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 79874 Sco 7.10 591.9 41.46 K5III
HIP 81312 Her 7.10 127.2 1.91 F8V
HIP 82506 Her 7.10 208.9 5.17 F4III
HIP 82936 Sco 7.10 1,289.2 196.61 O7
HIP 83642 Dra 7.10 542.7 34.87 K0
HIP 84267 Ara 7.10 491.2 28.55 A0V
HIP 84308 Oph 7.10 701.4 58.24 K0
HIP 84561 Her 7.10 623.6 46.00 B9
HIP 87140 Sco 7.10 715.3 60.53 B9V
HIP 88350 Her 7.10 265.2 8.32 F2
HIP 88720 Sgr 7.10 1,194.7 168.89 B7/B8III
HIP 89767 Oph 7.10 2,313.2 633.29 B8
HIP 90034 Sct 7.10 1,353.3 216.77 A1Ib
HIP 90229 Sgr 7.10 1,101.9 143.75 K1IIICN...
HIP 91112 Sgr 7.10 2,416.0 690.56 A3III
HIP 91629 CrA 7.10 682.3 55.11 A2IV
HIP 91736 Sgr 7.10 3,229.3 1,233.67 Asp...
HIP 92000 Sct 7.10 939.9 104.52 B8
HIP 92410 Lyr 7.10 386.0 17.64 A2
HIP 92412 ◈ Tel 7.10 688.1 56.03 A3III/IV
HIP 92965 Sct 7.10 872.1 90.03 K5
HIP 93517 Dra 7.10 765.6 69.37 A2
HIP 94192 Lyr 7.10 732.9 63.56 B9
HIP 94780 Lyr 7.10 811.3 77.91 G5
HIP 95164 Sgr 7.10 148.8 2.62 G1V
HIP 97824 Sgr 7.10 2,764.0 904.48 A2/A3IV
HIP 99394 Vul 7.10 426.3 21.52 A0
HIP 99476 Aql 7.10 370.6 16.26 F0
HIP 99667 Cyg 7.10 — 12,589,254 B0.5III
HIP 100680 Cap 7.10 688.1 56.03 A3
HIP 101186 Cyg 7.10 2,965.1 1,040.40 O9.5Ia
HIP 104667 Cep 7.10 574.2 39.01 B9
HIP 105518 Pav 7.10 1,113.2 146.69 M2III
HIP 105650 Cyg 7.10 1,080.0 138.04 B9
HIP 106863 Cyg 7.10 763.8 69.06 F0
HIP 107289 Ind 7.10 1,128.6 150.80 M2III
HIP 109197 Cep 7.10 1,347.8 214.98 A0
HIP 109226 Peg 7.10 507.2 30.45 K0
HIP 109794 Aqr 7.10 239.5 6.79 F6/F7V
HIP 109815 Peg 7.10 559.4 37.05 F5
HIP 110900 Peg 7.10 216.6 5.55 K0V
HIP 111263 Peg 7.10 950.9 107.05 K5
HIP 111992 Aqr 7.10 278.3 9.16 G1V
HIP 113671 Peg 7.10 468.6 25.99 K0III
HIP 113987 Peg 7.10 290.7 10.00 F5IV
HIP 114024 ◈ Peg 7.10 921.3 100.46 A0
HIP 114028 Peg 7.10 119.6 1.69 G0
HIP 114774 Peg 7.10 396.3 18.59 A0
HIP 115697 Peg 7.10 166.0 3.26 G0
HIP 116042 Peg 7.10 623.6 46.00 K2
HIP 116063 Tuc 7.10 100.0 1.18 G0V
HYG 118453 Pup 7.10 140.9 2.35 F8 IV-V
HYG 118759 UMa 7.10 89.8 0.95 G3 V
HD 224960 ◈ Cet 7.10 — 12,589,254 S7.3e
HIP 740 Peg 7.11 344.8 13.94 F5
HIP 852 ◈ Peg 7.11 1,190.4 166.11 M4III:
HIP 1755 Psc 7.11 629.6 46.47 A2
HIP 1854 Cet 7.11 571.2 38.26 K0III
HIP 2076 Phe 7.11 376.6 16.63 K0III/IV
HIP 3006 Cep 7.11 134.6 2.12 F8
← Previous Page 288 · 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.