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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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HD 112758 LHS 2656, 2MASS J12590162-0950029, TYC 5536-983-1, SAO 139081, HIP 63366, GJ 491, Gliese 491, BD −9° 3595 |
G9V | - | 65.5 ly |
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WT 1680 | - | 65.5 ly | |
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LSPM J0143+0014 | - | 65.5 ly | |
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Ross 644 | K7V | - | 65.5 ly |
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G 28-46 | M3V | - | 65.5 ly |
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HD 217107 6 G. Piscium, BD−03° 5539, FK5 3836, HIC 113421, HIP 113421, HR 8734, SAO 146412, CCDM J22583-0224AB, IRAS 22556-0239, 2MASS J22581556-0223432, TIC 38271828, TYC 5235-1468-1, YZ 92 7936 |
G8IV/V D | 0.97 M☉ | 65.5 ly |
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2MASS J06402517-2352194 | - | 65.5 ly | |
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G 187-13 | M4V | - | 65.5 ly |
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G 187-14 | M4V | - | 65.5 ly |
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LP 914-6 | M3.0Ve | - | 65.5 ly |
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UPM J0448-3539 | - | 65.5 ly | |
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UPM J0626+2032 | - | 65.6 ly | |
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LP 698-2 | M6Ve | - | 65.6 ly |
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HD 12058 | K4.5Vk: | - | 65.6 ly |
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PM J00468+1603 | M2.0Ve | - | 65.6 ly |
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Gaia EDR3 4123824295451214848 | - | 65.7 ly | |
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L 159-20 | M3.5 | - | 65.7 ly |
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LP 932-81 | M3 | - | 65.7 ly |
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Gaia EDR3 4307917069079963520 | - | 65.7 ly | |
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GD 356 | DAEH6.5 | - | 65.7 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
