List of stars in Scorpius

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

Name	B	F	Var	HD	HIP	RA	Dec	vis. mag.	abs. mag.	Dist. (ly)	Sp. class	Notes
Antares A	α	21		148478	80763	16^h 29^m 24.47^s	−26° 25′ 55.0″	0.91	−5.24	553	M1.5Iab-b	Cor Scorpii, Qalb al-Aqrab, Vespertilo; 16th brightest star; binary; semiregular variable, V_max = 0.75^m, V_min = 1.21^m, P = 2180 d
λ Sco	λ	35		158926	85927	17^h 33^m 36.53^s	−37° 06′ 13.5″	1.62	−5.05	703	B2IV+DA7.9	Shaula; β Cep and Algol variable, V_max = 1.59^m, V_min = 1.65^m, P = 0.21 d
θ Sco	θ			159532	86228	17^h 37^m 19.13^s	−42° 59′ 52.2″	1.86	−2.75	272	F1II	Sargas; suspected variable, V_max = 1.84^m, V_min = 1.88^m
δ Sco	δ	7		143275	78401	16^h 00^m 20.01^s	−22° 37′ 17.8″	2.29	−3.16	401	B0.2IVe	Dschubba, Al Jabba, Iclarkrau; γ Cas variable, V_max = 1.59^m, V_min = 2.32^m
ε Sco	ε	26		151680	82396	16^h 50^m 10.24^s	−34° 17′ 33.4″	2.29	0.78	65	K2IIIb	Wei, Larawag; suspected variable, V_max = 2.24^m, V_min = 2.35^m
κ Sco	κ			160578	86670	17^h 42^m 29.28^s	−39° 01′ 47.7″	2.39	−3.38	464	B1.5III	Girtab; β Cep variable, V_max = 2.41^m, V_min = 2.42^m, P = 0.20 d
β¹ Sco	β¹	8		144217	78820	16^h 05^m 26.23^s	−19° 48′ 19.4″	2.62	−3.44	530	B0.5V	Acrab, Elacrab, Graffias, Grafias, Grassias; suspected variable, V_max = 2.61^m, V_min = 2.67^m
υ Sco	υ	34		158408	85696	17^h 30^m 45.84^s	−37° 17′ 44.7″	2.70	−3.31	518	B2IV	Lesath, Lesuth
τ Sco	τ	23		149438	81266	16^h 35^m 52.96^s	−28° 12′ 57.5″	2.82	−2.78	430	B0V	Paikauhale,^[1] Alniyat, Al Niyat
π Sco	π	6		143018	78265	15^h 58^m 51.12^s	−26° 06′ 50.6″	2.89	−2.85	459	B1V + B2V	Fang; Nur;^[2] rotating ellipsoidal variable, V_max = 2.88^m, V_min = 2.91^m, P = 1.57 d
σ Sco	σ	20		147165	80112	16^h 21^m 11.32^s	−25° 35′ 33.9″	2.90	−3.86	734	B1III	Alniyat, Al Niyat, β Cep variable, V_max = 2.86^m, V_min = 2.94^m, P = 0.25 d
ι¹ Sco	ι¹			161471	87073	17^h 47^m 35.08^s	−40° 07′ 37.1″	2.99	−5.71	1791	F3Ia
μ¹ Sco	μ¹			151890	82514	16^h 51^m 52.24^s	−38° 02′ 50.4″	3.00	−4.01	821	B1.5IV + B	Xamidimura; β Lyr variable, V_max = 2.94^m, V_min = 3.22^m, P = 1.45 d
G Sco	G			161892	87261	17^h 49^m 51.45^s	−37° 02′ 36.1″	3.19	0.24	127	K0/K1III	γ Tel, Fuyue
η Sco	η			155203	84143	17^h 12^m 09.18^s	−43° 14′ 18.6″	3.32	1.61	72	F3p	suspected variable
μ² Sco	μ²			151985	82545	16^h 52^m 20.15^s	−38° 01′ 02.9″	3.56	−2.44	517	B2IV	Pipirima, Shéngōng (神宮),^[3]
ζ² Sco	ζ²			152334	82729	16^h 54^m 35.11^s	−42° 21′ 38.7″	3.62	0.30	150	K4III	suspected variable, V_max = 3.59^m, V_min = 3.65^m
ρ Sco	ρ	5		142669	78104	15^h 56^m 53.09^s	−29° 12′ 50.4″	3.87	−1.62	409	B2IV/V	Iklil, suspected variable
ω¹ Sco	ω¹	9		144470	78933	16^h 06^m 48.43^s	−20° 40′ 08.9″	3.93	−1.64	423	B1V	Jabhat al Akrab
ν Sco	ν	14		145502	79374	16^h 11^m 59.74^s	−19° 27′ 38.3″	4.00	−1.63	436	B2IV	Jabbah, Jabah; quintuple star
H Sco	H			149447	81304	16^h 36^m 22.46^s	−35° 15′ 19.3″	4.18	−0.90	339	K5III	β Nor; suspected variable, V_max = 4.15^m, V_min = 4.18^m
N Sco	N			148703	80911	16^h 31^m 22.94^s	−34° 42′ 15.6″	4.24	−2.56	746	B2III-IV	α Nor
Q Sco	Q			159433	86170	17^h 36^m 32.85^s	−38° 38′ 05.5″	4.26	1.03	144	G8/K0III/IV	suspected variable, V_max = 4.26^m, V_min = 4.29^m
ω² Sco	ω²	10		144608	78990	16^h 07^m 24.30^s	−20° 52′ 07.2″	4.31	−0.24	265	G6/G8III	Jabhat al Akrab; on 18 November 2038, it will be occulted by Venus over a small part of Southeast Africa, S Indian Ocean^[4]^: 166
ο Sco	ο	19		147084	80079	16^h 20^m 38.18^s	−24° 10′ 09.4″	4.55	−3.24	1177	A4II/III	suspected variable, V_max = 4.52^m, V_min = 4.58^m
13 Sco	c²	13		145482	79404	16^h 12^m 18.21^s	−27° 55′ 34.7″	4.58	−1.20	468	B2V
2 Sco	A	2		142114	77840	15^h 53^m 36.73^s	−25° 19′ 37.5″	4.59	−1.03	434	B2.5Vn
1 Sco	b	1		141637	77635	15^h 50^m 58.75^s	−25° 45′ 04.4″	4.63	−1.39	522	B1.5Vn
ζ¹ Sco	ζ¹			152236	82671	16^h 53^m 59.73^s	−42° 21′ 43.3″	4.70	−8.5	2600	B1Iae	in NGC 6231; luminous blue variable, V_max = 4.66^m, V_min = 4.86^m
ξ Sco A	ξ	(51)		144070		16^h 04^m 22.10^s	−11° 22′ 23.0″	4.77		92		51 Lib; sextuple star
ι² Sco	ι²			161912	87294	17^h 50^m 11.11^s	−40° 05′ 25.5″	4.78	−5.50	3705	A6Ib	suspected variable
22 Sco	i	22		148605	80815	16^h 30^m 12.48^s	−25° 06′ 54.6″	4.79	−0.61	393	B3V	suspected variable
HD 161840	(ξ)^[5]			161840	87220	17^h 49^m 10.47^s	−31° 42′ 11.5″	4.79	−1.56	607	B8Ib/II	Xi Telescopii
HD 146624	d			146624	79881	16^h 18^m 17.92^s	−28° 36′ 49.6″	4.80	1.63	140	A0V:
V1073 Sco	k		V1073	154090	83574	17^h 04^m 49.35^s	−34° 07′ 22.5″	4.83	−4.74	2672	B2Iab	α Cyg variable
HD 163145				163145	87846	17^h 56^m 47.43^s	−44° 20′ 31.9″	4.85	−0.29	347	K2III
HD 163376	y^[6]			163376	87936	17^h 57^m 47.81^s	−41° 42′ 58.5″	4.88	−1.24	547	M0III	suspected variable
β² Sco	β²			144218	78821	16^h 05^m 26.58^s	−19° 48′ 06.6″	4.90	−2.80	530	B2V	component of the β Sco system
ψ Sco	ψ	15		145570	79375	16^h 12^m 00.00^s	−10° 03′ 51.1″	4.93	1.41	165	A3IV
HD 143787				143787	78650	16^h 03^m 20.67^s	−25° 51′ 54.5″	4.96	0.90	212	K3III
HD 153613				153613	83336	17^h 01^m 52.65^s	−32° 08′ 36.2″	5.03	−0.86	491	B8V
HD 154948				154948	84033	17^h 10^m 42.35^s	−44° 33′ 27.2″	5.06	0.24	300	G8/K0III+..
ξ Sco B	ξ			144069	78727	16^h 04^m 22.3^s	−11° 22′ 18″	5.07		92	F5IV	component of the ξ Sco system
HD 145250				145250	79302	16^h 11^m 02.13^s	−29° 24′ 57.6″	5.09	0.62	255	K0III
HD 157243				157243	85162	17^h 24^m 13.09^s	−44° 09′ 45.0″	5.10	−1.73	756	B7III
Antares B	α	21		148479		16^h 29^m 24.2^s	−26° 25′ 51″	5.2	−0.9	553	B2.5V	component of the Antares system
HD 151804			V973	151804	82493	16^h 51^m 33.72^s	−41° 13′ 49.9″	5.23	−6.36	6792	O8Iaf	α Cyg variable, V_max = 5.22^m, V_min = 5.28^m
χ Sco	χ	17		145897	79540	16^h 13^m 50.91^s	−11° 50′ 15.8″	5.24	−0.41	439	K3III	Has a planet (b)
HD 148688			V1058	148688	80945	16^h 31^m 41.77^s	−41° 49′ 01.7″	5.31	−6.79	8579	B1Ia	α Cyg variable
HD 144690				144690	79050	16^h 08^m 07.52^s	−26° 19′ 36.0″	5.35	−0.23	425	M2III	variable star, ΔV = 0.008^m, P = 7.61 d
HD 147513				147513	80337	16^h 24^m 01.24^s	−39° 11′ 34.8″	5.37	4.82	42	G3/G5V	has a planet (b)
HD 142165				142165	77858	15^h 53^m 53.92^s	−24° 31′ 59.1″	5.38	−0.14	414	B5V
HR 5907			V1040	142184	77859	15^h 53^m 55.87^s	−23° 58′ 40.9″	5.41	0.01	393	B2V	Algol variable, V_max = 5.39^m, V_min = 5.43^m, P = 1.02 d
HD 147628				147628	80390	16^h 24^m 31.77^s	−37° 33′ 57.5″	5.42	−0.36	468	B8V	suspected rotating ellipsoidal variable, ΔV = 0.02^m
HD 142990			V913	142990	78246	15^h 58^m 34.87^s	−24° 49′ 53.1″	5.43	−0.45	488	B5V	SX Ari variable, V_max = 5.4^m, V_min = 5.47^m, P = 0.98 d
16 Sco	n^[6]	16		145607	79387	16^h 12^m 07.29^s	−08° 32′ 51.3″	5.43	1.01	250	A4V
HD 149404			V918	149404	81305	16^h 36^m 22.57^s	−42° 51′ 31.9″	5.46	−4.39	3047	O9Ia	rotating ellipsoidal variable, V_max = 5.42^m, V_min = 5.5^m, P = 9.81 d
HD 152234				152234	82676	16^h 54^m 01.84^s	−41° 48′ 23.0″	5.46	−5.84	5927	B0.5Ia	in NGC 6231; suspected variable
HD 151078				151078	82135	16^h 46^m 47.97^s	−39° 22′ 36.8″	5.48	0.21	369	K0III
27 Sco		27		152820	82960	16^h 57^m 11.17^s	−33° 15′ 34.1″	5.48	−1.25	724	K5III
18 Sco		18		146233	79672	16^h 15^m 37.13^s	−08° 22′ 05.7″	5.49	4.76	46	G1V	solar twin; suspected variable, V_max = 5.48^m, V_min = 5.59^m
HD 144987	r²^[6]			144987	79199	16^h 09^m 52.61^s	−33° 32′ 44.5″	5.50	−0.12	433	B8V
HD 146836	p^[6]			146836	79980	16^h 19^m 32.68^s	−30° 54′ 24.4″	5.53	2.44	135	F5IV
HD 156098				156098	84551	17^h 17^m 03.71^s	−32° 39′ 45.7″	5.53	2.01	165	F6V
HD 160668				160668	86698	17^h 42^m 51.09^s	−36° 56′ 43.8″	5.53	−0.57	542	K5III
HD 155806			V1075	155806	84401	17^h 15^m 19.25^s	−33° 32′ 54.3″	5.53	−5.13	4466	O8Ve	Be star
HD 162587				162587	87569	17^h 53^m 23.47^s	−34° 53′ 42.4″	5.58	−1.97	1055	K3III	in Messier 7
4 Sco		4		142445	77984	15^h 55^m 30.10^s	−26° 15′ 57.3″	5.63	0.02	432	A3V
HD 150742				150742	81972	16^h 44^m 42.60^s	−40° 50′ 22.6″	5.64	−0.26	492	B3V
HD 155259				155259	84150	17^h 12^m 16.22^s	−39° 30′ 24.4″	5.66	1.61	211	A0/A1V
12 Sco	c¹	12		145483	79399	16^h 12^m 16.05^s	−28° 25′ 01.9″	5.67	0.87	298	B9V
HD 159176			V1036	159176	86011	17^h 34^m 42.49^s	−32° 34′ 54.0″	5.69	−4.40	3396	O6V+...	in NGC 6383; trinary star; rotating ellipsoidal variable, V_max = 5.67^m, V_min = 5.73^m, P = 3.37 d
11 Sco		11		144708	79005	16^h 07^m 36.44^s	−12° 44′ 43.2″	5.75	0.17	426	B9V
HD 156293				156293	84690	17^h 18^m 47.84^s	−44° 07′ 46.9″	5.76	0.68	339	B9V	suspected variable
