Naines rouges | Stellar Catalog

	Mass	Distance
ADS 48 B ADS 48 B, HD 38B, SAO 36048, GC 72, GJ 4 B, CCDM J00057+4548B, WDS J00057+4549B	M0.5V	0.53 M☉	37.6 ly
Ross 119 GJ 9375, Gliese 9375, LFT 859, G 12-4, G 57-28, LHS 2472, LTT 13283, NLTT 28894, 2MASS J11540788+0948227, TIC 291108016, TYC 864-271-1, WISEA J115407.94+094814.2	M4.0V	-	37.6 ly
MCC 568 HIC 49969, HIP 49969, G 53-28, G 162-24, G 55-2, GJ 381 B, LFT 698, LHS 2230, L 968-22, LP 609-71, LTT 3730, NLTT 23666, 2MASS J10120466-0241044, TIC 77610900, TYC 4907-91-1, WDS J10121-0241AB, WISEA J101205.04-024111.4	M2.5V B	-	37.6 ly
Ross 85 LHS 2173, AC +13 1301, G 42-17, GJ 361, Gliese 361, HIC 47513, HIP 47513, LFT 670, LTT 12562, NLTT 22345, 2MASS J09411033+1312344, TIC 307646256, TYC 827-1159-1, WISEA J094109.88+131232.9	M2.5V	-	37.7 ly
Gliese 842 LHS 3741, DENIS J215934.4-594509, GJ 842, CD-60 7821, HIC 108569, HIP 108569, LFT 1672, L 165-2, LTT 8780, NLTT 52576, 2MASS J21593479-5945104, TIC 394015919, TYC 8820-224-1, WISEA J215935.92-594511.3	M0.5V	0.58 M☉	37.7 ly
SSSPM J1358-3938 2MASS J13580529-3937545, TIC 178930081, WISEA J135806.95-393804.2	M3.5 d	-	37.7 ly
HD 75632 BD+71 482A, G 252-24A, GC 12268, GJ 325, Gliese 325, HIC 43820, HIP 43820, 2MASS J08552479+7047389, WISE J085522.07+704735.1	M1V	-	37.8 ly
HD 75632 B	M1V	-	37.8 ly
Ross 52 B	M4	-	37.8 ly
SCR J1855-6914 2MASS J18554792-6914153, DENIS J185548.0-691415, TIC 381983159, WISEA J185548.76-691422.2	M6e D	-	37.9 ly
Wolf 230 G 97-20, G 85-41, GJ 3333, Gliese 3333, LTT 11586, NLTT 14527, 2MASS J05074924+1758584, TIC 27137427, WISEA J050749.30+175855.0	M2V	-	37.9 ly
L 308-57 2MASS J06210665-4905379, DENIS J062106.6-490537, TIC 238950307, Gaia DR2 5550620058937466880		-	38 ly
G 41-8 JNN 274, NLTT 20558, 2MASS J08561956+1239500, TIC 437041669, WDS J08563+1239AB, WISE J085619.51+123947.3	M6V C	-	38 ly
Gliese 2106 LTT 5557, NLTT 36550, GJ 2106, CD-56 5362, HIC 69454, HIP 69454, 2MASS J14131288-5644314, TIC 407559875, TYC 8673-4534-1, WISEA J141313.30-564429.5	M2V: D	0.5 M☉	38 ly
L 43-72 B		-	38.1 ly
LSR J2000+3057 2MASS J20000565+3057300, TIC 103245015, WISEA J200006.00+305745.6	M6Ve	-	38.1 ly
L 43-72 NLTT 45898, DENIS J181115.3-785922, 2MASS J18111528-7859227, TIC 276834958, WISEA J181115.56-785919.9	M4.5 D	-	38.1 ly
L 623-94 LHS 3064, DENIS J152212.8-274944, Gliese 2112, GJ 2112, 2MASS J15221293-2749436, NLTT 40004, WISEA J152213.31-274936.3	M3: E	-	38.2 ly
CD-35 2213 NLTT 14841, TSN 1, C* 315, CGCS 908, EUVE J0517-35.3, L 449-1, 2MASS J05172292-3521545, RBS 636, RE J0517-352, TIC 77957301, WDS J05174-3522AB, WISEA J051722.71-352156.4	M4Ve	-	38.2 ly
Gliese 572 GJ 572, BD+45 2247, G 179-6, G 201-30, HDS 2118A, HIC 73470, HIP 73470, LTT 14455, 2MASS J15005557+4525343, MCC 314, NLTT 39083, TIC 284266904, TYC 3481-1481-1, WISEA J150055.79+452537.7, RX J1500.9+4525 1	M0V	-	38.2 ly

