitude of 0.4244. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

Contents

A partial eclipse was visible for parts of eastern Russia, northwestern North America.

Eclipse details

Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse. [4]

April 6, 1913 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1913 April 06 at 15:54:06.5 UTC
Greatest Eclipse1913 April 06 at 17:33:07.1 UTC
Ecliptic Conjunction1913 April 06 at 17:48:01.1 UTC
Equatorial Conjunction1913 April 06 at 18:55:10.9 UTC
Last Penumbral External Contact1913 April 06 at 19:11:31.1 UTC
April 6, 1913 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.42437
Eclipse Obscuration0.30366
Gamma1.31475
Sun Right Ascension01h00m06.2s
Sun Declination+06°25'02.8"
Sun Semi-Diameter15'58.5"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension00h57m49.4s
Moon Declination+07°28'25.6"
Moon Semi-Diameter14'56.5"
Moon Equatorial Horizontal Parallax0°54'50.2"
ΔT15.0 s

Eclipse season

This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.

Eclipse season of March–April 1913
March 22
Descending node (full moon)
April 6
Ascending node (new moon)
Lunar eclipse chart close-1913Mar22.png SE1913Apr06P.png
Total lunar eclipse
Lunar Saros 121
Partial solar eclipse
Solar Saros 147

Eclipses in 1913

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 147

Inex

Triad

Solar eclipses of 1910–1913

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. [5]

The partial solar eclipse on August 31, 1913 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1910 to 1913
Ascending node Descending node
SarosMapGammaSarosMapGamma
117 May 9, 1910
SE1910May09T.png
Total
−0.9437122 November 2, 1910
SE1910Nov02P.png
Partial
1.0603
127 April 28, 1911
SE1911Apr28T.png
Total
−0.2294132 October 22, 1911
SE1911Oct22A.png
Annular
0.3224
137 April 17, 1912
SE1912Apr17H.png
Hybrid
0.528142 October 10, 1912
SE1912Oct10T.png
Total
−0.4149
147 April 6, 1913
SE1913Apr06P.png
Partial
1.3147152 September 30, 1913
SE1913Sep30P.png
Partial
−1.1005

Saros 147

This eclipse is a part of Saros series 147, repeating every 18 years, 11 days, and containing 80 events. The series started with a partial solar eclipse on October 12, 1624. It contains annular eclipses from May 31, 2003 through July 31, 2706. There are no hybrid or total eclipses in this set. The series ends at member 80 as a partial eclipse on February 24, 3049. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

The longest duration of annularity will be produced by member 38 at 9 minutes, 41 seconds on November 21, 2291. All eclipses in this series occur at the Moon’s ascending node of orbit. [6]

Series members 11–32 occur between 1801 and 2200:
111213
SE1805Jan30P.gif
January 30, 1805
SE1823Feb11P.gif
February 11, 1823
SE1841Feb21P.gif
February 21, 1841
141516
SE1859Mar04P.gif
March 4, 1859
SE1877Mar15P.gif
March 15, 1877
SE1895Mar26P.gif
March 26, 1895
171819
SE1913Apr06P.png
April 6, 1913
SE1931Apr18P.png
April 18, 1931
SE1949Apr28P.png
April 28, 1949
202122
SE1967May09P.png
May 9, 1967
SE1985May19P.png
May 19, 1985
SE2003May31A.png
May 31, 2003
232425
SE2021Jun10A.png
June 10, 2021
SE2039Jun21A.png
June 21, 2039
SE2057Jul01A.png
July 1, 2057
262728
SE2075Jul13A.png
July 13, 2075
SE2093Jul23A.png
July 23, 2093
SE2111Aug04A.png
August 4, 2111
293031
SE2129Aug15A.png
August 15, 2129
Saros147 30van80 SE2147Aug26A.jpg
August 26, 2147
Saros147 31van80 SE2165Sep05A.jpg
September 5, 2165
32
Saros147 32van80 SE2183Sep16A.jpg
September 16, 2183

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). All eclipses in this table occur at the Moon's ascending node.

