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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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LP 655-3 | M5.5Ve | - | 83.1 ly |
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Gaia DR2 1343301122619404160 | - | 83.1 ly | |
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LP 335-13 | M0V | - | 83.1 ly |
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G 206-3 | M3.5Ve | - | 83.1 ly |
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2MASSI J0148386-302439 | M7.5 | - | 83.1 ly |
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G 168-38 | M1.5Ve | - | 83.1 ly |
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2MASS J08151407+1030117 | M7 | - | 83.1 ly |
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Beta Ophiuchi Cebalrai, Celbalrai, Cheleb, Kelb Alrai, Bet Oph, β Oph, β Ophiuchi, 60 Oph, 60 Ophiuchi, BD+04°3489, FK5 665, HD 161096, HIP 86742, HR 6603, SAO 122671 |
K2IIICN0.5 | 1.8 M☉ | 83.1 ly |
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L 79-24 | M3.5 | - | 83.1 ly |
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LSPM J1859+0156 | M4.5V | - | 83.2 ly |
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UPM J1953+4217 | - | 83.2 ly | |
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2MASS J05523129-0002124 | - | 83.2 ly | |
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UCAC3 56-432979 | - | 83.2 ly | |
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CD-37 1501 | M2.5V | - | 83.2 ly |
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SCR J1738-5942 | - | 83.2 ly | |
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UCAC3 131-54431 | - | 83.2 ly | |
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2MASS J09544749+6702082 | DA | - | 83.2 ly |
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HD 111312 | K2.5Vk: | - | 83.2 ly |
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Gamma Ursae Majoris Phad, Phecda, Phekda, Phegda, Phekha, Phacd, Fekda, γ Ursae Majoris, γ UMa, Gamma UMa, 64 Ursae Majoris, BD+54 1475, FK5 447, GC 16268, HD 103287, HIC 58001, HIP 58001, HR 4554, PPM 33292, SAO 28179 |
A0 Ve | 2.9 M☉ | 83.2 ly |
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2MASS J05435795-2253063 | - | 83.2 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
