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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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PM J14321-7357 | - | 76.7 ly | |
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LP 758-19 | - | 76.7 ly | |
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G 255-55 | M2.0Ve | - | 76.7 ly |
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G 83-12 | - | 76.7 ly | |
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UPM J0111+0306 | - | 76.7 ly | |
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Gliese 3341 GJ 3341, LHS 1748, CD-31 2312, LFT 401, L 521-2, LP 892-26, LTT 2219, NLTT 14792, 2MASS J05154667-3117456, TIC 77897915, WISEA J051547.11-311742.7 |
M2 D | 0.47 M☉ | 76.7 ly |
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UPM J2057+2841 | - | 76.7 ly | |
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2MASS J14044948-3159330 | T1 | - | 76.7 ly |
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L 59-3 | M3 | - | 76.7 ly |
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G 161-51 | M3.5 | - | 76.8 ly |
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Smethells 119 | M4V | - | 76.8 ly |
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SCR J0608-7904 | - | 76.8 ly | |
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Epsilon Ceti * eps Cet, ε Cet, 83 Cet, BD−12° 501, HD 16620, HIP 12390, HR 781, SAO 148528 |
F5V | 1.4 M☉ | 76.8 ly |
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LP 645-46 | DA | - | 76.8 ly |
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HD 112914 | K3V | - | 76.8 ly |
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LP 522-46 | DA | - | 76.8 ly |
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HD 187456 | K3+V | - | 76.8 ly |
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UCAC3 272-282107 | M5.0 | - | 76.8 ly |
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Delta Herculis Aa Sarin, δ Her, 65 Her, BD 25° 3221, CCDM J17151+2451A, FK5 641, GC 23294, HD 156164, HIP 84379, HR 6410, SAO 84951 |
A1IVn | 2.4 M☉ | 76.8 ly |
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LSPM J0231+5245 | - | 76.8 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
