List of stars in Vela - 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....

Vela
Vela (constellation)
Vela is a constellation in the southern sky. Its name is Latin for the sails of a ship, and it was originally part of a larger constellation, the ship Argo Navis, which was later divided into three parts, the others being Carina and Puppis.-Stars:...

, sorted by decreasing brightness.

This constellation's Bayer designation

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...

s (Greek-letter star names) were given while it was still considered part of the constellation of Argo Navis

Argo Navis

Argo Navis was a large constellation in the southern sky that has since been divided into three constellations. It represented the Argo, the ship used by Jason and the Argonauts in Greek mythology...

. After Argo Navis was broken up into Carina

Carina (constellation)

Carina is a constellation in the southern sky. Its name is Latin for the keel of a ship, and it was formerly part of the larger constellation of Argo Navis until that constellation was divided in three.-Stars:...

, Vela, and Puppis

Puppis

Puppis is a constellation in the southern sky. Its name is the Latin word for the poop deck of a ship, and Puppis represents the deck of the ship and its deckhouses...

, these Greek-letter designations were kept, so that Vela does not have a full complement of Greek-letter designations. For example, since Argo Navis's alpha star went to Carina, there is no Alpha Velorum.

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...	G. Gould designation Gould designations for stars are similar to Flamsteed designations in the way that they number stars within a constellation in increasing order of right ascension. Each star is assigned an integer , followed by " G. " , and then 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
γ² Vel Gamma Velorum Gamma Velorum is a star system in the constellation Vela. At magnitude +1.7, it is one of the brightest stars in the night sky. It has the traditional names Suhail and Suhail al Muhlif, which confusingly also apply to Lambda Velorum...	γ²	9	68273	39953	1.75	−5.31	840	WC8 + O9I	Regor, Suhail, Suhail al Muhlif, Muliphein; double star 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... , Wolf-Rayet star Wolf-Rayet star Wolf–Rayet stars are evolved, massive stars , which are losing mass rapidly by means of a very strong stellar wind, with speeds up to 2000 km/s...
δ Vel Delta Velorum Delta Velorum is a star system in the constellation Vela. It is approximately 79.7 light years from Earth. It is sometimes given the name Koo She, Chinese for 'Bow and Arrows', along with ω Velorum and stars in Canis Major....	δ	65	74956	42913	1.93	−0.01	80	A1V	Koo She; quadruple 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... ; Algol variable Algol variable Algol variables or Algol-type binaries are a class of eclipsing binary stars where the orbital plane of the stars are coincident with the line of sight from Earth. When the cooler component passes in front of the hotter one, part of the latter's light is blocked, and the total brightness of the...
λ Vel Lambda Velorum Lambda Velorum is a star in the constellation Vela. It has the traditional name Suhail .Lambda Velorum is a supergiant or bright giant star of spectral class K5...	λ	100	78647	44816	2.23	−3.99	573	K4Ib-II	Suhail, Suhail al Muhlif, Al Suhail, Alsuhail, Suhail Alwazn, Muliphein
