June 2075 lunar eclipse GudangMovies21 Rebahinxxi LK21

    A partial lunar eclipse will occur at the Moon’s descending node of orbit on Friday, June 28, 2075, with an umbral magnitude of 0.6235. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. 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. Occurring only about 5.5 hours after perigee (on June 28, 2075, at 4:10 UTC), the Moon's apparent diameter will be larger.


    Visibility


    The eclipse will be completely visible over eastern Australia, western North America, Antarctica, and the central and eastern Pacific Ocean, seen rising over east Asia and western Australia and setting over much of North and South America.


    Eclipse details


    Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.


    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.


    Related eclipses




    = Eclipses in 2075

    =
    A penumbral lunar eclipse on January 2.
    A total solar eclipse on January 16.
    A partial lunar eclipse on June 28.
    An annular solar eclipse on July 13.
    A partial lunar eclipse on December 22.


    = Metonic

    =
    Preceded by: Lunar eclipse of September 9, 2071
    Followed by: Lunar eclipse of April 16, 2079


    = Tzolkinex

    =
    Preceded by: Lunar eclipse of May 17, 2068
    Followed by: Lunar eclipse of August 8, 2082


    = Half-Saros

    =
    Preceded by: Solar eclipse of June 22, 2066
    Followed by: Solar eclipse of July 3, 2084


    = Tritos

    =
    Preceded by: Lunar eclipse of July 28, 2064
    Followed by: Lunar eclipse of May 28, 2086


    = Lunar Saros 121

    =
    Preceded by: Lunar eclipse of June 17, 2057
    Followed by: Lunar eclipse of July 8, 2093


    = Inex

    =
    Preceded by: Lunar eclipse of July 18, 2046
    Followed by: Lunar eclipse of June 8, 2104


    = Triad

    =
    Preceded by: Lunar eclipse of August 27, 1988
    Followed by: Lunar eclipse of April 29, 2162


    = Lunar eclipses of 2074–2078

    =
    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 11, 2074 and August 7, 2074 occur in the previous lunar year eclipse set, and the penumbral lunar eclipses on April 27, 2078 and October 21, 2078 occur in the next lunar year eclipse set.


    = Saros 121

    =
    This eclipse is a part of Saros series 121, repeating every 18 years, 11 days, and containing 82 events. The series started with a penumbral lunar eclipse on October 6, 1047. It contains partial eclipses from May 10, 1408 through July 3, 1498; total eclipses from July 13, 1516 through May 26, 2021; and a second set of partial eclipses from June 6, 2039 through August 11, 2147. The series ends at member 82 as a penumbral eclipse on March 18, 2508.
    The longest duration of totality was produced by member 43 at 100 minutes, 29 seconds on October 18, 1660. All eclipses in this series occur at the Moon’s descending node of orbit.

    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.


    = 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.


    = 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 total solar eclipses of Solar Saros 128.


    See also


    List of lunar eclipses and List of 21st-century lunar eclipses


    References

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