March 1951 lunar eclipse

Last updated
Lunar eclipse chart close-1951Mar23.png

A penumbral lunar eclipse took place on Friday, March 23, 1951. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 64% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours and 34 minutes.

Contents

Visibility

Lunar eclipse from moon-1951Mar23.png

Member

This is the 20th member of Lunar Saros 141. The previous event was the March 1933 lunar eclipse. The next event is the April 1969 lunar eclipse.

Lunar year series

Lunar eclipse series sets from 1947–1951
Descending node Ascending node
Saros Date
Viewing
Type
Chart
SarosDate
Viewing
Type
Chart
111 1948 Apr 23
Lunar eclipse from moon-1948Apr23.png
Partial
Lunar eclipse chart close-1948Apr23.png
116 1948 Oct 18
Lunar eclipse from moon-1948Oct18.png
Penumbral
Lunar eclipse chart close-1948Oct18.png
121 1949 Apr 13
Lunar eclipse from moon-1949Apr13.png
Total
Lunar eclipse chart close-1949Apr13.png
126 1949 Oct 07
Lunar eclipse from moon-1949Oct07.png
Total
Lunar eclipse chart close-1949Oct07.png
131 1950 Apr 02
Lunar eclipse from moon-1950Apr02.png
Total
Lunar eclipse chart close-1950Apr02.png
136 1950 Sep 26
Lunar eclipse from moon-1950Sep26.png
Total
Lunar eclipse chart close-1950Sep26.png
141 1951 Mar 23
Lunar eclipse from moon-1951Mar23.png
Penumbral
Lunar eclipse chart close-1951Mar23.png
146 1951 Sep 15
Lunar eclipse from moon-1951Sep15.png
Penumbral
Lunar eclipse chart close-1951Sep15.png

Saros series

Lunar Saros 141, repeating every 18 years and 11 days, has a total of 72 lunar eclipse events including 26 total lunar eclipses.

First Penumbral Lunar Eclipse: 1608 Aug 25

First Partial Lunar Eclipse: 2041 May 16

First Total Lunar Eclipse: 2167 Aug 01

First Central Lunar Eclipse: 2221 Sep 02

Greatest Eclipse of the Lunar Saros 141: 2293 Oct 16

Last Central Lunar Eclipse: 2546 Mar 18

Last Total Lunar Eclipse: 2618 May 01

Last Partial Lunar Eclipse: 2744 Jul 16

Last Penumbral Lunar Eclipse: 2888 Oct 11

1901-2100

March 1915 lunar eclipse

March 1933 lunar eclipse

March 1951 lunar eclipse

April 1969 lunar eclipse

April 1987 lunar eclipse

April 2005 lunar eclipse

May 2023 lunar eclipse

May 2041 lunar eclipse

May 2059 lunar eclipse

June 2077 lunar eclipse

June 2095 lunar eclipse

See also

Notes


    Related Research Articles

    <span class="mw-page-title-main">April 2005 lunar eclipse</span> Penumbral lunar eclipse April 24, 2005

    A penumbral lunar eclipse took place on April 24, 2005, the first of two lunar eclipses in 2005. At maximum eclipse, 86.5% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours and 6 minutes overall, and was visible from east Asia, Australia, and the Americas.

    <span class="mw-page-title-main">December 2001 lunar eclipse</span> Penumbral lunar eclipse December 30, 2001

    A penumbral lunar eclipse took place on Sunday, December 30, 2001, the last of three lunar eclipses in 2001.

    <span class="mw-page-title-main">January 1999 lunar eclipse</span> Penumbral lunar eclipse January 31, 1999

    A penumbral lunar eclipse took place on Sunday, January 31, 1999, the first of two lunar eclipses in 1999.

    A penumbral lunar eclipse took place on Thursday, March 3, 1988, the first of two lunar eclipses in 1988, the second being on August 27, 1988. Earlier sources compute this as a 0.3% partial eclipse lasting under 14 minutes, and newest calculations list it as a penumbral eclipse that never enters the umbral shadow. In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth, and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours, 53 minutes and 50.6 seconds in all, though for most of it, the eclipse was extremely difficult or impossible to see. The Moon was 2.2 days after apogee, making it 6.1% smaller than average.

    A penumbral lunar eclipse took place on Wednesday, October 7, 1987, the second of two lunar eclipses in 1987, the first being on April 14, 1987. The Moon approached within 0.00949% of its diameter outside of touching the Earth’s umbral shadow at maximum eclipse; 98.63% of the Moon's disc was partially shaded by the Earth, with the overall eclipse lasting 4 hours and 14 minutes. While less dramatic than a partial eclipse, a shading across the Moon should have been readily visible to observers. The Moon was just 3.1 days after perigee, making it 2.1% larger than average.

