// Workers AI · dad joke modeAre stars in Andromeda list-worthy? They're stellar.

This is the list of notable stars in the constellation Andromeda, sorted by decreasing brightness.

Name	B	F	Var	HD	HIP	RA	Dec	vis. mag.	abs. mag.	Dist. (ly)	Sp. class	Notes
Alpheratz	α, (δ)^[a]	21		358	677	00^h 08^m 23.17^s	+29° 05′ 27.0″	2.07	−0.30	97	B9p	Alpheratz, Sirrah; α² CVn variable, ΔV = 0.04^m, P = 0.966222 d; spectroscopic binary, also δ Peg
Mirach	β	43		6860	5447	01^h 09^m 43.80^s	+35° 37′ 15.0″	2.07	−1.86	199	M0IIIvar	Mirach; variable, has a planet or brown dwarf (b)
γ¹ And	γ¹	57		12533	9640	02^h 03^m 53.92^s	+42° 19′ 47.5″	2.10	−3.08	355	K3IIb	Almach; quadruple star system
δ And	δ	31		3627	3092	00^h 39^m 19.60^s	+30° 51′ 40.4″	3.27	0.81	101	K3III...	spectroscopic binary; suspected variable
51 And	(υ)^[b]^[c]	51		9927	7607	01^h 37^m 59.50^s	+48° 37′ 42.6″	3.59	−0.04	174	K3III	Nembus; multiple star
ο And	ο	1		217675	113726	23^h 01^m 55.25^s	+42° 19′ 33.5″	3.62	−3.01	692	B6pv SB	Alfarasalkamil^[1] quadruple star system; γ Cas variable, V_max = 3.55^m, V_min = 3.78^m
λ And	λ	16		222107	116584	23^h 37^m 33.71^s	+46° 27′ 33.0″	3.81	1.75	84	G8III-IV	Udkadua,^[1] RS CVn variable, V_max = 3.65^m, V_min = 4.05^m, P = 53.95 d
μ And	μ	37		5448	4436	00^h 56^m 45.10^s	+38° 29′ 57.3″	3.86	0.75	136	A5V	multiple star
ζ And	ζ	34		4502	3693	00^h 47^m 20.39^s	+24° 16′ 02.6″	4.08	0.35	181	K1II	Shimu,^[1] β Lyr/RS CVn variable, V_max = 3.92^m, V_min = 4.14^m, P = 17.7696 d
υ And	υ^[d]^[e]	50		9826	7513	01^h 36^m 47.98^s	+41° 24′ 23.0″	4.10	3.45	44	F8V	Titawin,^[2] has four planets (b, c, d & e)
κ And	κ	19		222439	116805	23^h 40^m 24.44^s	+44° 20′ 02.3″	4.15	0.57	170	B9IVn	Kaffalmusalsala,^[1] triple star, has a planet (b)
φ And	φ	42		6811	5434	01^h 09^m 30.12^s	+47° 14′ 30.6″	4.26	−2.51	736	B7III	Junnanmen,^[1] emission-line star
ι And	ι	17		222173	116631	23^h 38^m 08.18^s	+43° 16′ 05.1″	4.29	−1.65	502	B8V	Rasalnaqa,^[1] Keff al Salsalat, Manus Catenata^[3]
π And	π	29		3369	2912	00^h 36^m 52.84^s	+33° 43′ 09.7″	4.34	−2.18	656	B5V	spectroscopic binary; suspected variable
ε And	ε	30		3546	3031	00^h 38^m 33.50^s	+29° 18′ 44.5″	4.34	0.77	169	G5III...
η And	η	38		5516	4463	00^h 57^m 12.43^s	+23° 25′ 03.9″	4.40	0.04	243	G8III-IV	Kui,^[1] spectroscopic binary
σ And	σ	25		1404	1473	00^h 18^m 19.71^s	+36° 47′ 07.2″	4.51	1.33	141	A2V	suspected variable
ν And	ν	35		4727	3881	00^h 49^m 48.83^s	+41° 04′ 44.2″	4.53	−2.06	679	B5V SB	spectroscopic binary
7 And		7		219080	114570	23^h 12^m 32.92^s	+49° 24′ 21.5″	4.53	2.58	80	F0V	Honores^[1]
