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 25351 Men 7.17 117.0 1.52 F8V
HIP 26783 Aur 7.17 425.2 20.06 A
HIP 26831 Lep 7.17 436.0 21.09 A2/A3III
HIP 27076 Ori 7.17 432.0 20.70 A3
HIP 27115 Ori 7.17 1,863.7 385.48 B8
HIP 27451 Ori 7.17 301.2 10.06 A5
HIP 27887 Pic 7.17 42.4 0.20 K3V
HIP 28056 Ori 7.17 516.1 29.54 A0V
HIP 28557 Col 7.17 640.8 45.54 A4V
HIP 28839 Pic 7.17 789.7 69.18 G8III
HIP 28919 Aur 7.17 1,025.6 116.73 B8
HIP 29425 ◈ Gem 7.17 — 11,803,206 M2Iabpe comp
HIP 30390 CMa 7.17 — 11,803,206 M1III
HIP 31956 Aur 7.17 221.1 5.43 F5
HIP 33611 CMa 7.17 1,399.8 217.37 B2V
HIP 33757 Gem 7.17 1,128.6 141.38 A0
HIP 34596 CMa 7.17 3,197.6 1,134.49 G8II
HIP 34686 Vol 7.17 970.7 104.52 K2III
HIP 34879 CMa 7.17 118.9 1.57 G1V
HIP 34992 Car 7.17 189.2 3.97 F3V
HIP 35011 Gem 7.17 1,076.4 128.59 K0
HIP 35437 Pup 7.17 147.6 2.42 F6V
HIP 35610 CMa 7.17 426.9 20.23 A7IV
HIP 35614 CMi 7.17 799.4 70.93 G5
HIP 36376 Gem 7.17 1,101.9 134.77 A3
HIP 36647 Gem 7.17 435.5 21.05 K1III
HIP 37563 Car 7.17 107.0 1.27 G2IV
HIP 38083 Mon 7.17 242.9 6.55 A3
HIP 38109 Cam 7.17 1,169.0 151.64 K0
HIP 38826 Pup 7.17 517.7 29.73 K0III
HIP 39214 Pup 7.17 549.1 33.45 A5IV
HIP 39468 Pup 7.17 193.8 4.17 F5V
HIP 39850 Car 7.17 584.5 37.91 Fm...
HIP 39979 Vel 7.17 — 11,803,206 K2/K3III
HIP 40280 Cnc 7.17 252.1 7.05 F8
HIP 40755 Vel 7.17 825.7 75.65 K2III
HIP 40952 Pup 7.17 91.5 0.93 G8:III...
HIP 41254 Vol 7.17 220.1 5.38 G3IV/V
HIP 41479 Hya 7.17 130.7 1.89 G0
HIP 42412 Hya 7.17 438.4 21.32 A0
HIP 43949 Lyn 7.17 553.7 34.01 K0
HIP 44107 UMa 7.17 640.8 45.54 G5
HIP 45740 Cnc 7.17 628.4 43.81 K0
HIP 46617 Ant 7.17 302.6 10.16 F2IV
HIP 46730 Ant 7.17 1,309.9 190.37 G8III
HIP 49457 Car 7.17 547.2 33.24 K2III
HIP 50671 Hya 7.17 106.8 1.26 G1V
HIP 51424 ◈ Car 7.17 1,254.4 174.58 M2III
HIP 52698 Hya 7.17 682.3 51.67 K1III
HIP 52916 Ant 7.17 558.5 34.61 B9.5V
HIP 53062 Dra 7.17 277.1 8.52 A3
HIP 56186 UMa 7.17 130.3 1.88 F5
HIP 57785 UMa 7.17 — 11,803,206 G8III
HIP 59030 Mus 7.17 229.2 5.83 G0V
HIP 63267 Vir 7.17 613.1 41.69 A3
HIP 64162 Cen 7.17 561.4 34.96 K0/K1III
HIP 64355 CVn 7.17 622.4 42.97 K0
HIP 65069 ◈ Com 7.17 273.9 8.32 F5
Dofida Cen 7.17 123.8 1.70 G2V
HIP 67652 Cen 7.17 215.1 5.14 F7/F8V
← Previous Page 308 · 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.