November 1974 lunar eclipse
total
DateNovember 29, 1974
Gamma0.3054
Magnitude1.2896
Saros ser125
Saros no46 of 72
Totality75 minutes, 45 seconds
Partiality208 minutes, 57 seconds
Penumbral333 minutes, 4 seconds
P 112:26:47
U 113:28:55
U 214:35:31
Greatest15:13:22
U 315:51:15
U 416:57:52
P 417:59:52
PreviousJune 1974
NextMay 1975

A total lunar eclipse occurred at the Moon’s descending node of orbit on Friday, November 29, 1974,[1] with an umbral magnitude of 1.2896. 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. Occurring about 3.6 days before perigee (on December 3, 1974, at 6:40 UTC), the Moon's apparent diameter was larger.[2]

Visibility

The eclipse was completely visible over Asia, Australia, and Alaska, seen rising over much of Africa, Europe, and the Middle East and setting over much of North America and the eastern Pacific Ocean.[3]

Eclipse details

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

November 29, 1974 Lunar Eclipse Parameters
ParameterValue
Penumbral Magnitude2.30575
Umbral Magnitude1.28961
Gamma0.30540
Sun Right Ascension16h20m46.5s
Sun Declination-21°29'03.2"
Sun Semi-Diameter16'13.0"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension04h20m41.2s
Moon Declination+21°46'53.8"
Moon Semi-Diameter15'57.5"
Moon Equatorial Horizontal Parallax0°58'34.1"
ΔT45.3 s

Eclipse season

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 November–December 1974
November 29
Descending node (full moon)
December 13
Ascending node (new moon)
Total lunar eclipse
Lunar Saros 125
Partial solar eclipse
Solar Saros 151

Eclipses in 1974

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 125

Inex

Triad

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[5] This lunar eclipse is related to two annular solar eclipses of Solar Saros 132.

November 23, 1965December 4, 1983

See also

Notes

  1. ^ "November 29–30, 1974 Total Lunar Eclipse (Blood Moon)". timeanddate. Retrieved 4 January 2025.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 4 January 2025.
  3. ^ "Total Lunar Eclipse of 1974 Nov 29". NASA. Retrieved 4 January 2025.
  4. ^ "Total Lunar Eclipse of 1974 Nov 29". EclipseWise.com. Retrieved 4 January 2025.
  5. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros