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Perseus
Abbreviation: Per
Genitive: Persei
Right Ascension: 3.71 hours
Declination: 41.77 degrees
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Perseus, the Rescuer of Andromeda, can be seen in late summer and autumn
in the Northern Hemisphere.
His quest was to bring back the head of Medusa, not knowing her whereabouts
he went to the three sisters of Polydectes, who were blind and shared a
glass eye. They refused to help him until he stole the eye and would not
return it until they told him where to find Medusa. Using a shield given
to him by Minerva, he avoided looking directly at Medusa and beheaded her.
Pegasus sprang out of the Medusa's blood and he rode him back to Artos,
where he found Andromeda chained to the rocks as a sacrifice to Cetus, using
the Gorgons head, Cetus turned to stone. Perseus and Andromeda fell in love,
both were placed among the stars.
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Bright Stars | Deep Sky |
Other Deep Sky | Variable Stars
| Double Stars |
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(Yale Bright Star Catalog) |
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Common Name
or Bayer Number
1 |
RA |
DEC |
Magnitude
2 |
MIRFAK |
3.00:24.00:19.36 |
+49.00:51.00:40.34 |
1.79 |
ALGOL |
3.00:8.00:10.13 |
+40.00:57.00:20.43 |
2.10 |
ATIK |
3.00:54.00:7.92 |
+31.00:53.00:1.01 |
2.85 |
EPS PER |
3.00:57.00:51.22 |
+40.00:0.00:36.72 |
2.89 |
GAM PER |
3.00:4.00:47.79 |
+53.00:30.00:23.29 |
2.93 |
DEL PER |
3.00:42.00:55.49 |
+47.00:47.00:15.30 |
3.01 |
RHO PER |
3.00:5.00:10.59 |
+38.00:50.00:25.01 |
3.30 |
ETA PER |
2.00:50.00:41.81 |
+55.00:53.00:43.80 |
3.76 |
NU PER |
3.00:45.00:11.63 |
+42.00:34.00:42.70 |
3.77 |
TAU PER |
2.00:54.00:15.45 |
+52.00:45.00:44.95 |
3.95 |
MENKIB |
3.00:58.00:57.90 |
+35.00:47.00:27.59 |
4.04 |
48 PER |
4.00:8.00:39.68 |
+47.00:42.00:45.09 |
4.04 |
IOT PER |
3.00:9.00:4.01 |
+49.00:36.00:47.89 |
4.05 |
PHI PER |
1.00:43.00:39.63 |
+50.00:41.00:19.48 |
4.07 |
THE PER |
2.00:44.00:11.98 |
+49.00:13.00:42.48 |
4.12 |
MU PER |
4.00:14.00:53.85 |
+48.00:24.00:33.60 |
4.14 |
LAM PER |
4.00:6.00:35.03 |
+50.00:21.00:4.58 |
4.29 |
SIG PER |
3.00:30.00:34.48 |
+47.00:59.00:42.89 |
4.36 |
24 PER |
2.00:59.00:3.67 |
+35.00:10.00:59.24 |
4.93 |
54 PER |
4.00:20.00:24.64 |
+34.00:34.00:0.27 |
4.93 |
4 PER |
2.00:2.00:18.10 |
+54.00:29.00:15.25 |
5.04 |
14 PER |
2.00:44.00:5.15 |
+44.00:17.00:49.32 |
5.43 |
2 PER |
1.00:52.00:9.35 |
+50.00:47.00:34.21 |
5.79 |
57 PER |
4.00:33.00:24.89 |
+43.00:3.00:49.99 |
6.09 |
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(PAS Catalog) |
Algol
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Algol (Beta Per) This famous variable star dips almost 1.5 magnitudes
every 2.86 days. Its variability is due to a faint star eclipsing a brighter
star. The eclipses last about 10 hours, so a significant brightening or
dimming can easily be observed in one night. Its minima are listed in Sky
and Telescope magazine every month, so if you haven't observed a variable
star yet, give this one a try.