Nom de l étoile

Mass

Distance

ADS 48 B

ADS 48 B, HD 38B, SAO 36048, GC 72, GJ 4 B, CCDM J00057+4548B, WDS J00057+4549B

M0.5V

0.53 M☉

37.6 ly

Ross 119

GJ 9375, Gliese 9375, LFT 859, G 12-4, G 57-28, LHS 2472, LTT 13283, NLTT 28894, 2MASS J11540788+0948227, TIC 291108016, TYC 864-271-1, WISEA J115407.94+094814.2

M4.0V

37.6 ly

MCC 568

HIC 49969, HIP 49969, G 53-28, G 162-24, G 55-2, GJ 381 B, LFT 698, LHS 2230, L 968-22, LP 609-71, LTT 3730, NLTT 23666, 2MASS J10120466-0241044, TIC 77610900, TYC 4907-91-1, WDS J10121-0241AB, WISEA J101205.04-024111.4

M2.5V B

37.6 ly

Ross 85

LHS 2173, AC +13 1301, G 42-17, GJ 361, Gliese 361, HIC 47513, HIP 47513, LFT 670, LTT 12562, NLTT 22345, 2MASS J09411033+1312344, TIC 307646256, TYC 827-1159-1, WISEA J094109.88+131232.9

M2.5V

37.7 ly

Gliese 842

LHS 3741, DENIS J215934.4-594509, GJ 842, CD-60 7821, HIC 108569, HIP 108569, LFT 1672, L 165-2, LTT 8780, NLTT 52576, 2MASS J21593479-5945104, TIC 394015919, TYC 8820-224-1, WISEA J215935.92-594511.3

M0.5V

0.58 M☉

37.7 ly

SSSPM J1358-3938

2MASS J13580529-3937545, TIC 178930081, WISEA J135806.95-393804.2

M3.5 d

37.7 ly

HD 75632

BD+71 482A, G 252-24A, GC 12268, GJ 325, Gliese 325, HIC 43820, HIP 43820, 2MASS J08552479+7047389, WISE J085522.07+704735.1

M1V

37.8 ly

HD 75632 B

M1V

37.8 ly

Ross 52 B

37.8 ly

SCR J1855-6914

2MASS J18554792-6914153, DENIS J185548.0-691415, TIC 381983159, WISEA J185548.76-691422.2

M6e D

37.9 ly

Wolf 230

G 97-20, G 85-41, GJ 3333, Gliese 3333, LTT 11586, NLTT 14527, 2MASS J05074924+1758584, TIC 27137427, WISEA J050749.30+175855.0

M2V

37.9 ly

L 308-57

2MASS J06210665-4905379, DENIS J062106.6-490537, TIC 238950307, Gaia DR2 5550620058937466880

38 ly

G 41-8

JNN 274, NLTT 20558, 2MASS J08561956+1239500, TIC 437041669, WDS J08563+1239AB, WISE J085619.51+123947.3

M6V C

38 ly

Gliese 2106

LTT 5557, NLTT 36550, GJ 2106, CD-56 5362, HIC 69454, HIP 69454, 2MASS J14131288-5644314, TIC 407559875, TYC 8673-4534-1, WISEA J141313.30-564429.5

