List of stars in Andromeda - AbsoluteAstronomy.com

This is the list of notable star

Star

A star is a massive, luminous sphere of plasma held together by gravity. At the end of its lifetime, a star can also contain a proportion of degenerate matter. The nearest star to Earth is the Sun, which is the source of most of the energy on Earth...

s in the constellation

Constellation

In modern astronomy, a constellation is an internationally defined area of the celestial sphere. These areas are grouped around asterisms, patterns formed by prominent stars within apparent proximity to one another on Earth's night sky....

Andromeda
Andromeda (constellation)
Andromeda is a constellation in the northern sky. It is named after Andromeda, the princess in the Greek legend of Perseus who was chained to a rock to be eaten by the sea monster Cetus...

, sorted by decreasing brightness.

Name	B Bayer designation A Bayer designation is a stellar designation in which a specific star is identified by a Greek letter, followed by the genitive form of its parent constellation's Latin name...	F Flamsteed designation Flamsteed designations for stars are similar to Bayer designations, except that they use numbers instead of Greek letters. Each star is assigned a number and the Latin genitive of the constellation it lies in...	HD Henry Draper Catalogue The Henry Draper Catalogue is an astronomical star catalogue published between 1918 and 1924, giving spectroscopic classifications for 225,300 stars; it was later expanded by the Henry Draper Extension , published between 1925 and 1936, which gave classifications for 46,850 more stars, and by the...	HIP	vis. mag. Apparent magnitude The apparent magnitude of a celestial body is a measure of its brightness as seen by an observer on Earth, adjusted to the value it would have in the absence of the atmosphere...	abs. mag. Absolute magnitude Absolute magnitude is the measure of a celestial object's intrinsic brightness. it is also the apparent magnitude a star would have if it were 32.6 light years away from Earth...	Dist. (ly)	Sp. class Stellar classification In astronomy, stellar classification is a classification of stars based on their spectral characteristics. The spectral class of a star is a designated class of a star describing the ionization of its chromosphere, what atomic excitations are most prominent in the light, giving an objective measure...	Notes
α And Alpha Andromedae Alpha Andromedae , which has the traditional names Alpheratz and Sirrah , is the brightest star in the constellation of Andromeda. Located immediately northeast of the constellation of Pegasus, it is the northeastern star of the Great Square of Pegasus...	α	21	358	677	2.07	−0.30	97	B9p	Alpheratz, Sirrah; α² CVn variable; spectroscopic binary
β And Beta Andromedae Beta Andromedae is a red giant star in the constellation of Andromeda. It has the traditional name Mirach . It has spectral class M0, and is approximately 200 light years away...	β	43	6860	5447	2.07	−1.86	199	M0IIIvar	Mirach; variable Variable star A star is classified as variable if its apparent magnitude as seen from Earth changes over time, whether the changes are due to variations in the star's actual luminosity, or to variations in the amount of the star's light that is blocked from reaching Earth...
γ¹ And Gamma Andromedae Gamma Andromedae is the third brightest star in the constellation of Andromeda. It is also known by the traditional name Almach , from the Arabic العناق الأرض al-‘anāq al-’arđ̧ "the caracal" .Another term for this star used by medieval astronomers...	γ¹	57	12533	9640	2.10	−3.08	355	B8V	Almach, Almaak, Alamak, Almak, Almaach, Khamis al Naamat, Quinta Struthionum; quadruple star system Star system A star system or stellar system is a small number of stars which orbit each other, bound by gravitational attraction. A large number of stars bound by gravitation is generally called a star cluster or galaxy, although, broadly speaking, they are also star systems.-Binary star systems:A stellar...
δ And	δ	31	3627	3092	3.27	0.81	101	K3III...	spectroscopic binary; suspected variable
Andromeda Galaxy Andromeda Galaxy The Andromeda Galaxy is a spiral galaxy approximately 2.5 million light-years from Earth in the constellation Andromeda. It is also known as Messier 31, M31, or NGC 224, and is often referred to as the Great Andromeda Nebula in older texts. Andromeda is the nearest spiral galaxy to the...	(n)	33			3.44 (nebulous)		2540000		BD+40°148; naked eye spiral galaxy Spiral galaxy A spiral galaxy is a certain kind of galaxy originally described by Edwin Hubble in his 1936 work The Realm of the Nebulae and, as such, forms part of the Hubble sequence. Spiral galaxies consist of a flat, rotating disk containing stars, gas and dust, and a central concentration of stars known as... in the Local group Local Group The Local Group is the group of galaxies that includes Earth's galaxy, the Milky Way. The group comprises more than 30 galaxies , with its gravitational center located somewhere between the Milky Way and the Andromeda Galaxy...