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Alpha Persei Group
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Alpha Persei Group When you look at Alpha Per, it is easy to see granulation
or condensation of the Milky Way in its region. Try looking at this area
with binoculars, and you will be stunned by the wealth of stars in this
area. This is actually a large open cluster having the designation Melotte
20, and contains over 100 stars. Give this area a peek.
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Epsilon Per
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Epsilon Per A difficult split, but a fine yellow-white and blue double
star.
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Eta Per
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Eta Per This double star is an easy split, and shows a pretty yellow-gold
primary and a fainter blue companion.
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M-34
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M-34 This is a fine open cluster, easily seen in binoculars as somewhat
box shaped, with many bright stars resolved. Through a telescope, it is
almost 40' in diameter, made up of primarily bright and some relatively
faint stars, and has a coarse appearance.
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M-76
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M-76 The Little Dumbbell planetary nebula resembles M-27 as seen though
a small telescope. It is bi-lobed, with the southern lobe the brighter of
the two, and the northern being somewhat rectangular. Some dark lanes or
patches are seen with averted vision. This object holds up to magnification
well.
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NGC 869 & 884
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NGC 869 & 884 The Double Cluster. This is one of the finest sights in
the sky. These two open clusters are both large and bright, and fall in
the same low power field of view. NGC 869 is the brighter and more concentrated
of the two, and is dominated by two bright orange stars near its center.
NGC 884 is slightly larger, and has many more orange-red stars. Both clusters
contain over 100 stars each.
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(Saguaro Astronomy Club Catalog) |
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Only Objects less than 10.0 Mag. |
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Object |
R.A. |
Dec. |
Object Type
3
|
Mag. |
Uranometria |
Tirion |
NGC 744 |
01 58.4 |
+55 29 |
OPNCL |
07.9 |
037 |
01 |
Basel 10 |
02 18.8 |
+58 19 |
OPNCL |
09.9 |
037 |
01 |
NGC 869 |
02 19.0 |
+57 09 |
OPNCL |
05.3 |
037 |
01 |
NGC 884 |
02 22.4 |
+57 07 |
OPNCL |
06.1 |
037 |
01 |
Czernik 8 |
02 33.0 |
+58 44 |
OPNCL |
09.7 |
038 |
01 |
NGC 957 |
02 33.6 |
+57 32 |
OPNCL |
07.6 |
038 |
01 |
Tr 2 |
02 37.3 |
+55 59 |
OPNCL |
05.9 |
038 |
01 |
NGC 1023 |
02 40.5 |
+39 03 |
GALXY |
09.4 |
062 |
04 |
NGC 1039 |
02 42.0 |
+42 47 |
OPNCL |
05.2 |
062 |
04 |
NGC 1245 |
03 14.7 |
+47 15 |
OPNCL |
08.4 |
063 |
04 |
Mel 20 |
03 22.0 |
+49 00 |
OPNCL |
01.2 |
063 |
04 |
NGC 1342 |
03 31.6 |
+37 20 |
OPNCL |
06.7 |
094 |
04 |
IC 348 |
03 44.5 |
+32 17 |
CL+NB |
07.3 |
095 |
04 |
NGC 1444 |
03 49.4 |
+52 40 |
OPNCL |
06.6 |
039 |
01 |
NGC 1496 |
04 04.4 |
+52 37 |
OPNCL |
09.6 |
039 |
01 |
NGC 1513 |
04 10.0 |
+49 31 |
OPNCL |
08.4 |
064 |
05 |
NGC 1528 |
04 15.4 |
+51 14 |
OPNCL |
06.4 |
039 |
01 |
NGC 1545 |
04 20.9 |
+50 15 |
OPNCL |
06.2 |
039 |
01 |
NGC 1582 |
04 32.0 |
+43 51 |
OPNCL |
07 |
065 |
05 |
Berk 68 |
04 44.5 |
+42 04 |
OPNCL |
09.8 |
065 |
05 |
Ru 148 |
04 46.5 |
+44 44 |
OPNCL |
09.5 |
065 |
05 |
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(General Catalog of Variable Stars) |
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Only Objects <= 8.0 magnitude |
|
GCVS ID |
R.A.
