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 43493 ◈ Vel 7.62 — 7,798,301 M2/M3III
HIP 68692 ◈ Cir 7.62 489.0 17.52 A5IV/Vs
HIP 100935 ◈ Mic 7.62 686.6 34.58 M7/M8III
HIP 21213 ◈ Cae 7.63 434.9 13.74 A4V
HIP 36227 ◈ Pup 7.63 — 7,726,806 B9Ib
HIP 33200 ◈ CMa 7.63 1,140.4 94.45 B3Ve
HIP 53806 ◈ Vel 7.63 1,052.1 80.39 B9V
HIP 26983 ◈ Pic 7.63 1,221.6 108.34 M2/M3III
HIP 44612 ◈ Vel 7.63 1,117.0 90.61 A2/3III(m)
HIP 96836 ◈ Cyg 7.63 1,832.3 243.89 C6.4e
HIP 90113 ◈ Sgr 7.63 2,548.1 471.63 K5/M0III:
HIP 96480 ◈ Cyg 7.64 1,090.8 85.66 B9
HIP 107823 ◈ Oct 7.64 967.8 67.42 B8V
HIP 52624 ◈ Vel 7.64 970.7 67.80 A3IV/V
HIP 70020 ◈ Vir 7.64 376.6 10.20 F2
HIP 4488 ◈ Cet 7.64 911.1 59.76 A0p...
HIP 76844 ◈ CrB 7.64 1,113.2 89.21 M5
HIP 113907 ◈ Cep 7.64 2,077.4 310.74 B1:V:var
HIP 54155 ◈ Leo 7.64 85.7 0.53 G5
HIP 74337 ◈ Boo 7.64 1,284.1 118.69 M0
HIP 17873 ◈ Tau 7.64 322.9 7.50 G0
HIP 60333 ◈ Vir 7.64 720.0 37.33 M...
HIP 32408 ◈ CMa 7.64 1,456.1 152.62 B5III
HIP 49784 ◈ Ant 7.64 529.5 20.17 A0V
HIP 30270 ◈ Aur 7.64 232.3 3.88 F8
HIP 90001 ◈ Sgr 7.64 2,398.2 413.81 B9V:
HIP 114025 ◈ Peg 7.64 658.9 31.25 G8II
HIP 44800 ◈ Cha 7.64 261.1 4.91 F7V
HIP 62484 ◈ Com 7.64 1,132.5 92.30 M0
HIP 21626 ◈ Tau 7.64 1,598.8 183.99 B2.5Vne
HIP 67013 ◈ Cen 7.64 260.1 4.87 K1Vp
HIP 37985 ◈ Pup 7.65 1,230.8 108.04 K7III
HIP 108859 ◈ Peg 7.65 161.9 1.87 F8
HIP 115262 ◈ Cep 7.65 668.4 31.86 F2
HIP 31062 ◈ Pic 7.65 598.5 25.54 K1III/IVp
HIP 107594 ◈ Cap 7.65 691.0 34.04 B9IIIsp...
HIP 108546 ◈ Cep 7.65 — 7,585,776 B1V
HIP 62738 ◈ UMa 7.65 1,140.4 92.73 M2
HIP 59136 ◈ CVn 7.65 1,698.7 205.68 K4III
HIP 60500 ◈ Vir 7.65 1,538.5 168.73 M4III
HIP 22513 ◈ Per 7.65 1,144.4 93.41 M0
HIP 102720 ◈ Vul 7.65 633.3 28.60 M3
HIP 96176 ◈ Sgr 7.66 1,124.7 89.37 M2III
HIP 16941 ◈ Cam 7.66 1,169.0 96.56 B2Vne
HIP 7576 ◈ Cet 7.66 78.1 0.43 G5
HIP 26284 ◈ Lep 7.66 1,545.8 168.89 C
HIP 88326 ◈ Ser 7.66 886.3 55.51 M2III
HIP 25284 ◈ Aur 7.66 2,489.7 438.13 B5
HIP 80478 ◈ Sco 7.66 1,336.7 126.24 Ap Si
HIP 44050 ◈ Cnc 7.66 791.6 44.30 M4III
HIP 92151 ◈ Aql 7.66 2,489.7 438.13 M...
HIP 5521 ◈ And 7.66 88.3 0.55 K0
HIP 22578 ◈ Tau 7.66 1,181.7 98.63 C5II
HIP 22247 ◈ Cae 7.66 — 7,516,229 C
HIP 87063 ◈ Sco 7.66 — 7,516,229 C
HIP 2180 ◈ And 7.67 — 7,447,320 N0v
HIP 4907 ◈ Cas 7.67 83.2 0.48 G5
HIP 107242 ◈ Cyg 7.67 — 7,447,320 C6II
HIP 38173 ◈ Pup 7.67 2,992.3 626.90 A0Ia(p)
HIP 67566 ◈ Cen 7.67 — 7,447,320 F8Ib/II
← Previous Page 41 · 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.