List of stars in Puppis - 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....

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...

, 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

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:...

, and Puppis, these Greek-letter designations were kept, so that Puppis 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 Puppis.

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
ζ Pup Zeta Puppis Zeta Puppis is a star in the constellation of Puppis. It is also known by the traditional names Naos and Suhail Hadar in Arabic....	ζ	248	66811	39429	2.21	−5.95	1399	O5Iaf	Naos, Suhail Hadar, Muliphein; 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...
π Pup Pi Puppis Pi Puppis is a star in the constellation Puppis.In Chinese, , meaning Bow and Arrow, refers to an asterism consisting of π Puppis, δ Canis Majoris, η Canis Majoris, c Puppis, ZI 674, ο Puppis, κ Puppis, ε Canis Majoris and κ Canis Majoris...	π	82	56855	35264	2.71	−4.92	1094	K3Ib
ρ Pup (15 Puppis)	ρ	253	67523	39757	2.83	1.41	63	F2mF5IIp	Tureis; 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...
τ Pup Tau Puppis Tau Puppis is a third-magnitude star in the constellation Puppis. Tau Puppis is an orange K-type giant with an apparent magnitude of +2.94. Tau Puppis is also a spectroscopic binary star system in which the multiple companions within the system cause the principal star's orange color to vary from...	τ	39	50310	32768	2.94	−0.80	183	K0III...
ν Pup	ν	20	47670	31685	3.17	−2.39	423	B8III SB
σ Pup Sigma Puppis Sigma Puppis is a star in the constellation Puppis.Sigma Puppis belongs to spectral class K5 and has apparent magnitude +3.3. It is approximately 184 light years from Earth.Coordinates for epoch J2000:* Right ascension: 7h27m35s...	σ	99	59717	36377	3.25	−0.51	184	K5III SB	Hadir
ξ Pup Xi Puppis Xi Puppis is a star of magnitude +3.34 in the constellation Puppis. It has the traditional name Asmidiske , a misplacement and mistransliteration of Aspidiske, the traditional name of ι Carinae.... (7 Puppis)	ξ	191	63700	38170	3.34	−4.74	1347	G6Ia	Asmidiske, Azmidiske
175 G. Pup	c	175	63032	37819	3.62	−4.52	1387	K4III
213 G. Pup	a	213	64440	38414	3.71	−1.41	345	G5III...
3 Pup	l	157	62623	37677	3.94			A2Iab
199 G. Pup	P	199	63922	38164	4.10	−4.80	1964	B0III
11 Pup	j	222	65228	38835	4.20	−1.74	502	F7/F8II
218 G. Pup	J	218	64760	38518	4.22	−4.65	1940	B0.5Ib
ο Pup	ο	183	63462	38070	4.40	−5.00	2470	B1IV:nne	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...
16 Pup		256	67797	39906	4.40	−1.41	472	B5V
73 G. Pup HD 56096 HD 56096 is a giant star that is also known as L² Puppis because it is located in the constellation of Puppis. It is a semi-regular pulsating star that varies in magnitude from 2.60 down to 6.00 with a period of 140.83 days. The variation in light may be caused by a combination of radial pulsations...	L²	73	56096	34922	4.42	0.50	198	M5e
279 G. Pup	h²	279	69142	40326	4.42	−0.47	310	K1II/III
267 G. Pup	h¹	267	68553	40091	4.44	−4.36	1874	K4III
289 G. Pup	q	289	70060	40706	4.44	2.16	93	A4m...
108 G. Pup HD 60532 HD 60532 is a white main sequence star located approximately 84 light-years away in the constellation of Puppis, taking its primary name from its Henry Draper Catalogue designation. It is calculated to be 1.44 times more massive than the Sun. The star is only 59% as old as our Sun and has...		108	60532	36795	4.46	2.41	84	F6V	text-align:left; > has two planets 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 60532 b HD 60532 b is an extrasolar planet located approximately 84 light-years away in the constellation of Puppis, orbiting the star HD 60532. This planet has a true mass of 3.15 times more than Jupiter which orbits at 0.77 AU and takes 201.83 days to revolve in an eccentric orbit. This planet was... & c HD 60532 c HD 60532 c is an extrasolar planet located approximately 84 light-years away in the constellation of Puppis, orbiting the star HD 60532. This planet has a true mass of 7.46 times more than Jupiter which orbits at 1.58 AU and takes 607 days to revolve in an eccentric orbit. This planet was... )
V Pup		233	65818	38957	4.47	−3.29	1164	B1Vp + B2
QW Pup	I	71	55892	34834	4.49	2.86	69	F0IV	text-align:left; >γ Dor variable Gamma Doradus variable Gamma Doradus variables are variable stars which display variations in luminosity due to non-radial pulsations of their surface. The stars are typically young, early F or late A type main sequence stars, and typical brightness fluctuations are 0.1 magnitudes with periods on the order of one day...
