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 47198	UMa	7.43	184.3	2.96	F5
HIP 48271	UMa	7.43	330.8	9.56	F3III
HIP 48683	Hya	7.43	430.9	16.22	A2V
HIP 48877	Hya	7.43	610.8	32.57	K3III
HIP 49475	Vel	7.43	230.3	4.63	F3V
HIP 49774	Hya	7.43	642.0	36.01	K2
HIP 49831	Leo	7.43	572.2	28.60	F0
HIP 49881	UMa	7.43	793.6	55.00	K0
HIP 50081	Leo	7.43	528.6	24.41	G5
HIP 51000	Hya	7.43	651.0	37.02	K0III
HIP 51752	Leo	7.43	656.2	37.60	K0
HIP 52332	Vel	7.43	273.2	6.52	F5V
HIP 53516	Hya	7.43	295.7	7.63	F0V
HIP 54232	UMa	7.43	1,575.6	216.77	K2
HIP 54317	Cen	7.43	2,174.4	413.05	K3III
HIP 54318	Leo	7.43	945.4	78.05	M2III
HIP 54975	Leo	7.43	744.6	48.44	K0
HIP 54984	Cen	7.43	162.3	2.30	F7V
HIP 56129	UMa	7.43	847.2	62.69	K0III-IV
HIP 57979	Crt	7.43	686.6	41.19	K0III
HIP 58092	Cen	7.43	916.2	73.32	K1/K2III
HIP 58928	Mus	7.43	821.6	58.94	K5III
HIP 59174	Com	7.43	424.7	15.75	A0V
HIP 59482	Hya	7.43	559.4	27.34	K1III
HIP 59532	Vir	7.43	113.7	1.13	G4V
HIP 59552	Cen	7.43	1,393.8	169.67	K3III
HIP 59689	Mus	7.43	—	9,289,664	B0.5Ib
HIP 60011	Crv	7.43	—	9,289,664	M1III
HIP 60518	Vir	7.43	515.3	23.18	K0
HIP 60825	Mus	7.43	157.6	2.17	F5V
HIP 61065	Cam	7.43	834.2	60.76	K0
HIP 61166	Cru	7.43	1,560.6	212.62	B8IV
HIP 62070 ◈	Vir	7.43	1,164.8	118.47	M3III:
HIP 63534	Cen	7.43	921.3	74.13	K2III
HIP 63708	Hya	7.43	192.6	3.24	F6V
HIP 63967	Cha	7.43	621.2	33.70	A5m...
HIP 64801	Cen	7.43	449.3	17.62	F2III
HIP 65036	Mus	7.43	145.0	1.83	G6IV-V
HIP 65700	Vir	7.43	445.0	17.28	K1III
HIP 65836	Com	7.43	402.2	14.13	F5
HIP 65942	Hya	7.43	351.5	10.78	A4IV
HIP 65972	Cen	7.43	526.9	24.25	F2/F3V
HIP 66546	Cen	7.43	—	9,289,664	A0III
HIP 67736	Cen	7.43	1,199.1	125.55	B8/B9III
HIP 67818	UMa	7.43	213.2	3.97	F5
HIP 67975	Cen	7.43	614.2	32.96	A1V
HIP 68341	Cir	7.43	—	9,289,664	B2/B3IV
HIP 69489	Cen	7.43	398.2	13.85	A4V
HIP 70651	Vir	7.43	893.6	69.76	K0
HIP 70760	Boo	7.43	224.5	4.40	G5
HIP 70963	UMi	7.43	460.0	18.48	A3
HIP 71142	Vir	7.43	300.1	7.86	K0
HIP 71463	Boo	7.43	924.0	74.54	K1III
HIP 71625	Cen	7.43	171.5	2.57	F5V
HIP 71900 ◈	Boo	7.43	1,568.1	214.78	M2
HIP 72990	Lib	7.43	325.2	9.23	F2
HIP 74853	Lup	7.43	1,062.4	98.54	M1III
HIP 77373	CrB	7.43	277.1	6.71	F6V
HIP 77901	Nor	7.43	1,842.7	296.48	B7IV
HIP 78518	Lup	7.43	1,274.0	141.78	K4/K5III

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.