51 And 51 Andromedae 51 Andromedae is a 4th magnitude star, the 5th brighest in the constellation Andromeda. It does not have a Bayer designation. It is occasionally called by the proper name Nembus in Bayer's Uranometria and Bode's star atlas Uranographia .Ptolemy included this star in Andromeda in the Almagest, but...		51	9927	7607	3.59	−0.04	174	K3III	multiple star Multiple star A multiple star consists of three or more stars which appear from the Earth to be close to one another in the sky. This may result from the stars being physically close and gravitationally bound to each other, in which case it is physical, or this closeness may be merely apparent, in which case...
ο And Omicron Andromedae Omicron Andromedae is a star system in the constellation Andromeda. It is approximately 692 light years from Earth....	ο	1	217675	113726	3.62	−3.01	692	B6pv SB	quadruple star system Star system A star system or stellar system is a small number of stars which orbit each other, bound by gravitational attraction. A large number of stars bound by gravitation is generally called a star cluster or galaxy, although, broadly speaking, they are also star systems.-Binary star systems:A stellar... ; γ Cas variable,
λ And Lambda Andromedae Lambda Andromedae is a binary star in the constellation Andromeda. It is approximately 84.2 light years from Earth....	λ	16	222107	116584	3.81	1.75	84	G8III-IV	RS CVn variable RS Canum Venaticorum variable RS Canum Venaticorum variables are a type of variable star. They are close binary stars having active chromospheres which can cause large stellar spots. These spots are believed to cause variations in their observed luminosity... ,
μ And Mu Andromedae Mu Andromedae is a star in the constellation Andromeda. It is approximately 136 light years from Earth.Mu Andromedae is a white A-type main sequence dwarf with an apparent magnitude of +3.86.-References:...	μ	37	5448	4436	3.86	0.75	136	A5V	multiple star
ζ And Zeta Andromedae Zeta Andromedae is a star system in the constellation Andromeda. It is approximately 181 light years from Earth....	ζ	34	4502	3693	4.08	0.35	181	K1II	β Lyr Beta Lyrae variable Beta Lyrae variables are a class of close binary stars. Their total brightness is variable because the two component stars orbit each other, and in this orbit one component periodically passes in front of the other one, thereby blocking its light. The two component stars of Beta Lyrae systems are... /RS CVn variable,
υ And Upsilon Andromedae Upsilon Andromedae is a binary star located approximately 44 light-years away from Earth in the constellation Andromeda. The primary star is a yellow-white dwarf star that is somewhat younger than the Sun...		50	9826	7513	4.10	3.45	44	F8V	has four planets Extrasolar planet An extrasolar planet, or exoplanet, is a planet outside the Solar System. A total of such planets have been identified as of . It is now known that a substantial fraction of stars have planets, including perhaps half of all Sun-like stars... (b Upsilon Andromedae b Upsilon Andromedae b, occasionally referred to as Upsilon Andromedae Ab , is an extrasolar planet approximately 44 light-years away from Earth in the constellation of Andromeda . The planet was discovered orbiting the Solar twin star, Upsilon Andromedae, approximately every five days... , c Upsilon Andromedae c Upsilon Andromedae c is an extrasolar planet or star orbiting the Sun-like star Upsilon Andromedae A every 241.2 days. Its discovery in April 1999 by Geoffrey Marcy and R. Paul Butler made Upsilon Andromedae the first known star to host a multiple-planet planetary system... , d Upsilon Andromedae d Upsilon Andromedae d is an extrasolar planet orbiting the Sun-like star Upsilon Andromedae A. Its discovery in April 1999 by Geoffrey Marcy and R. Paul Butler made Upsilon Andromedae the first star to be known to host a multiple-planet planetary system... & e Upsilon Andromedae e Upsilon Andromedae e is the outermost extrasolar planet orbiting the star Upsilon Andromedae in the constellation of Andromeda. This planet is more Jupiter-like than any other known exoplanet.-Discovery:... )
κ And Kappa Andromedae Kappa Andromedae is a star in the constellation Andromeda.Kappa Andromedae is a blue-white B-type subgiant with an apparent magnitude of +4.15. It is approximately 170 light years from Earth.-References:*...	κ	19	222439	116805	4.15	0.57	170	B9IVn	triple star
φ And Phi Andromedae Phi Andromedae is a binary star system near the border of the constellation of Andromeda, approximately 720 light years from the Earth...	φ	42	6811	5434	4.26	−2.51	736	B7III	Keun Nan Mun, Jūnnánmén (軍南門), emission-line star
ι And Iota Andromedae Iota Andromedae is a star in the constellation Andromeda.Iota Andromedae is a blue-white B-type main sequence dwarf with an apparent magnitude of +4.29...	ι	17	222173	116631	4.29	−1.65	502	B8V	Keff al Salsalat, Manus Catenata
π And Pi Andromedae Pi Andromedae is a spectroscopic binary in the constellation Andromeda. It is approximately 660 light years from Earth....	π	29	3369	2912	4.34	−2.18	656	B5V	spectroscopic binary; suspected variable
ε And Epsilon Andromedae Epsilon Andromedae is a G-type giant star in the constellation of Andromeda. It has an apparent visual magnitude of approximately 4.37....	ε	30	3546	3031	4.34	0.77	169	G5III...
