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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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|
PM J15546-1309 | - | 89.9 ly | |
|
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UPM J1306+1330 | - | 89.9 ly | |
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UCAC4 200-010229 | - | 89.9 ly | |
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WT 135 | M3.0VI | - | 89.9 ly |
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Gaia DR3 5854156118019936000 | - | 89.9 ly | |
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PM J15545-1310 | - | 90 ly | |
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HD 73524 | G0Vp | - | 90 ly |
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LP 644-40 | - | 90 ly | |
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G 203-71 | M2.5 | - | 90 ly |
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Ross 593 | M3 | - | 90 ly |
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2MASS J22273598+1614559 | - | 90 ly | |
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B Carinae B Car, CPD−60°1074, FK5 2636, GJ 297.1, Gliese 297.1, HD 68456, HIP 39903, HR 3220, SAO 250131 |
F6VFe-0.8CH-0.4 | 1.4 M☉ | 90 ly |
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13 Orionis | G3 | - | 90 ly |
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Beta Eridani bet Eri, Cursa/Kursa,[11] Dhalim,[12] β Eri, Beta Eri, 67 Eridani, 67 Eri, BD−05 1162, CCDM J05079-0506A, FK5 188, GC 6274, GJ 9175, Gliese 9175, HD 33111, HIP 23875, HR 1666, IDS 05030-0513 A, PPM 187729, SAO 131794, WDS 05078-0505A |
A3IV | 2 M☉ | 90 ly |
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LP 870-54 | M2.5 | - | 90 ly |
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2MASS J17503293+1759042 | T3.5 | - | 90 ly |
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G 272-147 | M4/5 | - | 90 ly |
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HD 40650 | F5 | - | 90 ly |
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G 111-52 | - | 90 ly | |
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G 264-20 | - | 90 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