θ And	θ	24		1280	1366	00^h 17^m 05.54^s	+38° 40′ 54.0″	4.61	0.16	253	A2V	suspected variable
3 And		3		218031	113919	23^h 04^m 10.83^s	+50° 03′ 06.1″	4.64	0.94	179	K0III
65 And		65		14872	11313	02^h 25^m 37.40^s	+50° 16′ 43.2″	4.73	−0.39	345	K4III	triple star
58 And		58		13041	9977	02^h 08^m 29.15^s	+37° 51′ 33.1″	4.78	0.86	198	A5IV-V
8 And		8		219734	115022	23^h 17^m 44.62^s	+49° 00′ 55.0″	4.82	−1.69	655	M2III	suspected variable
ω And	ω^[f]	48		8799	6813	01^h 27^m 39.09^s	+45° 24′ 25.0″	4.83	2.57	92	F5IV
γ² And	γ²	57		12534		02^h 03^m 54.70^s	+42° 19′ 51.0″	4.84	-0.3	350	B8V	component of the γ And system; triple star system
60 And	b	60		13520	10340	02^h 13^m 13.34^s	+44° 13′ 54.1″	4.84	−1.32	556	K4III	suspected variable
ξ And	ξ^[f]	46		8207	6411	01^h 22^m 20.39^s	+45° 31′ 43.5″	4.87	0.98	195	K0III-IV	Adhil
τ And	τ	53		10205	7818	01^h 40^m 34.80^s	+40° 34′ 37.6″	4.96	−1.64	681	B8III	suspected variable
41 H. And	υ^[g]			10307	7918	01^h 41^m 46.52^s	+42° 36′ 49.7″	4.96	4.45	41	G2V	spectroscopic binary
ψ And	ψ	20		223047	117221	23^h 46^m 02.04^s	+46° 25′ 13.0″	4.97	−3.05	1309	G5Ib	multiple star
22 And		22		571	841	00^h 10^m 19.24^s	+46° 04′ 20.2″	5.01	−2.44	1006	F2II
χ And	χ^[h]	52		10072	7719	01^h 39^m 21.02^s	+44° 23′ 10.1″	5.01	0.66	242	G8III...
41 And	(d)^[i]	41		6658	5317	01^h 08^m 00.72^s	+43° 56′ 32.1″	5.04	1.14	196	A3m
2 And		2		217782	113788	23^h 02^m 36.34^s	+42° 45′ 28.1″	5.09	−0.06	349	A3Vn	multiple star
V428 And			V428	3346	2900	00^h 36^m 46.47^s	+44° 29′ 18.6″	5.14	−1.38	656	K5III	semiregular variable, ΔV = 0.06^m, P = 11.5 d; has a possible planetary system
ρ And	ρ	27		1671	1686	00^h 21^m 07.23^s	+37° 58′ 07.3″	5.16	1.71	160	F5III
HD 2421				2421	2225	00^h 28^m 13.59^s	+44° 23′ 40.2″	5.18	0.63	265	A2Vs	spectroscopic binary
64 And		64		14770	11220	02^h 24^m 24.89^s	+50° 00′ 23.9″	5.19	−0.11	375	G8III
GN And		28	GN	2628	2355	00^h 30^m 07.34^s	+29° 45′ 06.1″	5.20	1.43	185	A7III	low-amplitude δ Sct variable, ΔV = 0.05^m, P = 0.0693041 d
14 And		14		221345	116076	23^h 31^m 17.20^s	+39° 14′ 11.0″	5.22	0.80	249	K0III	Veritate,^[2] suspected variable; has a planet (b)
49 And	A^[j]	49		9057	6999	01^h 30^m 06.10^s	+47° 00′ 26.6″	5.27	0.53	290	K0III
32 And		32		3817	3231	00^h 41^m 07.20^s	+39° 27′ 31.2″	5.30	0.18	344	G8III
4 And		4		218452	114200	23^h 07^m 39.28^s	+46° 23′ 14.3″	5.30	0.20	342	K5III	double star
6 Per	(h)^[k]	(6)^[4]		13530	10366	02^h 13^m 36.02^s	+51° 03′ 58.4″	5.31	1.38	199	G8III:var	spectroscopic binary; suspected variable
62 And	c	62		14212	10819	02^h 19^m 16.85^s	+47° 22′ 48.0″	5.31	0.84	255	A1V
