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| Star | Constellation | Magnitude | Distance (ly) | Luminosity (Suns) | Spectral type |
|---|---|---|---|---|---|
| HIP 82916 | Dra | 8.77 | 2,673.4 | 181.64 | K |
| HIP 23916 | Eri | 5.80 | 680.9 | 181.64 | B8V |
| HIP 49675 | Vel | 7.46 | 1,462.6 | 181.64 | K2III |
| HIP 92256 | Lyr | 7.32 | 1,370.4 | 181.47 | B8 |
| HIP 93059 | Dra | 8.65 | 2,528.3 | 181.47 | K5 |
| HIP 13384 ◈ | Eri | 7.03 | 1,199.1 | 181.47 | M5IIIvar |
| HIP 112988 | Cep | 8.65 | 2,528.3 | 181.47 | K0 |
| HIP 42658 | Cnc | 8.65 | 2,528.3 | 181.47 | K0 |
| HIP 25062 | Col | 8.60 | 2,470.9 | 181.47 | K2IV/V |
| HIP 117198 | Phe | 8.52 | 2,380.7 | 181.30 | G8III |
| HIP 34863 | Pup | 8.17 | 2,025.8 | 181.30 | K4/K5III: |
| HIP 97884 | Pav | 8.52 | 2,380.7 | 181.30 | G6IV |
| HIP 93419 | Vul | 6.74 | 1,048.7 | 181.30 | K2 |
| HIP 49656 | Leo | 8.79 | 2,695.5 | 181.30 | G5 |
| HIP 40913 | Lyn | 8.13 | 1,988.8 | 181.30 | G5 |
| HIP 7042 ◈ | Psc | 8.17 | 2,025.8 | 181.30 | Mb |
| HIP 106544 ◈ | Aqr | 6.41 | 901.0 | 181.30 | M3 |
| HIP 101336 | Cap | 7.33 | 1,376.2 | 181.30 | K4/K5III |
| 29Pi Leo | Leo | 4.68 | 406.2 | 181.30 | M2III |
| HIP 101929 | Ind | 8.52 | 2,380.7 | 181.30 | K3III |
| HIP 46409 | Vel | 8.79 | 2,695.5 | 181.30 | K1/K2III |
| HIP 31908 | Gem | 8.31 | 2,160.0 | 181.13 | K0 |
| HIP 89910 | Tel | 7.80 | 1,707.6 | 181.13 | B5III |
| HIP 79740 | Sco | 6.70 | 1,028.9 | 181.13 | B9III/IV |
| HIP 53410 | Crt | 8.94 | 2,886.3 | 181.13 | K1III |
| HIP 42803 | Pyx | 8.49 | 2,346.4 | 181.13 | G8III |
| HIP 20829 | Eri | 6.97 | 1,164.8 | 180.97 | G5 |
| HIP 103873 | Cyg | 8.57 | 2,434.0 | 180.97 | M... |
| HIP 36117 | Cam | 8.96 | 2,912.1 | 180.97 | G5 |
| HIP 90662 | Tel | 5.69 | 645.9 | 180.97 | K2III |
| 3 Cen ◈ | Cen | 4.32 | 343.7 | 180.97 | B5 |
| HIP 109531 | Peg | 7.26 | 1,331.2 | 180.97 | A0 |
| HIP 30461 | CMa | 6.68 | 1,019.2 | 180.97 | K0/K1III+.. |
| HIP 109743 ◈ | Cep | 9.10 | 3,106.2 | 180.97 | B8 |
| HIP 92570 | Lyr | 7.36 | 1,393.8 | 180.97 | K0 |
| HIP 43085 | Vel | 7.09 | 1,230.8 | 180.97 | B4V |
| HIP 90293 | Lyr | 7.36 | 1,393.8 | 180.97 | A0p |
| HIP 104449 | Cep | 6.53 | 950.9 | 180.97 | B7III |
| HIP 2145 | And | 7.67 | 1,606.7 | 180.80 | K0 |
| HIP 95577 | Sgr | 7.01 | 1,186.0 | 180.80 | K5III |
| HIP 112010 | Peg | 9.08 | 3,076.9 | 180.80 | K2 |
| HIP 85442 | Oph | 5.98 | 737.9 | 180.80 | B9.5IV |
| HIP 82848 ◈ | Sco | 7.67 | 1,606.7 | 180.80 | B7II |
| HIP 26964 ◈ | Tau | 6.23 | 827.8 | 180.80 | B2.5Ve |
| 48 Psc | Psc | 6.05 | 762.0 | 180.80 | K5III |
| HIP 111627 | Lac | 6.28 | 847.2 | 180.80 | K5 |
| Tau Pup | Pup | 2.94 | 182.0 | 180.80 | K0III... |
| Mu Lup | Lup | 4.27 | 335.6 | 180.63 | B8V |
| HIP 27208 | Lep | 7.86 | 1,753.5 | 180.63 | K3III |
| HIP 43459 | Pyx | 7.86 | 1,753.5 | 180.63 | B9.5III |
| HIP 82840 | UMi | 8.16 | 2,013.3 | 180.63 | M0 |
| HIP 30700 | Mon | 6.50 | 937.2 | 180.63 | B4V |
| HIP 102297 | Del | 7.21 | 1,299.4 | 180.63 | K0 |
| HIP 26881 | Ori | 7.66 | 1,598.8 | 180.63 | K0 |
| HIP 104910 | Aqr | 6.98 | 1,169.0 | 180.63 | K2 |
| HIP 48439 | LMi | 7.78 | 1,689.9 | 180.63 | K0 |
| HIP 28100 | Aur | 7.77 | 1,681.2 | 180.47 | B9 |
| HIP 38906 | Car | 6.86 | 1,105.6 | 180.47 | B9III |
| HIP 6047 | And | 6.78 | 1,065.9 | 180.47 | K5 |
| HIP 25779 ◈ | Tau | 7.77 | 1,681.2 | 180.47 | M... |