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 26212 Ori 6.72 1,614.6 437.72 B2IV-V
HIP 26518 Ori 6.72 679.5 77.55 G5
HIP 26930 Ori 6.72 335.9 18.95 K1IV
HIP 28813 Ori 6.72 134.1 3.02 F6V
HIP 29900 CMa 6.72 1,449.6 352.86 B5IV/V
HIP 29901 ◈ Aur 6.72 1,941.4 632.70 K2
HIP 30422 Mon 6.72 121.0 2.46 F5V
HIP 30493 Mon 6.72 789.7 104.71 B8
HIP 30735 Mon 6.72 2,013.3 680.46 F0
HIP 32106 Vol 6.72 438.4 32.27 B9.5/A0V
HIP 34588 CMi 6.72 1,025.6 176.69 K2
HIP 35261 CMa 6.72 151.0 3.83 F5
HIP 35310 CMi 6.72 135.7 3.09 G0
HIP 36210 Car 6.72 74.0 0.92 G5IV-V
HIP 36452 Pup 6.72 1,568.1 413.05 K3III
HIP 36809 Pup 6.72 191.9 6.18 G2V
HIP 36982 Cha 6.72 1,212.5 246.83 M0III
HIP 37261 Pup 6.72 838.4 118.03 B6V
HIP 38226 Car 6.72 1,424.3 340.72 K0II
HIP 39477 Cnc 6.72 358.4 21.58 K0
HIP 40581 Hya 6.72 489.7 40.29 B9
HIP 41837 Vol 6.72 547.2 50.30 K0/K1III
HIP 42327 Cnc 6.72 675.3 76.56 A5V
HIP 42381 Car 6.72 1,199.1 241.43 K4III
HIP 42628 Cnc 6.72 546.3 50.12 A0III
HIP 42912 Pyx 6.72 490.5 40.40 K3III
HIP 44431 Pyx 6.72 1,190.4 237.90 B8V
HIP 44753 Vel 6.72 1,524.1 390.12 K4III
HIP 45975 Hya 6.72 726.4 88.63 G8III
HIP 46238 Pyx 6.72 720.0 87.10 B9III
HIP 47299 Cha 6.72 576.2 55.77 K0III
HIP 48009 Hya 6.72 1,069.4 192.13 K4/K5III
HIP 48552 Sex 6.72 793.6 105.78 K5
HIP 48905 UMa 6.72 842.8 119.23 K2
HIP 48975 Vel 6.72 707.5 84.02 B8/B9V
HIP 49541 Hya 6.72 535.6 48.17 A8/A9IV/V
HIP 54019 Hya 6.72 626.0 65.83 A7IV
HIP 55802 Crt 6.72 339.4 19.34 A5IV/V
HIP 55863 ◈ Cen 6.72 — 17,864,876 M2Ib-II
HIP 59135 Hya 6.72 108.4 1.97 F7V
HIP 59143 Crv 6.72 127.9 2.74 G2V
HIP 60850 Vir 6.72 441.9 32.81 A0
HIP 61544 Cen 6.72 869.7 127.06 G8III
HIP 61905 Cen 6.72 442.5 32.90 K3III
HIP 63276 Cen 6.72 644.6 69.76 A3V
HIP 64590 Cen 6.72 494.9 41.15 K1III
HIP 64781 Com 6.72 451.1 34.17 K0
HIP 66398 Hya 6.72 398.2 26.64 A
HIP 69591 Cir 6.72 1,568.1 413.05 B5V
HIP 70356 Boo 6.72 216.7 7.88 F5
HIP 70671 Aps 6.72 497.9 41.65 K0III
HIP 72427 Cen 6.72 610.8 62.63 K0III
HIP 73480 Vir 6.72 240.0 9.67 F5
HIP 73500 Aps 6.72 901.0 136.27 B5V
HIP 74016 Boo 6.72 102.9 1.78 G5
HIP 77191 Lib 6.72 520.2 45.46 K1III
HIP 78221 Nor 6.72 362.8 22.10 A2V
HIP 81608 Oph 6.72 215.1 7.78 F8
HIP 81910 Sco 6.72 151.5 3.85 G2/G3V
25 Sco Sco 6.72 706.0 83.71 K0II
← Previous Page 190 · 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.