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 34543	Car	6.82	732.9	82.26	G5III
HIP 35461 ◈	CMa	6.82	2,174.4	724.44	B2V
HIP 35761	CMa	6.82	1,614.6	399.21	B3III
HIP 36068	CMa	6.82	1,038.7	165.20	B9IV
HIP 36687	Mon	6.82	393.0	23.66	A0
HIP 36884	CMi	6.82	1,510.0	349.30	K0
HIP 37013	Car	6.82	682.3	71.32	A0V
HIP 37501	Lyn	6.82	1,045.4	167.34	K0
HIP 37603	Pup	6.82	414.4	26.30	K1III/IV
HIP 38221	Gem	6.82	538.2	44.38	G8III
HIP 39282	Pup	6.82	—	16,292,960	B7II
HIP 39621	CMi	6.82	623.6	59.54	A0
HIP 42388	Vol	6.82	392.0	23.53	K0IV
HIP 43330	Hya	6.82	263.2	10.62	A5
HIP 45511	Hya	6.82	300.9	13.87	A3V
HIP 45565	Hya	6.82	426.3	27.85	F0
HIP 46053	Leo	6.82	1,568.1	376.70	M4III
HIP 46889	Car	6.82	2,189.0	733.84	B8III
HIP 48212	Leo	6.82	247.3	9.37	A5
HIP 49209	Hya	6.82	362.8	20.16	A3III
HIP 49823	Vel	6.82	600.7	55.26	G6III
HIP 51602	Sex	6.82	701.4	75.37	K0
HIP 51781	LMi	6.82	204.6	6.42	K2III
HIP 52324	Ant	6.82	372.3	21.22	A0V
HIP 53836	Vel	6.82	446.2	30.48	A0V
HIP 54231	Cen	6.82	384.6	22.66	A0V
HIP 54515	Leo	6.82	259.7	10.33	A2
HIP 54518 ◈	UMa	6.82	953.7	139.32	M0
HIP 54854	Cen	6.82	271.3	11.27	Am
HIP 55029	Leo	6.82	501.0	38.44	A0
HIP 57064	Cen	6.82	—	16,292,960	F0Ib-II
HIP 57522	Crt	6.82	704.4	76.00	K0/K1III
HIP 58466	Vir	6.82	782.1	93.67	K0
HIP 59528	Cru	6.82	470.6	33.92	A8IV
HIP 59753	Com	6.82	1,032.1	163.23	K2
HIP 60396	Crv	6.82	489.7	36.75	K0III
HIP 60845	Cru	6.82	157.8	3.81	G3V
HIP 62437	CVn	6.82	219.3	7.37	F0
HIP 63045	Cen	6.82	1,279.0	250.50	B5Vn
HIP 64312	Com	6.82	461.3	32.60	F2II
HIP 64365	Com	6.82	482.5	35.65	G5III
HIP 64532	UMa	6.82	82.5	1.04	G1V
HIP 64564	Cen	6.82	—	16,292,960	F8Ib
HIP 65414	Vir	6.82	392.5	23.59	K0
HIP 65528	Cen	6.82	1,035.4	164.13	K5/M0III
HIP 66042	CVn	6.82	673.9	69.57	G8III compSB
HIP 66376	Cen	6.82	294.6	13.29	A3m...
HIP 67543	Boo	6.82	344.8	18.21	G0
HIP 68108	Boo	6.82	485.4	36.07	K0
HIP 69449 ◈	Vir	6.82	1,655.6	419.95	M3III
HIP 69523	Boo	6.82	369.8	20.95	F0
HIP 70220	Vir	6.82	349.2	18.67	A2
HIP 70269	Vir	6.82	128.6	2.53	G0...
HIP 71348 ◈	Oct	6.82	1,591.0	387.61	M4III
HIP 71873	Lib	6.82	532.9	43.49	K0
HIP 72056	Lib	6.82	985.4	148.73	K2III
HIP 72868	Vir	6.82	767.4	90.20	K5III
HIP 73071	Boo	6.82	763.8	89.37	K2III
HIP 74037 ◈	Dra	6.82	311.2	14.83	F4III SB
HIP 74110	Cir	6.82	1,822.1	508.63	B3V

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.