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Double Cluster

From Wikipedia, the free encyclopedia

Double Cluster
Caldwell 14 - The Double Cluster taken by /u/ItFrightensMe
The Double Cluster, NGC 869 (above) and NGC 884 (below) with north to the left
Observation data (J2000.0 epoch)
Right ascension2h 20m
Declination57° 08
Distance7,460 and 7,640ly[1] (2,290 and 2340pc[1])
Apparent magnitude (V)3.7 and 3.8
Apparent dimensions (V)60
Physical characteristics
Other designationsCaldwell 14
Associations
ConstellationPerseus
See also: Open cluster, List of open clusters

The Double Cluster (also known as Caldwell 14) consists of the open clusters NGC 869 and NGC 884 (often designated h Persei and χ (chi) Persei, respectively), which are close together in the constellation Perseus. Both visible with the naked eye, NGC 869 and NGC 884 lie at a distance of about 7,500 light years in the Perseus Arm of the Milky Way galaxy.[2]

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  • Sirius Stargazing: The Double Cluster (Caldwell 14)
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Transcription

Welcome to Sirius Stargazing. I'm TK and in this episode we're going to look at two clusters, together known as the Double Cluster in Perseus. This really is a great target for your binoculars; two very fine bundles of stars in just one field of view, and I think once you've found it, this is something you're going to come back to again and again, challenging yourself to make out more stars every time when the conditions seem a little bit better. Although it's not the only instance where two clusters appear close together, the Perseus Double Cluster is really unrivalled in its brilliance and I think it rightly deserves to be called simply 'The Double Cluster'. It's certainly punchier than using the two clusters' catalogue numbers, which are NGC 869 and 884. NGC stands for 'New General Catalogue', a really extensive list of very varied objects that was completed in 1888 by the Danish-born astronomer, John Dreyer. Because Charles Messier didn't include the clusters together or even separately in his catalogue, which is a popular checklist for amateur astronomers, the English astronomer and broadcaster Sir Patrick Moore labelled them as number 14 in the Caldwell catalogue, which I think many of us fondly consider to be something of a sequel to Messier's. Over 7,200 light years away, these two clusters formed very recently from the same molecular cloud, or nebula, and all 600 or so of these stars are super young - somewhere around 10 million years old or less. That's at least five hundred times younger than our Sun. They're also supergiants, many thousands of times brighter than the Sun. So in terms of colour, they generally range from blue through to white, but dotted among them are a few prominent Red Giants. These particular stars are already approaching the end of their lives and they will surely explode in spectacular supernovas. Even though both clusters are quite easy to separate as fuzzy white blobs with the naked eye, by using your binoculars in very good conditions, you'll almost certainly see differences in the colours of some of the stars, but I think the most rewarding thing of all is seeing the true extent of the two clusters, not just the bright cores, and to help you with this I suggest using Averted Vision. Now this is a technique astronomers use to get a better view of fainter objects, essentially by not looking at them. When you find what you're looking for with binoculars or a telescope, it's instinctive to just stare at it intently, almost willing your eyes to adjust to it and make out more detail, but unfortunately when you do this, you're only making things more difficult for yourself. You see, your eyes have two vision systems, involving different types of photosensitive cells on the retina. In well-lit conditions, you use cones, which are sensitive to colour, but not useful for detecting dim sources of light. When your eyes dark adapt and your pupils dilate, you begin to use rods as well, which give you better night vision, but only allow you to see in black and white. Right in the centre of the retina for each eye is a small area called the 'fovea' where there are no rods - only cones. So this creates a blind spot at the very centre of your vision in dark conditions. To make the most of those rods, you're going to have to train yourself to look slightly away from what you want to see. Now, don't fret if you have trouble with this, its something that takes a lot of practise to really master, but I'm still pretty confident that you'll be impressed by the difference it makes even for the first time that you try it. By the way, in my experience its marginally better to look above the object than below it. Looking to one side would be optimal, but only if you're using one eye through a telescope. By using binoculars, you're already getting the benefit of using both your eyes, and this actually gives your brain twice the information with which to separate the light from the dark. Now, finding the Double Cluster isn't too tough, as you can see it with the naked eye once you know where to look. The easiest method is to take these two stars in the 'W' of Cassiopeia and to use them as pointers. Just draw an imaginary line through them and continue with it in the direction of Perseus, and I'm sure you won't miss the two distinct groups of stars like sprinklings of diamonds against the backdrop of the galaxy. So get practising with Averted Vision and see how many of these gems you can unlock. Until next time, clear skies.

Membership

NGC 869 has a mass of 4,700 solar masses and NGC 884 weighs in at 3,700 solar masses; both clusters are surrounded with a very extensive halo of stars, with a total mass for the complex of at least 20,000 solar masses.[1] They form the core of the Perseus OB1 association of young hot stars.[2]

Based on their individual stars, the clusters are relatively young, both 14 million years old.[1] In comparison, the Pleiades have an estimated age ranging from 75 million years to 150 million years.

