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Sagittarius
Abbreviation: Sgr
Genitive: Sagittarii
Right Ascension: 19.11 hours
Declination: -25.77 degrees
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Sagittarius, the Archer, can be seen in the summer in the Northern Hemisphere
and in winter in the Southern.
Sagittarius probably originated with the Babylonians. He stands with
his bow aimed at the heart of Scorpio. Sagittarius was Babylon's god of
War.
In Greek mythology, the centaur Chiron invented Sagittarius so that the
Argonauts could find their way to Colchis.
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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 |
KAUS AUSTRALIS |
18.00:24.00:10.32 |
-34.00:23.00:4.73 |
1.85 |
NUNKI |
18.00:55.00:15.92 |
-26.00:17.00:48.23 |
2.02 |
KAUS MEDIA |
18.00:20.00:59.65 |
-29.00:49.00:41.33 |
2.70 |
KAUS BOREALIS |
18.00:27.00:58.24 |
-25.00:25.00:18.15 |
2.81 |
PI SGR |
19.00:9.00:45.83 |
-21.00:1.00:25.06 |
2.89 |
ALNASL |
18.00:5.00:48.49 |
-30.00:25.00:26.69 |
2.99 |
ETA SGR |
18.00:17.00:37.64 |
-36.00:45.00:42.15 |
3.11 |
XI2 SGR |
18.00:57.00:43.79 |
-21.00:6.00:23.97 |
3.51 |
MU SGR |
18.00:13.00:45.81 |
-21.00:3.00:31.79 |
3.86 |
RUKBAT |
19.00:23.00:53.16 |
-40.00:36.00:57.58 |
3.97 |
IOT SGR |
19.00:55.00:15.69 |
-41.00:52.00:6.05 |
4.13 |
THE1 SGR |
19.00:59.00:44.18 |
-35.00:16.00:34.74 |
4.37 |
62 SGR |
20.00:2.00:39.49 |
-27.00:42.00:35.40 |
4.58 |
52 SGR |
19.00:36.00:42.43 |
-24.00:53.00:0.95 |
4.60 |
UPS SGR |
19.00:21.00:43.62 |
-15.00:57.00:18.09 |
4.61 |
56 SGR |
19.00:46.00:21.73 |
-19.00:45.00:40.01 |
4.88 |
43 SGR |
19.00:17.00:38.07 |
-18.00:57.00:10.72 |
4.90 |
61 SGR |
19.00:57.00:57.03 |
-15.00:29.00:29.43 |
5.02 |
55 SGR |
19.00:42.00:31.13 |
-16.00:7.00:26.43 |
5.06 |
54 SGR |
19.00:40.00:43.38 |
-16.00:17.00:35.66 |
5.30 |
KAP1 SGR |
20.00:22.00:27.51 |
-42.00:2.00:58.58 |
5.59 |
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(PAS Catalog) |
M-17
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M-17 The Omega or Swan Nebula. Probably my personal favorite example
of nebulosity, M-17 is seen as a curving check mark relatively bright nebulosity,
with many dark mottlings seen, especially along its straighter portion.
As with most astronomical objects, the longer this nebula is studied, the
more detail becomes apparent. A UHC filter is helpful, but definitely not
necessary with this celestial gem.
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M-18
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M-18 is an open cluster, and is best observed in small telescopes, which
show over a dozen of fairly bright stars (the Sky Catalog 2000 lists it
with 20 members).
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M-20
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M-20 The Trifid Nebula. Only a short distance north of M-8, this object
is rather easily found, but is considerably fainter than that object. A
double star is seen surrounded by a mostly circular patch of light. This
patch of light is divided into three separate regions by dark lanes which
intersect near its center. On a good night, a fainter region of reflection
nebulosity of almost equal size as the main portion can be seen to the north.
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M-21
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M-21 is an open cluster which shows quite a strong concentration of
stars near its center.
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M-22
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M-22 Probably the finest globular cluster easily seen by observers at
temperate northern latitudes. This cluster is about 15-20' in diameter,
and is fairly easily resolved to its center. Many stars are seen in this
rather loosely gathered globular cluster. This is a 'must see' object.
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M-23
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M-23 is an open cluster, and is a beautiful object for small telescopes
and binoculars in the summer Milky Way.
