| Back to Constellation Index |
|
Ophiuchus
Abbreviation: Oph
Genitive: Ophiuchi
Right Ascension: 17.18 hours
Declination: -4.24 degrees
|
|
Ophiuchus, the Serpent Bearer, is best seen in summer in the Northern
Hemisphere and winter in the Southern Hemisphere.
Ophiuchus vel Serpentarius, the Serpent Holder, is generally identified
with Aesculapius a physician who was later made a god. Serpents were always
associated with physicians as symbols of prudence, renovation, wisdom, and
the power of discovering healing herbs. The modern symbol for medicine derives
from this.
Aesculapius was the earliest of his professions trained by a centaur
Chiron and the ships surgeon of the Argo. He was so skilled in his profession
he could bring the dead back to life. After many successful operations and
numerous remarkable cures, Pluto fearful that his dominion would vanish,
convinced Zeus to strike Aesculapius with a thunderbolt and transfer him
to the stars.
|
|
Bright Stars | Deep Sky |
Other Deep Sky | Variable Stars
| Double Stars |
|
(Yale Bright Star Catalog) |
|
Common Name
or Bayer Number
1 |
RA |
DEC |
Magnitude
2 |
RASALHAGUE |
17.00:34.00:56.07 |
+12.00:33.00:36.14 |
2.08 |
ZET OPH |
16.00:37.00:9.54 |
-10.00:34.00:1.56 |
2.56 |
YED PRIOR |
16.00:14.00:20.74 |
-3.00:41.00:39.55 |
2.74 |
CEBALRAI |
17.00:43.00:28.35 |
+4.00:34.00:2.26 |
2.77 |
KAP OPH |
16.00:57.00:40.10 |
+9.00:22.00:30.09 |
3.20 |
YED POSTERIOR |
16.00:18.00:19.29 |
-4.00:41.00:32.99 |
3.24 |
THE OPH |
17.00:22.00:0.58 |
-24.00:59.00:58.25 |
3.27 |
NU OPH |
17.00:59.00:1.59 |
-9.00:46.00:25.10 |
3.34 |
72 OPH |
18.00:7.00:20.98 |
+9.00:33.00:49.87 |
3.73 |
GAM OPH |
17.00:47.00:53.56 |
+2.00:42.00:26.19 |
3.75 |
67 OPH |
18.00:0.00:38.71 |
+2.00:55.00:53.60 |
3.97 |
45 OPH |
17.00:27.00:21.28 |
-29.00:52.00:1.49 |
4.29 |
|
|
|
|
(PAS Catalog) |
M-10
|
M-10 This fine globular is rather well resolved even at low powers.
It is about 12' in diameter, and has a rather ragged circular shape with
stars resolved across its face. A chain of 6 foreground stars starts north
of the globular and ends to its south, seemingly bisecting the cluster.
|
M-107
|
M-107 This moderately faint object needed a high power and averted vision
to yield resolution. It is about 8' in diameter, and is slightly flattened
on its northern edge. The brightest area appears to be in the southwestern
corner.
|
M-12
|
M-12 Lying only a few degrees away from M-10, this object is slightly
smaller, about 8-10' in diameter. It is also well resolved across its face,
and is somewhat looser than that object. It is basically circular and has
a granular center.
|
M-14
|
M-14 This object yielded the least amount of detail in my telescope.
It is about 8' in diameter, with resolution hinted at the edges at 179X.
Little detail other than a granular core was noted.
|
M-19
|
M-19 This globular appeared as an milky patch of light about 8' in diameter,
with resolution around the edges. Its granular core is flanked by two stars,
one to the northwest, and one to the northeast, and appears somewhat ovoid
in shape.
|
M-62
|
M-62 A fine, bright globular cluster with resolution at the edges, and
a bright core. About 10' in diameter, this cluster's core is slightly offset
to the southeast. Stars seem to fan out to the west, giving this globular
rather unique appearance.
|
M-9
|
M-9 This globular cluster is about 6-8' in diameter, roughly circular,
with some resolution at the edges. The core is unresolved in my scope, and
is somewhat kidney bean shaped, and is elongated in the north to south direction.
