Solar eclipse of March 7, 1951

Last updated
Solar eclipse of March 7, 1951
SE1951Mar07A.png
Map
Type of eclipse
NatureAnnular
Gamma −0.242
Magnitude 0.9896
Maximum eclipse
Duration59 s (0 min 59 s)
Coordinates 17°42′S123°30′W / 17.7°S 123.5°W / -17.7; -123.5
Max. width of band38 km (24 mi)
Times (UTC)
Greatest eclipse20:53:40
References
Saros 129 (48 of 80)
Catalog # (SE5000) 9400

An annular solar eclipse occurred at the Moon's ascending node of orbit between Wednesday, March 7 and Thursday, March 8, 1951, [1] with a magnitude of 0.9896. 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. The Moon's apparent diameter was near the average diameter because it occurred 5.5 days after perigee (on March 2, 1951, at 7:10 UTC) and 7.4 days before apogee (on March 15, 1951, at 6:20 UTC). [2]

Contents

Annularity was visible from New Zealand on March 8 (Thursday), and northern Costa Rica, Nicaragua, and San Andrés Island in Colombia on March 7 (Wednesday). A partial eclipse was visible for parts of Oceania, western South America, southern North America, Central America, and the Caribbean.

Broadcast

This was the first solar eclipse in the world broadcast live on television. American stations such as WCBS-TV, WNET, and NBC News broadcast it live. The path of annularity did not pass the United States of America, and only a partial solar eclipse was visible from the southeastern half of the country. For example, in New York City, a partial solar eclipse occurred right before the sunset, whose gratitude (ratio of diameter covered by the moon) was only 17%, meaning only 8% of the total disk area was covered at the peak of the eclipse. The curator of the Hayden Planetarium in New York also asked "don’t get people too excited about it" in an interview with The New York Times, but many TV stations still incorporated the solar eclipse into their regular afternoon schedule and also some new TV technology was inaugurated. [3]

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]

March 7, 1951 Solar Eclipse Times
EventTime (UTC)
First Penumbral External Contact1951 March 07 at 18:04:26.8 UTC
First Umbral External Contact1951 March 07 at 19:05:55.2 UTC
First Central Line1951 March 07 at 19:06:44.2 UTC
First Umbral Internal Contact1951 March 07 at 19:07:33.2 UTC
First Penumbral Internal Contact1951 March 07 at 20:12:35.1 UTC
Equatorial Conjunction1951 March 07 at 20:39:08.0 UTC
Ecliptic Conjunction1951 March 07 at 20:51:00.5 UTC
Greatest Eclipse1951 March 07 at 20:53:39.9 UTC
Last Penumbral Internal Contact1951 March 07 at 21:35:03.7 UTC
Last Umbral Internal Contact1951 March 07 at 22:39:53.5 UTC
Last Central Line1951 March 07 at 22:40:45.3 UTC
Greatest Duration1951 March 07 at 22:40:45.3 UTC
Last Umbral External Contact1951 March 07 at 22:41:37.2 UTC
Last Penumbral External Contact1951 March 07 at 23:43:05.1 UTC
March 7, 1951 Solar Eclipse Parameters
ParameterValue
Eclipse Magnitude0.98959
Eclipse Obscuration0.97930
Gamma−0.24196
Sun Right Ascension23h10m14.1s
Sun Declination-05°20'18.6"
Sun Semi-Diameter16'06.8"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension23h10m40.8s
Moon Declination-05°32'31.4"
Moon Semi-Diameter15'42.0"
Moon Equatorial Horizontal Parallax0°57'37.1"
ΔT29.6 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. The first and last eclipse in this sequence is separated by one synodic month.

Eclipse season of February–March 1951
February 21
Descending node (full moon)
March 7
Ascending node (new moon)
March 23
Descending node (full moon)
Lunar eclipse chart close-1951Feb21.png SE1951Mar07A.png Lunar eclipse chart close-1951Mar23.png
Penumbral lunar eclipse
Lunar Saros 103
Annular solar eclipse
Solar Saros 129
Penumbral lunar eclipse
Lunar Saros 141

Eclipses in 1951

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 129

Inex

Triad

Solar eclipses of 1950–1953

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 July 11, 1953 occurs in the next lunar year eclipse set.

