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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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Star name Mass Distance

G 154-43
M5.0V - 43.1 ly

LP 500-35
M7V - 43.1 ly

BD+57 2735
M1.5Ve - 43.2 ly

HD 128165
HIC 71181, HIP 71181, SAO 29196, Gliese 556, GJ 556, GL 556, TYC-3860-1045-1, BD+53 1719
K3V 0.78 M☉ 43.2 ly

LP 35-347
M7V - 43.2 ly

58 Eridani
58 Eri, IX Eri, IX Eridani, BD−17°954, Gliese 177, GJ 177, HD 30495, HIC 22263, HIP 22263, HR 1532, SAO 149888, LTT 2088
G2.5IV-V 1.1 M☉ 43.2 ly

LP 912-33
M3 - 43.2 ly

G 44-42
M4V - 43.2 ly

LP 21-224
M4.0V - 43.2 ly

2MASS J11220826-3512363
TIC 57183112, WISEP J112208.14-351239.7
T2 0 M☉ 43.2 ly

SSSPM J0306-3648
M8.7V - 43.2 ly

LP 255-11
M4.0V - 43.3 ly

HD 214749
LTT 9143, GJ 868.0, Gliese 868.0, PLX 5486, UBV 19400, CD-30 19255, HD 214749, PLX 5486.00, UBV M 26543, CPC 17 12286, HIC 111960, PPM 274115, UGP 576, CPD-30 6663, HIP 111960, SAO 191319, WISEA J224043.67-294028.1, GCRV 73405, IRAS 22379-2955, SKY# 43116, Gaia DR1 6608490497012980224, GEN# +1.00214749, 2MASS J22404335-2940278, TIC 47295522, Gaia DR2 6608490501308343168, GJ 868, Gliese 868, NLTT 54520, TYC 6969-1175-1
K4.5Vk - 43.3 ly

BD-07 4156
M1V - 43.3 ly

G 23-24
M2.5Ve - 43.3 ly

LP 801-9
DC10 - 43.4 ly

2MASS J1225-2739
2MASS J12255432-2739466, 2MASSI J12255432-2739466, 2MASSW J1225543-273947, TIC 443626421, WDS J12259-2740AB
T5.5+T8 - 43.4 ly

2MASS J16283855+2308241
SDSS J162838.77+230821.1, TIC 345664442, WISE J162838.09+230822.7
T7.0 - 43.4 ly

2MASS J15530228+1532369
BUG 11, SDSS J155302.09+153237.8, TIC 172607100, WISE J155301.95+153238.8, EQ J1553+1532
T6.5+T7.5 - 43.4 ly

LP 357-56
- 43.5 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.
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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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