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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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PM J09484-5644 | - | 61.6 ly | |
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PM J20300+0023 | M4.0V | - | 61.6 ly |
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HD 266611 | K5V | - | 61.6 ly |
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LP 423-31 | M6.0V | - | 61.6 ly |
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UPM J0726-3033 | - | 61.6 ly | |
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Wolf 219 | DQ8 | - | 61.6 ly |
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G 141-53 LSPM J1859+0829, 2MASS J18593888+0829005, NLTT 47286, TIC 222490987, USNO-B1.0 0984-00437293 |
- | 61.6 ly | |
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6 Ceti 6 Cet, BD−16° 17, GJ 10, Gliese 10, HD 693, HIP 910, HR 33, SAO 147133 |
F8VFe-0.8CH-0.5 | 1.1 M☉ | 61.6 ly |
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G 260-1 | M5.0V | - | 61.6 ly |
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LSPM J0837+0333 | M4.0V | - | 61.6 ly |
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UCAC3 129-126893 | M3Ve | - | 61.6 ly |
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G 170-42 | - | 61.6 ly | |
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HD 153026 LTT 6774, GJ 646, Gliese 646, 2MASS J16585402-3933308, TIC 343110556, TYC 7872-336-1, WISEA J165854.31-393327.4 |
K5 | - | 61.7 ly |
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HD 5015 BD+60°124, GJ 41, Gliese 41, HIP 4151, HR 244, SAO 11444, WDS J00531+6107A |
F9V | 1.2 M☉ | 61.7 ly |
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L 626-41 | M3.5 | - | 61.7 ly |
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UCAC4 168-113269 | - | 61.7 ly | |
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G 249-32 | M4.5V | - | 61.7 ly |
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LSPM J1728+7108 | - | 61.7 ly | |
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2MASSW J1421314+182740 | M8.9V | - | 61.7 ly |
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LP 66-542 | M5.0 | - | 61.7 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
