Where Must the Moon Be in Order for a Lunar Eclipse to Occur?
When the Moon moves into the Earth's shadow
A lunar eclipse occurs when the Moon moves into the Earth's shadow.[1] This can occur only when the Sun, Earth, and Moon are exactly or very closely aligned (in syzygy) 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.[ citation needed ]
A totally eclipsed Moon is sometimes called a blood moon for its reddish color, which is caused by Earth completely blocking direct sunlight from reaching the Moon. The only light reflected from the lunar surface has been refracted by Earth's atmosphere. This light appears reddish for the same reason that a sunset or sunrise does: the Rayleigh scattering of bluer light.
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. A total lunar eclipse can last up to nearly 2 hours, while a total solar eclipse lasts only up to a few minutes at any given place, because the Moon's shadow is smaller. Also unlike solar eclipses, lunar eclipses are safe to view without any eye protection or special precautions, as they are dimmer than the full Moon.
For the date of the next eclipse, see § Recent and forthcoming lunar eclipses.
Types of lunar eclipse
A schematic diagram of the shadow cast by Earth. Within the umbra, the central region, the planet totally shields direct sunlight. In contrast, within the penumbra, the outer portion, the sunlight is only partially blocked. (Neither the Sun, Moon, and Earth sizes nor the distances between the bodies are to scale.)
A total penumbral lunar eclipse dims the Moon in direct proportion to the area of the Sun's disk covered by Earth. This comparison of the Moon (within the southern part of Earth's shadow) during the penumbral lunar eclipse of January 1999 (left) and the Moon outside the shadow (right) shows this slight darkening.
Earth's shadow can be divided into two distinctive parts: the umbra and penumbra. Earth totally occludes direct solar radiation within the umbra, the central region of the shadow. However, since the Sun's diameter appears about one-quarter of Earth's in the lunar sky, the planet only partially blocks direct sunlight within the penumbra, the outer portion of the shadow.
Penumbral lunar eclipse
This occurs when the Moon passes through Earth's penumbra. The penumbra causes a subtle dimming of the lunar surface, which is only visible to the naked eye when about 70% of the Moon's diameter has immersed into Earth's penumbra.[2] A special type of penumbral eclipse is a total penumbral lunar eclipse, during which the Moon lies exclusively within Earth's penumbra. Total penumbral eclipses are rare, and when these occur, the portion of the Moon closest to the umbra may appear slightly darker than the rest of the lunar disk.
Partial lunar eclipse
This occurs when only a portion of the Moon enters Earth's umbra, while a total lunar eclipse occurs when the entire Moon enters the planet's umbra. The Moon's average orbital speed is about 1.03 km/s (2,300 mph), or a little more than its diameter per hour, so totality may last up to nearly 107 minutes. Nevertheless, the total time between the first and the last contacts of the Moon's limb with Earth's shadow is much longer and could last up to 236 minutes.[3]
Total lunar eclipse
This occurs when the moon falls entirely within the earth's umbra. Just prior to complete entry, the brightness of the lunar limb-- the curved edge of the moon still being hit by direct sunlight-- will cause the rest of the moon to appear comparatively dim. The moment the moon enters a complete eclipse, the entire surface will become more or less uniformly bright. Later, as the moon's opposite limb is struck by sunlight, the overall disk will again become obscured. This is because as viewed from the Earth, the brightness of a lunar limb is generally greater than that of the rest of the surface due to reflections from the many surface irregularities within the limb: sunlight striking these irregularities is always reflected back in greater quantities than that striking more central parts, and is why the edges of full moons generally appear brighter than the rest of the lunar surface. This is similar to the effect of velvet fabric over a convex curved surface which to an observer will appear darkest at the center of the curve. It will be true of any planetary body with little or no atmosphere and an irregular cratered surface (e.g., Mercury) when viewed opposite the Sun.[4]
Central lunar eclipse
This is a total lunar eclipse during which the Moon passes through the centre of Earth's shadow, contacting the antisolar point. This type of lunar eclipse is relatively rare.