Under a clear, dark sky, see if you can find Barnard 64, the dark nebula
upon which M-9 is superimposed. I saw it as an amorphous region, about 3/4
of a degree in extent, which is almost devoid of stars just to the west
of the globular, and ever so slightly darker than the surrounding sky background.
|
NGC-6369
|
NGC 6369 This is a moderately bright planetary nebula which is almost
1' in diameter. It appears as a grey puff of light which, with averted vision,
has a darker center suggesting angularity (a ring shape). Try high powers
on this object.
|
|
|
|
(Saguaro Astronomy Club Catalog) |
|
Only Objects less than 10.0 Mag. |
|
Object |
R.A. |
Dec. |
Object Type
3
|
Mag. |
Uranometria |
Tirion |
NGC 6171 |
16 32.5 |
-13 03 |
GLOCL |
08.1 |
291 |
15 |
NGC 6218 |
16 47.2 |
-01 57 |
GLOCL |
06.6 |
246 |
15 |
NGC 6254 |
16 57.1 |
-04 06 |
GLOCL |
06.6 |
247 |
15 |
NGC 6266 |
17 01.2 |
-30 07 |
GLOCL |
06.6 |
376 |
22 |
NGC 6273 |
17 02.6 |
-26 16 |
GLOCL |
07.2 |
337 |
22 |
NGC 6284 |
17 04.5 |
-24 46 |
GLOCL |
09 |
337 |
22 |
NGC 6287 |
17 05.2 |
-22 42 |
GLOCL |
09.2 |
337 |
22 |
NGC 6293 |
17 10.2 |
-26 35 |
GLOCL |
08.2 |
337 |
22 |
NGC 6304 |
17 14.5 |
-29 28 |
GLOCL |
08.4 |
376 |
22 |
NGC 6316 |
17 16.6 |
-28 08 |
GLOCL |
09 |
376 |
22 |
NGC 6333 |
17 19.2 |
-18 31 |
GLOCL |
07.9 |
337 |
15 |
NGC 6342 |
17 21.2 |
-19 35 |
GLOCL |
09.9 |
338 |
15 |
NGC 6356 |
17 23.6 |
-17 49 |
GLOCL |
08.4 |
338 |
15 |
NGC 6355 |
17 24.0 |
-26 21 |
GLOCL |
09.6 |
338 |
22 |
NGC 6366 |
17 27.7 |
-05 05 |
GLOCL |
10.0 |
248 |
15 |
Tr 26 |
17 28.5 |
-29 29 |
OPNCL |
09.5 |
376 |
22 |
NGC 6402 |
17 37.6 |
-03 15 |
GLOCL |
07.6 |
248 |
15 |
NGC 6401 |
17 38.6 |
-23 55 |
GLOCL |
09.5 |
338 |
22 |
IC 4665 |
17 46.3 |
+05 43 |
OPNCL |
04.2 |
203 |
15 |
Cr 350 |
17 48.1 |
+01 18 |
OPNCL |
06.1 |
248 |
15 |
Mel 186 |
18 01.0 |
+03 00 |
OPNCL |
03 |
249 |
15 |
NGC 6572 |
18 12.1 |
+06 51 |
PLNNB |
09 |
204 |
15 |
NGC 6633 |
18 27.7 |
+06 34 |
OPNCL |
04.6 |
205 |
15 |
|
|
|
|
(General Catalog of Variable Stars) |
|
Only Objects <= 8.0 magnitude |
|
GCVS ID |
R.A.
(hh mm ss.ss) |
Dec.
(deg mm ss) |
Variable Type
4
|
Mag. Min |
Mag. Max |
U Oph |
17.00:13.00:59.40 |
+1.00:15.00:53.00 |
EA/DM |
6.56 |
5.84 |
Y Oph |
17.00:49.00:57.80 |
-6.00:7.00:59.00 |
DCEPS |
6.46 |
5.87 |
BF Oph |
17.00:2.00:59.30 |
-26.00:30.00:49.00 |
DCEP |
7.71 |
6.93 |
V0566 Oph |
17.00:54.00:24.30 |
+4.00:59.00:31.00 |
EW/KW |
7.96 |
7.46 |
V0986 Oph |
18.00:2.00:5.80 |
+1.00:54.00:54.00 |
* |
6.15 |
6.10 |
V1010 Oph |
16.00:46.00:36.20 |
-15.00:34.00:55.00 |
EB/KE |
7.00 |
6.10 |
V2048 Oph |
17.00:57.00:47.10 |
+4.00:22.00:12.00 |
GCAS+UV: |
4.85 |
4.55 |
V2052 Oph |
17.00:53.00:45.40 |
+0.00:40.00:35.00 |
BCEP |
5.84 |