There are more than 300 blue-white super-giant stars in each of the clusters. The clusters are also blueshifted, with NGC 869 approaching Earth at a speed of 39 km/s (24 mi/s) and NGC 884 approaching at a similar speed of 38 km/s (24 mi/s).[3] Their hottest main sequence stars are of spectral type B0. NGC 884 includes five prominent red supergiant stars, all variable and all around 8th magnitude: RS Persei, AD Persei, FZ Persei, V403 Persei, and V439 Persei.

History

The Double Cluster in Perseus (lower left of center, wide angle view)

Greek astronomer Hipparchus cataloged the object (a patch of light in Perseus) as early as 130 BCE. To Bedouin Arabs the cluster marked the tail of the smaller of two fish they visualized in this area, and it was shown on illustrations in Abd al-Rahman al-Sufi's Book of Fixed Stars.[4] However, the true nature of the Double Cluster was not discovered until the invention of the telescope, many centuries later. In the early 19th century William Herschel was the first to recognize the object as two separate clusters. The Double Cluster is not included in Messier's catalog, but is included in the Caldwell catalogue of popular deep-sky objects.[5][6]

The clusters were designated h Persei and χ Persei by Johann Bayer in his Uranometria (1603).[7] It is sometimes claimed that Bayer did not resolve the pair into two patches of nebulosity, and that χ refers to the Double Cluster and h to a nearby star.[8] Bayer's Uranometria chart for Perseus does not show them as nebulous objects, but his chart for Cassiopeia does, and they are described as Nebulosa Duplex in Schiller's Coelum Stellatum Christianum, which was assembled with Bayer's help.[9]

Location

The Double Cluster is circumpolar (continuously above the horizon) from most northern temperate latitudes. It is in proximity to the constellation Cassiopeia. This northern location renders this object invisible from locations south of about 30º south latitude, such as New Zealand, most of Australia and South Africa. The Double Cluster is approximately the radiant of the Perseid meteor shower, which peaks annually around August 12 or 13. Although easy to locate in the northern sky, observing the Double Cluster in its two parts requires optical aid. They are described as being an "awe-inspiring" and "breathtaking" sight, and are often cited as a target in astronomy observer's guides.[10]

The Double Cluster in Perseus
The Double Cluster in Perseus, visible light.

Mythology

Perseus was a famous hero of Greek mythology, a son of the Greek god Zeus. Along with beheading Medusa, Perseus performed other heroic deeds such as saving princess Andromeda who was chained to a rock as a sacrifice to a sea monster, Cetus. The gods commemorated Perseus by placing him among the stars, with the head of Medusa in one hand and the jeweled sword in the other. The Double Cluster represents the jeweled handle of his sword.[11]

References

  1. ^ a b c d Currie, Thayne; Hernandez, Jesus; Irwin, Jonathan; Kenyon, Scott J.; Tokarz, Susan; Balog, Zoltan; Bragg, Ann; Berlind, Perry; Calkins, Mike (2010). "The Stellar Population of h and χ Persei: Cluster properties, membership, and the intrinsic colors and temperatures of stars". The Astrophysical Journal Supplement. 186 (2): 191. arXiv:0911.5514. Bibcode:2010ApJS..186..191C. doi:10.1088/0067-0049/186/2/191. S2CID 16454332.
  2. ^ a b Keller, Stefan C.; Grebel, Eva K.; Miller, Grant J.; Yoss, Kenneth M. (2001). "UBVI and Hα photometry of the h and χ Persei cluster". The Astronomical Journal. 122 (1): 248. arXiv:astro-ph/0104179. Bibcode:2001AJ....122..248K. doi:10.1086/321139.
  3. ^ Kharchenko, N.V.; Piskunov, A.E.; Röser, S.; Schilbach, E.; Scholz, R.-D. (2005). "Astrophysical parameters of Galactic open clusters". Astronomy and Astrophysics. 438 (3): 1163. arXiv:astro-ph/0501674. Bibcode:2005A&A...438.1163K. doi:10.1051/0004-6361:20042523. S2CID 9079873.
  4. ^ Ridpath, Ian. Star Tales – Andromeda Galaxy and the Double Cluster in al-Sufi's Book of the Fixed Stars. Online edition. Retrieved 2021-09-19.
  5. ^ O'Meara, Stephen James (2002). The Caldwell Objects. Cambridge University Press. ISBN 978-0-521-82796-6.
  6. ^ "Introduction". Caldwell Club. astroleague.org. Retrieved 8 September 2006.
  7. ^ Ridpath, Ian. Star Tales – The Double Cluster. Online edition. Retrieved 2024-02-24.
  8. ^ O'Meara, Stephen James; Green, Daniel W.E. (February 2003). "The mystery of the Double Cluster". Sky and Telescope. Vol. 105, no. 2. pp. 116–119.
  9. ^ Wagman, Morton (2003). Lost Stars. McDonald & Woodward. p. 240. ISBN 0939923785.
  10. ^ Chaple, Glenn (January 2011). "A double take". Astronomy. Vol. 39, no. 1.
  11. ^ Ridpath, Ian. Star Tales – Perseus. Online edition. Retrieved 2021-09-19.

External links

This page was last edited on 24 February 2024, at 21:52
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