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 91786 Tel 9.34 148.0 0.33 K0V
63Eps Dra Dra 3.84 148.0 52.19 G8III
HIP 18893 Tau 6.91 148.1 3.09 F8
67Kap2Tau Tau 5.27 148.1 14.00 A7V
HIP 112219 Peg 7.99 148.1 1.14 G5V
HIP 114420 And 7.29 148.1 2.18 G0
HIP 116973 Aqr 10.09 148.1 0.17 K3/K4
HIP 4882 Phe 7.70 148.1 1.49 G0V
48 Tau ◈ Tau 6.31 148.1 5.38 F5Vvar
HIP 20699 Eri 9.73 148.1 0.23 K2V
HIP 36485 Gem 7.16 148.1 2.46 F5+...
HIP 48391 UMa 7.80 148.1 1.36 G0
HIP 105359 Aqr 8.51 148.1 0.71 G5
HIP 3428 And 10.97 148.2 0.07 M0
HIP 20690 Cam 8.59 148.2 0.66 G5
HIP 108598 Ind 9.57 148.2 0.27 K0V
HIP 4966 Cep 8.44 148.3 0.76 G5
HIP 7626 Psc 9.40 148.3 0.31 G5
HIP 12638 Per 8.70 148.3 0.60 G5
HIP 19510 Eri 11.46 148.3 0.05 —
HIP 21317 ◈ Tau 7.90 148.3 1.25 G1V
HIP 96725 Tel 9.04 148.3 0.44 K1V
HIP 113535 And 10.98 148.3 0.07 K5
HIP 4772 Tuc 6.91 148.3 3.10 G1/G2V
HIP 16783 Eri 8.85 148.3 0.52 K0V
HIP 26614 Lep 10.25 148.3 0.14 —
HIP 58876 Dra 7.92 148.3 1.22 F8
HIP 61633 CVn 11.44 148.3 0.05 K2V
HIP 94326 CrA 8.80 148.3 0.54 G5V
HIP 105707 Cyg 11.09 148.3 0.07 —
35 Peg Peg 4.78 148.3 22.06 K0III
HIP 15211 Eri 10.22 148.4 0.15 —
HIP 20199 Hor 8.26 148.4 0.90 G3IV/V
HIP 20605 Tau 11.66 148.4 0.04 M0.5Ve
HIP 37283 Lyn 6.89 148.4 3.16 F5
HIP 107299 Ind 6.49 148.4 4.57 F7IV/V
HIP 149 Peg 11.26 148.5 0.06 K3
HIP 25414 Cam 8.35 148.5 0.82 G5
HIP 46903 UMa 8.40 148.5 0.79 G0
HIP 70715 Boo 10.93 148.5 0.08 M0
HIP 104124 Vul 10.75 148.5 0.09 K7
HD 219430 Aqr 9.62 148.5 0.26 K3 V J
HYG 119554 Aqr 10.30 148.5 0.14 —
HIP 143 Peg 10.35 148.5 0.13 K3
HIP 4395 Tuc 7.17 148.5 2.45 G8IV
68Del3Tau ◈ Tau 4.30 148.5 34.42 A2IV
HIP 31187 CMa 8.97 148.5 0.47 K0V
HIP 49644 Car 8.83 148.5 0.53 G5
HIP 97704 Aql 9.36 148.5 0.33 G5
HIP 100836 Sgr 8.60 148.5 0.66 K0V
10The Psc Psc 4.27 148.5 35.38 K1III
105Ome2Aqr Aqr 4.49 148.5 28.89 B9V
Bet3Tuc Tuc 5.07 148.6 16.95 A0V
Eta Hor Hor 5.30 148.6 13.72 A6V
HIP 62896 Cen 4.25 148.6 36.07 A4IV
HIP 100405 Tel 8.39 148.6 0.80 G5V...
HIP 11476 Hyi 10.13 148.7 0.16 —
HIP 20652 Tau 11.06 148.7 0.07 K8
HIP 29882 Aur 6.68 148.7 3.85 F6V
HIP 32382 Aur 7.47 148.7 1.86 G0
← Previous Page 124 · 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.