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M-24
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M-24 The Small Sagittarius Star Cloud. This large and milky patch of
light is easily seen with the naked eye as a disconnected portion of the
Milky Way. Its large size makes it best seen in binoculars. Dark streaks
running its length are seen against a backdrop of countless stars. Within
its boundaries lies
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M-25
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M-25 is an open cluster.
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M-28
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M-28 is a globular cluster, which is slightly elliptical shaped according
to H. Shapley. To resolve it into stars, larger instruments are required;
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M-54
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M-54 is cataloged as a globular cluster, but it is actually too far
away to be in the Milky-Way galaxy. It is bright but small so that it may
be overlooked in smaller binoculars (i.e. taken for a star), its bright
core being only 2.1' in diameter, while the outlayers reach out to 6' on
photos, or even to 9.1' at very long exposures.
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M-55
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M-55 is a large globular cluster (about 19', roughly 2/3 of the Moon's
apparent diameter) but has such a loose appearence
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M-69
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M-69, similar as its neighbor M70, is one of the smaller and fainter
globular clusters in Messier's catalog. It can just be seen on a dark night
with a 7x50 or 10x50 pair of binoculars,
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M-70
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Appearing approximately as bright and big as its neighbor M69, globular
star cluster M70 is indeed only a little more luminous and little bigger,
and a bit more remote (28,000 light years). Both are quite close to the
galactic center, so they are both subject to quite strong tidal gravitational
forces.
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M-75
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M-75 is one of the more remote of Messier's globular clusters, lying
well beyond the Galactic center.
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M-8
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M-8 The Lagoon Nebula. With the possible exception of the Great Orion
Nebula (M-42), this is probably the finest cluster and nebula combination
in the heavens. A large and loosely scattered open cluster is seen in juxtaposition
with a large and swirling mist of nebulosity. Many dark regions can be seen
in looping patterns which are highlighted by the brighter regions. This
object is easily seen in finder scopes, binoculars, and with the naked eye.
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NGC-6440
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NGC 6440 This is a small, highly concentrated globular cluster with
an almost stellar core. I was not able to resolve it in my telescope, but
it makes a fine low power eyepiece pair with the next object.
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NGC-6445
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NGC 6445 This planetary nebula is rather large, about 50 seconds in
diameter. It is grey, and averted vision hints at a darker region near its
center, implying angularity. There is a field star very close to, but not
imbedded in the northwest side of the nebula.
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NGC-6603
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NGC 6603, which has sometimes been erroneously identified as M- 24.
This cluster is a small and tightly gathered grouping of stars which is
best seen through a telescope.
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NGC-6818
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NGC 6818 Another planetary nebula, about 15-20 seconds in diameter with
a definite blue-green color to it. It is slightly extended in the north-south
direction, and angularity is hinted at with averted vision.
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NGC-6822
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NGC 6822 Barnard's Galaxy. Only a short distance away from NGC 6818,
this elusive galaxy is actually a member of the Local Group of galaxies.
It is a low mass galaxy whose feeble light is spread over an area of about
15'x5', and is extended in the north-south direction. This faint object
is best seen on nights of excellent clarity, and with instruments of moderate
aperture.
