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| Messier 45: The Pleiades... |
Object: Messier 45
Type: Open cluster with reflection nebula
Constellation: Taurus
Distance: 440 light years
Equipment: Atik 460/EFW 2, Samyang 135mm lens@ F2, Vixen GPDX mount, guiding with Lodestar X2/PHD
Date: January 8th. 2023
Subframes: 12 x 300s each for LRGB, flats, bias as dark frames.
At a distance of about 440 light years, the Pleiades is one of the nearest star clusters to Earth. It is certainly the nearest Messier object to Earth, and is the most obvious star cluster to the naked eye in the night sky.
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| Location of image field of view in the night sky... |
The Pleiades have been traditionally known as a group of
seven stars. In various Greek and Roman writings, they are referred to as The
Starry Seven, The Seven Virgins or the Seven Atlantic Sisters. These ancient
descriptions come from days long before the advent of telescopes or binoculars,
yet today, only six Pleiads are easily visible to the unaided eye. This state
of affairs is supported by modern measurements of the brightness of the stars
of the Pleiades. Only six of them are above “fifth magnitude”, the
accepted threshold for naked eye visibility.
Magnitudes of the nine brightest members of the Pleiades are shown in the greyscale image below:
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| Magnitudes of the nine brightest Pleiads... |
With an apparent magnitude of +2.85, the brightest star in the cluster is Alcyone, a blue-white B-type giant, similar in type to the other bright B-type stars in the Pleiades cluster. Alcyone has a mass of 6 times that of the Sun, and an effective radius of almost ten times that of the Sun, but the actual radius is lesser at poles and greater at the equator due to its high rotational velocity, which causes it to have an ellipsoidal shape. Its temperature is approximately 12,300 K (over twice as hot as our Sun) with the actual temperature being greater at the poles and lesser at the equator. Its luminosity is 2,030 times that of the Sun.
The light of the cluster is dominated by hot blue luminous stars that have formed comparatively recently in astronomical terms. Ages for star clusters can be estimated by comparing the Hertzsprung–Russell 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.
One of the oldest traditions concerning the cluster is the
persistent myth of a “lost Pleiad”. The Greeks identified her as Electra, who
is said to have veiled her face at the burning of
The Greek poet Aratus (310-240 BC) refers to the tradition of the “Lost Pleiad” when he wrote:
“…Their number seven, though the myths oft say
And poets feign, that one has passed away…”
This tradition is not confined to Greek mythology. The story
of a lost Pleiad also appears in Japanese lore: the cluster is mentioned under
the name Mutsuraboshi ("six
stars") in the 8th-century Kojiki
(an early Japanese chronicle dating from the early 8th century), and is now known
as Subaru. A similar theme figures in
the legends of Australian aborigines, natives of the Gold Coast of Africa and
the head-hunters of
“Their Sister Stars that were once seven
Mourn for their missing mate in Heaven…”
It seems that the legend of the lost Pleiad may have a basis in fact, however. Those modern brightness measurements have revealed that the mythical mother of the Pleiades, Pleione, is variable in brightness by at least half a magnitude, and may well once have been above the threshold of naked eye visibility.
Galileo was the first astronomer to view the Pleiades through a telescope. He discovered that the cluster contains many stars too dim to be seen with the naked eye. He published his observations, including a sketch of the Pleiades showing 36 stars, in his treatise Sidereus Nuncius in March 1610.
Today, we know that the cluster is about 80 light-years across and contains over 1,000 statistically confirmed members, a figure that excludes an unresolved number of binary stars, which make up over 50% of the total stars in the cluster.
Curiously, the 11th century Talmud (the central text of Rabbinic Judaism) uses the term kimah to describe the number of stars in the Pleiades, a word which means “over one hundred”.
Another thing revealed by long exposure photography is that the Pleiades are veiled in fine, dense threads of nebulosity, like cirrus clouds or interstellar cobwebs. It is questionable whether these are truly visible to the naked eye today, yet some translations of the biblical Book of Job refer to the “Chains of the Pleiades”. The seventh century Arabian poet Amr al Kais also hints at the nebulosity:
“The hour when the Pleiades appeared in the firmament
Like the folds of a silken sash variously decked with gems…
Perhaps the most famous reference
to the Pleiades nebulosity in English literature occurs in Tennyson’s Locksley Hall…
“Many a night from yonder ivied casement, ere I went to rest
Did I look on great Orion, sloping slowly to the west
Many a night I saw the Pleiads, rising thro’ the mellow shade
Glitter like a swarm of fireflies tangled in a silver braid…”
Charles Messier measured the position of the cluster and included it as M45 in his catalogue of comet-like objects, published in 1771. 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. The brightest area of nebulosity (called “Tempel’s Nebula) lies to the south of Merope does indeed look comet-like in appearance, however, so perhaps that is why Messier included the Pleiades in his famous catalogue.
These reflection nebulae can clearly be seen in the main image above, and more detailed photographs of the area show a mass of fine filaments that glitter with reflected starlight.
They are included in the 1966 catalogue of reflection nebulae compiled by Sidney van den Bergh, and are shown marked on the grey scale image below:
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| van den Burgh reflection nebulae in the Pleiades... |
This dust was once thought to be left over material from the cluster star formation, but is now considered likely to be an unrelated dust cloud in the interstellar medium through which the stars are currently passing. The dust cloud is estimated to be moving at a speed of approximately 18 km/s relative to the stars in the cluster.
The long exposures used in this image show up the interstellar dust around the Pleiades as a brownish cloudy background.
The total mass contained in the cluster is estimated to be about 800 solar masses and is dominated by fainter and redder stars, although its visible light is dominated by young, hot blue stars. 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.
The Pleiades have long been known to be a physically related group of stars rather than just a chance alignment. 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. The cluster itself is moving at the leisurely pace of 32 km/sec towards the south of what is currently the constellation of Orion. Like most open clusters, the Pleiades will not stay gravitationally bound forever. Astronomers estimate that the cluster will survive for about another 250 million years, after which it will gradually disperse due to gravitational interactions with its galactic neighbourhood.