QZ Pup	b	214	64503	38455	4.49	−1.98	640	B2V
k¹ Pup K Puppis k Puppis is a Bayer designation given to an optical double star in the constellation Puppis, the two components being k1 Puppis and k2 Puppis. Note that the designation here is "k" not "kappa" as some astronomers teach. Many of Puppis' stellar designations are English labels...	k¹	133	61555	37229	4.50	−1.92	454	B6V	Markab, Markeb; component of the k Puppis system
127 G. Pup	f	127	61330	37096	4.53	−0.67	358	B8IV/V
		232	65810	39095	4.61	0.29	238	A1V
k² Pup K Puppis k Puppis is a Bayer designation given to an optical double star in the constellation Puppis, the two components being k1 Puppis and k2 Puppis. Note that the designation here is "k" not "kappa" as some astronomers teach. Many of Puppis' stellar designations are English labels...	k²	134	61556		4.62	-1.81	462	B5IV	component of the k Puppis system
1 Pup		155	62576	37648	4.63	−2.75	976	K5III
		216	64740	38500	4.63	−2.09	720	B1.5Vp
NV Pup (83 G. Pup)	v¹	83	57150	35363	4.65	−2.42	847	B2V+...	γ Cas variable
		100	59890	36514	4.65	−4.00	1753	G2Ib...
119 G. Pup	p	119	60863	36917	4.65	0.46	225	B8V
PU Pup (128 G. Pup)	m	128	61429	37173	4.69	−1.45	551	B8IV	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...
Q Pup	Q	196	63744	38089	4.69	0.48	227	K0III
19 Pup		263	68290	40084	4.72	0.95	185	K0III
		268	68601	40096	4.73	−6.04	4657	A7Ib
		78	56456	35020	4.75	−0.43	354	B8/B9V
χ Pup	χ	225	65456	38901	4.76	−3.47	1442	A7III
MX Pup (274 G. Pup)	r	274	68980	40274	4.78	−2.61	979	B2ne	γ Cas variable
KQ Pup		107	60414	36773	4.82	−5.25	3361	A4Ia
A Pup	A	67	54893	34495	4.83	−1.98	751	B3IV/V
294 G. Pup	w	294	70555	40945	4.83	−2.22	838	K2/K3III
143 G. Pup	d¹	143	61831	37297	4.84	−1.39	574	B3V
		97	59612	36431	4.85	−5.13	3228	A6Ib/II
OU Pup	L¹	72	56022	34899	4.87	1.14	181	Ap	α² CVn variable
H Pup	H	61	53811	34059	4.92	1.07	192	A4IV
		47	51799	33357	4.94	−2.62	1062	M1III
140 G. Pup		140	61772	37379	4.98	−1.60	676	K3III
		37	50235	32855	4.99	−2.23	906	K2/K3III
20 Pup		269	68752	40259	4.99	−2.89	1230	G5Ib/II
212 G. Pup		212	64379	38423	5.01	3.73	59	F3/F5V
		80	56779	35226	5.03	−2.31	959	B3V
4 Pup		167	62952	37891	5.03	0.73	236	F2V
		159	62644	37606	5.04	3.13	79	G5IV
Y Pup		21	47973	31765	5.05	−0.58	436	G8III
111 G. Pup	n	111	60584	36817	5.06	2.74	95	F6V
49 G. Pup	t	49	52092	33558	5.07	−1.77	760	B4IV/V
		185	63465	38010	5.07	−2.83	1240	B2IV/V
N Pup	N	228	65551	38872	5.08	−2.90	1283	B2.5IV
12 Pup		230	65699	39023	5.09	−1.82	786	G8II
OS Pup		276	69081	40321	5.09	−2.70	1177	B2V:	γ Cas variable
NW Pup (84 G. Pup)	v²	84	57219	35406	5.11	−1.93	836	A0V	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...
