# June 2058 lunar eclipse

A total lunar eclipse will occur at the Moon’s descending node of orbit on Thursday, June 6, 2058, with an umbral magnitude of 1.6628. It will be a central lunar eclipse, in which part of the Moon will pass through the center of the Earth's shadow. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 1.6 days before perigee (on June 8, 2058, at 9:30 UTC), the Moon's apparent diameter will be larger.
During the eclipse, IC 4634 will be occulted by the Moon over Antarctica. Deep-sky objects are rarely occulted during a total eclipse from any given spot on Earth.$^{:161}$

## Visibility

The eclipse will be completely visible over east Africa, Antarctica, west, central, and south Asia, and western Australia, seen rising over west Africa, Europe, and eastern South America and setting over east Asia and eastern Australia.

## Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
June 6, 2058 Lunar Eclipse Parameters :
| Parameter | Value |
| Penumbral Magnitude | 2.62261 |
| Umbral Magnitude | 1.66277 |
| Gamma | −0.11810 |
| Sun Right Ascension | 05h00m41.7s |
| Sun Declination | +22°43'57.0" |
| Sun Semi-Diameter | 15'45.8" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 17h00m35.5s |
| Moon Declination | -22°50'55.4" |
| Moon Semi-Diameter | 16'25.3" |
| Moon Equatorial Horizontal Parallax | 1°00'16.2" |
| ΔT | 90.8 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 May–June 2058 :
| May 22 Ascending node (new moon) | June 6 Descending node (full moon) | June 21 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 2058

* A partial solar eclipse on May 22.
* A total lunar eclipse on June 6.
* A partial solar eclipse on June 21.
* A partial solar eclipse on November 16.
* A total lunar eclipse on November 30.

### Metonic

* Preceded by: Lunar eclipse of August 18, 2054
* Followed by: Lunar eclipse of March 25, 2062

### Tzolkinex

* Preceded by: Lunar eclipse of April 26, 2051
* Followed by: Lunar eclipse of July 17, 2065

### Half-Saros

* Preceded by: Solar eclipse of May 31, 2049
* Followed by: Solar eclipse of June 11, 2067

### Tritos

* Preceded by: Lunar eclipse of July 7, 2047
* Followed by: Lunar eclipse of May 6, 2069

### Lunar Saros 131

* Preceded by: Lunar eclipse of May 26, 2040
* Followed by: Lunar eclipse of June 17, 2076

### Inex

* Preceded by: Lunar eclipse of June 26, 2029
* Followed by: Lunar eclipse of May 17, 2087

### Triad

* Preceded by: Lunar eclipse of August 6, 1971
* Followed by: Lunar eclipse of April 7, 2145

### Lunar eclipses of 2056–2060

This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.
The penumbral lunar eclipses on February 1, 2056 and July 26, 2056 occur in the previous lunar year eclipse set, and the penumbral lunar eclipses on April 15, 2060 and October 9, 2060 occur in the next lunar year eclipse set.
Lunar eclipse series sets from 2056 to 2060 :
| Descending node | Descending node | Descending node | Descending node | Ascending node | Ascending node | Ascending node | Ascending node |
| Saros | Date Viewing | Type Chart | Gamma | Saros | Date Viewing | Type Chart | Gamma |
| 111 | 2056 Jun 27 | Penumbral | 1.3769 | 116 | 2056 Dec 22 | Penumbral | −1.1559 |
| 121 | 2057 Jun 17 | Partial | 0.6167 | 126 | 2057 Dec 11 | Partial | −0.4853 |
| 131 | 2058 Jun 06 | Total | −0.1181 | 136 | 2058 Nov 30 | Total | 0.2208 |
| 141 | 2059 May 27 | Partial | −0.9097 | 146 | 2059 Nov 19 | Partial | 0.9004 |
| | | | | 156 | 2060 Nov 08 | Penumbral | 1.5332 |

