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 2814	Cas	6.89	—	15,275,661	A2
HIP 3995	Cet	6.89	297.6	12.72	F2
HIP 4049	Phe	6.89	311.8	13.96	F2/F3V
HIP 5363	Phe	6.89	268.4	10.35	A9V
HIP 5631	Psc	6.89	111.5	1.79	F5
HIP 6334	Psc	6.89	673.9	65.22	F0
HIP 6791	Cet	6.89	308.6	13.68	F3IV
HIP 7421	Psc	6.89	575.2	47.51	K1III
HIP 8734	And	6.89	180.7	4.69	F8
HIP 9358	Cet	6.89	314.5	14.20	A0
HIP 9540	Hyi	6.89	772.9	85.74	K2III
HIP 9829	Ari	6.89	74.3	0.79	G2V
HIP 10179	Hyi	6.89	827.8	98.45	K2III
HIP 10721	And	6.89	896.0	115.24	G5
HIP 11260	Cet	6.89	451.7	29.30	K0
HIP 11927	Cet	6.89	265.4	10.11	F3IV/V
HIP 13645 ◈	Ari	6.89	851.6	104.14	M3II-III
HIP 16782	Per	6.89	579.3	48.17	B8V
HIP 16914	Men	6.89	196.4	5.54	F0III
HIP 17549	Per	6.89	459.4	30.31	A0
HIP 17785	Ret	6.89	832.0	99.45	A4V
HIP 18437	Eri	6.89	345.1	17.11	A0V
HIP 18688	Per	6.89	639.5	58.72	A0
HIP 20037	Cam	6.89	440.2	27.82	B8
HIP 20243 ◈	Eri	6.89	976.5	136.90	M4III
HIP 21642	Per	6.89	419.8	25.30	K0
HIP 22309	Tau	6.89	261.8	9.84	F5
HIP 23011	Eri	6.89	504.1	36.48	A5
HIP 24038	Col	6.89	1,144.4	188.10	K5III
HIP 24441	Ori	6.89	795.5	90.87	M6V
HIP 24445	Cam	6.89	605.1	52.58	F0
HIP 26642	Lep	6.89	891.1	114.08	B8V+...
HIP 26842	Dor	6.89	504.1	36.48	A1V
HIP 27479	Col	6.89	1,087.2	169.67	K4III
HIP 28081	Lep	6.89	374.5	20.14	A1V
HIP 28374	Ori	6.89	640.8	58.94	A0
HIP 30328	Mon	6.89	333.2	15.94	A3
HIP 30418	Col	6.89	1,842.7	487.53	B5V
HIP 30583 ◈	CMa	6.89	942.6	127.64	A0V
HIP 31201	CMa	6.89	200.8	5.79	F8V
HIP 31568	Gem	6.89	108.0	1.67	G0
HIP 34152	CMa	6.89	3,166.6	1,440.12	K5/M0III
HIP 34266	Gem	6.89	1,254.4	225.94	K8III
HIP 35790	Car	6.89	278.1	11.11	K0/K1III
HIP 36260	Mon	6.89	456.8	29.98	K0
HIP 37069	Pup	6.89	358.8	18.48	K1III
HIP 37122	CMi	6.89	755.0	81.88	B9
HIP 37283	Lyn	6.89	148.4	3.16	F5
HIP 37616	Pup	6.89	1,045.4	156.89	G6/G8III
HIP 38591	Pup	6.89	1,655.6	393.73	M1III
HIP 39352	Pup	6.89	1,591.0	363.41	K1III + F/G
HIP 39362	Mon	6.89	847.2	103.09	K0
HIP 39433 ◈	Lyn	6.89	956.5	131.34	M5III
HIP 39523	Lyn	6.89	416.5	24.91	K0
HIP 41255	Pup	6.89	—	15,275,661	B4III/IV
HIP 41519	Lyn	6.89	371.9	19.86	K0
HIP 42403	Cnc	6.89	112.9	1.83	F8
HIP 42937	Pyx	6.89	224.9	7.26	F0V
HIP 43984	UMa	6.89	580.3	48.35	A2
HIP 44545	Vel	6.89	—	15,275,661	B5V

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.