		68	55526	34670	5.12	0.21	313	K2III
W Pup		162	62713	37664	5.12	1.02	215	K1III
X Pup		38	50223	32765	5.14	3.13	82	F5III
O Pup	O	231	65685	38917	5.14	0.32	300	K2III
9 Pup		205	64096	38382	5.16	4.05	54	G2V	HR 3064, Gl 291
6 Pup		190	63697	38211	5.17	0.72	253	K3III
		295	70556	40943	5.18	−3.31	1630	B2IV-V+...
C Pup	C	59	53704	34081	5.20	0.27	315	Am
		187	63578	38020	5.22	−3.33	1672	B1V
		234	65925	39061	5.22	1.41	189	F3V
F Pup	F	87	57240	35393	5.24	−0.55	469	A0V
MZ Pup		250	66888	39487	5.25	−4.03	2345	M2II
31 G. Pup	x	31	49591	32537	5.27	0.24	331	B8/B9V
		16	46273	30953	5.28	1.71	169	F2V
E Pup	E	70	55719	34802	5.30	−0.32	434	A3p...
188 G. Pup		188	63660	38146	5.32	0.35	321	G2
		302	71176	41260	5.32	−0.64	506	K4/K5III
		252	67456	39734	5.33	−2.54	1221	A3Ib/II
171 G. Pup		171	63077	37853	5.36	4.45	50	G0V
		227	65460	38846	5.36	−2.32	1120	B2.5V
98 G. Pup	y	98	59635	36363	5.41	−0.75	556	B3V
		150	62226	37450	5.41	−0.98	617	B3V
OW Pup (115 G. Pup)	z	115	60606	36778	5.42	−2.54	1273	B2Vne	text-align:left; >γ Cas variable
		215	64572	38497	5.44	−1.39	756	K1IIICN...
		309	71459	41323	5.45	−1.53	813	B3V
5 Pup		180	63336	38048	5.48	3.08	99	F5+...
		217	64802	38593	5.48	−1.47	801	B2V
V336 Pup		246	66624	39360	5.52	−0.35	486	Ap Si	α² CVn variable
		308	71377	41395	5.52	0.95	268	K1/K2III
18 Pup		262	68146	40035	5.53	3.77	73	F7V
		93	59256	36258	5.55	−1.03	674	B9Vsp...
		60	53705	34065	5.56	4.51	53	G3V...
		292	70442	40944	5.58	−0.12	450	A3V
		287	70002	40678	5.59	0.08	413	K2III
		156	62578	37623	5.60	−0.72	598	B5V
		197	63852	38200	5.61	−1.02	691	M0III
V390 Pup		161	62747	37751	5.62	−3.16	1863	B2II	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...
		204	64152	38375	5.62	1.00	274	K0III
		81	56813	35181	5.64	−0.99	692	K4III
		105	60341	36732	5.64	0.88	292	K0III
		154	62412	37590	5.64	0.59	333	K1III
V378 Pup		122	60855	36981	5.66	−2.87	1655	B2/3V(n)	Be star
		257	67880	39943	5.66	−1.59	921	B4V
		301	71141	41242	5.67	−0.76	631	A1III/IV
MY Pup (142 G. Pup)	y³	142	61715	37174	5.68	−5.26	5015	F4Iab	δ Cep variable
PT Pup		125	61068	37036	5.69	−2.89	1698	B2II	β Cep variable
130 G. Pup	y²	130	61391	37043	5.69	−0.23	497	B9V
10 Pup		206	64238	38427	5.69	−2.11	1185	F2IV/V
		293	70523	40990	5.71	0.99	286	K0III
PR Pup		77	56455	35029	5.72	0.14	425	A0p	α² CVn variable
144 G. Pup	d²	144	61878	37322	5.73	−0.64	612	B5V
G Pup	G	15	45572	30591	5.76	−0.82	675	B9V
145 G. Pup	d³	145	61899	37329	5.76	−1.91	1116	B3III
		278	69123	40344	5.77	1.56	227	K1III
		96	59550	36362	5.78	−1.95	1144	B2IV
		116	60666	36848	5.78	0.87	313	K1III
138 G. Pup	e	138	61641	37223	5.78	−1.58	964	B3III
D Pup	D	66	54475	34339	5.80	−1.26	842	B3V