κ Vel Kappa Velorum Kappa Velorum is a binary star in the constellation Vela. It also has the traditional name Markab, often spelled Markeb to distinguish it from similarly named stars such as Alpha Pegasi....	κ	129	81188	45941	2.47	−3.62	539	B2IV	Markab
μ Vel Mu Velorum Mu Velorum is a binary star in the constellation Vela. It is approximately 116 light years from Earth. Mu Velorum is approximately 38 solar diameters, almost as big as Aldebaran....	μ	229	93497	52727	2.69	−0.06	116	G5III SB	Peregrini, Alherem, Al Haram
N Vel HD 82668 N Velorum is a 3rd-magunitude star on the border between the constellations Carina and Vela. It is an orange K-type giant. It is approximately 250 light years from the Earth.The star should not be confused with n Velorum....	N	144	82668	46701	3.16	−1.15	238	K5III	Marut
φ Vel Phi Velorum Phi Velorum is a star in the constellation Vela. It has the traditional name Tseen Ke, from Chinese 天紀 "star chart". ....	φ	171	86440	48774	3.52	−5.34	1929	B5Ib	Tseen Ke
ο Vel Omicron Velorum Omicron Velorum is a star in the constellation Vela.Omicron Velorum is a blue-white B-type subgiant with a mean apparent magnitude of +3.60. It is approximately 495 light years from Earth. It is a variable star and its brightness varies from magnitude +3.55 to +3.67 with a period of 2.78 days....	ο	56	74195	42536	3.60	−2.31	495	B3IV	Xestus
ψ Vel Psi Velorum Psi Velorum is a binary star in the constellation Vela. It is approximately 60.5 light years from Earth, making it the nearest star of the constellation....	ψ	140	82434	46651	3.60	2.26	60	F2IV
c Vel HD 78004 HD 78004 is a star in the constellation Vela.HD 78004 is an orange K-type giant with an apparent magnitude of +3.75. It is approximately 309 light years from Earth.The star should not be confused with C Velorum....	c	97	78004	44511	3.75	−1.13	309	K2III
b Vel B Velorum (supergiant) b Velorum is a binary star in the constellation Vela. It is approximately 3100 light years from Earth.The primary component, b Velorum A, is a yellow-white F-type supergiant with a mean apparent magnitude of +3.77. It is classified as an irregular variable star and its brightness varies from...	b	53	74180	42570	3.77	−6.12	3105	F3Ia
p Vel P Velorum p Velorum is a triple star system in the constellation Vela. It is approximately 86.5 light years from Earth.The primary component, p Velorum A, is a yellow-white F-type subgiant with an apparent magnitude of +4.5. It is a spectroscopic binary whose components have an orbital period of 10.21 days...	p	222	92139	51986	3.84	1.72	86	A3m+...
q Vel Q Velorum (dwarf star) q Velorum is a star in the constellation Vela.q Velorum is a white A-type main sequence dwarf with an apparent magnitude of +3.85. It is approximately 103 light years from Earth....	q	191	88955	50191	3.85	1.36	103	A2V
a Vel HD 75063 HD 75063 is a star in the constellation Vela.HD 75063 is a white A-type giant with an apparent magnitude of +3.87. It is approximately 1500 light years from Earth....	a	66	75063	43023	3.87	−4.52	1552	A1III
d Vel	d	64	74772	42884	4.05	−0.18	228	G5III
e Vel	e	48	73634	42312	4.11	−4.11	1436	A6II
γ¹ Vel Gamma Velorum Gamma Velorum is a star system in the constellation Vela. At magnitude +1.7, it is one of the brightest stars in the night sky. It has the traditional names Suhail and Suhail al Muhlif, which confusingly also apply to Lambda Velorum...	γ¹	8	68243		4.27				component of the γ Vel system
x Vel	x	225	92449	52154	4.29	−2.92	901	G2II
M Vel	M	148	83446	47175	4.34	1.75	107	A5V
i Vel	i	239	95370	53773	4.37	0.39	204	A3IV
