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 103828 ◈ Cyg 6.18 976.5 263.27 M3Ib-II:
HIP 94685 ◈ Lyr 6.18 1,399.8 541.00 F6Ib-II
HIP 664 ◈ Psc 6.18 911.1 229.30 K2III
HIP 25776 ◈ Men 6.18 366.1 37.02 A1V
HIP 2388 ◈ Phe 6.18 422.5 49.29 F2III
HIP 82911 ◈ Sco 6.18 2,363.4 1,543.12 B0.5Ia
HIP 48782 ◈ Car 6.18 1,208.0 402.90 B3V
HIP 47145 ◈ Vel 6.18 230.3 14.66 F0p
HIP 82339 ◈ Oph 6.18 241.6 16.11 A3V
HIP 99221 ◈ Cap 6.18 552.8 84.41 B9.5III
HIP 29401 ◈ Mon 6.18 574.2 91.03 B9MNp...
70 Aqr ◈ Aqr 6.19 364.0 36.24 A9III-IV
HIP 92593 ◈ Her 6.19 682.3 127.41 B8Vnn
48 LMi ◈ LMi 6.19 387.8 41.15 A8V
HIP 106752 ◈ Cyg 6.19 550.9 83.02 A7III
HIP 89980 ◈ Sgr 6.19 1,065.9 310.74 M3III
HIP 51425 ◈ Car 6.19 876.8 210.28 B4IV
HIP 32434 ◈ Pup 6.19 1,325.8 480.84 B3Vne
HIP 58272 ◈ Hya 6.20 393.4 41.96 B9.5V
63 Her ◈ Her 6.20 268.4 19.53 A8V
HIP 50332 ◈ Vel 6.20 715.3 138.68 M4/M5III
HIP 107856 ◈ Cyg 6.20 1,016.1 279.77 B9p HgMn
HIP 68842 ◈ Cen 6.20 509.6 70.40 A5III/IV
HIP 61496 ◈ Crv 6.20 217.9 12.87 F0V
HIP 7493 ◈ And 6.20 512.8 71.32 K1III:
HIP 59678 ◈ Cru 6.20 — 28,840,315 B1.5Ia
HIP 58545 ◈ Cam 6.21 913.6 224.28 M2III
HIP 26779 ◈ Aur 6.21 40.0 0.43 K1V
44 Cet ◈ Cet 6.21 220.2 13.03 F0V
HIP 25785 ◈ Ori 6.21 541.8 78.85 K2IIIvar
HIP 28434 ◈ Lep 6.21 205.0 11.29 F2IV
HIP 20063 ◈ Per 6.22 395.8 41.69 B9V
27 Vir ◈ Vir 6.22 205.1 11.20 A7Vn
HIP 101810 ◈ Del 6.22 381.0 38.65 M6III
HIP 95154 ◈ Dra 6.22 1,259.3 422.28 C5II
HIP 97944 ◈ Sgr 6.22 45.8 0.56 K3/K4V
HIP 87850 ◈ Her 6.22 967.8 249.34 M6Sv
HIP 31766 ◈ Mon 6.23 2,174.4 1,247.38 O9.5II
HIP 26964 ◈ Tau 6.23 827.8 180.80 B2.5Ve
HIP 60813 ◈ Vir 6.23 241.1 15.33 F2III
HIP 38723 ◈ Lyn 6.23 192.4 9.76 A3p
HIP 26718 ◈ Aur 6.23 1,941.4 993.57 M2SIab
HIP 274 ◈ Cas 6.24 2,489.7 1,620.32 B3Ia
HIP 102158 ◈ Del 6.24 485.4 61.55 G8III
HIP 102770 ◈ Aqr 6.24 991.4 256.80 M3
HIP 46247 ◈ UMa 6.24 1,186.0 367.45 K2III
HIP 71876 ◈ Dra 6.24 132.6 4.60 F2V
9 Sge ◈ Sge 6.24 — 27,797,133 O8e
HIP 54708 ◈ Car 6.24 791.6 163.83 M4III
HIP 96721 ◈ Tel 6.24 364.4 34.71 Am
HIP 63820 ◈ Cen 6.24 1,190.4 370.17 M3/M4III
HIP 87655 ◈ Oph 6.24 271.8 19.30 F5Vn
HIP 4879 ◈ Tuc 6.25 867.4 194.80 M2III
HIP 82693 ◈ Oph 6.25 249.9 16.17 F0V
HIP 39530 ◈ Car 6.25 1,199.1 372.22 B2.5Vn
Gumala ◈ Sgr 6.25 89.9 2.09 F8V
53 Cnc ◈ Cnc 6.25 886.3 203.42 M3III
HIP 15204 ◈ Per 6.25 198.8 10.22 A1m
HIP 6952 ◈ Phe 6.25 1,012.9 265.71 M3III
HIP 13178 ◈ Per 6.25 — 27,542,287 A5Ia
← Previous Page 16 · 5,992 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.