No More Posts Available.

No more pages to load.

    • Source: Solar eclipse of September 22, 2052

      • An annular solar eclipse will occur at the Moon's ascending node of orbit between Sunday, September 22 and Monday, September 23, 2052, with a magnitude of 0.9734. 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 5.9 days before apogee (on September 28, 2052, at 20:25 UTC), the Moon's apparent diameter will be smaller.
      The path of annularity will be visible from parts of southern Indonesia, East Timor, the northern tip of Queensland, Australia, and New Caledonia. A partial solar eclipse will also be visible for parts of Australia, Indonesia, the Philippines, Oceania, and Antarctica.


      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.


      Related eclipses




      = Eclipses in 2052

      =
      A total solar eclipse on March 30.
      A penumbral lunar eclipse on April 14.
      An annular solar eclipse on September 22.
      A partial lunar eclipse on October 8.


      = Metonic

      =
      Preceded by: Solar eclipse of December 5, 2048
      Followed by: Solar eclipse of July 12, 2056


      = Tzolkinex

      =
      Preceded by: Solar eclipse of August 12, 2045
      Followed by: Solar eclipse of November 5, 2059


      = Half-Saros

      =
      Preceded by: Lunar eclipse of September 19, 2043
      Followed by: Lunar eclipse of September 29, 2061


      = Tritos

      =
      Preceded by: Solar eclipse of October 25, 2041
      Followed by: Solar eclipse of August 24, 2063


      = Solar Saros 135

      =
      Preceded by: Solar eclipse of September 12, 2034
      Followed by: Solar eclipse of October 4, 2070


      = Inex

      =
      Preceded by: Solar eclipse of October 14, 2023
      Followed by: Solar eclipse of September 3, 2081


      = Triad

      =
      Preceded by: Solar eclipse of November 23, 1965
      Followed by: Solar eclipse of July 25, 2139


      = Solar eclipses of 2051ā€“2054

      =
      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 eclipse on August 3, 2054 occurs in the next lunar year eclipse set.


      = Saros 135

      =
      This eclipse is a part of Saros series 135, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on July 5, 1331. It contains annular eclipses from October 21, 1511 through February 24, 2305; hybrid eclipses on March 8, 2323 and March 18, 2341; and total eclipses from March 29, 2359 through May 22, 2449. The series ends at member 71 as a partial eclipse on August 17, 2593. 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 was produced by member 16 at 10 minutes, 41 seconds on December 24, 1601, and the longest duration of totality will be produced by member 62 at 2 minutes, 27 seconds on May 12, 2431. All eclipses in this series occur at the Moonā€™s ascending 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 ascending node.


      = Tritos series

      =
      This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (ā‰ˆ 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 (ā‰ˆ 33 years minus 3 months) come close (ā‰ˆ 434.044 anomalistic months), so eclipses are similar in these groupings.


      = Inex series

      =
      This eclipse is a part of the long period inex cycle, repeating at alternating nodes, every 358 synodic months (ā‰ˆ 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 (ā‰ˆ 87 years minus 2 months) comes close (ā‰ˆ 1,151.02 anomalistic months), so eclipses are similar in these groupings.


      References




      External links


      NASA graphics

    Kata Kunci Pencarian: