Stars

119,625 real stars from the HYG catalog: every Hipparcos star, with distances, brightnesses, spectral types and luminosities.

Source: the HYG stellar database v4.1 (CC BY-SA), built from the Hipparcos, Yale and Gliese catalogs. 464 stars carry proper names; the rest go by catalog numbers, as astronomers know them. Blank cells mean the catalog holds no measured value, never a guess. The galaxy holds 100–400 billion stars; this is the well-measured neighborhood.

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The spectral classesO B A F G K M

Every star in the catalogue below belongs to one of these families, from hottest blue to coolest red. The Sun is a G.

White dwarf

Brown dwarf

Star	Constellation	Magnitude	Distance (ly)	Luminosity (Suns)	Spectral type
HIP 30545	Mon	5.88	109.5	4.37	F8V
47 Aur	Aur	5.88	610.8	135.77	K4III
12 Mon	Mon	5.88	562.3	115.13	K0V
HIP 31946	Cam	5.88	774.7	218.57	K0III
HIP 32226	Mon	5.88	2,861.0	2,978.52	B0III
HIP 33415	Aur	5.88	349.6	44.50	K0III:
HIP 40305	Lyn	5.88	574.2	120.01	G9III
HIP 41074	Pup	5.88	—	38,725,764	F2Iab
HIP 41935	Lyn	5.88	243.9	21.66	K2III
HIP 44024	Vel	5.88	1,035.4	390.12	G8/K0II
HIP 46620 ◈	Car	5.88	967.8	341.04	M2III
HIP 50685 ◈	UMa	5.88	402.2	58.88	A7Vn
HIP 53723	Crt	5.88	661.6	159.37	M1III
HIP 55086	UMa	5.88	448.6	73.25	K0III:
HIP 61181	Mus	5.88	347.7	44.01	K1III
25 Vir	Vir	5.88	225.1	18.45	A3V
HIP 62402	UMa	5.88	196.6	14.07	A9V
65 Vir	Vir	5.88	1,244.9	563.90	K3III
HIP 65550	CVn	5.88	411.8	61.72	K0III:
HIP 67194	CVn	5.88	171.4	10.70	A5V
HIP 71353	Cen	5.88	366.9	48.98	B6V
18 Lib	Lib	5.88	310.0	34.99	K3III-IV
HIP 73493	Cen	5.88	390.6	55.56	K2/K3III
Ome Oct	Oct	5.88	317.0	36.58	B9.5V
HIP 74901	Ser	5.88	726.4	192.13	K5III
HIP 83176	Oph	5.88	540.9	106.46	M1/M2III
HIP 87460 ◈	Sco	5.88	842.8	258.46	B6Ib
HIP 90915	Her	5.88	753.2	206.63	K5III
HIP 90930	Pav	5.88	354.9	45.84	K0III
HIP 94013 ◈	Cyg	5.88	231.6	19.53	K1IV
HIP 94630	Lyr	5.88	1,269.1	586.14	M0III
57 Sgr	Sgr	5.88	377.9	52.00	K0III
HIP 98609	Vul	5.88	1,080.0	424.62	B4V
HIP 104171	Cep	5.88	158.9	9.20	F3IV
44 Cap	Cap	5.88	435.5	69.06	A9/F0V
HIP 109972	Cep	5.88	616.6	138.42	G8III
HIP 111259	Lac	5.88	683.8	170.14	A6V
60 Aqr	Aqr	5.88	347.7	44.01	G6III
HIP 111934	PsA	5.88	693.9	175.39	K2/K3III
HIP 114366	Scl	5.88	649.7	153.60	K2III
HIP 1630	And	5.89	521.0	97.90	B7V
53 Psc ◈	Psc	5.89	1,038.7	389.05	B2.5IV
HIP 3170	Tuc	5.89	81.4	2.39	G1V
HIP 9001	And	5.89	921.3	306.20	K5III
HIP 9307	Ari	5.89	391.1	55.16	K0III-IV
112 Psc	Psc	5.89	109.3	4.31	G2IV
HIP 11033	Cet	5.89	442.5	70.66	K2III
HIP 11381	Cet	5.89	274.3	27.14	K2III
13 Tri	Tri	5.89	102.4	3.78	G0V
HIP 13121 ◈	Ari	5.89	397.3	56.91	A0V
HIP 13949	Per	5.89	648.4	151.64	K2
HIP 14502	Cas	5.89	618.9	138.17	B9V
HIP 18735	Tau	5.89	139.9	7.06	F4V...
HIP 19284	Tau	5.89	401.7	58.18	K5III
HIP 24162	Ori	5.89	122.7	5.43	F5V
HIP 28139	Ori	5.89	308.6	34.36	K2III
59 Ori ◈	Ori	5.89	364.4	47.91	A5me del Del
HIP 37031	CMi	5.89	128.2	5.93	G0V
HIP 37752	Pup	5.89	672.5	163.08	B8V
HIP 38267	Pup	5.89	246.2	21.86	K2III

Magnitude runs backwards: smaller numbers are brighter (the sky’s brightest star, Sirius, is −1.44). Naked-eye limit is about +6.5 under dark skies. Distances come from measured parallaxes; luminosities are computed from brightness plus distance.