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 42679 ◈ Vel 5.20 — 72,443,596 B5Iab
28 And ◈ And 5.20 204.7 28.55 A7III
Iot Ara ◈ Ara 5.21 934.5 589.39 B2IIIne
3 Vul ◈ Vul 5.22 393.0 103.28 B6III
45 Her ◈ Her 5.22 393.4 103.47 B9p (Cr)
11 Cam ◈ Cam 5.22 685.2 313.91 B2.5Ve
32 Vir ◈ Vir 5.22 252.6 42.66 A8m
67 UMa ◈ UMa 5.22 111.8 8.36 A7m
10 CMa ◈ CMa 5.23 — 70,469,307 B2V
HIP 39970 ◈ Vel 5.23 1,105.6 809.84 B1IVe
HIP 82493 ◈ Sco 5.23 — 70,469,307 O9e
17Sig CrB ◈ CrB 5.23 68.8 3.13 F8V
Taiyi 8 Dra ◈ Dra 5.23 95.5 6.05 A5n
HIP 44337 ◈ Vel 5.23 368.5 89.95 Ap Si
76Kap Cnc ◈ Cnc 5.23 531.2 186.90 B8IIIMNp
20 Eri ◈ Eri 5.24 486.8 155.60 B8/B9III
Rho Phe ◈ Phe 5.24 242.1 38.48 F2III
HIP 80620 ◈ Oph 5.24 577.3 218.78 M2 comp
1Ome Vir ◈ Vir 5.24 497.2 162.18 M4III
HIP 39487 ◈ Pup 5.25 2,090.7 2,841.84 M2II
96 Her ◈ Her 5.25 939.9 574.38 B3IV
12 Lac ◈ Lac 5.25 1,342.2 1,171.66 B2IIIv SB
58 Tau ◈ Tau 5.26 153.1 15.11 F0V
13 Boo ◈ Boo 5.26 549.1 194.27 M2III
18 Cep ◈ Cep 5.26 424.1 115.88 M5III
HIP 53154 ◈ Car 5.26 — 68,548,823 B9Ia
HIP 62027 ◈ Cru 5.27 1,217.0 945.37 B2pe
61Tau1Ari ◈ Ari 5.27 508.8 165.35 B5IV
HIP 50070 ◈ Vel 5.27 169.3 18.30 A7V
Iot TrA ◈ TrA 5.28 126.6 10.13 F4IV
HIP 58587 ◈ Crv 5.28 3,166.6 6,344.54 B2IV
HIP 26868 ◈ Col 5.29 428.6 115.13 B9/B9.5V
17 Com ◈ Com 5.29 237.7 35.42 A0p
14 Hya ◈ Hya 5.30 450.5 126.01 B9MNp...
82 Peg ◈ Peg 5.30 182.7 20.74 A4Vn
36 Lyn ◈ Lyn 5.30 581.4 209.89 B8IIIMNp
HIP 80945 ◈ Sco 5.31 2,718.0 4,545.69 B1Ia
HIP 15770 ◈ Per 5.32 541.8 178.98 B5V
HIP 97749 ◈ Sgr 5.32 301.4 55.41 A0p
40 Tau ◈ Tau 5.32 640.8 250.26 B3V
Xi Oct ◈ Oct 5.32 492.7 148.05 B6IV
HIP 93124 ◈ Aql 5.33 1,545.8 1,444.11 F8Ib
71 Peg ◈ Peg 5.33 520.2 163.53 M5IIIa
13 Sge ◈ Sge 5.33 1,019.2 627.48 M4IIIa
HIP 90074 ◈ Sgr 5.33 556.6 187.24 B7Ib/II
13 Peg ◈ Peg 5.34 109.0 7.11 F2III-IV
20Chi Ser ◈ Ser 5.34 219.8 28.92 A0p Sr
HIP 113327 ◈ Lac 5.34 821.6 404.02 B4IIIpe
56 Tau ◈ Tau 5.34 326.2 63.68 A0p Si
HIP 80782 ◈ Nor 5.35 1,822.1 1,969.70 B1.5Iap
HIP 52405 ◈ Car 5.36 — 62,517,269 B2.5Ia
HIP 26063 ◈ Ori 5.36 1,469.2 1,268.24 B1V
57 Psc ◈ Psc 5.36 776.6 354.49 M4III
HIP 89605 ◈ Tel 5.36 760.3 339.78 B3IIIpe
HIP 92989 ◈ CrA 5.36 430.3 108.84 B3V
Iot Tuc ◈ Tuc 5.36 304.3 54.40 G5III
HIP 79804 ◈ Dra 5.37 739.6 318.57 M4IIIa
HIP 73223 ◈ Aps 5.37 374.5 81.66 K4III
27 Cyg ◈ Cyg 5.38 78.1 3.52 K0IV
HIP 92202 ◈ Sct 5.38 — 61,376,201 K0Ibpvar
← Previous Page 8 · 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.