η And Eta Andromedae Eta Andromedae is a spectroscopic binary star in the constellation of Andromeda...	η	38	5516	4463	4.40	0.04	243	G8III-IV	spectroscopic binary
σ And Sigma Andromedae Sigma Andromedae is a star in the constellation Andromeda.Sigma Andromedae is a white A-type main sequence dwarf with an apparent magnitude of +4.51. It is approximately 141 light years from Earth....	σ	25	1404	1473	4.51	1.33	141	A2V	suspected variable
ν And Nu Andromedae Nu Andromedae is a binary star in the constellation Andromeda. It is approximately 680 light years from Earth.Nu Andromedae is spectroscopic binary whose components are a blue-white B-type main sequence dwarf and a yellow-white F-type main sequence dwarf...	ν	35	4727	3881	4.53	−2.06	679	B5V SB	spectroscopic binary
7 And 7 Andromedae 7 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 4.53....		7	219080	114570	4.53	2.58	80	F0V
θ And Theta Andromedae Theta Andromedae is a binary star in the constellation Andromeda. It is approximately 253 light years from Earth....	θ	24	1280	1366	4.61	0.16	253	A2V	suspected variable
3 And 3 Andromedae 3 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 4.64....		3	218031	113919	4.64	0.94	179	K0III
65 And 65 Andromedae 65 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 4.73.-References:*...		65	14872	11313	4.73	−0.39	345	K4III	triple star
58 And 58 Andromedae 58 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 4.78....		58	13041	9977	4.78	0.86	198	A5IV-V
8 And 8 Andromedae 8 Andromedae is a red giant star in the constellation Andromeda. Its apparent magnitude is 4.85.-Component:-References:#...		8	219734	115022	4.82	−1.69	655	M2III	suspected variable
ω And Omega Andromedae Omega Andromedae is a star in the constellation Andromeda. It is approximately 92.3 light years from Earth. This is a yellow-white F-type subgiant with an apparent magnitude of +4.83.-References:* *...	ω	48	8799	6813	4.83	2.57	92	F5IV
γ² And Gamma Andromedae Gamma Andromedae is the third brightest star in the constellation of Andromeda. It is also known by the traditional name Almach , from the Arabic العناق الأرض al-‘anāq al-’arđ̧ "the caracal" .Another term for this star used by medieval astronomers...	γ²	57	12534		4.84				component of the γ And system; triple star system
60 And 60 Andromedae 60 Andromedae is a yellow-orange giant star in the constellation Andromeda. Its apparent magnitude is 4.844.-References:#...	b	60	13520	10340	4.84	−1.32	556	K4III	suspected variable
ξ And Xi Andromedae Xi Andromedae is a binary star in the constellation Andromeda. It bears the traditional name Adhil, which is derived from the Arabic الذيل að-ðayl "the train"...	ξ	46	8207	6411	4.87	0.98	195	K0III-IV	Adhil
τ And Tau Andromedae Tau Andromedae is a star in the constellation Andromeda. It is approximately 681 light years from Earth. This is a blue-white B-type giant with an apparent magnitude of +4.96.-References:*...	τ	53	10205	7818	4.96	−1.64	681	B8III	suspected variable
41H. And HD 10307 HD 10307 is a star similar to the sun in mass, temperature and metal content, situated about 41 light-years from Earth in the constellation Andromeda...	υ		10307	7918	4.96	4.45	41	G2V	spectroscopic binary
ψ And Psi Andromedae Psi Andromedae is a double star system in the constellation Andromeda. It is approximately 1310 light years from Earth. The system consists of a spectroscopic binary with a yellow G-type supergiant and a white A-type main sequence dwarf. It has a combined apparent magnitude of +4.97.-References:*...	ψ	20	223047	117221	4.97	−3.05	1309	G5Ib	multiple star
22 And 22 Andromedae 22 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.01....		22	571	841	5.01	−2.44	1006	F2II
χ And Chi Andromedae Chi Andromedae is a star in the constellation Andromeda. It with φ And composed Chinese asterism 軍南門 , "the South Gate of the Camp"....	χ	52	10072	7719	5.01	0.66	242	G8III...
