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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 J09004-0652 | M4.04 | - | 96.2 ly |
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LP 373-29 | M6.5V | - | 96.2 ly |
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HD 121131 | K1V | - | 96.2 ly |
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LP 395-8 | - | 96.2 ly | |
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UCAC4 683-079854 | - | 96.2 ly | |
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CD-38 2136 | K3.5Vk: | - | 96.2 ly |
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G 83-29 | M3.04 | - | 96.2 ly |
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HD 6673 | K2.5V | - | 96.2 ly |
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G 33-39 | - | 96.2 ly | |
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LP 246-46 | - | 96.2 ly | |
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G 123-36 | M1.0Ve | - | 96.2 ly |
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DENIS J213856.8-211434 | M3.5 | - | 96.2 ly |
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BD+09 2366 | K5V | - | 96.3 ly |
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L 163-23 | - | 96.3 ly | |
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Iota Boötis Asellus Secondus[12], ι Boötis, 21 Boötis, BD+52°1784, FK5 528, GC 19269, HD 125161, HIP 69713, HR 5350, SAO 29071, PPM 34432, WDS J14162+5122, iot Boo, |
A7V | 1.7 M☉ | 96.3 ly |
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HD 46375 BD+05°1295, HIC 31246, HIP 31246, SAO 114040, SLE 299A, CoRoT 1889, 2MASS J06331263+0527464, TIC 234928947, TYC 154-891-1, WDS J06332+0528A |
G9V C | 0.92 M☉ | 96.3 ly |
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UCAC4 671-070265 | - | 96.3 ly | |
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SCR J0017-3219 | M4.5 | - | 96.3 ly |
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LSPM J1820+2841 | - | 96.3 ly | |
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L 127-20 | - | 96.3 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
