Solar eclipse of May 26, 1854
Template:Short description Script error: No such module "Solar eclipse". An annular solar eclipse occurred at the Moon's ascending node of orbit on Friday, May 26, 1854, with a magnitude of 0.9551. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 3.2 days before apogee (on May 30, 1854, at 2:25 UTC), the Moon's apparent diameter was smaller.[1]
The path of annularity was visible from parts of the modern-day Marshall Islands, southern Canada, Washington, northern Idaho, northern Montana, northern North Dakota, Minnesota, the upper peninsula of Michigan, New York, Vermont, New Hampshire, Massachusetts, and Maine. A partial solar eclipse was also visible for parts of Northeast Asia, northern Oceania, Hawaii, North America, Central America, the Caribbean, far northern South America, and northern Scandinavia.
Visibility
The annular path crossed close to the boundary between the United States and Canada.
Observations
| File:Solar eclipse 1854May28-Annular Daguerrotyped Alexander.png Annularity Daguerrotyped by Stephen Alexander from Ogdensburgh, New York |
| File:Eclipse of the Sun MET DP205277.jpg Partiality by Langenheim Brothers. |
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.[2]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 1854 May 26 at 17:45:31.9 UTC |
| First Umbral External Contact | 1854 May 26 at 18:52:54.1 UTC |
| First Central Line | 1854 May 26 at 18:55:03.1 UTC |
| First Umbral Internal Contact | 1854 May 26 at 18:57:12.6 UTC |
| First Penumbral Internal Contact | 1854 May 26 at 20:20:41.5 UTC |
| Greatest Eclipse | 1854 May 26 at 20:42:52.6 UTC |
| Ecliptic Conjunction | 1854 May 26 at 20:47:29.4 UTC |
| Equatorial Conjunction | 1854 May 26 at 20:56:05.1 UTC |
| Greatest Duration | 1854 May 26 at 20:59:47.7 UTC |
| Last Penumbral Internal Contact | 1854 May 26 at 21:04:43.2 UTC |
| Last Umbral Internal Contact | 1854 May 26 at 22:28:22.6 UTC |
| Last Central Line | 1854 May 26 at 22:30:34.0 UTC |
| Last Umbral External Contact | 1854 May 26 at 22:32:45.0 UTC |
| Last Penumbral External Contact | 1854 May 26 at 23:40:11.8 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 0.95510 |
| Eclipse Obscuration | 0.91221 |
| Gamma | 0.39177 |
| Sun Right Ascension | 04h13m05.4s |
| Sun Declination | +21°11'11.2" |
| Sun Semi-Diameter | 15'46.7" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 04h12m40.1s |
| Moon Declination | +21°31'39.9" |
| Moon Semi-Diameter | 14'51.7" |
| Moon Equatorial Horizontal Parallax | 0°54'32.6" |
| ΔT | 7.1 s |
Eclipse season
Script error: No such module "Labelled list hatnote". 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.
| May 12 Descending node (full moon) |
May 26 Ascending node (new moon) |
|---|---|
| File:SE1854May26A.png | |
| Partial lunar eclipse Lunar Saros 109 |
Annular solar eclipse Solar Saros 135 |
Related eclipses
Eclipses in 1854
- A partial lunar eclipse on May 12.
- An annular solar eclipse on May 26.
- A total lunar eclipse on November 4.
- A hybrid solar eclipse on November 20.
Metonic
- Preceded by: Solar eclipse of January 21, 1852
- Followed by: Solar eclipse of August 28, 1859
Tzolkinex
- Preceded by: Solar eclipse of April 15, 1847
- Followed by: Solar eclipse of July 8, 1861
Half-Saros
- Preceded by: Lunar eclipse of May 21, 1845
- Followed by: Lunar eclipse of June 1, 1863
Tritos
- Preceded by: Solar eclipse of June 27, 1843
- Followed by: Solar eclipse of April 25, 1865
Solar Saros 135
- Preceded by: Solar eclipse of May 15, 1836
- Followed by: Solar eclipse of June 6, 1872
Inex
- Preceded by: Solar eclipse of June 16, 1825
- Followed by: Solar eclipse of May 6, 1883
Triad
- Preceded by: Solar eclipse of July 25, 1767
- Followed by: Solar eclipse of March 27, 1941
Solar eclipses of 1852–1855
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.[3]
The partial solar eclipse on January 21, 1852 occurs in the previous lunar year eclipse set.
