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 93936 Aql 8.52 2,548.1 207.78 K5
HIP 11547 Ari 8.42 2,434.0 207.78 A2
HIP 99970 Pav 7.72 1,763.0 207.78 K2/K3III
HIP 95225 Aql 8.95 3,106.2 207.78 B9
HIP 116151 And 7.22 1,399.8 207.59 K2
HIP 102230 Mic 6.30 916.2 207.59 K1III
HIP 106869 Cep 7.23 1,405.8 207.59 K5III
HIP 30961 Mon 7.12 1,336.7 207.59 B2.5IV-V
HIP 39975 Mon 8.85 2,965.1 207.59 K2
HIP 9424 Cet 8.87 2,992.3 207.59 G5
HIP 33098 Gem 7.93 1,941.4 207.59 K0
HIP 35174 CMa 8.85 2,965.1 207.59 B9V
HIP 8767 Eri 8.25 2,249.4 207.59 K0II
HIP 4778 Psc 7.53 1,614.6 207.59 K0
HIP 100377 Cyg 7.64 1,698.7 207.59 K5
HIP 1131 ◈ Cep 8.25 2,249.4 207.59 M2
HIP 29355 Pup 7.22 1,399.8 207.59 K2/K3IIICN.
HIP 115959 And 7.97 1,976.7 207.59 A0
HIP 98424 Cyg 7.12 1,336.7 207.59 M3
HIP 95557 Sgr 5.71 698.4 207.59 B7IV
HIP 15753 Per 8.12 2,117.9 207.40 A0
HIP 23260 Pic 8.68 2,740.8 207.40 K2III
HIP 70418 Aps 6.42 967.8 207.40 B8V
HIP 11551 Eri 8.68 2,740.8 207.40 M1/M2III:
HIP 67868 Hya 7.83 1,853.2 207.40 K0III
HIP 110501 Peg 8.39 2,398.2 207.40 A2
HIP 36228 Car 8.70 2,764.0 207.20 B9V
HIP 27241 Ori 8.15 2,145.8 207.20 B9
HIP 100081 Cyg 7.62 1,681.2 207.20 A0
HIP 26292 Col 7.62 1,681.2 207.20 G8III
HIP 81997 Ara 7.92 1,929.9 207.20 B7II/III
HIP 116004 Psc 7.26 1,424.3 207.20 K0
HIP 45519 Cnc 8.70 2,764.0 207.20 K0
HIP 90400 Sgr 7.92 1,929.9 207.20 B5II
HIP 65185 Cen 8.49 2,508.9 207.01 K1III
HIP 49909 Vel 7.87 1,885.3 207.01 B5/B6III
HIP 15073 Cas 6.84 1,173.2 207.01 M2III
HIP 28562 Aur 5.98 789.7 207.01 K0
HIP 79011 Dra 8.18 2,174.4 207.01 K5
HIP 28718 Ori 7.27 1,430.5 207.01 B5
HIP 40937 Hya 7.28 1,436.8 207.01 K0
HIP 106429 Gru 5.57 653.6 206.82 K0III
HIP 106151 Cyg 7.29 1,443.2 206.82 A0
HIP 73354 Lup 6.10 834.2 206.82 F5III
HIP 34786 CMa 6.92 1,217.0 206.82 B4V
HIP 21648 Eri 8.33 2,329.7 206.82 G8/K0IIIwF7
HIP 45513 Vel 7.96 1,964.8 206.82 M0III
HIP 76885 Ser 8.04 2,038.5 206.82 K0
82 Vir Vir 5.03 509.6 206.82 M2III
HIP 102047 Cap 7.60 1,664.1 206.82 M2III
HIP 46593 Ant 7.40 1,517.0 206.63 K0III
HIP 80230 Nor 9.04 3,229.3 206.63 K7III
HIP 19529 Tau 6.97 1,244.9 206.63 B8
HIP 90915 Her 5.88 753.2 206.63 K5III
HIP 32708 CMa 7.43 1,538.5 206.63 K0III
HIP 33444 Lyn 6.03 807.3 206.63 K3III
HIP 57436 Crt 7.35 1,482.5 206.63 M0III
HIP 117819 Cep 8.41 2,416.0 206.63 B8
HIP 66431 Cen 7.41 1,524.1 206.63 K5III
HIP 97143 Sgr 7.35 1,482.5 206.63 K4III
← Previous Page 104 · 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.