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Solar eclipse of May 28, 1900
Thomas Smillie - Smithsonian Institution - Corona of the Sun during a Solar Eclipse (pd).jpg
Totality photographed in Wadesboro, North Carolina by Thomas Smillie for the Smithsonian Solar Eclipse Expedition to capture photographic proof of the solar corona
SE1900May28T.png
Map
Type of eclipse
Nature Total
Gamma 0.3943
Magnitude 1.0249
Maximum eclipse
Duration 2m 10s
Coordinates 44.8N 46.5W
Max. width of band 92 km
Times (UTC)
Greatest eclipse 14:53:56
References
Saros 126 (41 of 72)
Catalog # (SE5000) 9281

A total solar eclipse occurred on May 28, 1900. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partially obscuring Earth's view of the Sun. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across the surface of the Earth, while a partial solar eclipse will be visible over a region thousands of miles wide.

Contents

Viewing

In 1900 the Smithsonian Astrophysical Observatory, then based in Washington, D.C., loaded several railroad cars with scientific equipment and headed to Wadesboro, North Carolina. Scientists had determined that this small town would be the best location in North America for viewing an expected total solar eclipse, and the Smithsonian Solar Eclipse Expedition hoped to capture photographic proof of the solar corona during the event for further study. The team included Smithsonian photographer Thomas Smillie, who headed up the missions photographic component. Smillie rigged cameras to seven telescopes and successfully made eight glass-plate negatives, ranging in size from eleven by fourteen inches to thirty by thirty inches. At the time, Smillie's work was considered an amazing photographic and scientific achievement.

Solar eclipse 1900May28-map.png
A map from 1900
Solar eclipse 1900May28-stars.png
The stars during total eclipse

Related eclipses

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Saros 126

It is a part of Saros cycle 126, repeating every 18 year, 11 days, containing 71 events. The series started with partial solar eclipse on March 10, 1179. It contains annular eclipses from June 4, 1323 through April 4, 1910 and hybrid eclipses from April 14, 1828 through May 6, 1864. It contains total eclipses from May 17, 1882 through August 23, 2044. The series ends at member 72 as a partial eclipse on May 3, 2459. The longest duration of totality was 5 minutes, 46 seconds on November 22, 1593.[1]

Series members 39-49 occur between 1901 and 2100:

39 40 41
SE1918Jun08T.png
June 8, 1918
SE1936Jun19T.png
June 19, 1936
SE1954Jun30T.png
June 30, 1954
42 43 44
SE1972Jul10T.png
July 10, 1972
SE1990Jul22T.png
July 22, 1990
SE2008Aug01T.png
August 1, 2008
45 46 47
SE2026Aug12T.png
August 12, 2026
SE2044Aug23T.png
August 23, 2044
SE2062Sep03P.png
September 3, 2062
48 49
SE2080Sep13P.png
September 13, 2080
SE2098Sep25P.png
September 25, 2098

Notes

References


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