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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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Iota Leonis Aa ι Leo, 78 Leonis, Gliese 426.1, BD+11°2348, HD 99028, HIP 55642, HR 4399, SAO 99587 |
F1IV | 1.7 M☉ | 77 ly |
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UPM J1526+3305 | - | 77 ly | |
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UPM J1823-3451 | - | 77 ly | |
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HD 188559 | K3+V | - | 77 ly |
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G 251-27 | M3.0Ve | - | 77 ly |
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Gliese 27.1 Gaia DR2 4980466929964496128, GJ 27.1, HIC 3143, HIP 3143, TYC 7531-1014-1, 2MASS J00395880-4415117, CD-44 170, LHS 1122, Gliese 9018, GJ 9018, LFT 61, L 363-95, LTT 354, NLTT 2181, TIC 80417903, TYC 7531-1014-1, WISEA J003959.30-441513.9 |
M0.5V | 0.53 M☉ | 77 ly |
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Gaia DR2 5715478732169133952 | - | 77.1 ly | |
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BD-14 249 | M1V | - | 77.1 ly |
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SDSS J133559.70+402146.1 | - | 77.1 ly | |
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LP 330-40 | - | 77.1 ly | |
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BD+20 3009 | K5V | - | 77.1 ly |
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PM J07129+3547 | M2.5V | - | 77.1 ly |
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HD 23040 | K2 | - | 77.1 ly |
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2MASS J01410321+1804502 | L0.8V | - | 77.1 ly |
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2MASS J18105253-0708497 | - | 77.1 ly | |
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Gaia EDR3 4264353838563541504 | - | 77.1 ly | |
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HD 207496 Gaia DR3 6356417496318028800, TOI-1099
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K2.5Vk: | 0.8 M☉ | 77.1 ly |
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BD+29 5007 | K5V | - | 77.1 ly |
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Gaia EDR3 4315746558237234176 | - | 77.1 ly | |
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LP 776-12 | - | 77.1 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
