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October 1958 lunar eclipse

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Penumbral lunar eclipse October 27, 1958
October 1958 lunar eclipse
Penumbral eclipse
The Moon's hourly motion shown right to left
DateOctober 27, 1958
Gamma−1.1571
Magnitude−0.3118
Saros cycle145 (8 of 71)
Penumbral257 minutes, 56 seconds
Contacts (UTC)
P113:18:19
Greatest15:27:17
P417:36:15
← May 1958March 1959 →

A penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Monday, October 27, 1958, with an umbral magnitude of −0.3118. 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 only about 15 hours after apogee (on October 27, 1958, at 0:20 UTC), the Moon's apparent diameter was smaller.

Visibility

The eclipse was completely visible over Asia and Australia, seen rising over much of Africa, Europe, and the Middle East and setting over western North America and the central Pacific Ocean.

Eclipse details

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

October 27, 1958 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.78251
Umbral Magnitude −0.31176
Gamma −1.15707
Sun Right Ascension 14h05m52.5s
Sun Declination -12°45'16.4"
Sun Semi-Diameter 16'05.8"
Sun Equatorial Horizontal Parallax 08.9"
Moon Right Ascension 02h06m54.9s
Moon Declination +11°44'42.3"
Moon Semi-Diameter 14'42.6"
Moon Equatorial Horizontal Parallax 0°53'59.2"
ΔT 32.6 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.

Eclipse season of October 1958
October 12
Ascending node (new moon)
October 27
Descending node (full moon)
Total solar eclipse
Solar Saros 133
Penumbral lunar eclipse
Lunar Saros 145

Related eclipses

Eclipses in 1958

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 145

Inex

Triad

Lunar eclipses of 1955–1958

Lunar eclipse series sets from 1955–1958
Ascending node   Descending node
Saros Date
viewing
Type
chart
Saros Date
viewing
Type
chart
110 1955 Jun 5
Penumbral
115 1955 Nov 29
Partial
120 1956 May 24
Partial
125 1956 Nov 18
Total
130 1957 May 13
Total
135 1957 Nov 7
Total
140 1958 May 3
Partial
145 1958 Oct 27
Penumbral
Last set 1954 Jul 16 Last set 1955 Jan 8
Next set 1958 Apr 4 Next set 1959 Sep 17

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 solar eclipses of Solar Saros 152.

October 21, 1949 November 2, 1967

See also

Notes

  1. "October 27–28, 1958 Penumbral Lunar Eclipse". timeanddate. Retrieved 25 December 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 25 December 2024.
  3. "Penumbral Lunar Eclipse of 1958 Oct 27" (PDF). NASA. Retrieved 25 December 2024.
  4. "Penumbral Lunar Eclipse of 1958 Oct 27". EclipseWise.com. Retrieved 25 December 2024.
  5. Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros

External links

Lunar eclipses
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Lunar eclipses
by era
Lunar eclipses
by saros series
August 2017 lunar eclipse
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May 2022 lunar eclipse
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Penumbral eclipses
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