41 And 41 Andromedae 41 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.04....	(d)	41	6658	5317	5.04	1.14	196	A3m
2 And 2 Andromedae 2 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.09.-Components:-References:*...		2	217782	113788	5.09	−0.06	349	A3Vn	multiple star
V428 And			3346	2900	5.14	−1.38	656	K5III	semiregular variable , has a possible planetary system Planetary system A planetary system consists of the various non-stellar objects orbiting a star such as planets, dwarf planets , asteroids, meteoroids, comets, and cosmic dust...
ρ And Rho Andromedae Rho Andromedae is a star in the constellation Andromeda. It is a yellow-white F-type giant with an apparent magnitude of +5.16. This star is approximately 160 light years from Earth.-References:* *...	ρ	27	1671	1686	5.16	1.71	160	F5III
			2421	2225	5.18	0.63	265	A2Vs	spectroscopic binary
64 And 64 Andromedae 64 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.19.64 Andromedae is a deep-yellow coloured G-type giant. It is approximately 375 light years from Earth....		64	14770	11220	5.19	−0.11	375	G8III
GN And 28 Andromedae 28 Andromedae or is a star in the constellation Andromeda. Its apparent magnitude is 5.20.-References:*...		28	2628	2355	5.20	1.43	185	A7III	low-amplitude δ Sct variable Delta Scuti variable A Delta Scuti variable is a variable star which exhibits variations in its luminosity due to both radial and non-radial pulsations of the star's surface. Typical brightness fluctuations are from 0.003 to 0.9 magnitudes in V over a period of a few hours, although the amplitude and period of the... ,
14 And 14 Andromedae 14 Andromedae or 14 And is an orange giant star approximately 258 light-years away in the constellation of Andromeda. The star is a suspected variable star. It is thought that 14 Andromedae was formerly a white or a yellow-white dwarf star early in its life...		14	221345	116076	5.22	0.80	249	K0III	suspected variable; has a planet (b 14 Andromedae b 14 Andromeda b or 14 And b is an extrasolar planet approximately 249 light years away in the constellation of Andromeda. The 186-day period planet orbits about 83% the Earth-Sun distance from the giant star 14 Andromedae. It has a minimum mass 4.8 times the mass of Jupiter... )
49 And 49 Andromedae 49 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.27....	A	49	9057	6999	5.27	0.53	290	K0III
32 And 32 Andromedae 32 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.30....		32	3817	3231	5.30	0.18	344	G8III
4 And 4 Andromedae 4 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.30.-Components:-References:*...		4	218452	114200	5.30	0.20	342	K5III	double star
6 Per 6 Persei 6 Perseus is a star in the constellation Perseus and the constellation Andromeda. Its apparent magnitude is 1.38....		(6)	13530	10366	5.31	1.38	199	G8III:var	spectroscopic binary; suspected variable
62 And 62 Andromedae 62 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.31....	c	62	14212	10819	5.31	0.84	255	A1V
18 And 18 Andromedae 18 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.35....		18	222304	116709	5.35	−0.04	390	B9V
55 And 55 Andromedae 55 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.42.- References :*...		55	11428	8814	5.42	−0.67	540	K1III	double star
11 And		11	219945	115152	5.44	0.43	328	K0III
			3421	2942	5.45	−2.03	1022	G5III
36 And 36 Andromedae 36 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.46. Though appearing as a single star to the naked eye, 36 Andromedae is a close visual binary system with components of magnitudes 6.12 and 6.54, having an orbital period of 167.71 years.-References:*...		36	5286	4288	5.46	2.51	127	K1IV	suspected variable