HD 152408				152408	82775	16^h 54^m 58.51^s	−41° 09′ 03.1″	5.78	−6.56	9588	WN9ha	in NGC 6231; suspected variable, V_max = 5.77^m, V_min = 5.82^m
HD 148247				148247	80672	16^h 28^m 14.46^s	−37° 10′ 47.3″	5.79	0.84	319	K1IIICN...
HD 147723				147723	80399	16^h 24^m 39.77^s	−29° 42′ 16.8″	5.82	2.91	107	F9IV	Double star with HD 147722
V1003 Sco			V1003	149711	81472	16^h 38^m 26.30^s	−43° 23′ 54.2″	5.83	−0.79	686	B2.5IV	rotating ellipsoidal variable, ΔV = 0.03^m
HD 142883	h^[6]			142883	78168	15^h 57^m 40.47^s	−20° 58′ 58.9″	5.84	0.11	455	B3V	Algol variable, V_max = 5.84^m, V_min = 6.31^m, P = 9.20 d
HD 150331				150331	81741	16^h 41^m 45.50^s	−33° 08′ 44.2″	5.84	1.08	292	G1II
HD 152293				152293	82716	16^h 54^m 26.94^s	−42° 28′ 44.0″	5.84			F5Ib-II
HD 158799				158799	85889	17^h 33^m 07.39^s	−41° 10′ 23.0″	5.84	−1.55	982	B9Ib/II
HD 162391				162391	87472	17^h 52^m 19.76^s	−34° 25′ 00.6″	5.84	−0.95	744	G8/K0III	In Messier 7
HD 145191				145191	79320	16^h 11^m 17.77^s	−41° 07′ 10.2″	5.86	1.66	226	F0IV
HD 144844				144844	79098	16^h 08^m 43.73^s	−23° 41′ 07.3″	5.87	0.28	426	B9V	α² CVn variable, V_max = 5.87^m, V_min = 5.90^m, P = 2.69 d
3 Sco		3	V927	142301	77909	15^h 54^m 39.54^s	−25° 14′ 37.2″	5.87	0.14	455	B8III/IV	SX Ari variable, ΔV = 0.03^m, P = 1.46 d
HD 160928				160928	86847	17^h 44^m 42.01^s	−42° 43′ 45.5″	5.87	1.29	269	A2/A3IV/V
V957 Sco			V957	162374	87460	17^h 52^m 13.66^s	−34° 47′ 57.1″	5.87	−1.16	830	B6Ib	In Messier 7; SX Ari variable, ΔV = 0.05^m
V929 Sco			V929	144334	78877	16^h 06^m 06.38^s	−23° 36′ 22.5″	5.90	0.03	487	B8V	SX Ari variable, V_max = 5.89^m, V_min = 5.91^m, P = 1.50 d
HD 145838				145838	79596	16^h 14^m 22.37^s	−33° 00′ 39.8″	5.91	−0.56	643	K0III
V923 Sco			V923	153890	83491	17^h 03^m 50.87^s	−38° 09′ 09.0″	5.91	1.88	209	F3V	Algol variable, V_max = 5.86^m, V_min = 6.24^m, P = 34.83 d
Gliese 667 A				156384A	84709	17^h 18^m 56.36^s	−34° 59′ 22.5″	5.91	6.69	23	K4V	component of the Gliese 667 system; suspected variable, V_max = 5.88^m, V_min = 5.92^m
HD 157097				157097	85048	17^h 22^m 54.73^s	−37° 13′ 14.5″	5.91	0.36	421	K1III
HD 149886				149886	81523	16^h 39^m 05.24^s	−37° 13′ 02.1″	5.93	0.31	434	B9.5V+...
HD 154783				154783	83896	17^h 08^m 47.55^s	−30° 24′ 12.8″	5.93	1.36	267	Fm
HD 162189				162189	87390	17^h 51^m 32.57^s	−40° 46′ 20.4″	5.94	−0.83	738	M2III	semiregular variable
V1068 Sco			V1068	152161	82650	16^h 53^m 42.44^s	−43° 03′ 03.2″	5.95	−1.81	1160	M3II/III	slow irregular variable
HD 153368				153368	83235	17^h 00^m 36.99^s	−35° 56′ 02.3″	5.95	1.19	292	K2IIICN...
HD 155450				155450	84226	17^h 12^m 58.56^s	−32° 26′ 18.0″	5.95	−4.35	3747	B1Ib
HD 155826				155826	84425	17^h 15^m 36.08^s	−38° 35′ 34.6″	5.95	3.52	100	G0V
HD 146850	l²^[6]			146850	79938	16^h 19^m 00.43^s	−14° 52′ 22.2″	5.97	−1.15	865	K3IIICNpvar
HD 154310				154310	83693	17^h 06^m 20.20^s	−37° 13′ 39.1″	5.98	0.42	422	A2IV
HD 158105				158105	85543	17^h 28^m 56.09^s	−36° 46′ 41.8″	5.98	−0.47	637	K0III
HD 150894				150894	81992	16^h 45^m 00.21^s	−28° 30′ 34.8″	5.99	−0.83	755	A3IV
V906 Sco			V906	162724	87616	17^h 53^m 54.77^s	−34° 45′ 09.8″	6.00	−1.45	1009	B9V + B9V	In Messier 7, Algol variable, V_max = 5.96^m, V_min = 6.23^m, P = 2.79 d
BM Sco			BM	160371	86527	17^h 40^m 58.55^s	−32° 12′ 52.0″	6.01	−2.35	1531	K3III + (G)	in Messier 6; slow irregular variable, V_max = 5.25^m, V_min = 6.46^m
HD 162517				162517	87532	17^h 52^m 57.60^s	−35° 37′ 27.1″	6.03	1.99	209	F2V
HD 150608				150608	81904	16^h 43^m 47.60^s	−38° 09′ 22.5″	6.05	−0.62	703	B9II/III
HD 153072				153072	83100	16^h 58^m 52.25^s	−37° 37′ 13.5″	6.05	1.47	269	A3III	Shengong,^[7] suspected variable
HD 162496				162496	87516	17^h 52^m 49.22^s	−34° 06′ 53.4″	6.05	−0.60	697	K1III
HD 162926				162926	87722	17^h 55^m 08.03^s	−36° 28′ 32.3″	6.05	−0.75	748	B9.5III
HD 146001				146001	79622	16^h 14^m 53.44^s	−25° 28′ 36.9″	6.06	0.30	462	B8V	α² CVn variable
HD 152248			V1007	152248	82691	16^h 54^m 10.06^s	−41° 49′ 30.1″	6.06			O7e	in NGC 6231; β Lyr variable, ΔV = 0.24^m, P = 5.82 d
HD 143619				143619	78575	16^h 02^m 39.40^s	−29° 08′ 08.8″	6.07	0.37	451	K2/K3III
HD 148760				148760	80910	16^h 31^m 22.87^s	−26° 32′ 15.2″	6.07	1.87	225	K1III
