Constellation Sagittarius- The Archer
Created | Updated Jun 20, 2011
If the stars should appear one night
in a thousand years,
how would man believe and adore,
and preserve for many generations
the rememberance of the city of God
-Ralph Waldo Emerson
Latin: | Sagittarius |
Genitive: | Sagittarii |
Short form: | Sgr |
Area: | 867 sq deg |
Co-ordinates1: | 19h,-25° |
Zodiac: | yes |
Origin: | Ancient |
On a deserted beach long ago a young man looked up at more stars than he could possibly count. He was looking at the centre of our galaxy, the Milky Way, which lies in the constellation Sagittarius.
Douglas Adams started the first book in the Hitchiker series with the words
Far out in the uncharted backwaters of the unfashionable end of the Western arm of the Galaxy lies a small unregarded yellow sun.– Douglas Adams (Intro) The Hitchhiker's Guide to the Galaxy.He was of course referring to our own sun, and while we may quibble with the designations uncharted or unfashionable, no one is arguing about the words 'far out'. Those who read science-fiction might note that the opening quote from Emerson was also used to begin a story by Isaac Asimov called Nightfall. That story was about a civilisation living in the middle of a globular cluster much closer to the heart of the Galaxy. That civilisation also did not have street lights, and so, on that world, when it got dark it got really dark; and one was faced with unimaginable numbers of stars. Those numbers really exist, but, on Earth, for several reasons, a person living in some place like London, or Tokyo, or Los Angeles may never see them. Even those with a clear dark sky cannot see things like the Pistol Star without using an infrared telescope, because of all the dust and dark matter between our arm of the Galaxy and the central core.
The constellation Sagittarius appears in the summer sky east of Scorpius between 20° and 40° south of the Celestial Equator. Many star charts will show an asterism called
'The Teapot' here.
Scientific study of the sky in Sagittarius indicates that a resident
black hole lurks at the heart of the Milky Way here with a mass which has been calculated at greater than 2.6 million times that of our sun2.
Mythology
Saggitarius depicts a centaur holding a bow and arrow. Many sources say Ptolemy patterned both this constellation and the more southerly Centaurus after the same figure in mythology: the centaur named Chiron3. Most centaurs were a surly lot, but not Chiron. Educated by the Greek gods he was wise and kind. Amongst his students were Achilles,
Jason ,
Hercules, and Asclepius4 the latter two having their own constellations. According to some versions the Archer has his arrows poised to shoot the scorpion lest he decide to sting anyone.
Stars
In the table below you will find the first column contains letters such as alpha or beta. The scientific star names are from the lower case Greek alphabet. Where two stars share the same Greek letter they have been given a suffix such as xi-2. Sagittarius is one of those constellations where alpha is not the designation for the brightest star (epsilon is actually the brightest). Some stars have proper names as well, and where no such names were found HR designations have been used.
Star Table
Star | Designation | Name or catalogue number | Brightness (m) | Distance (light years) | SC5 |
α | Alpha | Rukbat | +3.97 | 170 | B8 |
β1 | Beta-1 | Arkab Prior | +4.01 | 378 | B9 |
β2 | Beta-2 | Arkab Posterior | +4.29 | 139 | F2 |
γ1 | Gamma-1 | 6742 | +2.69 | 1,500 | F4 |
γ2 | Gamma-2 | Alnasl | +2.69 | 96 | k0 |
δ | Delta | Kaus Meridionalis | +2.70 | 306 | K3 |
ε | Epsilon | Kaus Australis | +1.85 | 145 | B9 |
ζ | Zeta | Ascella | +2.60 | 89 | A2 |
η | Eta | 6832 | +3.11 | 149 | M2 |
θ1 | Theta-1 | 7623 | +4.37 | 617 | B2 |
θ2 | Theta-2 | 7623 | +4.37 | 157 | A4 |
ι | Iota | 7581 | +4.13 | 189 | K0 |
κ1 | Kappa-1 | 7779 | +5.59 | 244 | A0 |
κ2 | Kappa-2 | 7787 | +5.64 | 371 | A5 |
λ | Lambda | Kaus Borealis | +5.64 | 77 | K1 |
μ | Mu | Polis | +2.81 | 3,000 | B1 |
ν1 | Nu-1 | Ain Al Rami | +4.83 | 1,850 | K1 |
ν2 | Nu-2 | 7120 | +4.9 | 270 | K1 |
ξ1 | Xi-1 | 7150 | +5.1 | 2,350 | K0 |
ξ2 | Xi-2 | Nergal | +5.08 | 372 | G8 |
ο | Omicron | 7217 | +3.77 | 139 | K0 |
π | Pi | Albaldah | +2.89 | 440 | F2 |
ρ | Rho | 7340 | +3.93 | 122 | F0 |
σ | Sigma | Nunki | +2.02 | 224 | B2 |
τ | Tau | 7581 | +3.32 | 120 | K1 |
υ | Upsilon | 6832 | +4.61 | 1,672 | B2 (A1) |
φ | Phi | 7039 | +3.17 | 231 | B8 |
χ | Chi | 7362 | +5.43; 5.03 | 220 | A5 |
ψ | Psi | 7039 | +4.85 | 330 | K0 (A8) |
ω | Omega | Terebellum | +4.7 | 77.6 | G5 |
The Pistol Star
Until the advent of orbiting telescopes this star was unknown. It has been calculated that if the space between that solar system and ours was clear it would be a fourth magnitude star and appear in the chart above. However because of the intervening matter it is only visible in Infra-Red or X-ray.
