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List of nearest stars

        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.
    
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Stars 1381-1400
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Star name Mass Distance

G 221-22
M1V - 52 ly

Wolf 1246
M3.5V - 52.1 ly

HD 275122
Wolf 1325, LHS 1528, HIP 15366, GJ 134, GL 134, Gliese 134, TYC-2848-1804-1, BD +37 748
M1.5Ve - 52.1 ly

ULAS J090116.23-030635.0
T7.5 - 52.1 ly

2MASS J0642+4101
2MASS J06420559+4101599
L9 0.01 M☉ 52.1 ly

G 230-42
M4.0Ve - 52.1 ly

Gliese 676
CD–51°10924, HIC 85647, HIP 85647, LTT 6947, NLTT 44859, NSV 8846, DENIS J173011.2-513812, GJ 676 A, 2MASS J17301119-5138132, TIC 369021303, TYC 8354-785-1, WISEA J173010.92-513814.7
M0V 0.71 M☉ 52.1 ly

StM 162
- 52.1 ly

G 264-12
LSPM J2146+6648, NLTT 52122, 2MASS J21464021+6648105, TIC 322391844, WISEA J214640.94+664812.8
M4.0V C - 52.1 ly

BD+46 1635
K7V - 52.2 ly

G 152-50
M2.5V - 52.2 ly

LP 535-12
M6.5V - 52.2 ly

Gliese 777
BD+29°3872, GJ 777, HD 190360, HIC 98767, HIP 98767, HR 7670, LHS 3510, GJ 9683, Gliese 9683, 2MASS J20033732+2953493, TIC 105999792, TYC 2153-2883-1, WISEA J200337.97+295343.4
G7IV-V C 0.82 M☉ 52.2 ly

L 524-9
- 52.2 ly

G 193-81
M4V - 52.2 ly

G 96-10
L 1600-17, LP 202-2, LTT 11541, NLTT 14165, 2MASS J04560354+4313556, TIC 446098056, WISEA J045603.91+431353.9
M4.0V - 52.2 ly

UCAC4 255-076386
- 52.3 ly

EGGR 169
GJ 3285, Gliese 3285, G 83-10, LP 475-70, LSPM J0425+1211, 2MASS J04255373+1211485, TIC 60878053, WISEA J042553.67+121145.9
DA8 - 52.3 ly

UPM J0840-3832
- 52.3 ly

Ross 476
GJ 514.1, Gliese 514.1, GJ 9447, Gliese 9447, G 14-57, LHS 353, 2MASS J13300285-0842251, WISEA J133002.00-084230.4
M4V - 52.4 ly
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Frequently Asked Questions about nearby stars

What is the nearest star?

Nearest star is Proxima Centauri, located approximately 4.24 light-years (1.30 parsecs) from the Sun. It is part of the Alpha Centauri star system, which also includes Alpha Centauri A and Alpha Centauri B.

What are the nearest stars to Earth?

Nearest stars to Earth include the Alpha Centauri system (Alpha Centauri A, Alpha Centauri B, and Proxima Centauri), Barnard's Star, and Wolf 359. There are also brown dwarfs Luhman 16 and WISE 0855−0714.

What is the solar neighborhood?

Solar neighborhood (also Local Interstellar Cloud) is the region of interstellar space that surrounds the Sun with diameter about 15 light years. Stellar Catalog database includes all stars contained within this region.

How do astronomers measure distances to stars?

Astronomers use methods like parallax, standard candles, and redshift to measure distances to stars. Parallax is especially useful for nearby stars in our solar neighborhood, while other techniques help map the universe beyond.

Are there any exoplanets orbiting the nearest stars?

Yes, several exoplanets have been discovered orbiting the nearest stars. For example, Proxima Centauri has an exoplanet called Proxima Centauri b, which is located in the star's habitable zone and is the closest known exoplanet to Earth.

Why are the nearest stars important for astronomy and physics?

The nearest stars provide valuable laboratories for studying stellar evolution, space environments, and the fundamental physics of stars. Observing these stars helps astronomers understand the structure of our galaxy and the broader universe.
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exoplanet iconStellarGuide: Stars

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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 tag icon

Stellar Evolution

Stars are born and die in various ways depending on their mass, composition, and other factors. The most common life cycle for stars like our Sun involves several key stages.
Stellar evolution visualisation

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