Solar eclipse of February 23, 1906

Last updated
Solar eclipse of February 23, 1906
SE1906Feb23P.png
Map
Type of eclipse
NaturePartial
Gamma −1.2479
Magnitude 0.5386
Maximum eclipse
Coordinates 71°24′S170°18′W / 71.4°S 170.3°W / -71.4; -170.3
Times (UTC)
Greatest eclipse7:43:20
References
Saros 148 (15 of 75)
Catalog # (SE5000) 9294

A partial solar eclipse occurred at the Moon's descending node of orbit on Friday, February 23, 1906, [1] [2] [3] [4] with a magnitude of 0.5386. 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 Antarctica and Southern Australia.

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. [5]

February 23, 1906 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1906 February 23 at 05:57:45.1 UTC
Equatorial Conjunction1906 February 23 at 07:03:47.6 UTC
Greatest Eclipse1906 February 23 at 07:43:20.4 UTC
Ecliptic Conjunction1906 February 23 at 07:57:15.8 UTC
Last Penumbral External Contact1906 February 23 at 09:29:19.3 UTC
February 23, 1906 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.53864
Eclipse Obscuration0.42720
Gamma−1.24788
Sun Right Ascension22h22m48.6s
Sun Declination-10°07'11.2"
Sun Semi-Diameter16'09.6"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension22h24m05.7s
Moon Declination-11°14'43.4"
Moon Semi-Diameter15'21.4"
Moon Equatorial Horizontal Parallax0°56'21.5"
ΔT5.4 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 February 1906
February 9
Ascending node (full moon)
February 23
Descending node (new moon)
Lunar eclipse chart close-1906Feb09.png SE1906Feb23P.png
Total lunar eclipse
Lunar Saros 122
Partial solar eclipse
Solar Saros 148

Eclipses in 1906

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 148

Inex

Triad

Solar eclipses of 1902–1906

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. [6]

The partial solar eclipses on May 7, 1902 and October 31, 1902 occur in the previous lunar year eclipse set, and the partial solar eclipse on July 21, 1906 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1902 to 1906
Descending node Ascending node
SarosMapGammaSarosMapGamma
108 April 8, 1902
SE1902Apr08P.png
Partial
1.5024113October 1, 1902
118 March 29, 1903
SE1903Mar29A.png
Annular
0.8413123 September 21, 1903
SE1903Sep21T.png
Total
−0.8967
128 March 17, 1904
SE1904Mar17A.png
Annular
0.1299133 September 9, 1904
SE1904Sep09T.png
Total
−0.1625
138 March 6, 1905
SE1905Mar06A.png
Annular
−0.5768143
PSM V68 D565 Sun corona of August 30 1905 taken with 40 foot camera.png
August 30, 1905
SE1905Aug30T.png
Total
0.5708
148 February 23, 1906
SE1906Feb23P.png
Partial
−1.2479153 August 20, 1906
SE1906Aug20P.png
Partial
1.3731

Saros 148

This eclipse is a part of Saros series 148, repeating every 18 years, 11 days, and containing 75 events. The series started with a partial solar eclipse on September 21, 1653. It contains annular eclipses on April 29, 2014 and May 9, 2032; a hybrid eclipse on May 20, 2050; and total eclipses from May 31, 2068 through August 3, 2771. The series ends at member 75 as a partial eclipse on December 12, 2987. 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 22 at 22 seconds (by default) on May 9, 2032, and the longest duration of totality will be produced by member 54 at 5 minutes, 23 seconds on April 26, 2609. All eclipses in this series occur at the Moon’s descending node of orbit. [7]

Series members 10–31 occur between 1801 and 2200:
101112
SE1815Dec30P.gif
December 30, 1815
SE1834Jan09P.gif
January 9, 1834
SE1852Jan21P.gif
January 21, 1852
131415
SE1870Jan31P.gif
January 31, 1870
SE1888Feb11P.gif
February 11, 1888
SE1906Feb23P.png
February 23, 1906
161718
SE1924Mar05P.png
March 5, 1924
SE1942Mar16P.png
March 16, 1942
SE1960Mar27P.png
March 27, 1960
192021
SE1978Apr07P.png
April 7, 1978
SE1996Apr17P.png
April 17, 1996
SE2014Apr29A.png
April 29, 2014
222324
SE2032May09A.png
May 9, 2032
SE2050May20H.png
May 20, 2050
SE2068May31T.png
May 31, 2068
252627
SE2086Jun11T.png
June 11, 2086
Saros148 26van75 SE2104Jun22T.jpg
June 22, 2104
Saros148 27van75 SE2122Jul04T.jpg
July 4, 2122
282930
Saros148 28van75 SE2140Jul14T.jpg
July 14, 2140
SE2158Jul25T.png
July 25, 2158
Saros148 30van75 SE2176Aug04T.jpg
August 4, 2176
31
Saros148 31van75 SE2194Aug16T.jpg
August 16, 2194

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 descending node.

