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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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UPM J2336+2613 | - | 96.3 ly | |
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Wolf 411 | K5V | - | 96.3 ly |
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Gaia DR3 4356709207522366464 | - | 96.3 ly | |
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Gliese 3030 GJ 3030 |
M2.4 | - | 96.3 ly |
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Eta Ursae Minoris * eta UMi, η UMi, 21 Ursae Minoris, BD+76°596, FK5 612, GC 21999, HD 148048, HIP 79822, HR 6116, SAO 8470, CCDM 16176+7545 |
F5V | - | 96.3 ly |
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|
LP 162-24 | - | 96.3 ly | |
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UPM J1454-5809 | - | 96.3 ly | |
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Gaia DR3 4119098594498186368 | - | 96.3 ly | |
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G 111-6 | - | 96.3 ly | |
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Gaia DR3 4117875800025750400 | - | 96.3 ly | |
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Beta Ceti bet Cet, Diphda, Deneb Kaitos, β Cet, 16 Cet, BD−18 115, GJ 31, HD 4128, HIP 3419, HR 188, SAO 147420, PLX 134.00 |
G9.5IIICH-1 | 3.5 M☉ | 96.3 ly |
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G 28-44 | - | 96.3 ly | |
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Gaia EDR3 4261087704930345600 | - | 96.3 ly | |
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Gaia DR3 4319092647002433024 | - | 96.3 ly | |
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LP 226-38 | M4.5Ve | - | 96.3 ly |
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2MASS J14282092-0012155 | - | 96.3 ly | |
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PM J16203-1707 | ~ | - | 96.3 ly |
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G 166-44 | - | 96.4 ly | |
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Gaia DR3 5899725308679263360 | - | 96.4 ly | |
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UPM J1840-2013 | - | 96.4 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
