A shorter exposure shows less nebulosity.
The Pleiades (Ple.ia.des |[ˈpli.ə.diz]) - also known as
M45, the Seven Sisters, or Subaru (in Japan) - is the name of an open
cluster in the constellation of Taurus. It is among the nearest to the
Earth of all open clusters, probably the best known and certainly the most
striking to the naked eye. This asterism is sometimes referred to as the Maia Nebula,
perhaps erroneously considering that the reflection nebulosity surrounding Maia is extrinsic (see below).
The cluster is dominated by hot blue stars, which have formed within the last
100 million years. Dust that forms faint reflection nebulosity around the brightest
stars was thought at first to be left over from the formation of the cluster but is now known to be an unrelated dust cloud that
the stars are currently passing through. Astronomers estimate that the cluster will survive for about another 250 million years,
when it will have dispersed due to gravitational interactions with the spiral arms of the
galaxy and giant molecular clouds.
Observational history
The Pleiades are a prominent sight in winter in the Northern Hemisphere and in summer in the
Southern Hemisphere, and have been known since antiquity to cultures all around the
world, including the Māori and Australian
Aborigines, the Chinese, the Maya called them Tzab-ek,
the Aztec and the Sioux of North
America. Some Greek astronomers considered them to be a distinct constellation, and they are mentioned by Hesiod, and in Homer's Iliad and Odyssey. They are
also mentioned three times in the Bible (Job 9:9, 38:31;
Amos 5:8). The Pleiades (Krittika) are particularly
revered in Hindu mythology as the six mothers of the war god Skanda, who developed six faces, one for each of them. Some scholars of Islam suggested that the Pleiades (At-thuraiya) are the Star in Najm which is mentioned in the Quran.
They have long been known to be a physically related group of stars rather than any chance alignment. The Reverend
John Michell calculated in 1767 that the probability of a
chance alignment of so many bright stars was only 1 in 500,000, and so correctly surmised that the Pleiades and many other
clusters of stars must be physically related.[4] When
studies were first made of the stars' proper motions, it was found that they are all
moving in the same direction across the sky, at the same rate, further demonstrating that they were related.
Charles Messier measured the position of the cluster and included it as M45 in his
catalogue of comet-like objects, published
in 1771. Along with the Orion Nebula and the Praesepe cluster, Messier's inclusion of the Pleiades has been noted as curious, as most of Messier's
objects were much fainter and more easily confused with comets—something which seems scarcely possible for the Pleiades. One
possibility is that Messier simply wanted to have a larger catalogue than his scientific rival Lacaille, whose 1755 catalogue contained 42 objects, and so he
added some bright, well-known objects to boost his list.[5]
Distance
The distance to the Pleiades is an important first step in the so-called cosmic
distance ladder, a sequence of distance scales for the whole universe. The size of this first step calibrates the whole
ladder, and the scale of this first step has been estimated by many methods. As the cluster is so close to the Earth, its
distance is relatively easy to measure. Accurate knowledge of the distance allows astronomers to plot a Hertzsprung-Russell Diagram for the cluster which, when compared to those plotted for
clusters whose distance is not known, allows their distances to be estimated. Other methods can then extend the distance scale
from open clusters to galaxies and clusters of galaxies, and a cosmic distance
ladder can be constructed. Ultimately astronomers' understanding of the age and future evolution of the universe is
influenced by their knowledge of the distance to the Pleiades.
Results prior to the launch of the Hipparcos satellite generally found that the Pleiades
were about 135 parsecs away from Earth. Hipparcos caused consternation among astronomers by
finding a distance of only 118 parsecs by measuring the parallax of stars in the cluster—a
technique which should yield the most direct and accurate results. Later work has consistently found that the Hipparcos distance
measurement for the Pleiades was in error, but it is not yet known why the error occurred.[6] The distance to the Pleiades is currently thought to be the higher value of about
135 parsecs.[2][3]
Composition
X-ray images of the Pleiades reveal the stars with the hottest atmospheres. Green squares indicate the seven optically brightest
stars.
The cluster core radius is about 8 light years and tidal radius is about 43 light years.
The cluster contains over 1000 statistically confirmed members, although this figure excludes unresolved binary stars.[7] It is dominated by
young, hot blue stars, up to 14 of which can be seen with the naked eye depending
on local observing conditions. The arrangement of the brightest stars is somewhat similar to Ursa
Major and Ursa Minor. The total mass contained in the cluster is estimated to be about
800 solar masses.[8]
The cluster contains many brown dwarfs, which are objects with less than about 8% of the
Sun's mass, not heavy enough for nuclear fusion reactions to
start in their cores and become proper stars. They may constitute up to 25% of the total population of the cluster, although they
contribute less than 2% of the total mass.[9] Astronomers
have made great efforts to find and analyse brown dwarfs in the Pleiades and other young clusters, because they are still
relatively bright and observable, while brown dwarfs in older clusters have faded and are much more difficult to study.
Also present in the cluster are several white dwarfs. Given the young age of the cluster
normal stars are not expected to have had time to evolve into white dwarfs, a process which normally takes several billion years.
It is believed that, rather than being individual low- to intermediate-mass stars, the progenitors of the white dwarfs must have
been high-mass stars in binary systems. Transfer of mass from the higher-mass
star to its companion during its rapid evolution would result in a much quicker route to the formation of a white dwarf, although
the details of this supposed transfer from a deeper gravity well to a lesser are unexplained.
Age and future evolution
Ages for star clusters can be estimated by comparing the H-R diagram for
the cluster with theoretical models of stellar evolution, and using this technique,
ages for the Pleiades of between 75 and 150 million years have been estimated. The spread in estimated ages is a result of
uncertainties in stellar evolution models. In particular, models including a phenomenon known as convective overshoot, in which a convective zone within a
star penetrates an otherwise non-convective zone, result in higher apparent ages.
Another way of estimating the age of the cluster is by looking at the lowest-mass objects. In normal main sequence stars, lithium is rapidly destroyed in nuclear fusion reactions, but brown dwarfs can retain their lithium. Due to lithium's very low ignition
temperature of 2.5 million kelvins, the highest-mass brown dwarfs will burn it eventually,
and so determining the highest mass of brown dwarfs still containing lithium in the cluster can give an idea of its age. Applying
this technique to the Pleiades gives an age of about 115 million years.[10][11]
The cluster's relative motion will eventually lead it to be located, as seen from Earth
many millennia in the future, passing below the feet of what is currently the constellation of Orion. Also, like most open
clusters, the Pleiades will not stay gravitationally bound forever, as some component stars will be ejected after close
encounters and others will be stripped by tidal gravitational fields. Calculations suggest that the cluster will take about 250
million years to disperse, with gravitational interactions with giant molecular clouds
and the spiral arms of the galaxy also hastening its demise.
Reflection nebulosity
Hubble Space Telescope image of reflection nebulosity near Merope
Under ideal observing conditions, some hint of nebulosity may be seen around the cluster, and this shows up in long-exposure
photographs. It is a reflection nebula, caused by dust reflecting the blue light of
the hot, young stars.
It was formerly thought that the dust was left over from the formation of the cluster,
but at the age of about 100 million years generally accepted for the cluster, almost all the dust originally present would have
been dispersed by radiation pressure. Instead, it seems that the cluster is simply
passing through a particularly dusty region of the interstellar medium.
