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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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2MASS J21460802+3719549 | - | 82.7 ly | |
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G 272-34 | - | 82.7 ly | |
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68 Eridani HD 33256, 2MASS J05084368-0427225, CEL 545, GC 6292, GCRV 3054, GJ 189.2, GJ 9176, Gliese 9176, GSC 04759-01670, HIC 23941, HIP 23941, HR 1673, IRAS 05062-0431, PLX 1163, PLX 1163.00, PPM 187747, RAVE J050843.7-042722, ROT 731, SAO 131813, TD1 4093, TYC 4759-1670-1, UBV 4946, uvby98 100033256, YZ 94 1422, WEB 4668, 68 Eri, Gaia DR3 3212075924646082176, TIC 248411315 och UBV M 10661 |
F5.5VkF4mF2 | - | 82.7 ly |
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PM J10256+4750 | - | 82.7 ly | |
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1RXS J173405.5-711539 | M3.5 | - | 82.7 ly |
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UPM J0549-5224 | - | 82.7 ly | |
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G 193-36 | - | 82.7 ly | |
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G 173-18 | M1.3V | - | 82.7 ly |
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Gaia EDR3 3051506991743533184 | - | 82.7 ly | |
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UCAC4 139-189165 | - | 82.7 ly | |
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BD+01 2535 | K6V | - | 82.7 ly |
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LP 476-6 | M4.3V | - | 82.7 ly |
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LP 389-18 | M6 | - | 82.7 ly |
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G 49-22 | - | 82.8 ly | |
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UCAC4 160-044627 | - | 82.8 ly | |
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2MASS J06074202+4550435 | - | 82.8 ly | |
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G 41-10 | M4V | - | 82.8 ly |
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G 199-69 | M3Ve | - | 82.8 ly |
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G 235-29 | - | 82.8 ly | |
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G 46-24 | M1.0Ve | - | 82.8 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
