Solar eclipse of March 25, 1857

Solar eclipse of March 25, 1857
Map
Type of eclipse
Nature	Total
Gamma	-0.0892
Magnitude	1.0534
Maximum eclipse
Duration	268 sec (4 m 28 s)
Coordinates	2°24′S 153°24′W / 2.4°S 153.4°W
Max. width of band	177 km (110 mi)
Times (UTC)
Greatest eclipse	22:29:38
References
Saros	127 (49 of 82)
Catalog # (SE5000)	9179

A total solar eclipse occurred on March 25, 1857. 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. Totality began at sunrise over southeastern Australia on March 26, crossing the Pacific ocean, and ended near sunset across Mexico on March 25.

Related eclipses

Saros series 127

It is a part of Saros cycle 127, repeating every 18 years, 11 days, containing 82 events. The series started with partial solar eclipse on October 10, 991 AD. It contains total eclipses from May 14, 1352 through August 15, 2091. The series ends at member 82 as a partial eclipse on March 21, 2452. The longest duration of totality was 5 minutes, 40 seconds on August 30, 1532.^[1]

Series members 52–62 occur between 1901 and 2100
52	53	54
April 28, 1911	May 9, 1929	May 20, 1947
55	56	57
May 30, 1965	June 11, 1983	June 21, 2001
58	59	60
July 2, 2019	July 13, 2037	July 24, 2055
61	62
August 3, 2073	August 15, 2091

Notes

1. http://eclipse.gsfc.nasa.gov/SEsaros/SEsaros127.html

References

• NASA graphic
  • Googlemap
  • NASA Besselian elements
• The Sun, Charles Young, 1898,
• Observations made at Sydney during the Eclipse of the Sun, March 26, 1857 Clarke, W. B., Monthly Notices of the Royal Astronomical Society, Vol. 18, p. 39-44