Scorpius (abbr. Sco, gen. Scorpii)
The Scorpion; a prominent constellation
of the southern hemisphere and the eighth of the zodiac. Scorpius is one
of the few constellations to actually looks like what it represents. It
lies south of Ophiuchus and west of the northern
part of Centaurus. See below for details of
the constellation's brightest stars and interesting deep sky objects.
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Scorpius. © 2003 Torsten Bronger.
Copied here under the terms of the GNU Free Documentation License
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| Stars brighter than magnitude 4.0 |
| Star |
Visual
mag. |
Abs.
mag. |
Spectral
type |
Distance
(lt-yr) |
R.A. (h m s) |
Dec. ( ° ' '' ) |
| Alpha (Antares) |
1.06v |
-5.28 |
M1.5Iab+B4V |
604 |
16 29 24 |
-26 25 55 |
| Lambda (Shaula) |
1.62 |
-5.05 |
B2IV+B |
703 |
17 33 36 |
-37 06 14 |
| Theta (Sargas) |
1.86 |
-2.75 |
F1II |
272 |
17 37 19 |
-42 59 52 |
| Epsilon (Wei) |
2.29 |
0.78 |
K2.5III |
65 |
16 50 10 |
-34 17 36 |
| Delta (Dschubba)
|
2.29 |
-3.16 |
B0.3IV |
402 |
16 00 20 |
-22 37 18 |
| Kappa (Girtab) |
2.39 |
-3.38 |
B1.5III |
464 |
17 42 29 |
-39 01 48 |
| Beta (Graffias) |
2.56 |
-3.50 |
B1V+B2V |
530 |
16 05 26 |
-19 48 19 |
| Upsilon (Lesath) |
2.70 |
-3.31 |
B2IV |
519 |
17 30 46 |
-37 17 45 |
| Tau |
2.82 |
-2.78 |
B0V |
430 |
16 35 53 |
-28 12 58 |
| Sigma (Alniyat) |
2.90v |
-3.87 |
B2III+O9.5V |
735 |
16 21 11 |
-25 35 34 |
| Pi |
2.89 |
-2.86 |
B1V+B2V |
459 |
15 58 51 |
-26 06 50 |
| Iota-1 |
2.99 |
-5.71 |
F3Iae |
1,790 |
17 47 35 |
-40 07 37 |
| Mu-1 |
3.00 |
-4.01 |
B1.5V+B6.5V |
822 |
16 51 52 |
-38 02 51 |
| Eta |
3.32 |
1.61 |
F3Vp |
72 |
17 12 09 |
-43 14 21 |
| Mu-2 |
3.56 |
-2.44 |
B2IV |
517 |
16 52 20 |
-38 01 03 |
| Zeta-2 |
3.62 |
0.30 |
K4III |
151 |
16 54 35 |
-42 21 41 |
| Rho |
3.87 |
-1.63 |
B2IV |
409 |
15 56 53 |
-29 12 50 |
| Omega-1 (Jabhat al Akrab) |
3.93 |
-1.64 |
B1V |
424 |
16 06 48 |
-20 40 09 |
| Other objects of interest |
| Name |
Type of Object |
Notes |
| Butterfly Cluster
|
open cluster |
M6. See separate entry |
| M7 (NGC 6475) |
open cluster |
One of the finest open clusters in the northern hemisphere,
best seen with binoculars. It encompasses many bright stars loosely
concentrated at the center. Telescopes show, at the western edge,
but still within the cluster's boundaries, the faint globular cluster
NGC 6453. Magnitude 3.3; diameter 80'; R.A. 17h 53.9m, Dec. -22°
59' |
| NGC 6231 |
open cluster |
Over 100 stars in a compact 15' area; this cluster
lies on another spiral arm of our galaxy, closer to the galactic center |
| M4 (NGC 6121) |
globular cluster |
A large, loosely concentrated cluster, 1.5o W of
Antares. Some of its brightest members appear to form a bar through
the center. Magnitude 5.9; diameter 26.3'; R.A. 16h 23.6m, Dec. -26°
32' |
| M80 (NGC 6093) |
globular cluster |
A small, tightly concentrated object, difficult to
resolve into stars, and then only around the edges; a fuzzy ball seen
in binoculars. Magnitude 7.2; diameter 8.9'; R.A. 16h 17.0m, Dec.
-22° 59' |
| Scorpius X-1
|
X-ray binary |
See separate entry |
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