w Vel	w	91	77258	44191	4.45	0.50	201	Fp
J Vel	J	203	89890	50676	4.50	−3.65	1393	B3III	MV Vel; Be star Be star A Be star is a B-type star with prominent emission lines of hydrogen in its spectrum. The designation is combined by the spectral class, B, and the lowercase e denoting emission in the spectral classification system. Line emission from other atomic ions might be present as well, but is typically...
m Vel	m	163	85622	48374	4.58	−3.03	1083	G5Ib
GZ Vel		201	89682	50555	4.59	−3.71	1489	K3II
k Vel	k	117	79940	45448	4.63	1.10	166	F3/F5V
H Vel	H	88	76805	43878	4.68	−0.63	376	B5V
n Vel HD 74272 HD 74272 is a star in the constellation Vela.HD 74272 is a white A-type bright giant with an apparent magnitude of +4.74. It is approximately 2500 light years from Earth.The star should not be confused with N Velorum....	n	58	74272	42624	4.74	−4.08	1895	A5II
B Vel B Velorum B Velorum is a binary star in the constellation Vela. It is approximately 1510 light years from Earth.The primary component, B Velorum A, is a blue-white B-type main sequence dwarf with an apparent magnitude of +4.79. Its companion, the magnitude +6.3 B Velorum B, is 0.8 arcseconds away....	B	26	70930	41039	4.79	−3.54	1509	B1V
r Vel	r	204	89998	50799	4.82	0.88	200	K1IIIvar
HY Vel		62	74560	42726	4.83	−1.01	479	B3IV
Q Vel Q Velorum Q Velorum is a star in the constellation Vela.Q Velorum is a blue-white B-type subgiant with an apparent magnitude of +4.85. It is approximately 1080 light years from Earth....	Q	186	88206	49712	4.85	−2.76	1083	B3IV
Y Vel	Y	215	91324	51523	4.89	3.19	71	F6V
l Vel	l	115	79917	45439	4.92	0.73	225	K1III
g Vel G Velorum g Velorum is an A-type giant star in the constellation of Vela. It has an apparent visual magnitude of approximately 4.943....	g	76	75710	43347	4.94	−2.08	827	A2III
GX Vel		103	79186	45085	4.99			B5Ia	α Cyg variable Alpha Cygni variable Alpha Cygni variables are variable stars which exhibit non-radial pulsations, meaning that some portions of the stellar surface are contracting at the same time others parts expand. They are supergiant stars of spectral types B or A...
C Vel HD 73155 HD 73155 is a star in the constellation Vela.HD 73155 is an orange K-type bright giant with an apparent magnitude of +5.01. It is approximately 850 light years from Earth.The star should not be confused with c Velorum....	C	46	73155	42088	5.01	−2.14	876	K1/K2II
L Vel	L	146	83058	46950	5.01	−2.27	931	B1.5IV
t Vel	t	219	91504	51635	5.02	−2.34	964	K4III
		34	72127	41639	5.03	−6.61	6936	B+...
		3	67582	39690	5.04	−2.86	1240	K3III
		182	87783	49485	5.06	0.57	258	K0IV
F Vel	F	30	71935	41483	5.08	1.10	204	A9/F0III/IV
f Vel	f	78	75821	43413	5.09	−4.50	2694	B0III	KX Vel; spectroscopic binary
I Vel	I	136	81848	46283	5.09	−0.47	422	B6V
u Vel	u	160	85355	48224	5.09	−2.01	856	B7III
		118	80108	45505	5.12	−5.34	4025	K3Ib
		145	82984	46914	5.12	−2.22	959	B4IV
NO Vel		15	69144	40285	5.14	−2.23	970	B2.5IV	β Lyr variable 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...
		230	93563	52742	5.14	−0.99	548	B8/B9III
D Vel	D	63	74753	42834	5.15	−3.19	1516	B0IIIn
FZ Vel		90	77140	44093	5.17	1.02	221	Am	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...
		28	71510	41296	5.18	−1.40	674	B2V
NZ Vel		54	74146	42504	5.18	−0.41	428	B4IV
		7	68217	39961	5.20	−2.51	1136	B2IV-V
NY Vel		50	74067	42540	5.20	0.53	280	Ap (SiCr)	α² CVn variable
LN Vel		59	74371	42679	5.20	−4.39	2694	B5Iab	α Cyg variable
IS Vel		10	68324	39970	5.23	−2.02	921	B1IVe	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...
