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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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DENIS J123217.8-685600 | M8.0 | - | 69 ly |
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LP 153-7 | M5.0 | - | 69 ly |
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G 92-55 | M3 | - | 69 ly |
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UPM J2232-5611 | - | 69.1 ly | |
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LSPM J1205+7825 | M2.5Ve | - | 69.1 ly |
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LSPM J1853+2022 | - | 69.1 ly | |
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Gliese 520 BD+48 2138, GJ 520, G 177-46, HIP 66492, 2MASS J13375120+4808174, WISEA J133750.92+480816.3, TIC 332278062 |
M0.5V | - | 69.1 ly |
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LSPM J0834+4529 | - | 69.1 ly | |
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50 Persei 50 Per, BD+37° 882, FK5 2297, Gliese 9145, GJ 9145, HD 25998, HIC 19335, HIP 19335, HR 1278, SAO 57006 |
F8V | 1.2 M☉ | 69.1 ly |
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LSPM J0457+3331 | - | 69.1 ly | |
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51 Arietis 51 Ari, BD+26°503, GJ 120.2, Gliese 120.2, HD 18803, HIP 14150, SAO 75696 |
G8V | 1 M☉ | 69.1 ly |
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RR Caeli Gliese 2034, LTT 1951, LFT 349, L 302-89, BPM 31852, RR Cae, WD 0419-487 |
DA8 | 0.44 M☉ | 69.1 ly |
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LEHPM 5263 | - | 69.2 ly | |
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G 203-50 | M4.5Ve | - | 69.2 ly |
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LSPM J1335+6051 | - | 69.2 ly | |
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LEHPM 1018 | - | 69.2 ly | |
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BD+10 4534 | K7.5Ve | - | 69.2 ly |
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Gaia EDR3 3638560954457699200 | - | 69.2 ly | |
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G 80-14 | - | 69.2 ly | |
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40 Leonis 40 Leo, BD+20° 2466, HD 89449, HIP 50564, HR 4054, SAO 99065 |
F6IV-V | 1.4 M☉ | 69.2 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
