Solar eclipse of August 9, 1896
{{Short description|Total eclipse}}
{{Infobox solar eclipse|1896Aug09
| previous = Solar eclipse of February 13, 1896
| next = Solar eclipse of February 1, 1897
}}
A total solar eclipse occurred at the Moon's descending node of orbit on Sunday, August 9, 1896, with a magnitude of 1.0392. 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 2.5 days before perigee (on August 11, 1896, at 18:30 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=1896&n=136|publisher=timeanddate|access-date=27 August 2024}}
The path of totality was visible from parts of northern Norway, northern Sweden, the Russian Empire, and the Empire of Japan. A partial solar eclipse was also visible for much of Europe, Central Asia, East Asia, Northeast Asia, Alaska, and Greenland.
This event was the subject of the first organized eclipse expedition by the British Astronomical Association. A group of 165 amateur and professional astronomers sailed from Tilbury, England on July 25, heading toward Vadsø, Norway.{{Cite journal |last=Marriott |first=R. A. |date=June 1991 |title=Norway 1896: the BAA's first organised eclipse expedition |journal=Journal of the British Astronomical Association |volume=101 |issue=3 |pages=162–170 |bibcode=1991JBAA..101..162M}} This expedition failed to produce any usable results as they were frustrated by the weather conditions at the time of the eclipse.{{Cite journal |date=1898 |title=Expedition for the Observation of the Total Solar Eclipse, August 9th, 1896 |journal=Memoirs of the British Astronomical Association |volume=6 |pages=1–4 |bibcode=1898MmBAA...6....1.}} However, a smaller expedition to Novaya Zemlya on Sir George Baden-Powell's yacht Otario met with success.
Gallery
Solar eclipse 1896Aug09-Corona.png
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 1896 Aug 09|url=https://eclipsewise.com/solar/SEprime/1801-1900/SE1896Aug09Tprime.html|publisher=EclipseWise.com|access-date=27 August 2024}}
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|+August 9, 1896 Solar Eclipse Times ! Event ! Time (UTC) |
First Penumbral External Contact
| 1896 August 09 at 02:43:20.8 UTC |
First Umbral External Contact
| 1896 August 09 at 03:52:06.8 UTC |
First Central Line
| 1896 August 09 at 03:53:08.3 UTC |
First Umbral Internal Contact
| 1896 August 09 at 03:54:10.1 UTC |
Equatorial Conjunction
| 1896 August 09 at 04:37:13.0 UTC |
Ecliptic Conjunction
| 1896 August 09 at 05:01:41.9 UTC |
Greatest Duration
| 1896 August 09 at 05:08:37.2 UTC |
Greatest Eclipse
| 1896 August 09 at 05:09:00.1 UTC |
Last Umbral Internal Contact
| 1896 August 09 at 06:24:07.8 UTC |
Last Central Line
| 1896 August 09 at 06:25:11.8 UTC |
Last Umbral External Contact
| 1896 August 09 at 06:26:15.3 UTC |
Last Penumbral External Contact
| 1896 August 09 at 07:34:47.9 UTC |
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|+August 9, 1896 Solar Eclipse Parameters ! Parameter ! Value |
Eclipse Magnitude
| 1.03918 |
Eclipse Obscuration
| 1.07989 |
Gamma
| 0.69635 |
Sun Right Ascension
| 09h18m02.6s |
Sun Declination
| +15°44'00.4" |
Sun Semi-Diameter
| 15'46.9" |
Sun Equatorial Horizontal Parallax
| 08.7" |
Moon Right Ascension
| 09h19m10.6s |
Moon Declination
| +16°21'57.5" |
Moon Semi-Diameter
| 16'12.5" |
Moon Equatorial Horizontal Parallax
| 0°59'29.1" |
ΔT
| -5.8 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 August 1896 ! August 9 | August 23 Ascending node (full moon) |
200px | |
align=center
| Total solar eclipse | Partial lunar eclipse Lunar Saros 136 |
Related eclipses
= Eclipses in 1896 =
- An annular solar eclipse on February 13.