Solar eclipse series sets from 1950 to 1953
Ascending node Descending node
SarosMapGammaSarosMapGamma
119 March 18, 1950
SE1950Mar18A.png
Annular (non-central)
0.9988124 September 12, 1950
SE1950Sep12T.png
Total
0.8903
129 March 7, 1951
SE1951Mar07A.png
Annular
−0.242134 September 1, 1951
SE1951Sep01A.png
Annular
0.1557
139 February 25, 1952
SE1952Feb25T.png
Total
0.4697144 August 20, 1952
SE1952Aug20A.png
Annular
−0.6102
149 February 14, 1953
SE1953Feb14P.png
Partial
1.1331154 August 9, 1953
SE1953Aug09P.png
Partial
−1.344

Saros 129

This eclipse is a part of Saros series 129, repeating every 18 years, 11 days, and containing 80 events. The series started with a partial solar eclipse on October 3, 1103. It contains annular eclipses from May 6, 1464 through March 18, 1969; hybrid eclipses from March 29, 1987 through April 20, 2023; and total eclipses from April 30, 2041 through July 26, 2185. The series ends at member 80 as a partial eclipse on February 21, 2528. 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 was produced by member 34 at 5 minutes, 10 seconds on October 4, 1698, and the longest duration of totality will be produced by member 58 at 3 minutes, 43 seconds on June 25, 2131. All eclipses in this series occur at the Moon’s ascending node of orbit. [6]

Series members 40–61 occur between 1801 and 2200:
404142
SE1806Dec10A.gif
December 10, 1806
SE1824Dec20Am.gif
December 20, 1824
SE1842Dec31A.gif
December 31, 1842
434445
SE1861Jan11A.gif
January 11, 1861
SE1879Jan22A.gif
January 22, 1879
SE1897Feb01A.gif
February 1, 1897
464748
SE1915Feb14A.png
February 14, 1915
SE1933Feb24A.png
February 24, 1933
SE1951Mar07A.png
March 7, 1951
495051
SE1969Mar18A.png
March 18, 1969
SE1987Mar29H.png
March 29, 1987
SE2005Apr08H.png
April 8, 2005
525354
SE2023Apr20H.png
April 20, 2023
SE2041Apr30T.png
April 30, 2041
SE2059May11T.png
May 11, 2059
555657
SE2077May22T.png
May 22, 2077
SE2095Jun02T.png
June 2, 2095
Saros129 57van80 SE2113Jun13T.jpg
June 13, 2113
585960
Saros129 58van80 SE2131Jun25T.jpg
June 25, 2131
Saros129 59van80 SE2149Jul05T.jpg
July 5, 2149
Saros129 60van80 SE2167Jul16T.jpg
July 16, 2167
61
Saros129 61van80 SE2185Jul26T.jpg
July 26, 2185

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 24, 1916 and July 31, 2000
December 24–25October 12July 31–August 1May 19–20March 7
111113115117119
SE1916Dec24P.png
December 24, 1916
SE1924Jul31P.png
July 31, 1924
SE1928May19T.png
May 19, 1928
SE1932Mar07A.png
March 7, 1932
121123125127129
SE1935Dec25A.png
December 25, 1935
SE1939Oct12T.png
October 12, 1939
SE1943Aug01A.png
August 1, 1943
SE1947May20T.png
May 20, 1947
SE1951Mar07A.png
March 7, 1951
131133135137139
SE1954Dec25A.png
December 25, 1954
SE1958Oct12T.png
October 12, 1958
SE1962Jul31A.png
July 31, 1962
SE1966May20A.png
May 20, 1966
SE1970Mar07T.png
March 7, 1970
141143145147149
SE1973Dec24A.png
December 24, 1973
SE1977Oct12T.png
October 12, 1977
SE1981Jul31T.png
July 31, 1981
SE1985May19P.png
May 19, 1985
SE1989Mar07P.png
March 7, 1989
151153155
SE1992Dec24P.png
December 24, 1992
SE1996Oct12P.png
October 12, 1996
SE2000Jul31P.png
July 31, 2000

