Solar eclipse of October 2, 1978

Last updated
Solar eclipse of October 2, 1978
SE1978Oct02P.png
Map
Type of eclipse
NaturePartial
Gamma 1.1616
Magnitude 0.6905
Maximum eclipse
Coordinates 72°00′N159°36′E / 72°N 159.6°E / 72; 159.6
Times (UTC)
Greatest eclipse6:28:43
References
Saros 153 (7 of 70)
Catalog # (SE5000) 9461

A partial solar eclipse occurred at the Moon's ascending node of orbit on Monday, October 2, 1978, [1] with a magnitude of 0.6905. 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 North Asia and East Asia.

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]

October 2, 1978 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1978 October 02 at 04:31:44.0 UTC
Equatorial Conjunction1978 October 02 at 05:46:52.4 UTC
Greatest Eclipse1978 October 02 at 06:28:43.3 UTC
Ecliptic Conjunction1978 October 02 at 06:41:27.8 UTC
Last Penumbral External Contact1978 October 02 at 08:25:57.0 UTC
October 2, 1978 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.69055
Eclipse Obscuration0.60402
Gamma1.16164
Sun Right Ascension12h32m00.9s
Sun Declination-03°27'16.5"
Sun Semi-Diameter15'58.8"
Sun Equatorial Horizontal Parallax08.8"
Moon Right Ascension12h33m20.1s
Moon Declination-02°25'05.3"
Moon Semi-Diameter15'20.8"
Moon Equatorial Horizontal Parallax0°56'19.5"
ΔT49.3 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 September–October 1978
September 16
Descending node (full moon)
October 2
Ascending node (new moon)
Lunar eclipse chart close-1978Sep16.png SE1978Oct02P.png
Total lunar eclipse
Lunar Saros 127
Partial solar eclipse
Solar Saros 153

Eclipses in 1978

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 153

Inex

Triad

Solar eclipses of 1975–1978

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 1975 to 1978
Descending node Ascending node
SarosMapGammaSarosMapGamma
118 May 11, 1975
SE1975May11P.png
Partial
1.0647123 November 3, 1975
SE1975Nov03P.png
Partial
−1.0248
128 April 29, 1976
SE1976Apr29A.png
Annular
0.3378133 October 23, 1976
SE1976Oct23T.png
Total
−0.327
138 April 18, 1977
SE1977Apr18A.png
Annular
−0.399143 October 12, 1977
SE1977Oct12T.png
Total
0.3836
148 April 7, 1978
SE1978Apr07P.png
Partial
−1.1081153 October 2, 1978
SE1978Oct02P.png
Partial
1.1616

Saros 153

This eclipse is a part of Saros series 153, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on July 28, 1870. It contains annular eclipses from December 17, 2104 through May 26, 2970. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on August 22, 3114. 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 7 minutes, 1 seconds on September 5, 2537. All eclipses in this series occur at the Moon’s ascending node of orbit. [4]

Series members 1–19 occur between 1870 and 2200:
123
SE1870Jul28Pb.gif
July 28, 1870
SE1888Aug07P.gif
August 7, 1888
SE1906Aug20P.png
August 20, 1906
456
SE1924Aug30P.png
August 30, 1924
SE1942Sep10P.png
September 10, 1942
SE1960Sep20P.png
September 20, 1960
789
SE1978Oct02P.png
October 2, 1978
SE1996Oct12P.png
October 12, 1996
SE2014Oct23P.png
October 23, 2014
101112
SE2032Nov03P.png
November 3, 2032
SE2050Nov14P.png
November 14, 2050
SE2068Nov24P.png
November 24, 2068
131415
SE2086Dec06P.png
December 6, 2086
Saros153 14van70 SE2104Dec17A.jpg
December 17, 2104
Saros153 15van70 SE2122Dec28A.jpg
December 28, 2122
161718
Saros153 16van70 SE2141Jan08A.jpg
January 8, 2141
Saros153 17van70 SE2159Jan19A.jpg
January 19, 2159
Saros153 18van70 SE2177Jan29A.jpg
January 29, 2177
19
Saros153 19van70 SE2195Feb10A.jpg
February 10, 2195

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.

22 eclipse events between December 13, 1898 and July 20, 1982
December 13–14October 1–2July 20–21May 9February 24–25
111113115117119
SE1898Dec13P.gif
December 13, 1898
SE1906Jul21P.png
July 21, 1906
SE1910May09T.png
May 9, 1910
SE1914Feb25A.png
February 25, 1914
121123125127129
SE1917Dec14A.png
December 14, 1917
SE1921Oct01T.png
October 1, 1921
SE1925Jul20A.png
July 20, 1925
SE1929May09T.png
May 9, 1929
SE1933Feb24A.png
February 24, 1933
131133135137139
SE1936Dec13A.png
December 13, 1936
SE1940Oct01T.png
October 1, 1940
SE1944Jul20A.png
July 20, 1944
SE1948May09A.png
May 9, 1948
SE1952Feb25T.png
February 25, 1952
141143145147149
SE1955Dec14A.png
December 14, 1955
SE1959Oct02T.png
October 2, 1959
SE1963Jul20T.png
July 20, 1963
SE1967May09P.png
May 9, 1967
SE1971Feb25P.png
February 25, 1971
151153155
SE1974Dec13P.png
December 13, 1974
SE1978Oct02P.png
October 2, 1978
SE1982Jul20P.png
July 20, 1982

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
SE1805Jan30P.gif
January 30, 1805
(Saros 147)
SE1834Jan09P.gif
January 9, 1834
(Saros 148)
SE1862Dec21P.gif
December 21, 1862
(Saros 149)
SE1891Dec01P.gif
December 1, 1891
(Saros 150)
SE1920Nov10P.png
November 10, 1920
(Saros 151)
SE1949Oct21P.png
October 21, 1949
(Saros 152)
SE1978Oct02P.png
October 2, 1978
(Saros 153)
SE2007Sep11P.png
September 11, 2007
(Saros 154)
SE2036Aug21P.png
August 21, 2036
(Saros 155)
SE2065Aug02P.png
August 2, 2065
(Saros 156)
SE2094Jul12P.png
July 12, 2094
(Saros 157)
Saros158 04van70 SE2123Jun23P.jpg
June 23, 2123
(Saros 158)
Saros159 02van70 SE2152Jun03P.jpg
June 3, 2152
(Saros 159)
Saros160 01van71 SE2181May13P.jpg
May 13, 2181
(Saros 160)

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References

  1. "October 2, 1978 Partial Solar Eclipse". timeanddate. Retrieved 8 August 2024.
  2. "Partial Solar Eclipse of 1978 Oct 02". EclipseWise.com. Retrieved 8 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 153". eclipse.gsfc.nasa.gov.