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    • Source: Solar eclipse of January 16, 2075

      • A total solar eclipse will occur at the Moon's descending node of orbit on Wednesday, January 16, 2075, with a magnitude of 1.0311. 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 total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring about 1.5 days after perigee (on January 15, 2075, at 7:25 UTC), the Moon's apparent diameter will be larger.
      The path of totality will be visible from parts of Chile, Argentina, Paraguay, and Brazil. A partial solar eclipse will also be visible for parts of Oceania, Antarctica, and South America.


      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 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: Solar eclipse of March 31, 2071
      Followed by: Solar eclipse of November 4, 2078


      = Tzolkinex

      =
      Preceded by: Solar eclipse of December 6, 2067
      Followed by: Solar eclipse of February 27, 2082


      = Half-Saros

      =
      Preceded by: Lunar eclipse of January 11, 2066
      Followed by: Lunar eclipse of January 22, 2084


      = Tritos

      =
      Preceded by: Solar eclipse of February 17, 2064
      Followed by: Solar eclipse of December 16, 2085


      = Solar Saros 142

      =
      Preceded by: Solar eclipse of January 5, 2057
      Followed by: Solar eclipse of January 27, 2093


      = Inex

      =
      Preceded by: Solar eclipse of February 5, 2046
      Followed by: Solar eclipse of December 29, 2103


      = Triad

      =
      Preceded by: Solar eclipse of March 18, 1988
      Followed by: Solar eclipse of November 17, 2161


      = Solar eclipses of 2073–2076

      =
      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 1, 2076 and November 26, 2076 occur in the next lunar year eclipse set.


      = Saros 142

      =
      This eclipse is a part of Saros series 142, repeating every 18 years, 11 days, and containing 72 events. The series started with a partial solar eclipse on April 17, 1624. It contains a hybrid eclipse on July 14, 1768, and total eclipses from July 25, 1786 through October 29, 2543. There are no annular eclipses in this set. The series ends at member 72 as a partial eclipse on June 5, 2904. 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 will be produced by member 38 at 6 minutes, 34 seconds on May 28, 2291. 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.


      = 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.


      Notes




      References


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

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