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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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G 104-35 | M1.0Ve | - | 75.8 ly |
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LP 890-39 | DC | - | 75.8 ly |
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UPM J0558+3911 | - | 75.8 ly | |
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HD 208038 | K2.5V | - | 75.8 ly |
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G 132-4 | M3.0V | - | 75.8 ly |
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Alpha2 Librae α2 Lib, 9 Librae, BD−15 3966, FK5 548, HD 130841, HIP 72622, HR 5531, SAO 158840 |
kA2hA5mA4IV-V | 1.4 M☉ | 75.8 ly |
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Gaia EDR3 4147834330766001536 | - | 75.8 ly | |
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HD 106549 HD 106549, HIP 59780, 2MASS J12152709-3105387, TYC 7232-584-1, WISE J121527.23-310539.2 |
K7Vk: | - | 75.8 ly |
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BPM 46052 | M1V | - | 75.8 ly |
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CD-24 17578 | M0Vk: | - | 75.8 ly |
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G 158-8 | M3.5V | - | 75.8 ly |
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AT Coronae Borealis V* AT CrB |
K3V | - | 75.8 ly |
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G 255-49 | M1.5Ve | - | 75.8 ly |
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SIPS J1731-7851 | - | 75.8 ly | |
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Gaia EDR3 4277397070128040064 | - | 75.8 ly | |
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Gaia EDR3 2215027510585500672 | - | 75.8 ly | |
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G 247-12 | M4.5V | - | 75.8 ly |
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LP 341-25 | - | 75.9 ly | |
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LP 983-34 | M4 | - | 75.9 ly |
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Kappa Tucanae κ Tuc, HD 7788, HIP 5896, HR 377, SAO 248346 |
F6IV | 1.4 M☉ | 75.9 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