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 2200
SE1809Apr14A.gif
April 14, 1809
(Saros 116)
SE1820Mar14T.gif
March 14, 1820
(Saros 117)
SE1831Feb12A.gif
February 12, 1831
(Saros 118)
SE1842Jan11A.gif
January 11, 1842
(Saros 119)
SE1852Dec11T.gif
December 11, 1852
(Saros 120)
SE1863Nov11A.png
November 11, 1863
(Saros 121)
SE1874Oct10An.gif
October 10, 1874
(Saros 122)
SE1885Sep08T.png
September 8, 1885
(Saros 123)
SE1896Aug09T.png
August 9, 1896
(Saros 124)
SE1907Jul10A.png
July 10, 1907
(Saros 125)
SE1918Jun08T.png
June 8, 1918
(Saros 126)
SE1929May09T.png
May 9, 1929
(Saros 127)
SE1940Apr07A.png
April 7, 1940
(Saros 128)
SE1951Mar07A.png
March 7, 1951
(Saros 129)
SE1962Feb05T.png
February 5, 1962
(Saros 130)
SE1973Jan04A.png
January 4, 1973
(Saros 131)
SE1983Dec04A.png
December 4, 1983
(Saros 132)
SE1994Nov03T.png
November 3, 1994
(Saros 133)
SE2005Oct03A.png
October 3, 2005
(Saros 134)
SE2016Sep01A.png
September 1, 2016
(Saros 135)
SE2027Aug02T.png
August 2, 2027
(Saros 136)
SE2038Jul02A.png
July 2, 2038
(Saros 137)
SE2049May31A.png
May 31, 2049
(Saros 138)
SE2060Apr30T.png
April 30, 2060
(Saros 139)
SE2071Mar31A.png
March 31, 2071
(Saros 140)
SE2082Feb27A.png
February 27, 2082
(Saros 141)
SE2093Jan27T.png
January 27, 2093
(Saros 142)
SE2103Dec29A.png
December 29, 2103
(Saros 143)
SE2114Nov27A.png
November 27, 2114
(Saros 144)
SE2125Oct26T.png
October 26, 2125
(Saros 145)
SE2136Sep26T.png
September 26, 2136
(Saros 146)
Saros147 30van80 SE2147Aug26A.jpg
August 26, 2147
(Saros 147)
SE2158Jul25T.png
July 25, 2158
(Saros 148)
Saros149 29van71 SE2169Jun25T.jpg
June 25, 2169
(Saros 149)
Saros150 26van71 SE2180May24A.jpg
May 24, 2180
(Saros 150)
SE2191Apr23A.png
April 23, 2191
(Saros 151)

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
SE1806Jun16T.png
June 16, 1806
(Saros 124)
SE1835May27A.gif
May 27, 1835
(Saros 125)
SE1864May06H.gif
May 6, 1864
(Saros 126)
SE1893Apr16T.png
April 16, 1893
(Saros 127)
SE1922Mar28A.png
March 28, 1922
(Saros 128)
SE1951Mar07A.png
March 7, 1951
(Saros 129)
SE1980Feb16T.png
February 16, 1980
(Saros 130)
SE2009Jan26A.png
January 26, 2009
(Saros 131)
SE2038Jan05A.png
January 5, 2038
(Saros 132)
SE2066Dec17T.png
December 17, 2066
(Saros 133)
SE2095Nov27A.png
November 27, 2095
(Saros 134)
SE2124Nov06A.png
November 6, 2124
(Saros 135)
SE2153Oct17T.png
October 17, 2153
(Saros 136)
SE2182Sep27A.png
September 27, 2182
(Saros 137)

Notes

  1. "March 7, 1951 Annular Solar Eclipse". timeanddate. Retrieved 5 August 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 5 August 2024.
  3. Joe Rao (8 March 2011). "60 Years Ago: The World's 1st Televised Solar Eclipse". Space.com. Archived from the original on 21 September 2020.
  4. "Annular Solar Eclipse of 1951 Mar 07". EclipseWise.com. Retrieved 5 August 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 129". eclipse.gsfc.nasa.gov.

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References