OY Vel		94	77653	44337	5.23	−0.41	437	Ap Si	α² CVn variable
z Vel	z	112	79735	45344	5.24	−0.92	556	B4V+...
		114	79846	45328	5.26	−1.20	638	G8II/III
K Vel	K	122	80456	45631	5.26	−0.34	431	B7/B8III
LW Vel		189	88824	50070	5.27	1.78	163	A7V	δ Sct variable
		84	76360	43671	5.31	0.79	261	Am
		120	80170	45544	5.31	0.12	355	K2III
A Vel HD 72108 HD 72108 is a star system in the constellation Vela. It is approximately 1640 light years from Earth.The primary component, HD 72108 A, is a blue-white B-type subgiant with an apparent magnitude of +5.33. It is a spectroscopic binary, whose components are separated by 0.176 arcseconds...	A	33	72108	41616	5.33	−3.18	1638	B2IV
		143	82694	46811	5.35	−0.04	390	G8III
OP Vel		68	75149	43082	5.43	−4.59	3293	B3Ia	α Cyg variable
		150	83520	47204	5.44	1.16	234	A2/A3V
HW Vel		51	74071	42459	5.45	−0.25	451	B5V	β Cep variable
		141	82419	46594	5.45	−0.08	415	B8V
h Vel	h	74	75630	43325	5.47	−2.97	1590	A2/A3IV
HX Vel		60	74455	42712	5.48	−3.09	1689	B1.5Vn
KT Vel		61	74535	42715	5.49	−0.36	483	B8...	α² CVn variable
y Vel	y	151	83548	47267	5.51	−0.35	484	G8II
16 G. Vel		16	69194	40282	5.52	−1.30	753	M1III
		55	74196	42535	5.56	−0.24	472	B7Vn
IZ Vel		93	77475	44299	5.56	−0.24	471	B5V
KL Vel		106	79416	45189	5.56	−0.85	623	B8V	α² CVn variable
		126	81034	45924	5.56	−0.63	565	M3Ib
O Vel	O	154	84461	47717	5.56	0.38	355	A0V
		157	84816	47963	5.58	−2.64	1436	B2.5IV
		209	90677	51140	5.58	−2.87	1598	K3II/III
		193	89062	50241	5.59	−0.52	544	K4III
		128	81157	45920	5.61	0.98	275	A3IVs...
		162	85563	48348	5.62	0.56	335	K2III
NN Vel		6	68161	39919	5.66	−1.47	869	B8Ib/II	α Cyg variable
		202	89736	50609	5.66	−3.93	2694	K5/M0III
		52	74167	42564	5.67	−1.65	950	M0III
		247	96113	54137	5.67	1.01	279	A8III/IV
		39	72737	41861	5.68	−1.56	913	G8III+...
		87	76653	43797	5.70	3.79	79	F6V
		69	75276	43148	5.71	−4.52	3622	F0Ib
		167	86087	48613	5.71	0.76	319	A0V
		161	85483	48287	5.72	−0.59	597	K0IIICN...
		166	85980	48561	5.72	−1.35	845	B+...
		127	81136	45962	5.74	−0.47	570	G6/G8III
s Vel	s	217	91355	51561	5.76	0.00	463	B9
AH Vel		13	68808	40155	5.77	−2.49	1462	F7p	variable star 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... ; δ Cep variable
		105	79275	45122	5.78	−1.95	1144	B2IV-V
		190	88842	50078	5.78	0.83	318	A3IV/V
E Vel	E	47	73340	42177	5.79	0.01	466	B8 Si	HV Vel; α² CVn variable
		81	76110	43603	5.79	−1.36	876	K5/M0III
		199	89569	50493	5.80	3.03	117	F6V
		238	95347	53762	5.81	1.07	290	B8/B9V
		32	72067	41621	5.82	−2.63	1598	B2V
		12	68657	40077	5.83	−0.91	728	B3V
LR Vel		123	80558	45675	5.83	−8.02	19176	B7Iab	α Cyg variable
		111	79694	45314	5.85	−0.17	521	B6IV
k¹ Vel	k¹	113	79807	45386	5.85	−0.57	627	K0/K1III+..
		17	69302	40357	5.86	−1.35	903	B2IV-V
		89	77020	44024	5.88	−1.71	1072	G8/K0II
		27	71043	41081	5.89	1.57	238	A0V
		57	74273	42614	5.90	−2.56	1606	B1.5V
IW Vel		237	94985	53530	5.90	0.96	317	A7Vni	δ Sct variable
		218	91437	51610	5.91	0.48	397	G6/G8III
		42	72832	42001	5.92	−1.10	825	B5III
		82	76161	43589	5.92	−1.69	1087	B3Vn
		110	79621	45270	5.92	−0.23	554	B9V
V335 Vel		165	85953	48527	5.95	−2.64	1707	B2V
		1	67249	39527	5.96	−2.14	1358	G5II
		198	89461	50480	5.97	−0.17	551	B9V
		35	72232	41674	5.98	−0.45	629	B7IV
		187	88399	49844	5.98	1.81	223	K3III
		152	84228	47559	5.99	−3.60	2694	B4V
		14	68895	40183	6.00	−0.68	706	B5V
		77	75759	43392	6.00	−2.84	1906	O9V
		119	80057	45481	6.02	−4.60	4347	A1Ib+...
IU Vel		92	77320	44213	6.04	−1.39	1000	B3Vne	γ Cas variable
		124	80774	45814	6.04	0.05	513	K3/K4III
