March 1978 lunar eclipse
{{Short description|Total lunar eclipse March 24, 1978}}
{{Use dmy dates|date=January 2019}}
{{Infobox lunar eclipse
| type = total
| image = Lunar eclipse chart close-1978Mar24.png
| caption = The Moon's hourly motion shown right to left
| date = March 24, 1978
| gamma = −0.2140
| magnitude = 1.4518
| saros_ser = 122
| saros_no = 54 of 75
| totality = 90 minutes, 40 seconds
| partiality = 218 minutes, 33 seconds
| penumbral = 344 minutes, 56 seconds
| p1 = 13:29:51
| u1 = 14:33:07
| u2 = 15:37:03
| greatest = 16:22:22
| u3 = 17:07:43
| u4 = 18:11:40
| p4 = 19:14:47
| previous = September 1977
| next = September 1978
}}
A total lunar eclipse occurred at the Moon’s ascending node of orbit on Friday, March 24, 1978,{{cite web|title=March 24–25, 1978 Total Lunar Eclipse (Blood Moon)|url=https://www.timeanddate.com/eclipse/lunar/1978-march-24|publisher=timeanddate|access-date=4 January 2025}} with an umbral magnitude of 1.4518. It was a central lunar eclipse, in which part of the Moon passed through the center of the Earth's shadow. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. 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. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. The Moon's apparent diameter was near the average diameter because it occurred 7.1 days after apogee (on March 17, 1978, at 14:25 UTC) and 6.6 days before perigee (on March 31, 1978, at 5:45 UTC).{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=1978&n=136|publisher=timeanddate|access-date=4 January 2025}}
Visibility
The eclipse was completely visible over much of Asia and Australia, seen rising over Africa, Europe, and west and central Asia and setting over western North America and the central Pacific Ocean.{{cite web|title=Total Lunar Eclipse of 1978 Mar 24|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot1951/LE1978Mar24T.pdf|publisher=NASA|access-date=4 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=Total Lunar Eclipse of 1978 Mar 24|url=https://eclipsewise.com/lunar/LEprime/1901-2000/LE1978Mar24Tprime.html|publisher=EclipseWise.com|access-date=4 January 2025}}
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|+March 24, 1978 Lunar Eclipse Parameters ! Parameter ! Value |
Penumbral Magnitude
| 2.47900 |
Umbral Magnitude
| 1.45179 |
Gamma
| −0.21402 |
Sun Right Ascension
| 00h13m28.3s |
Sun Declination
| +01°27'32.7" |
Sun Semi-Diameter
| 16'02.4" |
Sun Equatorial Horizontal Parallax
| 08.8" |
Moon Right Ascension
| 12h13m13.4s |
Moon Declination
| -01°39'13.7" |
Moon Semi-Diameter
| 15'36.9" |
Moon Equatorial Horizontal Parallax
| 0°57'18.4" |
ΔT
| 48.8 s |
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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 March–April 1978 ! March 24 | |
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| Total lunar eclipse | Partial solar eclipse Solar Saros 148 |
Related eclipses
= Eclipses in 1978 =
- A total lunar eclipse on March 24.
- A partial solar eclipse on April 7.
- A total lunar eclipse on September 16.
- A partial solar eclipse on October 2.
= Metonic =
- Preceded by: Lunar eclipse of June 4, 1974
- Followed by: Lunar eclipse of January 9, 1982
= Tzolkinex =
- Preceded by: Lunar eclipse of February 10, 1971
- Followed by: Lunar eclipse of May 4, 1985
= Half-Saros =
- Preceded by: Solar eclipse of March 18, 1969
- Followed by: Solar eclipse of March 29, 1987
= Tritos =
- Preceded by: Lunar eclipse of April 24, 1967
- Followed by: Lunar eclipse of February 20, 1989
= Lunar Saros 122 =
- Preceded by: Lunar eclipse of March 13, 1960
- Followed by: Lunar eclipse of April 4, 1996
= Inex =
- Preceded by: Lunar eclipse of April 13, 1949
- Followed by: Lunar eclipse of March 3, 2007
= Triad =
- Preceded by: Lunar eclipse of May 23, 1891
- Followed by: Lunar eclipse of January 22, 2065
= Lunar eclipses of 1977–1980 =
{{Lunar eclipse set 1977-1980}}
= Saros 122 =
{{Lunar Saros series 122}}
= Tritos series =
{{Lunar Tritos series January 2000}}
= Inex series =
{{Lunar Inex series March 2007}}
= 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 solar eclipses of Solar Saros 129.
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See also
Notes
{{reflist}}
External links
- {{LEplot1951 link|1978|Mar|24|T}}
{{Lunar eclipses}}
{{DEFAULTSORT:Lunar eclipse 1978-03}}