Total penumbral lunar eclipse

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The penumbral lunar eclipse on March 14, 2006 was a total penumbral eclipse. Lunar eclipse chart close-06mar14.png
The penumbral lunar eclipse on March 14, 2006 was a total penumbral eclipse.

A total penumbral lunar eclipse is a lunar eclipse that occurs when the Moon becomes completely immersed in the penumbral cone of the Earth without touching the umbra. [1]

Contents

The path for the Moon to pass within the penumbra and outside the umbra is very narrow. It can only happen on the Earth's northern or southern penumbral edges. In addition, the size of the penumbra is sometimes too small where the Moon enters it to contain the Moon. The width of the Earth's penumbra is determined by the Sun's angular diameter at the time of the eclipse, and the Moon's angular diameter is larger than the Sun over part of its elliptical orbit, depending on whether the eclipse occurs at the nearest (perigee) or farthest point (apogee) in its orbit around the Earth. The majority of the time, the size of the Moon and the size of the Earth's penumbra where the Moon crosses it mean that most eclipses will not be total penumbral in nature.

Frequency

Total penumbral eclipses constitute a relatively small fraction of lunar eclipses, and the distribution of these events is uneven, occurring between 0 and 9 times per century. The period of this variation is approximately 600 years and also correlates with the frequency of total umbral eclipses and tetrads. [1]

The maximum number in Fred's 5K canon [N 1] is eight for saros 19. [2] Saros 32 and 132 have seven. [3] [4] Saros 58, 95, and 114 have six. [5] [6] [7]

Saros 114 is the only saros in the canon to have a total of seven total penumbral lunar eclipses that are not all in a row. [7] Likewise, saros 169 has five total penumbral eclipses, but only four of them occur consecutively. [8]

Saros series with multiple consecutive total penumbral eclipses

This table summarizes which saros series contain four or more consecutive total penumbral eclipses.

Saros
series
Consecutive total
penumbral eclipses
-3397 [9]
-26613 [9]
-2589 [9]
-24710 [9]
-23710 [9]
-22610 [9]
-21812 [9]
-1576 [9]
-1184 [9]
-1167 [9]
-10511 [9]
-399 [9]
-376 [9]
-269 [9]
19 [N 1] 8 [2]
32 [N 1] 7 [3]
58 [N 1] 6 [5]
95 [N 1] 6 [6]
114 [N 1] [N 2] 6 [7]
132 [N 1] 7 [4]
169 [N 1] [N 3] 4 [8]
1875 [9]
2554 [9]

Summary frequency of total penumbral, total umbral and tetrad events 501–2500

The frequency of total penumbral lunar eclipses varies by century with the frequency of total umbral eclipses.
A tetrad is a set of four total umbral eclipses within two years. Total penumbral eclipse frequency by century.png
The frequency of total penumbral lunar eclipses varies by century with the frequency of total umbral eclipses.
A tetrad is a set of four total umbral eclipses within two years.
CenturyTotal
penumbral
Total
umbral
Tetrads
501–6001630
601–7002580
701–8002693
801–9005888
901–10003786
1001–11003620
1101–12000600
1201–13001600
1301–14008776
1401–15004834
1501–16002766
1601–17002610
1701–18000600
1801–19002620
1901–20009815
2001–21005847
2101–22005694
2201–23001610
2301–24000600
2401–25006694

List of total penumbral lunar eclipse events 1901–2200

Ascending nodesDescending nodes
Saros DateViewingChartSarosDateViewingChart
110 1901 May 03 Lunar eclipse from moon-1901May03.png Lunar eclipse chart close-1901May03.png
114 1908 Dec 07 Lunar eclipse from moon-1908Dec07.png Lunar eclipse chart close-1908Dec07.png
114 1926 Dec 19 Lunar eclipse from moon-1926Dec19.png Lunar eclipse chart close-1926Dec19.png
114 1944 Dec 29 Lunar eclipse from moon-1944Dec29.png Lunar eclipse chart close-1944Dec29.png
116 1948 Oct 18 Lunar eclipse from moon-1948Oct18.png Lunar eclipse chart close-1948Oct18.png
114 1963 Jan 09 Lunar eclipse from moon-1963Jan09.png Lunar eclipse chart close-1963Jan09.png
114 1981 Jan 20 Lunar eclipse from moon-1981Jan20.png Lunar eclipse chart close-1981Jan20.png 113 1988 Mar 03 Lunar eclipse from moon-1988Mar03.png Lunar eclipse chart close-1988Mar03.png
114 1999 Jan 31 Lunar eclipse from moon-1999Jan31.png Lunar eclipse chart close-1999Jan31.png 113 2006 Mar 14 Lunar eclipse from moon-2006Mar14.png Lunar eclipse chart close-06mar14.png
119 2053 Aug 29 Lunar eclipse chart close-2053Aug29.png
142 2070 Apr 25 Lunar eclipse from moon-2070Apr25.png Lunar eclipse chart close-2070Apr25.png
120 2082 Aug 08 Lunar eclipse from moon-2082Aug08.png Lunar eclipse chart close-2082Aug08.png
148 2099 Sep 29 Lunar eclipse from moon-2099Sep29.png Lunar eclipse chart close-2099Sep29.png
145 2103 Jan 23
145 2121 Feb 02
145 2139 Feb 13