18 And		18		222304	116709	23^h 39^m 08.35^s	+50° 28′ 18.3″	5.35	−0.04	390	B9V
55 And		55		11428	8814	01^h 53^m 17.35^s	+40° 43′ 47.3″	5.42	−0.67	540	K1III	double star
11 And		11		219945	115152	23^h 19^m 29.79^s	+48° 37′ 30.7″	5.44	0.43	328	K0III
				3421	2942	00^h 37^m 21.23^s	+35° 23′ 58.2″	5.45	−2.03	1022	G5III
36 And		36		5286	4288	00^h 54^m 58.02^s	+23° 37′ 42.4″	5.46	2.51	127	K1IV	suspected variable
V340 And		15	V340	221756	116354	23^h 34^m 37.55^s	+40° 14′ 11.6″	5.55	1.28	233	A1III	low-amplitude δ Sct variable, ΔV = 0.007^m
PZ And		63	PZ	14392	10944	02^h 20^m 58.17^s	+50° 09′ 05.5″	5.57	0.38	356	B9p Si	α² CVn variable, ΔV = 0.05^m, P = 4.189 d
47 And		47		8374	6514	01^h 23^m 40.56^s	+37° 42′ 54.0″	5.60	1.54	211	A1m
				10204	7825	01^h 40^m 39.56^s	+43° 17′ 51.9″	5.63	1.05	268	A9IV:
44 And		44		6920	5493	01^h 10^m 18.85^s	+42° 04′ 53.7″	5.67	2.06	172	F8V
5 And		5		218470	114210	23^h 07^m 45.25^s	+49° 17′ 43.6″	5.68	3.02	111	F5V
HD 5788				5788	4675	01^h 00^m 03.55^s	+44° 42′ 47.9″	5.69	0.14	420	A2Vn	binary star with HD 5789
56 And		56		11749	9021	01^h 56^m 09.23^s	+37° 15′ 06.5″	5.69	0.73	320	G8III...	multiple star
23 And		23		905	1086	00^h 13^m 30.94^s	+41° 02′ 08.6″	5.71	2.99	114	F0IV
HD 16028				16028	12072	02^h 35^m 38.74^s	+37° 18′ 44.2″	5.72	−0.86	676	K4III	triple star
V388 And		13	V388	220885	115755	23^h 27^m 07.33^s	+42° 54′ 43.1″	5.75	0.97	294	B9III	α² CVn variable, V_max = 5.73^m, V_min = 5.77^m, P = 1.47931 d
12 And		12		220117	115280	23^h 20^m 53.17^s	+38° 10′ 56.9″	5.77	2.63	138	F5V	triple star
				1632	1657	00^h 20^m 45.54^s	+32° 54′ 40.4″	5.79	−0.69	646	K5III
45 And		45		7019	5550	01^h 11^m 10.29^s	+37° 43′ 26.9″	5.80	−1.44	916	B7III-IV	double star
HD 14622				14622	11090	02^h 22^m 50.36^s	+41° 23′ 47.5″	5.81	2.44	154	F0III-IV	has two optical companions
10 And		10		219981	115191	23^h 19^m 52.38^s	+42° 04′ 40.9″	5.81	−0.30	542	M0III
HD 222109				222109	116582	23^h 37^m 32.03^s	+44° 25′ 44.5″	5.81	−1.20	823	B8V	double star
HD 224635				224635	118281	23^h 59^m 29.33^s	+33° 43′ 26.9″	5.81	3.50	95	F8	multiple star
OU And			OU	223460	117503	23^h 49^m 40.96^s	+36° 25′ 31.4″	5.86	0.21	440	G1IIIe	FK Com variable, ΔV = 0.07^m, P = 24.2 d
				1439	1493	00^h 18^m 38.22^s	+31° 31′ 02.0″	5.88	−0.23	543	A0IV
HD 2767				2767	2475	00^h 31^m 25.61^s	+33° 34′ 54.1″	5.88	0.10	467	K1III...	binary star
HD 1606				1606	1630	00^h 20^m 24.39^s	+30° 56′ 08.2″	5.89	−0.37	582	B7V	suspected variable
				11727	9001	01^h 55^m 54.47^s	+37° 16′ 40.1″	5.89	−1.52	991	K5III	optical component of 56 And
