Jump to content

Solar eclipse of August 12, 2064: Difference between revisions

From Wikipedia, the free encyclopedia
Content deleted Content added
m Saros 146: I corrected the spelling of "August." WP:TYPO
Line 42: Line 42:


=== Saros 146 ===
=== Saros 146 ===
{{Solar Saros series 146}}
It is a part of [[Solar Saros 146|Saros cycle 146]], repeating every 18 years, 11 days, containing 76 events. The series started with partial solar eclipse on September 19, 1541. It contains total eclipses from May 29, 1938, through October 7, 2154, hybrid eclipses from October 17, 2172, through November 20, 2226, and annular eclipses from December 1, 2244, through August 10, 2659. The series ends at member 76 as a partial eclipse on December 29, 2893. The longest duration of totality was 5 minutes, 21 seconds on [[Solar eclipse of June 30, 1992|June 30, 1992]].
{| class="wikitable collapsible collapsed"
!colspan=3|Series members 21-37 occur between 1901 and 2200:
|-
!21
!22
!23
|- style="text-align:center;"
|[[File:SE1902May07P.png|150px]]<BR>[[solar eclipse of May 7, 1902|May 7, 1902]]
|[[File:SE1920May18P.png|150px]]<BR>[[solar eclipse of May 18, 1920|May 18, 1920]]
|[[File:SE1938May29T.png|150px]]<BR>[[solar eclipse of May 29, 1938|May 29, 1938]]
|-
!24
!25
!26
|- style="text-align:center;"
|[[File:SE1956Jun08T.png|150px]]<BR>[[solar eclipse of June 8, 1956|June 8, 1956]]
|[[File:SE1974Jun20T.png|150px]]<BR>[[solar eclipse of June 20, 1974|June 20, 1974]]
|[[File:SE1992Jun30T.png|150px]]<BR>[[solar eclipse of June 30, 1992|June 30, 1992]]
|-
!27
!28
!29
|- style="text-align:center;"
|[[File:SE2010Jul11T.png|150px]]<BR>[[solar eclipse of July 11, 2010|July 11, 2010]]
|[[File:SE2028Jul22T.png|150px]]<BR>[[solar eclipse of July 22, 2028|July 22, 2028]]
|[[File:SE2046Aug02T.png|150px]]<BR>[[solar eclipse of August 2, 2046|August 2, 2046]]
|-
!30
!31
!32
|- style="text-align:center;"
|[[File:SE2064Aug12T.png|150px]]<BR>[[solar eclipse of August 12, 2064|August 12, 2064]]
|[[File:SE2082Aug24T.png|150px]]<BR>[[solar eclipse of August 24, 2082|August 24, 2082]]
|[[File:SE2100Sep04T.png|150px]]<BR>[[solar eclipse of September 4, 2100|September 4, 2100]]
|-
!33
!34
!35
|- style="text-align:center;"
|[[File:SE2118Sep15T.png|150px]]<BR>September 15, 2118
|[[File:SE2136Sep26T.png|150px]]<BR>September 26, 2136
|[[File:SE2154Oct07T.png|150px]]<BR>October 7, 2154
|-
!36
!37
|- style="text-align:center;"
|[[File:SE2172Oct17H.png|150px]]<BR>October 17, 2172
|[[File:SE2190Oct29H.png|150px]]<BR>October 29, 2190
|}<noinclude>


=== Inex series ===
=== Inex series ===

Revision as of 02:16, 14 July 2024

Solar eclipse of August 12, 2064
Map
Type of eclipse
NatureTotal
Gamma−0.4652
Magnitude1.0495
Maximum eclipse
Duration268 s (4 min 28 s)
Coordinates10°54′S 96°00′W / 10.9°S 96°W / -10.9; -96
Max. width of band184 km (114 mi)
Times (UTC)
Greatest eclipse17:46:06
References
Saros146 (30 of 76)
Catalog # (SE5000)9651

A total solar eclipse will occur at the Moon's descending node of orbit on Tuesday, August 12, 2064, with a magnitude of 1.0495. 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. This eclipse will pass through the Chilean cities of Valparaíso and the capital Santiago.

Eclipses in 2064

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 146

Inex

Triad

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.[1]

The partial solar eclipses on July 3, 2065 and December 27, 2065 occur in the next lunar year eclipse set.

Solar eclipse series sets from 2062 to 2065
Ascending node   Descending node
Saros Map Gamma Saros Map Gamma
121 March 11, 2062

Partial
−1.0238 126 September 3, 2062

Partial
1.0191
131 February 28, 2063

Annular
−0.336 136 August 24, 2063

Total
0.2771
141 February 17, 2064

Annular
0.3597 146 August 12, 2064

Total
−0.4652
151 February 5, 2065

Partial
1.0336 156 August 2, 2065

Partial
−1.2759

Saros 146

This eclipse is a part of Saros series 146, repeating every 18 years, 11 days, and containing 76 events. The series started with a partial solar eclipse on September 19, 1541. It contains total eclipses from May 29, 1938 through October 7, 2154; hybrid eclipses from October 17, 2172 through November 20, 2226; and annular eclipses from November 30, 2244 through August 10, 2659. The series ends at member 76 as a partial eclipse on December 29, 2893. 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 was produced by member 26 at 5 minutes, 21 seconds on June 30, 1992, and the longest duration of annularity will be produced by member 63 at 3 minutes, 30 seconds on August 10, 2659. All eclipses in this series occur at the Moon’s descending node of orbit.[2]

Series members 16–37 occur between 1801 and 2200:
16 17 18

March 13, 1812

March 24, 1830

April 3, 1848
19 20 21

April 15, 1866

April 25, 1884

May 7, 1902
22 23 24

May 18, 1920

May 29, 1938

June 8, 1956
25 26 27

June 20, 1974

June 30, 1992

July 11, 2010
28 29 30

July 22, 2028

August 2, 2046

August 12, 2064
31 32 33

August 24, 2082

September 4, 2100

September 15, 2118
34 35 36

September 26, 2136

October 7, 2154

October 17, 2172
37

October 29, 2190

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.

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.

22 eclipse events between June 1, 2011 and October 24, 2098
May 31–June 1 March 19–20 January 5–6 October 24–25 August 12–13
118 120 122 124 126

June 1, 2011

March 20, 2015

January 6, 2019

October 25, 2022

August 12, 2026
128 130 132 134 136

June 1, 2030

March 20, 2034

January 5, 2038

October 25, 2041

August 12, 2045
138 140 142 144 146

May 31, 2049

March 20, 2053

January 5, 2057

October 24, 2060

August 12, 2064
148 150 152 154 156

May 31, 2068

March 19, 2072

January 6, 2076

October 24, 2079

August 13, 2083
158 160 162 164

June 1, 2087

October 24, 2098

Notes

  1. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  2. ^ "NASA - Catalog of Solar Eclipses of Saros 146". eclipse.gsfc.nasa.gov.

References