		216	91356	51560	6.04	0.21	477	B4
		29	71722	41373	6.05	1.79	232	A0V
		104	79241	45127	6.05	−1.92	1278	B5III
		134	81471	46093	6.05	−5.17	5719	A7Iab
		133	81411	46114	6.05	0.04	518	A6/A7III
		159	85250	48119	6.05	1.01	332	K0III
		173	86523	48835	6.06	−4.27	3791	B3V
KQ Vel		235	94660	53379	6.08	0.17	495	A0p...	α² CVn variable
		221	91805	51816	6.09	−1.12	901	G8/K0II/III
		99	78548	44708	6.10	−1.70	1185	B2IV-V
		211	90798	51245	6.10	−1.15	921	K4III
		224	92328	52112	6.10	−0.11	569	Am+...
		178	87363	49259	6.11	1.29	300	A0V
		248	96224	54185	6.11	0.12	514	B9V
IV Vel		172	86466	48799	6.13	−3.98	3432	B3IV	β Cep variable
		208	90518	51077	6.13	1.09	332	K1III
IP Vel		153	84400	47694	6.15	−1.96	1364	B6V	eclipsing binary
		240	95429	53771	6.15	2.26	195	A3III/IV
		188	88693	49994	6.16	1.11	334	K2IIICN...
		194	89104	50232	6.16	−2.04	1424	B2IV-V
MX Vel		2	67341	39584	6.18	−2.68	1929	B3Vnp	Be star
IM Vel		147	83368	47145	6.18	1.88	236	F0p	α² CVn variable
		149	83465	47172	6.18	0.80	388	K1III
		206	90393	51014	6.18	−0.09	586	G8III
		102	79091	45002	6.19	1.34	304	K1III
		135	81780	46297	6.19	1.37	300	A7III
		177	87152	49137	6.20	−2.03	1442	B2.5V
		196	89273	50332	6.20	−0.46	700	M4/M5III
		67	75081	43073	6.21	−0.51	720	B9V
		132	81369	46067	6.21	−1.49	1128	B7III
		180	87652	49394	6.23	0.17	532	B8/B9III
		205	90170	50903	6.24	1.98	232	K0IV
		43	72900	41986	6.25	−2.66	1976	K3III
			77580	44367	6.25	1.05	357	K1IIICN...
		116	79900	45413	6.25	−2.47	1811	B8V
IY Vel		85	76566	43807	6.26	−1.03	934	B3IV
		109	79524	45242	6.27	0.48	469	K2III
		131	81347	46045	6.27	−1.88	1393	B5V
		44	72993	42070	6.28	−1.13	988	M0III
		125	80781	45742	6.28	−3.83	3432	B5V
		73	75466	43195	6.29	0.52	464	B8V
		228	93453	52709	6.29	1.91	245	A4IV
		36	72350	41737	6.30	−2.88	2233	B4V
		37	72436	41806	6.31	−2.09	1560	B5V
		108	79523	45259	6.31	−0.40	715	A0V
GK Vel			81575	46194	6.31	−0.61	789	M5III
		121	80435	45603	6.33	−0.65	811	K3III
		4	67621	39691	6.34	−1.78	1370	B3III
			72650	41813	6.34	0.45	491	K3III
70 G. Vel HD 75289 HD 75289 is a 6th magnitude star in the constellation of Vela. Like our Sun, it is a yellow dwarf but slightly more massive, hotter and luminous. The spectral type of the star is G0 V...		70	75289	43177	6.35	4.04	94	G0V	has a planet 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 HD 75289 b HD 75289 b is an extrasolar planet orbiting the star HD 75289 in Vela constellation. It has a minimum mass half that of Jupiter, and it orbits in a very short orbit completing one circular revolution around the star in three and a half days. By studying the starlight scientists have concluded that... )
		41	72798	41941	6.36	−3.02	2451	B5III
HZ Vel		75	75654	43354	6.38	1.92	254	A2/A3II/III	δ Sct variable
		80	76004	43520	6.38	−1.60	1283	B3V
		38	72485	41781	6.39	−1.15	1052	B2.5V
		83	76230	43593	6.39	0.67	453	A0V
		95	77907	44423	6.39	−0.72	862	B6V
			86211	48706	6.39	−0.67	840	M1III
		169	86352	48730	6.39	−4.38	4657	B2IV-V
		184	88015	49619	6.40	−1.60	1299	B3III
		236	94724	53411	6.40	1.44	320	A0V
			76304	43673	6.42	−1.61	1315	K0II/III+..
		176	87122	49092	6.42	−0.70	867	B8
		71	75387	43209	6.43	−2.15	1698	B2IV
		223	92155	51984	6.43	−2.10	1655	B3Vn
		20	69596	40433	6.44	−0.32	734	K3/K4III
			73121	42123	6.44	3.64	118	G1V
		242	95509	53811	6.44	0.92	415	K3III
		19	69404	40397	6.45	−1.60	1331	B3Vnne
		23	70309	40749	6.45	−0.56	823	B3V
		49	73952	42400	6.45	0.50	505	B8Vn
			94508	53260	6.45	−11.16	108667	K2III
		11	68478	40016	6.46	−2.03	1630	B3IV
