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 96457 Cyg 7.00 827.8 88.96 K2
HIP 106103 Peg 6.41 630.9 88.96 K0
HIP 43940 Cam 9.83 3,048.2 88.96 K0
HIP 87591 Dra 9.75 2,938.3 88.96 K5
HIP 60925 CVn 8.45 1,614.6 88.96 K1III
HIP 20225 Cam 6.95 809.3 88.96 G5
HIP 31392 CMa 7.32 959.3 88.96 K4III
HIP 107149 PsA 7.09 862.8 88.96 K1III
13 Del Del 5.57 428.6 88.96 A0V
HIP 87175 Aps 7.68 1,132.5 88.96 B8/B9V
HIP 52199 Ant 7.27 937.2 88.88 K2III
HIP 113577 Cas 9.31 2,398.2 88.88 B5
HIP 99942 Vul 7.19 903.5 88.88 A0
HIP 117567 Aqr 5.70 454.9 88.88 K4III
HIP 19377 Cam 7.60 1,090.8 88.88 B9
10 Tri Tri 5.29 376.6 88.88 A2V
HIP 25213 Pic 8.43 1,598.8 88.88 B9V
HIP 99372 Cyg 8.63 1,753.5 88.88 B8V
HIP 99048 Aql 7.34 967.8 88.88 K5
HIP 43638 Hya 8.63 1,753.5 88.88 A0
HIP 49375 ◈ Ant 6.99 823.6 88.88 Ap (EuCr)
HIP 21457 Pic 8.80 1,896.3 88.88 G8III
HIP 19137 ◈ Tau 8.75 1,853.2 88.88 S42v
HIP 25017 Pic 6.67 710.6 88.80 K0IIICN...
HIP 46150 Vel 8.84 1,929.9 88.80 K0III
HIP 58255 Cen 8.84 1,929.9 88.80 K2III
HIP 58733 Cen 9.36 2,452.3 88.80 K1III
HIP 101794 Cyg 7.08 858.3 88.80 G0
HIP 109415 Oct 7.36 976.5 88.80 K1III
HIP 66417 Boo 5.72 458.7 88.80 M2III
HIP 74206 Lib 6.55 672.5 88.80 K4III
HIP 46060 Hya 8.54 1,681.2 88.80 G5
HIP 64989 Vir 8.42 1,591.0 88.80 K2
HIP 29161 Aur 8.06 1,347.8 88.80 B8
HIP 11888 ◈ Per 8.84 1,929.9 88.80 A2Iab
HIP 83171 Her 9.46 2,568.2 88.80 F5
HIP 54473 Cen 8.84 1,929.9 88.80 G8/K0III
HIP 39886 Lyn 8.54 1,681.2 88.80 K0
HIP 111471 Peg 7.38 985.4 88.80 K3III
HIP 45370 Vel 8.74 1,842.7 88.72 B8/B9V
HIP 83377 Aps 7.03 838.4 88.72 K1II
HIP 88939 Pav 9.10 2,174.4 88.72 B9.5V
HIP 7906 Tri 5.97 514.4 88.72 K0III
HIP 65112 ◈ Cen 5.47 408.7 88.72 B6V
HIP 108215 PsA 8.53 1,672.6 88.72 B3IV
HIP 91815 Dra 7.88 1,240.1 88.72 K5
HIP 107929 Cep 6.56 675.3 88.72 A1p
HIP 18213 Eri 5.11 346.2 88.72 B6/B7V
HIP 61927 CVn 6.89 785.9 88.72 K2IIICN...
HIP 56265 UMa 7.76 1,173.2 88.72 K1IV
HIP 58736 Cru 9.10 2,174.4 88.72 B9V
HIP 28784 Ori 7.76 1,173.2 88.72 K0
HIP 32839 Mon 6.87 778.4 88.63 B8
HIP 33970 CMa 7.14 881.5 88.63 B9V
HIP 48298 Leo 6.86 774.7 88.63 A0
HIP 66106 UMi 8.52 1,664.1 88.63 K0
HIP 112333 Tuc 7.94 1,274.0 88.63 K3III
HIP 108117 Cap 8.88 1,964.8 88.63 F5
HIP 64301 Cen 8.38 1,560.6 88.63 B8Vn
HIP 99259 Vul 7.94 1,274.0 88.63 B9
← Previous Page 285 · 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.