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 41627	Pyx	7.42	715.3	45.08	G6/G8III
HIP 41825	Car	7.42	1,132.5	113.03	B8IV:
HIP 41842	UMa	7.42	985.4	85.59	K5
HIP 42111	Lyn	7.42	827.8	60.42	G8III
HIP 42283	Hya	7.42	408.2	14.68	G5
HIP 42690	Vol	7.42	1,249.6	137.66	B8V
HIP 42734	Lyn	7.42	151.8	2.03	F8
HIP 43158	Pyx	7.42	2,363.4	492.49	B0II/III
HIP 43324	Car	7.42	274.8	6.66	F3V
HIP 43446	Cam	7.42	169.6	2.54	F2
HIP 43643	Vel	7.42	635.8	35.61	A1/A2V
HIP 44205	UMa	7.42	1,254.4	138.68	K0
HIP 44485	Vol	7.42	886.3	69.25	B9III/IV
HIP 44625	UMa	7.42	1,524.1	204.74	K0
HIP 44934	Pyx	7.42	576.2	29.27	G8III/IV
HIP 45445	Hya	7.42	823.6	59.81	K2III
HIP 45541	Car	7.42	1,424.3	178.81	B6Vne
HIP 46693	Dra	7.42	2,025.8	361.74	K0
HIP 47394	Vel	7.42	—	9,375,620	K2/K3III
HIP 48647	Ant	7.42	586.6	30.34	G8III
HIP 49019	UMa	7.42	275.2	6.67	K2
HIP 49565	LMi	7.42	209.3	3.86	F5
HIP 49953	Ant	7.42	658.9	38.26	K0III
HIP 49966	Leo	7.42	1,449.6	185.18	G5
HIP 50148	Ant	7.42	1,753.5	270.89	K3/K4III
HIP 50843 ◈	Car	7.42	1,929.9	328.40	B2evar
HIP 51131	Car	7.42	435.5	16.72	A0V
HIP 51575	Sex	7.42	230.0	4.66	F2
HIP 51703	Hya	7.42	616.6	33.51	K3III
HIP 51873	Cha	7.42	698.4	42.97	K0III
HIP 52632	LMi	7.42	377.9	12.59	F0
HIP 52893	Leo	7.42	339.7	10.18	A0
HIP 53638	Vel	7.42	956.5	80.61	K1III
HIP 54095	Ant	7.42	266.7	6.27	F2V
HIP 54358	Car	7.42	—	9,375,620	O8
HIP 56049	Leo	7.42	187.9	3.11	F8
HIP 56443	Cen	7.42	741.3	48.44	K1III
HIP 56746	Crt	7.42	494.2	21.52	A0V
HIP 56863	Cen	7.42	340.1	10.20	F5/F6V
HIP 56993	Cen	7.42	599.6	31.68	A0V
HIP 57653 ◈	Cen	7.42	2,398.2	506.76	M0III
HIP 57875	Crt	7.42	378.4	12.61	A9V
HIP 58567 ◈	Dra	7.42	672.5	39.85	F0
HIP 59228	UMa	7.42	610.8	32.87	K0III
HIP 59594	Com	7.42	401.7	14.22	Fp
HIP 59943 ◈	Cru	7.42	—	9,375,620	M0Ia/Iab
HIP 61169	Dra	7.42	760.3	50.96	G9III+...
HIP 61847	Mus	7.42	573.2	28.95	A5V
HIP 62422	Vir	7.42	1,347.8	160.10	K2
HIP 67850	Vir	7.42	429.2	16.23	F0/F2V
HIP 68151	Cen	7.42	2,280.8	458.35	K3III
HIP 68234	Boo	7.42	477.5	20.10	A0
HIP 68298 ◈	Cen	7.42	—	9,375,620	M0/M1III
HIP 68880	Boo	7.42	874.4	67.36	G5
HIP 69211	Hya	7.42	429.2	16.23	F5V
HIP 69283	Boo	7.42	237.4	4.97	F2
HIP 70228	Cen	7.42	—	9,375,620	B0.5Iab
HIP 70621 ◈	Boo	7.42	763.8	51.43	A0
HIP 71777	Boo	7.42	202.5	3.61	F5
HIP 72862	UMi	7.42	2,077.4	380.54	K5

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.