KK And			KK	9531	7321	01^h 34^m 16.60^s	+37° 14′ 13.9″	5.90	0.50	392	B8Vp(Si)	α² CVn variable, ΔV = 0.012^m, P = 0.6684 d
				16176	12181	02^h 36^m 57.08^s	+38° 44′ 02.3″	5.91	2.24	177	F5V
6 And		6		218804	114430	23^h 10^m 27.36^s	+43° 32′ 41.1″	5.91	3.65	112	F5V	Astrometric binary
				10975	8423	01^h 48^m 38.84^s	+37° 57′ 10.6″	5.94	1.06	308	K0III
39 And		39		6116	4903	01^h 02^m 54.28^s	+41° 20′ 42.7″	5.95	0.84	344	A5m	double star
				8671	6711	01^h 26^m 18.60^s	+43° 27′ 28.4″	5.98	2.90	135	F7V
AN And		9	AN	219815	115065	23^h 18^m 23.33^s	+41° 46′ 25.3″	5.98	0.17	472	A7m	β Lyr variable, V_max = 5.96^m, V_min = 6.11^m, P = 3.21952 d
HD 5608				5608	4552	00^h 58^m 14.19^s	+33° 57′ 03.8″	5.99	2.17	190	K0	has a planet (b)
				224165	117956	23^h 55^m 33.48^s	+47° 21′ 21.0″	6.01	−2.46	1614	G8Ib
				224342	118071	23^h 57^m 03.63^s	+42° 39′ 29.7″	6.01	−2.22	1442	F8III
				4335	3604	00^h 46^m 10.80^s	+44° 51′ 41.4″	6.03	0.32	452	B9.5IIIMNp.
				13594	10403	02^h 14^m 02.53^s	+47° 29′ 03.8″	6.05	2.96	135	F5V
HD 3883				3883	3269	00^h 41^m 35.98^s	+24° 37′ 44.6″	6.06	0.30	462	A7m	suspected variable
V439 And			V439	166	544	00^h 06^m 36.53^s	+29° 01′ 19.0″	6.07	5.39	45	K0V	BY Draconis variable, ΔV = 0.04^m, P = 6.23 d
				5118	4185	00^h 53^m 28.22^s	+37° 25′ 05.9″	6.07	0.77	374	K3III:
				221293	116030	23^h 30^m 39.54^s	+38° 39′ 44.0″	6.07	−0.33	621	G9III
HD 223229				223229	117340	23^h 47^m 33.05^s	+46° 49′ 57.3″	6.08	−1.96	1320	B3IV	suspected variable
				225239	394	00^h 04^m 53.21^s	+34° 39′ 34.4″	6.09	3.26	120	G2V
59 And A		59		13294	10176	02^h 10^m 52.83^s	+39° 02′ 22.5″	6.09	1.56	263	B9V	binary star
26 And		26		1438	1501	00^h 18^m 42.15^s	+43° 47′ 28.1″	6.10	−0.53	692	B8V	double star
				5526	4501	00^h 57^m 39.64^s	+45° 50′ 21.8″	6.10	0.45	439	K2III
HD 225218				225218	365	00^h 04^m 36.60^s	+42° 05′ 33.2″	6.11	−2.45	1680	B9III	double star
				7647	5993	01^h 17^m 05.05^s	+44° 54′ 07.5″	6.11	−0.18	590	K5
HD 1185				1185	1302	00^h 16^m 21.50^s	+43° 35′ 42.4″	6.12	1.28	303	A2V	double star
				218416	114162	23^h 07^m 10.05^s	+52° 48′ 59.6″	6.12	0.55	423	K0III
GO And			GO	4778	3919	00^h 50^m 18.21^s	+45° 00′ 08.1″	6.13	1.34	296	A0p...	α² CVn variable, ΔV = 0.04^m, P = 2.5481 d
				7158	5650	01^h 12^m 34.06^s	+45° 20′ 14.9″	6.13	−0.52	698	M1III
66 And		66		15138	11465	02^h 27^m 51.75^s	+50° 34′ 12.7″	6.16	2.54	173	F4V	spectroscopic binary
				14372	10924	02^h 20^m 41.50^s	+47° 18′ 39.0″	6.17	−0.87	836	B5V
				743	967	00^h 11^m 59.03^s	+48° 09′ 08.5″	6.18	0.05	550	K4III
				3411	2926	00^h 37^m 07.20^s	+24° 00′ 51.3″	6.18	1.13	334	K2III
