August 1969 lunar eclipse
Template:Short description Template:Infobox lunar eclipse A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Wednesday, August 27, 1969,[1] with an umbral magnitude of −0.9514. 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 2.25 days after perigee (on August 25, 1969, at 16:30 UTC), the Moon's apparent diameter was larger.[2]
This was the last lunar eclipse of Lunar Saros 108.
Visibility
The eclipse was completely visible over east and northeast Asia, Australia, western and central North America, western South America, and Antarctica.[3]
| File:Lunar eclipse from moon-1969Aug27.png File:Lunar eclipse chart close-1969Aug27.png |
Eclipse details
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.[4]
| Parameter | Value |
|---|---|
| Penumbral Magnitude | 0.01337 |
| Umbral Magnitude | −0.95141 |
| Gamma | −1.54066 |
| Sun Right Ascension | 10h23m30.2s |
| Sun Declination | +10°03'05.7" |
| Sun Semi-Diameter | 15'50.0" |
| Sun Equatorial Horizontal Parallax | 08.7" |
| Moon Right Ascension | 22h26m20.1s |
| Moon Declination | -11°25'58.1" |
| Moon Semi-Diameter | 16'24.7" |
| Moon Equatorial Horizontal Parallax | 1°00'13.8" |
| ΔT | 39.8 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. The first and last eclipse in this sequence is separated by one synodic month.
| August 27 Ascending node (full moon) |
September 11 Descending node (new moon) |
September 25 Ascending node (full moon) |
|---|---|---|
| File:Lunar eclipse chart close-1969Aug27.png | File:SE1969Sep11A.png | File:Lunar eclipse chart close-1969Sep25.png |
| Penumbral lunar eclipse Lunar Saros 108 |
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
- Followed by: Lunar eclipse of June 15, 1973
Tzolkinex
- Preceded by: Lunar eclipse of July 17, 1962
Lunar Saros 108
- Preceded by: Lunar eclipse of August 17, 1951
Inex
- Followed by: Lunar eclipse of August 8, 1998
Triad
- Followed by: Lunar eclipse of June 27, 2056
Lunar eclipses of 1969–1973
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 April 2, 1969 and September 25, 1969 occur in the previous lunar year eclipse set, and the lunar eclipses on June 15, 1973 (penumbral) and December 10, 1973 (partial) occur in the next lunar year eclipse set.
Saros 108
Template:Lunar Saros series 108
Tritos series
Template:Lunar Tritos series May 2002
Inex series
Template:Lunar Inex series July 2027
See also
Notes
<templatestyles src="Reflist/styles.css" />
Script error: No such module "Check for unknown parameters".
External links
- 1969 Aug 27 chart Eclipse Predictions by Fred Espenak, NASA/GSFC
Script error: No such module "Navbox".