See also

Notes

  1. 1 2 3 4 5 6 7 8 Total penumbral lunar eclipses are indicated by the Nx eclipse type in Fred Espenak's Lunar Eclipse canon.
  2. Saros 114 has seven total penumbral eclipses, but only six of them occur consecutively.
  3. Saros 169 has five total penumbral eclipses, but only four of them occur consecutively.

Related Research Articles

Eclipse Astronomical event where one body is hidden by another

An eclipse is an astronomical event that occurs when an astronomical object or spacecraft is temporarily obscured, by passing into the shadow of another body or by having another body pass between it and the viewer. This alignment of three celestial objects is known as a syzygy. Apart from syzygy, the term eclipse is also used when a spacecraft reaches a position where it can observe two celestial bodies so aligned. An eclipse is the result of either an occultation or a transit.

Lunar eclipse When the Moon moves into the Earths shadow

A lunar eclipse occurs when the Moon moves into the Earth's shadow. This can occur only when the Sun, Earth, and Moon are exactly or very closely aligned with Earth between the other two, and only on the night of a full moon. The type and length of a lunar eclipse depend on the Moon's proximity to either node of its orbit.

Solar eclipse of March 29, 2006 21st-century total solar eclipse

A total solar eclipse occurred on March 29, 2006. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. It was visible from a narrow corridor which traversed half the Earth. The magnitude, that is, the ratio between the apparent sizes of the Moon and that of the Sun, was 1.052, and it was part of Saros 139.

Magnitude of eclipse

The magnitude of eclipse is the fraction of the angular diameter of a celestial body being eclipsed. This applies to all celestial eclipses. The magnitude of a partial or annular solar eclipse is always between 0.0 and 1.0, while the magnitude of a total solar eclipse is always greater than or equal to 1.0.

February 2008 lunar eclipse

A total lunar eclipse occurred on February 20 and February 21, 2008. It was visible in the eastern evening sky on February 20 for all of North and South America, and on February 21 in the predawn western sky from most of Africa and Europe. Greatest Eclipse occurring on Thursday, February 21, 2008 at 03:26:03 UTC, totality lasting 49 minutes and 45.6 seconds.

April 2014 lunar eclipse

A total lunar eclipse took place on 15 April 2014. It was the first of two total lunar eclipses in 2014, and the first in a tetrad. Subsequent eclipses in the tetrad are those of 8 October 2014, 4 April 2015, and 28 September 2015. Occurring 6.7 days after apogee, the Moon's apparent diameter was smaller.

October 2014 lunar eclipse

A total lunar eclipse took place on 8 October 2014. It is the second of two total lunar eclipses in 2014, and the second in a tetrad. Other eclipses in the tetrad are those of 15 April 2014, 4 April 2015, and 28 September 2015. Occurring only 2.1 days after perigee, the Moon's apparent diameter was larger, 1960.6 arcseconds.

April 2015 lunar eclipse

A total lunar eclipse took place on 4 April 2015. It is the former of two total lunar eclipses in 2015, and the third in a tetrad. Other eclipses in the tetrad are those of 15 April 2014, 8 October 2014, and 28 September 2015.

September 2015 lunar eclipse

A total lunar eclipse took place between 27 and 28 September 2015. It was seen on Sunday evening, 27 September, in the Americas; while in Europe, Africa, and the Middle East, it was seen in the early hours of Monday morning, 28 September. It was the latter of two total lunar eclipses in 2015, and the final in a tetrad. Other eclipses in the tetrad are those of 15 April 2014, 8 October 2014, and 4 April 2015.

A penumbral lunar eclipse took place on January 20, 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.

January 2019 lunar eclipse

A total lunar eclipse occurred on 21 January 2019 UTC. For observers in the Americas, the eclipse took place between the evening of Sunday, 20 January and the early morning hours of Monday, 21 January. For observers in Europe and Africa, the eclipse occurred during the morning of 21 January. The Moon was near its perigee on 21 January and as such can be described as a "supermoon".