V340 And 15 Andromedae 15 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.55. Its estimated distance from the Earth is 233.47 light years.-References:*...		15	221756	116354	5.55	1.28	233	A1III	low-amplitude δ Sct Delta Scuti Delta Scuti is a white, F-type giant star in the constellation Scutum. It is approximately 187 light years from Earth. Delta Scuti is the prototype of the Delta Scuti type variable stars. It is a high-amplitude δ Scuti type pulsator with light variations of about 0.15 minutes... variable,
PZ And 63 Andromedae 63 Andromedae or PZ Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.57.-References:*...		63	14392	10944	5.57	0.38	356	B9p Si	α² CVn variable,
47 And 47 Andromedae 47 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.60....		47	8374	6514	5.60	1.54	211	A1m
			10204	7825	5.63	1.05	268	A9IV:
44 And 44 Andromedae 44 Andromedae is a F-type main sequence star in the constellation of Andromeda. It has an apparent visual magnitude of approximately 5.679....		44	6920	5493	5.67	2.06	172	F8V
5 And 5 Andromedae 5 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.68.Coordinates : RA = 23h07min45.3841sec Dec= +49°17'44.793"...		5	218470	114210	5.68	3.02	111	F5V
			5788	4675	5.69	0.14	420	A2Vn	binary star with HD 5789
56 And 56 Andromedae 56 Andromedae is a binary star in the constellation Andromeda. Its apparent magnitude is 5.69. This binary system is composed of two yellow giants and is located near the open cluster NGC 752.-References:*...		56	11749	9021	5.69	0.73	320	G8III...	multiple star
23 And 23 Andromedae 23 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.71....		23	905	1086	5.71	2.99	114	F0IV
			16028	12072	5.72	−0.86	676	K4III	triple star
V388 And 13 Andromedae 13 Andromedae or is a star in the constellation Andromeda. Its apparent magnitude is 5.75.-References:*...		13	220885	115755	5.75	0.97	294	B9III	α² CVn variable,
12 And 12 Andromedae 12 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.77.-Components:-References:*...		12	220117	115280	5.77	2.63	138	F5V	triple star
			1632	1657	5.79	−0.69	646	K5III
45 And 45 Andromedae 45 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.80. It is approximately 790 light years from Earth.-References:*...		45	7019	5550	5.80	−1.44	916	B7III-IV	double star
			14622	11090	5.81	2.44	154	F0III-IV	has two optical companions Double star In observational astronomy, a double star is a pair of stars that appear close to each other in the sky as seen from Earth when viewed through an optical telescope. This can happen either because the pair forms a binary star, i.e...
10 And 10 Andromedae 10 Andromedae is a M-type giant star in the constellation of Andromeda. It has an apparent visual magnitude of approximately 5.806....		10	219981	115191	5.81	−0.30	542	M0III
			222109	116582	5.81	−1.20	823	B8V	double star
			224635	118281	5.81	3.50	95	F8	multiple star
OU And OU Andromedae OU Andromedae is a rotationally variable star.-References:*...			223460	117503	5.86	0.21	440	G1IIIe	FK Com variable,
			1439	1493	5.88	−0.23	543	A0IV
			2767	2475	5.88	0.10	467	K1III...	binary star
			1606	1630	5.89	−0.37	582	B7V	suspected variable
			11727	9001	5.89	−1.52	991	K5III	optical component of 56 And
KK And KK Andromedae KK Andromedae is a variable star.-References:*...			9531	7321	5.90	0.50	392	B8Vp(Si)	α² CVn variable,
			16176	12181	5.91	2.24	177	F5V
6 And 6 Andromedae 6 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.91....		6	218804	114430	5.91	3.65	92	F5IV
			10975	8423	5.94	1.06	308	K0III
39 And 39 Andromedae 39 Andromedae or is a star in the constellation Andromeda. Its apparent magnitude is 5.95.-Components:-References:*...		39	6116	4903	5.95	0.84	344	A5m	double star
			8671	6711	5.98	2.90	135	F7V
AN And 9 Andromedae 9 Andromedae or AN Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 5.98.-References:*...		9	219815	115065	5.98	0.17	472	A7m	β Lyr variable,
			5608	4552	5.99	2.17	190	K0
			224165	117956	6.01	−2.46	1614	G8Ib
			224342	118071	6.01	−2.22	1442	F8III
			4335	3604	6.03	0.32	452	B9.5IIIMNp.
