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
Chi1For For 6.39 351.8 28.18 A1IV
HIP 16672 For 6.39 1,152.5 302.27 K3III
HIP 18769 Per 6.39 395.3 35.58 A0V
HIP 20039 Cep 6.39 1,042.0 247.06 K0
HIP 24955 Cam 6.39 385.5 33.82 G5
HIP 25667 Ori 6.39 797.4 144.68 A0Vn
HIP 28765 Aur 6.39 440.2 44.10 A7III
HIP 29798 Ori 6.39 959.3 209.51 K5II
HIP 30602 Mon 6.39 401.7 36.71 A0
HIP 31266 CMa 6.39 322.3 23.64 K0III+...
HIP 31662 Mon 6.39 497.2 56.23 K0
HIP 33154 Mon 6.39 533.8 64.86 A6Vn
HIP 33774 Pup 6.39 385.1 33.76 G8II/III
HIP 36141 CMi 6.39 1,336.7 406.63 B7II-III
HIP 36977 Car 6.39 578.3 76.14 K1/K2IIICN.
HIP 37951 Pup 6.39 743.0 125.66 B9III
HIP 40354 Cnc 6.39 1,190.4 322.40 G8III
HIP 41781 Vel 6.39 1,190.4 322.40 B2.5V
39 Cnc Cnc 6.39 608.5 84.26 K0III
HIP 43593 Vel 6.39 404.7 37.26 A0V
HIP 43853 Pyx 6.39 233.6 12.43 A4V
HIP 44331 Lyn 6.39 248.4 14.05 A9Vn
HIP 44423 Vel 6.39 849.4 164.13 B6V
HIP 44768 Cnc 6.39 189.7 8.20 F5V
HIP 47260 Dra 6.39 231.6 12.21 F2V+...
HIP 47627 Ant 6.39 1,101.9 276.44 Asp...
HIP 48706 Vel 6.39 731.3 121.67 M1III
HIP 48730 Vel 6.39 — 24,210,290 B2IV-V
HIP 50893 Sex 6.39 1,387.9 438.53 K5
HIP 54289 Car 6.39 439.0 43.85 A3V
HIP 54749 Crt 6.39 618.9 87.18 K3III
HIP 58809 Vir 6.39 228.7 11.90 F5
HIP 60454 Cen 6.39 371.9 31.48 F2V
HIP 60468 Hya 6.39 748.1 127.41 K5III
HIP 61719 Com 6.39 434.3 42.93 K1III
HIP 61748 ◈ CVn 6.39 439.0 43.85 A0p SrCrEu
HIP 62046 UMa 6.39 535.6 65.28 K0
HIP 67589 Dra 6.39 333.8 25.37 K2IV
HIP 68739 Vir 6.39 329.1 24.66 K0
HIP 68902 Cen 6.39 — 24,210,290 B0Ia
HIP 69065 Cen 6.39 366.9 30.62 G8/K0III
HIP 70385 Boo 6.39 1,988.8 900.33 K4III
HIP 70966 Cen 6.39 921.3 193.20 K3III
HIP 71168 ◈ Boo 6.39 244.7 13.63 F8IVw
HIP 71333 Cen 6.39 559.4 71.25 K2III
HIP 71406 Boo 6.39 380.6 32.96 K0
HIP 72000 Cir 6.39 — 24,210,290 B3V:
HIP 73118 Cir 6.39 1,832.3 764.19 B5V
HIP 75959 Aps 6.39 1,289.2 378.09 B3V
HIP 76006 CrB 6.39 243.9 13.54 F6III
HIP 77729 Lup 6.39 252.6 14.52 K0III
HIP 78870 Oph 6.39 478.9 52.19 K0
HIP 79385 CrB 6.39 698.4 110.97 K0
HIP 79867 Dra 6.39 591.9 79.73 K0
HIP 87670 Dra 6.39 523.5 62.40 K0
HIP 89010 Sgr 6.39 351.5 28.11 K0III
HIP 89943 Dra 6.39 557.5 70.73 K1III
HIP 92233 Oct 6.39 135.1 4.15 G2V
HIP 93437 Lyr 6.39 849.4 164.13 B5IV
HIP 94372 Sgr 6.39 451.1 46.30 K0III
← Previous Page 131 · 119,625 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.