		96	78005	44509	6.46	−1.27	1144	B4V
		130	81309	46075	6.47	1.45	329	A1m...
			68763	40160	6.48	−5.11	6792	K3III:
		40	72787	41970	6.48	−1.63	1364	B2/B3V
		101	79025	44979	6.48	0.49	513	A9Vn
			88862	50069	6.48	−0.53	821	K2III
		197	89328	50391	6.48	2.51	203	A8V+...
V361 Vel		244	95716	53940	6.48	−2.18	1762	M4III
		18	69168	40299	6.49	−0.96	1009	B3V
			71805	41426	6.49	2.82	176	F5V...
			72752	41905	6.49	−0.01	651	K2III
		79	75989	43528	6.49	−1.18	1113	Ap...
		164	85871	48469	6.50	−5.19	7087	B1V
		175	87030	49052	6.50	0.52	511	K0III
R Vel		183	87816	49477	6.50	1.09	394	K0III
HD 83443 HD 83443 HD 83443 is an orange dwarf star approximately 142 light-years away in the constellation of Vela. As of 2000, at least one extrasolar planet has been confirmed to be orbiting the star.- Planetary system :...			83443	47202	8.24	5.05	142	K0V	has a planet (b HD 83443 b HD 83443 b is an extrasolar planet approximately 142 light-years away in the constellation of Vela. It was discovered in 2000 by the Geneva Extrasolar Planet Search Team led by Michel Mayor. It has a minimum mass comparable to Saturn, and its orbit is one of the shortest known, 1/25th that of... )
HD 85390 HD 85390 HD 85390 is a main sequence star of spectral class K1 located approximately 111 light years away in the constellation Vela, appearing as 8.55 magnitude star. This star is smaller, cooler, dimmer, and less massive than our Sun. Also its metal content is seven-sixths as much as the Sun...			85390	48235	8.55	5.90	111	K1.5V	has a planet (b HD 85390 b HD 85390 b is an extrasolar planet which orbits the G-type main sequence star HD 85390, located approximately 111 light years away in the constellation Vela. This planet has at least one-seventh the mass of Jupiter and takes fifteen-sevenths years to orbit the star at a semimajor axis of 1.54 AU... )
HD 73526 HD 73526 HD 73526 is a yellow dwarf star about 323 light-years away in the constellation Vela.- Star :The star is cooler, more luminous, similar mass, and larger than our Sun...			73526	42282	9.00	4.12	309	G6V	has two planets (b HD 73526 b HD 73526 b is an extrasolar planet orbiting about 61 million miles away from its parent star. This planet is more massive than Jupiter in our solar system, so is most likely a gas giant. Based on its orbit and the stellar luminosity, the planet probably receives insolation 61% that of Mercury.... & c HD 73526 c HD 73526 c is an extrasolar planet orbiting about 97 million miles away from its parent star. Based on its mass, this planet is likely to be a gas giant. At the distance this planet orbits from its star, which is more luminous than our Sun, HD 73526 c would receive insolation 84% that of Venus.HD... )
V390 Vel					10.48		2600	F3e	very massive red giant Red giant A red giant is a luminous giant star of low or intermediate mass in a late phase of stellar evolution. The outer atmosphere is inflated and tenuous, making the radius immense and the surface temperature low, somewhere from 5,000 K and lower...
WASP-19 WASP-19 WASP-19 is a magnitude 12.3 star located in the Vela constellation of the southern hemisphere. This star has been found to host a transiting hot Jupiter-type planet in tight orbit.-Planetary system:...					12.3	5.3	815	G8V	has a transiting planet (b WASP-19b WASP-19b is an extrasolar planet, notable for possessing the shortest orbital period of any known planetary body: 0.7888399 days or approximately 18.932 hours.... )

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