M2V: D

0.5 M☉

38 ly

L 43-72 B

38.1 ly

LSR J2000+3057

2MASS J20000565+3057300, TIC 103245015, WISEA J200006.00+305745.6

M6Ve

38.1 ly

L 43-72

NLTT 45898, DENIS J181115.3-785922, 2MASS J18111528-7859227, TIC 276834958, WISEA J181115.56-785919.9

M4.5 D

38.1 ly

L 623-94

LHS 3064, DENIS J152212.8-274944, Gliese 2112, GJ 2112, 2MASS J15221293-2749436, NLTT 40004, WISEA J152213.31-274936.3

M3: E

38.2 ly

CD-35 2213

NLTT 14841, TSN 1, C* 315, CGCS 908, EUVE J0517-35.3, L 449-1, 2MASS J05172292-3521545, RBS 636, RE J0517-352, TIC 77957301, WDS J05174-3522AB, WISEA J051722.71-352156.4

M4Ve

38.2 ly

Gliese 572

GJ 572, BD+45 2247, G 179-6, G 201-30, HDS 2118A, HIC 73470, HIP 73470, LTT 14455, 2MASS J15005557+4525343, MCC 314, NLTT 39083, TIC 284266904, TYC 3481-1481-1, WISEA J150055.79+452537.7, RX J1500.9+4525 1

M0V

38.2 ly

Naines rouges nouvelles

Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774

Yesterday

Étoiles | Exoplanètes | Naines rouges | TESS

Image: Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774

A small planet candidate has been identified in the binary star system known as Gliese 774. The object, which is smaller than the Earth, orbits its host star approximately every 4.2 days. Observations from the Transiting Exoplanet Survey Satellite (TESS) captured the planet as it passed in front of its star, briefly blocking a tiny fraction of the starlight. This periodic dimming event allowed for the identification of the candidate despite the complex environment of a binary system, where two s...

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Ammonia and hydrogen may separate inside Uranus and Neptune

Yesterday

Étoiles | Exoplanètes | Naines rouge

Image: Ammonia and hydrogen may separate inside Uranus and Neptune

Uranus and Neptune may be experiencing ammonia rain: simulations show their expected temperature profiles cross the boundary where ammonia and hydrogen separate. In warmer sub-Neptune TOI-270 d, the two are likely to mix in all proportions....

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Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b

15. 10. 2026

Image: Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b

The exoplanet TOI-2257 b orbits its star once every 35 days with a high eccentricity. New models suggest its atmospheric and orbital fate depends on whether it is a gas-rich mini-Neptune or a rocky super-Earth. Higher eccentricity would confirm a gaseous nature....

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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.

Étoiles

Les étoiles sont d’immenses sphères de gaz chaud qui brillent en produisant de l’énergie grâce à la fusion nucléaire dans leur noyau. La plupart des étoiles sont composées principalement d’hydrogène et d’hélium. Au centre d’une étoile, la pression et la température élevées provoquent la fusion des atomes d’hydrogène en hélium, libérant ainsi une énorme quantité d’énergie sous forme de lumière et de chaleur.

More about Étoiles

Random terms

Position de la étoile Luminosité Température des étoiles Masse stellaire Taille de l´étoile L´âge des étoiles

TIC 220432308 1129 ly	+1	Two Validated Planets and 179 Candidates From a TESS Faint Star Transit Search in the ULTRASAT Fields yesterday
TOI 431 106 ly	+4	Thermal Evolution of Lava Planets Across System Ages: Predictions for Hell of a Survey yesterday
L 115-21 41.9 ly		A sub-Earth-sized TESS planet candidate in the nearby M-dwarf binary GJ 774, most likely orbiting GJ 774 A (TIC 351339274) yesterday
TOI-3686 841 ly		TOI-3686: A Hot Jupiter and Sub-Neptune In A 2:1 Mean-Motion Resonance yesterday
HD 112485 5881 ly		Ensemble pulsational characteristics of eclipsing binaries containing β Cep stars observed by the TESS mission 19. 10. 2026

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Frequently Asked Questions about nearby stars

What is the nearest star?

What are the nearest stars to Earth?

What is the solar neighborhood?

How do astronomers measure distances to stars?

Are there any exoplanets orbiting the nearest stars?

Why are the nearest stars important for astronomy and physics?

StellarGuide: Étoiles