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 93770 Lyr 6.32 1,456.1 514.75 M0III
HIP 63170 ◈ Cru 7.34 2,329.7 514.75 B0.5Ia
5Gam Mon Mon 3.99 497.9 514.75 K3III
HIP 28532 Cep 6.17 1,359.0 514.75 M0III
HIP 54572 ◈ Car 7.73 2,787.7 514.75 B2Ve
18 Dra Dra 4.84 736.2 514.28 K1p
HIP 116060 Aqr 6.39 1,503.0 514.28 K0
HIP 71003 Lup 7.28 2,265.0 514.28 Ap...
HIP 86725 Oph 6.40 1,510.0 514.28 F0III/IV
HIP 61266 Cru 7.75 2,811.7 514.28 B8III
HIP 97395 Cyg 7.64 2,673.4 514.28 K5
25 Vul Vul 5.50 997.4 513.81 B8IIIn
14 Pup Pup 6.12 1,325.8 512.86 B3III
HIP 42129 Car 5.27 896.0 512.39 B3V+...
HIP 50970 ◈ Vel 6.80 1,812.0 512.39 M5III
HIP 106973 Cyg 6.74 1,763.0 512.39 K1II-III
2Eps Crv Crv 3.02 317.9 512.39 K2III
HIP 34568 CMa 7.11 2,090.7 512.39 A1III
HIP 26439 Ori 7.11 2,090.7 512.39 B4V
HIP 56162 Cen 7.95 3,076.9 511.92 G8II
HIP 89330 Sgr 6.79 1,802.0 511.45 B7II
HIP 47694 ◈ Vel 6.15 1,342.2 511.45 B6V
HIP 76687 Nor 6.94 1,929.9 510.98 K2III
HIP 56875 Leo 7.20 2,174.4 510.50 F0IIIn
HIP 92733 Sgr 6.98 1,964.8 510.04 K2III
HIP 8020 Cas 6.33 1,456.1 510.04 B7II
HIP 692 Cet 7.76 2,811.7 509.57 K2
HIP 96159 ◈ Aql 6.61 1,655.6 509.57 M5III
HIP 74110 Cir 6.82 1,822.1 508.63 B3V
HIP 104592 Cyg 6.69 1,716.6 508.63 F0III
HIP 29794 Mon 7.60 2,609.2 508.16 K0
HIP 25896 Ori 7.45 2,434.0 507.69 B8
HIP 30779 Aur 7.55 2,548.1 507.69 K5III
HIP 108975 ◈ PsA 5.97 1,230.8 507.69 B3V (+B)
HIP 34495 Pup 4.83 728.0 507.69 B3IV/V
HIP 80911 Sco 4.24 554.7 507.22 B2III-IV
HIP 76207 Lup 5.82 1,148.4 507.22 M2III
HIP 60358 Com 7.86 2,938.3 507.22 K2III
HIP 59760 CVn 7.28 2,249.4 507.22 G5II
HIP 36500 ◈ Pup 7.62 2,630.3 507.22 B1/B2Ib/II
HIP 83323 ◈ Ara 6.26 1,405.8 507.22 B2IVne
HIP 57653 ◈ Cen 7.42 2,398.2 506.76 M0III
HIP 98773 Cyg 7.15 2,117.9 506.76 A2V+...
HIP 21601 Cam 6.64 1,672.6 505.82 K0
HIP 38262 Pup 7.21 2,174.4 505.82 K2
HIP 29678 Ori 5.91 1,194.7 505.36 B1V
HIP 115416 And 7.33 2,296.9 505.36 K2
5 Lib Lib 6.33 1,449.6 505.36 K2III
5Alp1Cap Cap 4.30 569.2 505.36 G3Ib
HIP 28431 Ori 7.44 2,416.0 504.89 K3Ib
HIP 46914 Vel 5.12 829.9 504.89 B4IV
HIP 99435 Dra 6.84 1,832.3 504.89 B0.5V
HIP 90314 Lyr 8.07 3,229.3 504.89 K2
HIP 36364 Pup 6.94 1,918.6 504.89 K1III
HIP 87395 Sco 7.79 2,836.1 504.43 G8III
HIP 44685 UMa 7.49 2,470.9 504.43 B2IV
HIP 43792 ◈ Vel 8.05 3,197.6 504.43 B3Vne
HIP 104688 Cyg 8.03 3,166.6 503.96 M0
HIP 107034 Peg 8.03 3,166.6 503.96 K5
HIP 107367 Aqr 6.98 1,953.0 503.96 K2
← Previous Page 27 · 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.