- A partial lunar eclipse on February 28.
- A total solar eclipse on August 9.
- A partial lunar eclipse on August 23.
= Metonic =
- Preceded by: Solar eclipse of October 20, 1892
- Followed by: Solar eclipse of May 28, 1900
= Tzolkinex =
- Preceded by: Solar eclipse of June 28, 1889
- Followed by: Solar eclipse of September 21, 1903
= Half-Saros =
- Preceded by: Lunar eclipse of August 3, 1887
- Followed by: Lunar eclipse of August 15, 1905
= Tritos =
- Preceded by: Solar eclipse of September 8, 1885
- Followed by: Solar eclipse of July 10, 1907
= Solar Saros 124 =
- Preceded by: Solar eclipse of July 29, 1878
- Followed by: Solar eclipse of August 21, 1914
= Inex =
- Preceded by: Solar eclipse of August 29, 1867
- Followed by: Solar eclipse of July 20, 1925
= Triad =
- Preceded by: Solar eclipse of October 9, 1809
- Followed by: Solar eclipse of June 11, 1983
= Solar eclipses of 1895–1899 =
{{Lunar year eclipse set info}}
The partial solar eclipses on March 26, 1895 and September 18, 1895 occur in the previous lunar year eclipse set, and the partial solar eclipse on December 13, 1898 occurs in the next lunar year eclipse set.
class="wikitable mw-collapsible mw-collapsed"
!class="nowrap" colspan="7" | Solar eclipse series sets from 1895 to 1899 |
scope="col" colspan="3" | Descending node
| rowspan="6" | ! scope="col" colspan="3" | Ascending node |
---|
style="text-align: center;"
! scope="col" | Saros ! scope="col" | Map ! scope="col" | Gamma ! scope="col" | Saros ! scope="col" | Map ! scope="col" | Gamma |
style="text-align: center;"
| 114 | August 20, 1895 | 1.3911 | 119 | February 13, 1896 | −0.9220 |
style="text-align: center;"
| 124 | August 9, 1896 | 0.6964 | 129 | February 1, 1897 | −0.1903 |
style="text-align: center;"
| 134 | July 29, 1897 | −0.0640 | 139 | January 22, 1898 | 0.5079 |
style="text-align: center;"
| 144 | July 18, 1898 | −0.8546 | 149 | January 11, 1899 | 1.1558 |
= Saros 124 =
{{Solar Saros series 124}}
= Metonic series =
{{Solar Metonic series 1866–1953}}
= Tritos series =
{{Solar Tritos series 2005 October 3}}
= Inex series =
{{Solar Inex series 2012 May 20}}
References
{{reflist}}
External links
{{Commons category|Solar eclipse of 1896 August 9}}
- [http://eclipse.gsfc.nasa.gov/5MCSEmap/1801-1900/1896-08-09.gif NASA graphics]
- [http://eclipse.gsfc.nasa.gov/SEsearch/SEsearchmap.php?Ecl=18960809 Googlemap]
- [http://eclipse.gsfc.nasa.gov/SEsearch/SEdata.php?Ecl=18960809 NASA Besselian elements]
- [https://web.archive.org/web/20090726174629/http://www.exploratorium.edu/eclipse/1896.html Corona and Coronet: Being a narrative of the Amherst Eclipse Expedition to Japan, in Mr. James's Schooner-Yacht Coronet, to Observe the Sun's Total Obscuration, 9th August, 1896], by Mabel Loomis Todd, Houghton, Mifflin and Company, publishers, 1898
- {{Cite book |last=Mabel Loomis Todd |url=https://books.google.com/books?id=FI0-AAAAYAAJ |title=Total Eclipses of the Sun |publisher=Little, Brown |year=1900}}
- [http://www.eclipse-2008.ru/eclipse/1896.php Solar eclipse of August 9, 1896 in Russia] {{Webarchive|url=https://web.archive.org/web/20090809113450/http://eclipse-2008.ru/eclipse/1896.php |date=August 9, 2009 }}
{{Solar eclipses}}