HD 146254	l¹^[6]			146254	79692	16^h 15^m 51.49^s	−14° 50′ 56.8″	6.09	−0.28	614	A0III	suspected variable, V_max = 6.06^m, V_min = 6.10^m
HD 155974				155974	84489	17^h 16^m 21.68^s	−35° 44′ 58.1″	6.09	3.55	105	F6V
HD 159707				159707	86311	17^h 38^m 08.45^s	−42° 52′ 48.7″	6.09	−0.54	692	B8V
HD 151771				151771	82453	16^h 51^m 00.04^s	−37° 30′ 52.1″	6.10	−0.99	853	B8II/III	suspected variable
HD 162817				162817	87671	17^h 54^m 27.12^s	−34° 28′ 00.2″	6.10	−0.96	842	B9.5/A0III
RR Sco			RR	152783	82912	16^h 56^m 37.85^s	−30° 34′ 48.1″	6.10		1150	M6IIIe	Mira variable, V_max = 5^m, V_min = 12.4^m, P = 281.45 d
HD 146954				146954	80066	16^h 20^m 32.63^s	−39° 25′ 48.8″	6.11	0.20	496	B9V
HD 154368			V1074	154368	83706	17^h 06^m 28.37^s	−35° 27′ 03.7″	6.13	−2.85	2040	O9.5Iab	α Cyg variable
HD 150591				150591	81914	16^h 43^m 54.09^s	−41° 06′ 47.9″	6.14	0.28	485	B6/B7V	suspected variable
HD 157486				157486	85237	17^h 25^m 02.67^s	−34° 41′ 45.6″	6.14	0.19	505	Ap...
HD 162586				162586	87567	17^h 53^m 19.58^s	−34° 43′ 50.9″	6.14	−0.88	825	B4III	in Messier 7
HD 142250				142250	77900	15^h 54^m 30.12^s	−27° 20′ 18.9″	6.15	0.09	531	B7V	has a planet (b)
HR 6522			V949	158741	85839	17^h 32^m 24.64^s	−34° 16′ 45.6″	6.16	1.06	341	F2IV	δ Sct variable, V_max = 6.13^m, V_min = 6.18^m, P = 0.22 d
HD 144927	r¹^[6]			144927	79173	16^h 09^m 31.76^s	−32° 38′ 56.2″	6.18	1.07	344	K1III
V861 Sco			V861	152667	82911	16^h 56^m 35.98^s	−40° 49′ 24.4″	6.18			B0Ia	in Trumpler 24; β Lyr variable, V_max = 6.07^m, V_min = 6.4^m, P = 7.85 d
HD 154153				154153	83650	17^h 05^m 48.47^s	−44° 06′ 18.4″	6.18	2.08	215	A4III
HD 162396				162396	87523	17^h 52^m 52.47^s	−41° 59′ 45.8″	6.19	3.62	107	F8V
HD 155940				155940	84445	17^h 15^m 51.36^s	−30° 12′ 38.2″	6.20	0.92	370	B9/B9.5V
RS Sco			RS	152476	82833	16^h 55^m 37.81^s	−45° 06′ 10.7″	6.20	−0.08	588	M6-7e	Mira variable, V_max = 5.96^m, V_min = 13.0^m, P = 319 d
HD 150573				150573	81903	16^h 43^m 45.70^s	−41° 07′ 08.9″	6.21	0.61	430	A4V
HD 143900				143900	78699	16^h 03^m 54.71^s	−24° 43′ 34.8″	6.22	−0.09	597	K2/K3III
HD 159633				159633	86246	17^h 37^m 26.92^s	−38° 03′ 58.9″	6.26	−3.44	2835	G2Ib
HD 154025				154025	83594	17^h 05^m 05.39^s	−45° 30′ 07.4″	6.28	1.33	319	A2V
HD 163433				163433	87948	17^h 57^m 57.80^s	−39° 08′ 11.3″	6.28	0.29	513	A0IV/V
V900 Sco			V900	152235	82669	16^h 53^m 58.85^s	−41° 59′ 39.6″	6.29			B1Ia	in Trumpler 24; rotating ellipsoidal variable, V_max = 6.29^m, V_min = 6.34^m, P = 2.63 d
HD 146834				146834	79945	16^h 19^m 07.71^s	−20° 13′ 04.9″	6.29	0.40	490	K0III
HD 152636				152636	82855	16^h 55^m 57.74^s	−33° 30′ 24.8″	6.29	0.03	581	K5III
ν Sco C	ν	14		145501		16^h 11^m 58.60^s	−19° 26′ 59.0″	6.30				component of the ν Sco system; α² CVn variable
HD 152424				152424	82783	16^h 55^m 03.33^s	−42° 05′ 27.0″	6.30			O9Ia	in Trumpler 24
HD 155276				155276	84151	17^h 12^m 16.55^s	−38° 49′ 20.7″	6.30	1.03	370	K1IIICN...
HD 158042				158042	85549	17^h 29^m 00.86^s	−43° 58′ 26.0″	6.30	−2.04	1516	B5III
HD 144585				144585	78955	16^h 07^m 03.53^s	−14° 04′ 16.8″	6.32	4.02	94	G5V
HD 144661				144661	79031	16^h 07^m 51.90^s	−24° 27′ 44.2″	6.32	0.97	384	B8IV/V
HD 145997				145997	79605	16^h 14^m 39.30^s	−18° 32′ 07.2″	6.32	1.63	282	K1III
HD 157038			V975	157038	85020	17^h 22^m 39.22^s	−37° 48′ 16.7″	6.33			B4Ia+...	α Cyg variable, V_max = 6.27^m, V_min = 6.35^m
HD 152431				152431	82731	16^h 54^m 35.94^s	−30° 35′ 14.4″	6.34	−0.09	631	A5IIIm...	suspected variable
HD 151965			V911	151965	82554	16^h 52^m 27.42^s	−40° 43′ 23.2″	6.35	0.07	588	B9p Si	α² CVn variable, V_max = 6.32^m, V_min = 6.38^m
V1077 Sco			V1077	156325	84650	17^h 18^m 20.51^s	−32° 33′ 11.1″	6.36	−1.57	1259	B5III	Be star
HD 158156				158156	85589	17^h 29^m 25.60^s	−38° 31′ 01.0″	6.38	1.34	332	A1V
HD 162678				162678		17^h 53^m 45.50^s	−34° 47′ 09.7″	6.38		980	B9V	in Messier 7
HD 145792			V1051	145792	79530	16^h 13^m 45.50^s	−24° 25′ 19.4″	6.40	0.69	453	B6IV	SX Ari variable
HD 146436				146436	79788	16^h 16^m 59.20^s	−20° 06′ 14.7″	6.40	−0.03	631	G8III
HD 145964				145964	79599	16^h 14^m 28.89^s	−21° 06′ 27.2″	6.41	1.29	345	B9V
