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Lista de Enanas marrones

        
    
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Estrellas 41-60
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Nombre de la estrella Mass Distance

Scholzs Star B
T5.5 0.06 M☉ 22.2 ly

WISE 1928+2356
WISE J192841.35+235604.9
T6 0.02 M☉ 22.3 ly

WISE 2056+1459
WISE J205628.91+145953.2, WISEPC J2056+1459
Y0 0.02 M☉ 22.7 ly

WISE J0005+3737
WISE J000517.48+373720.5
T9 0.02 M☉ 23.2 ly

WISEA J082507.37+280548.2
WISE J0825+2805
Y0.5 0 M☉ 23.5 ly

2MASS 0835-0819
2MASS J08354256-0819237, 2MUCD 10742, WISEA J083542.14-081920.1
L5 0.06 M☉ 23.6 ly

Gaia EDR3 3426333598021539840
- 23.6 ly

WISE 0607+2429
WISEP J060738.65+242953.4, 2MASS J06073908+2429574, TIC 81192866
L8 0.05 M☉ 23.8 ly

WISE 0049+2151
WISEP J004945.61+215120.0, WISE J004945.61+215120.0
T8.5 0.02 M☉ 24.1 ly

2MASS J1507-1627
2MASSW J1507476-162738, MUCD 11296, WISEA J150747.56-162749.3
L5 0.07 M☉ 24.2 ly

WISE 1405+5534
WISEPC J140518.40+553421.4, WISE J140518.39+553421.3
Y0 0.03 M☉ 24.5 ly

WISE 1800+0134
WISEP J180026.60+013453.1, DENIS J180026.4+013457, 2MASS J18002648+0134565
L7.5 0.05 M☉ 25.5 ly

2MASS 0729-3954
2MASS 0729-39, 2MASS J07290002-3954043, WISEA J072859.49-395345.3, TIC 173510894
T8 D 0.04 M☉ 25.8 ly

2MASSW J2148162+400359
L7 0.05 M☉ 26.4 ly

WISE 2220-3628
WISE J222055.31−362817.4
Y0 - 26.4 ly

UGPS J0521+3640
T8.5 0.02 M☉ 26.7 ly

Gaia EDR3 4479498508613790464
- 26.7 ly

2MASS 0036+1821
LSPM J0036+1821, 2MASS J00361617+1821104, 2MASSW J0036159+182110, USNO-B1.0 1083-00010105, Gaia DR3 2794735086363871360, BNA 1A, 2MASSW J0036162+182110, WDS J00363+1821A, Gaia DR2 2794735086363871360, CNS5 175, 2MUCD 20029, WISEA J003616.79+182111.6, TIC 426959594
L3.5 - 28.5 ly

Xi Ursae Majoris C
WISE J111838.70+312537.9, WISE J1118+3125
T8.5 - 28.8 ly

WISE 1217+1626
WISEPC J121756.91+162640.2, LIM 4, EQ J1217+1626, WISEA J121756.92+162640.3
T9 0.02 M☉ 28.9 ly
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Enanas marrones noticias

Massive brown dwarf HD 203771 b confirmed in eccentric orbit around orange dwarf
iconYesterday
iconEstrellas | Exoplanetas | Enana naranja | Enanas marrone
Image: Massive brown dwarf HD 203771 b confirmed in eccentric orbit around orange dwarf
The massive brown dwarf known as HD 203771 b has been characterized as orbiting its host orange dwarf star once every 1140 days. Brown dwarfs are often called failed stars because they are more massive than planets but not heavy enough to sustain the nuclear fusion that powers stars. This particular companion follows an eccentric, or elongated, path that is inclined at an angle of approximately 130 degrees relative to its host. The host star itself has a mass estimated at 0.79 times that of the ...
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Silicate clouds and gaseous silicon monoxide identified in three early L-dwarf objects
icon9. 10. 2026
iconEstrellas | Enanas marrones | Atmósferas planetari
Image: Silicate clouds and gaseous silicon monoxide identified in three early L-dwarf objects
Analysis of three early L-dwarfs, HD 89744 B, Gliese 1048 B, and LSPM J0632+5053 B, reveals gaseous silicon monoxide and silicate clouds in their atmospheres. JWST data confirms these mineral clouds form as silicon gas condenses, mimicking processes in giant planets....
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Exoplanet candidate PALTA-1 b found orbiting a nearby ultracool dwarf
icon9. 10. 2026
iconEstrellas | Exoplanetas | Enanas marrone
Image: Exoplanet candidate PALTA-1 b found orbiting a nearby ultracool dwarf
A new exoplanet candidate, PALTA-1 b, has been identified orbiting the nearby ultracool dwarf star DENIS-P J1253108-570924. The planet, which has a mass roughly equivalent to a fraction of Jupiter, was found after eight years of precise positional monitoring....
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study iconResearch in Enanas marrones

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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: Estrellas

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Estrellas
Las estrellas son enormes esferas de gas caliente que brillan al generar energía mediante fusión nuclear en sus núcleos. La mayoría de las estrellas están compuestas principalmente de hidrógeno y helio. En el centro de una estrella, la alta presión y temperatura hacen que los átomos de hidrógeno se fusionen en helio, liberando una enorme cantidad de energía en forma de luz y calor.
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