• Source: Solar eclipse of July 22, 2047

      • A partial solar eclipse will occur at the Moon's descending node of orbit between Monday, July 22 and Tuesday, July 23, 2047, with a magnitude of 0.3604. 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 partial solar eclipses in 2047, with the others occurring on January 26, June 23, and December 16.
      The partial solar eclipse will be visible for parts of southeastern Australia and New Zealand.


      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.


      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.


      Related eclipses




      = Eclipses in 2047

      =
      A total lunar eclipse on January 12.
      A partial solar eclipse on January 26.
      A partial solar eclipse on June 23.
      A total lunar eclipse on July 7.
      A partial solar eclipse on July 22.
      A partial solar eclipse on December 16.


      = Metonic

      =
      Preceded by: Solar eclipse of October 3, 2043


      = Tzolkinex

      =
      Followed by: Solar eclipse of September 2, 2054


      = Half-Saros

      =
      Preceded by: Lunar eclipse of July 16, 2038
      Followed by: Lunar eclipse of July 26, 2056


      = Tritos

      =
      Preceded by: Solar eclipse of August 21, 2036
      Followed by: Solar eclipse of June 21, 2058


      = Solar Saros 156

      =
      Preceded by: Solar eclipse of July 11, 2029
      Followed by: Solar eclipse of August 2, 2065


      = Inex

      =
      Preceded by: Solar eclipse of August 11, 2018
      Followed by: Solar eclipse of July 1, 2076


      = Triad

      =
      Preceded by: Solar eclipse of September 20, 1960
      Followed by: Solar eclipse of May 23, 2134


      = Solar eclipses of 2044–2047

      =
      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 23, 2047 and December 16, 2047 occur in the next lunar year eclipse set.


      = Saros 156

      =
      This eclipse is a part of Saros series 156, repeating every 18 years, 11 days, and containing 69 events. The series started with a partial solar eclipse on July 1, 2011. It contains annular eclipses from September 26, 2155 through April 7, 3075. There are no hybrid or total eclipses in this set. The series ends at member 69 as a partial eclipse on July 14, 3237. 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 29 at 8 minutes, 28 seconds on May 3, 2516. All eclipses in this series occur at the Moon’s descending node of orbit.


      = 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.


      = 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.
      The partial solar eclipses on November 16, 2134 (part of Saros 164) and October 16, 2145 (part of Saros 165) are also a part of this series but are not included in the table below.


      = 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.


      References




      External links


      Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
      Google interactive map
      Besselian elements

    Kata Kunci Pencarian: