Solar eclipse of March 25, 1857
{{Short description|Total eclipse}}
{{Infobox solar eclipse|1857Mar25
| previous = Solar eclipse of September 29, 1856
| next = Solar eclipse of September 18, 1857
}}
A total solar eclipse occurred at the Moon's ascending node of orbit between Wednesday, March 25 and Thursday, March 26, 1857, with a magnitude of 1.0534. 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 1.1 days before perigee (on March 26, 1857, at 23:55 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=1857&n=136|publisher=timeanddate|access-date=11 September 2024}}
The path of totality was visible from parts of modern-day southeastern Australia, Niue, the Cook Islands, Kiribati, Mexico. A partial solar eclipse was also visible for parts of Australia, Oceania, Hawaii, western North America, and Central America.
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 1857 Mar 25|url=https://eclipsewise.com/solar/SEprime/1801-1900/SE1857Mar25Tprime.html|publisher=EclipseWise.com|access-date=11 September 2024}}
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|+March 25, 1857 Solar Eclipse Times ! Event ! Time (UTC) |
First Penumbral External Contact
| 1857 March 25 at 19:50:30.7 UTC |
First Umbral External Contact
| 1857 March 25 at 20:45:26.6 UTC |
First Central Line
| 1857 March 25 at 20:46:23.7 UTC |
First Umbral Internal Contact
| 1857 March 25 at 20:47:20.8 UTC |
First Penumbral Internal Contact
| 1857 March 25 at 21:42:38.0 UTC |
Equatorial Conjunction
| 1857 March 25 at 22:24:29.2 UTC |
Ecliptic Conjunction
| 1857 March 25 at 22:28:42.5 UTC |
Greatest Eclipse
| 1857 March 25 at 22:29:37.6 UTC |
Greatest Duration
| 1857 March 25 at 22:31:46.5 UTC |
Last Penumbral Internal Contact
| 1857 March 25 at 23:16:44.6 UTC |
Last Umbral Internal Contact
| 1857 March 26 at 00:11:55.9 UTC |
Last Central Line
| 1857 March 26 at 00:12:54.3 UTC |
Last Umbral External Contact
| 1857 March 26 at 00:13:52.8 UTC |
Last Penumbral External Contact
| 1857 March 26 at 01:08:43.7 UTC |
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|+March 25, 1857 Solar Eclipse Parameters ! Parameter ! Value |
Eclipse Magnitude
| 1.05342 |
Eclipse Obscuration
| 1.10969 |
Gamma
| −0.08923 |
Sun Right Ascension
| 00h19m12.6s |
Sun Declination
| +02°04'51.1" |
Sun Semi-Diameter
| 16'01.4" |
Sun Equatorial Horizontal Parallax
| 08.8" |
Moon Right Ascension
| 00h19m23.1s |
Moon Declination
| +02°00'06.7" |
Moon Semi-Diameter
| 16'35.7" |
Moon Equatorial Horizontal Parallax
| 1°00'54.1" |
ΔT
| 7.0 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 March–April 1857 ! March 25 | |
200px | |
align=center
| Total solar eclipse | Penumbral lunar eclipse Lunar Saros 139 |
Related eclipses
= Eclipses in 1857 =
- An total solar eclipse on March 25.
- A penumbral lunar eclipse on April 9.
- A penumbral lunar eclipse on September 4.
- An annular solar eclipse on September 18.
- A penumbral lunar eclipse on October 3.
= Metonic =
- Preceded by: Solar eclipse of November 20, 1854
- Followed by: Solar eclipse of June 27, 1862
= Tzolkinex =
- Preceded by: Solar eclipse of February 12, 1850
- Followed by: Solar eclipse of May 6, 1864
= Half-Saros =
- Preceded by: Lunar eclipse of March 19, 1848
- Followed by: Lunar eclipse of March 31, 1866
= Tritos =
- Preceded by: Solar eclipse of April 25, 1846
- Followed by: Solar eclipse of February 23, 1868
= Solar Saros 127 =
- Preceded by: Solar eclipse of March 15, 1839
- Followed by: Solar eclipse of April 6, 1875
= Inex =
- Preceded by: Solar eclipse of April 14, 1828
- Followed by: Solar eclipse of March 5, 1886
= Triad =
- Preceded by: Solar eclipse of May 25, 1770
- Followed by: Solar eclipse of January 25, 1944
= Solar eclipses of 1856–1859 =
{{Lunar year eclipse set info}}
The partial solar eclipses on February 3, 1859 and July 29, 1859 occur in the next lunar year eclipse set.
class="wikitable mw-collapsible mw-collapsed"
!class="nowrap" colspan="7" | Solar eclipse series sets from 1856 to 1859 |
scope="col" colspan="3" | Ascending node
| rowspan="6" | ! scope="col" colspan="3" | Descending 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;"
| 117 | April 5, 1856 | −0.7906 | 122 | September 29, 1856 | 0.9420 |
style="text-align: center;"
| 127 | March 25, 1857 | −0.0892 | 132 | September 18, 1857 | 0.1912 |
style="text-align: center;"
| 137 | March 15, 1858 | 0.6461 | 142 | September 7, 1858 | −0.5609 |
style="text-align: center;"
| 147 | March 4, 1859 | 1.4192 | 152 | August 28, 1859 | −1.2569 |
= Saros 127 =
{{Solar Saros series 127}}
= Metonic series =
{{Metonic eclipse set info}} All eclipses in this table occur at the Moon's ascending node.
class="wikitable mw-collapsible mw-collapsed"
!colspan=5|24 eclipse events between March 25, 1819 and August 20, 1906 |
March 25–26
!January 11–12 !October 30–31 !August 18–20 !June 6–7 |
---|
107
!109 !111 !113 !115 |
style="text-align:center;"
|150px |150px |150px |150px |150px |
117
!119 !121 !123 !125 |
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|150px |150px |150px |150px |
127
!129 !131 !133 !135 |
style="text-align:center;"
|150px |150px |150px |150px |
137
!139 !141 !143 !145 |
style="text-align:center;"
|150px |150px |150px |150px |
147
!149 !151 !153 |
style="text-align:center;"
|150px |150px |
= Tritos series =
{{Solar Tritos series 2010 January 15}}
= Inex series =
{{Solar Inex series 2001 December 14}}
Notes
{{reflist}}
References
- [http://eclipse.gsfc.nasa.gov/5MCSEmap/1801-1900/1857-03-25.gif NASA graphic]
- [http://eclipse.gsfc.nasa.gov/SEsearch/SEsearchmap.php?Ecl=18570325 Googlemap]
- [http://eclipse.gsfc.nasa.gov/SEsearch/SEdata.php?Ecl=18570325 NASA Besselian elements]
- {{cite book|author=Charles Augustus Young|title=The Sun|url=https://archive.org/details/sun00youngoog|year=1895|publisher=D. Appleton|page=[https://archive.org/details/sun00youngoog/page/n27 3]}}
- [http://adsabs.harvard.edu/full/1857MNRAS..18...39C Observations made at Sydney during the Eclipse of the Sun, March 26, 1857] Clarke, W. B., Monthly Notices of the Royal Astronomical Society, Vol. 18, p. 39–44 [http://www.austehc.unimelb.edu.au/fam/1533.html]
{{Solar eclipses}}
{{Commons category}}