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 52032	LMi	6.42	1,443.2	460.89	K0
HIP 52929	UMa	6.42	901.0	179.64	K0
HIP 55003	Car	6.42	632.1	88.47	A3V
Groombridge 1830 ◈	UMa	6.42	29.7	0.19	G8Vp
HIP 58369	UMa	6.42	153.4	5.21	A9V
HIP 58436	Hya	6.42	1,052.1	245.02	A1IV/V
35 Vir	Vir	6.42	583.5	75.37	M4III
HIP 62904	Com	6.42	146.1	4.73	G5IV
HIP 65754	CVn	6.42	257.6	14.70	F0IV
HIP 65796	Vir	6.42	502.6	55.92	K0III
HIP 67104	Boo	6.42	420.3	39.12	K2
HIP 67199	Cen	6.42	342.2	25.94	A1V
HIP 68224	Hya	6.42	640.8	90.87	K1III
HIP 69340	Vir	6.42	145.0	4.65	F7V
HIP 70038	Vir	6.42	331.5	24.32	G5
HIP 70418	Aps	6.42	967.8	207.40	B8V
HIP 78476 ◈	TrA	6.42	1,387.9	426.58	F8II
HIP 81231	Her	6.42	521.0	60.09	A2V
HIP 84332 ◈	Sco	6.42	—	23,550,493	K0Ia
HIP 85019	Sco	6.42	119.5	3.16	F8V
HIP 85391	Oph	6.42	395.3	34.61	B9.5/A0V
HIP 85450 ◈	Oph	6.42	665.6	98.08	M4III
HIP 85826	Oph	6.42	441.3	43.13	B9.5V
HIP 88172	Her	6.42	1,128.6	282.10	B8Vn
HIP 88876 ◈	Sgr	6.42	1,449.6	465.16	A2/A3Iab
HIP 90971 ◈	Oph	6.42	1,822.1	735.19	B8IIIp SiSr:
HIP 94770	Pav	6.42	769.2	130.98	B8/B9V
HIP 95239	Tel	6.42	234.8	12.20	F0V
HIP 96919 ◈	Cyg	6.42	1,032.1	235.94	M5IIIa
HIP 97485 ◈	Cyg	6.42	—	23,550,493	B0.5Ibvar
HIP 101489	Del	6.42	948.1	198.98	K0
HIP 101552	Mic	6.42	586.6	76.21	B8V
HIP 102901	Mic	6.42	647.1	92.73	K5III
HIP 102993	Cyg	6.42	1,734.9	666.19	B3III
HIP 105091 ◈	Cep	6.42	2,740.8	1,662.65	B2III
HIP 106064	Peg	6.42	473.4	49.61	K5
HIP 106320	Oct	6.42	679.5	102.24	K3III
HIP 106564	PsA	6.42	1,190.4	313.62	B8IIIw
Pi 1Gru	Gru	6.42	532.1	62.69	S57:
HIP 111601	Peg	6.42	408.2	36.88	A1III
HIP 113904	Psc	6.42	289.1	18.50	F2V
HYG 119398	Cyg	6.42	68.2	1.03	G0 V
HIP 34	Peg	6.43	243.4	12.99	F7.5IV-V
HIP 635	Psc	6.43	598.5	78.56	B8IIIsp...
HIP 1269	Cas	6.43	433.7	41.27	G8III...
HIP 1821	Cet	6.43	1,101.9	266.44	M0III
HIP 2889	Tuc	6.43	691.0	104.71	K2/K3III
HIP 2954	Psc	6.43	728.0	116.31	K4III
HIP 3056	Scl	6.43	893.6	175.23	K4III
HIP 6789	Cet	6.43	418.7	38.44	K0/K1III
HIP 7443	Phe	6.43	124.5	3.40	F3/F5V
HIP 7597	Cet	6.43	821.6	148.05	K5
HIP 8957	Hyi	6.43	181.3	7.21	F2V
HIP 9655	Cet	6.43	1,320.5	382.65	K4III
HIP 10379	Per	6.43	—	23,334,581	A3Iab
HIP 10396	Cet	6.43	1,025.6	230.78	K0
HIP 16712	Cam	6.43	174.0	6.64	F5V
22 Tau	Tau	6.43	380.1	31.71	A0Vn
HIP 19509	Eri	6.43	858.3	161.58	K2IIIp...
HIP 22737	Dor	6.43	1,194.7	313.04	M0/M1III

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.