June 1965 lunar eclipse

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Template:Short description Template:Infobox lunar eclipse A partial lunar eclipse occurred at the Moon’s descending node of orbit on Monday, June 14, 1965,[1] with an umbral magnitude of 0.1767. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A partial lunar eclipse occurs when one part of the Moon is in the Earth's umbra, while the other part is in the Earth's penumbra. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. Occurring about 3.4 days before apogee (on June 17, 1965, at 10:50 UTC), the Moon's apparent diameter was smaller.[2]

Visibility

The eclipse was completely visible over South America, west and southern Africa, and Antarctica, seen rising over North America and the eastern Pacific Ocean and setting over Europe, northeast Africa, and west, central, and south Asia.[3]

File:Lunar eclipse from moon-1965Jun14.png File:Lunar eclipse chart close-1965Jun14.png

Eclipse details

Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]

June 14, 1965 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 1.23505
Umbral Magnitude 0.17670
Gamma −0.90055
Sun Right Ascension 05h28m37.7s
Sun Declination +23°14'54.4"
Sun Semi-Diameter 15'44.8"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 17h28m04.9s
Moon Declination -24°03'29.9"
Moon Semi-Diameter 14'52.7"
Moon Equatorial Horizontal Parallax 0°54'36.3"
ΔT 36.1 s

Eclipse season

Script error: No such module "Labelled list hatnote". 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.

Eclipse season of May–June 1965
May 30
Ascending node (new moon)
June 14
Descending node (full moon)
File:SE1965May30T.png File:Lunar eclipse chart close-1965Jun14.png
Total solar eclipse
Solar Saros 127
Partial lunar eclipse
Lunar Saros 139

Related eclipses

Eclipses in 1965

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 139

Inex

Triad

Lunar eclipses of 1962–1965

This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[5]

The penumbral lunar eclipses on February 19, 1962 and August 15, 1962 occur in the previous lunar year eclipse set.

Lunar eclipse series sets from 1962 to 1965
Descending node   Ascending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
109 1962 Jul 17
File:Lunar eclipse from moon-1962Jul17.png
Penumbral
File:Lunar eclipse chart close-1962Jul17.png
1.3371 114 1963 Jan 09
File:Lunar eclipse from moon-1963Jan09.png
Penumbral
File:Lunar eclipse chart close-1963Jan09.png
−1.0128
119 1963 Jul 06
File:Lunar eclipse from moon-1963Jul06.png
Partial
File:Lunar eclipse chart close-1963Jul06.png
0.6197 124 1963 Dec 30
File:Lunar eclipse from moon-1963Dec30.png
Total
File:Lunar eclipse chart close-1963Dec30.png
−0.2889
129 1964 Jun 25
File:Lunar eclipse from moon-1964Jun25.png
Total
File:Lunar eclipse chart close-1964Jun25.png
−0.1461 134 1964 Dec 19
File:Lunar eclipse from moon-1964Dec19.png
Total
File:Lunar eclipse chart close-1964Dec19.png
0.3801
139 1965 Jun 14
File:Lunar eclipse from moon-1965Jun14.png
Partial
File:Lunar eclipse chart close-1965Jun14.png
−0.9006 144 1965 Dec 08
File:Lunar eclipse from moon-1965Dec08.png
Penumbral
File:Lunar eclipse chart close-1965Dec08.png
1.0775

Saros 139

Template:Lunar Saros series 139

Tritos series

Template:Lunar Tritos series February 2009

Inex series

Template:Lunar Inex series May 2023

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[6] This lunar eclipse is related to two total solar eclipses of Solar Saros 146.

June 8, 1956 June 20, 1974
File:SE1956Jun08T.png File:SE1974Jun20T.png

See also

Notes

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  1. ↑ Script error: No such module "citation/CS1".
  2. ↑ Script error: No such module "citation/CS1".
  3. ↑ Script error: No such module "citation/CS1".
  4. ↑ Script error: No such module "citation/CS1".
  5. ↑ Script error: No such module "citation/CS1".
  6. ↑ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

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External links

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