| Total eclipse | |
 Map | |
| Gamma | 0.1763 |
|---|---|
| Magnitude | 1.0485 |
| Maximum eclipse | |
| Duration | 268 s (4 min 28 s) |
| Coordinates | 12°S109°W / 12°S 109°W /-12; -109 |
| Max. width of band | 164 km (102 mi) |
| Times (UTC) | |
| Greatest eclipse | 19:15:39 |
| References | |
| Saros | 130 (43 of 73) |
| Catalog # (SE5000) | 9172 |
← June 6, 1853 | |
A totalsolar eclipse occurred at the Moon'sdescending node of orbit on Wednesday, November 30, 1853, with amagnitude of 1.0485. Asolar eclipse occurs when theMoon passes betweenEarth and theSun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon'sapparent 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 8.5 hours beforeperigee (on December 1, 1853, at 3:45 UTC), the Moon's apparent diameter was larger.[1]
The path of totality was visible from parts of modern-dayPeru,Bolivia, andBrazil. A partial solar eclipse was also visible for parts of northernOceania,Hawaii, southernNorth America,Central America, theCaribbean, andSouth America.
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 | 1853 November 30 at 16:38:15.3 UTC |
| First Umbral External Contact | 1853 November 30 at 17:33:27.1 UTC |
| First Central Line | 1853 November 30 at 17:34:17.3 UTC |
| First Umbral Internal Contact | 1853 November 30 at 17:35:07.5 UTC |
| First Penumbral Internal Contact | 1853 November 30 at 18:31:47.1 UTC |
| Equatorial Conjunction | 1853 November 30 at 19:10:53.1 UTC |
| Ecliptic Conjunction | 1853 November 30 at 19:13:50.5 UTC |
| Greatest Eclipse | 1853 November 30 at 19:15:38.7 UTC |
| Greatest Duration | 1853 November 30 at 19:20:35.5 UTC |
| Last Penumbral Internal Contact | 1853 November 30 at 19:59:37.3 UTC |
| Last Umbral Internal Contact | 1853 November 30 at 20:56:12.6 UTC |
| Last Central Line | 1853 November 30 at 20:57:03.2 UTC |
| Last Umbral External Contact | 1853 November 30 at 20:57:53.8 UTC |
| Last Penumbral External Contact | 1853 November 30 at 21:53:03.3 UTC |
| Parameter | Value |
|---|---|
| Eclipse Magnitude | 1.04851 |
| Eclipse Obscuration | 1.09938 |
| Gamma | 0.17631 |
| Sun Right Ascension | 16h27m18.6s |
| Sun Declination | -21°44'59.0" |
| Sun Semi-Diameter | 16'13.6" |
| Sun Equatorial Horizontal Parallax | 08.9" |
| Moon Right Ascension | 16h27m30.3s |
| Moon Declination | -21°34'32.2" |
| Moon Semi-Diameter | 16'43.7" |
| Moon Equatorial Horizontal Parallax | 1°01'23.6" |
| ΔT | 7.1 s |
This eclipse is part of aneclipse 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 afortnight.
| November 30 Descending node (new moon) | December 15 Ascending node (full moon) |
|---|---|
| |
| Total solar eclipse Solar Saros 130 | Penumbral lunar eclipse Lunar Saros 142 |
This eclipse is a member of asemester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternatingnodes of the Moon's orbit.[3]
The partial solar eclipse onJanuary 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 Partial | −1.1111 | 120 | December 11, 1852 Total | 0.8551 | |
| 125 | June 6, 1853 Annular | −0.3686 | 130 | November 30, 1853 Total | 0.1763 | |
| 135 | May 26, 1854 Annular | 0.3918 | 140 | November 20, 1854 Hybrid | −0.5179 | |
| 145 | May 16, 1855 Partial | 1.1249 | 150 | November 9, 1855 Partial | −1.2767 | |
This eclipse is a part ofSaros series 130, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on August 20, 1096. It contains total eclipses from April 5, 1475 through July 18, 2232. There are no annular or hybrid eclipses in this set. The series ends at member 73 as a partial eclipse on October 25, 2394. Its eclipses are tabulated in three columns; every third eclipse in the same column is oneexeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of totality was produced by member 30 at 6 minutes, 41 seconds on July 11, 1619. All eclipses in this series occur at the Moon’sdescending node of orbit.[4]