		164	62781	37710	5.80	2.61	142	F0IV
		79	56733	35202	5.81	−0.78	679	B4V
QS Pup		200	63949	38159	5.82	−3.03	1918	B1.5IV	β Cep variable
		244	66598	39380	5.83	−0.18	518	K2/K3III
		106	60345	36721	5.84	0.98	306	A3III
M Pup	M	85	57197	35347	5.86	−0.54	621	B8II/III
112 G. Pup	n	112	60585		5.87
V392 Pup		176	63215	37915	5.87	−0.57	632	B5V	Be star
		298	70761	41074	5.88			F2Iab
		174	62893	37752	5.89	−0.46	608	B8V
		208	64225	38267	5.89	1.39	259	K2III
		91	59026	36143	5.90	−1.47	973	B4V
		178	63271	37995	5.90	−1.51	988	B1/B2V
		241	66358	39251	5.90	−0.41	595	A3IV
		141	61774	37364	5.92	−0.80	720	K0III
		2	41742	28790	5.93	3.77	88	F4V
		40	50445	32938	5.94	2.23	180	A3V
V363 Pup		69	55718	34817	5.94	−1.27	903	B4V
V397 Pup		195	63786	38167	5.94	0.11	478	B9V	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...
		76	56410	35054	5.95	−0.19	552	B4III/IV
			59499	36345	5.95	−0.31	582	B3V+...
285 G. Pup HD 69830 HD 69830 is an orange dwarf star approximately 41 light-years away in the constellation of Puppis. It has the Gould designation 285 G. Puppis, though this is infrequently used. In 2005, the Spitzer Space Telescope discovered a debris disk orbiting the star. The disk contains substantially more...		285	69830	40693	5.95	5.45	41	K0V	has three Neptune Neptune Neptune is the eighth and farthest planet from the Sun in the Solar System. Named for the Roman god of the sea, it is the fourth-largest planet by diameter and the third largest by mass. Neptune is 17 times the mass of Earth and is slightly more massive than its near-twin Uranus, which is 15 times... -mass planets 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 69830 b HD 69830 b is a Neptune-mass or Super-Earth mass extrasolar planet orbiting the star HD 69830. This planet is 10 times more massive than Earth, making it the least massive in the system. It also orbits quite close to its parent star and takes 82/3 days to complete an orbit.This is likely to be a... , c HD 69830 c HD 69830 c is the 2nd planet orbiting HD 69830. This is likely to be a rocky planet, not a gas giant. If it had formed as a gas giant, it would have stayed that way.-References:... , & d HD 69830 d HD 69830 d is an extrasolar planet orbiting the orange dwarf star HD 69830 every 197 days. It is the outermost known planet in its planetary system and possibly lies within its habitable zone.-Orbit and mass:... ), asteroid belt Asteroid belt The asteroid belt is the region of the Solar System located roughly between the orbits of the planets Mars and Jupiter. It is occupied by numerous irregularly shaped bodies called asteroids or minor planets...
		305	71267	41328	5.96	0.91	333	A3m...
