Solar eclipse of May 28, 1900
{{Short description|Total eclipse}}
{{Infobox solar eclipse|1900May28
| previous = Solar eclipse of December 3, 1899
| next = Solar eclipse of November 22, 1900
}}
A total solar eclipse occurred at the Moon's descending node of orbit on Monday, May 28, 1900,{{cite web|title=May 28, 1900 Total Solar Eclipse|url=https://www.timeanddate.com/eclipse/solar/1900-may-28|publisher=timeanddate|access-date=25 August 2024}}{{Cite news
| url = https://newspapers.com/article/knoxville-sentinel-sols-face-was-veiled/134153800/
| date = 1900-05-28
| page = 1
| title = SOL'S FACE WAS VEILED. Wonderful Eclipse Observed at Many Places.
| newspaper = Knoxville Sentinel
| location = Knoxville, Tennessee
| via = Newspapers.com
| access-date = 2023-10-27
}} with a magnitude of 1.0249. 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. Occurring about 3.9 days after perigee (on May 24, 1900, at 17:30 UTC), the Moon's apparent diameter was larger.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=1900&n=136|publisher=timeanddate|access-date=25 August 2024}}
The path of totality was visible from parts of Mexico, the states of Texas, Louisiana, Mississippi, Alabama, Georgia, South Carolina, North Carolina, and Virginia in the United States, Portugal, Spain, Algeria, Tripoli, and Egypt. A partial solar eclipse was also visible for parts of North America, Central America, the Caribbean, northern South America, Europe, West Africa, and North Africa.
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 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.{{cite web |title=Wadesboro Prime for Viewing of 1900 Solar Eclipse |url=https://www.ncdcr.gov/blog/2014/05/28/wadesboro-prime-for-viewing-of-1900-solar-eclipse |website=This Day in North Carolina History |date=28 May 2016 |publisher=N.C. Department of Natural & Cultural Resources |access-date=28 May 2019}} 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.{{cite web |last1=Foresta |first1=Merry |title=Smillie and the 1900 Eclipse |url=https://siarchives.si.edu/blog/smillie-and-1900-eclipse |website=Smithsonian Institution Archives}}
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.
The eclipse was filmed by Nevil Maskelyne in North Carolina.[https://www.theguardian.com/science/2019/may/30/captivating-bfi-shares-first-footage-of-a-solar-eclipse-from-1900-john-nevil-maskelyne "‘Captivating’ – BFI shares first footage of a solar eclipse from 1900"] (retrieved 30 May 2019) It was also observed from Mahelma in Algeria by John Evershed.{{Cite book|last=J. Evershed|url=https://archive.org/details/paper-doi-10_1098_rspl_1900_0041|title=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|date=1900-01-01|publisher=The Royal Society|language=English}}
240px A map from 1900 |240px |240px |
Eclipse details
Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.{{cite web|title=Total Solar Eclipse of 1900 May 28|url=https://eclipsewise.com/solar/SEprime/1801-1900/SE1900May28Tprime.html|publisher=EclipseWise.com|access-date=25 August 2024}}
class="wikitable" align="{{{align|left}}}" style="margin:{{#ifeq:{{{align}}}|left|0 0 0.5em 1em|0 1em 0.5em 0}}"
|+May 28, 1900 Solar Eclipse Times ! Event ! Time (UTC) |
First Penumbral External Contact
| 1900 May 28 at 12:12:21.6 UTC |
First Umbral External Contact
| 1900 May 28 at 13:14:08.2 UTC |
First Central Line
| 1900 May 28 at 13:14:27.0 UTC |
First Umbral Internal Contact
| 1900 May 28 at 13:14:45.8 UTC |
First Penumbral Internal Contact
| 1900 May 28 at 14:29:28.7 UTC |
Ecliptic Conjunction
| 1900 May 28 at 14:49:42.6 UTC |
Greatest Duration
| 1900 May 28 at 14:52:29.6 UTC |
Greatest Eclipse
| 1900 May 28 at 14:53:55.5 UTC |
Equatorial Conjunction
| 1900 May 28 at 14:56:57.5 UTC |
Last Penumbral Internal Contact
| 1900 May 28 at 15:18:16.5 UTC |
Last Umbral Internal Contact
| 1900 May 28 at 16:33:06.4 UTC |
Last Central Line
| 1900 May 28 at 16:33:22.5 UTC |
Last Umbral External Contact
| 1900 May 28 at 16:33:38.7 UTC |
Last Penumbral External Contact
| 1900 May 28 at 17:35:33.8 UTC |
class="wikitable" align="{{{align|right}}}" style="margin:{{#ifeq:{{{align}}}|right|0 0 0.5em 1em|0 1em 0.5em 0}}"
|+May 28, 1900 Solar Eclipse Parameters ! Parameter ! Value |
Eclipse Magnitude
| 1.02494 |
Eclipse Obscuration
| 1.05051 |
Gamma
| 0.39427 |
Sun Right Ascension
| 04h19m46.8s |
Sun Declination
| +21°27'14.4" |
Sun Semi-Diameter
| 15'46.6" |
Sun Equatorial Horizontal Parallax
| 08.7" |
Moon Right Ascension
| 04h19m39.8s |
Moon Declination
| +21°50'10.6" |
Moon Semi-Diameter
| 15'55.8" |
Moon Equatorial Horizontal Parallax
| 0°58'27.9" |
ΔT
| -2.2 s |
{{clear}}
Eclipse season
{{See also|Eclipse cycle}}
This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.