(hh mm ss.ss) |
Dec.
(deg mm ss) |
Variable Type
4
|
Mag. Min |
Mag. Max |
X Per |
3.00:52.00:15.10 |
+30.00:54.00:1.00 |
GCAS+XP |
7.00 |
6.03 |
AG Per |
4.00:3.00:43.50 |
+33.00:18.00:47.00 |
EA/DM |
7.00 |
6.69 |
AW Per |
4.00:44.00:25.40 |
+36.00:38.00:5.00 |
DCEP |
7.89 |
7.04 |
IW Per |
3.00:30.00:16.70 |
+39.00:43.00:57.00 |
ELL/DM |
5.84 |
5.79 |
IX Per |
3.00:31.00:53.80 |
+31.00:51.00:4.00 |
ELL |
0.02 |
6.66 |
KK Per |
2.00:6.00:48.40 |
+56.00:19.00:25.00 |
LC |
7.89 |
6.60 |
KP Per |
3.00:29.00:12.50 |
+44.00:41.00:14.00 |
BCEP |
0.14 |
6.37 |
KS Per |
4.00:45.00:20.10 |
+43.00:11.00:19.00 |
* |
0.25 |
7.60 |
LT Per |
2.00:54.00:14.70 |
+31.00:44.00:3.00 |
ACV |
5.14 |
5.03 |
MX Per |
4.00:5.00:1.30 |
+47.00:34.00:52.00 |
GCAS |
0.09 |
4.00 |
V0357 Per |
2.00:13.00:27.30 |
+56.00:29.00:16.00 |
BCEP: |
7.52 |
7.44 |
V0376 Per |
3.00:45.00:40.70 |
+43.00:48.00:38.00 |
DSCT |
5.91 |
5.77 |
V0380 Per |
3.00:59.00:51.80 |
+37.00:55.00:2.00 |
ACV |
0.03 |
7.76 |
V0383 Per |
3.00:3.00:26.40 |
+33.00:25.00:58.00 |
ACV: |
7.87 |
7.84 |
V0386 Per |
3.00:54.00:49.50 |
+34.00:40.00:18.00 |
DSCTC |
6.58 |
6.50 |
V0396 Per |
3.00:28.00:35.90 |
+47.00:51.00:17.00 |
SXARI |
5.53 |
5.45 |
V0423 Per |
3.00:12.00:53.40 |
+34.00:30.00:19.00 |
ELL: |
0.03 |
6.65 |
V0425 Per |
2.00:28.00:15.30 |
+57.00:28.00:36.00 |
ACYG |
7.10 |
6.98 |
V0436 Per |
1.00:48.00:41.30 |
+54.00:54.00:3.00 |
EA/D |
5.85 |
5.49 |
V0440 Per |
2.00:20.00:22.00 |
+55.00:8.00:17.00 |
DCEPS |
6.32 |
6.18 |
V0467 Per |
3.00:46.00:22.60 |
+32.00:56.00:23.00 |
E/D |
5.18 |
5.05 |
V0469 Per |
4.00:17.00:55.70 |
+46.00:22.00:53.00 |
BCEP |
4.86 |
4.81 |
V0472 Per |
2.00:5.00:9.90 |
+58.00:11.00:13.00 |
ACYG |
5.74 |
5.64 |
V0474 Per |
2.00:18.00:51.20 |
+55.00:37.00:5.00 |
ACYG |
5.25 |
5.15 |
V0475 Per |
2.00:23.00:9.60 |
+57.00:27.00:17.00 |
ACYG |
7.26 |
7.15 |
V0480 Per |
2.00:45.00:48.30 |
+56.00:52.00:38.00 |
ACYG |
6.30 |
6.23 |
V0490 Per |
4.00:3.00:28.20 |
+32.00:15.00:5.00 |
E: |
7.27 |
6.98 |
V0491 Per |
4.00:4.00:14.00 |
+37.00:56.00:41.00 |
BY |
0.03 |
7.10 |
V0492 Per |
4.00:28.00:37.20 |
+36.00:38.00:15.00 |
RS: |
0.07 |
6.70 |
V0496 Per |