HD 161390				161390	87042	17^h 47^m 07.30^s	−38° 06′ 43.5″	6.41	1.07	381	A0V
V951 Sco			V951	162725	87624	17^h 53^m 58.13^s	−34° 49′ 51.8″	6.41	−0.96	973	Ap...	in Messier 7, α² CVn variable, V_max = 6.39^m, V_min = 6.44^m, P = 4.46 d
V915 Sco			V915	155603	84332	17^h 14^m 27.66^s	−39° 45′ 59.9″	6.42			K0Ia	variable star, V_max = 6.22^m, V_min = 6.64^m
HD 157060				157060	85019	17^h 22^m 37.90^s	−35° 54′ 39.4″	6.42	3.58	121	F8V
HD 145100				145100	79203	16^h 09^m 55.31^s	−18° 20′ 25.6″	6.43	2.96	161	F3V
HD 149174				149174	81198	16^h 35^m 07.77^s	−45° 14′ 39.2″	6.43	0.06	614	K2/K3III	suspected variable, ΔV = 0.08^m
HD 158619				158619	85786	17^h 31^m 47.36^s	−33° 42′ 11.1″	6.43	0.98	401	K2III
HD 160748				160748	86716	17^h 43^m 06.86^s	−33° 03′ 04.6″	6.44	−3.13	2672	M1III	suspected variable
HD 147553				147553	80324	16^h 23^m 56.72^s	−33° 11′ 57.6″	6.45	1.11	381	A0V+...
HD 152249				152249		16^h 54^m 11.64^s	−41° 50′ 57.2″	6.45		5900	O9Ib(f)	in NGC 6231; suspected variable, V_max = 6.34^m, V_min = 6.51^m
HD 150638				150638	81891	16^h 43^m 38.73^s	−32° 06′ 21.2″	6.46	−0.44	784	B8V
HD 155985				155985	84556	17^h 17^m 05.54^s	−44° 46′ 42.9″	6.46			B0.5Iab:	Uñallamacha^[7], variable star, ΔV = 0.007^m, P = 293.25 d
HD 163234				163234	87865	17^h 56^m 55.89^s	−40° 18′ 20.3″	6.46	0.22	576	K3III
HD 150420				150420	81803	16^h 42^m 29.11^s	−37° 04′ 44.9″	6.47	1.09	388	G3III
HD 153919				153919	83499	17^h 03^m 56.77^s	−37° 50′ 39.0″	6.48			O5f
HD 159312				159312	86098	17^h 35^m 43.08^s	−37° 26′ 23.3″	6.48	1.40	338	A0V
HD 151932			V919	151932	82543	16^h 52^m 19.25^s	−41° 51′ 16.2″	6.49			WN7h	in Trumpler 24; Wolf–Rayet star, V_max = 6.45^m, V_min = 6.61^m, P = 2 d
HD 153234				153234	83202	17^h 00^m 14.26^s	−44° 59′ 18.5″	6.50	2.98	165	F3V
4U 1700-37			V884	153919	83499	17^h 03^m 56.77^s	−37° 50′ 38.9″	6.51		9100	O7.5Iaf	rotating ellipsoidal variable and high-mass X-ray binary, V_max = 6.51^m, V_min = 6.60^m, P = 3.41 d
HD 145102			V952	145102	79235	16^h 10^m 15.92^s	−26° 54′ 32.8″	6.57		547	B9p...	α² CVn variable, ΔV = 0.04^m, P = 1.42 d
V453 Sco			V453	163181	87810	17^h 56^m 16.08^s	−32° 28′ 30.0″	6.61	−5.43	8400	B0Ia	β Lyr variable, V_max = 6.36^m, V_min = 6.73^m, P = 12.01 d
RV Sco			RV	153004	83059	16^h 58^m 19.75^s	−33° 36′ 32.8″	6.61		1440	G0Ib	classical Cepheid, V_max = 6.61^m, V_min = 7.49^m, P = 6.06 d
HD 160529			V905	160529	86624	17^h 41^m 59.03^s	−33° 30′ 13.7″	6.66	−8.9	8150	A3Iae	luminous blue variable, V_max = 6.21^m, V_min = 6.97^m, P = 57 d
25 Sco		25		151179	82140	16^h 46^m 51.35^s	−25° 31′ 42.7″	6.72	−0.10	755	K0II
V636 Sco			V636	156979	85035	17^h 22^m 46.48^s	−45° 36′ 51.4″	6.74			F7/F8Ib/II + B9.5V	classical Cepheid, V_max = 6.4^m, V_min = 6.92^m, P = 6.80 d
V760 Sco			V760	147683	80405	16^h 24^m 43.72^s	−34° 53′ 37.5″	7.05		1280	B4V	Algol variable
HR 5999			V856	144668	79080	16^h 08^m 34.29^s	−39° 06′ 18.3″	7.05		531	A7IVe	UX Ori star, V_max = 6.77^m, V_min = 8.0^m
HD 143567				143567	78530	16^h 01^m 55^s	−21° 58′ 49″	7.18		511	B9V	has a planet (b)
Gliese 667 B				156384B		17^h 19^m 01.94^s	−34° 59′ 33.3″	7.24	8.02	23	K5	component of Gliese 667 system
HD 159868				159868	86375	17^h 38^m 59.53^s	−43° 08′ 43.8″	7.27	3.66	172	G5V	has two planets (b & c)
HD 147010			V933	147010	80024	16^h 20^m 05.49^s	−20° 03′ 23.0″	7.37		533	B9II/III	α² CVn variable, ΔV = 0.045^m, P = 3.92 d
HD 153950				153950	83547	17^h 04^m 30.87^s	−43° 18′ 35.2″	7.39	3.91	162	F8V	Rapeto,^[8] has a planet (b)
HD 153747			V922	153747	83410	17^h 02^m 53.82^s	−38° 27′ 36.8″	7.42		588	A0III	δ Sct variable
RY Sco			RY	162102	87345	17^h 50^m 32.34^s	−33° 42′ 20.4″	7.51			F6Ib	classical Cepheid, V_max = 7.51^m, V_min = 8.36^m, P = 20.32 d
HD 152219			V1292	152219		16^h 53^m 55.56^s	−41° 52′ 51.29″	7.57		5900	O9IV	in NGC 6231; Algol variable, V_max = 7.57^m, V_min = 7.80^m, P = 4.24 d
V393 Sco			V393	161741	87191	17^h 48^m 47.60^s	−35° 03′ 29.6″	7.59		2400	B3III	double periodic or Algol variable, V_max = 7.39^m, V_min = 8.31^m, P = 7.71 d
HD 152218			V1294	152218		16^h 53^m 59.99^s	−41° 42′ 52.8″	7.61			O9.5IV(n)	in Trumpler 24; Algol variable, V_max = 7.58^m, V_min = 7.67^m, P = 5.60 d