| Solar eclipse series sets from 1852 to 1855 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 115 | June 17, 1852 File:SE1852Jun17P.gif Partial |
−1.1111 | 120 | December 11, 1852 File:SE1852Dec11T.gif Total |
0.8551 | |
| 125 | June 6, 1853 File:SE1853Jun06A.gif Annular |
−0.3686 | 130 | November 30, 1853 File:SE1853Nov30T.png Total |
0.1763 | |
| 135 | May 26, 1854 File:SE1854May26A.png Annular |
0.3918 | 140 | November 20, 1854 File:SE1854Nov20H.png Hybrid |
−0.5179 | |
| 145 | May 16, 1855 File:SE1855May16P.gif Partial |
1.1249 | 150 | November 9, 1855 File:SE1855Nov09P.gif Partial |
−1.2767 | |
Saros 135
Template:Solar Saros series 135
Metonic series
The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's ascending node.
| 25 eclipse events between March 14, 1801 and August 7, 1888 | ||||
|---|---|---|---|---|
| March 14–15 | December 31–January 1 | October 19–20 | August 7 | May 26–27 |
| 107 | 109 | 111 | 113 | 115 |
| File:SE1801Mar14P.png March 14, 1801 |
File:SE1805Jan01P.gif January 1, 1805 |
File:SE1808Oct19P.gif October 19, 1808 |
File:SE1812Aug07P.gif August 7, 1812 |
File:SE1816May27A.gif May 27, 1816 |
| 117 | 119 | 121 | 123 | 125 |
| File:SE1820Mar14T.gif March 14, 1820 |
File:SE1824Jan01A.gif January 1, 1824 |
File:SE1827Oct20H.gif October 20, 1827 |
File:SE1831Aug07T.gif August 7, 1831 |
File:SE1835May27A.gif May 27, 1835 |
| 127 | 129 | 131 | 133 | 135 |
| File:SE1839Mar15T.gif March 15, 1839 |
File:SE1842Dec31A.gif December 31, 1842 |
File:SE1846Oct20A.gif October 20, 1846 |
File:SE1850Aug07T.gif August 7, 1850 |
File:SE1854May26A.png May 26, 1854 |
| 137 | 139 | 141 | 143 | 145 |
| File:SE1858Mar15A.gif March 15, 1858 |
File:SE1861Dec31T.gif December 31, 1861 |
File:SE1865Oct19A.png October 19, 1865 |
File:SE1869Aug07T.png August 7, 1869 |
File:SE1873May26P.gif May 26, 1873 |
| 147 | 149 | 151 | 153 | |
| File:SE1877Mar15P.gif March 15, 1877 |
File:SE1880Dec31P.gif December 31, 1880 |
File:SE1884Oct19P.gif October 19, 1884 |
File:SE1888Aug07P.gif August 7, 1888 | |
Tritos series
Template:Solar Tritos series 2007 March 19
Inex series
Template:Solar Inex series 2028 January 26
Notes
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References
- Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- Total Eclipses of the Sun, By Mabel Loomis Todd, 1894, new and revised edition by David P. Todd, 1900. [1]
- Suggestions relative to the observation of the solar eclipse of May 26, 1854, Astronomical Journal, vol. 3, iss. 70, p. 169–172 (1854). Alexander, S.
- On the solar eclipse of 1854, May 26, Bartlett, W. H. C. Astronomical Journal, vol. 4, iss. 77, p. 33–35 (1854).
- Observation of the annular eclipse of May 26, in the suburbs of Ogdensburgh, N. Y. Astronomical Journal, vol. 3, iss. 70, p. 169–172 (1854). Alexander, S.
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