			13594	10403	6.05	2.96	135	F5V
			3883	3269	6.06	0.30	462	A7m	suspected variable
V439 And HD 166 HD 166 or V439 Andromedae is a 6th magnitude star in the constellation Andromeda, approximately 45 light years away from Earth. It is a variable star of the BY Draconis type, with a variation in brightness smaller than 0.2 magnitude...			166	544	6.07	5.39	45	K0V	BY Draconis variable BY Draconis variable BY Draconis variables are main sequence variable stars of late spectral types, usually K or M. The name comes from the archetype for this category of variable star system, BY Draconis. They exhibit variations in their luminosity due to rotation of the star coupled with star spots, and other...
			5118	4185	6.07	0.77	374	K3III:
			221293	116030	6.07	−0.33	621	G9III
			223229	117340	6.08	−1.96	1320	B3IV	suspected variable
			225239	394	6.09	3.26	120	G2V
59 And A 59 Andromedae 59 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 6.09.In August 2010 was reported that 5 planets were discovered in its orbit, and that some characteristics resemble our solar system.-Components:...		59	13294	10176	6.09	1.56	263	B9V	binary star
26 And 26 Andromedae 26 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 6.10.-Components:-References:*...		26	1438	1501	6.10	−0.53	692	B8V	double star
			5526	4501	6.10	0.45	439	K2III
			225218	365	6.11	−2.45	1680	B9III	double star
			7647	5993	6.11	−0.18	590	K5
			1185	1302	6.12	1.28	303	A2V	double star
			218416	114162	6.12	0.55	423	K0III
GO And GO Andromedae HD 4778 or GO Andromedae is a variable star.-References:* *...			4778	3919	6.13	1.34	296	A0p...	α² CVn variable,
			7158	5650	6.13	−0.52	698	M1III
66 And 66 Andromedae 66 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 6.16.-References:*...		66	15138	11465	6.16	2.54	173	F4V	spectroscopic binary
			14372	10924	6.17	−0.87	836	B5V
			743	967	6.18	0.05	550	K4III
			3411	2926	6.18	1.13	334	K2III
			221776	116365	6.18	−0.41	678	K5	double star
			16327	12287	6.19	1.60	270	F6III	triple star
			221246	115996	6.19	−0.91	856	K5III	member of the NGC 7686 NGC 7686 NGC 7686 is a moderate-sized open cluster in the constellation Andromeda, containing about 40 stars. At magnitude 5.6, it is an easy target for binoculars and small telescopes.-External links:*... star cluster
OP And OP Andromedae OP Andromedae is a variable star.-References:*...			9746	7493	6.20	0.65	420	K1III:	BY Dra variable BY Draconis variable BY Draconis variables are main sequence variable stars of late spectral types, usually K or M. The name comes from the archetype for this category of variable star system, BY Draconis. They exhibit variations in their luminosity due to rotation of the star coupled with star spots, and other... ,
			400	699	6.21	3.61	108	F8IV
			14213	10814	6.21	0.50	452	A4V
			952	1123	6.22	1.45	293	A1V
			895	1076	6.24	0.78	403	G0III	triple star
			222451	116824	6.24	3.01	144	F1V
			224906	137	6.25	−1.80	1331	B9IIIp Mn
			11613	8922	6.25	1.13	345	K2
			220105	115261	6.25	1.73	261	A5Vn	double star
			221661	116292	6.25	0.12	548	G8II
			2942	2583	6.26	0.47	469	G8II	triple star
			8774	6776	6.27	3.12	139	F7IVsvar
			2507	2270	6.28	0.51	464	G5III
			8375	6512	6.28	2.43	192	G8IV
			11624	8930	6.28	0.25	525	K0	member of the NGC 752 NGC 752 NGC 752 is an open cluster in the constellation Andromeda. The cluster was discovered by Caroline Herschel in 1783 and cataloged by her brother William Herschel in 1786, although an object that may have been NGC 752 was described by Giovanni Batista Hodierna before 1654.The large cluster lies... star cluster
			7758	6087	6.29	−2.07	1531	K0
			16350	12305	6.29	−0.47	734	B9.5V
			219962	115171	6.29	0.47	475	K1III
			217314	113501	6.31	−0.26	672	K2
			10597	8127	6.32	0.23	540	K5III
			219290	114714	6.32	0.82	411	A0V
			10486	8044	6.33	2.61	181	K2IV
			10874	8370	6.33	2.50	190	F6V
			1075	1208	6.34	−1.70	1320	K5
HD 8673 HD 8673 HD 8673 is an F-type main sequence star approximately 125 light-years away in the constellation of Andromeda. It has an apparent magnitude and absolute magnitude of 6.31 and 3.40 respectively...			8673	6702	6.34	3.43	125	F7V	has a planet (b)
			1083	1215	6.35	0.84	412	A1Vn	double star
			1527	1575	6.35	0.25	541	K1III
			221970	116505	6.35	1.92	251	F6V
