List of stars in Cancer

This is the list of notable stars in the constellation Cancer. The 121 stars are sorted by decreasing brightness, beginning with Beta Cancri, the brightest star in Cancer.

Name	B	F	Var	HD	HIP	RA	Dec	vis. mag.	abs. mag.	Dist. (ly)	Sp. class	Notes
β Cnc	β	17		69267	40526	08^h 16^m 30.95^s	+09° 11′ 08.4″	3.53	−1.22	290	K4III	Tarf, Al Tarf; variable star, ΔV = 0.005^m, P = 6.01 d, has a planet (b)
δ Cnc	δ	47		74442	42911	08^h 44^m 41.11^s	+18° 09′ 17.5″	3.94	0.84	136	K0III	Asellus Australis
ι Cnc A	ι	48		74739	43103	08^h 46^m 41.83^s	+28° 45′ 36.0″	4.03	−0.77	298	G8Iab:	component of the ι Cnc system
α Cnc	α	65		76756	44066	08^h 58^m 29.20^s	+11° 51′ 28.0″	4.26	0.63	173	A5m	Acubens, Sertan; suspected variable, Vmax = 4.20^m, Vmin = 4.27^m
γ Cnc	γ	43		74198	42806	08^h 43^m 17.21^s	+21° 28′ 06.9″	4.66	1.23	181	A1IV	Asellus Borealis
ζ Cnc	ζ	16		68255 68256 68257	40167	08^h 12^m 12.71^s	+17° 38′ 53.3″	4.67	2.63	83	F7V+F9V +G0V+?	Tegmine, quaternary star
HD 71115				71115	41325	08^h 25^m 54.79^s	+07° 33′ 52.3″	5.13	−0.08	359	G8II	double star
8 Cnc		8		66664	39567	08^h 05^m 04.51^s	+13° 07′ 06.1″	5.14	1.09	210	A1V
χ Cnc	χ	18		69897	40843	08^h 20^m 03.87^s	+27° 13′ 07.0″	5.14	3.84	59	F6V	suspected variable
ξ Cnc	ξ	77		78515	44946	09^h 09^m 21.53^s	+22° 02′ 43.6″	5.16	−0.18	380	K0III	Nahn
ο^1 Cnc	ο^1	62		76543	43970	08^h 57^m 14.91^s	+15° 19′ 21.8″	5.22	1.77	160	A5III	α^2 CVn variable
ρ^2 Cnc	ρ^2	58		76219	43834	08^h 55^m 39.69^s	+27° 55′ 39.2″	5.23	−1.00	574	G8II-III
σ^3 Cnc	σ^3	64		76813	44154	08^h 59^m 32.68^s	+32° 25′ 07.1″	5.23	0.27	320	G9III	suspected variable
κ Cnc	κ	76		78316	44798	09^h 07^m 44.82^s	+10° 40′ 05.6″	5.23	−0.63	484	B8IIImnp	α^2 CVn variable, Vmax = 5.22^m, Vmin = 5.27^m, P = 5.0035 d
μ^2 Cnc	μ^2	10		67228	39780	08^h 07^m 45.84^s	+21° 34′ 55.1″	5.30	3.46	76	G2IV
θ Cnc	θ	31		72094	41822	08^h 31^m 35.77^s	+18° 05′ 40.4″	5.33	−0.57	494	K5III	suspected variable
η Cnc	η	33		72292	41909	08^h 32^m 42.52^s	+20° 26′ 28.6″	5.33	0.43	312	K3III
82 Cnc	π^2	82		79554	45410	09^h 15^m 13.88^s	+14° 56′ 29.5″	5.36	−1.30	701	K1III
57 Cnc		57		75959	43721	08^h 54^m 14.70^s	+30° 34′ 45.0″	5.40	0.15	365	G7III
τ Cnc	τ	72		78235	44818	09^h 08^m 00.07^s	+29° 39′ 15.2″	5.42	0.91	260	G8III
60 Cnc		60		76351	43851	08^h 55^m 55.56^s	+11° 37′ 33.8″	5.44	−0.82	582	K5III
σ^2 Cnc	σ^2	59		76398	43932	08^h 56^m 56.63^s	+32° 54′ 38.1″	5.44	1.56	195	A7IV
ν Cnc	ν	69		77350	44405	09^h 02^m 44.27^s	+24° 27′ 10.6″	5.45	−0.28	457	A0pSi	α^2 CVn variable, Vmax = 5.33^m, Vmin = 5.49^m, P = 4.20 d
27 Cnc		27	BP	71250	41400	08^h 26^m 43.95^s	+12° 39′ 17.5″	5.56	−1.98	1052	M3III	semiregular variable, Vmax = 5.41^m, Vmin = 5.75^m, P = 40 d
φ^1 Cnc	φ^1	22		71093	41377	08^h 26^m 27.73^s	+27° 53′ 37.9″	5.58	0.15	398	K5III
3 Cnc		3		65759	39177	08^h 00^m 47.31^s	+17° 18′ 31.4″	5.60	−1.12	721	K3III
15 Cnc		15	BM	68351	40240	08^h 13^m 08.87^s	+29° 39′ 23.7″	5.62	−1.52	872	B9p SiCr	α^2 CVn variable, Vmax = 5.53^m, Vmin = 5.65^m, P = 3.31 d
45 Cnc	A^1	45		74228	42795	08^h 43^m 12.34^s	+12° 40′ 51.1″	5.62	−1.87	1028	A3V+...	suspected variable
49 Cnc	b	49	BI	74521	42917	08^h 44^m 45.04^s	+10° 04′ 54.2″	5.63	0.15	408	A1p...	α^2 CVn variable, Vmax = 5.58^m, Vmin = 5.71^m, P = 6.91 d
σ^1 Cnc	σ^1	51		75698	43584	08^h 52^m 34.62^s	+32° 28′ 26.8″	5.67	1.69	204	A8Vms	suspected variable
ο^2 Cnc	ο^2	63		76582	44001	08^h 57^m 35.16^s	+15° 34′ 52.4″	5.68	2.22	161	F0IV
υ^1 Cnc	υ^1	30		72041	41816	08^h 31^m 30.57^s	+24° 04′ 52.4″	5.71	1.40	237	F0IIIn	suspected variable
ψ^2 Cnc	ψ^2	14		67767	40023	08^h 10^m 27.23^s	+25° 30′ 29.4″	5.73	2.61	137	G8IV	suspected variable
1 Cnc		1		64960	38848	07^h 56^m 59.47^s	+15° 47′ 25.4″	5.80	0.04	462	K3III
HD 69994				69994	40866	08^h 20^m 20.93^s	+20° 44′ 52.2″	5.80	−0.17	510	K1III
HD 77445				77445	44406	09^h 02^m 44.82^s	+07° 17′ 53.7″	5.85	−0.69	664	K3III:	suspected variable
ω^1 Cnc	ω^1	2		65714	39191	08^h 00^m 55.87^s	+25° 23′ 34.2″	5.87	−1.82	660	G8III:
50 Cnc	A^2	50		74873	43121	08^h 46^m 56.06^s	+12° 06′ 36.3″	5.89	1.96	199	A1V
66 Cnc		66		77104	44307	09^h 01^m 24.13^s	+32° 15′ 08.3″	5.89	−0.08	509	A2V
HD 72945				72945	42172	08^h 35^m 51.05^s	+06° 37′ 13.9″	5.91	3.79	87	F8V
λ Cnc	λ	19		70011	40881	08^h 20^m 32.15^s	+24° 01′ 20.5″	5.92	0.37	419	B9.5V	Piautos
36 Cnc	c	36		73143	42265	08^h 37^m 05.79^s	+09° 39′ 20.1″	5.92	0.17	461	A3V	suspected eclipsing binary
20 Cnc	d^1	20		70569	41117	08^h 23^m 21.87^s	+18° 19′ 56.2″	5.94	0.52	395	A9V
29 Cnc		29		71555	41578	08^h 28^m 37.35^s	+14° 12′ 39.1″	5.94	1.07	308	A5V
75 Cnc		75		78418	44892	09^h 08^m 47.42^s	+26° 37′ 48.0″	5.95	3.47	102	G5IV
1 LMi		(1)		73192	42365	08^h 38^m 19.00^s	+32° 48′ 07.3″	5.96	0.70	367	K2III:
55 Cnc	ρ^1	55		75732	43587	08^h 52^m 36.13^s	+28° 19′ 53.0″	5.96	5.47	41	G8V	Copernicus,[1] binary star; has five planets (b, c, d, e, f)
μ^1 Cnc	μ^1	9	BL	66875	39659	08^h 06^m 18.40^s	+22° 38′ 07.8″	5.97	−0.45	626	M3III	semiregular variable, Vmax = 5.97^m, Vmin = 6.04^m
5 Cnc		5		65873	39236	08^h 01^m 30.29^s	+16° 27′ 19.2″	5.99	0.19	472	B9.5Vn
HD 68461				68461	40231	08^h 12^m 59.74^s	+16° 30′ 51.7″	6.03	−0.02	528	G8III
HD 72617				72617	42049	08^h 34^m 13.35^s	+08° 27′ 08.5″	6.04	2.22	189	F3IV
79 Cnc		79		78715	45033	09^h 10^m 20.86^s	+21° 59′ 47.1″	6.04	0.49	420	G8III
RS Cnc			RS	78712	45058	09^h 10^m 38.81^s	+30° 57′ 47.6″	6.04	0.61	397	M6S	Technetium star; semiregular variable, Vmax = 5.33^m, Vmin = 6.94^m, P = 242.2 d
HD 65257				65257	38975	07^h 58^m 31.48^s	+16° 31′ 07.3″	6.05	−2.11	1399	K0	suspected variable
