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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

2MASS J0041-5621
DENIS J004135.3-562112, 2MASS J00413538-5621127
M6.5 0.03 M☉ 113 ly

HD 74014
K0III - 114 ly

HD 45652
HIP 30905
K5 0.92 M☉ 114 ly

SCR J1931-2724
- 114 ly

HD 65216
HD 65216, GSC 08915-02808, SAO 250002, Gaia DR3 5287961677550103424, CD-63 359, HIC 38558, TIC 382625142, Gaia DR2 5287961677550103424, CPC 20.1 1968, HIP 38558, TYC 8915-2808-1, Gaia DR1 5287961673251752320, CPD-63 834, 2MASS J07534133-6338502, uvby98 100065216, GEN# +1.00065216, PPM 356315, WDS J07537-6339A
G5V 0.95 M☉ 115 ly

TOI 7166
LP 577-37
M4.5V 0.19 M☉ 115 ly

HD 73344
TIC 175193677, BD+24 1968, FK5 4776, HIP 42403, 2MASS J08384552+2341094, TYC 1942-1827-1, WISEA J083845.48+234107.7, EPIC 212178066
F6V C 1.2 M☉ 115 ly

TOI-1634
UCAC4 636-014493, 2MASS J03453363+3706438, TIC 201186294, PM J03455+3706
M2 0.5 M☉ 115 ly

HIP 66074
BD+75 510, Gaia 3, Gaia-3, WIS 225 A
K7V 0.71 M☉ 115 ly

HD 60779
HD 60779
G1V 1.1 M☉ 116 ly

HD 110106
K3V - 116 ly

LHS 1903
Gaia DR2 978086481343568128, Gaia DR3 978086481343568128, HIP 34730, G 107-55, LSPM J0711 4819, NLTT 17491, TOI-1730, TIC 318022259, TYC 3396-1862-1, 2MASS J07112794 4819501
M0.5V - 116 ly

CD-27 1462
K7Ve - 116 ly

LHS 6343
0.36 M☉ 116 ly

LSPM J1639+2412
~ - 116 ly

HD 149499
RST 869, HIP 81478, 2MASS J16383108-5728112, TIC 221970504, V841 Ara, WISEA J163831.21-572811.2, Gaia DR3 5927299651589762048
K0V C - 117 ly

2MASS J03413724+5513068
M2V - 117 ly

Gliese 3275
LP 415-636, 2E 993, 2MASS J04220827+1915218
M3 0 M☉ 117 ly

TOI 5720
TIC 230055368, 2MASS J11211567+2516255
M3.5 0.38 M☉ 117 ly

WISEA J032504.52-504403.0
T8 - 117 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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