25 eclipse events between April 5, 1837 and June 17, 1928
April 5–6January 22–23November 10–11August 28–30June 17–18
107109111113115
SE1837Apr05P.png
April 5, 1837
SE1841Jan22P.gif
January 22, 1841
SE1844Nov10P.gif
November 10, 1844
SE1848Aug28P.gif
August 28, 1848
SE1852Jun17P.gif
June 17, 1852
117119121123125
SE1856Apr05T.gif
April 5, 1856
SE1860Jan23A.gif
January 23, 1860
SE1863Nov11A.gif
November 11, 1863
SE1867Aug29T.gif
August 29, 1867
SE1871Jun18A.gif
June 18, 1871
127129131133135
SE1875Apr06T.gif
April 6, 1875
SE1879Jan22A.gif
January 22, 1879
SE1882Nov10A.gif
November 10, 1882
SE1886Aug29T.png
August 29, 1886
SE1890Jun17A.gif
June 17, 1890
137139141143145
SE1894Apr06H.gif
April 6, 1894
SE1898Jan22T.png
January 22, 1898
SE1901Nov11A.png
November 11, 1901
SE1905Aug30T.png
August 30, 1905
SE1909Jun17H.png
June 17, 1909
147149151153155
SE1913Apr06P.png
April 6, 1913
SE1917Jan23P.png
January 23, 1917
SE1920Nov10P.png
November 10, 1920
SE1924Aug30P.png
August 30, 1924
SE1928Jun17P.png
June 17, 1928

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.

The partial solar eclipse on October 24, 2098 (part of Saros 164) is also a part of this series but is not included in the table below.

Series members between 1801 and 2011
SE1804Feb11H.png
February 11, 1804
(Saros 137)
SE1815Jan10A.png
January 10, 1815
(Saros 138)
SE1825Dec09H.png
December 9, 1825
(Saros 139)
SE1836Nov09T.png
November 9, 1836
(Saros 140)
SE1847Oct09A.png
October 9, 1847
(Saros 141)
SE1858Sep07T.png
September 7, 1858
(Saros 142)
SE1869Aug07T.png
August 7, 1869
(Saros 143)
SE1880Jul07A.png
July 7, 1880
(Saros 144)
SE1891Jun06A.png
June 6, 1891
(Saros 145)
SE1902May07P.png
May 7, 1902
(Saros 146)
SE1913Apr06P.png
April 6, 1913
(Saros 147)
SE1924Mar05P.png
March 5, 1924
(Saros 148)
SE1935Feb03P.png
February 3, 1935
(Saros 149)
SE1946Jan03P.png
January 3, 1946
(Saros 150)
SE1956Dec02P.png
December 2, 1956
(Saros 151)
SE1967Nov02T.png
November 2, 1967
(Saros 152)
SE1978Oct02P.png
October 2, 1978
(Saros 153)
SE1989Aug31P.png
August 31, 1989
(Saros 154)
SE2000Jul31P.png
July 31, 2000
(Saros 155)
SE2011Jul01P.png
July 1, 2011
(Saros 156)

Inex series

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.

Series members between 1801 and 2200
SE1826Jun05P.gif
June 5, 1826
(Saros 144)
SE1855May16P.gif
May 16, 1855
(Saros 145)
SE1884Apr25P.gif
April 25, 1884
(Saros 146)
SE1913Apr06P.png
April 6, 1913
(Saros 147)
SE1942Mar16P.png
March 16, 1942
(Saros 148)
SE1971Feb25P.png
February 25, 1971
(Saros 149)
SE2000Feb05P.png
February 5, 2000
(Saros 150)
SE2029Jan14P.png
January 14, 2029
(Saros 151)
SE2057Dec26T.png
December 26, 2057
(Saros 152)
SE2086Dec06P.png
December 6, 2086
(Saros 153)
Saros154 12van71 SE2115Nov16A.jpg
November 16, 2115
(Saros 154)
Saros155 13van71 SE2144Oct26T.jpg
October 26, 2144
(Saros 155)
Saros156 10van69 SE2173Oct07A.jpg
October 7, 2173
(Saros 156)

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References

  1. "April 6, 1913 Partial Solar Eclipse". timeanddate. Retrieved 31 July 2024.
  2. "APRIL HEAVENS ARE DESCRIBED". The Times-Democrat. New Orleans, Louisiana. 1913-04-06. p. 59. Retrieved 2023-11-03 via Newspapers.com.
  3. "THE HEAVENS IN APRIL". The Commercial Appeal. Memphis, Tennessee. 1913-04-06. p. 74. Retrieved 2023-11-03 via Newspapers.com.
  4. "Partial Solar Eclipse of 1913 Apr 06". EclipseWise.com. Retrieved 31 July 2024.
  5. 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.
  6. "NASA - Catalog of Solar Eclipses of Saros 147". eclipse.gsfc.nasa.gov.