The relative distance of the Moon from Earth at the time of an eclipse can affect the eclipse's duration. In particular, when the Moon is near apogee, the farthest point from Earth in its orbit, its orbital speed is the slowest. The diameter of Earth's umbra does not decrease appreciably within the changes in the Moon's orbital distance. Thus, the concurrence of a totally eclipsed Moon near apogee will lengthen the duration of totality.
Selenelion
A selenelion or selenehelion, also called a horizontal eclipse, occurs where and when both the Sun and an eclipsed Moon can be observed at the same time. The event can only be observed just before sunset or just after sunrise, when both bodies will appear just above opposite horizons at nearly opposite points in the sky. A selenelion occurs during every total lunar eclipse-- it is an experience of the observer, not a planetary event separate from the lunar eclipse itself. Typically, observers on Earth located on high mountain ridges undergoing false sunrise or false sunset at the same moment of a total lunar eclipse will be able to experience it. Although during selenelion the Moon is completely within the Earth's umbra, both it and the Sun can be observed in the sky because atmospheric refraction causes each body to appear higher (i.e., more central) in the sky than its true geometric planetary position.[5]
Timing
As viewed from Earth, the Earth's shadow can be imagined as two concentric circles. As the diagram illustrates, the type of lunar eclipse is defined by the path taken by the Moon as it passes through Earth's shadow. If the Moon passes through the outer circle but does not reach the inner circle, it is a penumbral eclipse; if only a portion of the moon passes through the inner circle, it is a partial eclipse; and if entire Moon passes through the inner circle at some point, it is a total eclipse.
Contact points relative to the Earth's umbral and penumbral shadows, here with the Moon near is descending node
The timing of total lunar eclipses is determined by what are known as its "contacts" (moments of contact with Earth's shadow):[6]
- P1 (First contact): Beginning of the penumbral eclipse. Earth's penumbra touches the Moon's outer limb.
- U1 (Second contact): Beginning of the partial eclipse. Earth's umbra touches the Moon's outer limb.
- U2 (Third contact): Beginning of the total eclipse. The Moon's surface is entirely within Earth's umbra.
- Greatest eclipse: The peak stage of the total eclipse. The Moon is at its closest to the center of Earth's umbra.
- U3 (Fourth contact): End of the total eclipse. The Moon's outer limb exits Earth's umbra.
- U4 (Fifth contact): End of the partial eclipse. Earth's umbra leaves the Moon's surface.
- P4 (Sixth contact): End of the penumbral eclipse. Earth's penumbra no longer makes contact with the Moon.
Danjon scale
The following scale (the Danjon scale) was devised by André Danjon for rating the overall darkness of lunar eclipses:[7]
- L = 0: Very dark eclipse. Moon almost invisible, especially at mid-totality.
- L = 1: Dark eclipse, gray or brownish in coloration. Details distinguishable only with difficulty.
- L = 2: Deep red or rust-colored eclipse. Very dark central shadow, while outer edge of umbra is relatively bright.
- L = 3: Brick-red eclipse. Umbral shadow usually has a bright or yellow rim.
- L = 4: Very bright copper-red or orange eclipse. Umbral shadow is bluish and has a very bright rim.
Lunar versus solar eclipse
A solar eclipse occurs in the daytime at new moon, when the Moon is between Earth and the Sun, while a lunar eclipse occurs at night at full moon, when Earth passes between the Sun and the Moon.
There is often confusion between a solar eclipse and a lunar eclipse. While both involve interactions between the Sun, Earth, and the Moon, they are very different in their interactions.
Lunar eclipse appearance
In a lunar eclipse, the Moon often passes through two regions of Earth's shadow: an outer penumbra, where direct sunlight is dimmed, and an inner umbra, where indirect and much dimmer sunlight refracted by Earth's atmosphere shines on the Moon, leaving a reddish color. This can be seen in different exposures of a partial lunar eclipse, for example here with exposures of 1/80, 2/5, and 2 seconds.
