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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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HD 31000 TYC 2399-1394-1, USNO-A2 1200-02602146, HIP 22776 |
G5V | - | 89.8 ly |
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Gaia DR3 3033360205164329600 | - | 89.8 ly | |
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HD 55458 | K1V | - | 89.8 ly |
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LP 95-282 | - | 89.8 ly | |
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UPM J1301+6708 | - | 89.8 ly | |
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Gaia DR3 4115934096833258496 | - | 89.8 ly | |
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HD 179949 13 Sgr, V5652 Sgr, CD−24° 15161, GJ 749, Gliese 749, HD 179949, HIC 94645, HIP 94645, HR 7291, SAO 187883, 2MASS J19153322-2410455, Gumala, TIC 2288734, TYC 6875-3273-1, WISEA J191533.32-241046.3 |
F8V C | 1.2 M☉ | 89.8 ly |
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LP 827-294 | M3 | - | 89.8 ly |
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G 200-29 | - | 89.8 ly | |
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LSPM J0612+0024 | - | 89.8 ly | |
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LP 237-32 | M3.8V | - | 89.8 ly |
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Gaia DR3 4268042871883857408 | - | 89.8 ly | |
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LSPM J1920+1531 | - | 89.8 ly | |
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L 536-155 2MASS J10194735-3402219, WISE J101947.04-340220.2, TIC 71407717 |
DAH D | - | 89.8 ly |
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RGO 3693 UCAC4 311-000999 |
- | 89.9 ly | |
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UCAC4 550-089355 | - | 89.9 ly | |
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G 198-19 | ~ | - | 89.9 ly |
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LP 649-93 | M8V | - | 89.9 ly |
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Gaia DR3 4120465287390368128 | - | 89.9 ly | |
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Gaia DR3 4144874651706930048 | - | 89.9 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
