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 91091 Tel 7.39 906.0 74.34 K0III
HIP 91588 CrA 7.39 459.4 19.12 G2IV
HIP 92143 CrA 7.39 355.7 11.46 A7V
HIP 92330 ◈ Pav 7.39 430.3 16.78 A2mA5-A9
HIP 92737 Lyr 7.39 1,109.4 111.48 K5
HIP 92837 ◈ Aql 7.39 271.3 6.67 F5
HIP 92914 Aql 7.39 364.4 12.03 K2III
HIP 93022 Lyr 7.39 847.2 65.04 A0
HIP 93812 Sgr 7.39 867.4 68.17 Ap
HIP 95192 Aql 7.39 1,098.2 109.24 K2
HIP 95388 Lyr 7.39 1,331.2 160.55 B8
HIP 95682 Aql 7.39 1,117.0 113.03 K0
HIP 96691 Vul 7.39 480.3 20.91 F6IV
HIP 96741 Sgr 7.39 657.6 39.19 A2V
HIP 97478 Vul 7.39 — 9,638,290 B2III
HIP 97540 Pav 7.39 888.7 71.58 K3III
HIP 97777 Cyg 7.39 457.4 18.97 A0
HIP 97965 Cyg 7.39 827.8 62.12 K0
HIP 98607 Cyg 7.39 474.8 20.42 A0
HIP 100543 Vul 7.39 718.4 46.77 K5
HIP 100776 Del 7.39 2,280.8 471.19 K5
HIP 101047 Del 7.39 1,598.8 231.63 A0
HIP 101054 Vul 7.39 253.6 5.83 F2
HIP 101088 Cap 7.39 653.6 38.69 K0III
HIP 101335 Aql 7.39 1,080.0 105.68 K2
HIP 102336 Mic 7.39 1,353.3 165.96 K2III
HIP 103012 Cyg 7.39 937.2 79.58 A2
HIP 103035 Cep 7.39 683.8 42.34 G7II-III
HIP 104073 Del 7.39 1,896.3 325.69 A2
HIP 105223 Cep 7.39 678.1 41.65 K0
HIP 108377 Oct 7.39 749.8 50.96 K0III
HIP 108908 PsA 7.39 911.1 75.23 B8V
HIP 109247 Lac 7.39 2,740.8 680.46 K5
HIP 109322 Peg 7.39 356.5 11.51 G0
HIP 109677 Peg 7.39 221.1 4.43 G0
HIP 110182 Lac 7.39 1,405.8 179.14 K0
HIP 110658 Peg 7.39 331.1 9.94 Am
HIP 110809 Peg 7.39 1,598.8 231.63 K2
HIP 112022 Peg 7.39 — 9,638,290 B2IV
HIP 112957 Lac 7.39 356.8 11.53 G0
HIP 113063 Peg 7.39 649.7 38.23 K1III
HIP 114164 Aqr 7.39 511.2 23.68 A0
HIP 114398 Psc 7.39 443.1 17.80 B9
HIP 114883 Cep 7.39 363.2 11.96 A5
HIP 115363 And 7.39 931.9 78.70 K0
HIP 115493 Scl 7.39 3,229.3 944.50 M1/M2III
HIP 117387 Cas 7.39 409.7 15.21 A0
HIP 118107 Scl 7.39 1,744.1 275.68 K1III
HIP 55 Tuc 7.40 211.8 4.03 G2IV/V
HIP 785 Tuc 7.40 753.2 50.96 M2III
HIP 1732 Cet 7.40 194.0 3.38 G1V
HIP 2374 Psc 7.40 776.6 54.15 K0
HIP 3541 And 7.40 939.9 79.29 B8
HIP 4051 Cas 7.40 748.1 50.26 G5
HIP 4736 Cet 7.40 647.1 37.60 A3
HIP 6064 Cas 7.40 — 9,549,926 B1V
HIP 6076 Phe 7.40 393.4 13.89 A7m...
HIP 7419 Per 7.40 886.3 70.53 K2
HIP 7745 Cas 7.40 1,802.0 291.61 B8Iab
HIP 7855 And 7.40 231.6 4.82 F8
← Previous Page 386 · 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.