The Moon does not completely darken as it passes through the umbra because of the refraction of sunlight by Earth's atmosphere into the shadow cone; if Earth had no atmosphere, the Moon would be completely dark during the eclipse.[8] The reddish coloration arises because sunlight reaching the Moon must pass through a long and dense layer of Earth's atmosphere, where it is scattered. Shorter wavelengths are more likely to be scattered by the air molecules and small particles; thus, the longer wavelengths predominate by the time the light rays have penetrated the atmosphere. Human vision perceives this resulting light as red. This is the same effect that causes sunsets and sunrises to turn the sky a reddish color. An alternative way of conceiving this scenario is to realize that, as viewed from the Moon, the Sun would appear to be setting (or rising) behind Earth.
From the Moon, a lunar eclipse would show a ring of reddish-orange light surrounding a silhouetted Earth in the lunar sky.
The amount of refracted light depends on the amount of dust or clouds in the atmosphere; this also controls how much light is scattered. In general, the dustier the atmosphere, the more that other wavelengths of light will be removed (compared to red light), leaving the resulting light a deeper red color. This causes the resulting coppery-red hue of the Moon to vary from one eclipse to the next. Volcanoes are notable for expelling large quantities of dust into the atmosphere, and a large eruption shortly before an eclipse can have a large effect on the resulting color.
Lunar eclipse in culture
Several cultures have myths related to lunar eclipses or allude to the lunar eclipse as being a good or bad omen. The Egyptians saw the eclipse as a sow swallowing the Moon for a short time; other cultures view the eclipse as the Moon being swallowed by other animals, such as a jaguar in Mayan tradition, or a three legged toad in China. Some societies thought it was a demon swallowing the Moon, and that they could chase it away by throwing stones and curses at it.[9] The Ancient Greeks correctly believed the Earth was round and used the shadow from the lunar eclipse as evidence.[10] Some Hindus believe in the importance of bathing in the Ganges River following an eclipse because it will help to achieve salvation.[11]
Inca
Similarly to the Mayans, the Inca believed that lunar eclipses occurred when a jaguar would eat the Moon, which is why a blood moon looks red. The Incans also believed that once the jaguar finished eating the Moon, it could come down and devour all the animals on Earth, so they would take spears and shout at the Moon to keep it away.[12]
Mesopotamians
The ancient Mesopotamians believed that a lunar eclipse was when the Moon was being attacked by seven demons. This attack was more than just one on the Moon, however, for the Mesopotamians linked what happened in the sky with what happened on the land, and because the king of Mesopotamia represented the land, the seven demons were thought to be also attacking the king. In order to prevent this attack on the king, the Mesopotamians made someone pretend to be the king so they would be attacked instead of the true king. After the lunar eclipse was over, the substitute king was made to disappear (possibly by poisoning).[12]
Chinese
In some Chinese cultures, people would ring bells to prevent a dragon or other wild animals from biting the Moon.[13] In the nineteenth century, during a lunar eclipse, the Chinese navy fired its artillery because of this belief.[14] During the Zhou Dynasty in the Book of Songs, the sight of a red Moon engulfed in darkness was believed to foreshadow famine or disease.[15]
Blood moon
Certain lunar eclipses have been referred to as "blood moons" in popular articles but this is not a scientifically-recognized term.[16] This term has been given two separate, but overlapping, meanings.
The first, and simpler, meaning relates to the reddish color a totally eclipsed Moon takes on to observers on Earth.[17] As sunlight penetrates the atmosphere of Earth, the gaseous layer filters and refracts the rays in such a way that the green to violet wavelengths on the visible spectrum scatter more strongly than the red, thus giving the Moon a reddish cast.[18]
The second meaning of "blood moon" has been derived from this apparent coloration by two fundamentalist Christian pastors, Mark Blitz and John Hagee.[16] [19] They claimed that the 2014–15 "lunar tetrad" of four lunar eclipses coinciding with the feasts of Passover and Tabernacles matched the "moon turning to blood" described in the Book of Joel of the Hebrew Bible.[19] This tetrad was claimed to herald the Second Coming of Christ and the Rapture as described in the Book of Revelation on the date of the first of the eclipses in this sequence on April 15, 2014.[20]
Occurrence
This collage shows the transitional stages of a lunar eclipse.
