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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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CD-32 12693 | M1.5 | - | 71.7 ly |
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HD 164922 BD +26°3151, Gliese 700.2, GJ 700.2, Gliese 9613, GJ 9613, LFT 1388, SAO 85678, HIC 88348, HIP 88348, 2MASS J18023085+2618471, LHS 3353, WISEA J180231.16+261840.6, TIC 159019691, TYC 2099-2717-1 |
G9V C | 0.87 M☉ | 71.7 ly |
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UCAC4 097-041773 | - | 71.7 ly | |
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LP 239-52 | M5.5Ve | - | 71.7 ly |
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LP 734-34 | M4.5V | - | 71.7 ly |
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CD-30 1270 | M1V | - | 71.8 ly |
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2MASS J0859+6341 | L0 | - | 71.8 ly |
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LP 197-48 | M5.0 | - | 71.8 ly |
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LP 376-62 | M6V | - | 71.8 ly |
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Alpha Hydri α Hyi, CD−62° 71, GJ 83, Gliese 83, HIP 9236, HR 591, SAO 248474 |
F0IV | 2 M☉ | 71.8 ly |
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HD 119802 | K3V | - | 71.8 ly |
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2MASS J1553+1400 2MASS J15531993+1400337 |
M9e | - | 71.8 ly |
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G 35-35 | M4V | - | 71.8 ly |
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BD+27 273 | M1V | - | 71.8 ly |
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CD-44 3484 | M0 | - | 71.8 ly |
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Gaia EDR3 6724003200082572928 | - | 71.8 ly | |
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G 73-66 | M3.5 | - | 71.8 ly |
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G 206-37 | M3.5 | - | 71.8 ly |
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G 61-41 | M3.5Ve | - | 71.8 ly |
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EGGR 7 | DA5.9 | - | 71.8 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
