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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 | ||
|---|---|---|---|---|
|
|
LP 92-279 TIC 149927512 |
0.25 M☉ | 92.2 ly | |
|
|
LP 559-44 | ~ | - | 92.2 ly |
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|
UCAC4 483-053012 | - | 92.2 ly | |
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|
PW Andromedae V* PW And |
K2V | - | 92.2 ly |
|
|
LSPM J1703+2433 | - | 92.2 ly | |
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G 145-36 | - | 92.2 ly | |
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Gaia DR3 4267635846461036928 | - | 92.2 ly | |
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PM J16513-5406 | - | 92.2 ly | |
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LSPM J2329+4644S | - | 92.2 ly | |
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Gaia DR2 5716540143147016192 | - | 92.2 ly | |
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G 188-40 | - | 92.2 ly | |
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|
HD 207897 G 261-47, G 265-42, HIC 107038, HIP 107038, LSPM J2140+8420, LTT 16367, NLTT 52064, 2MASS J21404490+8420005, TIC 264678534, TOI-1611, TYC 4649-124-1, WISEA J214047.16+842001.1, Gaia DR2 2300641567596591488 |
K0V | 0.82 M☉ | 92.2 ly |
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|
2MASS J08441409-2924121 | L4.0 | - | 92.3 ly |
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BD+03 3032 | K5V | - | 92.3 ly |
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PM J12368-0159 | M3.5V | - | 92.3 ly |
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LP 785-7 | - | 92.3 ly | |
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Gaia DR3 4037059736852099456 | - | 92.3 ly | |
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2MASS J12084952+3021010 | - | 92.3 ly | |
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RX J1117.0-8028 | M4e | - | 92.3 ly |
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Gaia DR3 4059922775527398912 | - | 92.3 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
