// Workers AI · dad joke modeAre stars in Pavo egg-cellent? Yes, they're poultry in space.

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

Name	B	Var	HD	HIP	RA	Dec	vis. mag.	abs. mag.	Dist. (ly)	Sp. class	Notes
α Pav	α		193924	100751	20^h 25^m 38.85^s	−56° 44′ 05.6″	1.94	−1.81	183	B2IV	Peacock, Joo Tseo; suspected variable, V_max = 1.93^m, V_min = 1.96^m
β Pav	β		197051	102395	20^h 44^m 57.56^s	−66° 12′ 11.7″	3.42	0.29	137	A5IV
δ Pav	δ		190248	99240	20^h 08^m 41.86^s	−66° 10′ 45.6″	3.55	4.62	20	G5IV-Vvar	Nearby Sun-like star
η Pav	η		160635	86929	17^h 45^m 44.00^s	−64° 43′ 25.4″	3.61	−1.67	371	K1III
ε Pav	ε		188228	98495	20^h 00^m 35.39^s	−72° 54′ 36.7″	3.97	1.41	106	A0V	suspected variable, V_max = 3.93^m, V_min = 3.97^m
ζ Pav	ζ		171759	91792	18^h 43^m 02.13^s	−71° 25′ 39.8″	4.01	−0.03	210	K2III
γ Pav	γ		203608	105858	21^h 26^m 26.49^s	−65° 22′ 05.3″	4.21	4.39	30	F6V	suspected variable, V_max = 4.17^m, V_min = 4.30^m
λ Pav	λ		173948	92609	18^h 52^m 13.04^s	−62° 11′ 15.2″	4.22	−4.50	1811	B2II-III	γ Cas variable, V_max = 4^m, V_min = 4.26^m
π Pav	π		165040	88866	18^h 08^m 34.79^s	−63° 40′ 05.0″	4.33	1.19	138	Am
ξ Pav	ξ		168339	90098	18^h 23^m 13.62^s	−61° 29′ 38.1″	4.35	−1.20	420	M1III SB
κ Pav	κ		174694	93015	18^h 56^m 57.04^s	−67° 14′ 00.7″	4.40	−1.71	543	F5Ib-II:	W Vir variable, V_max = 3.91^m, V_min = 4.78^m, P = 9.083 d
ν Pav	ν		169978	90797	18^h 31^m 22.43^s	−62° 16′ 41.5″	4.63	−1.20	479	B8III	53 Per variable, V_max = 4.60^m, V_min = 4.64^m, P = 0.85584 d
φ¹ Pav	φ¹		195627	101612	20^h 35^m 34.77^s	−60° 34′ 52.7″	4.75	2.55	90	F1III
HD 172555			172555	92024	18^h 45^m 26.86^s	−64° 52′ 15.2″	4.78	2.45	95	A7V
ρ Pav	ρ		195961	101773	20^h 37^m 35.24^s	−61° 31′ 47.1″	4.85	0.98	195	Fm...	δ Sct variable, ΔV = 0.055^m, P = 0.1141 d
NU Pav	(λ²)^[a]^[b]	NU	189124	98608	20^h 01^m 44.72^s	−59° 22′ 33.0″	4.95	−0.67	434	M6III	semiregular variable, V_max = 4.91^m, V_min = 5.26^m, P = 60 d
ο Pav	ο		201371	104755	21^h 13^m 20.44^s	−70° 07′ 34.4″	5.06	−2.12	888	M2III	semiregular variable, V_max = 5.00^m, V_min = 5.10^m, P = 228.3 d
φ² Pav	φ²		196378	101983	20^h 40^m 02.27^s	−60° 32′ 51.0″	5.11	3.19	79	F8V
ω Pav	ω^[c]		175329	93163	18^h 58^m 36.59^s	−60° 12′ 02.3″	5.14	−0.86	516	K1III-IV	suspected variable
υ Pav	υ		196519	102157	20^h 41^m 57.06^s	−66° 45′ 38.3″	5.14	−1.92	840	B8Vvar
HD 188162			188162	98174	19^h 57^m 06.28^s	−58° 54′ 04.7″	5.24	0.41	302	B9.5IV
HD 177389			177389	94150	19^h 09^m 52.62^s	−68° 25′ 27.6″	5.31	2.48	120	G8/K0III/IV
μ² Pav	μ²		188887	98624	20^h 01^m 52.40^s	−66° 56′ 37.7″	5.32	1.04	234	K2IVCN...
HD 186219			186219	97534	19^h 49^m 25.29^s	−72° 30′ 12.3″	5.39	2.30	135	A4III
HD 186957	(λ¹)^[a]^[d]		186957	97646	19^h 50^m 44.78^s	−59° 11′ 37.1″	5.41	0.90	260	A0IV
