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 54196 LMi 7.60 180.9 2.44 G0
HIP 54671 Cen 7.60 565.3 23.86 A2IV
HIP 55167 Leo 7.60 653.6 31.89 K2
HIP 55399 Cen 7.60 282.6 5.96 F3V
HIP 56216 UMa 7.60 1,832.3 250.73 K5
HIP 56832 Vir 7.60 114.3 0.98 G5
HIP 56897 Cen 7.60 — 7,943,282 O7
HIP 57078 Crt 7.60 191.4 2.74 F5V
HIP 57293 Cen 7.60 823.6 50.68 A1V
HIP 57840 Cen 7.60 588.7 25.87 K0III
HIP 58064 Cen 7.60 1,069.4 85.43 K2/K3III
HIP 58093 Vir 7.60 195.5 2.85 G5
HIP 58498 Cru 7.60 — 7,943,282 K4/K5Ib:
HIP 59546 Cru 7.60 1,545.8 178.48 B9.5/A0IV
HIP 60154 Vir 7.60 973.6 70.79 K0
HIP 60709 Cen 7.60 803.3 48.17 A3V
HIP 61353 Vir 7.60 326.5 7.96 A5
HIP 61696 CVn 7.60 891.1 59.32 A0p
HIP 61925 CVn 7.60 1,083.6 87.66 K0III
HIP 62206 Vir 7.60 1,062.4 84.26 K0
HIP 62624 Cru 7.60 2,329.7 405.14 B9.5IV
HIP 62968 Cen 7.60 595.2 26.45 F3/F5III
HIP 64585 Cen 7.60 862.8 55.62 K0III
HIP 64932 Vir 7.60 658.9 32.42 K0
HIP 65217 Com 7.60 1,076.4 86.54 G8III
HIP 65697 Vir 7.60 1,598.8 190.90 K0
HIP 65901 Cen 7.60 976.5 71.19 K0III
HIP 66611 Cen 7.60 668.4 33.36 K2/K3III
HIP 66927 Vir 7.60 849.4 53.85 K0
HIP 67050 Vir 7.60 2,313.2 399.58 K2
HIP 67263 ◈ CVn 7.60 3,076.9 706.64 M...
HIP 67615 Boo 7.60 985.4 72.51 K1III
HIP 67785 Vir 7.60 541.8 21.92 F8
HIP 68136 Hya 7.60 665.6 33.08 B9.5V
HIP 68784 Cir 7.60 594.1 26.35 F2Ib/II
HIP 69055 Aps 7.60 362.4 9.81 A7V
HIP 69287 Cen 7.60 495.7 18.35 F3/F5IV:
HIP 69841 Boo 7.60 1,510.0 170.29 K0
HIP 70347 Boo 7.60 679.5 34.48 K0
HIP 70352 Dra 7.60 1,792.1 239.88 K2
HIP 70372 Boo 7.60 1,681.2 211.06 M0
HIP 70738 Boo 7.60 718.4 38.55 G5IV
HIP 70828 ◈ Boo 7.60 950.9 67.55 K0
HIP 71631 ◈ Dra 7.60 111.3 0.93 F8
HIP 72521 Vir 7.60 755.0 42.58 K5III
HIP 72653 Boo 7.60 1,217.0 110.56 K0
HIP 72706 Boo 7.60 272.3 5.54 K0
HIP 72909 Cir 7.60 991.4 73.38 B7/B8IV/V
HIP 73504 Cir 7.60 1,853.2 256.33 B8II
HIP 74271 Lup 7.60 101.3 0.77 K0IV-V
HIP 74987 Boo 7.60 580.3 25.14 A0
HIP 75221 Lup 7.60 2,630.3 516.65 G1IV/V
HIP 75594 Lup 7.60 734.6 40.29 G8III
HIP 77596 Ser 7.60 749.8 42.00 K0
HIP 77951 Lup 7.60 682.3 34.77 G8/K0III
HIP 78368 Ser 7.60 807.3 48.66 K2
HIP 78782 Sco 7.60 472.0 16.64 K0III/IV
HIP 79541 Sco 7.60 539.1 21.70 F8V
HIP 79775 Sco 7.60 1,496.1 167.19 B3III
HIP 80765 Her 7.60 713.7 38.02 G5III
← Previous Page 473 · 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.