3.00:31.00:56.30 |
+37.00:50.00:57.00 |
ACV |
7.79 |
7.70 |
V0505 Per |
2.00:17.00:45.70 |
+54.00:16.00:54.00 |
EA/DM |
7.46 |
6.87 |
V0509 Per |
3.00:0.00:30.40 |
+47.00:39.00:14.00 |
DSCT |
6.64 |
6.47 |
V0510 Per |
3.00:10.00:29.70 |
+43.00:40.00:40.00 |
RS |
0.22 |
7.30 |
bet Per |
3.00:4.00:54.40 |
+40.00:45.00:52.00 |
EA/SD |
3.39 |
2.12 |
gam Per |
3.00:1.00:9.60 |
+53.00:18.00:44.00 |
EA/GS |
0.55 |
3.63 |
del Per |
3.00:39.00:21.00 |
+47.00:37.00:48.00 |
GCAS: |
3.04 |
2.99 |
eps Per |
3.00:54.00:29.40 |
+39.00:52.00:3.00 |
BCEP |
3.00 |
2.88 |
ksi Per |
3.00:55.00:42.80 |
+35.00:38.00:57.00 |
* |
4.06 |
4.00 |
omi Per |
3.00:41.00:10.60 |
+32.00:7.00:53.00 |
ELL |
3.88 |
3.79 |
rho Per |
3.00:1.00:57.80 |
+38.00:38.00:53.00 |
SRB |
4.00 |
3.30 |
tau Per |
2.00:50.00:41.90 |
+52.00:33.00:34.00 |
EA/GS |
4.07 |
3.94 |
phi Per |
1.00:40.00:30.80 |
+50.00:26.00:16.00 |
GCAS |
4.11 |
3.96 |
psi Per |
3.00:32.00:55.50 |
+48.00:1.00:41.00 |
GCAS |
4.28 |
4.17 |
b Per |
4.00:14.00:28.40 |
+50.00:10.00:29.00 |
ELL |
4.68 |
4.52 |
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(Saguaro Astronomy Club Catalog) |
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Only Objects <= 8.0 magnitude |
|
Name |
R.A.
(hh mm.m) |
Dec.
(deg mm) |
Mag
5 |
Sep
6 |
PA
7 |
Tirion |
Uranometria |
STF 162 |
01 49.2 |
47 53 |
6.5, 7.0 |
2.00 |
202 |
4 |
61 |
STT 25 |
02 16.8 |
57 03 |
6.4, 7.2 |
103.00 |
204 |
1 |
37 |
HJ 1123 |
02 42.0 |
42 47 |
8.0, 8.0 |
20.00 |
248 |
4 |
62 |
STF 307 |
02 50.7 |
55 53 |
3.9, 7.9 |
28.30 |
301 |
1 |
38 |
STF 331 |
03 00.8 |
52 20 |
5.4, 6.8 |
12.30 |
85 |
1 |
38 |
STF 369 |
03 17.1 |
40 29 |
6.7, 8.0 |
3.80 |
29 |
4 |
63 |
BU 533 |
03 35.6 |
31 41 |
7.6, 7.6 |
1.10 |
43 |
4 |
94 |
S 430 |
03 38.3 |
44 48 |
8.0, 8.0 |
41.10 |
95 |
4 |
63/ 64 |
STF 425 |
03 40.1 |
34 07 |
7.6, 7.6 |
1.80 |
74 |
4 |
94/ 95 |
BU 545 |
04 07.4 |
38 01 |
8.0, 7.1 |
233.10 |
30 |
5 |
64/ 95 |
STF 552 |
04 31.4 |
40 01 |
7.0, 7.2 |
9.00 |
114 |
5 |
65 |
SHJ 44 |
04 33.4 |
43 03 |
6.1, 6.8 |
116.20 |
198 |
5 |
65 |
S 451 |
04 36.3 |
47 21 |
7.5, 7.6 |
58.40 |
199 |
5 |
65 |
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