HD 221776				221776	116365	23^h 34^m 46.73^s	+38° 01′ 26.3″	6.18	−0.41	678	K5	double star
				16327	12287	02^h 38^m 17.86^s	+37° 43′ 36.6″	6.19	1.60	270	F6III	triple star
HD 221246				221246	115996	23^h 30^m 07.39^s	+49° 07′ 59.3″	6.19	−0.91	856	K5III	member of the NGC 7686 star cluster
OP And			OP	9746	7493	01^h 36^m 27.21^s	+48° 43′ 22.2″	6.20	0.65	420	K1III:	BY Dra variable, ΔV = 0.09^m
				400	699	00^h 08^m 41.02^s	+36° 37′ 38.7″	6.21	3.61	108	F8IV
				14213	10814	02^h 19^m 10.84^s	+46° 28′ 20.2″	6.21	0.50	452	A4V
				952	1123	00^h 14^m 02.29^s	+33° 12′ 21.9″	6.22	1.45	293	A1V
HD 895				895	1076	00^h 13^m 23.93^s	+26° 59′ 15.4″	6.24	0.78	403	G0III	triple star
				222451	116824	23^h 40^m 40.47^s	+36° 43′ 14.6″	6.24	3.01	144	F1V
				224906	137	00^h 01^m 43.85^s	+42° 22′ 01.7″	6.25	−1.80	1331	B9IIIp Mn
				11613	8922	01^h 54^m 53.75^s	+40° 42′ 07.9″	6.25	1.13	345	K2
HD 220105				220105	115261	23^h 20^m 44.11^s	+44° 06′ 58.5″	6.25	1.73	261	A5Vn	double star
				221661	116292	23^h 33^m 42.99^s	+45° 03′ 29.1″	6.25	0.12	548	G8II
HD 2942				2942	2583	00^h 32^m 49.09^s	+28° 16′ 48.8″	6.26	0.47	469	G8II	triple star
				8774	6776	01^h 27^m 06.21^s	+34° 22′ 39.3″	6.27	3.12	139	F7IVsvar
				2507	2270	00^h 28^m 56.67^s	+36° 53′ 58.9″	6.28	0.51	464	G5III
				8375	6512	01^h 23^m 37.31^s	+34° 14′ 44.2″	6.28	2.43	192	G8IV
				11624	8930	01^h 54^m 57.63^s	+37° 07′ 42.0″	6.28	0.25	525	K0
				7758	6087	01^h 18^m 10.14^s	+47° 25′ 11.0″	6.29	−2.07	1531	K0
				16350	12305	02^h 38^m 27.94^s	+38° 05′ 21.0″	6.29	−0.47	734	B9.5V
				219962	115171	23^h 19^m 41.37^s	+48° 22′ 51.1″	6.29	0.47	475	K1III
				217314	113501	22^h 59^m 10.37^s	+52° 39′ 16.0″	6.31	−0.26	672	K2
				10597	8127	01^h 44^m 26.53^s	+46° 08′ 23.2″	6.32	0.23	540	K5III
				219290	114714	23^h 14^m 14.34^s	+50° 37′ 04.5″	6.32	0.82	411	A0V
				10486	8044	01^h 43^m 16.39^s	+45° 19′ 21.5″	6.33	2.61	181	K2IV
				10874	8370	01^h 47^m 48.00^s	+46° 13′ 47.6″	6.33	2.50	190	F6V
				1075	1208	00^h 15^m 06.93^s	+31° 32′ 08.7″	6.34	−1.70	1320	K5
HD 8673				8673	6702	01^h 26^m 08.62^s	+34° 34′ 47.7″	6.34	3.43	125	F7V	has a planet (b)
				1083	1215	00^h 15^m 10.55^s	+27° 17′ 00.5″	6.35	0.84	412	A1Vn	double star
				1527	1575	00^h 19^m 41.58^s	+40° 43′ 46.2″	6.35	0.25	541	K1III
				221970	116505	23^h 36^m 30.52^s	+32° 54′ 15.1″	6.35	1.92	251	F6V
CG And			CG	224801	63	00^h 00^m 43.62^s	+45° 15′ 12.0″	6.36	−0.23	678	B9p SiEu	α² CVn variable, V_max = 6.32^m, V_min = 6.42^m, P = 3.73975 d
HD 16004				16004	12057	02^h 35^m 27.89^s	+39° 39′ 52.1″	6.36	0.11	580	B9MNp...	triple star