HD 65522				65522	39067	07^h 59^m 35.07^s	+13° 14′ 31.9″	6.05	1.22	301	K2
28 Cnc		28	CX	71496	41574	08^h 28^m 36.80^s	+24° 08′ 42.2″	6.05	1.45	271	F0Vn	δ Sct variable, ΔV = 0.025^m, P = 0.096 d
67 Cnc		67		77190	44342	09^h 01^m 48.88^s	+27° 54′ 10.0″	6.07	2.23	191	A8Vn	suspected variable
HD 68099				68099	40085	08^h 11^m 16.60^s	+09° 49′ 16.6″	6.08	−1.06	872	B6III
21 Cnc		21		70734	41163	08^h 23^m 55.21^s	+10° 37′ 55.6″	6.11	−1.56	1113	M2III	suspected variable
25 Cnc	d^2	25		71030	41319	08^h 25^m 49.99^s	+17° 02′ 47.9″	6.11	2.85	147	F6V
46 Cnc		46		74485	42954	08^h 45^m 21.42^s	+30° 41′ 51.9″	6.12	0.30	477	G5III
φ^2 Cnc A	φ^2	23		71150	41404	08^h 26^m 47.08^s	+26° 56′ 07.7″	6.14	1.50	276	A3V	component of the φ^2 Cnc system; suspected variable
HD 80546				80546	45896	09^h 21^m 27.17^s	+32° 54′ 07.9″	6.16	1.22	317	K3III
HD 76508				76508	43957	08^h 57^m 08.30^s	+17° 08′ 37.8″	6.17	0.82	384	K1III
φ^2 Cnc B	φ^2	23		71151		08^h 26^m 47.00^s	+26° 56′ 07.0″	6.19	1.55	276	A6V	component of the φ^2 Cnc system
HD 76629				76629	44010	08^h 57^m 42.03^s	+09° 23′ 16.0″	6.19	−1.15	956	G8III
HD 66552				66552	39535	08^h 04^m 45.32^s	+18° 50′ 31.4″	6.21	1.40	299	B9V
HD 66684				66684	39607	08^h 05^m 37.05^s	+27° 31′ 47.1″	6.21	−1.08	934	A0V	suspected variable, Vmax = 6.16^m, Vmin = 6.21^m
4 LMi		(4)		73596	42538	08^h 40^m 18.31^s	+31° 56′ 31.1″	6.21	1.05	350	F5III	suspected variable
HD 67959				67959	40058	08^h 10^m 58.90^s	+14° 37′ 46.3″	6.22	−0.04	581	A1V
12 Cnc		12		67483	39874	08^h 08^m 42.44^s	+13° 38′ 27.4″	6.25	1.59	278	F3V
53 Cnc		53	BO	75716	43575	08^h 52^m 28.60^s	+28° 15′ 33.0″	6.25	−0.92	886	M3III	slow irregular variable, Vmax = 5.9^m, Vmin = 6.37^m
61 Cnc		61		76572	44031	08^h 57^m 58.63^s	+30° 14′ 01.5″	6.25	2.75	164	F6V
HD 72505				72505	42010	08^h 33^m 45.06^s	+13° 15′ 26.7″	6.26	1.40	306	K0III
HD 69478				69478	40617	08^h 17^m 31.66^s	+08° 51′ 58.8″	6.28	−1.28	1062	G8III
ε Cnc	ε	41		73731	42556	08^h 40^m 27.03^s	+19° 32′ 41.4″	6.29	0.16	548	Am	Meleph, in Beehive Cluster
HD 65735				65735	39180	08^h 00^m 48.10^s	+19° 48′ 58.4″	6.30	1.18	345	K1III
FZ Cnc			FZ	76830	44126	08^h 59^m 10.76^s	+18° 08′ 06.1″	6.30	−0.35	697	M4IIIvar	semiregular variable
4 Cnc	ω^2	4		65856	39263	08^h 01^m 43.77^s	+25° 05′ 22.0″	6.32	0.00	598	A1V
HD 72943				72943	42187	08^h 36^m 07.71^s	+15° 18′ 49.3″	6.33	1.77	267	F0IV
HD 65757				65757	39194	08^h 01^m 00.79^s	+23° 34′ 59.4″	6.34	1.70	276	K1III-IV
υ^2 Cnc	υ^2	32		72324	41940	08^h 33^m 00.14^s	+24° 05′ 05.7″	6.35	0.80	421	G9III
54 Cnc		54		75528	43454	08^h 51^m 01.53^s	+15° 21′ 01.7″	6.36	3.35	130	G2IV
HD 68776				68776	40354	08^h 14^m 21.01^s	+13° 02′ 54.0″	6.39	−0.49	776	G8III
39 Cnc		39		73665	42516	08^h 40^m 06.44^s	+20° 00′ 28.1″	6.39	0.11	587	K0III	in Beehive Cluster; suspected variable
