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 63085 Mus 7.50 484.6 19.23 A4IV/V
HIP 63891 Com 7.50 662.9 35.97 K0III
HIP 64260 Cen 7.50 494.2 19.99 G8III
HIP 64859 Cen 7.50 552.8 25.03 A3IV
HIP 65953 ◈ CVn 7.50 865.1 61.26 M0
HIP 66083 CVn 7.50 642.0 33.76 K0
HIP 66109 Cen 7.50 376.2 11.59 F8V
HIP 66305 Com 7.50 326.5 8.73 F2
HIP 67060 Vir 7.50 3,166.6 821.11 B1Ib
HIP 67381 UMa 7.50 382.4 11.97 F0
HIP 67504 CVn 7.50 945.4 73.18 K3III
HIP 67541 Vir 7.50 1,863.7 284.45 M1III
HIP 68825 UMi 7.50 626.0 32.09 K0
HIP 69194 Boo 7.50 621.2 31.59 A2
HIP 69509 Boo 7.50 988.4 79.95 A0
HIP 69522 Vir 7.50 474.1 18.40 K0
HIP 71367 Vir 7.50 676.7 37.50 K0III
HIP 72604 Boo 7.50 122.9 1.24 G5
HIP 72652 Lib 7.50 553.7 25.10 K1III
HIP 74220 Lup 7.50 1,069.4 93.67 B9V
HIP 74458 Dra 7.50 390.1 12.46 A2
HIP 75386 Oct 7.50 386.9 12.26 G6III
HIP 75967 Lup 7.50 423.0 14.66 K0III
HIP 76098 Lup 7.50 654.9 35.12 A0V
HIP 76558 CrB 7.50 611.9 30.65 K2
HIP 76635 Ser 7.50 181.9 2.71 G0V
HIP 77309 Dra 7.50 771.1 48.66 A2
HIP 77624 CrB 7.50 553.7 25.10 K0
HIP 78563 ◈ Sco 7.50 931.9 71.12 M2/M3III
HIP 79452 CrB 7.50 595.2 29.00 K2
HIP 79862 CrB 7.50 123.2 1.24 G0
HIP 80525 Nor 7.50 2,313.2 438.13 K3III
HIP 80734 Her 7.50 515.3 21.74 K0
HIP 80939 Her 7.50 386.0 12.20 A3...
HIP 81096 Nor 7.50 1,173.2 112.72 K3III
HIP 81459 Her 7.50 205.4 3.45 G5V
HIP 81541 Oph 7.50 642.0 33.76 K0
HIP 81704 Her 7.50 243.0 4.84 F0
HIP 82397 Sco 7.50 347.7 9.90 A3V
HIP 82778 Ara 7.50 801.4 52.58 K1III
HIP 82962 Her 7.50 635.8 33.08 K0
HIP 83456 Oph 7.50 632.1 32.72 K2/K3III
HIP 85499 Ara 7.50 876.8 62.92 M0III
HIP 85673 Sco 7.50 758.5 47.12 F2/F3III
HIP 86302 Her 7.50 167.0 2.28 G0
HIP 88025 Pav 7.50 598.5 29.32 K0III
HIP 89998 Lyr 7.50 1,812.0 268.91 K5
HIP 90584 Oph 7.50 449.3 16.52 G0
HIP 91039 Dra 7.50 867.4 61.60 K0
HIP 91263 Dra 7.50 791.6 51.33 A0
HIP 91507 Lyr 7.50 151.1 1.87 F5
HIP 92227 Sct 7.50 2,329.7 444.22 M0/M1III
HIP 92236 Aql 7.50 869.7 61.94 B9
HIP 92505 ◈ Sgr 7.50 — 8,709,636 B8II/III
HIP 93481 Oct 7.50 913.6 68.36 Ap...
HIP 93915 Tel 7.50 488.3 19.52 A9/F0IV
HIP 94328 Lyr 7.50 675.3 37.33 A0
HIP 95563 Tel 7.50 883.9 63.97 K3III
HIP 96053 Sgr 7.50 339.7 9.45 F5/F6V
HIP 96063 Cyg 7.50 710.6 41.34 K3III
← Previous Page 429 · 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.