Solar eclipse of March 27, 1960

Last updated
Solar eclipse of March 27, 1960
SE1960Mar27P.png
Map
Type of eclipse
NaturePartial
Gamma −1.1537
Magnitude 0.7058
Maximum eclipse
Coordinates 72°06′S151°54′E / 72.1°S 151.9°E / -72.1; 151.9
Times (UTC)
Greatest eclipse7:25:07
References
Saros 148 (18 of 75)
Catalog # (SE5000) 9420

A partial solar eclipse occurred at the Moon's descending node of orbit on Sunday, March 27, 1960, [1] with a magnitude of 0.7058. 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 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. [2]

March 27, 1960 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1960 March 27 at 05:28:45.5 UTC
Equatorial Conjunction1960 March 27 at 06:43:57.7 UTC
Greatest Eclipse1960 March 27 at 07:25:07.4 UTC
Ecliptic Conjunction1960 March 27 at 07:37:51.6 UTC
Last Penumbral External Contact1960 March 27 at 09:21:54.0 UTC
March 27, 1960 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.70578
Eclipse Obscuration0.62365
Gamma−1.15375
Sun Right Ascension00h24m22.7s
Sun Declination+02°38'08.8"
Sun Semi-Diameter16'01.4"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension00h25m42.2s
Moon Declination+01°35'48.1"
Moon Semi-Diameter15'29.5"
Moon Equatorial Horizontal Parallax0°56'51.5"
ΔT33.3 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 1960
March 13
Ascending node (full moon)
March 27
Descending node (new moon)
Lunar eclipse chart close-1960Mar13.png SE1960Mar27P.png
Total lunar eclipse
Lunar Saros 122
Partial solar eclipse
Solar Saros 148

Eclipses in 1960

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 148

Inex

Triad

Solar eclipses of 1957–1960

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. [3]

Solar eclipse series sets from 1957 to 1960
Descending node Ascending node
SarosMapGammaSarosMapGamma
118 April 30, 1957
SE1957Apr30A.png
Annular (non-central)
0.9992123 October 23, 1957
SE1957Oct23T.png
Total (non-central)
1.0022
128 April 19, 1958
SE1958Apr19A.png
Annular
0.275133 October 12, 1958
SE1958Oct12T.png
Total
−0.2951
138 April 8, 1959
SE1959Apr08A.png
Annular
−0.4546143 October 2, 1959
SE1959Oct02T.png
Total
0.4207
148 March 27, 1960
SE1960Mar27P.png
Partial
−1.1537153 September 20, 1960
SE1960Sep20P.png
Partial
1.2057

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. [4]

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 March 27, 1884 and August 20, 1971
March 27–29January 14November 1–2August 20–21June 8
108110112114116
SE1884Mar27P.gif
March 27, 1884
SE1895Aug20P.gif
August 20, 1895
SE1899Jun08P.gif
June 8, 1899
118120122124126
SE1903Mar29A.png
March 29, 1903
SE1907Jan14T.png
January 14, 1907
SE1910Nov02P.png
November 2, 1910
SE1914Aug21T.png
August 21, 1914
SE1918Jun08T.png
June 8, 1918
128130132134136
SE1922Mar28A.png
March 28, 1922
SE1926Jan14T.png
January 14, 1926
SE1929Nov01A.png
November 1, 1929
SE1933Aug21A.png
August 21, 1933
SE1918Jun08T.png
June 8, 1937
138140142144146
SE1941Mar27A.png
March 27, 1941
SE1945Jan14A.png
January 14, 1945
SE1948Nov01T.png
November 1, 1948
SE1952Aug20A.png
August 20, 1952
SE1956Jun08T.png
June 8, 1956
148150152154
SE1960Mar27P.png
March 27, 1960
SE1964Jan14P.png
January 14, 1964
SE1967Nov02T.png
November 2, 1967
SE1971Aug20P.png
August 20, 1971

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 eclipses on November 16, 2134 (part of Saros 164) and October 16, 2145 (part of Saros 165) are also a part of this series but are not included in the table below.

Series members between 1801 and 2069
SE1807Jun06H.png
June 6, 1807
(Saros 134)
SE1818May05A.gif
May 5, 1818
(Saros 135)
SE1829Apr03T.gif
April 3, 1829
(Saros 136)
SE1840Mar04A.png
March 4, 1840
(Saros 137)
SE1851Feb01A.gif
February 1, 1851
(Saros 138)
SE1861Dec31T.gif
December 31, 1861
(Saros 139)
SE1872Nov30H.gif
November 30, 1872
(Saros 140)
SE1883Oct30A.gif
October 30, 1883
(Saros 141)
SE1894Sep29T.gif
September 29, 1894
(Saros 142)
SE1905Aug30T.png
August 30, 1905
(Saros 143)
SE1916Jul30A.png
July 30, 1916
(Saros 144)
SE1927Jun29T.png
June 29, 1927
(Saros 145)
SE1938May29T.png
May 29, 1938
(Saros 146)
SE1949Apr28P.png
April 28, 1949
(Saros 147)
SE1960Mar27P.png
March 27, 1960
(Saros 148)
SE1971Feb25P.png
February 25, 1971
(Saros 149)
SE1982Jan25P.png
January 25, 1982
(Saros 150)
SE1992Dec24P.png
December 24, 1992
(Saros 151)
SE2003Nov23T.png
November 23, 2003
(Saros 152)
SE2014Oct23P.png
October 23, 2014
(Saros 153)
SE2025Sep21P.png
September 21, 2025
(Saros 154)
SE2036Aug21P.png
August 21, 2036
(Saros 155)
SE2047Jul22P.png
July 22, 2047
(Saros 156)
SE2058Jun21P.png
June 21, 2058
(Saros 157)
SE2069May20P.png
May 20, 2069
(Saros 158)

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
SE1815Jul06T.png
July 6, 1815
(Saros 143)
SE1844Jun16P.png
June 16, 1844
(Saros 144)
SE1873May26P.png
May 26, 1873
(Saros 145)
SE1902May07P.png
May 7, 1902
(Saros 146)
SE1931Apr18P.png
April 18, 1931
(Saros 147)
SE1960Mar27P.png
March 27, 1960
(Saros 148)
SE1989Mar07P.png
March 7, 1989
(Saros 149)
SE2018Feb15P.png
February 15, 2018
(Saros 150)
SE2047Jan26P.png
January 26, 2047
(Saros 151)
SE2076Jan06T.png
January 6, 2076
(Saros 152)
Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
(Saros 153)
Saros154 13van71 SE2133Nov26A.jpg
November 26, 2133
(Saros 154)
Saros155 14van71 SE2162Nov07T.jpg
November 7, 2162
(Saros 155)
Saros156 11van69 SE2191Oct18A.jpg
October 18, 2191
(Saros 156)

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References

  1. "March 27, 1960 Partial Solar Eclipse". timeanddate. Retrieved 6 August 2024.
  2. "Partial Solar Eclipse of 1960 Mar 27". EclipseWise.com. Retrieved 6 August 2024.
  3. 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.
  4. "NASA - Catalog of Solar Eclipses of Saros 148". eclipse.gsfc.nasa.gov.