HD 78175				78175	44768	09^h 07^m 27.01^s	+22° 58′ 51.1″	6.39	2.54	192	F5V
X Cnc			X	76221	43811	08^h 55^m 22.88^s	+17° 13′ 52.5″	6.40	−3.95	3622	C6,4	semiregular variable, Vmax = 5.69^m, Vmin = 6.94^m, P = 180 d
HD 80064				80064	45614	09^h 17^m 51.36^s	+11° 30′ 04.1″	6.40	0.30	542	A2IV
HD 75469				75469	43427	08^h 50^m 45.13^s	+18° 49′ 56.1″	6.41	−0.43	762	A2Vs
HD 69629				69629	40675	08^h 18^m 14.43^s	+15° 40′ 40.6″	6.42	0.56	485	K0
HD 73710				73710	42549	08^h 40^m 22.11^s	+19° 40′ 11.9″	6.42	−0.41	756	K0III	in Beehive Cluster
ψ^1 Cnc	ψ^1	13		67690	40007	08^h 10^m 13.12^s	+25° 50′ 40.4″	6.44	−1.06	1032	K0
HD 73599				73599	42462	08^h 39^m 24.57^s	+08° 01′ 03.6″	6.46	0.32	551	K1III
HD 77660				77660	44574	09^h 04^m 55.12^s	+32° 22′ 37.2″	6.46	1.96	259	A8V
HD 67542				67542	39958	08^h 09^m 35.19^s	+29° 05′ 35.1″	6.47	−3.93	3928	G0II
HD 68703				68703	40342	08^h 14^m 11.14^s	+17° 40′ 33.3″	6.47	1.45	329	A0Vne...
HD 78234				78234	44825	09^h 08^m 04.21^s	+32° 32′ 25.6″	6.47	1.32	349	F2V
34 Cnc		34		72359	41904	08^h 32^m 39.87^s	+10° 03′ 57.7″	6.48	0.38	541	A1V	suspected variable
HD 78661				78661	44984	09^h 09^m 46.45^s	+11° 33′ 52.3″	6.48	3.60	123	F2p	suspected variable
HD 79248				79248	45272	09^h 13^m 37.27^s	+21° 16′ 59.6″	6.48	0.57	496	A2V
HD 76908				76908	44148	08^h 59^m 26.89^s	+13° 04′ 27.9″	6.49	−1.50	1294	K5III
81 Cnc	π^1	81		79096	45170	09^h 12^m 17.87^s	+14° 59′ 43.6″	6.49	4.93	67	G9V
HD 72115				72115	41833	08^h 31^m 41.31^s	+18° 59′ 16.0″	6.50	−0.99	1025	K0
24 Cnc A		24		71152	41389	08^h 26^m 39.82^s	+24° 32′ 03.7″	6.51	2.11	248	F0III	component of the 24 Cnc system; suspected variable
37 Cnc		37		73316	42353	08^h 38^m 05.19^s	+09° 34′ 28.7″	6.54	1.25	373	A1V
35 Cnc		35		72779	42133	08^h 35^m 19.47^s	+19° 35′ 24.3″	6.55	0.28	585	G0III
ι Cnc B	ι	48		74738	43100	08^h 46^m 40.00^s	+28° 45′ 54.6″	6.58	2.77	188	G8II...	component of the ι Cnc system
40 Cnc		40		73666	42523	08^h 40^m 11.47^s	+19° 58′ 16.2″	6.61	0.40	570	A1V	in Beehive Cluster; blue straggler
83 Cnc		83		80218	45699	09^h 18^m 58.91^s	+17° 42′ 20.4″	6.61	3.64	128	F5
38 Cnc		38	BT	73575	42485	08^h 39^m 42.68^s	+19° 46′ 42.5″	6.66	0.59	531	F0III	in Beehive Cluster; δ Sct variable, ΔV = 0.06^m, P = 0.10 d
70 Cnc		70		77557	44512	09^h 04^m 09.87^s	+27° 53′ 53.9″	6.67	0.33	605	A1V
2 LMi		(2)		73427	42472	08^h 39^m 31.87^s	+32° 30′ 56.2″	6.69	−1.18	1220	K5
3 LMi		(3)		73508	42503	08^h 39^m 56.35^s	+32° 43′ 38.2″	6.71	0.66	528	K0
EP Cnc			EP	73819	42600	08^h 40^m 56.30^s	+19° 34′ 49.2″	6.76	0.6	556	A6Vn	in Beehive Cluster; δ Sct variable, ΔV = 0.03^m
42 Cnc		42		73785	42578	08^h 40^m 43.23^s	+19° 43′ 09.6″	6.83	0.87	506	A9III	in Beehive Cluster
7 Cnc		7		66347	39447	08^h 03^m 50.48^s	+22° 04′ 14.9″	6.84	0.28	668	K0
