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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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Gaia EDR3 4119946455341946880 | - | 72.6 ly | |
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L 353-143 | M5V | - | 72.6 ly |
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G 127-35 | M1V | - | 72.6 ly |
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NSN 237 | - | 72.6 ly | |
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39 Leonis 39 Leo, BD+23 2207, GJ 387, Gliese 387, HD 89125, HIP 50384, HR 4039, SAO 81270 |
F6V | 0.98 M☉ | 72.6 ly |
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LP 821-54 | - | 72.6 ly | |
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LSPM J1619+0140 | M5V | - | 72.6 ly |
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2MASS J05000865-1216025 | - | 72.7 ly | |
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L 387-60 | M1: | - | 72.7 ly |
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G 116-77 | M1.0Ve | - | 72.7 ly |
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L 120-191 | M1 | - | 72.7 ly |
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PM J19427-1723 | M4.0 | - | 72.7 ly |
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84 Ceti 84 Cet, BD–01 377, HD 16765, HIP 12530, HR 790, SAO 130055 |
F7V | 1.2 M☉ | 72.7 ly |
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LSPM J0154+5741S | M3.5V | - | 72.7 ly |
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Epsilon Cygni Aa Aljanah, Gienah, ε Cyg, 53 Cygni, BD +33°4018, FK5 780, GCTP 4959.00, Gliese 806.1, Gl 806.1, HD 197989, HIC 102488, HIP 102488, HR 7949, LHS 5358, SAO 70474, WDS 20462+3358 |
K0III | 2 M☉ | 72.7 ly |
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LSPM J1920+2848 | - | 72.7 ly | |
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UPM J0600-3742 | - | 72.7 ly | |
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WT 1371 | - | 72.7 ly | |
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LP 714-37 | M5.5 | - | 72.7 ly |
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LP 387-31 | M3.16 | - | 72.7 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