CG And CG Andromedae CG Andromedae is a variable star.-References:*...			224801	63	6.36	−0.23	678	B9p SiEu	α² CVn variable,
			16004	12057	6.36	0.11	580	B9MNp...	triple star
			13818	10562	6.37	0.61	462	G9III-IV
LN And LN Andromedae LN Andromedae is a variable star.-References:*...			217811	113802	6.37	−1.42	1177	B2V	double star; short-period β Cep variable Beta Cephei variable Beta Cephei variables are variable stars which exhibit variations in their brightness due to pulsations of the stars' surfaces. The point of maximum brightness roughly corresponds to the maximum contraction of the star. Typically, Beta Cephei variables change in brightness by 0.01 to 0.3... ,
V385 And V385 Andromedae V385 Andromedae is an irregular variable.-References:*...			220524	115530	6.37	−1.55	1249	M0	irregular variable Irregular variable An irregular variable is a type of variable star in which variations in brightness show no regular periodicity. There are two main sub-types of irregular variable: eruptive and pulsating.Eruptive irregular variables are divided into three categories:... ,
GY And			9996	7651	6.38	0.66	455	B9Vp (Cr-Eu)	Promethium Promethium Promethium is a chemical element with the symbol Pm and atomic number 61. It is notable for being the only exclusively radioactive element besides technetium that is followed by chemical elements with stable isotopes.- Prediction :... lines; α² CVn variable,
			13013	9983	6.38	0.78	430	G8III
			218365	114152	6.38	−0.08	638	K0
			9712	7444	6.39	1.01	388	K1III
V529 And			8801	6794	6.42	2.69	182	Am...	δ Scuti variable Delta Scuti variable A Delta Scuti variable is a variable star which exhibits variations in its luminosity due to both radial and non-radial pulsations of the star's surface. Typical brightness fluctuations are from 0.003 to 0.9 magnitudes in V over a period of a few hours, although the amplitude and period of the... ,
			217731	113750	6.43	1.22	359	K0
			222641	116941	6.43	−0.48	786	K5III	suspected variable
			7853	6140	6.44	0.71	456	A5m	double star
			14221	10830	6.44	2.39	210	F4V
			219668	114981	6.44	2.10	241	K0IV
			6114	4911	6.46	1.39	337	A9V	double star
			11884	9163	6.48	−1.24	1140	K0
ET And ET Andromedae ET Andromedae is a variable star.-References:*...			219749	115036	6.48	0.36	545	B9Vp(Si)	α² CVn variable,
			222399	116781	6.49	1.74	291	F2IV	double star
PY And			3322	2865	6.50		701	B8IIImnp...	α² CVn variable
			800	1009	6.50	0.50	517	K0
59 And B 59 Andromedae 59 Andromedae is a star in the constellation Andromeda. Its apparent magnitude is 6.09.In August 2010 was reported that 5 planets were discovered in its orbit, and that some characteristics resemble our solar system.-Components:...		59	13295	10180	6.82	−1.76	1698	A1Vn	component of the 59 And system
R And R Andromedae R Andromedae is a Mira-type variable star in the constellation Andromeda. Its spectral class is type S, because it shows absorption bands of zirconium monoxide in its spectrum...			1967	1901	7.39		54000	S6.5IIIeZr6Ti2	Mira variable Mira variable Mira variables , named after the star Mira, are a class of pulsating variable stars characterized by very red colors, pulsation periods longer than 100 days, and light amplitudes greater than one magnitude in infrared and 2.5 magnitude in visual... ,
HD 13931 HD 13931 HD 13931 is an 8th magnitude G-type star located approximately 144 light years away in the constellation Andromeda. This star is larger, hotter, brighter, and more massive than our Sun. Also its metal content is about 8% greater than the Sun...			13931	10626	7.61	4.38	144	G0	has a planet (b HD 13931 b HD 13931 b is an extrasolar planet which orbits the G-type star HD 13931, located approximately 144 light years away in the constellation Andromeda. This planet takes 11.55 years to orbit the star at the average distance of 5.15 AU or 770 Gm. The planet’s eccentricity is about the same as Earth... )
