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July 1962 lunar eclipse

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Penumbral lunar eclipse July 17, 1962
July 1962 lunar eclipse
Penumbral eclipse
The Moon's hourly motion shown right to left
DateJuly 17, 1962
Gamma1.3371
Magnitude−0.5835
Saros cycle109 (70 of 73)
Penumbral168 minutes, 16 seconds
Contacts (UTC)
P110:30:13
Greatest11:54:15
P413:18:29
← February 1962August 1962 →

A penumbral lunar eclipse occurred at the Moon’s descending node of orbit on Tuesday, July 17, 1962, with an umbral magnitude of −0.5835. 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 days before perigee (on July 20, 1962, at 11:00 UTC), the Moon's apparent diameter was larger.

Visibility

The eclipse was completely visible over Australia, Antarctica, and the Pacific Ocean, seen rising over east and southeast Asia and setting over much of North America and western South America.

Eclipse details

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

July 17, 1962 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.39245
Umbral Magnitude −0.58347
Gamma 1.33712
Sun Right Ascension 07h45m18.8s
Sun Declination +21°14'17.1"
Sun Semi-Diameter 15'44.2"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 19h44m51.2s
Moon Declination -19°55'25.0"
Moon Semi-Diameter 16'07.5"
Moon Equatorial Horizontal Parallax 0°59'10.9"
ΔT 34.3 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 July–August 1962
July 17
Descending node (full moon)
July 31
Ascending node (new moon)
August 15
Descending node (full moon)
Penumbral lunar eclipse
Lunar Saros 109
Annular solar eclipse
Solar Saros 135
Penumbral lunar eclipse
Lunar Saros 147

Related eclipses

Eclipses in 1962

Metonic

Tzolkinex

Half-Saros

Tritos

Lunar Saros 109

Inex

Triad

Lunar eclipses of 1962–1965

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.

The penumbral lunar eclipses on February 19, 1962 and August 15, 1962 occur in the previous lunar year eclipse set.

Lunar eclipse series sets from 1962 to 1965
Descending node   Ascending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
109 1962 Jul 17
Penumbral
1.3371 114 1963 Jan 09
Penumbral
−1.0128
119 1963 Jul 06
Partial
0.6197 124 1963 Dec 30
Total
−0.2889
129 1964 Jun 25
Total
−0.1461 134 1964 Dec 19
Total
0.3801
139 1965 Jun 14
Partial
−0.9006 144 1965 Dec 08
Penumbral
1.0775

Saros 109

This eclipse is a part of Saros series 109, repeating every 18 years, 11 days, and containing 71 or 72 events (depending on the source). The series started with a penumbral lunar eclipse on June 27, 736 AD. It contains partial eclipses from September 22, 880 AD through April 16, 1223; total eclipses from April 27, 1241 through October 17, 1529; and a second set of partial eclipses from October 28, 1547 through May 22, 1872. The series ends at member 71 as a penumbral eclipse on August 8, 1998, though some sources count a possible penumbral eclipse on August 18, 2016 as the last eclipse of the series.

The longest duration of totality was produced by member 35 at 99 minutes, 45 seconds on July 1, 1349. All eclipses in this series occur at the Moon’s descending node of orbit.

Greatest First
The greatest eclipse of the series occurred on 1349 Jul 01, lasting 99 minutes, 45 seconds. Penumbral Partial Total Central
736 Jun 27
880 Sep 22
1241 Apr 27
1295 May 30
Last
Central Total Partial Penumbral
1421 Aug 13
1529 Oct 17
1872 May 22
1998 Aug 08

Eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.

Series members 61–72 occur between 1801 and 2016:
61 62 63
1818 Apr 21 1836 May 01 1854 May 12
64 65 66
1872 May 22 1890 Jun 03 1908 Jun 14
67 68 69
1926 Jun 25 1944 Jul 06 1962 Jul 17
70 71 72
1980 Jul 27 1998 Aug 08 2016 Aug 18

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 partial solar eclipses of Solar Saros 116.

July 11, 1953 July 22, 1971

See also

Notes

  1. "July 17, 1962 Penumbral Lunar Eclipse". timeanddate. Retrieved 29 December 2024.
  2. "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 29 December 2024.
  3. "Penumbral Lunar Eclipse of 1962 Jul 17" (PDF). NASA. Retrieved 29 December 2024.
  4. "Penumbral Lunar Eclipse of 1962 Jul 17". EclipseWise.com. Retrieved 29 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. "NASA - Catalog of Lunar Eclipses of Saros 109". eclipse.gsfc.nasa.gov.
  7. Listing of Eclipses of series 109
  8. 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
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August 2017 lunar eclipse
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May 2022 lunar eclipse
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February 2017 lunar eclipse
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