80 Cnc		80		79009	45153	09^h 11^m 56.93^s	+18° 02′ 39.0″	6.87	1.08	470	A0	[2][3]
11 Cnc		11		67402	39888	08^h 08^m 49.60^s	+27° 28′ 49.5″	6.88	0.15	944	K0III	Double
78 Cnc		78		78479	44918	09^h 09^m 02.31^s	+17° 28′ 10.7″	7.18	0.5	706	K3III
VZ Cnc			VZ	73857	42594	08^h 40^m 52.13^s	+09° 49′ 27.1″	7.18	1.21	509	A9III	double-mode δ Sct variable, Vmax = 7.18^m, Vmin = 7.91^m, P = 0.18 d
ADS 7284			IP	79969	45617	09^h 17^m 53.46^s	+28° 33′ 37.9″	7.21	6.03	56.28	K3V	BY Dra variable, ΔV = 0.02^m, P = 43.4 d
52 Cnc		52		75558	43463	08^h 51^m 10.83^s	+15° 59′ 57.8″	7.38	1.03	607	G5
68 Cnc		68		77230	44336	09^h 01^m 43.66^s	+17° 04′ 51.8″	7.38		620	A2Vn	[4][3]
V Cnc			V	70276	40977	08^h 21^m 42.84^s	+17° 17′ 07.2″	7.50			S0-6/6e	Mira variable, Vmax = 7.5^m, Vmin = 13.9^m, P = 270 d
T Cnc			T		43905	08^h 56^m 40.15^s	+19° 50′ 57.0″	7.60			C	semiregular variable, Vmax = 7.6^m, Vmin = 10.5^m, P = 482 d
BU Cnc			BU	73576		08^h 39^m 44.67^s	+19° 16′ 30.8″	7.68	1.44	577	A7Vn	in Beehive Cluster; δ Sct variable, ΔV = 0.03^m, P = 0.071 d
BN Cnc			BN	73763		08^h 40^m 39.24^s	+19° 13′ 41.8″	7.80	1.56	577	A9V	in Beehive Cluster; δ Sct variable, ΔV = 0.03^m, P = 0.039 d
HD 72490				72490	41997	08^h 33^m 36.6^s	+13° 33′ 03″	7.8		405	G5	has a planet (b)
24 Cnc B		24		71153		08^h 26^m 40.10^s	+24° 32′ 07.0″	7.81				component of the 24 Cnc system
BY Cnc			BY	74050	42705	08^h 42^m 10.81^s	+18° 56′ 03.7″	7.91	2.21	451	A7Vn	in Beehive Cluster; δ Sct variable, ΔV = 0.01^m, P = 0.058 d
HD 74028			BX	74028		08^h 42^m 06.50^s	+19° 24′ 40.5″	7.96	1.72	577	A7V	in Beehive Cluster; δ Sct variable, ΔV = 0.02^m, P = 0.044 d
44 Cnc		44		74200	42791	08^h 43^m 08.36^s	+18° 09′ 02.0″	8.03	1.29	726	K0	its radius is about 12.11 R☉.[5][6]
HD 79498				79498	45406	09^h 15^m 09^s	+23° 22′ 32″	8.03	4.72	150	G5	has a planet (b)
71 Cnc		71		77802	44637	09^h 05^m 45.52^s	+17° 23′ 24.5″	8.10	1.53	672	A2
CY Cnc			CY	73345		08^h 38^m 37.86^s	+19° 59′ 23.1″	8.14	1.88	582	F0V	in Beehive Cluster; δ Sct variable, ΔV = 0.02^m, P = 0.1 d
BQ Cnc			BQ	73729		08^h 40^m 26.75^s	+20° 10′ 55.2″	8.19	1.95	577	F2Vn	in Beehive Cluster; δ Sct variable, ΔV = 0.02^m, P = 0.074 d
HD 73534				73534	42446	08^h 39^m 15.80^s	+12° 57′ 37.3″	8.24	3.30	316	G5IV	Gakyid; has a planet (b)
BR Cnc			BR	73175	42319	08^h 37^m 40.71^s	+19° 31′ 06.3″	8.26	1.91	608	F0Vn	in Beehive Cluster; δ Sct variable, ΔV = 0.02^m, P = 0.038 d
S Cnc			S	74307	42853	08^h 43^m 56.14^s	+19° 02′ 03.0″	8.35	1.03	950	B9.5V+ G8-9III-IV	Algol variable, Vmax = 8.29^m, Vmin = 10.25^m, P = 9.48 d
BW Cnc			BW	73798		08^h 40^m 52.48^s	+20° 15′ 59.5″	8.48	2.24	577	F0Vn	in Beehive Cluster; δ Sct variable, ΔV = 0.01^m, P = 0.072 d
TW Cnc			TW	71780		08^h 29^m 37.32^s	+12° 27′ 20.3″	8.49			G8III+...	Algol variable, Vmax = 8.5^m, Vmin = 8.97^m, P = 70.76 d
