Partial eclipse | |||||||||||||
The Moon's hourly motion shown right to left | |||||||||||||
Date | March 2, 1961 | ||||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|---|
Gamma | 0.5541 | ||||||||||||
Magnitude | 0.8006 | ||||||||||||
Saros cycle | 132 (27 of 71) | ||||||||||||
Partiality | 192 minutes, 51 seconds | ||||||||||||
Penumbral | 347 minutes, 38 seconds | ||||||||||||
| |||||||||||||
← September 1960August 1961 → |
A partial lunar eclipse occurred at the Moon’s ascending node of orbit on Thursday, March 2, 1961, with an umbral magnitude of 0.8006. 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 3.7 days after apogee (on February 26, 1961, at 21:10 UTC), the Moon's apparent diameter was smaller.
Visibility
The eclipse was completely visible over east and northeast Asia, Australia, and northwestern North America, seen rising over east Africa, eastern Europe and much of Asia and setting over much of North America and northwestern South America.
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 | 1.88284 |
Umbral Magnitude | 0.80062 |
Gamma | 0.55406 |
Sun Right Ascension | 22h52m38.0s |
Sun Declination | -07°09'38.0" |
Sun Semi-Diameter | 16'08.1" |
Sun Equatorial Horizontal Parallax | 08.9" |
Moon Right Ascension | 10h53m13.0s |
Moon Declination | +07°38'40.5" |
Moon Semi-Diameter | 14'54.5" |
Moon Equatorial Horizontal Parallax | 0°54'43.0" |
ΔT | 33.6 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.
February 15 Descending node (new moon) |
March 2 Ascending node (full moon) |
---|---|
Total solar eclipse Solar Saros 120 |
Partial lunar eclipse Lunar Saros 132 |
Related eclipses
Eclipses in 1961
- A total solar eclipse on February 15.
- A partial lunar eclipse on March 2.
- An annular solar eclipse on August 11.
- A partial lunar eclipse on August 26.
Metonic
- Preceded by: Lunar eclipse of May 13, 1957
- Followed by: Lunar eclipse of December 19, 1964
Tzolkinex
- Preceded by: Lunar eclipse of January 19, 1954
- Followed by: Lunar eclipse of April 13, 1968
Half-Saros
- Preceded by: Solar eclipse of February 25, 1952
- Followed by: Solar eclipse of March 7, 1970
Tritos
- Preceded by: Lunar eclipse of April 2, 1950
- Followed by: Lunar eclipse of January 30, 1972
Lunar Saros 132
- Preceded by: Lunar eclipse of February 20, 1943
- Followed by: Lunar eclipse of March 13, 1979
Inex
- Preceded by: Lunar eclipse of March 22, 1932
- Followed by: Lunar eclipse of February 9, 1990
Triad
- Preceded by: Lunar eclipse of May 1, 1874
- Followed by: Lunar eclipse of January 1, 2048
Lunar eclipses of 1958–1962
Ascending node | Descending node | |||||||
---|---|---|---|---|---|---|---|---|
Saros | Date Viewing |
Type Chart |
Gamma | Saros | Date Viewing |
Type Chart |
Gamma | |
102 | 1958 Apr 04 |
Penumbral |
-1.53805 | |||||
112 | 1959 Mar 24 |
Partial |
-0.87571 | 117 | 1959 Sep 17 |
Penumbral |
1.02963 | |
122 | 1960 Mar 13 |
Total |
-0.17990 | 127 | 1960 Sep 05 |
Total |
0.24219 | |
132 | 1961 Mar 02 |
Partial |
0.55406 | 137 | 1961 Aug 26 |
Partial |
-0.48947 | |
142 | 1962 Feb 19 |
Penumbral |
1.25115 | 147 | 1962 Aug 15 |
Penumbral |
-1.22104 | |
Last set | 1958 May 03 | Last set | 1958 Oct 27 | |||||
Next set | 1963 Jan 09 | Next set | 1962 Jul 17 |
Saros 132
Lunar saros series 132, repeating every 18 years and 11 days, has a total of 71 lunar eclipse events including 44 umbral lunar eclipses (32 partial lunar eclipses and 12 total lunar eclipses).
Greatest | First | |||
---|---|---|---|---|
The greatest eclipse of the series will occur on 2123 Jun 9, lasting 106 minutes. |
Penumbral | Partial | Total | Central |
1492 May 12 |
1636 Aug 16 |
2015 Apr 4 |
2069 May 6 | |
Last | ||||
Central | Total | Partial | Penumbral | |
2177 Jul 11 |
2213 Aug 2 |
2429 Dec 11 |
2754 Jun 26 |
There are 11 series events between 1901 and 2100, grouped into threes (called an exeligmos), each column with approximately the same viewing longitude on earth.
1907 Jan 29 | 1925 Feb 8 | 1943 Feb 20 | |||
1961 Mar 2 | 1979 Mar 13 | 1997 Mar 24 | |||
2015 Apr 4 | 2033 Apr 14 | 2051 Apr 26 | |||
2069 May 6 | 2087 May 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 total solar eclipses of Solar Saros 139.
February 25, 1952 | March 7, 1970 |
---|---|
See also
Notes
- "March 2–3, 1961 Partial Lunar Eclipse". timeanddate. Retrieved 29 December 2024.
- "Moon Distances for London, United Kingdom, England". timeanddate. Retrieved 29 December 2024.
- "Partial Lunar Eclipse of 1961 Mar 02" (PDF). NASA. Retrieved 29 December 2024.
- "Partial Lunar Eclipse of 1961 Mar 02". EclipseWise.com. Retrieved 29 December 2024.
- Listing of Eclipses of series 132
- Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros
External links
- 1961 Mar 02 chart Eclipse Predictions by Fred Espenak, NASA/GSFC
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