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
80 Peg ◈ Peg 5.77 845.0 287.61 M3III
HIP 117887 ◈ Psc 5.78 637.0 162.03 M5IIb
HIP 72208 ◈ Boo 5.78 807.3 260.14 M5III
HIP 8778 ◈ Cet 5.78 307.1 37.64 F0V
56 Ari ◈ Ari 5.78 502.6 100.83 B9p Si
HIP 101475 ◈ Cyg 5.78 431.4 74.27 B9sp...
1 Cam ◈ Cam 5.78 — 42,461,956 B0III SB
56 Eri ◈ Eri 5.78 — 42,461,956 B2Ve
HIP 42177 ◈ Vel 5.79 446.2 78.70 B8 Si
HIP 45915 ◈ UMa 5.79 751.5 223.46 M4IIIa
35 Aql ◈ Aql 5.79 199.6 15.76 A0V
HIP 83150 ◈ TrA 5.79 787.8 245.47 Ap Si
HIP 16591 ◈ Per 5.79 182.8 13.22 A5m
HIP 26169 ◈ Men 5.79 1,087.2 467.30 M2/M3III
HIP 418 ◈ Cas 5.80 723.2 204.93 B8MNp...
74 Aqr ◈ Aqr 5.80 825.7 267.18 B8IV/V
HIP 87812 ◈ Oph 5.82 1,359.0 710.56 B2IV-V
HIP 38159 ◈ Pup 5.82 1,929.9 1,433.51 B1.5IV
HIP 31173 ◈ Aur 5.82 262.8 26.57 A3m + A3m
HIP 16846 ◈ Tau 5.82 100.1 3.85 G5IV/V +K1IV
HIP 81472 ◈ Sco 5.83 627.2 149.97 B2.5IV
HIP 45675 ◈ Vel 5.83 — 40,550,854 B7Iab
HIP 67861 ◈ Cen 5.83 — 40,550,854 B2IIIe
HIP 85760 ◈ Aps 5.83 883.9 297.85 M3III
105 Tau ◈ Tau 5.84 1,080.0 440.55 B2Ve
HIP 106062 ◈ Peg 5.84 665.6 167.34 M4III
HIP 69829 ◈ Boo 5.84 762.0 219.38 M3III
HIP 20271 ◈ Eri 5.85 789.7 233.35 B5III
HIP 21604 ◈ Tau 5.85 329.8 40.70 B8V
HIP 112997 ◈ Peg 5.86 292.0 31.62 K1III SB
HIP 69929 ◈ Vir 5.86 332.8 41.08 Ap Si(Cr)
HIP 117503 ◈ And 5.86 423.0 66.37 G1IIIe
HIP 72567 ◈ Boo 5.86 59.3 1.30 G2V
HIP 82172 ◈ Her 5.86 755.0 211.45 M4IIIa
HIP 37915 ◈ Pup 5.87 590.9 128.23 B5V
HIP 35626 ◈ CMa 5.87 639.5 150.24 M3III
HIP 62641 ◈ CVn 5.87 358.0 47.08 A3V
3 Sco ◈ Sco 5.87 515.3 97.54 B8III/IV
HIP 5926 ◈ Cas 5.87 2,764.0 2,808.02 K1V
33 Gem ◈ Gem 5.87 858.3 270.64 B7III
HIP 87460 ◈ Sco 5.88 842.8 258.46 B6Ib
HIP 94013 ◈ Cyg 5.88 231.6 19.53 K1IV
HIP 50685 ◈ UMa 5.88 402.2 58.88 A7Vn
HIP 46620 ◈ Car 5.88 967.8 341.04 M2III
HIP 11348 ◈ Cet 5.88 251.3 22.99 Ap SrCrEu
HIP 77442 ◈ CrB 5.89 — 38,370,725 C00 (F8pe)
HIP 96620 ◈ Cyg 5.89 133.3 6.42 F6Vasv
HIP 105269 ◈ Cyg 5.89 2,160.0 1,682.67 F2Ib
53 Psc ◈ Psc 5.89 1,038.7 389.05 B2.5IV
HIP 13121 ◈ Ari 5.89 397.3 56.91 A0V
HIP 72432 ◈ Cen 5.89 514.4 95.50 M5III
HIP 84500 ◈ Oph 5.89 653.6 154.03 B5Vnn
HIP 96234 ◈ Sgr 5.89 423.0 64.57 A5IV-III
HIP 52043 ◈ Car 5.89 1,006.7 365.43 B3IV
59 Ori ◈ Ori 5.89 364.4 47.91 A5me del Del
HIP 7321 ◈ And 5.90 467.9 78.27 B9IV
HIP 53530 ◈ Vel 5.90 335.9 40.33 A7Vni
HIP 78877 ◈ Sco 5.90 526.1 98.90 B8V
HIP 74386 ◈ Ser 5.90 723.2 186.90 M4III
56 Leo ◈ Leo 5.91 388.7 53.51 M5IIIvar
← Previous Page 12 · 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.