V438 Pup		307	71302	41250	5.97	−3.92	3105	B3V	Algol variable
		92	59136	36236	5.98	−1.18	881	B5III
		235	65904	39014	5.98	−1.61	1076	B4V
V468 Pup (146 G. Pup)	d⁴	146	61925	37345	5.99	−2.10	1353	B4III	Be star
		239	66210	39122	6.01	0.70	377	A2V
		303	71196	41282	6.01	3.36	111	F2/F3V
		177	63118	37823	6.02	−1.15	886	B6IV
		223	65211	38732	6.02	−1.08	856	B6V
		94	59438	36395	6.05	3.39	111	F5V
QU Pup		210	64365	38370	6.05	−2.61	1762	B2IV	β Cep variable
2 Pup A		166	62864	37843	6.06	0.85	359	A6/A7
		275	69080	40341	6.07	−2.35	1575	B2V
		312	71487	41361	6.07	−0.30	613	B9IV/V
		63	54153	34253	6.09	−0.44	660	G0III
		226	65442	38845	6.09	−0.58	703	K3III
		113	60646	36807	6.11	1.39	287	A9IV
		194	63822	38246	6.11	−2.69	1874	K1III
		277	69082	40324	6.11	−2.18	1482	B2IV/V
14 Pup		247	66834	39524	6.12	−2.30	1575	B3III
		291	70302	40876	6.12	−0.58	712	G8/K0III
PY Pup		240	66255	39153	6.13	−2.20	1509	A0p	α² CVn variable
22 Pup		296	70673	41067	6.13	0.63	411	K0III
V368 Pup		90	58634	35960	6.14	−0.50	694	A8V	δ Sct variable
T Pup		189	63640	38074	6.14	−0.19	600	M2III
		220	64876	38635	6.14	−0.45	678	K4III
		62	53952	34200	6.15	2.42	182	F2V
		251	67243	39617	6.15	−3.94	3396	G1Ib
		282	69511	40485	6.15	−2.67	1895	K2III
		297	70612	40947	6.15	2.01	219	A4V
		23	48383	32007	6.16	−1.40	1058	B4V
		149	62082	37465	6.16	−0.95	860	M0/M1III
V339 Pup		30	49336	32434	6.19	−2.05	1449	B3Vne	Be star
		137	61642	37202	6.20	0.79	393	G8III
			60325	36736	6.21	−2.12	1509	B2II
		229	65598	38879	6.21	−1.24	1009	B5V
		260	67977	39920	6.21	0.82	389	G8III
		281	69445	40476	6.22	1.07	349	G6:III+...
		48	51825	33451	6.23	3.05	141	F5V
		51	52362	33590	6.23	0.66	424	A0V
		186	63655	38184	6.23	−2.57	1874	B8/B9II
		45	51266	33139	6.24	2.59	175	K0/K1III
		7	42448	29129	6.26	−0.55	751	B8II
			59235	36264	6.26	−0.28	664	K4III
		46	51682	33394	6.27	−0.21	644	K2III
V376 Pup		110	60559	36728	6.27	−0.30	672	B8IV (p Si)	β Lyr variable
		264	68242	39974	6.27	−1.12	979	B+...
		9	42834	29304	6.28	−0.26	663	A0V
		26	48543	32091	6.28	1.48	298	A+...
PX Pup		221	65183	38792	6.28	−1.59	1221	M5/M6III
		249	66812	39420	6.28	−0.61	780	G8II
		300	70946	41107	6.28	−1.88	1399	M2III
		27	48797	32208	6.30	0.17	549	A8:+...
		86	57299	35463	6.31	−0.45	734	K2/K3III
			63291	37939	6.31	0.00	597	K3III
QY Pup			63302	38031	6.31	−2.91	2280	K3Iab/b
		242	66435	39299	6.31	−0.70	823	M3III
NP Pup		44	51208	33189	6.32	−1.79	1364	C3II
		89	58420	35893	6.32	−0.33	697	B5V
		201	63948	38183	6.32	1.30	329	K0III
21 Pup		284	69665	40604	6.32	−0.78	858	A1V
OX Pup		182	63401	37982	6.33	−0.28	685	Ap Si	α² CVn variable
		126	61227	37089	6.34	−9.14	40750	F0Ib
			63696	38206	6.34	−0.96	939	K5III
		209	64287	38355	6.34	−2.09	1583	B2IV-V
		1	41700	28764	6.35	4.22	87	G0IV-V
		104	60312	36657	6.35	−0.43	739	B8V
		236	66005	39035	6.35	−1.63	1283	B2IV-V
			66885	39514	6.35	−0.66	823	K5/M0III
PQ Pup		258	67888	39866	6.36	−2.32	1772	B3V	γ Cas variable
8 Pup		203	64077	38372	6.37	2.00	244	F3IV
		237	66006	39038	6.37	−0.68	838	B2IV-V
		255	67751	39876	6.37	−1.87	1449	A3III
		131	61453	37128	6.38	0.18	566	K4III
		179	63323	38037	6.38	−2.95	2397	K5II/III
			69002	40291	6.38	1.07	377	K2III
		54	52703	33774	6.39	0.85	418	G8II/III
		170	63112	37951	6.39	−0.96	962	B9III
			60951	36986	6.40	−0.23	691	K1II
		135	61589	37289	6.40	−0.15	667	K3III
		272	68862	40220	6.40	0.22	561	A3V
		153	62318	37461	6.41	−1.31	1140	B7IV/V
		41	50621	32918	6.42	−0.22	695	K2/K3III
		160	62712	37666	6.42	0.17	580	B8IV