### Saros 131

This eclipse is a part of Saros series 131, repeating every 18 years, 11 days, and containing 72 events. The series started with a penumbral lunar eclipse on May 10, 1427. It contains partial eclipses from July 25, 1553 through March 22, 1932; total eclipses from April 2, 1950 through September 3, 2202; and a second set of partial eclipses from September 13, 2220 through April 9, 2563. The series ends at member 72 as a penumbral eclipse on July 7, 2707.
The longest duration of totality will be produced by member 38 at 100 minutes, 36 seconds on June 28, 2094. All eclipses in this series occur at the Moon’s descending node of orbit.
| Greatest | First | First | First | First |
| The greatest eclipse of the series will occur on 2094 Jun 28, lasting 100 minutes, 36 seconds. | Penumbral | Partial | Total | Central |
| The greatest eclipse of the series will occur on 2094 Jun 28, lasting 100 minutes, 36 seconds. | 1427 May 10 | 1553 Jul 25 | 1950 Apr 02 | 2022 May 16 |
| Last ||||
| The greatest eclipse of the series will occur on 2094 Jun 28, lasting 100 minutes, 36 seconds. | Central | Total | Partial | Penumbral |
| The greatest eclipse of the series will occur on 2094 Jun 28, lasting 100 minutes, 36 seconds. | 2148 Jul 31 | 2202 Sep 03 | 2563 Apr 09 | 2707 Jul 07 |
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.
Series members 22–43 occur between 1801 and 2200: :
| 22 | 22 | 23 | 23 | 24 | 24 |
| 1806 Jan 05 | 1806 Jan 05 | 1824 Jan 16 | 1824 Jan 16 | 1842 Jan 26 | 1842 Jan 26 |
| 25 | 25 | 26 | 26 | 27 | 27 |
| 1860 Feb 07 | 1860 Feb 07 | 1878 Feb 17 | 1878 Feb 17 | 1896 Feb 28 | 1896 Feb 28 |
| 28 | 28 | 29 | 29 | 30 | 30 |
| 1914 Mar 12 | 1914 Mar 12 | 1932 Mar 22 | 1932 Mar 22 | 1950 Apr 02 | 1950 Apr 02 |
| 31 | 31 | 32 | 32 | 33 | 33 |
| 1968 Apr 13 | 1968 Apr 13 | 1986 Apr 24 | 1986 Apr 24 | 2004 May 04 | 2004 May 04 |
| 34 | 34 | 35 | 35 | 36 | 36 |
| 2022 May 16 | 2022 May 16 | 2040 May 26 | 2040 May 26 | 2058 Jun 06 | 2058 Jun 06 |
| 37 | 37 | 38 | 38 | 39 | 39 |
| 2076 Jun 17 | 2076 Jun 17 | 2094 Jun 28 | 2094 Jun 28 | 2112 Jul 09 | 2112 Jul 09 |
| 40 | 40 | 41 | 41 | 42 | 42 |
| 2130 Jul 21 | 2130 Jul 21 | 2148 Jul 31 | 2148 Jul 31 | 2166 Aug 11 | 2166 Aug 11 |
| 43 ||
| 2184 Aug 21 ||