σ Pav	σ		197635	102773	20^h 49^m 18.28^s	−68° 46′ 35.0″	5.41	0.56	305	K0III
ι Pav	ι		165499	89042	18^h 10^m 26.26^s	−62° 00′ 10.0″	5.47	4.22	58	G0V
SX Pav		SX	203881	106044	21^h 28^m 44.79^s	−69° 30′ 19.0″	5.47	0.05	396	M5III	semiregular variable, V_max = 5.18^m, V_min = 5.99^m, P = 50.87 d
HD 179366			179366	94789	19^h 17^m 12.22^s	−66° 39′ 39.7″	5.52	0.73	296	A4IV/V
HD 166599			166599	89487	18^h 15^m 40.66^s	−63° 03′ 19.1″	5.58	0.79	296	K0III/IV
HD 198160			198160	102962	20^h 51^m 38.40^s	−62° 25′ 45.2″	5.67	1.35	238	A2
HD 200525			200525	104440	21^h 09^m 21.52^s	−73° 10′ 20.2″	5.67	4.31	61	G3IV
θ Pav	θ		173168	92294	18^h 48^m 37.96^s	−65° 04′ 39.0″	5.71	1.51	226	A9V
HD 169836			169836	90664	18^h 29^m 56.68^s	−57° 31′ 23.1″	5.74	0.54	357	K0III
HD 188097			188097	98332	19^h 58^m 41.18^s	−69° 09′ 49.4″	5.74	1.48	232	Am
μ¹ Pav	μ¹		188584	98478	20^h 00^m 23.11^s	−66° 56′ 56.0″	5.75	1.64	216	K0IV
HD 200751			200751	104364	21^h 08^m 32.71^s	−63° 55′ 41.8″	5.75	−0.13	489	K0III
HD 172211			172211	91854	18^h 43^m 37.32^s	−64° 33′ 04.7″	5.76	0.26	410	K0III
HD 161814			161814	87393	17^h 51^m 35.47^s	−60° 09′ 50.5″	5.78	0.50	371	K0III
HD 169570			169570	90930	18^h 32^m 55.33^s	−73° 57′ 55.4″	5.88	0.69	356	K0III
HD 175986			175986	93574	19^h 03^m 29.68^s	−68° 45′ 19.9″	5.89	2.12	185	F8V
HD 160720			160720	86871	17^h 44^m 55.84^s	−57° 32′ 43.8″	5.97	0.49	406	G8III
HD 175401			175401	93287	19^h 00^m 03.55^s	−66° 39′ 12.7″	5.98	0.33	439	K0III
HD 182709			182709	95999	19^h 31^m 10.94^s	−68° 26′ 02.0″	5.98	−1.54	1042	K4/K5III	suspected variable
HD 172630			172630	92008	18^h 45^m 11.50^s	−61° 05′ 42.5″	6.04	−1.47	1035	K3III
HD 172881			172881	92394	18^h 49^m 43.68^s	−72° 59′ 44.6″	6.04	−0.73	736	B9.5IV/V
NZ Pav		NZ	186786	97674	19^h 51^m 01.09^s	−65° 36′ 16.9″	6.04	2.15	196	F2III-IV	δ Sct variable, ΔV = 0.017^m, P = 0.08 d
HD 189567			189567	98959	20^h 05^m 31.49^s	−67° 19′ 09.3″	6.07	4.83	58	G2V	has a planet (b)
HD 184996			184996	96882	19^h 41^m 37.24^s	−65° 51′ 15.3″	6.08	−0.74	753	M0III
HD 191603			191603	99762	20^h 14^m 26.96^s	−63° 24′ 57.1″	6.09	1.80	235	F0IV
HD 195402			195402	101626	20^h 35^m 51.67^s	−69° 36′ 37.7″	6.09	−0.94	830	K2III
HD 203212			203212	105768	21^h 25^m 18.01^s	−71° 47′ 56.7″	6.09	0.03	531	K2III
HD 168740		V346	168740	90304	18^h 25^m 31.63^s	−63° 01′ 16.6″	6.13	1.87	232	A3V	δ Sct variable
HD 167425			167425	89805	18^h 19^m 40.08^s	−63° 53′ 09.2″	6.17	4.37	75	F9V
HD 200924			200924	104597	21^h 11^m 20.87^s	−72° 32′ 39.4″	6.18	0.79	390	K1III
HD 184585			184585	96607	19^h 38^m 25.92^s	−57° 58′ 59.5″	6.19	0.34	482	K0III
HD 186837			186837	97611	19^h 50^m 21.75^s	−61° 03′ 40.1″	6.21	−0.99	898	B5V
