do not follow here
Stellar Catalog more icon Catalogue étoile more icon
Naines rouges
more icon
Filter stellar categories
Recommended categories

Liste des Naines rouges

        
    
Plus à propos Naines rouges
Advertisement
<< <
Etoile 401-420
>
Nom de l étoile Mass Distance

Gliese 4048
LHS 462, GJ 4048, G 204-58, 2MASS J18180427+3846342, NLTT 46274, TIC 76349247, WISEA J181803.91+384621.7
M3V 0.32 M☉ 37.1 ly

Gliese 4049
G 204-57, LHS 461, GJ 4049, Gliese 4048 B, 2MASS J18180345+3846359, NLTT 46272, TIC 76349243, WISEA J181803.10+384623.4
M4V - 37.1 ly

LSR J0539+4038
2MASS J05392474+4038437, TIC 239097694, WISEA J053925.39+403834.1
M8.0Ve - 37.1 ly

LP 838-16
M3 - 37.2 ly

WOH G 618
2MASS J05532643-7133502, TIC 31381302, WISEA J055326.47-713345.6
M6.0 D - 37.2 ly

G 34-23
LP 351-34, LTT 10491, 2MASS J01221027+2209032, NLTT 4534, TIC 411628298, WISEA J012210.48+220901.5
M4.0V C - 37.2 ly

Ross 52
GJ 568, GJ 568 A, Gliese 568, G 166-53, G 167-3, HIC 72896, HIP 72896, LFT 1155, LHS 2997, LTT 14417, NLTT 38729, 2MASS J14535144+2333208, TIC 311182575, TYC 2017-588-3, WISEA J145350.90+233321.9
M3V - 37.3 ly

PM J05366+1117
2MASS J05363846+1117487, TIC 436248798, WDS J05365+1120B
M4.0V - 37.3 ly

OT Serpentis
BD+21 2763, GJ 9520, Gliese 9520, HIC 75187, HIP 75187, 2MASS J15215291+2058394, RBS 1489, TIC 355793860, TYC 1493-378-1, USNO-B1.0 1109-00243006, V* OT Ser
M1.0V 0.55 M☉ 37.3 ly

Gliese 3417 B
M5 V 0 M☉ 37.4 ly

Gliese 1187
GJ 1187, G 201-27, LHS 3006, LP 98-348, 2MASS J14575374+5639242, NLTT 38963, TIC 405503787, WISEA J145754.09+563917.6
M5.5V - 37.4 ly

UCAC2 16493854
- 37.5 ly

Gliese 3417
G 250-31, HEN 2, LHS 1885, NLTT 17183, PLX 1611.01, 2MASS J06575703+6219197, GJ 3417
M6 V 0.16 M☉ 37.5 ly

RX J0713.1-0511
TYC 4823-2265-1, TIC 23369524, 2MASS J07131123-0511482, SCR J0713-0511
M3Ve - 37.5 ly

PM J00156+4735
TYC 3251-1875-1, 2MASS J00153905+4735220, TIC 440065990
- 37.5 ly

ADS 48 F
ADS 48 F, HIP 428, GJ 2, Gliese 2, CCDM J00057+4548F, WDS J00057+4549F, BD+44 4548
M2Ve 0.49 M☉ 37.5 ly

Gliese 494
BEU 16, G 60-57, G 61-27, BD+13 2618, GJ 494, HIC 63510, HIP 63510, LFT 964, LHS 2665, LTT 13752, NLTT 32600, 2MASS J13004666+1222325, Ross 458, TIC 88138162, TYC 886-839-1, V* DT Vir, WISEA J130046.11+122232.4, Wolf 462, DT Virginis, DT Vir
M0V 0.51 M☉ 37.5 ly

Gliese 494 B
M7V 0.09 M☉ 37.5 ly

Gliese 3668
LHS 306, LP 732-35, GJ 3668, 2MASS J11310835-1457201, NLTT 27616, WISEA J113108.68-145735.8
M5 - 37.5 ly

UCAC4 427-122653
2MASS J21471744-0444406, TIC 24352777, WISEA J214717.63-044440.6, PM J21472-0444
M4.0V - 37.5 ly
<< <
Etoile 401-420
>
Charger toutes les étoiles
dans le catalogue

Naines rouges nouvelles

Sub-Earth-sized planet candidate observed around the red dwarf Gliese 774
iconYesterday
iconÉtoiles | 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...
Read article tag icon
Advertisement
Ammonia and hydrogen may separate inside Uranus and Neptune
iconYesterday
iconÉtoiles | 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....
Read article tag icon
Orbital and atmospheric evolution of the mini-Neptune TOI-2257 b
icon15. 10. 2026
iconÉtoiles | Exoplanètes | Naines rouges | Super-Terre | Atmosphères planétaires | TESS
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....
Read article tag icon

study iconResearch in Naines rouges

line

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: Étoiles

line
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 tag icon

Advertisement