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Our Milky Way galaxy contains billions of stars, ranging from massive, bright stars to small, faint stellar remnants. Some stars exist on their own, while many are part of binary or multiple star systems. This page presents a list of the nearest stars to the Solar System, helping to map our local stellar neighborhood and understand the diversity of stars closest to us.
The list can be filtered by stellar category, allowing you to explore specific types of stars such as red dwarfs, Sun-like stars, white dwarfs, or brown dwarfs. This flexible view makes it easier to compare different stellar populations and focus on objects of interest. While the main emphasis is on nearby stars, the catalog also extends beyond the immediate neighborhood, offering a broader perspective on stellar types within our galaxy.
| Star name | Mass | Distance | ||
|---|---|---|---|---|
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G 42-25 | - | 85.4 ly | |
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Gaia DR3 4124216821020272512 | - | 85.4 ly | |
|
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PM J05569+0155 | - | 85.4 ly | |
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DO Canum Venaticorum DO CVn |
K0 | - | 85.4 ly |
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LP 374-30 | - | 85.4 ly | |
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KPP 3859 | - | 85.4 ly | |
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G 82-28 | M4Ve | - | 85.4 ly |
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HD 356314 | M0 | - | 85.4 ly |
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Gaia DR3 4040737976951183488 | - | 85.5 ly | |
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Gaia DR3 6029040726730634368 | - | 85.5 ly | |
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Gaia DR3 4285535964446640128 | - | 85.5 ly | |
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SCR J1805-2042 | - | 85.5 ly | |
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Epsilon Cephei ε Cephei, 23 Cephei, BD+56 2741, HD 211336, HIP 109857, HR 8494, SAO 34227 |
F0 IV | 1.6 M☉ | 85.5 ly |
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|
SCR J0327-3634 | M3e | - | 85.5 ly |
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LSPM J0533+3740 | - | 85.5 ly | |
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G 177-8 | - | 85.5 ly | |
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PM J14343+6043 | - | 85.5 ly | |
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DENIS J170547.4-544151 | M8.5 | - | 85.5 ly |
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StKM 1-626 | M0.5Ve | - | 85.5 ly |
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HD 60532 108 G. Puppis, BD–21° 2007, GC 10134, HIC 36795, HIP 36795, HR 2906, GJ 279, Gliese 279, SAO 174009, 2MASS J07340317-2217457, FK5 288, TIC 456871289, TYC 5991-217-1 |
F6IV-V C | 1.4 M☉ | 85.5 ly |
StellarGuide: Stars
Stars are enormous spheres of hot gas that shine by generating energy through nuclear fusion in their cores. Most stars are made primarily of hydrogen and helium. In the center of a star, intense pressure and temperature cause hydrogen atoms to fuse into helium, releasing a tremendous amount of energy as light and heat.More about Stars