At least two lunar eclipses and as many as five occur every year, although total lunar eclipses are significantly less common. If the date and time of an eclipse is known, the occurrences of upcoming eclipses are predictable using an eclipse cycle, like the saros.
Recent and forthcoming lunar eclipses
Eclipses occur only during an eclipse season, when the Sun appears to pass near either node of the Moon's orbit.
| Lunar eclipse series sets from 2002–2005 | ||||||||
|---|---|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||||
| Saros Photo | Date View | Type Chart | Gamma | Saros Photo | Date View | Type Chart | Gamma | |
| 111 | 2002 May 26 | penumbral | 1.1759 | 116 | 2002 Nov 20 | penumbral | -1.1127 | |
121 | 2003 May 16 | total  | 0.4123 | 126 | 2003 Nov 09 | total  | -0.4319 | |
131 | 2004 May 04 | total  | -0.3132 | 136 | 2004 Oct 28 | total  | 0.2846 | |
| 141 | 2005 Apr 24 | penumbral | -1.0885 | 146 | 2005 Oct 17 | partial | 0.9796 | |
| Last set | 2002 Jun 24 | Last set | 2001 Dec 30 | |||||
| Next set | 2006 Mar 14 | Next set | 2006 Sep 7 | |||||
| Lunar eclipse series sets from 2006–2009 | ||||||||
|---|---|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||||
| Saros # and photo | Date Viewing | Type Chart | Gamma | Saros # and photo | Date Viewing | Type Chart | Gamma | |
113 | 2006 Mar 14 | penumbral | 1.0211 | 118 | 2006 Sep 7 | partial | -0.9262 | |
123 | 2007 Mar 03 | total  | 0.3175 | 128 | 2007 Aug 28 | total  | -0.2146 | |
133 | 2008 Feb 21 | total  | -0.3992 | 138 | 2008 Aug 16 | partial | 0.5646 | |
143 | 2009 Feb 09 | penumbral | -1.0640 | 148 | 2009 Aug 06 | penumbral | 1.3572 | |
| Last set | 2005 Apr 24 | Last set | 2005 Oct 17 | |||||
| Next set | 2009 Dec 31 | Next set | 2009 Jul 07 | |||||
| Lunar eclipse series sets from 2009–2013 | ||||||||
|---|---|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||||
| Saros # Photo | Date Viewing | Type chart | Gamma | Saros # Photo | Date Viewing | Type chart | Gamma | |
| 110 | 2009 Jul 07 | penumbral | -1.4916 | 115 | 2009 Dec 31 | partial | 0.9766 | |
120 | 2010 Jun 26 | partial | -0.7091 | 125 | 2010 Dec 21 | total  | 0.3214 | |
130 | 2011 Jun 15 | total  | 0.0897 | 135 | 2011 Dec 10 | total  | -0.3882 | |
140 | 2012 Jun 04 | partial | 0.8248 | 145 | 2012 Nov 28 | penumbral | -1.0869 | |
| 150 | 2013 May 25 | penumbral | 1.5351 | |||||
| Last set | 2009 Aug 06 | Last set | 2009 Feb 9 | |||||
| Next set | 2013 Apr 25 | Next set | 2013 Oct 18 | |||||
| Lunar eclipse series sets from 2013–2016 | ||||||||
|---|---|---|---|---|---|---|---|---|
| Ascending node | Descending node | |||||||
| Saros | Viewing date | Type | Gamma | Saros | Viewing date | Type | Gamma | |
112 | 2013 Apr 25 | Partial | -1.0121 | 117 | 2013 Oct 18 | Penumbral | 1.1508 | |
122 | 2014 Apr 15 | Total  | -0.3017 | 127 | 2014 Oct 08 | Total  | 0.3827 | |
132 | 2015 Apr 04 | Total  | 0.4460 | 137 | 2015 Sep 28 | Total  | -0.3296 | |
| 142 | 2016 Mar 23 | Penumbral | 1.1592 | 147 | 2016 Sep 16 | Penumbral | -1.0549 | |
