do not follow here
Stellar Catalog more icon
Nearby stars catalogue
more icon
Filter stellar categories
Recommended categories

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.
    
Advertisement
<< <
Stars 9881-9900
>
Star name Mass Distance

TOI 880
TIC 34077285
- 198 ly

TOI 5319
M1V 0.5 M☉ 198 ly

TOI 521
- 199 ly

HD 184010
HD 184010
K0III-IV D 1.4 M☉ 200 ly

HIP 65407
K0 0.93 M☉ 201 ly

TOI 4342
TIC 354944123
M0V 0.63 M☉ 201 ly

TOI 1075
0.6 M☉ 201 ly

HIP 65
TOI-129
K4V 0.78 M☉ 202 ly

K2-141
K7V 0.71 M☉ 202 ly

HD 140283
BD−10 4149, GJ 1195, Gliese 1195, HIP 76976, SAO 159459, ,
G0IV-V m-5 0.81 M☉ 202 ly

TOI 122
TOI-122, TOI-122
0.31 M☉ 203 ly

TOI 2081
TIC 321669174, 2MASS J17371272+5301326, WISE J173712.60+530132.2
M1.0 0.54 M☉ 203 ly

2MASS J1155-4008
NGTS-EB-8, 2MASS J11551666-4008570, TIC 165227846
0.25 M☉ 203 ly

K2-2
HIP 116454, BD-00 4534, TOI-6836
K2V 0.78 M☉ 204 ly

HD 177830
BD+25°3719, GJ 743.2, Gliese 743.2, HIC 93746, HIP 93746, GSC 02126-01196, SAO 86791
K0IV 1.5 M☉ 205 ly

HD 25295
TOI 4602, TIC 467651916, HIP 18841, HD 25295, TYC 2357-595-1, 2MASS J04022420 3119501, Gaia 169256041140206848
G5 0.9 M☉ 205 ly

HIP 82724
HIC 82724, 2MASS J16543253-6224142, GSC 09043-00362, HDS 2393A, TYC 9043-362-1, TIC 447555555, Gaia DR2 5818211949014482816
K0 IV 0 M☉ 205 ly

TOI 178
2MASS J00291228-3027133, Gaia DR2 2318295979126499200, TIC 251848941, TYC 6991-00475-1
K7V 0.65 M☉ 205 ly

HD 22946
TOI 411
F7/8V 1.1 M☉ 205 ly

HD 190228
G5IV 1.3 M☉ 205 ly
<< <
Stars 9881-9900
>
Load all stars
in the catalogue

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.
Advertisement

exoplanet iconStellarGuide: Stars

line
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

Advertisement