V703 Sco			V703	160589	86650	17^h 42^m 16.81^s	−32° 31′ 23.6″	7.85		556	A9V	double-mode δ Sct variable, V_max = 7.58^m, V_min = 8.04^m, P = 0.12 d
V482 Sco			V482	158443	85701	17^h 30^m 48.38^s	−33° 36′ 36.0″	7.91			F9II	classical Cepheid, V_max = 7.63^m, V_min = 8.3^m, P = 4.53 d
HD 147873				147873	80486	17^h 30^m 48.38^s	−33° 36′ 36.0″	7.96		342	G1V	has two planets (b & c)
AH Sco			AH	155161	84071	17^h 11^m 17.02^s	−32° 19′ 30.7″	8.10		12000	M4-5Ia-Iab	semiregular variable, V_max = 6.7^m, V_min = 9.5^m, P = 735 d; one of the largest known stars
HD 145377				145377	79346	16^h 11^m 36.45^s	−27° 04′ 41.4″	8.12	4.31	188	G3V	has a planet (b)
HD 144432				144432	78943	16^h 06^m 57.95^s	−27° 43′ 09.8″	8.19		522	F0IIIe+K7V	triple system; Herbig Ae/Be star
V1034 Sco			V1034			16^h 54^m 19.85^s	−41° 50′ 09.4″	8.23		5900	O8V	in NGC 6231; Algol variable, V_max = 8.23^m, V_min = 8.63^m, P = 2.44 d
RZ Sco			RZ	144018	78746	16^h 04^m 36.13^s	−24° 06′ 00.6″	8.3			M3e	semiregular variable, V_max = 8.3^m, V_min = 12.3^m, P = 162.1 d
HD 158393			V965	158393	85680	17^h 30^m 33.36^s	−33° 39′ 15.9″	8.57		937	G5:IIIe +F0/2IV/V	RS CVn variable, V_max = 8.46^m, V_min = 8.67^m, P = 30.52 d
V500 Sco			V500	316354	87173	17^h 48^m 37.50^s	−30° 28′ 33.5″	8.81		1060	K0	classical Cepheid, V_max = 8.4^m, V_min = 9.13^m, P = 9.32 d
HD 142666			V1026	142666		15^h 56^m 40.02^s	−22° 01′ 40.0″	8.86			A8Ve	UX Ori star, V_max = 8.57^m, V_min = 9.5^m
V907 Sco			V907	163302		17^h 56^m 55.56^s	−34° 45′ 01.2″	8.86			B9V	Algol variable, V_max = 8.61^m, V_min = 9.2^m, P = 3.78 d
V718 Sco			V718	145718	79476	16^h 13^m 11.59^s	−22° 29′ 06.7″	8.86		383	A8III/IV	UX Ori star, V_max = 8.75^m, V_min = 10.30^m
V701 Sco			V701	317844	85985	17^h 34^m 24.51^s	−32° 30′ 16.0″	8.97		3500	B5V	W UMa variable, V_max = 8.63^m, V_min = 9.05^m, P = 0.76 d
AK Sco			AK	152404	82747	16^h 54^m 44.85^s	−36° 53′ 18.6″	9.00		335	F5Ve	UX Ori star, V_max = 8.7^m, V_min = 12.8^m
HD 326823			V1104	326823		17^h 06^m 53.91^s	−42° 39′ 39.7″	9.03			O+...	luminous blue variable, V_max = 8.88^m, V_min = 9.20^m, P = 6.12 d
HD 162020				162020	87330	17^h 50^m 38.35^s	−40° 19′ 06.1″	9.12		95.94	K3V	has a brown dwarf companion
GSC 06214-00210						16^h 21^m 55^s	−20° 43′ 07″	9.15		473	M1	has a planet (b)
KQ Sco			KQ	328953	82498	16^h 51^m 38.55^s	−45° 25′ 36.1″	9.33		1120	K7	classical Cepheid, V_max = 9.33^m, V_min = 10.26^m, P = 28.71 d
HD 318107			V970	318107		17^h 39^m 41.26^s	−32° 17′ 57.4″	9.34			B8	α² CVn variable
WR 86			V1035	156327	84655	17^h 18^m 23.06^s	−34° 24′ 30.6″	9.35		1770	WC7+B0III	β Cep variable, ΔV = 0.017^m, P = 0.15 d
CD -35 11760			V1037	320156		17^h 37^m 58.50^s	−35° 23′ 04.32″	9.83			B4Ibe	PV Tel variable, V_max = 9.62^m, V_min = 9.83^m
AI Sco			AI	320921		17^h 56^m 18.57^s	−33° 48′ 43.4″	9.98			G4	RV Tau variable, V_max = 8.88^m, V_min = 11.6^m, P = 71.9 d
Gliese 667 C				156384C		17^h 18^m 58.69^s	−34° 59′ 48.3″	10.22	11.00	23	M1.5	component of Gliese 667 system; has two planets (b) (c)
Pismis 24-1				319718		17^h 24^m 43.41^s	−34° 11′ 56.5″	10.43	−7.3	8150	O3 If*	one of the most luminous stars known
Gliese 682					86214	17^h 37^m 03.66^s	−44° 19′ 09.2″	10.95		16.557	M3.5
CD -38 10980						16^h 23^m 33.84^s	−39° 13′ 46.2″	11.03		42.89	DA2	white dwarf
Scorpius X-1			V818			16^h 19^m 55.07^s	−15° 38′ 24.8″	11.1		11000	Oev	low-mass X-ray binary
HIP 79431					79431	16^h 12^m 41.77^s	−18° 52′ 31.8″	11.34	10.47	49	M3V	Sharjah,^[9] has a planet (b)
V921 Sco			V921			16^h 59^m 06.79^s	−42° 42′ 08.6″	11.43			Bep	γ Cas variable, ΔV = 0.3^m
WASP-17						15^h 59^m 50.95^s	−28° 03′ 42.3″	11.59		1000	F4	Dìwö,^[10] has a transiting planet (b)
HK Sco			HK			16^h 54^m 41.04^s	−30° 23′ 06.7″	11.7				Z And variable, V_max = 11.7^m, V_min = 14.7^m, P = 458 d
T Sco			T			16^h 17^m 02.83^s	−22° 58′ 31.3″	12.0		32600		in Messier 80; nova, V_max = 6.8^m, V_min = <12.0^m
V866 Sco			V866			16^h 11^m 31.40^s	−18° 38′ 24.5″	12.05			K5	T Tau star, ΔV = 0.5^m, P = 6.78 d
V1094 Sco			V1094			16^h 08^m 36.18^s	−39° 23′ 02.5″	12.5			K6	young stellar object, ΔV = 0.5^m
1RXS J160929.1−210524						16^h 09^m 30.31^s	−21° 04′ 57.6″	12.97	7.17	470	K7V	has a planet (b)