| Last set | 2013 May 25 | Last set | 2012 Nov 28 | |||||
| Next set | 2017 Feb 11 | Next set | 2016 Aug 18 | |||||
| Lunar eclipse series sets from 2016–2020 | ||||||||
|---|---|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||||
| Saros | Date | Type Viewing | Gamma | Saros | Date Viewing | Type Chart | Gamma | |
| 109 | 2016 Aug 18 | Penumbral | 1.5641 | 114 | 2017 Feb 11 | Penumbral | -1.0255 | |
119 | 2017 Aug 07 | Partial | 0.8669 | 124 | 2018 Jan 31 | Total  | -0.3014 | |
129 | 2018 Jul 27 | Total  | 0.1168 | 134 | 2019 Jan 21 | Total  | 0.3684 | |
139 | 2019 Jul 16 | Partial | -0.6430 | 144 | 2020 Jan 10 | Penumbral | 1.2406 | |
| 149 | 2020 Jul 05 | Penumbral | -1.3639 | |||||
| Last set | 2016 Sep 16 | Last set | 2016 Mar 23 | |||||
| Next set | 2020 Jun 05 | Next set | 2020 Nov 30 | |||||
| Lunar eclipse series sets from 2020–2023 | ||||||||
|---|---|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||||
| Saros | Date | Type Viewing | Gamma | Saros | Date Viewing | Type Chart | Gamma | |
111 | 2020 Jun 05 | Penumbral | 1.24063 | 116 | 2020 Nov 30 | Penumbral | -1.13094 | |
121 | 2021 May 26 | Total  | 0.47741 | 126 | 2021 Nov 19 | Partial | -0.45525 | |
| 131 | 2022 May 16 | Total  | -0.25324 | 136 | 2022 Nov 08 | Total  | 0.25703 | |
| 141 | 2023 May 05 | Penumbral | -1.03495 | 146 | 2023 Oct 28 | Partial | 0.94716 | |
| Last set | 2020 Jul 05 | Last set | 2020 Jan 10 | |||||
| Next set | 2024 Mar 25 | Next set | 2024 Sep 18 | |||||
| Lunar eclipse series sets from 2024–2027 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Date | Type Viewing | Saros | Date Viewing | Type Chart | |
| 113 | 2024 Mar 25 | Penumbral | 118 | 2024 Sep 18 | Partial | |
| 123 | 2025 Mar 14 | Total  | 128 | 2025 Sep 07 | Total  | |
| 133 | 2026 Mar 03 | Total  | 138 | 2026 Aug 28 | Partial | |
| 143 | 2027 Feb 20 | Penumbral | 148 | 2027 Aug 17 | Penumbral | |
| Last set | 2023 May 05 | Last set | 2023 Oct 28 | |||
| Next set | 2028 Jan 12 | Next set | 2027 Jul 18 | |||
| Lunar eclipse series sets from 2027–2031 | ||||||
|---|---|---|---|---|---|---|
| Descending node | Ascending node | |||||
| Saros | Date Viewing | Type Chart | Saros | Date Viewing | Type Chart | |
| 110 | 2027 Jul 18 | Penumbral | 115 | 2028 Jan 12 | Partial | |
| 120 | 2028 Jul 06 | Partial | 125 | 2028 Dec 31 | Total  | |
| 130 | 2029 Jun 26 | Total  | 135 | 2029 Dec 20 | Total  | |
| 140 | 2030 Jun 15 | Partial | 145 | 2030 Dec 09 | Penumbral | |
| 150 | 2031 Jun 05 | Penumbral | ||||
| Last set | 2027 Aug 17 | Last set | 2027 Feb 20 | |||
| Next set | 2031 May 07 | Next set | 2031 Oct 30 | |||
See also
- Lists of lunar eclipses and List of 21st-century lunar eclipses
- Lunar occultation
- Moon illusion
- Orbit of the Moon
- Solar eclipse
References
- ^ McClure, Bruce (July 27, 2018). "Century's Longest Lunar Eclipse July 27". EarthSky . Retrieved August 1, 2018.
- ^ H. Mucke, J. Meeus (1992). Canon of Lunar Eclipses -2002 to +2526 (3rd ed.). Astronomisches Büro Wien. p. V.