Studies show that the dust responsible for the nebulosity is not uniformly distributed, but is concentrated mainly in two
layers along the line of sight to the cluster. These layers may have been formed by deceleration due to radiation pressure as the
dust has moved towards the stars.[12]
Names and technical information
The nine brightest stars of the Pleiades are named for the Seven Sisters of
Greek mythology: Sterope, Merope, Electra, Maia,
Taygete, Celaeno and Alcyone,
along with their parents Atlas and Pleione. As daughters of Atlas, the Hyades were sisters
of the Pleiades. The English name of the cluster itself is of Greek origin, though of
uncertain etymology. Suggested derivations include: from πλεîν plein, to sail, making the Pleiades the "sailing ones";
from pleos, full or many; or from peleiades, flock of doves. The following table
gives details of the brightest stars in the cluster:
Pleiades Bright Stars
| Name |
Pronunciation (IPA & respelling) |
Designation |
Apparent magnitude |
Stellar classification |
| Alcyone |
/æl'saɪəni/, al-sye'-ə-nee |
Eta (25) Tauri |
2.86 |
B7IIIe |
| Atlas |
/'ætləs/, at'-ləs |
27 Tauri |
3.62 |
B8III |
| Electra |
/i'lɛktrə/, ee-lek'-trə |
17 Tauri |
3.70 |
B6IIIe |
| Maia |
/'meɪə, 'maɪə/; may'-ə, mye'-ə |
20 Tauri |
3.86 |
B7III |
| Merope |
/'mɛrəpi/, mair'-ə-pee |
23 Tauri |
4.17 |
B6IVev |
| Taygeta |
/tei'ɪʤəti/, tay-ij'-ə-tee |
19 Tauri |
4.29 |
B6V |
| Pleione |
/'plaɪəni/, plye'-ə-nee |
28 (BU) Tauri |
5.09 (var.) |
B8IVep |
| Celaeno |
/sə'lino/, sə-lee'-no |
16 Tauri |
5.44 |
B7IV |
| Asterope |
/ə'stɛrəpi/, ə-stair'-ə-pee |
21 and 22 Tauri |
5.64;6.41 |
B8Ve/B9V |
| — |
— |
18 Tauri |
5.65 |
B8V |
In folklore
| “ |
Can you bind the beautiful Pleiades?
Can you loose the cords of Orion? |
” |
| |
|
The Pleiades' high visibility in the night sky has guaranteed it a special place in many cultures, both ancient and modern. In
Greek mythology, they represented the Seven
Sisters, while to the Vikings, they were Freyja's
hens, and their name in many old European languages compares them to a hen with chicks.
To the Bronze Age people of Europe, such as the Celts (and
probably considerably earlier), the Pleiades were associated with mourning and with funerals, since at that time in history, on
the cross-quarter day between the autumn
equinox and the winter solstice (see Samhain,
also Halloween or All Souls
Day), which was a festival devoted to the remembrance of the dead, the cluster rose in the eastern sky as the sun's light
faded in the evening. It was from this acronychal rising that the Pleiades became
associated with tears and mourning. As a result of precession over the centuries, the
Pleiades no longer marked the festival, but the association has nevertheless persisted, and accounts for the significance of the
Pleiades astrologically.
The early Monte Alto Culture and others in Guatemala such as Ujuxte and Takalik
Abaj, made its early observatories, using the Pleiades and Eta Draconnis as reference, they were called the
seven sisters, and thought to be their original land.[13]
A bronze disk, 1600 BC, from Nebra, Germany, is one of the oldest known representations of the cosmos. The Pleiades are top
right. See
Nebra sky disk
Heliacal risings very often mark important calendar points for ancient peoples.[14] The heliacal rising of the Pleiades (around June) also begins the new year for the Māori of New Zealand, who call the Pleiades Matariki. There is an analogous holiday in Hawaiʻi known as Makaliʻi.
The ancient Aztecs of Mexico and Central America based their calendar upon the Pleiades. Their calendric year began when priests
first remarked the asterism rising heliacally in the east, immediately before the sun's dawn light obliterated the view of the
stars.
Indigenous Australians
Depending on the tribe or clan, some Indigenous Australian peoples believed
the Pleiades was a woman who had been nearly raped by Kidili, the
man in the moon.