    A penumbral lunar eclipse took place on Tuesday, April 14, 1987, the first of two lunar eclipses in 1987, the second being on October 7, 1987. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 77.703% of the Moon's disc was partially shaded by the Earth, which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours, 54 minutes and 12.8 seconds. The Moon was just 4.6 days before perigee, making it 0.5% larger than average.

    A penumbral lunar eclipse took place on Thursday, November 8, 1984, the last of three lunar eclipses in 1984. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 90% of the Moon's disc was partially shaded by the Earth, which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 28 minutes.

    A penumbral lunar eclipse took place on Tuesday, December 20, 1983, the second of two lunar eclipses in 1983. At the maximum eclipse, 89% of the Moon's disk was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours and 2 minutes overall.

    A penumbral lunar eclipse took place on Tuesday, January 20, 1981, the first of two lunar eclipses in 1981. In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth, and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours and 24 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see. The moon's apparent diameter was larger because the eclipse occurred 5.2 days after perigee.

    A penumbral lunar eclipse took place on Saturday, March 1, 1980, the first of three penumbral lunar eclipses in 1980. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 65.455% of the Moon's disc was partially shaded by the Earth, which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours, 58 minutes and 33.3 seconds.

    A penumbral lunar eclipse took place at the Moon's descending node of the orbit on Tuesday, August 26, 1980, the last of three penumbral lunar eclipses in 1980 with a penumbral magnitude of 0.70891. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 70.891% of the Moon's disc was partially shaded by the Earth, which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours, 34 minutes and 26 seconds.

    <span class="mw-page-title-main">January 2038 lunar eclipse</span>

    A penumbral lunar eclipse will take place on January 21, 2038. It will be visible to the naked eye as 89.96% of the Moon will be immersed in Earth's penumbral shadow. It is the first of 4 penumbral lunar eclipses in 2038, with the next eclipse on 17 June.

    A partial lunar eclipse will take place on May 16, 2041.

    A penumbral lunar eclipse took place on Saturday, November 6, 1976, the second of two lunar eclipses in 1976, the first being on May 13. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 83.827% of the Moon's disc was partially shaded by the Earth, which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours, 25 minutes and 52.1 seconds. Occurring only 0.3 days after apogee, the moon's apparent diameter was 6.5% smaller than average.

    A penumbral lunar eclipse took place on Wednesday, April 2, 1969, the first of three penumbral lunar eclipses in 1969, the second being on Wednesday, August 27, and the last being on Thursday, September 25. This subtle penumbral eclipse may have been visible to a skilled observer at maximum eclipse. 70.337% of the Moon's disc was partially shaded by the Earth, which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 3 hours, 43 minutes and 46.9 seconds. Occurring only 4.2 days before perigee, the Moon's apparent diameter was 0.9% larger than average.

    <span class="mw-page-title-main">September 1969 lunar eclipse</span> Penumbral lunar eclipse September 25 1969

    A penumbral lunar eclipse took place on Thursday, September 25, 1969, the last of three penumbral lunar eclipses in 1969, the first being on Wednesday, April 2, and the second being on Wednesday, August 27. At maximum eclipse, 90% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours and 5 minutes overall.

    <span class="mw-page-title-main">December 1965 lunar eclipse</span> Penumbral lunar eclipse December 8, 1965

    A penumbral lunar eclipse took place on Wednesday, December 8, 1965. At maximum eclipse, 88% of the Moon's disc was partially shaded by the Earth, which caused a slight shadow gradient across its disc; this subtle effect may have been visible to careful observers. No part of the Moon was in complete shadow. The eclipse lasted 4 hours and 1 minute overall.

    <span class="mw-page-title-main">January 1963 lunar eclipse</span> Penumbral lunar eclipse January 9, 1963

    A penumbral lunar eclipse took place on Wednesday, January 9, 1963, the first of three lunar eclipses in 1963.

    <span class="mw-page-title-main">Lunar Saros 112</span>

    Saros cycle series 112 for lunar eclipses occurs at the moon's ascending node, 18 years 11 and 1/3 days. It contains 72 events, with 15 total eclipses, starting in 1364 and ending in 1616. Solar Saros 119 interleaves with this lunar Saros with an event occurring every 9 years 5 days alternating between each saros series.

    <span class="mw-page-title-main">March 1933 lunar eclipse</span> Penumbral lunar eclipse March 12, 1933

    A penumbral lunar eclipse took place on Sunday, March 12, 1933. This very subtle penumbral eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 26 minutes, just 59% of the Moon's disc was in partial shadow.