French
DeutschSolar eclipse of July 18, 1860
| Solar eclipse of July 18, 1860 | |
|---|---|
 Map | |
| Type of eclipse | |
| Nature | Total |
| Gamma | 0.5487 |
| Magnitude | 1.05 |
| Maximum eclipse | |
| Duration | 219 s (3 min 39 s) |
| Coordinates | 52°30′N 20°18′W / 52.5°N 20.3°W |
| Max. width of band | 198 km (123 mi) |
| Times (UTC) | |
| Greatest eclipse | 14:26:24 |
| References | |
| Saros | 124 (46 of 73) |
| Catalog # (SE5000) | 9188 |
A total solar eclipse occurred at the Moon's descending node of orbit on Wednesday, July 18, 1860, with a magnitude of 1.0500. 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 2.2 days before perigee (on July 20, 1860, at 19:15 UTC), the Moon's apparent diameter was larger.[1]
The path of totality was visible from parts of modern-day northwestern Oregon, Washington, northern Idaho, northwestern Montana, Canada, Spain, Algeria, Tunisia, Libya, Egypt, Sudan, and Eritrea. A partial solar eclipse was also visible for parts of North America, Europe, West Asia, North Africa, and West Africa.
Coronal Mass Ejection
[edit]The first coronal mass ejection may have been observed as coronal loops progressing during this total eclipse.[2]
_et_..._(illisible)_coll._humide_-_Fonds_Trutat_-_MHNT.PHa.814.105.jpg)
Eclipse details
[edit]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.[3]
| Event | Time (UTC) |
|---|---|
| First Penumbral External Contact | 1860 July 18 at 11:54:56.3 UTC |
| First Umbral External Contact | 1860 July 18 at 12:57:13.1 UTC |
| First Central Line | 1860 July 18 at 12:58:21.9 UTC |
| First Umbral Internal Contact | 1860 July 18 at 12:59:31.0 UTC |
| Equatorial Conjunction | 1860 July 18 at 14:09:18.4 UTC |
| Ecliptic Conjunction | 1860 July 18 at 14:20:40.8 UTC |
| Greatest Duration | 1860 July 18 at 14:24:54.3 UTC |
| Greatest Eclipse | 1860 July 18 at 14:26:24.2 UTC |
| Last Umbral Internal Contact | 1860 July 18 at 15:53:26.2 UTC |
| Last Central Line | 1860 July 18 at 15:54:37.2 UTC |
| Last Umbral External Contact | 1860 July 18 at 15:55:48.0 UTC |
| Last Penumbral External Contact | 1860 July 18 at 16:57:54.9 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 1.05000 |
| Eclipse Obscuration | 1.10249 |
| Gamma | 0.54871 |
| Sun Right Ascension | 07h52m23.3s |
| Sun Declination | +20°56'51.5" |
| Sun Semi-Diameter | 15'44.4" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 07h53m03.2s |
| Moon Declination | +21°28'15.4" |
| Moon Semi-Diameter | 16'18.0" |
| Moon Equatorial Horizontal Parallax | 0°59'49.1" |
| ΔT | 7.7 s |
Eclipse season
[edit]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.
| July 18 Descending node (new moon) | August 1 Ascending node (full moon) |
|---|---|
| |
| Total solar eclipse Solar Saros 124 | Partial lunar eclipse Lunar Saros 136 |
Related eclipses
[edit]Eclipses in 1860
[edit]- An annular solar eclipse on January 23.
- A partial lunar eclipse on February 7.
- A total solar eclipse on July 18.
- A partial lunar eclipse on August 1.
- A penumbral lunar eclipse on December 28.
Metonic
[edit]- Preceded by: Solar eclipse of September 29, 1856
- Followed by: Solar eclipse of May 6, 1864
Tzolkinex
[edit]- Preceded by: Solar eclipse of June 6, 1853
- Followed by: Solar eclipse of August 29, 1867
Half-Saros
[edit]- Preceded by: Lunar eclipse of July 13, 1851
- Followed by: Lunar eclipse of July 23, 1869
Tritos
[edit]- Preceded by: Solar eclipse of August 18, 1849
- Followed by: Solar eclipse of June 18, 1871
Solar Saros 124
[edit]- Preceded by: Solar eclipse of July 8, 1842
- Followed by: Solar eclipse of July 29, 1878
Inex
[edit]- Preceded by: Solar eclipse of August 7, 1831
- Followed by: Solar eclipse of June 28, 1889
Triad
[edit]- Preceded by: Solar eclipse of September 16, 1773
- Followed by: Solar eclipse of May 20, 1947
Solar eclipses of 1859–1862
[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.[4]
The partial solar eclipses on March 4, 1859 and August 28, 1859 occur in the previous lunar year eclipse set, and the partial solar eclipse on November 21, 1862 occurs in the next lunar year eclipse set.
