# Solar eclipse of May 31, 2068

A total solar eclipse will occur at the Moon's descending node of orbit on Thursday, May 31, 2068, with a magnitude of 1.011. 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 4.7 days after perigee (on May 26, 2068, at 10:10 UTC), the Moon's apparent diameter will be larger.
The path of totality will be visible from parts of Australia and New Zealand. A partial solar eclipse will also be visible for parts of Australia, Indonesia, Antarctica, and western Oceania.

## 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.
May 31, 2068 Solar Eclipse Times :
| Event | Time (UTC) |
| First Penumbral External Contact | 2068 May 31 at 01:32:00.7 UTC |
| First Umbral External Contact | 2068 May 31 at 02:50:55.9 UTC |
| First Central Line | 2068 May 31 at 02:50:59.6 UTC |
| First Umbral Internal Contact | 2068 May 31 at 02:51:03.4 UTC |
| Equatorial Conjunction | 2068 May 31 at 03:52:45.4 UTC |
| Greatest Duration | 2068 May 31 at 03:54:49.9 UTC |
| Greatest Eclipse | 2068 May 31 at 03:56:39.1 UTC |
| Ecliptic Conjunction | 2068 May 31 at 04:05:16.2 UTC |
| Last Umbral Internal Contact | 2068 May 31 at 05:02:20.5 UTC |
| Last Central Line | 2068 May 31 at 05:02:21.5 UTC |
| Last Umbral External Contact | 2068 May 31 at 05:02:22.5 UTC |
| Last Penumbral External Contact | 2068 May 31 at 06:21:24.8 UTC |
May 31, 2068 Solar Eclipse Parameters :
| Parameter | Value |
| Eclipse Magnitude | 1.01098 |
| Eclipse Obscuration | 1.02209 |
| Gamma | −0.79704 |
| Sun Right Ascension | 04h35m49.8s |
| Sun Declination | +22°01'13.9" |
| Sun Semi-Diameter | 15'46.5" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 04h35m58.7s |
| Moon Declination | +21°15'11.0" |
| Moon Semi-Diameter | 15'47.8" |
| Moon Equatorial Horizontal Parallax | 0°57'58.6" |
| ΔT | 96.3 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 May 2068 :
| May 17 Ascending node (full moon) | May 31 Descending node (new moon) |
| Partial lunar eclipse Lunar Saros 122 | Total solar eclipse Solar Saros 148 |

## Related eclipses
### Eclipses in 2068

* A partial lunar eclipse on May 17.
* A total solar eclipse on May 31.
* A total lunar eclipse on November 9.
* A partial solar eclipse on November 24.

### Metonic

* Preceded by: Solar eclipse of August 12, 2064
* Followed by: Solar eclipse of March 19, 2072

### Tzolkinex

* Preceded by: Solar eclipse of April 20, 2061
* Followed by: Solar eclipse of July 13, 2075

### Half-Saros

* Preceded by: Lunar eclipse of May 27, 2059
* Followed by: Lunar eclipse of June 6, 2077

### Tritos

* Preceded by: Solar eclipse of July 1, 2057
* Followed by: Solar eclipse of May 1, 2079

### Solar Saros 148

* Preceded by: Solar eclipse of May 20, 2050
* Followed by: Solar eclipse of June 11, 2086

### Inex

* Preceded by: Solar eclipse of June 21, 2039
* Followed by: Solar eclipse of May 11, 2097

### Triad

* Preceded by: Solar eclipse of July 31, 1981
* Followed by: Solar eclipse of April 2, 2155

### Solar eclipses of 2065–2069

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 February 5, 2065 and August 2, 2065 occur in the previous lunar year eclipse set, and the partial solar eclipses on April 21, 2069 and October 15, 2069 occur in the next lunar year eclipse set.
Solar eclipse series sets from 2065 to 2069 :
| Descending node | Descending node | Descending node | Ascending node | Ascending node | Ascending node |
| Saros | Map | Gamma | Saros | Map | Gamma |
| 118 | July 3, 2065 Partial | 1.4619 | 123 | December 27, 2065 Partial | −1.0688 |
| 128 | June 22, 2066 Annular | 0.733 | 133 | December 17, 2066 Total | −0.4043 |
| 138 | June 11, 2067 Annular | −0.0387 | 143 | December 6, 2067 Hybrid | 0.2845 |
| 148 | May 31, 2068 Total | −0.797 | 153 | November 24, 2068 Partial | 1.0299 |
| 158 | May 20, 2069 Partial | −1.4852 |

