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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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V2213 Ophiuchi V2213 Oph, HD 154417, Gliese 9583, GJ 9583, GJ 654.1, HIP 83601, HR 6349, 2MASS J17051682+0042090, TIC 297236135, TYC 398-1908-1, LSPM J1705+0042, LTT 15050 |
F8.5IV-V | - | 67.2 ly |
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PM J22280-0411 | - | 67.2 ly | |
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SCR J1117-3202 | - | 67.2 ly | |
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LP 297-12 | - | 67.2 ly | |
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SDSS J091614.94+213950.8 | M9V | - | 67.2 ly |
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HD 285190 | M1.5V | - | 67.2 ly |
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Wolf 945 | M4V | - | 67.2 ly |
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HD 219623 BD+52°3410, GJ 4324, Gliese 4324, HD 219623, HIP 114924, HR 8853, SAO 35285 |
F8V | 1.2 M☉ | 67.2 ly |
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L 989-38 | M2V | - | 67.2 ly |
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2MASS J0443-3202 2MASS J04430581-3202090 |
L6.4:V | - | 67.2 ly |
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HD 23588 | K5V | - | 67.3 ly |
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V* V2367 Oph GJ 1212, Gliese 1212, HIP 84277, LP 687-12, 2MASS J17134048-0825144, TIC 1825871, TYC 5644-820-1, WISEA J171340.16-082519.0 |
M3.5 | - | 67.3 ly |
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LP 257-28 | DC9 | - | 67.3 ly |
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PM J01344+6426W | - | 67.3 ly | |
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L 300-117 | - | 67.3 ly | |
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Gaia EDR3 6063368716645888384 | - | 67.3 ly | |
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Gaia EDR3 1820834656271108864 | - | 67.3 ly | |
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LEHPM 927 | - | 67.3 ly | |
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L 235-35 | - | 67.3 ly | |
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LP 322-288 | M6V | - | 67.3 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