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(Saguaro Astronomy Club Catalog) |
|
Only Objects less than 10.0 Mag. |
|
Object |
R.A. |
Dec. |
Object Type
3
|
Mag. |
Uranometria |
Tirion |
Cr 347 |
17 46.4 |
-29 18 |
OPNCL |
08.8 |
377 |
22 |
NGC 6440 |
17 48.9 |
-20 22 |
GLOCL |
09.7 |
338 |
22 |
Cr 351 |
17 49.4 |
-28 44 |
OPNCL |
09.3 |
377 |
22 |
NGC 6469 |
17 52.9 |
-22 21 |
OPNCL |
08.2 |
339 |
22 |
NGC 6652 |
18 35.8 |
-32 59 |
GLOCL |
08.9 |
378 |
22 |
NGC 6494 |
17 56.8 |
-19 01 |
OPNCL |
05.5 |
339 |
15 |
NGC 6507 |
17 59.6 |
-17 24 |
OPNCL |
09.6 |
339 |
15 |
Tr 31 |
17 59.9 |
-28 11 |
OPNCL |
09.8 |
377 |
22 |
Bochum 14 |
18 02.0 |
-23 42 |
OPNCL |
09.3 |
339 |
22 |
NGC 6514 |
18 02.3 |
-23 02 |
CL+NB |
06.3 |
339 |
22 |
NGC 6523 |
18 03.1 |
-24 23 |
CL+NB |
05 |
339 |
22 |
NGC 6520 |
18 03.4 |
-27 54 |
OPNCL |
07.6 |
339 |
22 |
NGC 6522 |
18 03.6 |
-30 02 |
GLOCL |
08.6 |
377 |
22 |
NGC 6531 |
18 04.6 |
-22 30 |
OPNCL |
05.9 |
339 |
22 |
NGC 6530 |
18 04.8 |
-24 20 |
OPNCL |
04.6 |
339 |
22 |
NGC 6528 |
18 04.8 |
-30 03 |
GLOCL |
09.5 |
377 |
22 |
NGC 6546 |
18 07.2 |
-23 20 |
OPNCL |
08 |
339 |
22 |
NGC 6544 |
18 07.3 |
-25 00 |
GLOCL |
08.3 |
339 |
22 |
NGC 6553 |
18 09.3 |
-25 54 |
GLOCL |
08.3 |
339 |
22 |
Cr 367 |
18 09.6 |
-23 59 |
OPNCL |
06.4 |
339 |
22 |
NGC 6568 |
18 12.8 |
-21 36 |
OPNCL |
08.6 |
339 |
22 |
NGC 6569 |
18 13.6 |
-31 50 |
GLOCL |
08.7 |
377 |
22 |
NGC 6583 |
18 15.8 |
-22 08 |
OPNCL |
10.0 |
339 |
22 |
Cr 469 |
18 16.4 |
-18 13 |
OPNCL |
09.1 |
339 |
15 |
Mel 197 |
18 17.0 |
-18 35 |
OPNCL |
04 |
339 |
22 |
NGC 6595 |
18 17.0 |
-19 53 |
OPNCL |
07 |
339 |
15 |
NGC 6613 |
18 19.9 |
-17 08 |
OPNCL |
06.9 |
339 |
15 |
NGC 6618 |
18 20.8 |
-16 11 |
CL+NB |
06 |
294 |
15 |
NGC 6624 |
18 23.7 |
-30 22 |
GLOCL |
08.3 |
378 |
22 |
NGC 6626 |
18 24.5 |
-24 52 |
GLOCL |
06.9 |
340 |
22 |
Tr 33 |
18 24.8 |
-19 41 |
OPNCL |
07.8 |
340 |
15 |
NGC 6638 |
18 30.9 |
-25 30 |
GLOCL |
09.2 |
340 |
22 |
IC 4725 |
18 31.6 |
-19 15 |
OPNCL |
04.6 |
340 |
15 |
NGC 6642 |
18 31.9 |
-23 29 |
GLOCL |
08.8 |
340 |
22 |
NGC 6645 |
18 32.6 |
-16 54 |
OPNCL |
08.5 |
295 |
15 |
NGC 6647 |
18 33.3 |
-17 20 |
OPNCL |
08 |
340 |
15 |
NGC 6637 |
18 34.4 |
-32 21 |
GLOCL |
07.7 |
378 |
22 |
NGC 6656 |
18 36.4 |
-23 54 |
GLOCL |
05.1 |
340 |
22 |
NGC 6681 |
18 43.2 |
-32 18 |
GLOCL |
08.1 |
378 |
22 |
Cr 394 |
18 53.5 |
-20 23 |
OPNCL |
06.3 |
340 |
22 |
NGC 6716 |