IRAS 17163−3907						17^h 19^m 49.33^s	−39° 10′ 37.9″	13.1				in Fried Egg Nebula; yellow hypergiant
CL Sco			CL			16^h 54^m 51.98^s	−30° 37′ 18.2″	13.25			M4	Z And variable and re-radiating binary system, V_max = 10.8^m, V_min = 13.7^m, P = 625 d
GRO J1655-40			V1033			16^h 54^m 00.14^s	−39° 50′ 44.9″	14.2			B9V	X-ray nova containing black hole, V_max = 14^m, V_min = 17.3^m
XTE J1739-302						17^h 39^m 11.58^s	−30° 20′ 37.6″	14.8			O8.5Iab(f)	high-mass X-ray binary
OGLE-2005-BLG-390L						17^h 54^m 19^s	−30° 22′ 38″	15.7		21000	M4	has a planet (b)
Th 28			V1190			16^h 08^m 29.73^s	−39° 03′ 11.0″	16.42			K0:	T Tau star, V_max = 16.42^m, V_min = 16.93^m
MXB 1735-44			V926			17^h 38^m 58.3^s	−44° 27′ 00″	17.4				X-ray burster, ΔV = 0.2^m, P = 0.19 d
Wray 17-96						17^h 41^m 35.2^s	−30° 06′ 39.6″	17.8	−10.9	15000	B3	luminous blue variable, one of the most luminous stars known
V992 Sco			V992			17^h 07^m 17.44^s	−43° 15′ 22.0″	18.0				nova, V_max = 7.26^m, V_min = 18.0^m, P = 0.15 d
V1187 Sco			V1187			17^h 29^m 18.81^s	−31° 46′ 01.5″	18.0				nova, V_max = 9.6^m, V_min = 18^m
V1186 Sco			V1186			17^h 12^m 51.21^s	−30° 56′ 37.2″	18.0				nova, V_max = 9.7^m, V_min = <18^m
GX 349+2			V1101			17^h 05^m 44.49^s	−36° 25′ 23.1″	18.6				low-mass X-ray binary, V_max = 18.3^m, V_min = 19.3^m, P = 0.94 d
U Sco			U			16^h 22^m 30.80^s	−17° 52′ 43.2″	19.3				recurrent nova and eclipsing binary, V_max = 7.5^m, V_min = 19.3^m, P = 1.23 d
V745 Sco			V745			17^h 55^m 22.27^s	−33° 15′ 58.5″	19.3				nova and rotating ellipsoidal variable, V_max = 9.4^m, V_min = 19.3^m, P = 510 d
OGLE-2005-BLG-071L						17^h 50^m 09^s	−34° 40′ 23″	19.5		11000	M?	has a planet (b)
V1280 Sco			V1280			16^h 57^m 40.91^s	−32° 20′ 36.4″	20.0				nova, V_max = 3.78^m, V_min = <20.0^m
V1309 Sco			V1309			17^h 57^m 33.02^s	−30° 43′ 10.4″	20.4				luminous red nova, V_max = 7.9^m, V_min = 20.4^m
PSR B1620−26						16^h 23^m 38.22^s	−26° 31′ 53.8″	21.30				in Messier 4; pulsar/white dwarf binary; has a planet
MOA-2008-BLG-310L						17^h 05^m 14.53^s	−34° 46′ 41.0″	23.38		20000		has a planet (b)
FQ Sco			FQ			17^h 08^m 04.51^s	−32° 42′ 02.2″					SS Cyg variable
V455 Sco			V455			17^h 07^m 21.73^s	−34° 05′ 14.5″					Z And variable
V893 Sco			V893			16^h 15^m 15.15^s	−28° 37′ 30.1″					SU UMa variable and eclipsing binary
V1018 Sco			V1018			17^h 35^m 02.72^s	−33° 33′ 29.4″					semiregular variable
H1-36						17^h 49^m 48.22^s	−33° 01′ 27.9″				M8	in NGC 6441; symbiotic star
IGR J17252-3616						17^h 25^m 11.4^s	−36° 16′ 59″				B0-1Ia	high-mass X-ray binary
OAO 1657-415						17^h 00^m 47.9^s	−41° 40′ 23″				B3:Ia-ab...	high-mass X-ray binary
Rapid Burster						17^h 33^m 24.61^s	−33° 23′ 19.8″					low-mass X-ray binary
GX 340+0						16^h 45^m 47.7^s	−45° 36′ 40″					low-mass X-ray binary
H1743-322						17^h 46^m 15.61^s	−32° 14′ 00.6″					low-mass X-ray binary
OAO 1657-415						17^h 00^m 48.884^s	−41° 39′ 21.46″			23200	Ofpe/WN9 + Q	high-mass X-ray binary
IGR J17091-3624						17^h 09^m 08^s	−36° 22′ 24″				B9V	low-mass X-ray binary containing black hole
4U 1702-42						17^h 06^m 15.31^s	−43° 02′ 08.7″					low-mass X-ray binary
4U 1705-44						17^h 08^m 54.47^s	−44° 06′ 07.4″					low-mass X-ray binary
4U 1722-307						17^h 27^m 33.25^s	−30° 48′ 07.4″					in Terzan 2; low-mass X-ray binary
4U 1728-34						17^h 31^m 57.73^s	−33° 50′ 02.5″					low-mass X-ray binary
4U 1746-371						17^h 50^m 12.66^s	−37° 03′ 08.2″					in NGC 6441; low-mass X-ray binary
XTE J1751-305						17^h 51^m 13.49^s	−30° 37′ 23.4″					low-mass X-ray binary
XTE J1720-318			V1228			17^h 19^m 58.99^s	−31° 45′ 01.3″					X-ray nova
GCRT J1745−3009						17^h 45^m 05^s	−30° 09′ 54″				B9V	radio source; possible pulsar
OGLE-2007-BLG-368L						17^h 56^m 25.96^s	−32° 14′ 14.7″			19230	late K?	has a planet (b)
UScoCTIO 108						16^h 05^m 53.94^s	−18° 18′ 42.7″				M7	has a low-mass companion
PSR B1706−44						17^h 09^m 42.73^s	−44° 29′ 08.2″					pulsar
PSR B1737−30						17^h 40^m 33.82^s	−30° 15′ 43.5″					pulsar
PSR J1614−2230						16^h 14^m 36.51^s	−22° 30′ 31.1″					binary millisecond 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 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.]

