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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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UCAC4 577-099502 | - | 80.6 ly | |
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Wolf 755 | M0V | - | 80.6 ly |
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LSPM J0553+1520 | - | 80.6 ly | |
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HD 12051 | G9V | - | 80.6 ly |
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HD 1562 | G1V | - | 80.7 ly |
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2MASS J10044030-1318186 | L1 | - | 80.7 ly |
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DENIS J081244.2-450433 | - | 80.7 ly | |
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HD 104731 TYC 7763-1047-1, USNO-A2 0450-13777979, HR 4600, HIP 58803, CD-41 6938，SAO 223193 |
F5V | - | 80.7 ly |
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LP 213-67 | M6.5Ve | - | 80.7 ly |
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HD 195564 BD−10° 5423, FK5 1536, GJ 792.1, HD 195564, HIP 101345, HR 7845, SAO 163665 |
G2.5IV | 1.1 M☉ | 80.7 ly |
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Wolf 1040 | M3.5: | - | 80.7 ly |
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HD 197396 TYC 1646-677-1, HIP 102226, USNO-A2 1050-18447769 |
K2.5V | - | 80.7 ly |
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Ross 451 | esdM0 | - | 80.7 ly |
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G 188-19 | M4 | - | 80.7 ly |
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Gaia EDR3 4276948538120524288 | - | 80.7 ly | |
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PM J10061-4949 | M3 | - | 80.7 ly |
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HD 91889 BD-11 2918，SAO 156095，HD 91889，HR 4158 |
F8V | - | 80.7 ly |
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LP 579-24 | M5V | - | 80.7 ly |
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LP 993-98 | M5.5 | - | 80.7 ly |
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WD 1856+534 LP 141-14, LSPM J1857+5330, 2MASS J18573936+5330332, NLTT 47263, TIC 267574918, TOI-1690, WDS J18576+5331C, WISE J185739.62+533032.9, |
DA | 0.61 M☉ | 80.7 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