				13818	10562	02^h 15^m 57.69^s	+47° 48′ 43.4″	6.37	0.61	462	G9III-IV
LN And			LN	217811	113802	23^h 02^m 45.15^s	+44° 03′ 31.6″	6.37	−1.42	1177	B2V	double star; not variable despite designation
V385 And			V385	220524	115530	23^h 24^m 08.88^s	+41° 36′ 46.3″	6.37	−1.55	1249	M0	irregular variable, V_max = 6.36^m, V_min = 6.47^m
GY And			GY	9996	7651	01^h 38^m 31.84^s	+45° 23′ 58.9″	6.38	0.66	455	B9Vp (Cr-Eu)	Promethium lines; α² CVn variable, V_max = 6.27^m, V_min = 6.44^m, P = 8000 d
				13013	9983	02^h 08^m 33.55^s	+44° 27′ 34.4″	6.38	0.78	430	G8III
				218365	114152	23^h 07^m 04.99^s	+35° 38′ 11.3″	6.38	−0.08	638	K0
				9712	7444	01^h 35^m 52.46^s	+41° 04′ 35.1″	6.39	1.01	388	K1III
V529 And			V529	8801	6794	01^h 27^m 26.67^s	+41° 06′ 04.0″	6.42	2.69	182	Am...	δ Scuti variable, ΔV = 0.03^m, P = 0.40331 d
				217731	113750	23^h 02^m 11.32^s	+44° 34′ 22.4″	6.43	1.22	359	K0
HD 222641				222641	116941	23^h 42^m 14.68^s	+44° 59′ 30.3″	6.43	−0.48	786	K5III	suspected variable
HD 7853				7853	6140	01^h 18^m 47.02^s	+37° 23′ 10.7″	6.44	0.71	456	A5m	double star
				14221	10830	02^h 19^m 22.77^s	+48° 57′ 19.0″	6.44	2.39	210	F4V
				219668	114981	23^h 17^m 16.59^s	+45° 09′ 51.5″	6.44	2.10	241	K0IV
HD 6114				6114	4911	01^h 03^m 01.47^s	+47° 22′ 34.3″	6.46	1.39	337	A9V	double star
				11884	9163	01^h 57^m 59.23^s	+47° 05′ 43.9″	6.48	−1.24	1140	K0
ET And			ET	219749	115036	23^h 17^m 55.99^s	+45° 29′ 20.2″	6.48	0.36	545	B9Vp(Si)	α² CVn variable, ΔV = 0.03^m, P = 1.61888 d
HD 222399				222399	116781	23^h 40^m 02.82^s	+37° 39′ 10.2″	6.49	1.74	291	F2IV	double star
PY And			PY	3322	2865	00^h 36^m 20.00^s	+27° 15′ 17″	6.50	-0.16	701	B8IIImnp...	α² CVn variable, ΔV = ~0.03^m
				800	1009	00^h 12^m 34.08^s	+44° 42′ 26.1″	6.50	0.50	517	K0
59 And B		59		13295	10180	02^h 10^m 53.67^s	+39° 02′ 36.0″	6.82	−1.76	1698	A1Vn	component of the 59 And system
HD 222155				222155	116616	23^h 38^m 00^s	+48° 59′ 47″	7.1	3.65	160	G2V	has a planet (b)
HD 16175				16175	12191	02^h 37^m 01.91^s	+42° 03′ 45.5″	7.28	3.40	195	G0	Buna; has a planet (b)
R And			R	1967	1901	00^h 24^m 01.95^s	+38° 34′ 37.3″	7.39	-5.19	790	S6.5IIIeZr6Ti2	Mira variable, V_max = 5.8^m, V_min = 15.2^m, P = 409.2 d
HD 1605				1605	1640	00^h 20^m 32.0^s	+30° 58′ 29″	7.52	2.88	276	K1IV	has two planets (b & c)
HD 13931				13931	10626	02^h 16^m 47.38^s	+43° 46′ 22.8″	7.52	4.3	144	G0	has a planet (b)
HD 5583				5583		00^h 57^m 57.0^s	+34° 59′ 08″	7.6	0.88	721	K0	has a planet (b)
RW And			RW	4489		00^h 47^m 18.92^s	+32° 41′ 08.6″	7.9	-0.52	1375	M5e-M10e(S6,2e)	Mira variable, V_max = 7.9^m, V_min = 15.7^m, P = 430 d
