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Solar eclipse of March 7, 1970

A total solar eclipse occurred at the Moon's ascending node of orbit on Saturday, March 7, 1970, with a magnitude of 1.0414. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.3 days after perigee, this eclipse occurred when the Moon's apparent diameter was larger.

Scientific effects
This eclipse slowed a radio transmission of atomic time from North Carolina to Washington, D.C. == Observations ==
Observations
An observation team from the Swiss Federal Observatory observed the total eclipse in Nejapa and Miahuatlán, Mexico. The weather conditions were good at both locations. Miahuatlán offered particularly good observation conditions with an altitude of 1,620 metres above sea level, high air quality and solar zenith angle of 63° at the time of the eclipse. The team took images of the corona and analyzed them with a polarizing filter. Austrian-American physicist Erwin Saxl and American physicist Mildred Allen reported anomalous changes in the period of a torsion pendulum when observing a partial solar eclipse with a magnitude of 0.954 from Harvard, Massachusetts, called the "Saxl Effect". Visible Planets and Stars During totality, other celestial objects brighter than magnitude 1.5 often become visible. By far the brightest and therefore easiest object seen around totality on 7/3/1970 was Venus, which lay about an hour east of the eclipsed Sun. Mars and Saturn were about three hours east of the Sun with Saturn the brighter planet, while Mercury, 16 days away from superior conjunction (and therefore showing most of its sunlit side, making it bright), was an hour or so west of the Sun. Of the stars, Fomalhaut was almost due south of the Sun, the Summer Triangle of Vega, Deneb and Altair was well up in the west, and recently risen Aldebaran and Capella were in the east and northeast respectively. == In popular culture ==
In popular culture
CBS showed the first color broadcast of a total eclipse. This eclipse might be referenced in the second episode of the first season of The Mary Tyler Moore Show when a guest of Mary's accidentally exposes a roll of film that Howard Arnell, an ex-boyfriend of Mary's, says, "It's just the pictures I took of the total eclipse of the sun." The eclipse may be referenced in the 1972 hit popular song “You're So Vain” by Carly Simon, although in context, the lyrics more closely align with a different eclipse two years later. == Eclipse details ==
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. == Eclipse season ==
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. == Related eclipses ==
Related eclipses
Eclipses in 1970 A partial lunar eclipse on February 21. • A total solar eclipse on March 7.A partial lunar eclipse on August 17. • An annular solar eclipse on August 31. Metonic • Preceded by: Solar eclipse of May 20, 1966 • Followed by: Solar eclipse of December 24, 1973 Tzolkinex • Preceded by: Solar eclipse of January 25, 1963 • Followed by: Solar eclipse of April 18, 1977 Half-Saros • Preceded by: Lunar eclipse of March 2, 1961 • Followed by: Lunar eclipse of March 13, 1979 Tritos • Preceded by: Solar eclipse of April 8, 1959 • Followed by: Solar eclipse of February 4, 1981 Solar Saros 139 • Preceded by: Solar eclipse of February 25, 1952 • Followed by: Solar eclipse of March 18, 1988 Inex • Preceded by: Solar eclipse of March 27, 1941 • Followed by: Solar eclipse of February 16, 1999 Triad • Preceded by: Solar eclipse of May 6, 1883 • Followed by: Solar eclipse of January 5, 2057 Solar eclipses of 1968–1971 Saros 139 Metonic series Tritos series Inex series ==Notes==
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