Andromeda is an autumn constellation that is V shaped the best time of year to view Andromeda is during the month of November with the suggested time being 9pm. It occupies 722 square degrees and is located close to the North Pole in the first quadrant of the Northern Hemisphere. Andromeda can be seen at latitudes between +90 degrees and -40 degrees. Using the equatorial coordinate system Andromeda’s right ascension is between 22h and 57.5m and 2h 39.3m and its declination is between 53.19 degrees and 21.68 degrees.
Objects of Interest
Andromeda is home to a large spiral galaxy known as the Andromeda Galaxy. There is a wide hazy patch located half way up on the right side of the constellation this is known as the Andromeda Galaxy. The Andromeda Galaxy is the most distant object visible to the naked eye. The galaxy includes NGC206, a bright giant star cloud. It is known for 14 dwarf galaxies as its satellites. Messier 32 and Messier 110 are the two that are the easiest to find in the night sky. The first elliptical galaxy ever discovered is Messier 32. It is a satellite galaxy to the Andromeda Galaxy. M32
is small, but quite bright, and can easily be seen in a small telescope. [10] The galaxy is suspected to have been much larger at one point, but then lost its outer stars and globular clusters when it collided with the Andromeda Galaxy. Messier 110 is a dwarf elliptical galaxy. It is often classified as a dwarf spheroidal galaxy. In the halo that surrounds it there are eight globular clusters. Atypical
for a dwarf elliptical galaxy, M110 is showing signs of recent star formation. It does not appear to have a supermassive black hole, or at least there is no evidence that one exists at the center of the galaxy.
Name
|
B
|
F
|
HD
|
HIP
|
RA
|
Dec
|
vis.
mag.
|
abs.
mag.
|
Dist. (ly)
|
Sp. class
|
Notes
|
ω And
|
ω[12]
|
48
|
8799
|
6813
|
01h 27m 39.09s
|
+45° 24′ 25.0″
|
4.83
|
2.57
|
92
|
F5IV
|
|
ψ And
|
ψ
|
20
|
223047
|
117221
|
23h 46m 02.04s
|
+46° 25′ 13.0″
|
4.97
|
−3.05
|
1309
|
G5Ib
|
multiple star
|
χ And
|
χ[14]
|
52
|
10072
|
7719
|
01h 39m 21.02s
|
+44° 23′ 10.1″
|
5.01
|
0.66
|
242
|
G8III...
|
|
φ And
|
φ
|
42
|
6811
|
5434
|
01h 09m 30.12s
|
+47° 14′ 30.6″
|
4.26
|
−2.51
|
736
|
B7III
|
Keun Nan Mun, Jūnnánmén (軍南門),[9][10] emission-line star
|
υ And
|
[7][8]
|
50
|
9826
|
7513
|
01h 36m 47.98s
|
+41° 24′ 23.0″
|
4.10
|
3.45
|
44
|
F8V
|
Adhab; has four planets (b, c, d & e)
|
τ And
|
τ
|
53
|
10205
|
7818
|
01h 40m 34.80s
|
+40° 34′ 37.6″
|
4.96
|
−1.64
|
681
|
B8III
|
suspected variable
|
σ And
|
σ
|
25
|
1404
|
1473
|
00h 18m 19.71s
|
+36° 47′ 07.2″
|
4.51
|
1.33
|
141
|
A2V
|
suspected variable
|
ρ And
|
ρ
|
27
|
1671
|
1686
|
00h 21m 07.23s
|
+37° 58′ 07.3″
|
5.16
|
1.71
|
160
|
F5III
|
|
π And
|
π
|
29
|
3369
|
2912
|
00h 36m 52.84s
|
+33° 43′ 09.7″
|
4.34
|
−2.18
|
656
|
B5V
|
spectroscopic binary; suspected variable
|
ο And
|
ο
|
1
|
217675
|
113726
|
23h 01m 55.25s
|
+42° 19′ 33.5″
|
3.62
|
−3.01
|
692
|
B6pv SB
|
quadruple star system; γ Cas variable, Vmax = 3.55m, Vmin = 3.78m
|
ξ And
|
ξ[12]
|
46
|
8207
|
6411
|
01h 22m 20.39s
|
+45° 31′ 43.5″
|
4.87
|
0.98
|
195
|
K0III-IV
|
Adhil
|
ν And
|
ν
|
35
|
4727
|
3881
|
00h 49m 48.83s
|
+41° 04′ 44.2″
|
4.53
|
−2.06
|
679
|
B5V SB
|
spectroscopic binary
|
μ And
|
μ
|
37
|
5448
|
4436
|
00h 56m 45.10s
|
+38° 29′ 57.3″
|
3.86
|
0.75
|
136
|
A5V
|
multiple star
|
λ And
|
λ
|
16
|
222107
|
116584
|
23h 37m 33.71s
|
+46° 27′ 33.0″
|
3.81
|
1.75
|
84
|
G8III-IV
|
RS CVn variable, Vmax = 3.65m, Vmin = 4.05m, P = 53.95 d
|
κ And
|
κ
|
19
|
222439
|
116805
|
23h 40m 24.44s
|
+44° 20′ 02.3″
|
4.15
|
0.57
|
170
|
B9IVn
|
triple star, has a planet (b)
|
ι And
|
ι
|
17
|
222173
|
116631
|
23h 38m 08.18s
|
+43° 16′ 05.1″
|
4.29
|
−1.65
|
502
|
B8V
|
Keff al Salsalat, Manus Catenata[11]
|
θ And
|
θ
|
24
|
1280
|
1366
|
00h 17m 05.54s
|
+38° 40′ 54.0″
|
4.61
|
0.16
|
253
|
A2V
|
suspected variable
|
η And
|
η
|
38
|
5516
|
4463
|
00h 57m 12.43s
|
+23° 25′ 03.9″
|
4.40
|
0.04
|
243
|
G8III-IV
|
spectroscopic binary
|
ζ And
|
ζ
|
34
|
4502
|
3693
|
00h 47m 20.39s
|
+24° 16′ 02.6″
|
4.08
|
0.35
|
181
|
K1II
|
β Lyr/RS CVn variable, Vmax = 3.92m, Vmin = 4.14m, P = 17.7696 d
|
ε And
|
ε
|
30
|
3546
|
3031
|
00h 38m 33.50s
|
+29° 18′ 44.5″
|
4.34
|
0.77
|
169
|
|
|
Table 1 #14
Image #15
Bibliography
-
http://www.topastronomer.com/StarCharts/Constellations/Andromeda.php
-
http://womenshistory.about.com/od/goddessgreece/a/andromeda.htm
-
http://ancienthistory.about.com/od/myths/g/Andromeda.htm
-
http://www.windows2universe.org/mythology/andromeda.html
-
http://www.windows2universe.org/the_universe/Constellations/andromeda.html
-
http://www.theoi.com/Heros/Perseus2.html
-
http://space.about.com/od/starsplanetsgalaxies/ig/Constellations-Pictures/andromeda.htm
-
http://en.wikipedia.org/wiki/Andromeda_(mythology)
-
http://minos-minal-omfalos.blogspot.com/2012/11/andromeda-kolebka-czowieka-myslacego_20.html
-
http://www.constellation-guide.com/constellation-list/andromeda-constellation/
-
http://www.astrostudio.org/xhip.php?hip=5447
-
http://www.dibonsmith.com/and_con.htm
-
http://apod.nasa.gov/apod/ap961121.html
-
http://en.wikipedia.org/wiki/List_of_stars_in_Andromeda
-
http://www.bisque.com/tom/constellation/andromeda.asp