Solar eclipse of May 28, 1900

Solar eclipse of May 28, 1900
Totality photographed in Wadesboro, North Carolina, by Thomas Smillie for the Smithsonian Solar Eclipse Expedition to capture photographic proof of the solar corona
Map
Type of eclipse
Nature	Total
Gamma	0.3943
Magnitude	1.0249
Maximum eclipse
Duration	130 sec (2 m 10 s)
Coordinates	44°48′N 46°30′W / 44.8°N 46.5°W / 44.8; -46.5
Max. width of band	92 km (57 mi)
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 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.

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.

It is a part of Saros cycle 126, repeating every 18 years, 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, 1810 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 central eclipse (annular or total) was 5 minutes, 46 seconds of annularity on November 22, 1593. The longest duration of totality was 2 minutes, 36 seconds on July 10, 1972.