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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 | ||
|---|---|---|---|---|
|
|
LP 792-16 | M3.0 | - | 73.2 ly |
|
|
TOI 4336 TIC 166184428, 2MASS J13442546-4020155, WISE J134425.61-402014.8, UCAC4 249-060094 |
0.33 M☉ | 73.2 ly | |
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|
CD-47 399 GJ 3090, Gliese 3090 |
M2V | 0.52 M☉ | 73.2 ly |
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|
HD 304391 | K3.5V(k) | - | 73.2 ly |
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LSPM J2044+1339 | M5.0Ve | - | 73.3 ly |
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HD 59468 CD-51 2507, Gl 275, Gliese 275, HIP 36210 |
G6.5V | - | 73.3 ly |
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HD 18455 | K2V | - | 73.3 ly |
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PM J08202+0532 | M2.0Ve | - | 73.3 ly |
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LP 786-15 | - | 73.3 ly | |
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Gaia EDR3 1855837849445750912 | - | 73.3 ly | |
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2MASS J05160945-0445499 | T5.5 | - | 73.3 ly |
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|
2MASS J1207+0244 2MASS J12074717+0244249, 2MASS 1207 |
L6.5 | - | 73.3 ly |
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G 32-18 | M4.0 | - | 73.3 ly |
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TYC 5060-53-1 | - | 73.3 ly | |
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TOI-270 L 231-32, LEHPM 3808, 2MASS J04333970-5157222, TIC 259377017, UCAC4 191-004642 |
M3.0V C | 0.4 M☉ | 73.3 ly |
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HD 210667 | G9V | - | 73.3 ly |
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LP 912-49 | M5.5Ve | - | 73.3 ly |
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HD 11373 | K3Vk | - | 73.3 ly |
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G 247-45 | - | 73.3 ly | |
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G 14-46 | M3: | - | 73.3 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