18 54.6 |
-19 53 |
OPNCL |
07.5 |
340 |
15 |
Pal 9 |
18 55.1 |
-22 42 |
GLOCL |
09.2 |
340 |
22 |
NGC 6715 |
18 55.1 |
-30 29 |
GLOCL |
07.7 |
378 |
22 |
NGC 6723 |
18 59.6 |
-36 38 |
GLOCL |
07.3 |
378 |
22 |
NGC 6809 |
19 40.0 |
-30 58 |
GLOCL |
07 |
379 |
22 |
NGC 6818 |
19 44.0 |
-14 09 |
PLNNB |
10.0 |
297 |
16 |
NGC 6822 |
19 44.9 |
-14 45 |
GALXY |
08.8 |
297 |
16 |
NGC 6864 |
20 06.1 |
-21 55 |
GLOCL |
08.6 |
343 |
23 |
|
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|
(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 Sgr |
18.00:28.00:56.50 |
-19.00:9.00:42.00 |
DCEP |
7.15 |
6.28 |
W Sgr |
18.00:1.00:49.50 |
-29.00:35.00:3.00 |
DCEP |
5.14 |
4.29 |
X Sgr |
17.00:44.00:24.70 |
-27.00:48.00:49.00 |
DCEP |
4.90 |
4.20 |
Y Sgr |
18.00:18.00:26.50 |
-18.00:53.00:3.00 |
DCEP |
6.24 |
5.25 |
RS Sgr |
18.00:14.00:17.20 |
-34.00:7.00:35.00 |
EA/SD |
6.97 |
6.01 |
YZ Sgr |
18.00:46.00:35.10 |
-16.00:46.00:52.00 |
DCEP |
7.76 |
7.02 |
AP Sgr |
18.00:10.00:0.20 |
-23.00:7.00:52.00 |
DCEP |
7.41 |
6.52 |
BB Sgr |
18.00:48.00:2.00 |
-20.00:21.00:19.00 |
DCEP |
7.30 |
6.55 |
V0350 Sgr |
18.00:42.00:19.10 |
-20.00:42.00:1.00 |
DCEP |
7.83 |
7.08 |
V0356 Sgr |
18.00:44.00:54.40 |
-20.00:19.00:49.00 |
EA/DS: |
7.66 |
6.84 |
V0505 Sgr |
19.00:50.00:17.20 |
-14.00:43.00:58.00 |
EA/SD |
7.51 |
6.46 |
V1647 Sgr |
17.00:55.00:49.50 |
-36.00:56.00:8.00 |
EA/DM |
7.57 |
6.94 |
V1942 Sgr |
19.00:16.00:17.80 |
-16.00:0.00:3.00 |
LB |
7.00 |
6.74 |
V2509 Sgr |
18.00:12.00:28.40 |
-35.00:39.00:16.00 |
EB/KE |
7.71 |
7.35 |
V3508 Sgr |
18.00:28.00:27.40 |
-19.00:11.00:41.00 |
GCAS |
8.00 |
7.70 |
V3790 Sgr |
19.00:30.00:28.20 |
-16.00:43.00:6.00 |
LB: |
7.54 |
7.24 |
V3792 Sgr |
18.00:5.00:48.50 |
-25.00:28.00:54.00 |
EB/DM |
6.88 |
6.43 |
V3872 Sgr |
19.00:59.00:35.20 |
-27.00:51.00:2.00 |
LB |
4.64 |
4.45 |
V3877 Sgr |
18.00:33.00:5.00 |
-35.00:29.00:20.00 |
SRB |
7.30 |
6.84 |
V3879 Sgr |
18.00:39.00:58.40 |
-19.00:20.00:1.00 |
SRB |
6.58 |
6.05 |
V3880 Sgr |
19.00:5.00:56.00 |
-22.00:19.00:12.00 |
M |
3.10 |
1.70 |
V3894 Sgr |
17.00:45.00:20.10 |
-26.00:57.00:33.00 |
EB/D |
6.39 |
6.21 |
V3903 Sgr |
18.00:6.00:14.30 |
-23.00:59.00:52.00 |
INA: |
7.45 |
7.00 |
V3954 Sgr |
19.00:8.00:0.50 |
-15.00:9.00:39.00 |
LB: |
7.52 |
7.15 |
V3961 Sgr |
19.00:48.00:27.10 |
-40.00:0.00:10.00 |
ACV |
5.34 |
5.28 |
V3966 Sgr |
17.00:55.00:6.00 |
-28.00:54.00:30.00 |
M |
7.32 |
7.00 |
V3968 Sgr |
