September 1969 lunar eclipse
{{Short description|Penumbral lunar eclipse September 25 1969}}
{{Infobox lunar eclipse
| type = penumbral
| image = Lunar eclipse chart close-1969Sep25.png
| caption = The Moon's hourly motion shown right to left
| date = September 25, 1969
| gamma = 1.0656
| magnitude = −0.0952
| saros_ser = 146
| saros_no = 8 of 72
| penumbral = 245 minutes, 9 seconds
| p1 = 18:07:03
| greatest = 20:09:39
| p4 = 22:12:12
| previous = August 1969
| next = February 1970
}}
A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, September 25, 1969,{{cite web|title=September 25–26, 1969 Penumbral Lunar Eclipse|url=https://www.timeanddate.com/eclipse/lunar/1969-september-25|publisher=timeanddate|access-date=2 January 2025}} with an umbral magnitude of −0.0952. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A penumbral lunar eclipse occurs when part or all of the Moon's near side passes into 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 after perigee (on September 22, 1969, at 11:45 UTC), the Moon's apparent diameter was larger.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=1969&n=136|publisher=timeanddate|access-date=2 January 2025}}
Visibility
The eclipse was completely visible over Europe, Africa, and Asia, seen rising over eastern South America and west Africa and setting over northeast Asia and Australia.{{cite web|title=Penumbral Lunar Eclipse of 1969 Sep 25|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot1951/LE1969Sep25N.pdf|publisher=NASA|access-date=2 January 2025}}
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Eclipse details
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.{{cite web|title=Penumbral Lunar Eclipse of 1969 Sep 25|url=https://eclipsewise.com/lunar/LEprime/1901-2000/LE1969Sep25Nprime.html|publisher=EclipseWise.com|access-date=2 January 2025}}
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|+September 25, 1969 Lunar Eclipse Parameters ! Parameter ! Value |
Penumbral Magnitude
| 0.90080 |
Umbral Magnitude
| −0.09519 |
Gamma
| 1.06558 |
Sun Right Ascension
| 12h09m26.5s |
Sun Declination
| -01°01'23.8" |
Sun Semi-Diameter
| 15'57.2" |
Sun Equatorial Horizontal Parallax
| 08.8" |
Moon Right Ascension
| 00h07m25.1s |
Moon Declination
| +01°56'11.3" |
Moon Semi-Diameter
| 16'01.1" |
Moon Equatorial Horizontal Parallax
| 0°58'47.2" |
ΔT
| 39.9 s |
{{clear}}
Eclipse season
{{See also|Eclipse cycle}}
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. The first and last eclipse in this sequence is separated by one synodic month.
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|+ Eclipse season of August–September 1969 ! August 27 | ||
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| Penumbral lunar eclipse | Annular solar eclipse Solar Saros 134 | Penumbral lunar eclipse Lunar Saros 146 |
Related eclipses
= Eclipses in 1969 =
- An annular solar eclipse on March 18.
- A penumbral lunar eclipse on April 2.
- A penumbral lunar eclipse on August 27.
- An annular solar eclipse on September 11.
- A penumbral lunar eclipse on September 25.
= Metonic =
- Preceded by: Lunar eclipse of December 8, 1965
- Followed by: Lunar eclipse of July 15, 1973
= Tzolkinex =
- Preceded by: Lunar eclipse of August 15, 1962
- Followed by: Lunar eclipse of November 6, 1976
= Half-Saros =
- Preceded by: Solar eclipse of September 20, 1960
- Followed by: Solar eclipse of October 2, 1978
= Tritos =
- Preceded by: Lunar eclipse of October 27, 1958
- Followed by: Lunar eclipse of August 26, 1980
= Lunar Saros 146 =
- Preceded by: Lunar eclipse of September 15, 1951
- Followed by: Lunar eclipse of October 7, 1987
= Inex =
- Preceded by: Lunar eclipse of October 16, 1940
- Followed by: Lunar eclipse of September 6, 1998
= Triad =
- Preceded by: Lunar eclipse of November 25, 1882
- Followed by: Lunar eclipse of July 26, 2056
= Lunar eclipses of 1966–1969 =
{{Lunar eclipse set 1966–1969}}
= Saros 146 =
{{Lunar Saros series 146}}
= Tritos series =
{{Lunar Tritos series June 2002}}
= Inex series =
{{Lunar Inex series August 2027}}
= Half-Saros cycle =
A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros This lunar eclipse is related to two partial solar eclipses of Solar Saros 153.
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See also
Notes
{{reflist}}
External links
- {{LEplot1951 link|1969|Sep|25|N}}
{{Lunar eclipses}}
{{DEFAULTSORT:Lunar eclipse 1969-09}}
{{lunar-eclipse-stub}}