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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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HD 94765 | K0V | - | 56.4 ly |
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LP 134-7 | - | 56.4 ly | |
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LP 739-2 | M4.5V | - | 56.4 ly |
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EGGR 378 | DA3.4 | - | 56.5 ly |
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Wolf 1450 | M3 | - | 56.5 ly |
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StM 162 | M4.0Ve | - | 56.5 ly |
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L 74-208 | - | 56.5 ly | |
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UPM J0850-2822 | - | 56.6 ly | |
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Gaia EDR3 4077001760212546432 | - | 56.6 ly | |
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Gaia EDR3 4525711600783788160 | M5.5 | - | 56.6 ly |
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HD 10647 q01 Eri, q1 Eridani, 5 G. Eridani, Gliese 3109, GJ 3109, HR 506, HIC 7978, HIP 7978, SAO 232501, CPD−54° 365, WISE J014229.49-534428.1, TIC 229137615, TYC 8475-527-1, 2MASS J01422932-5344271 |
F9V | 1.1 M☉ | 56.6 ly |
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Iota Horologii ι Hor, GJ 108, Gliese 108, HD 17051, HIC 12653, HIP 12653, HR 810, 2MASS J02423346-5048008, LTT 1322, NLTT 8800, TIC 166853853, TYC 8056-1164-1, WISEA J024233.84-504758.7 |
F8V C | 1.3 M☉ | 56.6 ly |
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G 21-13 | M2.5Ve | - | 56.6 ly |
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LP 768-712 | M3.0 | - | 56.6 ly |
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RX J1206.9+7007 | M3.5 | - | 56.6 ly |
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Gaia EDR3 2052469973468984192 | M2V | - | 56.6 ly |
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G 136-72 | M4.27 | - | 56.7 ly |
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LSPM J2127+5553 | - | 56.7 ly | |
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2MASS J11155037-6731332 | - | 56.7 ly | |
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HD 200968 | K1IV | - | 56.7 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
