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 30822 ◈ Aur 7.83 582.4 20.49 F0
HIP 1543 ◈ Cas 7.83 520.2 16.35 F0
HIP 71820 ◈ Vir 7.83 662.9 26.55 A2
HIP 10304 ◈ Phe 7.84 562.3 18.93 F0V
HIP 103026 ◈ Aqr 7.84 1,325.8 105.20 M4III:
HIP 91224 ◈ Ser 7.84 1,614.6 156.03 A0p
HIP 18912 ◈ Per 7.84 506.5 15.36 A0p
HIP 17042 ◈ Per 7.84 584.5 20.46 A0
HIP 31719 ◈ Aur 7.84 1,055.5 66.68 M5
HIP 14450 ◈ Per 7.84 832.0 41.46 B9V
HIP 70290 ◈ Cen 7.84 1,976.7 233.99 M5II
HIP 98719 ◈ Aql 7.84 — 6,367,955 Ape
HIP 50463 ◈ Vel 7.84 458.1 12.57 A3mA6-A7
HIP 50272 ◈ Car 7.84 — 6,367,955 B1Ia
HIP 48027 ◈ Cha 7.84 942.6 53.21 M2III
HIP 61507 ◈ Cen 7.84 2,001.0 239.66 M2III
HIP 103447 ◈ Aqr 7.84 1,874.5 210.28 M...
HIP 116601 ◈ Phe 7.84 918.7 50.54 M4III
HIP 84745 ◈ Sco 7.84 2,363.4 334.50 B2V:ne
HIP 111957 ◈ Peg 7.84 1,152.5 79.51 M...
HIP 108426 ◈ Cep 7.85 2,203.8 288.14 G0
HIP 20436 ◈ Per 7.85 1,802.0 192.66 K5
HIP 37927 ◈ Pup 7.85 1,173.2 81.66 A8V
HIP 112250 ◈ Peg 7.85 2,508.9 373.25 K2
HIP 34852 ◈ CMa 7.85 2,764.0 453.31 B2Vn(e)
HIP 86650 ◈ Sco 7.85 556.6 18.38 A9V
HIP 87797 ◈ Oph 7.85 1,953.0 226.15 M...
HIP 52291 ◈ Car 7.85 — 6,309,573 M2III
HIP 13221 ◈ Cas 7.85 1,792.1 190.55 B8
HIP 90907 ◈ Sct 7.85 — 6,309,573 B1Ia
HIP 47727 ◈ UMa 7.85 174.2 1.80 G2Vn
HIP 103246 ◈ Del 7.85 869.7 44.87 A0p
HIP 22260 ◈ Men 7.85 1,462.6 126.82 Fm...
HIP 62355 ◈ CVn 7.85 1,449.6 124.62 M2III
HIP 10463 ◈ Per 7.85 1,802.0 192.66 B2IV-Ve
HIP 75641 ◈ Boo 7.86 1,496.1 131.58 B9
HIP 34326 ◈ Mon 7.86 1,411.9 117.17 N5
HIP 98826 ◈ Aql 7.86 — 6,251,727 B9
HIP 13968 ◈ Cet 7.86 372.7 8.17 G2III
HIP 52567 ◈ Ant 7.86 731.3 31.42 A5/7V (+F)
HIP 13276 ◈ Cas 7.86 2,346.4 323.59 B9III
HIP 46919 ◈ UMa 7.86 377.9 8.39 G5
HIP 117647 ◈ And 7.86 732.9 31.56 F0
HIP 94169 ◈ Aql 7.86 — 6,251,727 A0
HIP 41980 ◈ Pyx 7.86 — 6,251,727 B3III
HIP 41278 ◈ Pup 7.86 228.1 3.06 G1V
HIP 39290 ◈ Pup 7.87 1,489.3 129.18 B5V
HIP 37961 ◈ Cam 7.87 1,853.2 199.89 B9
HIP 37595 ◈ Cam 7.87 1,164.8 79.00 K0
HIP 56249 ◈ Cen 7.87 — 6,194,411 B9.5V
HIP 80830 ◈ Nor 7.87 782.1 35.61 M2/M3III
HIP 59653 ◈ Cru 7.87 2,380.7 329.91 B5Ve
HIP 56851 ◈ Cen 7.87 548.2 17.49 G8IV
HIP 75994 ◈ Aps 7.87 471.3 12.93 F3V
HIP 85905 ◈ Oph 7.87 916.2 48.89 M...
HIP 68023 ◈ Vir 7.87 1,113.2 72.18 Kp...
HIP 10541 ◈ Per 7.87 — 6,194,411 B0III
HIP 10522 ◈ Cet 7.87 2,160.0 271.64 M3/M4III
HIP 33274 ◈ CMa 7.88 1,907.3 209.89 B8III
HIP 17590 ◈ Cam 7.88 1,038.7 62.23 M0III
← Previous Page 46 · 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.