References

ESA (1997). "The Hipparcos and Tycho Catalogues". Retrieved 2006-12-26.
Kostjuk, N. D. (2002). "HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index". Retrieved 2006-12-26.
Roman, N. G. (1987). "Identification of a Constellation from a Position". Retrieved 2006-12-26.
Gould, B. A. "Uranometria Argentina". Reprinted and updated by Pilcher, F. Archived from the original on 2012-02-27. Retrieved 2010-07-16.
"AAVSO Website". American Association of Variable Star Observers. Retrieved 9 March 2014.
"Naming Stars". Retrieved 13 December 2017.

↑ "IAU Catalog of Star Names". International Astronomical Union. Retrieved 2018-09-17.
↑ JPL Technical Memorandum 33-507, "A Reduced Star Catalog Containing 537 Named Stars", Nov. 15 1971, page 18
↑ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 10 日
↑ Meeus, Jan (2002). "Mutual occultations of planets". More Mathematical Astronomy Morsels (PDF). pp. 174–185. ISBN 0943396743.
↑ Designated Xi Telescopii by Bode, no longer in use
1 2 3 4 5 6 7 8 Designated by Johann Bode, now no longer in use
1 2 IAU-Catalog of Star Names
↑ "Madagascar". NameExoWorlds. Retrieved 2020-03-12.
↑ "United Arab Emirates". NameExoWorlds. Retrieved 2020-03-12.
↑ "Costa Rica". NameExoWorlds. Retrieved 2020-03-12.

[IAU-CSN-1] "IAU Catalog of Star Names". International Astronomical Union. Retrieved 2018-09-17.

[2] JPL Technical Memorandum 33-507, "A Reduced Star Catalog Containing 537 Named Stars", Nov. 15 1971, page 18

[3] (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 10 日

[Mus2002-4] Meeus, Jan (2002). "Mutual occultations of planets". More Mathematical Astronomy Morsels (PDF). pp. 174–185. ISBN 0943396743.

[5] Designated Xi Telescopii by Bode, no longer in use

[Bode-6] 1 2 3 4 5 6 7 8 Designated by Johann Bode, now no longer in use

[exopla.net-7] 1 2 IAU-Catalog of Star Names

[8] "Madagascar". NameExoWorlds. Retrieved 2020-03-12.

[9] "United Arab Emirates". NameExoWorlds. Retrieved 2020-03-12.

[10] "Costa Rica". NameExoWorlds. Retrieved 2020-03-12.

[1]

See also

References