Explore the Universe. Understand Everything In It.
★
Menu
Home Tonight's Sky News
Explore Solar System PlanetsMoons StarsExoplanets GalaxiesBlack Holes NebulaeAsteroids & Comets Constellations Space Exploration Space Industry
Sky Astronomy Calendar Launches
Learn & Tools Start Learning Astrophysics Scale of the Universe Timeline Glossary A–Z People Young Astronomers Top Lists Tools Compare Worlds Ask the Atlas AI Agents API
About About us Methodology Contact

Guided View
New to astronomy? We explain every term as you browse, in plain English. Same pages, with the help built in.

Expert View
You know the sky. Just the content, clean and compact, with no extra explanations. This is the default view.

Interface language
Light mode

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.

Deep guides: The SunProxima CentauriAlpha CentauriSiriusBetelgeusePolarisVegaVY Canis MajorisTRAPPIST-1Barnard's StarRigelDenebAltairAntares How stars live & die →

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.

O
B
A
F
G
K
M
White dwarf
Brown dwarf
Brightest in our sky Nearest to the Sun Most luminous Stars with proper names Variable stars
StarConstellationMagnitude Distance (ly)Luminosity (Suns)Spectral type
HIP 9234 ◈ And 7.60 568.2 24.10 M8
HIP 9369 Ari 7.60 723.2 39.05 G5
HIP 9596 Cet 7.60 2,380.7 423.06 G5
HIP 9961 Eri 7.60 706.0 37.22 K1III
HIP 9974 And 7.60 187.0 2.61 F5
HIP 11870 Per 7.60 422.5 13.33 A3III
HIP 11950 For 7.60 332.5 8.26 A9V
HIP 12850 Eri 7.60 965.0 69.50 G5/G6III
HIP 12915 Per 7.60 1,614.6 194.63 K0
HIP 13767 For 7.60 397.8 11.81 F0V
HIP 13821 Per 7.60 388.7 11.28 A5
HIP 14035 For 7.60 360.0 9.67 F8V
HIP 14361 Eri 7.60 263.9 5.20 F5V
HIP 15272 Ret 7.60 553.7 22.89 K2III
HIP 15550 Ari 7.60 401.7 12.04 A2+...
HIP 16116 Tau 7.60 566.2 23.94 F0
HIP 16593 ◈ Tau 7.60 2,001.0 298.95 M...
HIP 16724 ◈ Per 7.60 942.6 66.37 B8Vp
HIP 16796 Tau 7.60 858.3 55.00 K0
HIP 17036 Cam 7.60 620.1 28.71 A0
HIP 17271 Per 7.60 497.2 18.45 G5
HIP 18185 Eri 7.60 1,449.6 156.89 K0
HIP 18839 Eri 7.60 200.2 2.99 F8/G0V
HIP 19281 Tau 7.60 529.5 20.93 B9m
HIP 19377 Cam 7.60 1,090.8 88.88 B9
HIP 19541 Per 7.60 486.8 17.70 G5
HIP 20402 Cep 7.60 667.0 33.20 A0
HIP 20471 Eri 7.60 982.4 72.04 K2
HIP 21878 Per 7.60 189.0 2.67 F8
HIP 22787 Cae 7.60 82.1 0.50 K0V
HIP 23061 Cae 7.60 500.2 18.69 K1IV
HIP 23884 Tau 7.60 118.7 1.05 G5IV
HIP 24173 Dor 7.60 774.7 44.83 K5III
HIP 24229 Ori 7.60 1,716.6 219.99 K0
HIP 24540 Aur 7.60 867.4 56.18 A2
HIP 25263 Pic 7.60 726.4 39.41 A2V
HIP 25437 Lep 7.60 462.6 15.98 A5III/IV
HIP 25796 Pic 7.60 1,235.4 113.97 K5III
HIP 26075 Aur 7.60 561.4 23.53 G5
HIP 26288 Lep 7.60 1,065.9 84.80 K3III
HIP 26581 Ori 7.60 1,309.9 128.12 B3V
HIP 26761 Tau 7.60 185.2 2.56 F8
HIP 27218 Tau 7.60 585.6 25.61 F2
HIP 27263 Ori 7.60 364.8 9.94 G5
HIP 27331 Col 7.60 553.7 22.89 A0V
HIP 27873 Col 7.60 476.8 16.98 A2m...
HIP 28018 Lep 7.60 1,832.3 250.73 K0III
HIP 28272 Tau 7.60 525.2 20.61 K0
HIP 28698 Aur 7.60 657.6 32.30 K0
HIP 28778 ◈ Lep 7.60 313.6 7.35 A9V
HIP 29101 Ori 7.60 1,475.8 162.63 A0
HIP 29794 Mon 7.60 2,609.2 508.16 K0
HIP 29954 Dor 7.60 219.0 3.58 F3V
HIP 30176 Mon 7.60 1,087.2 88.23 B9
HIP 30713 CMa 7.60 404.7 12.22 A3V
HIP 30873 Pup 7.60 847.2 53.60 A1V
HIP 31683 CMa 7.60 1,568.1 183.65 M0III
HIP 31965 Lyn 7.60 131.4 1.29 G0
HIP 32351 Men 7.60 264.1 5.21 F0/F2V
HIP 32396 Vol 7.60 550.0 22.59 K2III
← Previous Page 471 · 119,625 stars in this view Next →
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.