# Solar eclipse of June 1, 2030

An annular solar eclipse will occur at the Moon's descending node of orbit on Saturday, June 1, 2030, with a magnitude of 0.9443. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 23 hours after apogee (on May 31, 2030, at 7:15 UTC), the Moon's apparent diameter will be smaller.
The annular eclipse will start in northern Africa and will cross the Eurasian continent, including Algeria, Tunisia, Libya, Malta, Greece, northwestern Turkey, southeastern Bulgaria, southeastern Ukraine, Russia, northern Kazakhstan, northeastern China and northern Japan. It will also pass through a number of large cities such as Tripoli, Athens, Istanbul, Krasnodar, Rostov-on-Don, Volgograd, Omsk, Krasnoyarsk and Sapporo. The greatest eclipse will be near the border of Tomsk and Novosibirsk oblasts, ~200 km west of Tomsk. A partial eclipse will be visible for much of North Africa, Europe, Asia, Alaska, and northern Canada.

## Images

Animated path

## 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.
June 1, 2030 Solar Eclipse Times :
| Event | Time (UTC) |
| First Penumbral External Contact | 2030 June 01 at 03:35:53.3 UTC |
| First Umbral External Contact | 2030 June 01 at 04:48:25.8 UTC |
| First Central Line | 2030 June 01 at 04:51:16.8 UTC |
| First Umbral Internal Contact | 2030 June 01 at 04:54:09.4 UTC |
| Ecliptic Conjunction | 2030 June 01 at 06:22:30.7 UTC |
| Greatest Eclipse | 2030 June 01 at 06:29:12.9 UTC |
| Greatest Duration | 2030 June 01 at 06:29:55.1 UTC |
| Equatorial Conjunction | 2030 June 01 at 06:31:58.0 UTC |
| Last Umbral Internal Contact | 2030 June 01 at 08:04:14.9 UTC |
| Last Central Line | 2030 June 01 at 08:07:06.9 UTC |
| Last Umbral External Contact | 2030 June 01 at 08:09:57.3 UTC |
| Last Penumbral External Contact | 2030 June 01 at 09:22:29.8 UTC |
June 1, 2030 Solar Eclipse Parameters :
| Parameter | Value |
| Eclipse Magnitude | 0.94426 |
| Eclipse Obscuration | 0.89163 |
| Gamma | 0.56265 |
| Sun Right Ascension | 04h37m01.2s |
| Sun Declination | +22°03'55.3" |
| Sun Semi-Diameter | 15'46.4" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 04h36m55.8s |
| Moon Declination | +22°34'11.5" |
| Moon Semi-Diameter | 14'42.7" |
| Moon Equatorial Horizontal Parallax | 0°53'59.6" |
| ΔT | 74.0 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 June 2030 :
| June 1 Descending node (new moon) | June 15 Ascending node (full moon) |
| Annular solar eclipse Solar Saros 128 | Partial lunar eclipse Lunar Saros 140 |

## Related eclipses
### Eclipses in 2030

* An annular solar eclipse on June 1.
* A partial lunar eclipse on June 15.
* A total solar eclipse on November 25.
* A penumbral lunar eclipse on December 9.

### Metonic

* Preceded by: Solar eclipse of August 12, 2026
* Followed by: Solar eclipse of March 20, 2034

### Tzolkinex

* Preceded by: Solar eclipse of April 20, 2023
* Followed by: Solar eclipse of July 13, 2037

### Half-Saros

* Preceded by: Lunar eclipse of May 26, 2021
* Followed by: Lunar eclipse of June 6, 2039

### Tritos

* Preceded by: Solar eclipse of July 2, 2019
* Followed by: Solar eclipse of April 30, 2041

### Solar Saros 128

* Preceded by: Solar eclipse of May 20, 2012
* Followed by: Solar eclipse of June 11, 2048

### Inex

* Preceded by: Solar eclipse of June 21, 2001
* Followed by: Solar eclipse of May 11, 2059

### Triad

* Preceded by: Solar eclipse of August 1, 1943
* Followed by: Solar eclipse of April 2, 2117

