Become a fan of h2g2
Camelopardalis | Cancer | Canes Venatici | Canis Major | Canis Minor | Capricornus | Carina | Cassiopeia | Centaurus
Cepheus | Cetus | Chamæleon | Circinus | Columba | Coma Berenices | Corona Australis | Corona Borealis | Corvus
Crater | Crux | Cygnus | Delphinus | Dorado | Draco | Equuleus | Eridanus | Fornax | Gemini | Grus | Hercules | Horologium
Hydra | Hydrus | Indus | Lacerta | Leo | Leo Minor | Lepus | Libra | Lupus | Lynx | Lyra | Mensa | Microscopium | Monoceros
Musca | Norma | Octans | Ophiuchus | Orion | Pavo | Pegasus | Perseus | Phoenix | Pictor | Pisces | Piscis Austrinus
Puppis | Pyxis | Reticulum | Sagitta | Sagittarius | Scorpius | Sculptor | Scutum | Serpens | Sextans | Taurus
Telescopium | Triangulum | Triangulum Australe | Tucana | Ursa Major | Ursa Minor | Vela | Virgo | Volans | Vulpecula
|Area:||386 sq deg|
|Co-ordinates1:||Right Ascension 13h, Declination +20°|
|Origin:||Modern (16th Century)|
The Constellation Coma Berenices
Coma Berenices lies between Canes Venatici, Ursa Major, Leo, Virgo and Boötes. Though only a small constellation, Coma Berenices boasts eight Messier objects, the Coma Star Cluster (Melotte 111), three globular clusters, three extrasolar planets (to 2007), a meteor shower and the nearest massive cluster of galaxies, known as the 'Coma Cluster' (also Abell 1656).
In 1536 German globe maker Caspar Vopel created two new constellations, Coma Berenices and Antinous2, to the original 48 drawn up by Ptolemy. The stars which made up both figures had been catalogued, but were not specifically part of any recognised constellations. Coma Berenices' stars had previously been listed as part of Leo (the tip of the lion's tail) or Virgo (wisp of hair). Tycho Brahe is credited with popularising Coma3 Berenices (Berenice's Hair) after he included it in his star catalogue of the late 16th Century.
Ptolemy III of Egypt led an assault against the Syrians around 243 BC. His wife Queen Berenice4 made a pact with the goddess Aphrodite, that in return for protecting the king, she would cut off her much-envied lustrous long hair. When he arrived home safely, Queen Berenice kept her side of the bargain and offered the shorn locks of hair at the altar in the goddess's temple. Unfortunately the hair then vanished, which quite rightly upset the ruling couple. Luckily Konon of Samos, the royal astronomer, was able to convince them that the goddess was so delighted by her tribute that she had honoured the queen in return by forming a new constellation, thereafter named 'Berenice's Hair'. It is possibly this tale which inspired Caspar Vopel to create Coma Berenices.
The scientific star names are simple to understand (if you know your Greek alphabet). For example, 'alpha' means that it is the brightest star in that constellation. The next brightest is designated 'beta', etc. Combining Greek letters with the genitive of the constellation name, this is known as the 'Bayer designation'. Some stars have proper names as well; for example, alpha Com is Deneb. Others are known by their catalogue number.
The Stars of Coma Berenices
That's how it usually works, but sometimes the measurements at the time of cataloguing were a little tangled up, and we end up with a beta star being the brightest in a constellation, as is the case here.
Alpha Com is a binary system and is the only one of the Coma Berenices constellation which has a common name. The name Diadem was supposed to reflect the jewel in the crown on the queen's head. Beta Com is a yellow dwarf measuring just above the brightness of Diadem; it's also one of the closest stars to our Solar System. Gamma Com is just a shade less bright than Diadem, but the orange giant is a lot further away at 170 light years5 distant. An attractive pair catalogued 24 Com consists of a 5th mag orange giant which contrasts beautifully with the 7th mag blue-white companion.
The Coma Star Cluster (Melotte 111) is an open cluster situated just below gamma Com. The shape of the cluster is roughly three-sided, with around 30 stars total, none of which are over 5th mag. This cluster is viewable with binoculars, and worth seeking out.
Coma Berenices Star Table
|β Com||beta Com||43 Com||+4.23||30||Yellow dwarf|
|α Com||alpha Com||Diadem (42 Com)||+4.32||65||Binary system|
|γ Com||gamma Com||15 Com||+4.35||170||Orange giant|
|24 Com||HD 109511||24 Com||+6/+8||600||Double star system|
New General Catalogue (NGC)
The NGC was compiled by John Louis Emil Dreyer (the director of the Armagh Observatory from 1882 - 1916).
|Catalogue Number||Type||Brightness (m)||Distance
|NGC 4147||Globular cluster||+10.2||63,000|
|NGC 5024 (M53)||Globular cluster||+7.6||58,000|
|NGC 5053||Globular cluster||+9.0||55,000|
Galaxies are categorised by their shape:
- Spirals have 'arms' which rotate either clockwise (CW) or anti-clockwise (ACW) and they may have a central bar.
- Elliptical galaxies have no arms and are usually shaped like rugby balls.
- Lenticular galaxies are a mix between spiral and elliptical.