U Cnc			U	72863		08^h 35^m 46.29^s	+18° 53′ 44.5″	8.50			M2e	Mira variable, Vmax = 8.5^m, Vmin = 15.5^m, P = 306 d
BS Cnc			BS	73450		08^h 39^m 09.10^s	+19° 35′ 32.6″	8.59	2.35	577	A9V	in Beehive Cluster; δ Sct variable, ΔV = 0.02^m, P = 0.051 d
R Cnc			R	69243	40534	08^h 16^m 33.90^s	+11° 43′ 35.0″	8.64	-0.36	2060	M6.5-9e	Mira variable, Vmax = 6.07^m, Vmin = 11.9^m, P = 357 d
BV Cnc			BV	73746		08^h 40^m 32.97^s	+19° 11′ 39.6″	8.65	2.41	577	F0V	in Beehive Cluster; δ Sct variable, ΔV = 0.02^m, P = 0.21 d
RZ Cnc			RZ	73343	42432	08^h 39^m 08.54^s	+31° 47′ 44.4″	8.67	0.48	1420	K2III	RS CVn variable, Vmax = 8.67^m, Vmin = 10.03^m, P = 21.64 d
HD 74721				74721	43018	08^h 45^m 59.26^s	+13° 15′ 48.6″	8.72			A0V	horizontal branch star
HD 77065				77065	44259	09^h 00^m 47.0^s	+21° 27′ 13″	8.8	6.3	103	G5	has a planet (b)
UU Cnc			UU		39341	08^h 02^m 30.90^s	+15° 10′ 41.9″	8.85			K4III...	β Lyr variable, Vmax = 8.68^m, Vmin = 9.35^m, P = 96.71 d
HIP 41378					41378	08^h 26^m 28.0^s	+10° 04′ 49″	8.9	3.58	378		has six planets (b, c, d, e, f & g)
RX Cnc			RX	68775	40388	08^h 14^m 43.54^s	+24° 44′ 05.3″	9.20	1.92	931	M8	semiregular variable
HD 80653				80653		09^h 21^m 21.0^s	+14° 22′ 05″	9.50		358	G5	semiregular variable
WY Cnc			WY		44349	09^h 01^m 55.45^s	+26° 41′ 22.7″	9.60	5.05	264.6	G5V	RS CVn variable, Vmax = 9.51^m, Vmin = 10.14^m, P = 0.83 d
TX Cnc			TX			08^h 40^m 01.70^s	+18° 59′ 59.5″	9.97	3.55	626	G0-G1V	in Beehive Cluster; W UMa variable, Vmax = 10^m, Vmin = 10.35^m, P = 0.38 d
RU Cnc			RU		42303	08^h 37^m 30.13^s	+23° 33′ 41.6″	10.20	2.97	911	F9V:+...	RS CVn variable, Vmax = 10.1^m, Vmin = 11.25^m, P = 10.17 d
TU Cnc			TU			08^h 52^m 16.65^s	+09° 05′ 18.8″	10.53			A2	Algol variable
SY Cnc			SY			09^h 01^m 03.32^s	+17° 53′ 56.2″	10.60			G8V	Z Cam variable
EX Cnc			EX			08^h 51^m 34.32^s	+11° 51′ 10.5″	10.95	1.34	2720	A7	in Messier 67; δ Sct variable, ΔV = 0.05^m, P = 0.049 d
TT Cnc			TT		41936	08^h 32^m 55.18^s	+13° 11′ 28.5″	11.10			F0	RR Lyr variable, Vmax = 10.93^m, Vmin = 11.57^m, P = 0.56 d
ES Cnc			ES			08^h 51^m 20.79^s	+11° 53′ 26.2″	11.16	1.55	2720	F4	in Messier 67; RS CVn variable, Vmax = 11.16^m, Vmin = 11.28^m, P = 1.07 d
HAT-P-31						08^h 06^m 09^s	+26° 25′ 36″	11.66	3.91	1155		has a transiting planet (b)
CU Cnc			CU		41824	08^h 31^m 37.57^s	+19° 23′ 39.4″	11.80	11.58	36.07	M5Ve	Algol variable and flare star, Vmax = 11.68^m, Vmin = 11.80^m, P = 2.77 d
WASP-65						08^h 53^m 18.0^s	+08° 31′ 23″	11.9	4.44	1011	G6	has a transiting planet (b)
SS Cnc			SS			08^h 06^m 25.60^s	+23° 15′ 05.7″	12.11			A8.5	RR Lyr variable, Vmax = 11.49^m, Vmin = 12.72^m, P = 0.37 d
