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 57649 ◈ Cen 10.19 — 731,139 G5
HIP 45266 ◈ Hya 10.19 1,430.5 14.06 CVIIe
HIP 97281 ◈ Vul 10.19 — 731,139 WN+...
HIP 47177 ◈ Vel 10.20 — 724,436 —
HIP 20387 ◈ Tau 10.20 627.2 2.68 F8Ve-K1Ve(T)
HIP 30449 ◈ Aur 10.20 — 724,436 CVIIe+
HIP 99503 ◈ Aql 10.20 — 724,436 M3e-M5.5e
HIP 44995 ◈ Cnc 10.20 — 724,436 M6.5e-M9e
HIP 23873 ◈ Aur 10.20 211.5 0.30 G5Ve(T)
HIP 26247 ◈ Cam 10.21 — 717,794 M6
HIP 116103 ◈ Phe 10.21 506.5 1.73 F8
HIP 12235 ◈ Cas 10.21 888.7 5.33 A3 + K
HIP 25299 ◈ Ori 10.21 1,575.6 16.75 A5III:var
HIP 76551 ◈ CrB 10.21 — 717,794 G0
HIP 101985 ◈ Mic 10.22 1,284.1 11.03 M4e
HIP 30618 ◈ Aur 10.22 330.1 0.73 F8
HIP 31624 ◈ Mon 10.22 — 711,214 —
HIP 73708 ◈ Lib 10.22 908.5 5.52 R6
HIP 76658 ◈ CrB 10.23 679.5 3.06 A8V SB
HIP 98553 ◈ Aql 10.23 — 704,693 F6Iab
HIP 66189 ◈ Cen 10.23 1,364.7 12.34 —
HIP 23727 ◈ Cep 10.23 — 704,693 A5V comp
HIP 44216 ◈ Car 10.24 404.2 1.07 —
HIP 94438 ◈ Lyr 10.24 — 698,232 M5IIIevar
HIP 23165 ◈ Ori 10.24 2,912.1 55.67 C0ev
HIP 39144 ◈ Pup 10.24 — 698,232 F8
HIP 73612 ◈ Boo 10.25 1,744.1 19.79 A0
HIP 88775 ◈ Pav 10.25 — 691,831 Ke
HIP 50615 ◈ Car 10.25 2,398.2 37.39 A1IV
HIP 28368 ◈ Cam 10.25 44.1 0.01 M1
HIP 97184 ◈ Aql 10.26 — 685,488 M4e
HIP 99820 ◈ Cyg 10.26 2,051.3 27.11 A3e+G5
HIP 63911 ◈ Mus 10.26 698.4 3.14 Fp
HIP 58907 ◈ Hya 10.26 1,545.8 15.40 A2:
HIP 102141 ◈ Mic 10.27 34.9 0.01 Mpe
HIP 98542 ◈ Aql 10.27 2,218.7 31.42 R4
HIP 67359 ◈ Cen 10.27 3,229.3 66.56 M6II:e
HIP 100582 ◈ Cyg 10.27 1,038.7 6.89 N0v
HIP 65660 ◈ Vir 10.27 632.1 2.55 A0p
HIP 114290 ◈ Peg 10.27 — 679,204 A6.7
HIP 2552 ◈ Cas 10.27 32.8 0.01 M2.5Ve
HIP 88242 ◈ Her 10.28 2,568.2 41.73 F3II-III
HIP 89972 ◈ Her 10.29 456.8 1.31 A0
HIP 115986 ◈ Peg 10.29 2,695.5 45.54 F0V
HIP 112460 ◈ Lac 10.29 16.7 0.00 M4.5Ve
HIP 82977 ◈ Oph 10.29 478.2 1.43 A1IV
HIP 90092 ◈ Dra 10.29 2,160.0 29.24 A5
HIP 22943 ◈ Ori 10.29 — 666,807 G4
HIP 32915 ◈ Mon 10.29 755.0 3.57 G7.5
HIP 117239 ◈ Peg 10.30 — 660,693 M0
HIP 226 ◈ Scl 10.30 — 660,693 F0/F2V
HIP 63706 ◈ CVn 10.30 — 660,693 K3III
HIP 97923 ◈ Sgr 10.31 — 654,636 F5
HIP 71313 ◈ Cir 10.31 — 654,636 A0
HIP 57009 ◈ Hya 10.31 — 654,636 Me
HIP 77157 ◈ Lup 10.31 460.7 1.31 Ge
HIP 102088 ◈ Cyg 10.31 — 654,636 WNs...
HIP 21467 ◈ Tau 10.31 718.4 3.18 A7V
HIP 11582 ◈ For 10.31 2,249.4 31.13 C8
HIP 86509 ◈ Oph 10.32 143.3 0.13 K7V
← Previous Page 90 · 5,992 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.