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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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LSPM J0530+1514 | M3.0Ve | - | 64.2 ly |
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LP 862-184 | M4 | - | 64.2 ly |
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PM J16377-2013 | M4 | - | 64.2 ly |
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LSPM J2346+1129 | M9 | - | 64.2 ly |
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MCC 253 | M0V | - | 64.2 ly |
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G 188-49 | K7.5Ve | - | 64.2 ly |
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BD+21 2486 | - | 64.2 ly | |
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HD 352860 | K6V | - | 64.2 ly |
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Gaia DR2 3330473222213987072 | - | 64.2 ly | |
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Gaia DR3 4109528651372564096 | - | 64.2 ly | |
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2MASS J1706-1314 2MASS J17065487-1314396 |
L5pec | - | 64.2 ly |
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|
Eta Crucis η Cru, CD−63° 2145, GJ 9388, Gliese 9388, HD 105211, HIP 59072, HR 4616, SAO 251742, eta Cru |
F2V | - | 64.2 ly |
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SIPS J1426-2946 | - | 64.2 ly | |
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LP 314-44 | M6.5Ve | - | 64.2 ly |
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2MASS J0014-4844 2MASS J00145575-4844171 |
L2.5 | - | 64.2 ly |
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PM J16591+2058 | - | 64.2 ly | |
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LDS 5035 CD-24 17443, HIP 113602, 2MASS J23003338-2357097, GJ 4308, Gliese 4308, TIC 204291257, TYC 6971-588-1 |
M1:V | - | 64.3 ly |
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CD-38 13254 2MASS J18594945-3812561, TIC 254010456, TYC 7916-873-1 |
G0E | - | 64.3 ly |
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HD 128642 | G5 | - | 64.3 ly |
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Ross 776 | M3.3V | - | 64.3 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
