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 76073 Lup 6.82 945.4 136.90 B9IV/V
HIP 76573 ◈ Ser 6.82 686.6 72.24 MIII
HIP 77315 Lup 6.82 480.3 35.35 A0V
HIP 77534 Lib 6.82 143.6 3.16 F3V
HIP 81028 Her 6.82 424.7 27.62 G5
HIP 81757 Dra 6.82 351.8 18.97 A2
HIP 82254 Sco 6.82 751.5 86.54 B4V
HIP 82580 UMi 6.82 326.2 16.29 F0
HIP 82790 Oph 6.82 408.7 25.59 K0
HIP 83999 Oph 6.82 290.7 12.94 G5
HIP 84229 Ara 6.82 194.3 5.78 F5V
HIP 84275 Her 6.82 622.4 59.32 K0
HIP 85278 Oph 6.82 682.3 71.32 A2/A3IV
HIP 87365 Oph 6.82 840.6 108.24 K5
HIP 87494 Oph 6.82 429.7 28.29 K0
HIP 88702 Pav 6.82 — 16,292,960 B3III
HIP 89082 Her 6.82 979.4 146.96 K0
HIP 89277 Oph 6.82 376.2 21.68 A2
HIP 89342 Tel 6.82 369.4 20.89 A1V
HIP 92442 ◈ Sct 6.82 1,259.3 243.00 C5II
HIP 93350 Lyr 6.82 112.8 1.95 F8
HIP 93397 Lyr 6.82 585.6 52.53 A0
HIP 94680 Lyr 6.82 2,363.4 855.85 B9
HIP 94822 ◈ Vul 6.82 939.9 135.27 B5V SB
HIP 95083 Sgr 6.82 458.7 32.24 K0III
HIP 95116 Sge 6.82 204.5 6.40 A0+...
HIP 96065 ◈ Tel 6.82 721.6 79.73 M4III
HIP 96329 Sge 6.82 1,003.6 154.31 K7III
HIP 97050 Vul 6.82 924.0 130.74 B5V
HIP 97788 Vul 6.82 746.4 85.35 K2
HIP 99856 Aql 6.82 552.8 46.82 F5
HIP 100982 Cap 6.82 607.4 56.49 G5
HIP 101022 Aql 6.82 103.3 1.64 G0
HIP 101412 Cyg 6.82 2,673.4 1,094.46 M0
HIP 103114 Cap 6.82 795.5 96.92 K0III
HIP 103420 Cep 6.82 478.9 35.12 K2
HIP 105298 Cyg 6.82 586.6 52.72 K2
HIP 107657 Cyg 6.82 718.4 79.07 A0
HIP 107896 Peg 6.82 299.8 13.77 F6V
HIP 109862 Lac 6.82 586.6 52.72 K0
HIP 111805 Lac 6.82 124.6 2.38 G0
HIP 111807 Peg 6.82 328.8 16.55 A3
HIP 111852 Cep 6.82 847.2 109.95 F8
HIP 112981 Lac 6.82 797.4 97.36 B9
HIP 113872 PsA 6.82 1,090.8 182.31 M1III
HIP 115197 Gru 6.82 982.4 147.77 K1III
HIP 117656 Psc 6.82 657.6 66.25 K2
HIP 117672 And 6.82 874.4 117.06 K0
HIP 121 Peg 6.83 737.9 82.64 K2III
HIP 631 Tuc 6.83 407.2 25.17 K1/K2III
HIP 858 And 6.83 997.4 150.94 K4III
HIP 1456 And 6.83 668.4 67.80 K0
HIP 2415 Psc 6.83 345.1 18.08 A0
HIP 3122 Cet 6.83 228.4 7.91 F5
HIP 4703 Psc 6.83 1,076.4 175.87 K2
HIP 4878 Psc 6.83 185.8 5.24 F5
HIP 7413 Cas 6.83 1,000.5 151.91 G5
HIP 8225 Psc 6.83 516.1 40.40 A5
HIP 8914 Per 6.83 532.1 42.97 K2
HIP 12048 Cet 6.83 127.1 2.45 G5IV
← Previous Page 213 · 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.