GRB 34 Groombridge 34 Groombridge 34 is a binary star system located about 11.7 light years from our own Sun. It consists of two red dwarf stars in a nearly circular orbit with a separation of about 147 astronomical units. Both stars in this pair exhibit variability due to random flares and they have been given variable...			1326	1475	8.01	10.25	11.62	M6Ve + M1Ve	16th closest star system, binary Binary star A binary star is a star system consisting of two stars orbiting around their common center of mass. The brighter star is called the primary and the other is its companion star, comes, or secondary... ; both components GQ And and GX And flare star Flare star A flare star is a variable star that can undergo unpredictable dramatic increases in brightness for a few minutes. It is believed that the flares on flare stars are analogous to solar flares in that they are due to magnetic reconnection in the atmospheres of the stars. The brightness increase is... s, ,
HD 15082 HD 15082 HD 15082 is a star located 378 light years away in the constellation of Andromeda. The star is a Delta Scuti variable, and also a planetary transit variable. It is the first Delta Scuti variable known to host a planet...			15082	11397	8.3	3.0	377	A5	has a transiting planet WASP-33b
SAO 73745 SAO 73745 SAO 73745 is a 9th magnitude star in the constellation Andromeda. It is a yellow star of the spectral type G0, meaning it possesses a surface temperature of approximately 6,000 degrees. It is located within 30 arcminutes of the star Alpheratz....					9.04			G0
Z And Z Andromedae Z Andromedae is a symbiotic variable star with an hourglass-shaped nebula . It is the prototype for symbiotic variables, which are a subset of cataclysmic variables.-External links:* * * * * *...			221650	116287	10.53	2.38	1393	M2III + B1eq	prototype of Z And variables,
HAT-P-6 HAT-P-6 HAT-P-6 is a star in the constellation Andromeda, located approximately 650 light years or 200 parsecs away from the Earth. It is an F-type star, implying that it is hotter and more massive than our Sun. The apparent magnitude of the star is +10.54, which can only be visible through the telescope...					10.54	4.03	650	F	has a transiting planet (b HAT-P-6b HAT-P-6b is a transiting extrasolar planet located approximately 650 light-years away in the constellation of Andromeda, orbiting the star HAT-P-6. This hot Jupiter planet orbits with a semi-major axis of about 7.832 gigameters, and takes 92 hours, 28 minutes, 17 seconds and 9 deciseconds to orbit... )
HAT-P-16					10.8	3.9	766	F8	has a transiting planet (b)
HAT-P-32					11.29		1044	F/G	has a transiting planet (b HAT-P-32b HAT-P-32b is a planet in the orbit of the G-type or F-type star HAT-P-32, which is approximately 1,044 light years away from Earth. HAT-P-32b was first recognized as a possible planet by the planet-searching HATNet Project in 2004, although difficulties in measuring its radial velocity prevented... )
WASP-1 WASP-1 WASP-1 is a metal rich magnitude 12 star located about 1240 light-years away in the Andromeda constellation.-Planetary system:In 2006 the extrasolar planet WASP-1b was discovered by the SuperWASP project using the transit method....					11.79	3.89	1239	F7V	has a transiting planet (b WASP-1b WASP-1b is an extrasolar planet orbiting the star WASP-1 located over 1000 light-years away in the constellation Andromeda. In recognition of the regional support given to the project on La Palma, the discoverers gave the planet the alternative designation Garafia-1.-Orbit and mass:The planet's... )
Ross 248					12.29	14.79	10.32	M6e	HH And; 8th closest star system, flare star
HAT-P-19					12.9		701	K	has a transiting planet (b)
HAT-P-28					13.03		1288	G3	has a transiting planet (b)
S And S Andromedae \|- style="background-color: #A0B0FF;" colspan="3"\| Database References\|- bgcolor="#FFFAFA"\| Simbad \|\| \|- bgcolor="#FFFAFA"\| \|\|...							2600000	Ia	SN 1885A; BD+40°147a; type Ia supernova Supernova A supernova is a stellar explosion that is more energetic than a nova. It is pronounced with the plural supernovae or supernovas. Supernovae are extremely luminous and cause a burst of radiation that often briefly outshines an entire galaxy, before fading from view over several weeks or months... in the Andromeda Galaxy Andromeda Galaxy The Andromeda Galaxy is a spiral galaxy approximately 2.5 million light-years from Earth in the constellation Andromeda. It is also known as Messier 31, M31, or NGC 224, and is often referred to as the Great Andromeda Nebula in older texts. Andromeda is the nearest spiral galaxy to the... ,

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