# Solar eclipse of April 11, 2051

A partial solar eclipse will occur at the Moon's descending node of orbit between Monday, April 10 and Tuesday, April 11, 2051, with a magnitude of 0.9849. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
The umbral shadow of the Moon will pass just above the North Pole. It will be the largest partial solar eclipse in 21st century.
The maximal phase of the partial eclipse (0.98) will be recorded in the Barents Sea. The partial solar eclipse will be visible for parts of Asia, Alaska, and western Canada.

## 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.
April 11, 2051 Solar Eclipse Times :
| Event | Time (UTC) |
| First Penumbral External Contact | 2051 April 11 at 00:12:31.3 UTC |
| Ecliptic Conjunction | 2051 April 11 at 02:00:30.3 UTC |
| Greatest Eclipse | 2051 April 11 at 02:10:38.6 UTC |
| Equatorial Conjunction | 2051 April 11 at 02:41:35.1 UTC |
| Last Penumbral External Contact | 2051 April 11 at 04:08:32.1 UTC |
April 11, 2051 Solar Eclipse Parameters :
| Parameter | Value |
| Eclipse Magnitude | 0.98490 |
| Eclipse Obscuration | 0.98811 |
| Gamma | 1.01694 |
| Sun Right Ascension | 01h18m13.3s |
| Sun Declination | +08°15'12.8" |
| Sun Semi-Diameter | 15'57.8" |
| Sun Equatorial Horizontal Parallax | 08.8" |
| Moon Right Ascension | 01h17m01.7s |
| Moon Declination | +09°14'52.8" |
| Moon Semi-Diameter | 16'42.8" |
| Moon Equatorial Horizontal Parallax | 1°01'20.2" |
| ΔT | 84.9 s |

## Eclipse season

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.
Eclipse season of April 2051 :
| April 11 Descending node (new moon) | April 26 Ascending node (full moon) |
| Partial solar eclipse Solar Saros 120 | Total lunar eclipse Lunar Saros 132 |

## Related eclipses
### Eclipses in 2051

* A partial solar eclipse on April 11.
* A total lunar eclipse on April 26.
* A partial solar eclipse on October 4.
* A total lunar eclipse on October 19.

### Metonic

* Preceded by: Solar eclipse of June 23, 2047
* Followed by: Solar eclipse of January 27, 2055

### Tzolkinex

* Preceded by: Solar eclipse of February 28, 2044
* Followed by: Solar eclipse of May 22, 2058

### Half-Saros

* Preceded by: Lunar eclipse of April 5, 2042
* Followed by: Lunar eclipse of April 15, 2060

### Tritos

* Preceded by: Solar eclipse of May 11, 2040
* Followed by: Solar eclipse of March 11, 2062

### Solar Saros 120

* Preceded by: Solar eclipse of March 30, 2033
* Followed by: Solar eclipse of April 21, 2069

### Inex

* Preceded by: Solar eclipse of April 30, 2022
* Followed by: Solar eclipse of March 21, 2080

### Triad

* Preceded by: Solar eclipse of June 10, 1964
* Followed by: Solar eclipse of February 9, 2138

### Solar eclipses of 2051–2054

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.
The partial solar eclipse on August 3, 2054 occurs in the next lunar year eclipse set.
Solar eclipse series sets from 2051 to 2054 :
| Descending node | Descending node | Descending node | Ascending node | Ascending node | Ascending node |
| Saros | Map | Gamma | Saros | Map | Gamma |
| 120 | April 11, 2051 Partial | 1.0169 | 125 | October 4, 2051 Partial | −1.2094 |
| 130 | March 30, 2052 Total | 0.3238 | 135 | September 22, 2052 Annular | −0.448 |
| 140 | March 20, 2053 Annular | −0.4089 | 145 | September 12, 2053 Total | 0.314 |
| 150 | March 9, 2054 Partial | −1.1711 | 155 | September 2, 2054 Partial | 1.0215 |

### Saros 120

This eclipse is a part of Saros series 120, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 27, 933 AD. It contains annular eclipses from August 11, 1059 through April 26, 1492; hybrid eclipses from May 8, 1510 through June 8, 1564; and total eclipses from June 20, 1582 through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. 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 annularity was produced by member 11 at 6 minutes, 24 seconds on September 11, 1113, and the longest duration of totality was produced by member 60 at 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occur at the Moon’s descending node of orbit.
Series members 50–71 occur between 1801 and 2195: :
| 50 | 51 | 52 |
| November 19, 1816 | November 30, 1834 | December 11, 1852 |
| 53 | 54 | 55 |
| December 22, 1870 | January 1, 1889 | January 14, 1907 |
| 56 | 57 | 58 |
| January 24, 1925 | February 4, 1943 | February 15, 1961 |
| 59 | 60 | 61 |
| February 26, 1979 | March 9, 1997 | March 20, 2015 |
| 62 | 63 | 64 |
| March 30, 2033 | April 11, 2051 | April 21, 2069 |
| 65 | 66 | 67 |
| May 2, 2087 | May 14, 2105 | May 25, 2123 |
| 68 | 69 | 70 |
| June 4, 2141 | June 16, 2159 | June 26, 2177 |
| 71 |
| July 7, 2195 |

### 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 descending node.
22 eclipse events between June 23, 2047 and November 16, 2134 :
| June 22–23 | April 10–11 | January 27–29 | November 15–16 | September 3–5 |
| 118 | 120 | 122 | 124 | 126 |
| June 23, 2047 | April 11, 2051 | January 27, 2055 | November 16, 2058 | September 3, 2062 |
| 128 | 130 | 132 | 134 | 136 |
| June 22, 2066 | April 11, 2070 | January 27, 2074 | November 15, 2077 | September 3, 2081 |
| 138 | 140 | 142 | 144 | 146 |
| June 22, 2085 | April 10, 2089 | January 27, 2093 | November 15, 2096 | September 4, 2100 |
| 148 | 150 | 152 | 154 | 156 |
| June 22, 2104 | April 11, 2108 | January 29, 2112 | November 16, 2115 | September 5, 2119 |
| 158 | 160 | 162 | 164 |
| June 23, 2123 | | | November 16, 2134 |

### Tritos series

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 2018 and 2200 :
| July 13, 2018 (Saros 117) | June 12, 2029 (Saros 118) | May 11, 2040 (Saros 119) | April 11, 2051 (Saros 120) | March 11, 2062 (Saros 121) |
| February 7, 2073 (Saros 122) | January 7, 2084 (Saros 123) | December 7, 2094 (Saros 124) | November 6, 2105 (Saros 125) | October 6, 2116 (Saros 126) |
| September 6, 2127 (Saros 127) | August 5, 2138 (Saros 128) | July 5, 2149 (Saros 129) | June 4, 2160 (Saros 130) | May 5, 2171 (Saros 131) |
| April 3, 2182 (Saros 132) | March 3, 2193 (Saros 133) |

### Inex series

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 :
| September 19, 1819 (Saros 112) | August 28, 1848 (Saros 113) | August 9, 1877 (Saros 114) |
| July 21, 1906 (Saros 115) | June 30, 1935 (Saros 116) | June 10, 1964 (Saros 117) |
| May 21, 1993 (Saros 118) | April 30, 2022 (Saros 119) | April 11, 2051 (Saros 120) |
| March 21, 2080 (Saros 121) | March 1, 2109 (Saros 122) | February 9, 2138 (Saros 123) |
| January 21, 2167 (Saros 124) | December 31, 2195 (Saros 125) | |