### Saros 148

This eclipse is a part of Saros series 148, repeating every 18 years, 11 days, and containing 75 events. The series started with a partial solar eclipse on September 21, 1653. It contains annular eclipses on April 29, 2014 and May 9, 2032; a hybrid eclipse on May 20, 2050; and total eclipses from May 31, 2068 through August 3, 2771. The series ends at member 75 as a partial eclipse on December 12, 2987. 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 22 at 22 seconds (by default) on May 9, 2032, and the longest duration of totality will be produced by member 54 at 5 minutes, 23 seconds on April 26, 2609. All eclipses in this series occur at the Moon’s descending node of orbit.
Series members 10–31 occur between 1801 and 2200: :
| 10 | 11 | 12 |
| December 30, 1815 | January 9, 1834 | January 21, 1852 |
| 13 | 14 | 15 |
| January 31, 1870 | February 11, 1888 | February 23, 1906 |
| 16 | 17 | 18 |
| March 5, 1924 | March 16, 1942 | March 27, 1960 |
| 19 | 20 | 21 |
| April 7, 1978 | April 17, 1996 | April 29, 2014 |
| 22 | 23 | 24 |
| May 9, 2032 | May 20, 2050 | May 31, 2068 |
| 25 | 26 | 27 |
| June 11, 2086 | June 22, 2104 | July 4, 2122 |
| 28 | 29 | 30 |
| July 14, 2140 | July 25, 2158 | August 4, 2176 |
| 31 |
| August 16, 2194 |

### 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 1, 2011 and October 24, 2098 :
| May 31–June 1 | March 19–20 | January 5–6 | October 24–25 | August 12–13 |
| 118 | 120 | 122 | 124 | 126 |
| June 1, 2011 | March 20, 2015 | January 6, 2019 | October 25, 2022 | August 12, 2026 |
| 128 | 130 | 132 | 134 | 136 |
| June 1, 2030 | March 20, 2034 | January 5, 2038 | October 25, 2041 | August 12, 2045 |
| 138 | 140 | 142 | 144 | 146 |
| May 31, 2049 | March 20, 2053 | January 5, 2057 | October 24, 2060 | August 12, 2064 |
| 148 | 150 | 152 | 154 | 156 |
| May 31, 2068 | March 19, 2072 | January 6, 2076 | October 24, 2079 | August 13, 2083 |
| 158 | 160 | 162 | 164 |
| June 1, 2087 | | | October 24, 2098 |

### 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 2200 :
| June 16, 1806 (Saros 124) | May 16, 1817 (Saros 125) | April 14, 1828 (Saros 126) | March 15, 1839 (Saros 127) | February 12, 1850 (Saros 128) |
| January 11, 1861 (Saros 129) | December 12, 1871 (Saros 130) | November 10, 1882 (Saros 131) | October 9, 1893 (Saros 132) | September 9, 1904 (Saros 133) |
| August 10, 1915 (Saros 134) | July 9, 1926 (Saros 135) | June 8, 1937 (Saros 136) | May 9, 1948 (Saros 137) | April 8, 1959 (Saros 138) |
| March 7, 1970 (Saros 139) | February 4, 1981 (Saros 140) | January 4, 1992 (Saros 141) | December 4, 2002 (Saros 142) | November 3, 2013 (Saros 143) |
| October 2, 2024 (Saros 144) | September 2, 2035 (Saros 145) | August 2, 2046 (Saros 146) | July 1, 2057 (Saros 147) | May 31, 2068 (Saros 148) |
| May 1, 2079 (Saros 149) | March 31, 2090 (Saros 150) | February 28, 2101 (Saros 151) | January 29, 2112 (Saros 152) | December 28, 2122 (Saros 153) |
| November 26, 2133 (Saros 154) | October 26, 2144 (Saros 155) | September 26, 2155 (Saros 156) | August 25, 2166 (Saros 157) | July 25, 2177 (Saros 158) |
| June 24, 2188 (Saros 159) | May 24, 2199 (Saros 160) |

### 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 :
| November 29, 1807 (Saros 139) | November 9, 1836 (Saros 140) | October 19, 1865 (Saros 141) |
| September 29, 1894 (Saros 142) | September 10, 1923 (Saros 143) | August 20, 1952 (Saros 144) |
| July 31, 1981 (Saros 145) | July 11, 2010 (Saros 146) | June 21, 2039 (Saros 147) |
| May 31, 2068 (Saros 148) | May 11, 2097 (Saros 149) | April 22, 2126 (Saros 150) |
| April 2, 2155 (Saros 151) | March 12, 2184 (Saros 152) | |