- Source: Solar eclipse of October 14, 2042
An annular solar eclipse will occur at the Moon's descending node of orbit on Tuesday, October 14, 2042, with a magnitude of 0.93. 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 9 hours before apogee (on October 14, 2042, at 11:00 UTC), the Moon's apparent diameter will be smaller.
The path of annularity will be visible from parts of the Andaman and Nicobar Islands, southern Thailand, Malaysia, Indonesia, East Timor, Australia, and New Zealand. A partial solar eclipse will be visible for parts of South Asia, Southeast Asia, Australia, Oceania, and Antarctica.
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.
Related eclipses
= Eclipses in 2042
=A penumbral lunar eclipse on April 5.
A total solar eclipse on April 20.
A penumbral lunar eclipse on September 29.
An annular solar eclipse on October 14.
= Metonic
=Preceded by: Solar eclipse of December 26, 2038
Followed by: Solar eclipse of August 2, 2046
= Tzolkinex
=Preceded by: Solar eclipse of September 2, 2035
Followed by: Solar eclipse of November 25, 2049
= Half-Saros
=Preceded by: Lunar eclipse of October 8, 2033
Followed by: Lunar eclipse of October 19, 2051
= Tritos
=Preceded by: Solar eclipse of November 14, 2031
Followed by: Solar eclipse of September 12, 2053
= Solar Saros 144
=Preceded by: Solar eclipse of October 2, 2024
Followed by: Solar eclipse of October 24, 2060
= Inex
=Preceded by: Solar eclipse of November 3, 2013
Followed by: Solar eclipse of September 23, 2071
= Triad
=Preceded by: Solar eclipse of December 14, 1955
Followed by: Solar eclipse of August 15, 2129
= Solar eclipses of 2040–2043
=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.
= Saros 144
=This eclipse is a part of Saros series 144, repeating every 18 years, 11 days, and containing 70 events. The series started with a partial solar eclipse on April 11, 1736. It contains annular eclipses from July 7, 1880 through August 27, 2565. There are no hybrid or total eclipses in this set. The series ends at member 70 as a partial eclipse on May 5, 2980. 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 51 at 9 minutes, 52 seconds on December 29, 2168. 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/SEplot2001/SE2042Oct14A.GIF
Kata Kunci Pencarian:
- Daftar gerhana matahari pada abad ke-21
- Solar eclipse of October 14, 2042
- October 14 solar eclipse
- Solar eclipse of October 2, 2024
- Solar eclipse of November 14, 2031
- Solar eclipse of October 14, 2023
- List of solar eclipses visible from Australia
- Solar eclipse of April 20, 2042
- Solar eclipse of April 8, 2024
- Solar eclipse of April 20, 2023
- Solar eclipse of March 29, 2025
