Solar eclipse of October 13, 2061

Future annular solar eclipse
62°06′S 54°24′W / 62.1°S 54.4°W / -62.1; -54.4Max. width of band743 km (462 mi)Times (UTC)Greatest eclipse10:32:10ReferencesSaros154 (9 of 71)Catalog # (SE5000)9645

An annular solar eclipse will occur at the Moon's descending node of orbit on Thursday, October 13, 2061, with a magnitude of 0.9469. 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.

Related eclipses

Eclipses in 2061

Metonic

Tzolkinex

Half-Saros

  • Preceded by: Lunar eclipse of October 8, 2052
  • Followed by: Lunar eclipse of October 19, 2070

Tritos

Solar Saros 154

Inex

Triad

Solar eclipses of 2058–2061

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]

Solar eclipses 2059 to 2061
119 May 22, 2058

Partial
124 November 16, 2058

Partial
129 May 11, 2059

Total
134 November 5, 2059

Annular
139 April 30, 2060

Total
144 October 24, 2060

Annular
149 April 20, 2061

Total
154 October 13, 2061

Annular

Saros 154

It is a part of Saros cycle 154, repeating every 18 years, 11 days, containing 71 events. The series started with a partial solar eclipse on July 19, 1917. It contains annular eclipses from October 3, 2043, through March 27, 2332, hybrid eclipses from April 7, 2350, through April 29, 2386, and total eclipses from May 9, 2404, through May 29, 3035. The series ends at member 71 as a partial eclipse on August 25, 3179. The longest duration of totality will be 4 minutes, 50 seconds on July 25, 2530.

Series members 1-16 occur between 1901 and 2200:
1 2 3

July 19, 1917

July 30, 1935

August 9, 1953
4 5 6

August 20, 1971

August 31, 1989

September 11, 2007
7 8 9

September 21, 2025

October 3, 2043

October 13, 2061
10 11 12

October 24, 2079

November 4, 2097

November 16, 2115
13 14 15

November 26, 2133

December 8, 2151

December 18, 2169
16

December 29, 2187

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.[2]

Octon series with 21 events between May 21, 1993 and August 2, 2065
May 20–21 March 8–9 December 25–26 October 13–14 August 1–2
98 100 102 104 106
May 21, 1955 March 9, 1959 December 26, 1962 October 14, 1966 August 2, 1970
108 110 112 114 116
May 21, 1974 March 9, 1978 December 26, 1981 October 14, 1985 August 1, 1989
118 120 122 124 126

May 21, 1993

March 9, 1997

December 25, 2000

October 14, 2004

August 1, 2008
128 130 132 134 136

May 20, 2012

March 9, 2016

December 26, 2019

October 14, 2023

August 2, 2027
138 140 142 144 146

May 21, 2031

March 9, 2035

December 26, 2038

October 14, 2042

August 2, 2046
148 150 152 154 156

May 20, 2050

March 9, 2054

December 26, 2057

October 13, 2061

August 2, 2065
158 160 162 164 166

May 20, 2069
March 8, 2073 December 26, 2076 October 13, 2080 August 1, 2084

References

  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. ^ Note S1: Eclipses & Predictions in Freeth, Tony (2014). "Eclipse Prediction on the Ancient Greek Astronomical Calculating Machine Known as the Antikythera Mechanism". PLOS ONE. 9 (7): e103275. Bibcode:2014PLoSO...9j3275F. doi:10.1371/journal.pone.0103275. PMC 4116162. PMID 25075747.

External links

  • http://eclipse.gsfc.nasa.gov/SEplot/SEplot2051/SE2061Oct13A.GIF
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