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 | |
Type of eclipse | |
Nature | Total |
Gamma | 0.3943 |
Magnitude | 1.0249 |
Maximum eclipse | |
Duration | 130 s (2 min 10 s) |
Coordinates | 44°48′N 46°30′W / 44.8°N 46.5°W |
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.[1] 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.
Viewing
[edit]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 the total solar eclipse, and the Smithsonian Solar Eclipse Expedition hoped to capture photographic images of the solar corona during the event for further study.[2] The team included Thomas Smillie, the mission's photographer. 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. Smillie's work was considered an amazing photographic and scientific achievement.[3]
In addition to the team from the Smithsonian:
[s]cientific expeditions were mounted from some of the world’s preeminent astronomy programs including Princeton University, the University of Chicago, . . . and the British Astronomical Association. S. P. Langley and C. A. Young, two of the founders of modern astronomy, were also there.
According to Wadesboro's newspaper, the Anson Independent, the public came out in droves. Extra trains—including a special excursion train from Charlotte—brought out hundreds of people, and by the time the eclipse’s effects were beginning to be seen around 7:30 a.m., the streets were packed, and people were vying for better spots from rooftops and windows..
The same local newspaper described the total eclipse itself as lasting for less than a minute and a half, and recorded that though a large crowd was on hand, it was nearly silent during that entire time. The paper also mentioned that the drop in temperature from the shadow caused by the eclipse was quite significant.[2]
The eclipse was filmed by Nevil Maskelyne in North Carolina.[4] It was also observed from Mahelma in Algeria by John Evershed.[5]
![]() A map from 1900 |
![]() The stars during total eclipse |
Recording of the eclipse |
Next Solar Eclipses in Central Europe (120° east of USA)
[edit]Related eclipses
[edit]Solar eclipses of 1898–1902
[edit]This eclipse is a member of a semester series. An eclipse 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.[6]
The partial solar eclipse on April 8, 1902 occurs in the next lunar year eclipse set.
Solar eclipse series sets from 1898 to 1902 | ||||||
---|---|---|---|---|---|---|
Ascending node | Descending node | |||||
Saros | Map | Gamma | Saros | Map | Gamma | |
111 | December 13, 1898![]() Partial |
−1.5252 | 116 | June 8, 1899![]() Partial |
1.2089 | |
121 | December 3, 1899![]() Annular |
−0.9061 | 126 | May 28, 1900![]() Total |
0.3943 | |
131 | November 22, 1900![]() Annular |
−0.2245 | 136 | May 18, 1901![]() Total |
−0.3626 | |
141 | November 11, 1901![]() Annular |
0.4758 | 146 | May 7, 1902![]() Partial |
−1.0831 | |
151 | October 31, 1902![]() Partial |
1.1556 |
Saros 126
[edit]This eclipse is a part of Saros series 126, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on March 10, 1179. It contains annular eclipses from June 4, 1323 through April 4, 1810; hybrid eclipses from April 14, 1828 through May 6, 1864; and total eclipses from May 17, 1882 through August 23, 2044. The series ends at member 72 as a partial eclipse on May 3, 2459. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of annularity was produced by member 11 at 6 minutes, 30 seconds on June 26, 1359, and the longest duration of totality was produced by member 45 at 2 minutes, 36 seconds on July 10, 1972. All eclipses in this series occur at the Moon’s descending node of orbit.[7]
Series members 36–57 occur between 1801 and 2200: | ||
---|---|---|
36 | 37 | 38 |
![]() April 4, 1810 |
![]() April 14, 1828 |
![]() April 25, 1846 |
39 | 40 | 41 |
![]() May 6, 1864 |
![]() May 17, 1882 |
![]() May 28, 1900 |
42 | 43 | 44 |
![]() June 8, 1918 |
![]() June 19, 1936 |
![]() June 30, 1954 |
45 | 46 | 47 |
![]() July 10, 1972 |
![]() July 22, 1990 |
![]() August 1, 2008 |
48 | 49 | 50 |
![]() August 12, 2026 |
![]() August 23, 2044 |
![]() September 3, 2062 |
51 | 52 | 53 |
![]() September 13, 2080 |
![]() September 25, 2098 |
![]() October 6, 2116 |
54 | 55 | 56 |
![]() October 17, 2134 |
![]() October 28, 2152 |
![]() November 8, 2170 |
57 | ||
![]() November 18, 2188 |
Notes
[edit]- ^ "SOL'S FACE WAS VEILED. Wonderful Eclipse Observed at Many Places". Knoxville Sentinel. Knoxville, Tennessee. 1900-05-28. p. 1. Retrieved 2023-10-27 – via Newspapers.com.
- ^ a b "Wadesboro Prime for Viewing of 1900 Solar Eclipse". This Day in North Carolina History. N.C. Department of Natural & Cultural Resources. 28 May 2016. Retrieved 28 May 2019.
- ^ Foresta, Merry. "Smillie and the 1900 Eclipse". Smithsonian Institution Archives.
- ^ "‘Captivating’ – BFI shares first footage of a solar eclipse from 1900" (retrieved 30 May 2019)
- ^ J. Evershed (1900-01-01). Solar Eclipse of May 28, 1900. Preliminary Report of the Expedition to the South Limit of Totality to Obtain Photographs of the Flash Spectrum in High Solar Latitudes. The Royal Society.
- ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
- ^ "NASA - Catalog of Solar Eclipses of Saros 126". eclipse.gsfc.nasa.gov.
References
[edit]Media related to Solar eclipse of 1900 May 28 at Wikimedia Commons
- NASA graphic
- Photos and sketches of the Solar Corona May 28, 1900
- The Total Solar Eclipse, 1900 Report of the expeditions organized by the British Astronomical Association to observe the total solar eclipse of 1900, May 28, A Publication of the British Astronomical Association, Chapter VII: "Elche" (Spain), by Mr. E. W. Johnson
- Total Eclipses of the Sun, By Mabel Loomis Todd, 1894, new and revised edition by David Peck Todd, 1900.
- Lewis E. Jewell et al. "Reports concerning the total solar eclipse of May 28, 1900 and of May 17, 1901”, Publications of the U.S. Naval Observatory 4 (1906) app. 1, 94–97, 121–151, 203–215, 299–307 and pl. LXXII.
- Russia expedition for solar eclipse of May 28, 1900 Archived August 8, 2009, at the Wayback Machine
- "Print from Glass Plate Negative of eclipse, Wilkes County, Georgia, 1900 May 28". Vanishing Georgia, Georgia Archives. Digital Library of Georgia. Retrieved 5 April 2018.