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
43Kap Cap Cap 4.72 294.1 91.62 G8III
27Omi Aur Aur 5.46 413.4 91.62 A0p...
HIP 12349 Ari 7.11 883.9 91.62 F7IV..
HIP 4973 Hyi 8.54 1,707.6 91.62 B8III
HIP 86960 ◈ Oph 7.34 982.4 91.54 B5V
HIP 78328 Dra 8.61 1,763.0 91.54 G5
HIP 72084 Lib 9.31 2,434.0 91.54 F7V
HIP 100228 Aql 7.93 1,289.2 91.54 G5
HIP 3432 ◈ And 9.36 2,489.7 91.54 F3IV-V
HIP 74316 Dra 7.59 1,101.9 91.54 K5
HIP 88009 Pav 7.88 1,259.3 91.54 A2/A3III
HIP 9439 Eri 8.10 1,393.8 91.54 A5/A6V
HIP 35969 Gem 7.59 1,101.9 91.54 A0
HIP 45909 Cnc 9.08 2,189.0 91.54 G5
HIP 19566 Per 8.98 2,090.7 91.54 K0
HIP 95974 Sgr 6.93 813.4 91.54 K1III
HIP 109408 Gru 6.43 645.9 91.54 K3III
HIP 116367 Cep 8.41 1,606.7 91.45 K2
HIP 39349 Pup 8.12 1,405.8 91.45 B9V
HIP 26122 Lep 6.72 737.9 91.45 M0III
HIP 35388 Aur 9.17 2,280.8 91.45 A2
HIP 38928 Cam 8.86 1,976.7 91.45 K0
HIP 76239 UMi 7.65 1,132.5 91.45 A2
HIP 10013 ◈ Ari 8.53 1,698.7 91.45 M0
HIP 72650 Lib 7.72 1,169.0 91.37 K2III
HIP 85514 Oph 9.01 2,117.9 91.37 A0
HIP 85948 Ara 7.45 1,032.1 91.37 M0III
HIP 62166 Vir 8.52 1,689.9 91.37 K5
HIP 85625 Oph 8.77 1,896.3 91.37 K2
HIP 95889 Tel 8.90 2,013.3 91.37 K3III
HIP 10028 And 7.16 903.5 91.37 B9
HIP 9740 ◈ And 9.01 2,117.9 91.37 A5
HIP 4475 Cas 6.44 648.4 91.37 G8IV
Del Ant Ant 5.57 434.3 91.37 B9/B9.5V
HIP 27445 Col 8.90 2,013.3 91.37 K3IV
HIP 36880 Mon 8.66 1,802.0 91.37 A0
HIP 107842 Ind 7.47 1,042.0 91.37 K1III
HIP 109616 Aqr 8.72 1,853.2 91.37 G5
HIP 105890 Peg 8.97 2,077.4 91.29 K5
HIP 100757 Cyg 8.38 1,583.3 91.29 K2
3 Psc Psc 6.22 585.6 91.29 G4III
HIP 36276 Mon 8.59 1,744.1 91.29 K2
HIP 46507 Vel 8.51 1,681.2 91.29 K0III
HIP 39040 Cnc 9.43 2,568.2 91.29 G5
HIP 64418 Cen 8.15 1,424.3 91.29 K2III
HIP 5606 And 7.80 1,212.5 91.29 G5
HIP 65366 Com 7.39 1,003.6 91.29 K0
HIP 2490 Psc 6.89 797.4 91.29 K0
HIP 47602 Leo 7.26 945.4 91.29 K1III
HIP 68418 CVn 6.63 707.5 91.29 K2
HIP 31589 Pic 8.50 1,672.6 91.20 B9.5V
28 LMi LMi 5.52 424.1 91.20 K1III
HIP 62949 ◈ Cru 9.07 2,174.4 91.20 B2III
116 Tau Tau 5.52 424.1 91.20 B9.5Vn
HIP 91249 Lyr 8.50 1,672.6 91.20 K5
HIP 12254 Cas 9.07 2,174.4 91.20 G5V
HIP 58441 Mus 7.73 1,173.2 91.20 K2III
HIP 51333 Ant 7.23 931.9 91.20 G8III
HIP 51893 Leo 9.50 2,651.7 91.20 A2
67 Leo Leo 5.70 460.7 91.20 A3IV
← Previous Page 277 · 109,400 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.