Another version, often painted by Gabriella Possum Nungurayyi as this is her dreaming (or creation story), daughter of the late Clifford Possum Tjapaltjarri from the Central desert art movement of Papunya, depicts the story of seven Napaltjarri sisters being chased by a man named Jilbi
Tjakamarra. He would practice love magic to seduce the sisters but they had no intention of being with him and ran away. They sat
down at Uluru to search for honey ants but when they saw Jilbi, they went to Kurlunyalimpa and
with the spirits of Uluru, transformed into stars. Jilbi transforms himself into what is commonly known as the Morning Star in Orion's belt [citation needed], thus continuing to chase the seven
sisters across the sky. (Source:Aboriginal Fine Art
Gallery)
Native Americans
The Sioux of North America had a legend that linked the
origin of the Pleiades to Devils Tower. According to the Seris (of northwestern Mexico), these stars are seven women who are giving birth. The constellation is known as
Cmaamc, which is apparently an archaic plural of the noun cmaam "woman".[15]
It was common among the indigenous peoples of the Americas to
measure keenness of vision by the number of stars the viewer could see in the
Pleiades, a practice which was also used in historical Europe, especially in Greece.
The Native American tribe, the Kiowa, had a myth similar to the Sioux that explained the creation of the Pleiades. According
to the Kiowa there were seven young maidens that went out to play and were spotted by several giant bears. The bears saw the
young women and began to chase them. In an effort to escape the bears the women climbed on top of a rock and prayed to the spirit
of the rock to save them. Hearing their prayers the rock began to rise from the ground towards the Heavens so that the bears
couldn't reach the maidens. The seven women reached the sky and were then turned into the star constellation we know today. The
bears in an effort to climb the rock left deep claw marks in the sides which had become too steep to climb. The rock later became
known as Devil's Tower which is located in the state of Wyoming.[citation needed]
In the ancient Andes, the Pleiades were associated with abundance, because they return to the
Southern Hemisphere sky each year at harvest-time. In Quechua they are called collca', or storehouse.
Ukrainian
In Ukrainian traditional folklore the Pleiades are known as Стожари (Stozhary), Волосожари
(Volosozhary), or Баби-Звізди (Baby-Zvizdy).
'Stozhary' can be etymologically traced to "стожарня" (stozharnya) meaning a 'granary', 'storehouse for hay and crops', or can
also be reduced to the root "сто-жар", (sto-zhar) meaning 'hundred-fold glowing'.[16]
'Volosozhary' (the ones who's hair is glowing), or 'Baby-Zvizdy' (female-stars) refer to the female tribal deities.
Accordingly to the legend, seven maids lived long time ago. They used to dance the traditional round dances and sing the glorious
songs to honor the gods. After their death the gods turned them into water nymphs, and, having taken them to the Heavens, settled
them upon the seven stars, where they dance their round dances (symbolic for moving the time) till now. (see article in Ukrainian
Wikipedia)
In Ukraine this asterism is considered a female talisman until recent times.
Other cultures
In Japan, the Pleiades are known as 昴 Subaru, and have given their name to the car manufacturer
whose logo incorporates six stars to represent the five smaller companies that merged into one. Subaru Telescope, located in Mauna Kea Observatory on Hawaii, is named after the Pleiades also.
In Chinese constellations, they are 昴 mao, the Hairy Head of the white tiger of the West, while the name of the Hindu God
Kartikeya means him of the Pleiades.
In the Swahili language of East Africa they are
called "kilimia" (Proto-Bantu *ki-dimida in Bantu
areas E, F, G, J, L, and S) which comes from the verb -lima meaning "dig" or "cultivate" as their visibility was taken as
a sign to prepare digging as the onset of the rain was near.
In the closely related Sesotho language of the Southern Africa's Basotho people the Pleiades is called "Seleme se
setshehadi" ("the female planter"). Its disappearance in April (the 10th month) and the appearance of the star Achernar signals the beginning of the cold season. Like many other Southern African cultures, Basotho associate
its visibility with agriculture and plenty.
In Western astrology they represent coping with sorrow[17] and were considered a single one of the medieval fixed stars. As such, they are associated with
quartz and fennel.
In Indian astrology the Pleiades were known as the asterism (nakshatra) Kṛttikā (which in Sanskrit is translated as "the cutters.")[18] The Pleiades are called the star of fire, and their ruling deity is the Vedic god
Agni, the god of the sacred fire. It is one of the most prominent of the nakshatras, and is
associated with anger and stubbornness.