class="wikitable"
|+ Eclipse season of May–June 1900 ! May 28 | |
200px | |
align=center
| Total solar eclipse | Penumbral lunar eclipse Lunar Saros 138 |
Related eclipses
= Eclipses in 1900 =
- A total solar eclipse on May 28.
- A penumbral lunar eclipse on June 13.
- An annular solar eclipse on November 22.
- A penumbral lunar eclipse on December 6.
= Metonic =
- Preceded by: Solar eclipse of August 9, 1896
- Followed by: Solar eclipse of March 17, 1904
= Tzolkinex =
- Preceded by: Solar eclipse of April 16, 1893
- Followed by: Solar eclipse of July 10, 1907
= Half-Saros =
- Preceded by: Lunar eclipse of May 23, 1891
- Followed by: Lunar eclipse of June 4, 1909
= Tritos =
- Preceded by: Solar eclipse of June 28, 1889
- Followed by: Solar eclipse of April 28, 1911
= Solar Saros 126 =
- Preceded by: Solar eclipse of May 17, 1882
- Followed by: Solar eclipse of June 8, 1918
= Inex =
- Preceded by: Solar eclipse of June 18, 1871
- Followed by: Solar eclipse of May 9, 1929
= Triad =
- Preceded by: Solar eclipse of July 27, 1813
- Followed by: Solar eclipse of March 29, 1987
= Solar eclipses of 1898–1902 =
{{Solar eclipse set 1898–1902}}
= Saros 126 =
{{Solar Saros series 126}}
= Metonic series =
{{Solar Metonic series 1866–1953}}
= Tritos series =
{{Solar Tritos series 2009 July 22}}
= Inex series =
{{Solar Inex series 2016 March 9}}
Notes
{{reflist}}
References
- {{commonscatinline}}
- [http://eclipse.gsfc.nasa.gov/5MCSEmap/1801-1900/1900-05-28.gif NASA graphic]
- [http://eclipse.gsfc.nasa.gov/SEsearch/SEsearchmap.php?Ecl=19000528 Googlemap]
- [http://eclipse.gsfc.nasa.gov/SEsearch/SEdata.php?Ecl=19000528 NASA Besselian elements]
- [http://xjubier.free.fr/en/site_pages/solar_eclipses/Solar_Corona_Shape_pg02.html Photos and sketches of the Solar Corona May 28, 1900]
- [https://web.archive.org/web/20100206221846/http://www.exploratorium.edu/eclipse/1900.html 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
- [https://books.google.com/books?id=FI0-AAAAYAAJ 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.
- [http://www.eclipse-2008.ru/eclipse/1900.php Russia expedition for solar eclipse of May 28, 1900] {{Webarchive|url=https://web.archive.org/web/20090808024916/http://www.eclipse-2008.ru/eclipse/1900.php |date=August 8, 2009 }}
- {{cite web|title=Print from Glass Plate Negative of eclipse, Wilkes County, Georgia, 1900 May 28|url=http://dlg.galileo.usg.edu/vanga/id:wlk048|website=Vanishing Georgia, Georgia Archives|publisher=Digital Library of Georgia|access-date=5 April 2018}}
{{Solar eclipses}}