Solar eclipse of October 2, 1959

Solar eclipse of October 2, 1959
Map
Type of eclipse
Nature Total
Gamma 0.4207
Magnitude 1.0325
Maximum eclipse
Duration 182 sec (3 m 2 s)
Coordinates 20°24′N 1°24′W / 20.4°N 1.4°W / 20.4; -1.4
Max. width of band 120 km (75 mi)
Times (UTC)
Greatest eclipse 12:27:00
References
Saros 143 (20 of 72)
Catalog # (SE5000) 9419

A total solar eclipse occurred on October 2, 1959. 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.

Observations

Totality began over Boston, Massachusetts at sunrise. Viewing the eclipse was rained out, but it was reported that the brightening of the sky after the eclipse was a startling and impressive sight.[1] A few photographers captured the eclipse from airplanes above the clouds, and a multiple exposure was made atop the R. C. A. building in New York City.[2] The next total eclipse over Boston, the solar eclipse of May 1, 2079, will also be a sunrise event.[3]

The event was also observed at the Canarian Island of Fuerta Ventura by a team of Dutch astronomers of the university of Utrecht and Amsterdam.[4][5]

Solar eclipses of 1957-1960

Each member 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.

Solar eclipse series sets from 1957–1960
Descending node   Ascending node
SarosMap SarosMap
118
April 30, 1957
Annular		 123
October 23, 1957
Total
128
April 19, 1958
Annular		 133
October 12, 1958
Total
138
April 8, 1959
Annular		 143
October 2, 1959
Total
148
March 27, 1960
Partial		 153
September 20, 1960
Partial

Solar 143

It is a part of Saros cycle 143, repeating every 18 years, 11 days, containing 72 events. The series started with partial solar eclipse on March 7, 1617 and total event from June 24, 1797 through October 24, 1995. It has hybrid eclipses from November 3, 2013 through December 6, 2067, and annular eclipses from December 16, 2085 through September 16, 2536. The series ends at member 72 as a partial eclipse on April 23, 2873. The longest duration of totality was 3 minutes, 50 seconds on August 19, 1887.[6]

See also

Notes

  1. ↑ Journal of the Royal Astronomical Society of Canada, Vol. 54, p.43,
  2. ↑ Sky and Telescope, Vol. XIX, No. 1, p. 4.
  3. ↑ http://www.space.com/spacewatch/050408_solar_eclipse.html
  4. ↑ http://www.staff.science.uu.nl/~rutte101/Utrecht_eclipse.html
  5. ↑ Report of the Netherlands expedition for the observation of the total solar eclipse on october 2, 1959. Houtgast, J., Proceedings of the Royal Netherlands Academy of Arts and Sciences, Vol. 63, Nr. 5, p. 611 (1960)
  6. ↑ http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros143.html

References

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