Penumbral eclipse | |||||||||
The Moon's hourly motion shown right to left | |||||||||
Date | June 15, 1973 | ||||||||
---|---|---|---|---|---|---|---|---|---|
Gamma | −1.3217 | ||||||||
Magnitude | −0.6020 | ||||||||
Saros cycle | 110 (69 of 72) | ||||||||
Penumbral | 204 minutes, 36 seconds | ||||||||
| |||||||||
← January 1973July 1973 → |
A penumbral lunar eclipse occurred at the Moon’s ascending node of orbit on Friday, June 15, 1973, with an umbral magnitude of −0.6020. 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 3 hours after apogee (on June 15, 1973, at 18:05 UTC), the Moon's apparent diameter was smaller.
This eclipse was the second of four lunar eclipses in 1973, with the others occurring on January 18 (penumbral), July 15 (penumbral), and December 10 (partial).
Visibility
The eclipse was completely visible over much of Africa, eastern Europe, the western half of Asia, and Antarctica, seen rising over much of South America, western Europe, and west Africa and setting over east Asia and Australia.
Eclipse details
Shown below is a table displaying details about this particular solar eclipse. It describes various parameters pertaining to this eclipse.
Parameter | Value |
---|---|
Penumbral Magnitude | 0.46852 |
Umbral Magnitude | −0.60197 |
Gamma | −1.32166 |
Sun Right Ascension | 05h36m24.5s |
Sun Declination | +23°19'56.0" |
Sun Semi-Diameter | 15'44.6" |
Sun Equatorial Horizontal Parallax | 08.7" |
Moon Right Ascension | 17h36m42.3s |
Moon Declination | -24°31'09.1" |
Moon Semi-Diameter | 14'42.4" |
Moon Equatorial Horizontal Parallax | 0°53'58.5" |
ΔT | 43.8 s |
Eclipse season
See also: Eclipse cycleThis 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.
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 |
Related eclipses
Eclipses in 1973
- An annular solar eclipse on January 4.
- A penumbral lunar eclipse on January 18.
- A penumbral lunar eclipse on June 15.
- A total solar eclipse on June 30.
- A penumbral lunar eclipse on July 15.
- A partial lunar eclipse on December 10.
- An annular solar eclipse on December 24.
Metonic
- Preceded by: Lunar eclipse of August 27, 1969
- Followed by: Lunar eclipse of April 4, 1977
Tzolkinex
- Preceded by: Lunar eclipse of May 4, 1966
- Followed by: Lunar eclipse of July 27, 1980
Half-Saros
- Preceded by: Solar eclipse of June 10, 1964
- Followed by: Solar eclipse of June 21, 1982
Tritos
- Preceded by: Lunar eclipse of July 17, 1962
- Followed by: Lunar eclipse of May 15, 1984
Lunar Saros 110
- Preceded by: Lunar eclipse of June 5, 1955
- Followed by: Lunar eclipse of June 27, 1991
Inex
- Preceded by: Lunar eclipse of July 6, 1944
- Followed by: Lunar eclipse of May 26, 2002
Triad
- Preceded by: Lunar eclipse of August 14, 1886
- Followed by: Lunar eclipse of April 15, 2060
Lunar eclipses of 1973–1976
Lunar eclipse series sets from 1973–1976 | ||||||||
---|---|---|---|---|---|---|---|---|
Ascending node | Descending node | |||||||
Saros | Date Viewing |
Type Chart |
Gamma | Saros | Date Viewing |
Type Chart |
Gamma | |
110 | 1973 Jun 15 |
Penumbral |
−1.32166 | 115 | 1973 Dec 10 |
Partial |
0.96441 | |
120 | 1974 Jun 04 |
Partial |
−0.54887 | 125 | 1974 Nov 29 |
Total |
0.30540 | |
130 | 1975 May 25 |
Total |
0.23674 | 135 | 1975 Nov 18 |
Total |
−0.41343 | |
140 | 1976 May 13 |
Partial |
0.95860 | 145 | 1976 Nov 06 |
Penumbral |
−1.12760 | |
Last set | 1973 Jul 15 | Last set | 1973 Jan 18 | |||||
Next set | 1977 Apr 04 | Next set | 1977 Sep 27 |
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 117.
June 10, 1964 | June 21, 1982 |
---|---|
See also
Notes
- "June 15–16, 1973 Penumbral Lunar Eclipse". timeanddate. Retrieved 3 January 2025.
- "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 3 January 2025.
- "Penumbral Lunar Eclipse of 1973 Jun 15" (PDF). NASA. Retrieved 3 January 2025.
- "Penumbral Lunar Eclipse of 1973 Jun 15". EclipseWise.com. Retrieved 3 January 2025.
- Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
External links
- 1973 Jun 15 chart Eclipse Predictions by Fred Espenak, NASA/GSFC
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