May 1958 lunar eclipse

May 1958 lunar eclipse
Partial eclipse
The Moon's hourly motion shown right to left
DateMay 3, 1958
Gamma1.0188
Magnitude0.0092
Saros cycle140 (22 of 80)
Partiality21 minutes, 2 seconds
Penumbral242 minutes, 13 seconds
Contacts (UTC)
P110:11:48
U112:02:22
Greatest12:12:57
U412:23:24
P414:14:01

A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Saturday, May 3, 1958,[1] with an umbral magnitude of 0.0092. 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 1.2 days after perigee (on May 2, 1958, at 7:00 UTC), the Moon's apparent diameter was larger.[2]

Visibility

The eclipse was completely visible over northeast Asia, Australia, and Antarctica, seen rising over east, southeast, and south Asia and setting over much of North America and western South America.[3]

Eclipse details

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

May 3, 1958 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.96760
Umbral Magnitude 0.00919
Gamma 1.01884
Sun Right Ascension 02h40m25.8s
Sun Declination +15°36'27.0"
Sun Semi-Diameter 15'51.8"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 14h41m19.7s
Moon Declination -14°35'56.8"
Moon Semi-Diameter 16'33.1"
Moon Equatorial Horizontal Parallax 1°00'44.9"
ΔT 32.4 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 April–May 1958
April 4
Ascending node (full moon)		 April 19
Descending node (new moon)
 May 3
Ascending node (full moon)
Penumbral lunar eclipse
Lunar Saros 102		 Annular solar eclipse
Solar Saros 128		 Partial lunar eclipse
Lunar Saros 140

Eclipses in 1958

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 140

Inex

Triad

Lunar eclipses of 1955–1958

This eclipse is a member of a semester series. An eclipse in a semester series of lunar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.[5]

The penumbral lunar eclipse on January 8, 1955 occurs in the previous lunar year eclipse set, and the penumbral lunar eclipse on April 4, 1958 occurs in the next lunar year eclipse set.

Lunar eclipse series sets from 1955 to 1958
Ascending node   Descending node
Saros Date
Viewing 		Type
Chart 		Gamma Saros Date
Viewing 		Type
Chart 		Gamma
110 1955 Jun 05
 Penumbral
 −1.2384 115 1955 Nov 29
 Partial
 0.9551
120 1956 May 24
 Partial
 −0.4726 125 1956 Nov 18
 Total
 0.2917
130 1957 May 13
 Total
 0.3046 135 1957 Nov 07
 Total
 −0.4332
140 1958 May 03
 Partial
 1.0188 145 1958 Oct 27
 Penumbral
 −1.1571

Half-Saros cycle

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[6] This lunar eclipse is related to two partial solar eclipses of Solar Saros 147.

April 28, 1949 May 9, 1967

See also

Notes

  1. ^ "May 3, 1958 Partial Lunar Eclipse". timeanddate. Retrieved 25 December 2024.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 25 December 2024.
  3. ^ "Partial Lunar Eclipse of 1958 May 03" (PDF). NASA. Retrieved 25 December 2024.
  4. ^ "Partial Lunar Eclipse of 1958 May 03". EclipseWise.com. Retrieved 25 December 2024.
  5. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.
  6. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros


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