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July 1973 lunar eclipse

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Penumbral lunar eclipse
July 1973 lunar eclipse
Penumbral eclipse
The Moon's hourly motion shown right to left
DateJuly 15, 1973
Gamma 1.5178
Magnitude −0.9581
Saros cycle 148 (1 of 71)
Penumbral99 minutes, 5 seconds
Contacts (UTC)
P110:49:07
Greatest11:38:35
P412:28:12

A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Sunday, July 15, 1973,[1] with an umbral magnitude of −0.9581. 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 after apogee (on July 12, 1973, at 22:45 UTC), the Moon's apparent diameter was smaller.[2]

This eclipse was the third of four lunar eclipses in 1973, with the others occurring on January 18 (penumbral), June 15 (penumbral), and December 10 (partial).

This was the first lunar eclipse of Saros series 148.

Visibility

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The eclipse was completely visible over Australia, western North America, and Antarctica, seen rising over east Asia and setting over central North America and western South America.[3]

Eclipse details

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

July 15, 1973 Lunar Eclipse Parameters
Parameter Value
Penumbral Magnitude 0.10468
Umbral Magnitude −0.95805
Gamma 1.51782
Sun Right Ascension 07h38m36.3s
Sun Declination +21°30'35.7"
Sun Semi-Diameter 15'44.1"
Sun Equatorial Horizontal Parallax 08.7"
Moon Right Ascension 19h37m04.9s
Moon Declination -20°10'55.9"
Moon Semi-Diameter 14'48.4"
Moon Equatorial Horizontal Parallax 0°54'20.5"
ΔT 43.9 s

Eclipse season

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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 June–July 1973
June 15
Ascending node (full moon)
June 30
Descending node (new moon)
July 15
Ascending node (full moon)
Penumbral lunar eclipse
Lunar Saros 110
Total solar eclipse
Solar Saros 136
Penumbral lunar eclipse
Lunar Saros 148
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Eclipses in 1973

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Metonic

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Tzolkinex

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Half-Saros

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Tritos

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Lunar Saros 148

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Inex

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Triad

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Lunar eclipses of 1969–1973

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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 eclipses on April 2, 1969 and September 25, 1969 occur in the previous lunar year eclipse set, and the lunar eclipses on June 15, 1973 (penumbral) and December 10, 1973 (partial) occur in the next lunar year eclipse set.

Lunar eclipse series sets from 1969 to 1973
Ascending node   Descending node
Saros Date
Viewing
Type
Chart
Gamma Saros Date
Viewing
Type
Chart
Gamma
108 1969 Aug 27
Penumbral
−1.5407 113 1970 Feb 21
Partial
0.9620
118 1970 Aug 17
Partial
−0.8053 123 1971 Feb 10
Total
0.2741
128 1971 Aug 06
Total
−0.0794 133 1972 Jan 30
Total
−0.4273
138 1972 Jul 26
Partial
0.7117 143 1973 Jan 18
Penumbral
−1.0845
148 1973 Jul 15
Penumbral
1.5178

Saros 148

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This eclipse is a part of Saros series 148, repeating every 18 years, 11 days, and containing 70 events. The series started with a penumbral lunar eclipse on July 15, 1973. It contains partial eclipses from October 10, 2117 through May 5, 2460; total eclipses from May 17, 2478 through September 14, 2676; and a second set of partial eclipses from September 25, 2694 through May 25, 3091. The series ends at member 70 as a penumbral eclipse on August 9, 3217.

The longest duration of totality will be produced by member 37 at 104 minutes, 29 seconds on July 10, 2568. All eclipses in this series occur at the Moon’s ascending node of orbit.[6]

Greatest First
The greatest eclipse of the series will occur on 2568 Jul 10, lasting 104 minutes, 29 seconds.[7] Penumbral Partial Total Central
1973 Jul 15
2117 Oct 10
2478 May 25
2514 Jun 08
Last
Central Total Partial Penumbral
2622 Aug 13
2676 Sep 14
3091 May 25
3217 Aug 09

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 1–13 occur between 1973 and 2200:
1 2 3
1973 Jul 15 1991 Jul 26 2009 Aug 06
4 5 6
2027 Aug 17 2045 Aug 27 2063 Sep 07
7 8 9
2081 Sep 18 2099 Sep 29 2117 Oct 10
10 11 12
2135 Oct 22 2153 Nov 01 2171 Nov 12
13
2189 Nov 22

Tritos series

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This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.

Series members between 1801 and 2060
1809 Oct 23
(Saros 133)
1820 Sep 22
(Saros 134)
1831 Aug 23
(Saros 135)
1842 Jul 22
(Saros 136)
1853 Jun 21
(Saros 137)
1864 May 21
(Saros 138)
1875 Apr 20
(Saros 139)
1886 Mar 20
(Saros 140)
1897 Feb 17
(Saros 141)
1908 Jan 18
(Saros 142)
1918 Dec 17
(Saros 143)
1929 Nov 17
(Saros 144)
1940 Oct 16
(Saros 145)
1951 Sep 15
(Saros 146)
1962 Aug 15
(Saros 147)
1973 Jul 15
(Saros 148)
1984 Jun 13
(Saros 149)
2060 Nov 08
(Saros 156)

Half-Saros cycle

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A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half saros).[8] This lunar eclipse is related to two partial solar eclipses of Solar Saros 155.

July 9, 1964 July 20, 1982

See also

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Notes

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  1. ^ "July 15, 1973 Penumbral Lunar Eclipse". timeanddate. Retrieved 3 January 2025.
  2. ^ "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 3 January 2025.
  3. ^ "Penumbral Lunar Eclipse of 1973 Jul 15" (PDF). NASA. Retrieved 3 January 2025.
  4. ^ "Penumbral Lunar Eclipse of 1973 Jul 15". EclipseWise.com. Retrieved 3 January 2025.
  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 148". eclipse.gsfc.nasa.gov.
  7. ^ Listing of Eclipses of series 148
  8. ^ Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
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