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 91137 Sgr 6.86 436.0 28.05 A0V
HIP 92262 Sct 6.86 173.8 4.46 F6V
HIP 92336 Dra 6.86 403.7 24.05 A2
HIP 93204 Lyr 6.86 686.6 69.63 A2
HIP 93499 Dra 6.86 672.5 66.74 K0
HIP 93546 Tel 6.86 204.4 6.17 K0IV
HIP 93972 Aql 6.86 563.3 46.86 K0
HIP 94045 Sgr 6.86 767.4 86.94 B8IV
HIP 94505 Dra 6.86 499.5 36.81 A2
HIP 94940 ◈ Sgr 6.86 1,744.1 449.16 C
HIP 96558 Sgr 6.86 533.8 42.07 G8/K0III
HIP 96577 Sgr 6.86 407.7 24.55 K0III
HIP 96932 Sgr 6.86 143.7 3.05 F5V
HIP 98291 Sge 6.86 867.4 111.07 B8
HIP 99035 Cyg 6.86 1,025.6 155.31 K5III
HIP 99873 Del 6.86 228.9 7.73 F0
HIP 100116 Sge 6.86 1,583.3 370.17 K5
HIP 100475 Cyg 6.86 356.8 18.79 A0
HIP 101263 Vul 6.86 662.9 64.86 A3
HIP 103654 Pav 6.86 129.2 2.46 G5IV
HIP 103748 Mic 6.86 495.7 36.27 A3III/IV
HIP 103850 Cyg 6.86 1,080.0 172.19 K5Ib
HIP 104293 Aqr 6.86 256.2 9.69 A3
HIP 104434 Mic 6.86 521.0 40.07 K0III
HIP 105986 Cyg 6.86 1,672.6 413.05 B3III
HIP 106115 Cap 6.86 633.3 59.21 K4III
HIP 106230 Cep 6.86 164.5 3.99 K0
HIP 106586 PsA 6.86 175.3 4.53 F5V
HIP 107300 Ind 6.86 147.6 3.22 F6IV/V
HIP 108029 Cep 6.86 2,718.0 1,090.44 K0
HIP 109304 Lac 6.86 787.8 91.62 A0
HIP 110159 Peg 6.86 435.5 28.00 K2
HIP 110706 Cep 6.86 1,009.8 150.52 M4III
HIP 112525 Ind 6.86 385.1 21.90 A7IV
HIP 112932 Peg 6.86 193.4 5.53 F5
HIP 113085 Aqr 6.86 1,083.6 173.30 K2/K3III
HIP 114010 Aqr 6.86 620.1 56.75 K0III
HIP 116421 Peg 6.86 107.5 1.71 F9V
HIP 118179 Tuc 6.86 275.5 11.20 G8IV
HIP 619 And 6.87 527.8 40.74 G5
HIP 981 Cas 6.87 391.1 22.37 F0
HIP 2243 ◈ And 6.87 723.2 76.49 A2p...
HIP 2517 Psc 6.87 1,087.2 172.82 K5III
HIP 3042 Tuc 6.87 380.6 21.18 A1m...
HIP 4006 Cas 6.87 — 15,559,656 B5Ia
HIP 4058 And 6.87 417.1 25.44 K2
HIP 5232 Cas 6.87 569.2 47.38 A2V...
HIP 6139 Cas 6.87 584.5 49.98 G5
HIP 6441 Psc 6.87 847.2 105.00 G5
HIP 7330 ◈ Scl 6.87 1,503.0 330.52 M0III
HIP 8856 Per 6.87 653.6 62.46 K0
HIP 9151 And 6.87 143.8 3.03 F5
HIP 9242 Cas 6.87 763.8 85.35 G5
HIP 9359 And 6.87 883.9 114.29 G5
HIP 9517 Ari 6.87 494.9 35.84 K0
HIP 10787 Cet 6.87 807.3 95.32 K5III
HIP 15615 Cas 6.87 1,019.2 151.91 K0
HIP 15869 Eri 6.87 643.3 60.53 A2/A3IV/V
HIP 16986 Per 6.87 1,664.1 405.14 B9
HIP 17601 Eri 6.87 460.0 30.96 K0
← Previous Page 223 · 119,625 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.