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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 2421-2440
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Star name Mass Distance

LP 829-41
M5.5Ve - 62.9 ly

LP 694-16
M4 - 62.9 ly

HD 21209
K3.5V - 62.9 ly

HD 148653
K3V - 63 ly

MV Ursae Majoris
PLX 2696, SBC9 681, LSPM J1138 + 4219, ASCC 408284, USNO-B1.0 1323-00273854, GSC 03015-01701, AG + 42 1102, AGKR 10454, BD + 43 2135, Ci 18 1435, Ci 20 654, Furuhjelm I-867, G 122-38, G 176-45, GC 15983, GCRV 7082, GEN # +1.00101206, GJ 10167, Gliese 10167, HIC 56829, HIP 56829, LHS 6210, LTT 13186, NGP 43 2, NLTT 28095, PPM 52559, SAO 43847, SBC7 438, J859171713028185921 TYC 301381, PLX 2696,00, [ZEH2003] RX J1138.9 + 4219 1, RX J1138.9 + 4219, 1RXS J113858.9 + 421 957, WISEA J113859.59 + 421948,3, Gaia DR1 772395270561409920, MV UMa
K5V - 63 ly

HD 194640
HIP 100925, TYC 7455-1420-1, Gliese 790, GJ 790
G8V - 63 ly

G 242-60
M3.5 - 63 ly

StKM 1-852
M2.5Ve - 63 ly

G 189-38
M2+V - 63 ly

G 168-24
M3.0Ve - 63 ly

HD 130307
K1V - 63 ly

2MASSI J1424187-351432
M6.5 - 63 ly

GIC 84
G 115-69
M5V - 63 ly

LDS 9172
G 247-22, 2MASS J04331742+6846543, TIC 280978675, WISEA J043318.02+684649.4
M5.0 - 63 ly

PM J07105-0842
M3.5V - 63.1 ly

EC 19249-7343
DENIS J193101.3-733705, TIC 340844848, WISEA J193101.98-733706.8
- 63.1 ly

LP 777-1
DAH9 - 63.1 ly

2MASS J02132880+4444453
L1.5 - 63.1 ly

LP 604-16
M5V - 63.1 ly

110 Herculis
BD+20° 3926, FK5 703, Gliese 9635, GJ 9635, HD 173667, HIP 92043, HR 7061, SAO 86406, 110 Her
F5.5IV-V - 63.1 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.
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

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