5.81 |
V2105 Oph |
16.00:25.00:1.60 |
-7.00:29.00:7.00 |
SRB: |
5.38 |
5.00 |
V2106 Oph |
16.00:46.00:35.90 |
-21.00:45.00:58.00 |
SR |
7.46 |
7.38 |
V2111 Oph |
16.00:42.00:34.30 |
-2.00:59.00:39.00 |
SR |
7.08 |
6.69 |
V2112 Oph |
17.00:16.00:26.00 |
+6.00:8.00:11.00 |
DSCTC |
6.52 |
6.50 |
V2113 Oph |
17.00:17.00:15.10 |
+2.00:11.00:21.00 |
SR: |
6.81 |
6.59 |
V2114 Oph |
17.00:25.00:20.00 |
+8.00:28.00:59.00 |
SR |
6.51 |
6.40 |
V2118 Oph |
17.00:59.00:12.60 |
+11.00:17.00:7.00 |
* |
7.09 |
7.02 |
V2125 Oph |
17.00:32.00:17.90 |
-22.00:0.00:43.00 |
ACV |
0.04 |
6.57 |
V2126 Oph |
17.00:57.00:42.50 |
+0.00:37.00:51.00 |
ACV |
0.00 |
6.36 |
V2133 Oph |
16.00:33.00:43.70 |
-2.00:13.00:10.00 |
BY |
0.04 |
6.57 |
V2213 Oph |
17.00:2.00:44.00 |
+0.00:46.00:28.00 |
BY |
0.04 |
6.01 |
V2215 Oph |
17.00:13.00:8.70 |
-26.00:28.00:33.00 |
RS |
6.34 |
6.26 |
V2266 Oph |
17.00:20.00:12.00 |
-22.00:44.00:54.00 |
M |
7.88 |
6.52 |
V2291 Oph |
18.00:23.00:14.40 |
+8.00:0.00:9.00 |
EA/GS |
1.10 |
7.02 |
V2292 Oph |
16.00:50.00:27.40 |
+0.00:4.00:32.00 |
BY: |
0.04 |
6.78 |
V2294 Oph |
17.00:17.00:9.00 |
-8.00:44.00:0.00 |
M |
5.70 |
3.99 |
V2296 Oph |
17.00:25.00:40.00 |
+5.00:4.00:42.00 |
M |
4.10 |
3.00 |
V2297 Oph |
17.00:30.00:49.00 |
+8.00:22.00:42.00 |
M |
7.50 |
6.70 |
V2300 Oph |
17.00:57.00:41.20 |
+6.00:33.00:20.00 |
ELL: |
0.02 |
6.70 |
V2302 Oph |
18.00:6.00:56.00 |
+9.00:11.00:42.00 |
M |
5.50 |
4.07 |
zet Oph |
16.00:34.00:24.10 |
-10.00:28.00:3.00 |
GCAS |
2.58 |
2.56 |
tet Oph |
17.00:18.00:56.20 |
-24.00:57.00:5.00 |
BCEP |
3.31 |
3.25 |
kap Oph |
16.00:55.00:18.00 |
+9.00:27.00:5.00 |
LB: |
5.00 |
4.10 |
khi Oph |
16.00:24.00:7.30 |
-18.00:20.00:40.00 |
GCAS |
5.00 |
4.18 |
ome Oph |
16.00:29.00:10.10 |
-21.00:21.00:40.00 |
ACV |
4.51 |
4.44 |
|
|
|
|
(Saguaro Astronomy Club Catalog) |
|
Only Objects <= 8.0 magnitude |
|
Name |
R.A.
(hh mm.m) |
Dec.
(deg mm) |
Mag
5 |
Sep
6 |
PA
7 |
Tirion |
Uranometria |
H 19 |
16 25.6 |
-23 26 |
5.2, 5.9 |
3.10 |
342 |
22 |
336 |
H 19 |
16 25.6 |
-23 26 |
5.2, 7.8 |
151.00 |
344 |
22 |
336 |
H 19 |
16 25.6 |
-23 26 |
5.2, 6.9 |
156.00 |
253 |
22 |
336 |
SHJ 243 |
17 15.4 |
-26 33 |
5.3, 5.3 |
4.60 |
154 |
22 |
337 |
SHJ 243 |
17 15.4 |
-26 33 |
6.3, 7.8 |
732.00 |
74 |
22 |
337 |
SHJ 243 |
17 15.4 |
-26 33 |
5.3, 8.0 |
10.80 |
316 |
22 |
337 |
H 25 |
17 18.0 |
-24 17 |
5.4, 6.9 |
10.20 |
355 |
22 |
337/ 338 |
SHJ 251 |
17 39.1 |
02 01 |
6.4, 7.5 |
111.20 |
328 |
15 |
248 |
STF 2202 |
17 44.6 |
02 34 |
6.2, 6.6 |
20.60 |
93 |
15 |
248 |
S 694 |
17 52.0 |
01 06 |
6.8, 7.1 |
81.80 |
237 |
15 |
248/ 249 |
STF 2262 |
18 03.0 |
-08 11 |
5.3, 6.0 |
1.90 |
278 |
15/ 16 |
294 |
STF 2276 |
18 05.7 |
12 00 |
7.0, 7.4 |
6.90 |
257 |
15/ 16 |
204 |
|