May 2021 lunar eclipse Total lunar eclipse

A total lunar eclipse occurred on 26 May 2021. A lunar eclipse occurs when the Moon moves into the Earth's shadow. This can occur only when the Sun, Earth, and Moon are exactly or very closely aligned with Earth between the other two, which can only happen at a full moon. The eclipsed moon appeared as a faint red disk in the sky due to a small amount of light being refracted through the earth's atmosphere; this appearance gives a lunar eclipse its nickname of a Blood Moon.

November 2020 lunar eclipse

A penumbral lunar eclipse took place on 30 November 2020. A penumbral lunar eclipse occurs at full moon when the Moon passes through Earth's penumbral shadow.

July 1963 lunar eclipse Partial lunar eclipse

A partial lunar eclipse took place on July 6, 1963 with an umbral eclipse magnitude of 0.70602. The Moon was strikingly shadowed in this deep partial eclipse which lasted 3 hours exactly, with 71% of the Moon in darkness at maximum. A partial lunar eclipse occurs when the Earth moves between the Sun and Moon but the three celestial bodies do not form a straight line in space. When that happens, a small part of the Moon's surface is covered by the darkest, central part of the Earth's shadow, called the umbra. The rest of the Moon is covered by the outer part of the Earth's shadow called the penumbra. It was the second of three lunar eclipses in 1963, the first was a penumbral lunar eclipse on January 9, 1963 and the third and last was on December 30, 1963.

November 1955 lunar eclipse

A partial lunar eclipse took place on November 29, 1955 with an umbral eclipse magnitude of 0.11899. A partial lunar eclipse happens when the Earth moves between the Sun and the Full Moon, but they are not precisely aligned. Only part of the Moon's visible surface moves into the dark part of the Earth's shadow. A partial lunar eclipse occurs when the Earth moves between the Sun and Moon but the three celestial bodies do not form a straight line in space. When that happens, a small part of the Moon's surface is covered by the darkest, central part of the Earth's shadow, called the umbra. The rest of the Moon is covered by the outer part of the Earth's shadow called the penumbra. It was the second of two lunar eclipses in 1955, first being the penumbral lunar eclipse on June 5.

Gamma (eclipse)

Gamma of an eclipse describes how centrally the shadow of the Moon or Earth strikes the other body. This distance, measured at the moment when the axis of the shadow cone passes closest to the center of the Earth or Moon, is stated as a fraction of the equatorial radius of the Earth or Moon.

Solar eclipse of November 22, 1984 20th-century total solar eclipse

A total solar eclipse occurred on November 22, 1984. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Totality was visible in Indonesia, Papua New Guinea and southern Pacific Ocean. West of the International Date Line the eclipse took place on November 23, including all land in the path of totality. Occurring only 2.1 days after perigee, the Moon's apparent diameter was fairly larger.

Solar eclipse of March 29, 1987 20th-century total solar eclipse

A total solar eclipse occurred at the Moon's ascending node of the orbit on March 29, 1987. It was a hybrid eclipse, with only a small portion of the central path as total, lasting a maximum of only 7.57 seconds. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Totality of this eclipse was not visible on any land, while annularity was visible in southern Argentina, Gabon, Equatorial Guinea, Cameroon, Central African Republic, Sudan, Ethiopia, Djibouti and Somaliland.

August 2053 lunar eclipse Penumbral

A penumbral lunar eclipse will take place on August 29, 2053.

References

  1. 1 2 "Total Penumbral lunar eclipses, Jean Meeus, 1980" (PDF).
  2. 1 2 "NASA - Catalog of Lunar Eclipses in Saros 19". eclipse.gsfc.nasa.gov.
  3. 1 2 "NASA - Catalog of Lunar Eclipses in Saros 32". eclipse.gsfc.nasa.gov.
  4. 1 2 "NASA - Catalog of Lunar Eclipses in Saros 132". eclipse.gsfc.nasa.gov.
  5. 1 2 "NASA - Catalog of Lunar Eclipses in Saros 58". eclipse.gsfc.nasa.gov.
  6. 1 2 "NASA - Catalog of Lunar Eclipses in Saros 95". eclipse.gsfc.nasa.gov.
  7. 1 2 3 "NASA - Catalog of Lunar Eclipses in Saros 114". eclipse.gsfc.nasa.gov.
  8. 1 2 "NASA - Catalog of Lunar Eclipses in Saros 169". eclipse.gsfc.nasa.gov.
  9. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 John Irwin (2017). "Consecutive penumbral total lunar eclipses". Archived from the original (PNG) on 2017-02-25. Retrieved 2018-09-08.The dot color indicates the sign (positive/negative) of the eclipse gamma.