Groombridge 34				1326	1475	00^h 18^m 22.9^s	+44° 01′ 22″	8.01	10.25	11.62	M6Ve + M1Ve	16th closest star system, binary; both components GQ and GX And flare stars
HD 15082				15082	11397	02^h 26^m 51.06^s	+37° 33′ 01.7″	8.3	3.0	377	A5	has a transiting planet WASP-33b
RU And			RU			01^h 38^m 37^s	38° 40′ 12″	9.9			M5e-M6e	a variable star in the constellation of Andromeda. It is classified as a semiregular variable pulsating giant star, and varies from an apparent visual magnitude of 14.5 at minimum brightness to a magnitude of 9.9 at maximum brightness, with a period of approximately 238.3 days.^[5]^[6]
Y And				10112		01^h 39^m 36.89^s	+39° 20′ 35″	10.39		8,000	M3-4.5e	Mira Cet variable
Z And			Z	221650	116287	23^h 33^m 39.95^s	+48° 49′ 05.9″	10.53	2.38	1393	M2III + B1eq	prototype of Z And variables, V_max = 7.7^m, V_min = 11.3^m
HAT-P-6						23^h 39^m 05.81^s	+42° 27′ 57.5″	10.54	4.03	650	F	Sterrennacht; has a transiting planet (b)
HAT-P-16						00^h 38^m 17.56^s	+42° 27′ 47.2″	10.8	3.9	766	F8	has a transiting planet (b)
HAT-P-32						02^h 01^m 10^s	+46° 41′ 16″	11.29	3.76	1044	F/G	has a transiting planet (b)
WASP-1						00^h 20^m 40.08^s	+31° 59′ 23.8″	11.79	3.89	1239	F7V	has a transiting planet (b)
Ross 248						23^h 41^m 54.99^s	+44° 10′ 40.8″	12.29	14.79	10.32	M6e	HH And; 8th closest star system, flare star
HAT-P-19						00^h 38^m 04^s	+34° 42′ 42″	12.9	6.24	701	K	has a transiting planet (b)
HAT-P-28						00^h 52^m 00^s	+34° 43′ 42″	13.03	5.05	1288	G3	has a transiting planet (b)
HAT-P-53						01^h 27^m 29.0^s	+38° 58′ 05″	13.73	4.45	2345		has a transiting planet (b)
S And			S			00^h 42^m 43.11^s	+41° 16′ 04.2″			2600000	Ia	SN 1885A; BD+40°147a; type Ia supernova in the Andromeda Galaxy, V_max = 5.8^m, V_min = < 16^m
Table legend: • Name = Proper name • B = Bayer designation • F or/and G. = Flamsteed designation or Gould designation • Var = Variable-star designation • HD = Henry Draper Catalogue designation number • HIP = Hipparcos Catalogue designation number • RA = Right ascension for the Epoch/Equinox J2000.0 • Dec = Declination for the Epoch/Equinox J2000.0 • vis. mag. = visual magnitude (m or m_v), also known as apparent magnitude • abs. mag. = absolute magnitude (M_v) • Dist. (ly) = Distance in light-years from Earth • Sp. class = Spectral class of the star in the stellar classification system • Notes = Common name(s) or alternate name(s); comments; notable properties [for example: multiple star status, range of variability if it is a variable star, exoplanets, etc.]