HD 187653			187653	97971	19^h 54^m 40.45^s	−61° 10′ 14.9″	6.21	1.36	304	A3V
HD 172781			172781	92021	18^h 45^m 23.93^s	−56° 52′ 54.9″	6.22	−0.39	685	K3III
HD 196317			196317	101965	20^h 39^m 51.72^s	−62° 54′ 27.4″	6.22	0.64	426	K1III
τ Pav	τ		179009	94724	19^h 16^m 28.60^s	−69° 11′ 26.7″	6.25	−0.14	619	A6IV/V
HD 192531			192531	100165	20^h 19^m 03.01^s	−63° 13′ 50.0″	6.27	0.59	445	K0III
Y Pav		Y	203133	105678	21^h 24^m 16.73^s	−69° 44′ 01.9″	6.28	−1.52	1181	C5II	semiregular variable, V_max = 5.79^m, V_min = 6.90^m, P = 449 d
HD 176522			176522	93629	19^h 04^m 01.00^s	−57° 57′ 35.9″	6.30	0.11	565	G6II/III
HD 166841			166841	89674	18^h 18^m 00.96^s	−68° 13′ 45.2″	6.32	−0.33	697	B9V
HD 202299			202299	105148	21^h 18^m 00.47^s	−64° 40′ 53.4″	6.32	0.18	552	B8V	suspected variable, V_max = 6.30^m, V_min = 6.33^m
HD 181019			181019	95369	19^h 24^m 05.51^s	−68° 22′ 15.9″	6.33	−0.25	676	K2III
HD 195772			195772	101684	20^h 36^m 38.33^s	−63° 07′ 14.8″	6.34	2.50	191	F2V
HD 172021			172021	91733	18^h 42^m 22.63^s	−64° 38′ 34.7″	6.35	−0.51	767	A5V
HD 162521			162521	87822	17^h 56^m 24.18^s	−65° 43′ 15.5″	6.36	3.67	113	F8V
HD 191095			191095	99453	20^h 11^m 07.41^s	−57° 31′ 27.0″	6.36	0.65	452	A1V	variable star
HD 199475			199475	103752	21^h 01^m 28.03^s	−68° 12′ 34.6″	6.36	1.76	272	A2V
HD 184586			184586	96734	19^h 39^m 52.13^s	−66° 41′ 07.5″	6.37	1.31	335	A0Vn
HD 165497			165497	89006	18^h 09^m 57.59^s	−59° 02′ 24.6″	6.38	−0.09	642	K4III
HD 188164			188164	98346	19^h 58^m 52.93^s	−68° 45′ 44.7″	6.38	1.28	341	A2V
HD 164871			164871	88815	18^h 07^m 48.37^s	−64° 33′ 00.1″	6.40	0.32	535	K2/K3III
HD 170525			170525	90981	18^h 33^m 29.44^s	−58° 42′ 30.7″	6.40	2.89	164	G5IV
HD 161475			161475	87264	17^h 49^m 53.01^s	−61° 42′ 52.8″	6.41	−0.22	689	B9IV
HD 195190			195190	101570	20^h 35^m 06.34^s	−71° 11′ 19.7″	6.41	−0.55	805	K2III
HD 179419			179419	94770	19^h 17^m 00.53^s	−65° 13′ 39.5″	6.42	−0.24	700	B8/B9V
HD 186584			186584	97569	19^h 49^m 53.42^s	−66° 48′ 47.1″	6.44	−1.15	1076	K4III
HD 190222			190222	99200	20^h 08^m 20.48^s	−66° 21′ 16.8″	6.45	−1.28	1144	K5III
HD 166251			166251	89370	18^h 14^m 16.36^s	−63° 41′ 22.3″	6.47	0.10	614	K4III
HD 174877	χ^[e]^[f]		174877	93012	18^h 56^m 54.70^s	−62° 48′ 06.9″	6.47	−1.24	1136	K3III
HD 161955			161955	87564	17^h 53^m 18.22^s	−65° 29′ 18.4″	6.48	0.47	519	K0/K1III
HD 175007			175007	93238	18^h 59^m 29.27^s	−70° 28′ 06.1″	6.49	1.33	351	A8V
HD 192887			192887	100379	20^h 21^m 28.46^s	−66° 44′ 58.9″	6.49	3.27	143	F6V
V Pav		V	160435	86728	17^h 43^m 18.94^s	−57° 43′ 26.3″	6.84		1210	C+	semiregular variable, V_max = 6.3^m, V_min = 7.17^m, P = 226.1 d
HD 164427			164427	88531	18^h 04^m 42.60^s	−59° 12′ 34.5″	6.84		123.9	G0+V	has a low-mass companion