EW Cnc			EW			08^h 51^m 32.58^s	+11° 50′ 40.6″	12.27	2.66	2720	F0	in Messier 67; δ Sct variable, ΔV = 0.02^m, P = 0.053 d
HV Cnc			HV			08^h 51^m 17.99^s	+11° 45′ 54.2″	12.73	3.12	2720		in Messier 67; Algol variable
EV Cnc			EV			08^h 51^m 28.15^s	+11° 49′ 27.5″	12.78	3.17	2720	F3	in Messier 67; W UMa variable, ΔV = 0.13^m, P = 0.44 d
AD Cnc			AD			08^h 46^m 20.10^s	+10° 20′ 07.2″	13.10			K0V	W UMa variable, Vmax = 13.1^m, Vmin = 13.4^m, P = 0.28 d
Gliese 299						08^h 11^m 57.575^s	+08° 46′ 22.05″	13.24		22	M4.5 Ve	a red dwarf, 15.5% as massive as the Sun,[7] 17.9% as wide,[8] and has a surface temperature of about 3,050 K.[9][10][11][12]
HAT-P-43						08^h 35^m 42.0^s	+10° 12′ 24″	13.36		1771		has a transiting planet (b)
AH Cnc			AH			08^h 51^m 37.85^s	+11° 50′ 57.1″	13.41	3.8	2720	F7V	in Messier 67; W UMa variable, Vmax = 13.31^m, Vmin = 13.96^m, P = 0.36 d
HU Cnc			HU			08^h 51^m 13.36^s	+11° 51′ 40.1″	13.61	4	2720	G8IV	in Messier 67; RS CVn variable, Vmax = 13.45^m, Vmin = 13.61^m, P = 18.39 d
AC Cnc			AC			08^h 44^m 27.11^s	+12° 52′ 31.9″	13.80			K1-3V	Algol variable and nova-like star, Vmax = 13.8^m, Vmin = 15.4^m, P = 0.30 d
G 9-38			EI			08^h 58^m 15.19^s	+19° 45′ 47.1″			17.2	M5.5V	flare star
YBP 1194						08^h 51^m 00.81^s	+11° 48′ 52.8″	14.61	5	2720	G5V	in Messier 67; solar twin; has 3 planets
DX Cnc			DX			08^h 29^m 49.35^s	+26° 46′ 33.7″	14.81	17.01	11.82	M6.5V	flare star
AT Cnc			AT			08^h 28^m 36.93^s	+25° 20′ 03.0″	15.2			DAe...	Z Cam variable, Vmax = 12.57^m, Vmin = 15.2^m, P = 0.20 d
LHS 2090						09^h 00^m 23.59^s	+21° 50′ 05.4″	16.10	17.08	20.782	M6.5V	[13][14][15][16][17]
YZ Cnc			YZ			08^h 10^m 56.65^s	+28° 08′ 33.5″	16.3				SU UMa variable, Vmax = 10.5^m, Vmin = 16.3^m, P = 0.087 d
EG Cnc			EG			08^h 43^m 03.99^s	+27° 51′ 49.7″	17.0				Huruhata's Variable; WZ Sge variable, Vmax = 11.9^m, Vmin = 17.0^m, P = 0.060 d
DW Cnc			DW			07^h 58^m 53.05^s	+16° 16′ 45.2″	17.5			O...	dwarf nova, Vmax = 11.36^m, Vmin = 17.5^m, P = 0.0060 d
AZ Cnc			AZ			08^h 40^m 29.75^s	+18° 14′ 09.2″	17.59	16.86	45.7	M6.0V	flare star
GY Cnc			GY			09^h 09^m 50.55^s	+18° 49′ 47.5″	17.8				dwarf nova and eclipsing binary, Vmax = 12.5^m, Vmin = 17.8^m, P = 0.18 d
AR Cnc			AR			09^h 22^m 07.55^s	+31° 03′ 14.5″	18.7				dwarf nova and Algol variable, Vmax = 15.3^m, Vmin = 18.7^m, P = 0.21 d
RX J0806.3+1527			HM			08^h 06^m 22.95^s	+15° 27′ 31.1″			160		AM Canum Venaticorum star
AK Cnc			AK			08^h 55^m 21.18^s	+11° 18′ 15.3″					SU UMa variable
CC Cnc			CC			08^h 36^m 19.15^s	+21° 21′ 05.3″				K0V	SU UMa variable
PSR B0823+26						08^h 26^m 51.44^s	+26° 37′ 22.8″					pulsar
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 mv), also known as apparent magnitude  • abs. mag. = absolute magnitude (Mv)  • 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.]

