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September 1933 lunar eclipse

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Penumbral lunar eclipse September 4 1933
September 1933 lunar eclipse
Penumbral eclipse
The Moon's hourly motion shown right to left
DateSeptember 4, 1933
Gamma1.1776
Magnitude−0.3012
Saros cycle146 (6 of 72)
Penumbral221 minutes, 24 seconds
Contacts (UTC)
P13:01:11
Greatest4:51:56
P46:42:34
← August 1933January 1934 →

A penumbral lunar eclipse will occur at the Moon’s ascending node of orbit on Monday, September 4, 1933, with an umbral magnitude of −0.7336. 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 3.9 days after perigee (on August 31, 1933, at 6:30 UTC), the Moon's apparent diameter was larger.

This eclipse was the last of four penumbral lunar eclipses in 1933, with the others occurring on February 10, March 12, and August 5.

Visibility

The eclipse was completely visible over much of North and South America, seen rising over northwestern North America and the central Pacific Ocean and setting over Africa and Europe.

Eclipse details

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

September 4, 1933 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.69558
Umbral Magnitude −0.30117
Gamma 1.17763
Sun Right Ascension 10h50m36.8s
Sun Declination +07°22'09.8"
Sun Semi-Diameter 15'51.8"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 22h48m27.5s
Moon Declination -06°21'19.9"
Moon Semi-Diameter 15'54.9"
Moon Equatorial Horizontal Parallax 0°58'24.5"
ΔT 23.9 s

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.

Eclipse season of August–September 1933
August 5
Ascending node (full moon)
August 21
Descending node (new moon)
September 4
Ascending node (full moon)
Penumbral lunar eclipse
Lunar Saros 108
Annular solar eclipse
Solar Saros 134
Penumbral lunar eclipse
Lunar Saros 146

Related eclipses

Eclipses in 1933

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 146

Inex

Triad

Lunar eclipses of 1930–1933

Lunar eclipse series sets from 1930–1933
Descending node   Ascending node
Saros Date
viewing
Type
chart
Saros Date
viewing
Type
chart
111 1930 Apr 13
Partial
116 1930 Oct 07
Partial
121 1931 Apr 02
Total
126 1931 Sep 26
Total
131 1932 Mar 22
Partial
136 1932 Sep 14
Partial
141 1933 Mar 12
Penumbral
146 1933 Sep 04
Penumbral

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros). This lunar eclipse is related to two total solar eclipses of Solar Saros 153.

August 30, 1924 September 10, 1942

See also

External links

Lunar eclipses
Lists of lunar eclipses
Lunar eclipses
by era
Lunar eclipses
by saros series
August 2017 lunar eclipse
Partial eclipses
May 2022 lunar eclipse
Total eclipses
February 2017 lunar eclipse
Penumbral eclipses
Partial
Total
Related
  • Category
  • symbol denotes next eclipse in series
Stub icon

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  1. "September 3–4, 1933 Penumbral Lunar Eclipse". timeanddate. Retrieved 16 December 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 16 December 2024.
  3. "Penumbral Lunar Eclipse of 1933 Sep 04" (PDF). NASA. Retrieved 16 December 2024.
  4. "Penumbral Lunar Eclipse of 1933 Sep 04". EclipseWise.com. Retrieved 16 December 2024.
  5. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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