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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 841-860
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Star name Mass Distance

G 194-47
M3.5V - 43.9 ly

MCC 573
dM3.0 - 43.9 ly

LP 639-1
M5.03 - 43.9 ly

G 172-1
M3.7V - 44 ly

LP 672-42
HIC 56157, HIP 56157, 2MASS J11304179-0805425, TIC 285972083, TYC 5509-47-1, WISEA J113041.56-080540.1
M3.0V - 44 ly

Upsilon Andromedae
Titawin, 50 Andromedae, υ-Andromedæ, BD+40 332, CCDM 01367+4125, FK5 1045, GC 1948, GCTP 331.00, Gliese 61, Gl 61, HD 9826, HIC 7513, HIP 7513, HR 458, LTT 10561, SAO 37362, WDS 01368+4124A, 2MASS J01364784+4124200, Gaia DR2 348020448377061376
F9V 1.3 M☉ 44 ly

2MASS J0642-6707
SCR J0642-6707, TIC 176935123, 2MASS J06422703-6707193
M5.0 - 44 ly

2MASS J1254-0122
2MASS J12545393-0122474
T2e: - 44 ly

G 192-11
M0.0V - 44 ly

UCAC4 672-033085
PM J05050+4414
M5.0V - 44 ly

L 266-69
2MASS J16331968-5207561, NLTT 42999, TIC 23257970, WISEA J163319.44-520759.9
M4e - 44 ly

BD+62 780
K7V - 44 ly

HD 120476
Gl 528, Gliese 528, HIC 67422, HIP 67422, LHS 6259, LTT 14035, NLTT 35353, BD+27 2296,
K4V - 44 ly

Gliese 1073
G 81-39, GJ 1073, G 96-6, 2MASS J04523448+4042255, NLTT 14072, TIC 187391650, WISEA J045235.67+404212.7
M5V - 44 ly

G 129-47
M3V - 44 ly

G 248-12
M4.5 - 44.1 ly

PM J17476-5436
DC - 44.1 ly

2MASS J1555-0956
2MASS J15551573-0956055
L1.6V - 44.1 ly

HD 10436
BD+63° 229, Gliese 69, GJ 69, HD 10436, HIP 8070, SAO 11943, LHS 1291
K5Vbe 0.62 M☉ 44.1 ly

L 744-10
M4.5 - 44.1 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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