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Solar eclipse of August 2, 2065 GudangMovies21 Rebahinxxi LK21
A partial solar eclipse will occur at the Moon's descending node of orbit on Sunday, August 2, 2065, with a magnitude of 0.4903. 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 2065, with the others occurring on February 5, July 3, and December 27.
The partial solar eclipse will be visible for parts of eastern South Africa, southern Madagascar, and Antarctica.
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.
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 2065
=
A total lunar eclipse on January 22.
A partial solar eclipse on February 5.
A partial solar eclipse on July 3.
A total lunar eclipse on July 17.
A partial solar eclipse on August 2.
A partial solar eclipse on December 27.
= Metonic
=
Preceded by: Solar eclipse of October 13, 2061
Followed by: Solar eclipse of May 20, 2069
= Tzolkinex
=
Preceded by: Solar eclipse of June 21, 2058
Followed by: Solar eclipse of September 12, 2072
= Half-Saros
=
Preceded by: Lunar eclipse of July 26, 2056
Followed by: Lunar eclipse of August 7, 2074
= Tritos
=
Preceded by: Solar eclipse of September 2, 2054
Followed by: Solar eclipse of July 1, 2076
= Solar Saros 156
=
Preceded by: Solar eclipse of July 22, 2047
Followed by: Solar eclipse of August 13, 2083
= Inex
=
Preceded by: Solar eclipse of August 21, 2036
Followed by: Solar eclipse of July 12, 2094
= Triad
=
Preceded by: Solar eclipse of October 2, 1978
Followed by: Solar eclipse of June 3, 2152
= Solar eclipses of 2062–2065
=
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 July 3, 2065 and December 27, 2065 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.
= 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
http://eclipse.gsfc.nasa.gov/SEplot/SEplot2051/SE2065Aug02P.GIF
Kata Kunci Pencarian:
Solar eclipse of August 2, 2065 - Wikipedia
Solar eclipse of August 2, 2065 - Wikipedia
Solar eclipse of August 2, 2065 - Alchetron, the free social encyclopedia
Solar eclipse of August 2, 2065 - Wikiwand
Solar eclipse of August 2, 2065 - Wikipedia
Solar eclipse of August 2, 2065 - Wikipedia
Solar eclipse of August 2, 2065 - Wikipedia
Solar eclipse of August 2, 2065 - Wikipedia
Solar eclipse of February 5, 2065 - Wikiwand
Partial Solar Eclipse on February 5, 2065
Solar eclipse of July 3, 2065 - Alchetron, the free social encyclopedia
Solar eclipse of August 21, 2036 - Wikiwand