		265	68450	40063	6.42	−2.96	2451	B0III
			69904	40639	6.42	−4.18	4289	M0III + A3/5
			61750	37375	6.43	0.34	538	K2
		202	64042	38316	6.43	0.48	505	B9.5V
		286	69879	40656	6.43	0.65	466	K0III
		57	53253	33909	6.44	0.95	408	A0V
		290	70235	40787	6.44	−0.55	815	B8Ib/II
		304	71231	41306	6.44	−0.21	698	K1III
		207	64181	38292	6.45	0.27	561	G6III
			64974	38686	6.45	−1.54	1294	K4III
			63399	37996	6.46	0.87	428	K1III
			65638	38925	6.46	0.24	573	K0III
		43	50860	33015	6.47	0.90	424	B8V
			54179	34177	6.47	−0.44	787	K3III
		4	42168	28988	6.48	1.19	372	K1III
		8	42683	29185	6.48	2.58	196	F8V
V420 Pup			67698	39834	6.49		1299	B3III/IV	Be star
		193	63734	38209	6.49	0.96	417	K2III
		139	61672	37293	6.50	−0.50	819	B6V
			67408	39730	6.50	0.05	637	K1III
2 Pup B			62863	37842	7.03	1.57	402	A0/A1V
HD 70642 HD 70642 HD 70642 is a yellow dwarf star in the constellation of Puppis located 93.8 light years away. This star has about the same mass and radius as the Sun, is slightly cooler and less luminous, and is richer in abundance of iron relative to hydrogen....			70642	40952	7.18	4.89	94	G6V	has a planet (b HD 70642 b HD 70642 b is an extrasolar planet orbiting the star HD 70642 at 3.23 AU distance and takes 5.66 years to revolve. This planet may have systems of moons like Jupiter. This planet was discovered on July 3, 2003.-External links:*... )
HD 50499 HD 50499 HD 50499 is a yellow dwarf star approximately 154 light-years away in the constellation of constellation of Puppis. It is suspected that the star is hotter, larger, and more massive than the Sun. The magnitude is 7, this star is too faint to be in naked eye visibility...			50499	32970	7.22		154	GIV	has a planet (b HD 50499 b HD 50499 b is an extrasolar planet approximately 154 light-years away in the constellation of Puppis. The planet is suspected to be a gas giant with mass of 1.7 times Jupiter. It is a long period, taking 351 weeks to orbit the star... ) and unconfirmed planet (c)
HD 48265 HD 48265 \|- bgcolor = "#FFFAFA"HD 48265 is a G type star in the southern constellation Puppis. It is a 8th magnitude star at a distance of about 285 light years from Earth.-Planetary system:...			48265	31895	8.07	3.36	285	G5IV/V	has a planet (b HD 48265 b HD 48265 b is an extrasolar planet located approximately 285 light-years away in the constellation of Puppis, orbiting the 8th magnitude G-type main sequence star HD 48265. This planet has a minimum mass of 1.2 times that of Jupiter. Because the inclination is not known, the true mass is not known... )
NGC 2423-3 NGC 2423-3 NGC 2423-3 is a red giant star approximately 2498 light-years away in the constellation of Puppis. The star is part of the NGC 2423 open cluster . The star has an apparent magnitude of nine and an absolute magnitude of zero, with a mass of 2.4 times the Sun...					9.45	0.03	2500		individual star of open cluster Open cluster An open cluster is a group of up to a few thousand stars that were formed from the same giant molecular cloud and have roughly the same age. More than 1,100 open clusters have been discovered within the Milky Way Galaxy, and many more are thought to exist... NGC 2423, has a planet (b NGC 2423-3 b NGC 2423-3b is an extrasolar planet approximately 2498 light-years away in the constellation of Puppis. The planet was announced in 2007 to be orbiting the red giant star NGC 2423-3 . The planet has a mass at least 10.6 times that of Jupiter... )

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