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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 681-700
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Star name Mass Distance

G 207-19
M3V - 40.7 ly

LHS 475
L 22-69, GJ 4102, Gliese 4102, LFT 1458, 2MASS J19205439-8233170, TIC 369327947, TOI-910, WISEA J192056.23-823329.0
M3.5V 0.26 M☉ 40.7 ly

G 205-35
M4 - 40.7 ly

Gaia EDR3 5600272629670698880
- 40.7 ly

Gliese 3250
LHS 1593, G 79-70, GJ 3250, G 7-4, LTT 11262, NLTT 11842, 2MASS J03472091+0841464, TIC 468889408, WISEA J034721.21+084140.2, Gaia DR2 3278325004913943808, Karmn J03473+086, PLX 823.01, USNO-B1.0 0986-00032676
M5V - 40.7 ly

LP 649-72
2MASS J02141251-0357434, LHS 1363, NLTT 7395, WISEA J021412.91-035745.1
M5.5V C - 40.7 ly

HD 21531
K5V - 40.7 ly

PM J07199+8404
M2.5Ve - 40.8 ly

L 211-59
M4V - 40.8 ly

WISEP J180435.40+311706.1
T9.5: - 40.8 ly

LP 888-18
M7.5V - 40.8 ly

SCR J1841-4347
- 40.8 ly

Gliese 1029
GJ 1029, G 69-47, LHS 135, LTT 17177, NLTT 3592, 2MASS J01053732+2829339, TIC 15615674, WISEA J010539.17+282931.6
M5.42 - 40.8 ly

VB 24
M3V - 40.8 ly

UCAC4 767-032810
- 40.9 ly

Lambda Aurigae
15 Aurigae, BD+39° 1248, FK5 1145, GJ 197, Gliese 197, HD 34411, HIP 24813, HIC 24813, HR 1729, LFT 403, LHS 1753, LTT 11625, SAO 40233, NLTT 14837, TIC 409104974, TYC 2900-2157-1, STF 5003A, 15 Aur, TD1 4327, Al Hurr, * lam Aur
G1.5IV-VFe-1 1.1 M☉ 41 ly

CFBDS J003402-005206
T8+/Y? - 41 ly

SIPS J0921-2104
L1 - 41 ly

HD 69830
285 G. Puppis, BD−12°2449, Gliese 302, GJ 302, HIP 40693, HR 3259, LHS 245, SAO 154093, 2MASS J08182389-1237541, Gaia DR2 5726982995343100928
G8V 0.86 M☉ 41 ly

G 76-62
M5.04 - 41.1 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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