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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.
| Star name | Mass | Distance | ||
|---|---|---|---|---|
|
|
LSPM J1754+1251 | M2.0Ve | - | 67.5 ly |
|
|
HD 137778 | K1V | - | 67.5 ly |
|
|
G 64-28 | M3.0V | - | 67.5 ly |
|
|
2MASS J1746+5034 2MASS J17461199+5034036 |
L5.7V | - | 67.5 ly |
|
|
LP 356-15 L 1307-14 C, HAT 259-00479, TIC 25909530, WISEA J032413.01+234617.8, LTT 11121, 2MASS J03241281+2346193 |
M2.5Ve | - | 67.5 ly |
|
|
UCAC4 326-054121 TIC 37926636, 2MASS J09053652-2453176, WISE J090536.51-245317.6 |
- | 67.5 ly | |
|
|
L 38-47 | M3 | - | 67.5 ly |
|
|
UPM J0432+6300 | - | 67.5 ly | |
|
|
Gaia DR2 6067637295632046464 | - | 67.5 ly | |
|
|
L 886-6 | DA7.6 | - | 67.5 ly |
|
|
2MASS J2259-5420 2MASS J22590642-5420357 |
- | 67.5 ly | |
|
|
2MASSI J1526140+204341 | L5 | - | 67.5 ly |
|
|
CD-36 9107 | M0 | - | 67.5 ly |
|
|
LP 474-219 | - | 67.5 ly | |
|
|
LSPM J0225+6229 | - | 67.5 ly | |
|
|
LP 758-16 | M5.5Ve | - | 67.5 ly |
|
|
G 10-52 | M3.5V | - | 67.5 ly |
|
|
2MASS J1138-3455 | - | 67.6 ly | |
|
|
L 17-50 | - | 67.6 ly | |
|
|
LP 584-4 | M6.5e | - | 67.6 ly |
StellarGuide: 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