22 eclipse events between February 23, 1830 and July 19, 1917
February 22–23December 11–12September 29–30July 18–19May 6–7
108110112114116
SE1830Feb23P.gif
February 23, 1830
SE1841Jul18P.gif
July 18, 1841
Saros116 63van70 SE1845May06A.jpg
May 6, 1845
118120122124126
SE1849Feb23A.gif
February 23, 1849
SE1852Dec11T.gif
December 11, 1852
SE1856Sep29A.gif
September 29, 1856
SE1860Jul18T.gif
July 18, 1860
SE1864May06H.gif
May 6, 1864
128130132134136
SE1868Feb23A.gif
February 23, 1868
SE1871Dec12T.gif
December 12, 1871
SE1875Sep29A.gif
September 29, 1875
SE1879Jul19A.png
July 19, 1879
SE1883May06T.png
May 6, 1883
138140142144146
SE1887Feb22A.png
February 22, 1887
SE1890Dec12H.gif
December 12, 1890
SE1894Sep29T.gif
September 29, 1894
SE1898Jul18A.gif
July 18, 1898
SE1902May07P.png
May 7, 1902
148150152154
SE1906Feb23P.png
February 23, 1906
SE1909Dec12P.png
December 12, 1909
SE1913Sep30P.png
September 30, 1913
SE1917Jul19P.png
July 19, 1917

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.

Series members between 1801 and 1982
SE1807Nov29H.gif
November 29, 1807
(Saros 139)
SE1818Oct29T.gif
October 29, 1818
(Saros 140)
SE1829Sep28A.gif
September 28, 1829
(Saros 141)
SE1840Aug27T.gif
August 27, 1840
(Saros 142)
SE1851Jul28T.png
July 28, 1851
(Saros 143)
SE1862Jun27P.gif
June 27, 1862
(Saros 144)
SE1873May26P.gif
May 26, 1873
(Saros 145)
SE1884Apr25P.gif
April 25, 1884
(Saros 146)
SE1895Mar26P.gif
March 26, 1895
(Saros 147)
SE1906Feb23P.png
February 23, 1906
(Saros 148)
SE1917Jan23P.png
January 23, 1917
(Saros 149)
SE1927Dec24P.png
December 24, 1927
(Saros 150)
SE1938Nov21P.png
November 21, 1938
(Saros 151)
SE1949Oct21P.png
October 21, 1949
(Saros 152)
SE1960Sep20P.png
September 20, 1960
(Saros 153)
SE1971Aug20P.png
August 20, 1971
(Saros 154)
SE1982Jul20P.png
July 20, 1982
(Saros 155)

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
SE1819Apr24P.png
April 24, 1819
(Saros 145)
SE1848Apr03P.png
April 3, 1848
(Saros 146)
SE1877Mar15P.gif
March 15, 1877
(Saros 147)
SE1906Feb23P.png
February 23, 1906
(Saros 148)
SE1935Feb03P.png
February 3, 1935
(Saros 149)
SE1964Jan14P.png
January 14, 1964
(Saros 150)
SE1992Dec24P.png
December 24, 1992
(Saros 151)
SE2021Dec04T.png
December 4, 2021
(Saros 152)
SE2050Nov14P.png
November 14, 2050
(Saros 153)
SE2079Oct24A.png
October 24, 2079
(Saros 154)
Saros155 11van71 SE2108Oct05T.jpg
October 5, 2108
(Saros 155)
Saros156 08van69 SE2137Sep15P.jpg
September 15, 2137
(Saros 156)
Saros157 07van70 SE2166Aug25A.jpg
August 25, 2166
(Saros 157)
Saros158 08van70 SE2195Aug05T.jpg
August 5, 2195
(Saros 158)

Notes

  1. "February 23, 1906 Partial Solar Eclipse". timeanddate. Retrieved 31 July 2024.
  2. "Page 37". The Albury Banner, Wodonga Express and Riverina Stock Journal. Albury, New South Wales, Australia. 1906-02-23. p. 37. Retrieved 2023-11-01 via Newspapers.com.
  3. "Partial eclipse of the sun". The Daily Telegraph. Sydney, New South Wales, Australia. 1906-02-24. p. 12. Retrieved 2023-11-01 via Newspapers.com.
  4. "Partial sun eclipse". The Age. Melbourne, Victoria, Victoria, Australia. 1906-02-24. p. 11. Retrieved 2023-11-01 via Newspapers.com.
  5. "Partial Solar Eclipse of 1906 Feb 23". EclipseWise.com. Retrieved 31 July 2024.
  6. 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.
  7. "NASA - Catalog of Solar Eclipses of Saros 148". eclipse.gsfc.nasa.gov.

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References