Notes

↑ Also designated Delta Pegasi (δ Peg) by Bayer
↑ Bayer designated it as υ Per.
↑ Bode lettered it as 2.υ, in his "Verzeichniss".
↑ Flamsteed lettered it as υ.^{[citation needed]}
↑ Bode lettered it as 1.υ in his "Verzeichniss".^{[citation needed]}
1 2 Flamsteed unlettered it in his catalogue and atlas.^{[citation needed]}
↑ Bayer originally lettered it as υ.^{[citation needed]}
↑ Flamsteed lettered it as λ.^{[citation needed]}
↑ Flamsteed lettered it as d.^{[citation needed]}
↑ Flamsteed lettered it as ξ.^{[citation needed]}
↑ Flamsteed lettered it as h Per.^{[citation needed]}

References

1 2 3 4 5 6 7 8 IAU-Catalog of Star Names
1 2 Final Results of NameExoWorlds Public Vote Released
↑ E.B Knobel – On a catalogue of stars in the Calendarium of Al Achsasi Al Mouakket
↑ Persei, on the constellation boundary between Andromeda with Perseus
↑ RU And, database entry, Combined General Catalog of Variable Stars (GCVS4.2, 2004 Ed.), N. N. Samus, O. V. Durlevich, et al., CDS ID II/250 Accessed on line 2009-06-30.
↑ V* RU And -- Semiregular Pulsating Variable Star, database entry, SIMBAD. Accessed on line 2009-06-30.

Bayer J. (1603). Uranometria. Augsburg: Christophorus Mangus.
Bevis J. (c. 1750). Uranographia Britannica.
Bode J. E. (1782). Vorstellung der Gestirne. Berlin / Stralsund: Gottlieb August Lange.
Fortin J. (1776). Atlas Celeste de Flamsteed (2^eme ed.). Paris.
ESA (1997). "The Hipparcos and Tycho Catalogues". Retrieved 26 December 2006.
Kostjuk, N. D. (2002). "HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index". Retrieved 26 December 2006.
Roman, N. G. (1987). "Identification of a Constellation from a Position". Retrieved 26 December 2006.
"SIMBAD Astronomical Database". Centre de Données astronomiques de Strasbourg. Retrieved 4 January 2007.
Samus, N. N.; Durlevich, O. V.; et al. (2004). "Combined General Catalogue of Variable Stars (GCVS4.2)". Retrieved 28 March 2012.
Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS database, version 2012Feb)". Retrieved 28 March 2012.
Wagman, Morton (2003). Lost Stars: Lost, Missing and Troublesome Stars from the Catalogues of Johannes Bayer, Nicholas Louis de Lacaille, John Flamsteed, and Sundry Others. Blacksburg, Virginia: The McDonald & Woodward Publishing Company. pp. 23–24. Bibcode:2003lslm.book.....W. ISBN 978-0-939923-78-6.
Werner, Helmut; Schmeidler, Felix (1986). Synopsis der Nomenklatur der Fixsterne. Stuttgart: Wissenschaftliche Verlagsgesellschaft mbH. pp. 50–53. ISBN 978-3-8047-0739-9.

[1] Also designated Delta Pegasi (δ Peg) by Bayer

[2] Bayer designated it as υ Per.

[3] Bode lettered it as 2.υ, in his "Verzeichniss".

[5] Flamsteed lettered it as υ.^{[citation needed]}

[6] Bode lettered it as 1.υ in his "Verzeichniss".^{[citation needed]}

[flamerror-9] 1 2 Flamsteed unlettered it in his catalogue and atlas.^{[citation needed]}

[10] Bayer originally lettered it as υ.^{[citation needed]}

[11] Flamsteed lettered it as λ.^{[citation needed]}

[12] Flamsteed lettered it as d.^{[citation needed]}

[13] Flamsteed lettered it as ξ.^{[citation needed]}

[14] Flamsteed lettered it as h Per.^{[citation needed]}

[exopla.net-4] 1 2 3 4 5 6 7 8 IAU-Catalog of Star Names

[NameExoWorlds-7] 1 2 Final Results of NameExoWorlds Public Vote Released

[8] E.B Knobel – On a catalogue of stars in the Calendarium of Al Achsasi Al Mouakket

[15] Persei, on the constellation boundary between Andromeda with Perseus

[gcvs-16] RU And, database entry, Combined General Catalog of Variable Stars (GCVS4.2, 2004 Ed.), N. N. Samus, O. V. Durlevich, et al., CDS ID II/250 Accessed on line 2009-06-30.

[17] V* RU And -- Semiregular Pulsating Variable Star, database entry, SIMBAD. Accessed on line 2009-06-30.

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This page was redesigned at the edge.

A page that knows where it met you.

// Workers AI · dad joke modeAre stars in Andromeda list-worthy? They're stellar.

See also

References