See also

• List of stars by constellation

References

1. Final Results of NameExoWorlds Public Vote Released
2. Abt, Helmut A. (2004). "Spectral Classification of Stars in A Supplement to the Bright Star Catalogue". The Astrophysical Journal Supplement Series. 155 (1): 175–177. Bibcode:2004ApJS..155..175A. doi:10.1086/423803.
3. van Leeuwen, F. (November 2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.
4. Bidelman, William P.; Ratcliff, Stephen J.; Svolopoulos, Sotirios (1988). "Spectral types of 80 early-type stars of variable radial velocity". Astronomical Society of the Pacific. 100: 828. Bibcode:1988PASP..100..828B. doi:10.1086/132242.
5. "44 Cancri - HD74200 - HIP42791". Universe Guide. Retrieved 24 September 2017.
6. SIMBAD, 44 Cancri (Retrieved 24 September 2017)
7. Jenkins, J. S.; Ramsey, L. W.; Jones, H. R. A.; Pavlenko, Y.; Gallardo, J.; Barnes, J. R.; Pinfield, D. J. (2009). "Rotational Velocities for M Dwarfs". The Astrophysical Journal. 704 (2): 975–988. arXiv:0908.4092. Bibcode:2009ApJ...704..975J. doi:10.1088/0004-637X/704/2/975.
8. Dittmann, Jason A.; Irwin, Jonathan M.; Charbonneau, David; Berta-Thompson, Zachory K. (2014). "Trigonometric Parallaxes for 1507 Nearby Mid-to-late M Dwarfs". The Astrophysical Journal. 784 (2): 156. arXiv:1312.3241. Bibcode:2014ApJ...784..156D. doi:10.1088/0004-637X/784/2/156.
9. Lépine, Sébastien (2013). "A Spectroscopic Catalog of the Brightest (J < 9) M Dwarfs in the Northern Sky". The Astronomical Journal. 145 (4). arXiv:1206.5991. Bibcode:2013AJ....145..102L. doi:10.1088/0004-6256/145/4/102.
10. Cutri, R. M.; et al. (2003). "2MASS All-Sky Catalog of Point Sources". VizieR On-line Data Catalog. Bibcode:2003yCat.2246....0C.
11. Wilson, Ralph Elmer (1953). "General catalogue of stellar radial velocities". Bibcode:1953GCRV..C......0W. Cite journal requires |journal= (help)
12. Zacharias, N. (2012). "The fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)". VizieR On-line Data Catalog. Bibcode:2012yCat.1322....0Z.
13. Cutri, R. M.; et al. (2003). "2MASS All-Sky Catalog of Point Sources". VizieR On-line Data Catalog. Bibcode:2003yCat.2246....0C.
14. Alonso-Floriano, F. J.; et al. (2015). "CARMENES input catalogue of M dwarfs. I. Low-resolution spectroscopy with CAFOS". Astronomy & Astrophysics. 577: A128. arXiv:1502.07580. Bibcode:2015A&A...577A.128A. doi:10.1051/0004-6361/201525803.
15. Lépine, Sébastien; Shara, Michael M. (2005). "A Catalog of Northern Stars with Annual Proper Motions Larger than 0.″15 (LSPM-NORTH Catalog)". The Astronomical Journal. 129 (3): 1483. arXiv:astro-ph/0412070. Bibcode:2005AJ....129.1483L. doi:10.1086/427854.
16. "LHS 2090". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 29 January 2018.
17. Henry, T. J.; Jao, Wei-Chun; Subasavage, John P.; Beaulieu, Thomas D.; Ianna, Philip A.; Costa, Edgardo; Méndez, René A. (2006). "The Solar Neighborhood. XVII. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample" (PDF). The Astronomical Journal. 132 (6): 2360–2371. arXiv:astro-ph/0608230. Bibcode:2006AJ....132.2360H. doi:10.1086/508233.CS1 maint: multiple names: authors list (link)

Bibliography

• 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.
• Gould, B. A. "Uranometria Argentina". Reprinted and updated by Pilcher, F. Archived from the original on 27 February 2012. Retrieved 19 July 2010.
• Samus, N. N.; Durlevich, O. V.; et al. (2004). "Combined General Catalogue of Variable Stars (GCVS4.2)". Retrieved 4 April 2012.
• Samus, N. N.; Durlevich, O. V.; et al. (2012). "General Catalog of Variable Stars (GCVS database, version 2012Feb)". Retrieved 4 April 2012.
• "AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
• "Naming Stars". Retrieved 4 July 2018.