Located in our galaxy's central bulge, originally this star was one of the most massive in existance ( 200 times the size of our sun). It is still a giant and in the course of its life has thrown out an emission nebula over four light years in diameter.
Nebulae Star Clusters and Galaxies
The NGC catalogue was compiled by John Louis Emil Dreyer (the director of the Armagh Observatory from 1882 to 1916). The M numbers are from the Catalogue of Charles Messier. These Messier Objects were compiled during the 1700s and predate the NGC Catalogue.
Table
Catalogue | Name | Type | Brightness (m) | Distance (light years) |
M6 | Butterfly cluster | G | +5.3 | 1,600 |
M8 | Lagoon nebula | N | +6.0 | 5200 |
M17 | Omega nebula | E | +7.0 | greater than 5,000 |
M18 | Star cluster | O | +7.5 | 4,000 |
M20 | Trifid nebula | E/R | +9.0 | less than 9,000 |
M21 | Open cluster | O | +7.5 | 4,250 |
M22 | Star cluster | G | +5.1 | 10,400 |
M23 | Open cluster | O | +5.5 | 2,000 |
M24 | Star cloud | -- | -- | 10,000 to 16,000 |
M25 | Open cluster | O | +4.6 | 2,000 |
M28 | Star cluster | G | +6.9 | 15,000 |
M54 | Star cluster | G | +7.6 | 87,000 |
M55 | Star cluster | G | +6.3 | 17,300 |
M69 | Star cluster | G | +7.9 | 29,700 |
M70 | Star cluster | G | +7.6 | 29,300 |
M75 | Star cluster | G | +8.5 | 67,500 |
NGC6520 | Star cluster | G | +8.0 | 6,300 |
NGC6522 | Star cluster | G | +8.6 | 26,000 |
SAGDEG | Galaxy | ElG | +4.6 | 88,000 |
SAGDIG | Galaxy | IrG | +15.5 | 4,200,000 |
Legend:
N=Nebulosa6,
E=Emission, R=Reflection, P=Planetary, G=Globular, O=Open, ElG=Elliptical galaxy, IrG=Irregular galaxy
A Stellar Mystery
The stars in M24 are not gravitationally bound together.
They just happen to lie in the same direction. Astronomers sometimes bring up the idea that the sky should be lit up everywhere- but it is not. So why is the sky dark, if we have so large a number of stars out there? Some say that interstellar dust is the reason, but their arguments are hardly convincing. Others blame
dark matter , that unknown substance that makes up a sizable percentage of the mass of the universe. Whichever answer is correct, it is visibly apparent that M24 has less of it than most places; and so we see many stars ranging from 10 to 16 thousand light years away clearly which would otherwise be somewhat dimmed.
Extrasolar Planets
Over 2,000 years ago the Greek philosophers Aristotle and Epicurus argued about whether there were other Earth-like planets orbiting distant suns. Today scientists are coming up with ways to actually detect such planets, and the techniques are being fine-tuned so planets throughout our galaxy can be discovered and studied.
There have been 10 extrasolar planets found in the constellation Sagittarius, two of which orbit the star HD169830. The size of the extrasolar planets use as reference the mass of Jupiter, our Solar System's largest planet. This is known by astronomers as the 'Jovian scale'.
Extrasolar Planets Table
Star name or catalogue number | Planet catalogue number | year discovered | Planet size (Jovian scale) | Orbital distance (AU7) | Orbital Period |
HD169830 | HD169830b | 2000 | 2.88 | 0.81 | 225 earth days |
HD169830 | HD169830c | 2003 | 4.04 | 3.6 | 5.75 earth yrs. |
HD179949 | HD179949b | 2000 | 0.916 | 0.04 | 3.092 earth days |
HD190647 | HD190647b | 2007 | 1.9 | 2.07 | 2.84 earth years |
OGLE TR-10 | OGLE TR10b | 2004 | 0.63 | 0.41 | 3.1 earth days |
OGLE 2005-BLG-169L | OGLE 2005-BLG-169Lb | 2005 | 0.041 | 2.7 | 9 earth yrs. |
OGLE-2003-_BLG 235L | OGLE 235-MOA 53b | 2004 | 2.6 | 5.1 | 4.69 earth days |
OGLE-2005-BLG-390L | OGLE-2005-BLG-390Lb | 2005 | 0.0188 | 2.6 | 9.6 earth yrs. |
SWEEPS-04 9 | SWEEPS-04b | 2006 | 3.8 | 0.05 | 4.2 earth days |
SWEEPS-11 | SWEEPS-11b | 2006 | 9.7 | 0.03 | 1.8 earth days |