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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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EGGR 436 | DA9P | - | 53.7 ly |
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G 100-50 | M5.0V | - | 53.7 ly |
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HD 158614 STF 2173, BD−00°3300, Gliese 678, GJ 678, HIP 85667, HR 6516, SAO 141702, WDS J17304-0104 |
G9-IV-VHdel1 | 0.96 M☉ | 53.7 ly |
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UCAC4 554-051865 2MASS J15183145+2036279, TIC 355740719 |
M4.5V | - | 53.7 ly |
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Gaia DR2 6411063808332359808 1RXS J221545.5-585642 |
~ | - | 53.7 ly |
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L 315-66 | M4 | - | 53.8 ly |
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G 28-39 | M0V | - | 53.8 ly |
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GR* 422 | - | 53.8 ly | |
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Gaia DR2 2206265777300448768 | - | 53.8 ly | |
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BD+66 582 | K5 | - | 53.8 ly |
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Wolf 457 | DAQZ8 | - | 53.8 ly |
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9 Puppis BU 101, 9 Pup, BD−13° 2267, GC 10629, Gliese 291, GJ 291, HD 64096, HIP 38382, HR 3064, SAO 153500, ADS 6420, WDS J07518-1354, 2MASS J07514629-1353526 |
G1V | 1.1 M☉ | 53.8 ly |
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SCR J0827-2526 | - | 53.8 ly | |
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SCR J0420-7005 | M6Ve | - | 53.8 ly |
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GD 279 WD 0148+467, HIP 8709 |
DA3.6 | - | 53.9 ly |
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L 454-9 | DA8.0 | - | 53.9 ly |
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L 763-66 | M1 | - | 53.9 ly |
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LEHPM 3719 | - | 53.9 ly | |
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G 195-36 | M3V | - | 53.9 ly |
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WISEA J2332-4325 WISEA J233226.54-432510.9 |
T9 | - | 53.9 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