HD 179140	(ψ)^[g]		179140	94570	19^h 14^m 47.46^s	―58° 00′ 24.2″	7.23		172	G2V
AR Pav		AR		89886	18^h 20^m 27.88^s	−66° 04′ 42.9″	7.40		2300	B1	Z And and Algol variable, V_max = 7.40^m, V_min = 13.620^m, P = 604.6 d
R Pav		R	165961	89258	18^h 12^m 52.95^s	−63° 36′ 57.3″	7.50		1100	M4.5e	Mira variable, V_max = 6.86^m, V_min = 14.0^m, P = 234 d
HD 196050			196050	101806	20^h 37^m 51.71^s	−60° 38′ 04.1″	7.6	4.2	153	G3V	has a planet (b)
KZ Pav		KZ	199005	103542	20^h 58^m 40.10^s	−70° 25′ 19.8″	7.71		434	F6V	Algol variable, V_max = 7.71^m, V_min = 9.3^m, P = 0.9498768 d
HD 175167			175167	93281	19^h 00^m 00.84^s	−69° 56′ 39.3″	8.00	3.87	219	G5IV/V	has a planet (b)
HD 181433			181433	95467	19^h 25^m 09.57^s	−66° 28′ 07.7″	8.38	6.24	87	K5V	has three planets (b, c & d)
HD 175607			175607	93373	19^h 01^m 05.0^s	−66° 11′ 34″	8.6		148	G6V	has two planets (b &c)
HD 190984			190984	99496	20^h 11^m 30.72^s	−64° 37′ 13.7″	8.73	2.34	618	F8V	has a planet (b)
MW Pav		MW	197070	102508	20^h 46^m 27.75^s	−71° 56′ 58.5″	8.79		682	F3IV/V	W UMa variable, V_max = 8.51^m, V_min = 8.95^m, P = 0.794994 d
X Pav		X	191155 191171	99512	20^h 11^m 45.86^s	−59° 56′ 12.8″	9.20		2190	M6/M7III:p	semiregular variable
Gliese 693				86990	17^h 46^m 34.23^s	−57° 18′ 08.6″	10.78		19.011	M2.0	suspected variable
V347 Pav		V347			18^h 44^m 48.25^s	−74° 18′ 34.2″	14.85			CV	AM Her variable, V_max = 14.85^m, V_min = 16.67^m, P = 0.062553 d
SCR 1845-6357					18^h 45^m 05.42^s	−63° 57′ 47.6″	17.40		12.565	M8.5	has a planet or brown dwarf companion
BD Pav		BD			18^h 43^m 11.92^s	−57° 30′ 44.9″					U Gem and W UMa variable
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

1 2 In Bode's Uranographia
↑ This is Lacaille's Lambda² Indi. It was included in Pavo and it's no longer used.
↑ Also labelled Omega Telescopii (ω Tel/ω Telescopii) by Bode in his Uranographia
↑ This is Lacaille's Lambda¹ Indi. It was included in Pavo and it's no longer used.
↑ In Bode’s Uranographia
↑ This designation was dropped by Benjamin Gould
↑ Labelled Psi Telescopii (ψ Tel/ψ Telescopii) by Bode ion his Uranographia

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.

[Bode-1] 1 2 In Bode's Uranographia

[2] This is Lacaille's Lambda² Indi. It was included in Pavo and it's no longer used.

[3] Also labelled Omega Telescopii (ω Tel/ω Telescopii) by Bode in his Uranographia

[4] This is Lacaille's Lambda¹ Indi. It was included in Pavo and it's no longer used.

[5] In Bode’s Uranographia

[6] This designation was dropped by Benjamin Gould

[7] Labelled Psi Telescopii (ψ Tel/ψ Telescopii) by Bode ion his Uranographia

[a]

[b]

[c]

[d]

[e]

[f]

[g]

See also

References