17.00:55.00:13.00 |
-28.00:54.00:24.00 |
M |
7.32 |
7.00 |
V3970 Sgr |
17.00:55.00:19.00 |
-29.00:12.00:54.00 |
M |
6.42 |
6.00 |
V3972 Sgr |
17.00:55.00:33.00 |
-29.00:7.00:6.00 |
M |
7.15 |
6.68 |
V3977 Sgr |
17.00:56.00:4.00 |
-28.00:58.00:48.00 |
M |
7.84 |
7.34 |
V3980 Sgr |
17.00:56.00:20.00 |
-28.00:50.00:30.00 |
M |
7.30 |
7.13 |
V3982 Sgr |
17.00:56.00:32.00 |
-29.00:14.00:12.00 |
M |
6.71 |
6.49 |
V3984 Sgr |
17.00:56.00:38.60 |
-33.00:24.00:22.00 |
GCAS |
0.18 |
7.38 |
V3985 Sgr |
17.00:56.00:37.00 |
-28.00:59.00:24.00 |
SR: |
6.60 |
6.25 |
V3987 Sgr |
17.00:56.00:46.00 |
-28.00:53.00:30.00 |
M |
6.39 |
6.12 |
V3990 Sgr |
17.00:57.00:8.00 |
-28.00:55.00:30.00 |
M |
7.83 |
7.36 |
V3991 Sgr |
17.00:57.00:10.00 |
-28.00:50.00:6.00 |
SR: |
7.62 |
7.47 |
V3992 Sgr |
17.00:57.00:11.00 |
-29.00:6.00:54.00 |
M |
7.28 |
6.80 |
V3995 Sgr |
17.00:57.00:34.00 |
-29.00:11.00:12.00 |
M |
6.98 |
6.69 |
V3996 Sgr |
17.00:57.00:37.00 |
-29.00:10.00:24.00 |
M |
7.80 |
7.41 |
V3999 Sgr |
17.00:59.00:7.00 |
-29.00:59.00:18.00 |
M |
6.58 |
5.67 |
V4000 Sgr |
17.00:59.00:19.00 |
-30.00:6.00:54.00 |
M |
7.31 |
6.44 |
V4001 Sgr |
17.00:59.00:29.00 |
-30.00:5.00:30.00 |
M |
6.57 |
5.77 |
V4005 Sgr |
18.00:0.00:42.00 |
-30.00:1.00:0.00 |
M |
7.10 |
7.03 |
V4008 Sgr |
18.00:11.00:29.00 |
-27.00:58.00:18.00 |
M: |
7.15 |
7.02 |
V4010 Sgr |
18.00:12.00:19.00 |
-27.00:59.00:24.00 |
M |
6.28 |
6.15 |
V4024 Sgr |
19.00:5.00:20.40 |
-19.00:22.00:13.00 |
GCAS |
5.60 |
5.34 |
V4026 Sgr |
19.00:44.00:16.70 |
-17.00:12.00:6.00 |
SR: |
6.90 |
6.69 |
V4028 Sgr |
18.00:18.00:26.60 |
-24.00:56.00:22.00 |
SR: |
6.38 |
6.10 |
V4031 Sgr |
18.00:26.00:16.90 |
-25.00:17.00:25.00 |
GCAS |
6.67 |
6.52 |
V4035 Sgr |
17.00:59.00:6.00 |
-30.00:0.00:42.00 |
M |
7.89 |
7.10 |
V4036 Sgr |
17.00:59.00:14.00 |
-30.00:5.00:42.00 |
M |
7.20 |
6.95 |
V4037 Sgr |
17.00:59.00:23.00 |
-30.00:0.00:0.00 |
M |
5.81 |
5.74 |
V4038 Sgr |
17.00:59.00:56.00 |
-30.00:5.00:30.00 |
M |
7.24 |
6.94 |
V4039 Sgr |
18.00:0.00:8.00 |
-30.00:12.00:12.00 |
M |
7.23 |
7.01 |
V4042 Sgr |
18.00:1.00:2.00 |
-29.00:48.00:36.00 |
M |
7.48 |
6.71 |
V4044 Sgr |
18.00:1.00:31.00 |
-29.00:52.00:54.00 |
M |
7.07 |
6.66 |
V4045 Sgr |
18.00:8.00:47.50 |
-28.00:54.00:51.00 |
ACV |
6.54 |
6.51 |
V4050 Sgr |
18.00:19.00:29.70 |
-36.00:41.00:41.00 |
ACV |
0.01 |
5.31 |
V4062 Sgr |
19.00:35.00:49.10 |
-28.00:43.00:19.00 |
ACV |
6.75 |
6.71 |
V4063 Sgr |