- ^ Karttunen, Hannu (2007). Fundamental Astronomy. Springer. p. 139. ISBN9783540341444.
- ^ "Lunar Limb Magic". Astronomy.com. 27 November 2018.
- ^ "Observing Blog - In Search of Selenelion". Sky & Telescope. 2010-06-26. Archived from the original on 2011-12-20. Retrieved 2011-12-08 .
- ^ Clarke, Kevin. "On the nature of eclipses". Inconstant Moon. Cyclopedia Selenica. Retrieved 19 December 2010.
- ^ Deans, Paul; MacRobert, Alan M. (July 16, 2006). "Observing and Photographing Lunar Eclipses". Sky & Telescope. F+W.
- ^ Espenak, Fred; Meeus, Jean. "Visual Appearance of Lunar Eclipses". NASA.
The troposphere and stratosphere act together as a ring-shaped lens that refracts heavily reddened sunlight into Earth's umbral shadow.
- ^ Littmann, Mark; Espenak, Fred; Willcox, Ken (2008). "Chapter 4: Eclipses in Mythology". Totality Eclipses of the Sun (3rd ed.). New York: Oxford University Press. ISBN978-0-19-953209-4.
- ^ Pollack, Rebecca. "Ancient Myths Revised with Lunar Eclipse". University of Maryland. Retrieved 2 October 2014.
- ^ Ani. "Hindus take a dip in the Ganges during Lunar Eclipse". Yahoo News . Retrieved 2 October 2014.
- ^ a b Lee, Jane (14 April 2014). "Lunar Eclipse Myths From Around the World". National Geographic . Retrieved 9 October 2014.
- ^ Quilas, Ma Evelyn. "Interesting Facts and Myths about Lunar Eclipse". LA Times . Retrieved 2 October 2014.
- ^ "Mythology of the Lunar Eclipse". LifeAsMyth.com.
- ^ Kaul, Gayatri (15 June 2011). "What Lunar Eclipse Means in Different Parts of the World". India.com . Retrieved 6 October 2014.
- ^ a b Sappenfield, Mark (13 April 2014). "Blood Moon to arrive Monday night. What is a Blood Moon?". Christian Science Monitor . Retrieved 8 February 2018.
- ^ Nigro, Nicholas (2010). Knack Night Sky: Decoding the Solar System, from Constellations to Black Holes. Globe Pequot. pp. 214–5. ISBN978-0-7627-6604-8.
- ^ "All you need to know about the 'blood moon'". theguardian. 28 September 2015.
- ^ a b "What is a Blood Moon?". Earth & Sky. 24 April 2014. Retrieved 30 May 2014.
- ^ Bailey, Sarah Pulliam (15 April 2014). "'Blood moon' sets off apocalyptic debate among some Christians". The Washington Post. Religion News Service. Retrieved 8 February 2018.
- ^ "Lunar Eclipse @ ESO". European Southern Observatory. Retrieved 14 August 2017.
Further reading
- Bao-Lin Liu, Canon of Lunar Eclipses 1500 B.C.-A.D. 3000. Willmann-Bell, Richmond VA, 1992
- Jean Meeus and Hermann Mucke Canon of Lunar Eclipses -2002 to +2526 (3rd edition). Astronomisches Büro, Vienna, 1992
- Espenak, F., Fifty Year Canon of Lunar Eclipses: 1986–2035. NASA Reference Publication 1216, 1989
- Espenak, F. Thousand Year Canon of Lunar Eclipses 1501 to 2500, Astropixels Publishing, Portal AZ, 2014
External links
- Lunar Eclipse Essentials: video from NASA
- Animated explanation of the mechanics of a lunar eclipse, University of South Wales
- U.S. Navy Lunar Eclipse Computer
- NASA Lunar Eclipse Page
- Search among the 12,064 lunar eclipses over five millennium and display interactive maps
- Lunar Eclipses for Beginners
- Tips on photographing the lunar eclipse from New York Institute of Photography
- Lunar Eclipse 08 October 2014 on YouTube
Where Must the Moon Be in Order for a Lunar Eclipse to Occur?
Source: https://en.wikipedia.org/wiki/Lunar_eclipse
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