### 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 :
| 1807 May 21 (Saros 108) | 1807 May 21 (Saros 108) | 1818 Apr 21 (Saros 109) | 1818 Apr 21 (Saros 109) | 1829 Mar 20 (Saros 110) | 1829 Mar 20 (Saros 110) | 1840 Feb 17 (Saros 111) | 1840 Feb 17 (Saros 111) | 1851 Jan 17 (Saros 112) | 1851 Jan 17 (Saros 112) |
| 1861 Dec 17 (Saros 113) | 1861 Dec 17 (Saros 113) | 1872 Nov 15 (Saros 114) | 1872 Nov 15 (Saros 114) | 1883 Oct 16 (Saros 115) | 1883 Oct 16 (Saros 115) | 1894 Sep 15 (Saros 116) | 1894 Sep 15 (Saros 116) | 1905 Aug 15 (Saros 117) | 1905 Aug 15 (Saros 117) |
| 1916 Jul 15 (Saros 118) | 1916 Jul 15 (Saros 118) | 1927 Jun 15 (Saros 119) | 1927 Jun 15 (Saros 119) | 1938 May 14 (Saros 120) | 1938 May 14 (Saros 120) | 1949 Apr 13 (Saros 121) | 1949 Apr 13 (Saros 121) | 1960 Mar 13 (Saros 122) | 1960 Mar 13 (Saros 122) |
| 1971 Feb 10 (Saros 123) | 1971 Feb 10 (Saros 123) | 1982 Jan 09 (Saros 124) | 1982 Jan 09 (Saros 124) | 1992 Dec 09 (Saros 125) | 1992 Dec 09 (Saros 125) | 2003 Nov 09 (Saros 126) | 2003 Nov 09 (Saros 126) | 2014 Oct 08 (Saros 127) | 2014 Oct 08 (Saros 127) |
| 2025 Sep 07 (Saros 128) | 2025 Sep 07 (Saros 128) | 2036 Aug 07 (Saros 129) | 2036 Aug 07 (Saros 129) | 2047 Jul 07 (Saros 130) | 2047 Jul 07 (Saros 130) | 2058 Jun 06 (Saros 131) | 2058 Jun 06 (Saros 131) | 2069 May 06 (Saros 132) | 2069 May 06 (Saros 132) |
| 2080 Apr 04 (Saros 133) | 2080 Apr 04 (Saros 133) | 2091 Mar 05 (Saros 134) | 2091 Mar 05 (Saros 134) | 2102 Feb 03 (Saros 135) | 2102 Feb 03 (Saros 135) | 2113 Jan 02 (Saros 136) | 2113 Jan 02 (Saros 136) | 2123 Dec 03 (Saros 137) | 2123 Dec 03 (Saros 137) |
| 2134 Nov 02 (Saros 138) | 2134 Nov 02 (Saros 138) | 2145 Sep 30 (Saros 139) | 2145 Sep 30 (Saros 139) | 2156 Aug 30 (Saros 140) | 2156 Aug 30 (Saros 140) | 2167 Aug 01 (Saros 141) | 2167 Aug 01 (Saros 141) | 2178 Jun 30 (Saros 142) | 2178 Jun 30 (Saros 142) |
| 2189 May 29 (Saros 143) | 2189 May 29 (Saros 143) | 2200 Apr 30 (Saros 144) | 2200 Apr 30 (Saros 144) |

### 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 :
| 1826 Nov 14 (Saros 123) | 1826 Nov 14 (Saros 123) | 1855 Oct 25 (Saros 124) | 1855 Oct 25 (Saros 124) | 1884 Oct 04 (Saros 125) | 1884 Oct 04 (Saros 125) |
| 1913 Sep 15 (Saros 126) | 1913 Sep 15 (Saros 126) | 1942 Aug 26 (Saros 127) | 1942 Aug 26 (Saros 127) | 1971 Aug 06 (Saros 128) | 1971 Aug 06 (Saros 128) |
| 2000 Jul 16 (Saros 129) | 2000 Jul 16 (Saros 129) | 2029 Jun 26 (Saros 130) | 2029 Jun 26 (Saros 130) | 2058 Jun 06 (Saros 131) | 2058 Jun 06 (Saros 131) |
| 2087 May 17 (Saros 132) | 2087 May 17 (Saros 132) | 2116 Apr 27 (Saros 133) | 2116 Apr 27 (Saros 133) | 2145 Apr 07 (Saros 134) | 2145 Apr 07 (Saros 134) |
| 2174 Mar 18 (Saros 135) ||

### Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two annular solar eclipses of Solar Saros 138.
| May 31, 2049 | June 11, 2067 |