19.00:39.00:35.90 |
-24.00:29.00:52.00 |
DSCT |
0.12 |
7.90 |
V4064 Sgr |
19.00:48.00:5.50 |
-27.00:36.00:1.00 |
ACV |
7.36 |
7.23 |
V4088 Sgr |
18.00:48.00:8.50 |
-20.00:21.00:36.00 |
E |
7.87 |
7.49 |
V4089 Sgr |
19.00:30.00:42.90 |
-40.00:8.00:38.00 |
EA/DM |
6.07 |
5.87 |
V4090 Sgr |
19.00:36.00:31.50 |
-39.00:32.00:53.00 |
EA/DM |
6.81 |
6.58 |
V4120 Sgr |
18.00:0.00:59.00 |
-20.00:19.00:30.00 |
M |
1.00 |
0.60 |
V4133 Sgr |
20.00:0.00:14.80 |
-38.00:59.00:35.00 |
ACV |
6.92 |
6.90 |
V4138 Sgr |
19.00:19.00:42.80 |
-20.00:44.00:17.00 |
RS |
6.85 |
6.57 |
V4153 Sgr |
19.00:17.00:18.00 |
-14.00:32.00:46.00 |
EA: |
7.87 |
7.64 |
V4180 Sgr |
18.00:27.00:21.00 |
-26.00:32.00:24.00 |
M |
7.89 |
6.84 |
V4184 Sgr |
18.00:29.00:3.00 |
-24.00:59.00:36.00 |
M |
4.26 |
3.21 |
V4190 Sgr |
18.00:32.00:22.20 |
-20.00:52.00:54.00 |
DSCTC |
6.48 |
6.44 |
V4198 Sgr |
19.00:4.00:12.80 |
-18.00:48.00:59.00 |
* |
6.29 |
6.23 |
V4199 Sgr |
19.00:18.00:41.40 |
-19.00:19.00:46.00 |
* |
6.26 |
6.18 |
V4200 Sgr |
19.00:51.00:18.20 |
-24.00:4.00:1.00 |
BY |
0.07 |
6.18 |
V4201 Sgr |
17.00:50.00:11.00 |
-26.00:56.00:0.00 |
SR |
2.20 |
7.76 |
V4333 Sgr |
19.00:33.00:31.30 |
-18.00:57.00:53.00 |
DSCT |
5.60 |
5.48 |
eta Sgr |
18.00:14.00:14.60 |
-36.00:46.00:43.00 |
LB: |
3.12 |
3.05 |
mu Sgr |
18.00:10.00:46.30 |
-21.00:4.00:25.00 |
EA+ACYG |
3.88 |
3.80 |
rho 1 Sgr |
19.00:18.00:46.40 |
-17.00:56.00:35.00 |
DSCTC |
3.94 |
3.90 |
ups Sgr |
19.00:18.00:51.80 |
-16.00:3.00:2.00 |
EB/GS |
4.61 |
4.53 |
|
|
|
|
(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 |
HJ 5003 |
17 59.1 |
-30 18 |
5.0, 7.0 |
6.00 |
106 |
22 |
377 |
BU 132 |
18 11.2 |
-19 50 |
6.9, 7.3 |
1.30 |
195 |
15/ 16 |
339 |
BU 760 |
18 17.7 |
-36 44 |
3.2, 7.8 |
3.60 |
105 |
22 |
377/ 378 |
JC 6 |
18 25.4 |
-20 32 |
5.1, 7.6 |
1.70 |
288 |
15/ 16 |
339/ 340 |
BU 133 |
18 27.7 |
-26 38 |
6.9, 7.0 |
1.30 |
247 |
22 |
339/ 340 |
STN 62 |
18 34.5 |
-34 49 |
7.6, 7.9 |
2.10 |
134 |
22 |
378 |
H 126 |
19 04.4 |
-21 32 |
7.5, 7.8 |
1.20 |
204 |
22 |
341 |
STN 46 |
19 07.8 |
-15 59 |
6.8, 7.3 |
4.80 |
195 |
16 |
296 |
HJ 5094 |
19 12.8 |
-33 51 |
7.3, 7.9 |
24.70 |
187 |
22 |
379 |
S 715 |
19 17.6 |
-15 58 |
7.0, 7.5 |
8.40 |
16 |
16 |
296 |
DUN 226 |
19 22.6 |
-44 27 |
4.3, 7.4 |
28.30 |
77 |
22 |
410 |
S 722 |
19 39.1 |
-16 54 |
7.1, 7.6 |
10.20 |
236 |
16 |
297 |
DUN 230 |
20 17.8 |
-40 11 |
7.7, 8.0 |
9.80 |
117 |
23 |
380/ 381/ 411 |
|