- Source: Solar eclipse of March 30, 2033
A total solar eclipse will occur at the Moon's descending node of orbit on Wednesday, March 30, 2033, with a magnitude of 1.0462. 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 11 hours after perigee (on March 30, 2033, at 7:10 UTC), the Moon's apparent diameter will be larger.
Totality will be visible from parts of the Russian Far East and Alaska, including in the cities of Nome, Alaska and Utqiaġvik, Alaska in the mid-morning hours. A partial eclipse will be visible for parts of eastern Russia, Hawaii, North America, Greenland, and Iceland. This will be the last of 55 umbral eclipses in Solar Saros 120.
Images
Animated path
Details of totality in some places or cities
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 2033
=A total solar eclipse on March 30.
A total lunar eclipse on April 14.
A partial solar eclipse on September 23.
A total lunar eclipse on October 8.
= Metonic
=Preceded by: Solar eclipse of June 12, 2029
Followed by: Solar eclipse of January 16, 2037
= Tzolkinex
=Preceded by: Solar eclipse of February 17, 2026
Followed by: Solar eclipse of May 11, 2040
= Half-Saros
=Preceded by: Lunar eclipse of March 25, 2024
Followed by: Lunar eclipse of April 5, 2042
= Tritos
=Preceded by: Solar eclipse of April 30, 2022
Followed by: Solar eclipse of February 28, 2044
= Solar Saros 120
=Preceded by: Solar eclipse of March 20, 2015
Followed by: Solar eclipse of April 11, 2051
= Inex
=Preceded by: Solar eclipse of April 19, 2004
Followed by: Solar eclipse of March 11, 2062
= Triad
=Preceded by: Solar eclipse of May 30, 1946
Followed by: Solar eclipse of January 30, 2120
= Solar eclipses of 2033–2036
=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 July 23, 2036 occurs in the next lunar year eclipse set.
= Saros 120
=This eclipse is a part of Saros series 120, repeating every 18 years, 11 days, and containing 71 events. The series started with a partial solar eclipse on May 27, 933 AD. It contains annular eclipses from August 11, 1059 through April 26, 1492; hybrid eclipses from May 8, 1510 through June 8, 1564; and total eclipses from June 20, 1582 through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. 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 11 at 6 minutes, 24 seconds on September 11, 1113, and the longest duration of totality was produced by member 60 at 2 minutes, 50 seconds on March 9, 1997. 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 April 8, 1902 (part of Saros 108) and January 5, 1935 (part of Saros 111) 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
http://eclipse.gsfc.nasa.gov/SEplot/SEplot2001/SE2033Mar30T.GIF
Kata Kunci Pencarian:
- Daftar gerhana matahari pada abad ke-21
- Solar eclipse of March 30, 2033
- March 2024 lunar eclipse
- Solar eclipse of March 20, 2015
- Solar eclipse of April 30, 2022
- List of solar eclipses visible from the United States
- Solar eclipse of April 8, 2024
- Solar eclipse of March 30, 2052
- Solar eclipse of August 12, 2026
- Solar eclipse of August 23, 2044
- List of solar eclipses visible from Russia
