# Solar eclipse of July 1, 2076

A partial solar eclipse will occur at the Moon's ascending node of orbit on Wednesday, July 1, 2076, with a magnitude of 0.2746. 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.
This will be the third of four solar eclipses in 2076, with the others occurring on January 6, June 1, and November 26.
The partial solar eclipse will be visible for parts of Greenland, northern Canada, Alaska, and the Russian Far East.

## 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.
July 1, 2076 Solar Eclipse Times :
| Event | Time (UTC) |
| First Penumbral External Contact | 2076 July 01 at 05:30:23.1 UTC |
| Greatest Eclipse | 2076 July 01 at 06:50:43.3 UTC |
| Equatorial Conjunction | 2076 July 01 at 06:53:58.3 UTC |
| Ecliptic Conjunction | 2076 July 01 at 07:06:45.0 UTC |
| Last Penumbral External Contact | 2076 July 01 at 08:11:05.4 UTC |
July 1, 2076 Solar Eclipse Parameters :
| Parameter | Value |
| Eclipse Magnitude | 0.27461 |
| Eclipse Obscuration | 0.16287 |
| Gamma | 1.40052 |
| Sun Right Ascension | 06h44m59.8s |
| Sun Declination | +23°01'35.5" |
| Sun Semi-Diameter | 15'43.9" |
| Sun Equatorial Horizontal Parallax | 08.6" |
| Moon Right Ascension | 06h44m53.2s |
| Moon Declination | +24°17'50.8" |
| Moon Semi-Diameter | 14'52.7" |
| Moon Equatorial Horizontal Parallax | 0°54'36.1" |
| ΔT | 102.6 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. The first and last eclipse in this sequence is separated by one synodic month.
Eclipse season of June–July 2076 :
| June 1 Ascending node (new moon) | June 17 Descending node (full moon) | July 1 Ascending node (new moon) |
| Partial solar eclipse Solar Saros 119 | Total lunar eclipse Lunar Saros 131 | Partial solar eclipse Solar Saros 157 |

## Related eclipses
### Eclipses in 2076

* A total solar eclipse on January 6.
* A partial solar eclipse on June 1.
* A total lunar eclipse on June 17.
* A partial solar eclipse on July 1.
* A partial solar eclipse on November 26.
* A total lunar eclipse on December 10.

### Metonic

* Preceded by: Solar eclipse of September 12, 2072

### Tzolkinex

* Preceded by: Solar eclipse of May 20, 2069
* Followed by: Solar eclipse of August 13, 2083

### Half-Saros

* Preceded by: Lunar eclipse of June 27, 2067
* Followed by: Lunar eclipse of July 7, 2085

### Tritos

* Preceded by: Solar eclipse of August 2, 2065
* Followed by: Solar eclipse of June 1, 2087

### Solar Saros 157

* Preceded by: Solar eclipse of June 21, 2058
* Followed by: Solar eclipse of July 12, 2094

### Inex

* Preceded by: Solar eclipse of July 22, 2047
* Followed by: Solar eclipse of June 12, 2105

### Triad

* Preceded by: Solar eclipse of August 31, 1989

### Solar eclipses of 2073–2076

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 eclipses on June 1, 2076 and November 26, 2076 occur in the next lunar year eclipse set.
Solar eclipse series sets from 2073 to 2076 :
| Descending node | Descending node | Descending node | Ascending node | Ascending node | Ascending node |
| Saros | Map | Gamma | Saros | Map | Gamma |
| 122 | February 7, 2073 Partial | 1.1651 | 127 | August 3, 2073 Total | −0.8763 |
| 132 | January 27, 2074 Annular | 0.4251 | 137 | July 24, 2074 Annular | −0.1242 |
| 142 | January 16, 2075 Total | −0.2799 | 147 | July 13, 2075 Annular | 0.6583 |
| 152 | January 6, 2076 Total | −0.9373 | 157 | July 1, 2076 Partial | 1.4005 |

### Saros 157

This eclipse is a part of Saros series 157, repeating every 18 years, 11 days, and containing 70 events. The series will start with a partial solar eclipse on June 21, 2058. It contains annular eclipses from August 25, 2166 through March 10, 2491; hybrid eclipses from March 22, 2509 through April 12, 2545; and total eclipses from April 24, 2563 through April 21, 3158. The series ends at member 70 as a partial eclipse on July 17, 3302. 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 will be produced by member 15 at 4 minutes, 16 seconds on November 22, 2310, and the longest duration of totality will be produced by member 38 at 5 minutes, 57 seconds on July 31, 2725. All eclipses in this series occur at the Moon’s ascending node of orbit.
Series members 1–8 occur between 2058 and 2200: :
| 1 | 2 | 3 |
| June 21, 2058 | July 1, 2076 | July 12, 2094 |
| 4 | 5 | 6 |
| July 23, 2112 | August 4, 2130 | August 14, 2148 |
| 7 | 8 |
| August 25, 2166 | September 4, 2184 |

### 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.
21 eclipse events between July 1, 2000 and July 1, 2076 :
| July 1–2 | April 19–20 | February 5–7 | November 24–25 | September 12–13 |
| 117 | 119 | 121 | 123 | 125 |
| July 1, 2000 | April 19, 2004 | February 7, 2008 | November 25, 2011 | September 13, 2015 |
| 127 | 129 | 131 | 133 | 135 |
| July 2, 2019 | April 20, 2023 | February 6, 2027 | November 25, 2030 | September 12, 2034 |
| 137 | 139 | 141 | 143 | 145 |
| July 2, 2038 | April 20, 2042 | February 5, 2046 | November 25, 2049 | September 12, 2053 |
| 147 | 149 | 151 | 153 | 155 |
| July 1, 2057 | April 20, 2061 | February 5, 2065 | November 24, 2068 | September 12, 2072 |
| 157 |
| July 1, 2076 |

### 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 1801 and 2087 :
| August 17, 1803 (Saros 132) | July 17, 1814 (Saros 133) | June 16, 1825 (Saros 134) | May 15, 1836 (Saros 135) | April 15, 1847 (Saros 136) |
| March 15, 1858 (Saros 137) | February 11, 1869 (Saros 138) | January 11, 1880 (Saros 139) | December 12, 1890 (Saros 140) | November 11, 1901 (Saros 141) |
| October 10, 1912 (Saros 142) | September 10, 1923 (Saros 143) | August 10, 1934 (Saros 144) | July 9, 1945 (Saros 145) | June 8, 1956 (Saros 146) |
| May 9, 1967 (Saros 147) | April 7, 1978 (Saros 148) | March 7, 1989 (Saros 149) | February 5, 2000 (Saros 150) | January 4, 2011 (Saros 151) |
| December 4, 2021 (Saros 152) | November 3, 2032 (Saros 153) | October 3, 2043 (Saros 154) | September 2, 2054 (Saros 155) | August 2, 2065 (Saros 156) |
| July 1, 2076 (Saros 157) | June 1, 2087 (Saros 158) |

### 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 :
| December 30, 1815 (Saros 148) | December 9, 1844 (Saros 149) | November 20, 1873 (Saros 150) |
| October 31, 1902 (Saros 151) | October 11, 1931 (Saros 152) | September 20, 1960 (Saros 153) |
| August 31, 1989 (Saros 154) | August 11, 2018 (Saros 155) | July 22, 2047 (Saros 156) |
| July 1, 2076 (Saros 157) | June 12, 2105 (Saros 158) | May 23, 2134 (Saros 159) |
| | April 12, 2192 (Saros 161) | |