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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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LP 634-24 | M0V | - | 89.1 ly |
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HD 186306 | G9V | - | 89.1 ly |
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UPM J1704-5125 | - | 89.1 ly | |
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2MASS J08215010+4532019 | M7.5 | - | 89.1 ly |
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LSPM J0006+0439 | - | 89.1 ly | |
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HD 361 | G1V | - | 89.1 ly |
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UPM J1237-8433 | - | 89.1 ly | |
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CD-36 862 | M1.5V | - | 89.1 ly |
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LSPM J1905+1740 | - | 89.1 ly | |
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G 237-54 | - | 89.1 ly | |
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Gliese 3473 GJ 3473, LHS 1972, LDS 5160A, G 50-16, 2MASS J08022287+0320196, NLTT 18833, TIC 452866790, TOI-488, WISEA J080222.59+032015.6 |
M4V C | 0.36 M☉ | 89.1 ly |
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KX Comae Berenices V* KX Com |
M2.5 | - | 89.1 ly |
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LP 458-43 | M5.0 | - | 89.1 ly |
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Gaia DR2 4143776239543076864 | - | 89.1 ly | |
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Gaia DR3 802677749236996224 | - | 89.1 ly | |
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LEHPM 3068 | M6e | - | 89.1 ly |
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36 Doradus CD−63°218, FK5 2452, GJ 9194, Gliese 9194, HD 40409, HIP 27890, HR 2102, SAO 249390 |
K2III-IV | 1.1 M☉ | 89.1 ly |
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APMPM J0446-4233 | - | 89.1 ly | |
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UCAC4 383-008489 | - | 89.1 ly | |
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UCAC2 1564860 | - | 89.1 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