### Solar eclipses of 2029–2032

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 January 14, 2029 and July 11, 2029 occur in the previous lunar year eclipse set.
Solar eclipse series sets from 2029 to 2032 :
| Descending node | Descending node | Descending node | Ascending node | Ascending node | Ascending node |
| Saros | Map | Gamma | Saros | Map | Gamma |
| 118 | June 12, 2029 Partial | 1.29431 | 123 | December 5, 2029 Partial | −1.06090 |
| 128 | June 1, 2030 Annular | 0.56265 | 133 | November 25, 2030 Total | −0.38669 |
| 138 | May 21, 2031 Annular | −0.19699 | 143 | November 14, 2031 Hybrid | 0.30776 |
| 148 | May 9, 2032 Annular | −0.93748 | 153 | November 3, 2032 Partial | 1.06431 |

### Saros 128

This eclipse is a part of Saros series 128, repeating every 18 years, 11 days, and containing 73 events. The series started with a partial solar eclipse on August 29, 984 AD. It contains total eclipses from May 16, 1417 through June 18, 1471; hybrid eclipses from June 28, 1489 through July 31, 1543; and annular eclipses from August 11, 1561 through July 25, 2120. The series ends at member 73 as a partial eclipse on November 1, 2282. 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 27 at 1 minutes, 45 seconds on June 7, 1453, and the longest duration of annularity was produced by member 48 at 8 minutes, 35 seconds on February 1, 1832. All eclipses in this series occur at the Moon’s descending node of orbit.
Series members 47–68 occur between 1801 and 2200: :
| 47 | 48 | 49 |
| January 21, 1814 | February 1, 1832 | February 12, 1850 |
| 50 | 51 | 52 |
| February 23, 1868 | March 5, 1886 | March 17, 1904 |
| 53 | 54 | 55 |
| March 28, 1922 | April 7, 1940 | April 19, 1958 |
| 56 | 57 | 58 |
| April 29, 1976 | May 10, 1994 | May 20, 2012 |
| 59 | 60 | 61 |
| June 1, 2030 | June 11, 2048 | June 22, 2066 |
| 62 | 63 | 64 |
| July 3, 2084 | July 15, 2102 | July 25, 2120 |
| 65 | 66 | 67 |
| August 5, 2138 | August 16, 2156 | August 27, 2174 |
| 68 |
| September 6, 2192 |

### 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 :
| March 14, 1801 (Saros 107) | February 12, 1812 (Saros 108) | January 12, 1823 (Saros 109) | | November 10, 1844 (Saros 111) |
| | | August 9, 1877 (Saros 114) | July 9, 1888 (Saros 115) | June 8, 1899 (Saros 116) |
| May 9, 1910 (Saros 117) | April 8, 1921 (Saros 118) | March 7, 1932 (Saros 119) | February 4, 1943 (Saros 120) | January 5, 1954 (Saros 121) |
| December 4, 1964 (Saros 122) | November 3, 1975 (Saros 123) | October 3, 1986 (Saros 124) | September 2, 1997 (Saros 125) | August 1, 2008 (Saros 126) |
| July 2, 2019 (Saros 127) | June 1, 2030 (Saros 128) | April 30, 2041 (Saros 129) | March 30, 2052 (Saros 130) | February 28, 2063 (Saros 131) |
| January 27, 2074 (Saros 132) | December 27, 2084 (Saros 133) | November 27, 2095 (Saros 134) | October 26, 2106 (Saros 135) | September 26, 2117 (Saros 136) |
| August 25, 2128 (Saros 137) | July 25, 2139 (Saros 138) | June 25, 2150 (Saros 139) | May 25, 2161 (Saros 140) | April 23, 2172 (Saros 141) |
| March 23, 2183 (Saros 142) | February 21, 2194 (Saros 143) |

### 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 :
| October 20, 1827 (Saros 121) | September 29, 1856 (Saros 122) | September 8, 1885 (Saros 123) |
| August 21, 1914 (Saros 124) | August 1, 1943 (Saros 125) | July 10, 1972 (Saros 126) |
| June 21, 2001 (Saros 127) | June 1, 2030 (Saros 128) | May 11, 2059 (Saros 129) |
| April 21, 2088 (Saros 130) | April 2, 2117 (Saros 131) | March 12, 2146 (Saros 132) |
| February 21, 2175 (Saros 133) | | |