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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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L 123-30 | M2.0V | - | 63.7 ly |
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SIPS J0641-4322 | L2.4:V | - | 63.7 ly |
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HD 188474 TIC 271478281, LTT 7876, GJ 1246, Gliese 1246, HIP 98130, 2MASS J19563704-3120071, TYC 7439-410-1, TOI 2194 |
K3.5Vk: | 0.74 M☉ | 63.8 ly |
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HD 216520 2MASS J22473183+8341493, BD+82 704, HIC 112527, HIP 112527, LSPM J2247+8341, SAO 3796, TIC 264899051, TYC 4650-00917-1, WISE J224731.02+834150.7, GC 31860, WISEA J224731.02+834150.7 |
K0 V | 0.82 M☉ | 63.8 ly |
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CD-50 13863 | M3V | - | 63.8 ly |
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LP 666-11 | M6.0V | - | 63.8 ly |
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HD 137763 | G9V | - | 63.8 ly |
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LP 728-70 | M4.0 | - | 63.8 ly |
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HD 26347 BD-20 793 |
G2/3V | - | 63.8 ly |
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WT 2180 | M5.5V | - | 63.8 ly |
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L 258-146 | M3 | - | 63.8 ly |
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G 237-61 | M3.0Ve | - | 63.8 ly |
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SIPS J1712-0323 | - | 63.8 ly | |
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L 59-2 | M3.0 | - | 63.8 ly |
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PM J20223+3217 | M3.5Ve | - | 63.8 ly |
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L 339-106 | M3 | - | 63.8 ly |
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2MASS J07542987+7909546 | T2p? | - | 63.8 ly |
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EGGR 140 | DA3.0 | - | 63.8 ly |
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PM J13386-1132 | M4.5V | - | 63.8 ly |
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G 13-27 | - | 63.8 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