- Seyfert galaxies, named after their discoverer, American astronomer Carl Seyfert, have black holes at their core.
- Peculiar galaxies which appear in the Atlas of Peculiar Galaxies produced by Halton Arp are samples of unusual galaxies for study in the hope of understanding how galaxies evolve. Some galaxies are merging, others have a particular quirk, but all are unique.
|Catalogue Number||Type||Brightness (m)||Distance
|NGC 4192 (M98)||ACW spiral||+10.7||55m|
|NGC 4254 (M99)||CW spiral||+10.1||55m|
|NGC 4321 (M100)||ACW spiral||+10.6||53m|
|NGC 4382 (M85)||Lenticular||+9.3||53m|
|NGC 4414||ACW spiral||+10.9||62m|
|NGC 4450||CW spiral||+10.9||55m|
|NGC 4501 (M88)||ACW Spiral||+10.3||50m|
|NGC 4548 (M91)||CW barred spiral||+10.9||63m|
|NGC 4559||ACW spiral||+10.4||30m|
|NGC 4565||Edge-on spiral||+10.4||50m|
|NGC 4725||Barred CW spiral||+10.1||42m|
|NGC 4826 (M64)||CW spiral||+9.6||17m|
NGC 4565 is a spectacular edge-on spiral known by the common name Needle Galaxy. NGC 4651 is also known as the Umbrella Galaxy because there's a tidal star stream surrounding it; it's all that remains of another galaxy which strayed too close and was absorbed. This post-merger is classified 'peculiar' and appears on the Arp catalogue at number 189.
The Coma Galaxy Cluster, also known as Abell 1656, is the 'nearest' cluster of galaxies to us, although it is still 280 million light-years away at the lowest estimate. It contains roughly 1,000 galaxies spreading across 20 million light-years. It is one of the best studied areas of the sky thanks to its polar position. It was in this region that dark matter was first discovered outside our own galaxy. NGC 4874 (260,000 light years diameter) and NGC 4889 (330,000 light years diameter) in the Coma Galaxy Cluster are classified as supergiant ellipticals; they are much bigger than our own Milky Way galaxy.
French astronomer Charles Messier (1730 - 1817) created a catalogue of 110 astronomical objects which retains his name over two centuries later. Included in Messier's list are nebulae, open star clusters, globular star clusters and galaxies. There are eight Messier objects in Coma Berenices:
- M53 is a globular cluster.
- M64 is a spiral galaxy known as the Black Eye Galaxy.
- M85 is a lenticular galaxy.
- M88 is a spiral galaxy.
- M91 is a barred spiral galaxy.
- M98 is a spiral galaxy.
- M99 is a spiral galaxy.
- M100 is a spiral galaxy.
The debris which creates a meteor shower comes from the tail of a comet, as the Earth crosses where the comet passed previously on its own orbit. Imagine a trail of breadcrumbs, or sawdust like that used in hashing. The particular dust which causes the Coma Berenicids meteor shower comes from comet Lowe which was first discovered on 30 December, 1912, by amateur astronomer B Lowe in South Australia. The Coma Berenicids meteor shower usually happens between 8 December and 23 January.
Extrasolar Planets in Coma Berenices
There have been some extrasolar planetary systems found in the constellation Coma Berenices. Figures given in the table below are the length of the planet's orbital period around its parent star, which we know of as a year. The mass of the extrasolar planet is compared to that of Jupiter, our Solar System's largest planet, known by astronomers as the 'Jovian scale'.
HD 108874 b, discovered in 2003, orbits a yellow dwarf star and inhabits the 'Goldilocks zone'. As it is a gas giant it is not a candidate for extra-terrestrial life. However, if the planet has any rocky moons with an atmosphere then there's a distinct possibility.
Extrasolar Planets Table
|Star name or
|Year of discovery||Comments|
|HD 114762||HD 114762 b||11||84||1989||Eccentric orbit|
|HD 108874||HD 108874 b||1.4||400||2003||Gas giant: habitable zone|
|HD 108874||HD 108874 c||1.05||1,680||2005||Gas giant: eccentric orbit|
|11 Com||11 Com b||19.4||326||2008||possible Brown Dwarf|
Down To Earth
While this article is primarily about the constellation which honours Queen Berenice, the author thought you might like to read about some of the other instances where Berenice has appeared.
- Berenice, Regina d'Egitto is an opera by Handel — not one of his best-loved, though. It is thought not to have been performed from 1743 until 1985, a wait of 242 years for tickets!
- Bérénice is a 1671 tragic play written by French playwright Jean Racine.
- Berenice Abbott (1898 - 1991) was a well-known US photographer, and author of the 1941 A Guide to Better Photography.
- Edgar Allen Poe wrote about a Berenice in an 1835 horror story, in which her cousin Egaeus had a sick obsession with her; not really suitable for Jackanory viewers.
- Berenice or Berenikë was a common female name among the Greek rulers of Egypt during the Ptolemaic Dynasty (305 - 30 BC). The city of Berenikë on the Red Sea was lost for millennia until rediscovered by Belzoni in the 18th Century. It was named after the first Egyptian Berenice, wife of Pharaoh Ptolemy I and grandmother of the Berenice after whom the constellation was named.