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 94055 Aql 8.54 2,861.0 257.04 K2
87 Vir Vir 5.41 676.7 257.04 M2III
HIP 43040 Pyx 8.56 2,886.3 257.04 K2III
HIP 98428 Sge 7.66 1,907.3 257.04 B2V
HIP 37366 Pup 7.93 2,160.0 257.04 B9
HIP 73131 Lup 7.66 1,907.3 257.04 A0V
HIP 102770 ◈ Aqr 6.24 991.4 256.80 M3
HIP 87711 Sco 7.55 1,812.0 256.80 K1III
HIP 63297 Dra 6.44 1,087.2 256.80 K0
HIP 111649 Peg 6.30 1,019.2 256.80 K5
HIP 1941 ◈ Psc 7.55 1,812.0 256.80 M...
HIP 1925 Cas 7.55 1,812.0 256.80 B9
HIP 113684 Cas 6.24 991.4 256.80 K2II
HIP 17141 Tau 8.72 3,106.2 256.80 K2
HIP 55828 Hya 8.72 3,106.2 256.80 K5
HIP 37302 Pup 8.08 2,313.2 256.80 K1III
HIP 84049 Her 8.58 2,912.1 256.80 K2
HIP 50719 Hya 6.71 1,230.8 256.80 G8II
HIP 1974 Psc 8.64 2,992.3 256.57 A0
HIP 19770 Cam 7.30 1,614.6 256.57 K0
HIP 35181 Pup 5.64 751.5 256.57 K4III
HIP 99196 Cyg 8.02 2,249.4 256.57 B9.5V
HIP 99728 Cyg 8.60 2,938.3 256.57 B9IV
HIP 98548 Aql 7.48 1,753.5 256.33 K2
HIP 89060 Sgr 7.89 2,117.9 256.33 B1Ib
HIP 73504 Cir 7.60 1,853.2 256.33 B8II
HIP 86552 Ara 5.78 801.4 256.33 A0V
HIP 26032 ◈ Ori 7.89 2,117.9 256.33 C6II
HIP 20918 Cam 8.45 2,740.8 256.33 F0
HIP 17510 Cep 8.31 2,568.2 256.09 K0
HIP 18067 Cam 6.31 1,022.4 256.09 B9IVp
HIP 92098 Lyr 6.06 911.1 256.09 B6V
HIP 81144 Nor 7.39 1,681.2 256.09 A0Ia
HIP 85687 Her 7.69 1,929.9 256.09 K5
HIP 87771 Sco 7.92 2,145.8 256.09 K1III
Thuban 11Alp Dra Dra 3.67 303.1 256.09 A0III SB
HIP 82158 Dra 7.05 1,436.8 255.86 K2
HIP 91361 Lyr 6.92 1,353.3 255.86 A0
HIP 71492 ◈ Cen 6.78 1,269.1 255.86 G0/G1Ib
HIP 46696 UMa 7.53 1,792.1 255.86 A2
HIP 7289 ◈ Tri 6.93 1,359.0 255.62 M4III
HIP 50179 Vel 7.73 1,964.8 255.62 G5III
HIP 85389 Ara 5.28 635.8 255.62 B8V
HIP 7939 ◈ Cas 6.69 1,217.0 255.62 B8IIIp (Si)
HIP 56180 Cen 7.21 1,545.8 255.62 B8/B9IV
7Zet1CrB CrB 4.64 473.4 255.62 B7V+...
HIP 23404 Ori 7.17 1,517.0 255.39 B8
HIP 93960 Lyr 8.01 2,233.9 255.39 A0
HIP 86432 ◈ Sco 7.16 1,510.0 255.39 B3IV/V
HIP 6016 Cas 7.68 1,918.6 255.39 K2
HIP 33431 Car 7.63 1,874.5 255.15 M1III
HIP 99900 Cap 8.28 2,528.3 255.15 K5
HIP 115218 Cas 6.39 1,058.9 255.15 K1V
HIP 58964 Cen 8.23 2,470.9 255.15 K2III
HIP 35201 ◈ CMa 8.23 2,470.9 255.15 M1/M2III
HIP 111504 Oct 6.15 948.1 255.15 K1III
HIP 69584 Cir 6.95 1,370.4 255.15 B5III
HIP 29037 Ori 8.15 2,380.7 254.92 B9
HIP 38691 Mon 7.34 1,639.0 254.92 B8
HIP 89466 Her 8.15 2,380.7 254.92 K0
← Previous Page 77 · 109,400 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.