| Series members 41–62 occur between 1801 and 2200: | ||
|---|---|---|
| 41 | 42 | 43 |
 November 9, 1817 |  November 20, 1835 |  November 30, 1853 |
| 44 | 45 | 46 |
 December 12, 1871 |  December 22, 1889 |  January 3, 1908 |
| 47 | 48 | 49 |
 January 14, 1926 |  January 25, 1944 |  February 5, 1962 |
| 50 | 51 | 52 |
 February 16, 1980 |  February 26, 1998 |  March 9, 2016 |
| 53 | 54 | 55 |
 March 20, 2034 |  March 30, 2052 |  April 11, 2070 |
| 56 | 57 | 58 |
 April 21, 2088 |  May 3, 2106 |  May 14, 2124 |
| 59 | 60 | 61 |
 May 25, 2142 |  June 4, 2160 |  June 16, 2178 |
| 62 | ||
 June 26, 2196 | ||
Themetonic 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 February 12, 1812 and September 18, 1895 | ||||
|---|---|---|---|---|
| February 11–12 | November 30–December 1 | September 17–19 | July 7–8 | April 25–26 |
| 108 | 110 | 112 | 114 | 116 |
 February 12, 1812 |  September 19, 1819 |  July 8, 1823 |  April 26, 1827 | |
| 118 | 120 | 122 | 124 | 126 |
 February 12, 1831 |  November 30, 1834 |  September 18, 1838 |  July 8, 1842 |  April 25, 1846 |
| 128 | 130 | 132 | 134 | 136 |
 February 12, 1850 | November 30, 1853 |  September 18, 1857 |  July 8, 1861 |  April 25, 1865 |
| 138 | 140 | 142 | 144 | 146 |
 February 11, 1869 |  November 30, 1872 |  September 17, 1876 |  July 7, 1880 |  April 25, 1884 |
| 148 | 150 | 152 | ||
 February 11, 1888 |  December 1, 1891 |  September 18, 1895 | ||
This eclipse is a part of atritos cycle, repeating at alternating nodes every 135synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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 | ||||
|---|---|---|---|---|
 April 4, 1810 (Saros 126) |  March 4, 1821 (Saros 127) |  February 1, 1832 (Saros 128) |  December 31, 1842 (Saros 129) | November 30, 1853 (Saros 130) |
 October 30, 1864 (Saros 131) |  September 29, 1875 (Saros 132) |  August 29, 1886 (Saros 133) |  July 29, 1897 (Saros 134) |  June 28, 1908 (Saros 135) |
 May 29, 1919 (Saros 136) |  April 28, 1930 (Saros 137) |  March 27, 1941 (Saros 138) |  February 25, 1952 (Saros 139) |  January 25, 1963 (Saros 140) |
 December 24, 1973 (Saros 141) |  November 22, 1984 (Saros 142) |  October 24, 1995 (Saros 143) |  September 22, 2006 (Saros 144) |  August 21, 2017 (Saros 145) |
 July 22, 2028 (Saros 146) |  June 21, 2039 (Saros 147) |  May 20, 2050 (Saros 148) |  April 20, 2061 (Saros 149) |  March 19, 2072 (Saros 150) |
 February 16, 2083 (Saros 151) |  January 16, 2094 (Saros 152) |  December 17, 2104 (Saros 153) |  November 16, 2115 (Saros 154) |  October 16, 2126 (Saros 155) |
 September 15, 2137 (Saros 156) |  August 14, 2148 (Saros 157) |  July 15, 2159 (Saros 158) |  June 14, 2170 (Saros 159) |  May 13, 2181 (Saros 160) |
 April 12, 2192 (Saros 161) | ||||
This eclipse is a part of the long periodinex cycle, repeating at alternating nodes, every 358synodic months (≈ 10,571.95 days, or 29 years minus 20 days). Their appearance and longitude are irregular due to a lack of synchronization with theanomalistic 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 | ||
|---|---|---|
 December 20, 1824 (Saros 129) | November 30, 1853 (Saros 130) |  November 10, 1882 (Saros 131) |
 October 22, 1911 (Saros 132) |  October 1, 1940 (Saros 133) |  September 11, 1969 (Saros 134) |
 August 22, 1998 (Saros 135) |  August 2, 2027 (Saros 136) |  July 12, 2056 (Saros 137) |
 June 22, 2085 (Saros 138) |  June 3, 2114 (Saros 139) |  May 14, 2143 (Saros 140) |
 April 23, 2172 (Saros 141) | ||
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