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 50600 Hya 9.24 3,197.6 168.58 K0
HIP 96449 Cyg 6.60 948.1 168.58 K5
HIP 104111 Aqr 7.15 1,221.6 168.58 K5
HIP 44571 Cnc 7.80 1,647.3 168.58 K2III
HIP 84950 Dra 5.69 623.6 168.58 K5III
HIP 23436 ◈ Tau 8.36 2,131.7 168.58 B1Ve
HIP 43743 Cnc 9.24 3,197.6 168.58 A2
HIP 45563 Cam 8.17 1,953.0 168.42 B3
HIP 85210 Sco 8.17 1,953.0 168.42 M3III
HIP 7631 And 8.60 2,380.7 168.42 A0
HIP 108030 Cep 7.41 1,376.2 168.42 G8II
HIP 59680 Com 7.41 1,376.2 168.42 G8III
HIP 7087 Scl 7.96 1,772.6 168.42 M2/M3III
HIP 62147 Vir 8.17 1,953.0 168.42 K0
HIP 34248 ◈ CMa 6.34 840.6 168.42 B3V
HIP 100642 Sgr 8.25 2,025.8 168.42 K3III
HIP 89361 CrA 7.26 1,284.1 168.42 B8/B9III
HIP 117988 Aqr 8.60 2,380.7 168.42 K2
HIP 92478 ◈ Her 8.57 2,346.4 168.27 B5III SB
HIP 37899 Pup 8.39 2,160.0 168.27 G8III
HIP 97427 Sgr 9.02 2,886.3 168.27 K0III
HIP 40740 Pup 7.08 1,181.7 168.27 B9III
HIP 94484 Lyr 7.12 1,203.5 168.27 A0
HIP 6457 Scl 7.33 1,325.8 168.27 M1III
HIP 9031 For 8.07 1,863.7 168.27 K2:III:
HIP 44258 ◈ Hya 9.00 2,861.0 168.27 A1V
HIP 30546 ◈ Car 8.80 2,609.2 168.27 M2/M3III
HIP 114083 And 8.42 2,189.0 168.11 A0
HIP 116851 Aqr 6.61 950.9 168.11 M1III
HIP 55546 UMa 7.44 1,393.8 168.11 K0
HIP 106108 Cyg 6.72 1,000.5 168.11 A3
HIP 99512 ◈ Pav 8.42 2,189.0 168.11 M8III
HIP 118291 Phe 8.01 1,812.0 168.11 K2III
HIP 46519 Hya 7.13 1,208.0 167.96 M1III
HIP 29839 Ori 6.56 929.2 167.96 B7III
HIP 27478 Tau 7.28 1,294.3 167.96 K2II
HIP 47958 Car 8.48 2,249.4 167.96 A3IV
HIP 43286 Car 8.45 2,218.7 167.96 G8III
HIP 78694 Nor 7.87 1,698.7 167.96 B8IV/V
HIP 31770 Gem 8.48 2,249.4 167.96 K0
HIP 118151 Scl 7.13 1,208.0 167.96 K5III
25 Lyn Lyn 6.25 805.3 167.96 K2III:
HIP 101285 Cyg 6.14 765.6 167.96 K5III
Psi Phe ◈ Phe 4.39 341.9 167.80 M4III SB
HIP 21461 Cae 8.91 2,740.8 167.80 K0III/IV
HIP 68662 UMi 7.74 1,598.8 167.80 K5
HIP 72268 ◈ Vir 7.23 1,264.2 167.80 M...
HIP 67958 Vir 6.97 1,120.8 167.65 G6/G8III+..
HIP 39149 Pup 7.49 1,424.3 167.65 A1IV
HIP 38447 Gem 8.59 2,363.4 167.65 K0
HIP 33440 Car 8.59 2,363.4 167.65 K1III
HIP 36940 Pup 7.85 1,681.2 167.65 B8II
HIP 36009 CMa 7.93 1,744.1 167.65 B5V
HIP 30613 Gem 7.14 1,212.5 167.65 K0III
HIP 53847 UMa 8.31 2,077.4 167.65 G5
36 Peg Peg 5.60 596.3 167.49 K5III
HIP 44055 Car 7.84 1,672.6 167.49 B8III
50 Cet Cet 5.41 546.3 167.49 K1III
HIP 26678 Ori 7.84 1,672.6 167.49 K2
HIP 67372 CVn 7.70 1,568.1 167.49 K0
← Previous Page 138 · 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.