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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 240-45 | - | 89.7 ly | |
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SCR J2216-4800 | - | 89.7 ly | |
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UCAC4 271-087330 | - | 89.7 ly | |
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2MASS J21274780-7508308 | - | 89.7 ly | |
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PM J07365-0039 | M3.5V | - | 89.7 ly |
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Gaia DR3 5871522869817098240 | - | 89.7 ly | |
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HD 174719 TYC 452-237-1, USNO-A2 0900-13661819, HIP 92569 |
G5/6V | - | 89.7 ly |
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Gaia DR3 4113092580854650112 | - | 89.7 ly | |
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Wolf 335 | M1.0V | - | 89.7 ly |
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StM 258 | M3.5Ve | - | 89.7 ly |
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HD 60272 | G9V | - | 89.7 ly |
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Gaia DR3 4155383783818917760 | - | 89.7 ly | |
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G 57-17 | M4.0V | - | 89.7 ly |
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37 Capricorni HIP 106559, HD 205289, TYC 6369-1185-1, HR 8245, 37-Cap, BD-20 6237 |
F5VFe-0.8CH-0.4 | - | 89.7 ly |
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TYC 9403-634-1 | - | 89.7 ly | |
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TOI-836 HIC 73427, HIP 73427, CD-23 12010, 2MASS J15001942-2427147, LTT 5972, NLTT 39000, SAO 183077, TIC 440887364, TYC 6752-835-1, WISEA J150019.25-242714.9 |
K7V C | 0.68 M☉ | 89.7 ly |
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2MASS J06242138+2815056 | - | 89.7 ly | |
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G 87-9 BD+35 1493, GJ 3411, Gliese 3411, 2MASS J06493584+3508263, TYC 2444-837-1, HIP 32723, LP 254-40 |
K6V | - | 89.7 ly |
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LP 484-5 | - | 89.7 ly | |
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UCAC4 380-073828 | DAH | - | 89.7 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
