February 1970 lunar eclipse
{{Short description|Partial lunar eclipse February 21, 1970}}
{{Infobox lunar eclipse
| type = partial
| image = Lunar eclipse chart close-1970Feb21.png
| caption = The Moon's hourly motion shown right to left
| date = February 21, 1970
| gamma = 0.9620
| magnitude = 0.0464
| saros_ser = 113
| saros_no = 61 of 71
| partiality = 52 minutes, 40 seconds
| penumbral = 298 minutes, 32 seconds
| p1 = 6:00:46
| u1 = 8:03:45
| greatest = 8:30:03
| u4 = 8:56:26
| p4 = 10:59:18
| previous = September 1969
| next = August 1970
}}
A partial lunar eclipse occurred at the Moon’s descending node of orbit on Saturday, February 21, 1970,{{cite web|title=February 20–21, 1970 Partial Lunar Eclipse|url=https://www.timeanddate.com/eclipse/lunar/1970-february-21|publisher=timeanddate|access-date=3 January 2025}} with an umbral magnitude of 0.0464. 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 2.4 days after apogee (on February 18, 1970, at 23:05 UTC), the Moon's apparent diameter was smaller.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=1970&n=136|publisher=timeanddate|access-date=3 January 2025}}
Visibility
The eclipse was completely visible over northeast Asia, North America, and northwestern South America, seen rising over east Asia and Australia and setting over much of South America, western Europe, and west Africa.{{cite web|title=Partial Lunar Eclipse of 1970 Feb 21|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot1951/LE1970Feb21P.pdf|publisher=NASA|access-date=3 January 2025}}
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Eclipse details
Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse.{{cite web|title=Partial Lunar Eclipse of 1970 Feb 21|url=https://eclipsewise.com/lunar/LEprime/1901-2000/LE1970Feb21Pprime.html|publisher=EclipseWise.com|access-date=3 January 2025}}
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|+February 21, 1970 Lunar Eclipse Parameters ! Parameter ! Value |
Penumbral Magnitude
| 1.14027 |
Umbral Magnitude
| 0.04639 |
Gamma
| 0.96198 |
Sun Right Ascension
| 22h17m07.7s |
Sun Declination
| -10°39'28.9" |
Sun Semi-Diameter
| 16'10.2" |
Sun Equatorial Horizontal Parallax
| 08.9" |
Moon Right Ascension
| 10h18m43.4s |
Moon Declination
| +11°26'05.5" |
Moon Semi-Diameter
| 14'47.0" |
Moon Equatorial Horizontal Parallax
| 0°54'15.2" |
ΔT
| 40.3 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.
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|+ Eclipse season of February–March 1970 ! February 21 | |
200px | 200px |
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| Partial lunar eclipse | Total solar eclipse Solar Saros 139 |
Related eclipses
= Eclipses in 1970 =
- A partial lunar eclipse on February 21.
- A total solar eclipse on March 7.
- A partial lunar eclipse on August 17.
- An annular solar eclipse on August 31.
= Metonic =
- Preceded by: Lunar eclipse of May 4, 1966
- Followed by: Lunar eclipse of December 10, 1973
= Tzolkinex =
- Preceded by: Lunar eclipse of January 9, 1963
- Followed by: Lunar eclipse of April 4, 1977
= Half-Saros =
- Preceded by: Solar eclipse of February 15, 1961
- Followed by: Solar eclipse of February 26, 1979
= Tritos =
- Preceded by: Lunar eclipse of March 24, 1959
- Followed by: Lunar eclipse of January 20, 1981
= Lunar Saros 113 =
- Preceded by: Lunar eclipse of February 11, 1952
- Followed by: Lunar eclipse of March 3, 1988
= Inex =
- Preceded by: Lunar eclipse of March 13, 1941
- Followed by: Lunar eclipse of January 31, 1999
= Triad =
- Preceded by: Lunar eclipse of April 22, 1883
- Followed by: Lunar eclipse of December 22, 2056
= Lunar eclipses of 1969–1973 =
{{Lunar eclipse set 1969–1973}}
= Metonic series =
{{Metonic lunar eclipse 1951–2027}}
= Saros 113 =
{{Lunar Saros series 113}}
= Tritos series =
{{Lunar Tritos series November 2002}}
= Inex series =
{{Lunar Inex series January 2028}}
= 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 total solar eclipses of Solar Saros 120.
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See also
Notes
{{reflist}}
External links
- {{LEplot1951 link|1970|Feb|21|P}}
{{Lunar eclipses}}
{{DEFAULTSORT:Lunar eclipse 1970-02}}