The word has acquired a meaning of "multitude", inspiring the name of the French literary movement La Pléiade and an earlier group of Alexandrian poets, the
Alexandrian Pleiad.
References
- ^ a b c d SIMBAD Astronomical Database. Results for NGC 2244. Retrieved on 2007-04-20.
- ^ a b Percival, S. M.; Salaris, M.; Groenewegen, M. A. T. (2005), The distance to the Pleiades. Main
sequence fitting in the near infrared, Astronomy and Astrophysics, v.429, p.887.
- ^ a b Zwahlen, N.; North, P.; Debernardi, Y.; Eyer, L.; Galland, F.; Groenewegen,
M. A. T.; Hummel, C. A. (2004), A purely geometric distance to the binary star Atlas, a member of the Pleiades, Astronomy and Astrophysics,
v.425, p.L45.
- ^ Michell J. (1767), An Inquiry into the probable Parallax, and Magnitude,
of the Fixed Stars, from the Quantity of Light which they afford us, and the particular Circumstances of their Situation,
Philosophical Transactions, v. 57, p. 234-264
- ^ Frommert, Hartmut (1998) "Messier Questions &
Answers". Retrieved March 1, 2005.
- ^ Soderblom D.R., Nelan E., Benedict G.F., McArthur B., Ramirez I., Spiesman
W., Jones B.F. (2005), Confirmation of Errors in Hipparcos Parallaxes from Hubble Space Telescope Fine Guidance Sensor Astrometry of the
Pleiades, The Astronomical Journal, v. 129, pp. 1616-1624.
- ^ Adams, Joseph D.; Stauffer, John R.; Monet, David G.; Skrutskie, Michael
F.; Beichman, Charles A. (2001), The Mass and Structure of the Pleiades Star Cluster from 2MASS, The Astronomical Journal, v.121, p.2053.
- ^ Adams, Joseph D.; Stauffer, John R.; Monet, David G.; Skrutskie, Michael
F.; Beichman, Charles A. (2001), The Mass and Structure of the Pleiades Star Cluster from 2MASS, The Astronomical Journal, v.121, p.2053.
- ^ Moraux, E.; Bouvier, J.; Stauffer, J. R.; Cuillandre, J.-C. (2003),
Brown dwarfs in the
Pleiades cluster: Clues to the substellar mass function, Astronomy and Astrophysics, v.400, p.891.
- ^ Basri G., Marcy G. W., Graham J. R. (1996), Lithium in Brown Dwarf Candidates:
The Mass and Age of the Faintest Pleiades Stars, Astrophysical Journal v.458, p.600
- ^ Ushomirsky, G., Matzner, C., Brown, E., Bildsten, L., Hilliard, V.,
Schroeder, P. (1998), Light-Element Depletion in Contracting Brown Dwarfs and Pre-Main-Sequence Stars, Astrophysical Journal v.497,
p.253
- ^ Gibson, Steven J.; Nordsieck, Kenneth H. (2003), The Pleiades Reflection Nebula. II.
Simple Model Constraints on Dust Properties and Scattering Geometry, The Astrophysical Journal, v.589, p. 362
- ^ Maya Astronomy
- ^ Brad Schaefer (Yale University). Heliacal Rising: Definitions,
Calculations, and some Specific Cases (Essays from Archaeoastronomy & Ethnoastronomy News, the Quarterly Bulletin
of the Center for Archaeoastronomy, Number 25.)
- ^ Moser, Mary B.; Stephen A. Marlett (2005). Comcáac quih yaza quih hant ihíip hac: Diccionario seri-español-inglés (in Spanish and English).
Hermosillo, Sonora and Mexico City: Universidad de Sonora and Plaza y Valdés Editores.
- ^ The Comprehensive Dictionary of the Contemporary Ukrainian Language. ©
Perun Publishers, 2005.
- ^ Morse, Eric (1988). The Living Stars. London: Amethyst Books.
- ^ Dennis M. Harness. The Nakshatras: The Lunar Mansions of Vedic
Astrology. Lotus Press (Twin Lakes WI, 1999.) ISBN 978-0-914955-83-2
External links
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