| Solar eclipse series sets from 1859 to 1862 | ||||||
|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||
| Saros | Map | Gamma | Saros | Map | Gamma | |
| 109 | February 3, 1859 Partial | −1.5659 | 114 | July 29, 1859 Partial | 1.2598 | |
| 119 | January 23, 1860 Annular | −0.8969 | 124 | July 18, 1860 Total | 0.5487 | |
| 129 | January 11, 1861 Annular | −0.1766 | 134 | July 8, 1861 Annular | −0.2231 | |
| 139 | December 31, 1861 Total | 0.5187 | 144 | June 27, 1862 Partial | −1.0252 | |
| 149 | December 21, 1862 Partial | 1.1633 | ||||
Saros 124
[edit]This eclipse is a part of Saros series 124, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on March 6, 1049. It contains total eclipses from June 12, 1211 through September 22, 1968, and a hybrid eclipse on October 3, 1986. There are no annular eclipses in this set. The series ends at member 73 as a partial eclipse on May 11, 2347. 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 totality was produced by member 39 at 5 minutes, 46 seconds on May 3, 1734. All eclipses in this series occur at the Moon’s descending node of orbit.[5]
| Series members 43–64 occur between 1801 and 2200: | ||
|---|---|---|
| 43 | 44 | 45 |
 June 16, 1806 |  June 26, 1824 |  July 8, 1842 |
| 46 | 47 | 48 |
July 18, 1860 |  July 29, 1878 |  August 9, 1896 |
| 49 | 50 | 51 |
 August 21, 1914 |  August 31, 1932 |  September 12, 1950 |
| 52 | 53 | 54 |
 September 22, 1968 |  October 3, 1986 |  October 14, 2004 |
| 55 | 56 | 57 |
 October 25, 2022 |  November 4, 2040 |  November 16, 2058 |
| 58 | 59 | 60 |
 November 26, 2076 |  December 7, 2094 |  December 19, 2112 |
| 61 | 62 | 63 |
 December 30, 2130 |  January 9, 2149 |  January 21, 2167 |
| 64 | ||
 January 31, 2185 | ||
Metonic series
[edit]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 descending node.
| 22 eclipse events between February 23, 1830 and July 19, 1917 | ||||
|---|---|---|---|---|
| February 22–23 | December 11–12 | September 29–30 | July 18–19 | May 6–7 |
| 108 | 110 | 112 | 114 | 116 |
 February 23, 1830 |  July 18, 1841 |  May 6, 1845 | ||
| 118 | 120 | 122 | 124 | 126 |
 February 23, 1849 |  December 11, 1852 |  September 29, 1856 |  July 18, 1860 |  May 6, 1864 |
| 128 | 130 | 132 | 134 | 136 |
 February 23, 1868 |  December 12, 1871 |  September 29, 1875 |  July 19, 1879 |  May 6, 1883 |
| 138 | 140 | 142 | 144 | 146 |
 February 22, 1887 |  December 12, 1890 |  September 29, 1894 |  July 18, 1898 |  May 7, 1902 |
| 148 | 150 | 152 | 154 | |
 February 23, 1906 |  December 12, 1909 |  September 30, 1913 |  July 19, 1917 | |
Tritos series
[edit]This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | ||||
|---|---|---|---|---|
 December 21, 1805 (Saros 119) |  November 19, 1816 (Saros 120) |  October 20, 1827 (Saros 121) |  September 18, 1838 (Saros 122) |  August 18, 1849 (Saros 123) |
July 18, 1860 (Saros 124) |  June 18, 1871 (Saros 125) |  May 17, 1882 (Saros 126) |  April 16, 1893 (Saros 127) |  March 17, 1904 (Saros 128) |
 February 14, 1915 (Saros 129) |  January 14, 1926 (Saros 130) |  December 13, 1936 (Saros 131) |  November 12, 1947 (Saros 132) |  October 12, 1958 (Saros 133) |
 September 11, 1969 (Saros 134) |  August 10, 1980 (Saros 135) |  July 11, 1991 (Saros 136) |  June 10, 2002 (Saros 137) |  May 10, 2013 (Saros 138) |
 April 8, 2024 (Saros 139) |  March 9, 2035 (Saros 140) |  February 5, 2046 (Saros 141) |  January 5, 2057 (Saros 142) |  December 6, 2067 (Saros 143) |
 November 4, 2078 (Saros 144) |  October 4, 2089 (Saros 145) |  September 4, 2100 (Saros 146) |  August 4, 2111 (Saros 147) |  July 4, 2122 (Saros 148) |
 June 3, 2133 (Saros 149) |  May 3, 2144 (Saros 150) |  April 2, 2155 (Saros 151) |  March 2, 2166 (Saros 152) |  January 29, 2177 (Saros 153) |
 December 29, 2187 (Saros 154) |  November 28, 2198 (Saros 155) | |||
Inex series
[edit]This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee). However, groupings of 3 inex cycles (≈ 87 years minus 2 months) comes close (≈ 1,151.02 anomalistic months), so eclipses are similar in these groupings.
| Series members between 1801 and 2200 | ||
|---|---|---|
 August 28, 1802 (Saros 122) |  August 7, 1831 (Saros 123) | July 18, 1860 (Saros 124) |
 June 28, 1889 (Saros 125) |  June 8, 1918 (Saros 126) |  May 20, 1947 (Saros 127) |
 April 29, 1976 (Saros 128) |  April 8, 2005 (Saros 129) |  March 20, 2034 (Saros 130) |
 February 28, 2063 (Saros 131) |  February 7, 2092 (Saros 132) |  January 19, 2121 (Saros 133) |
 December 30, 2149 (Saros 134) |  December 9, 2178 (Saros 135) | |
See also
[edit]References
[edit]- ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 5 September 2024.
- ^ Coronal Mass Ejections from the Sun - Propagation and Near Earth Effects
- ^ "Total Solar Eclipse of 1860 Jul 18". EclipseWise.com. Retrieved 5 September 2024.
- ^ 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 124". eclipse.gsfc.nasa.gov.
- NASA chart graphics
- Googlemap
- NASA Besselian elements
- Sketch of Solar Corona 1860 July 18
- Russia expedition for solar eclipse of July 18, 1860
- Mabel Loomis Todd (1900). Total Eclipses of the Sun. Little, Brown.
.jpg)
