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Lista de Enanas naranjas

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Más sobre Enana naranja
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Estrellas 381-400
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Nombre de la estrella Mass Distance

BD+75 403
 K5 - 68.7 ly

HD 218572
 K3+Vk: - 68.7 ly

BD+33 99
 K5-V - 68.7 ly

HD 7693
 K2V - 68.8 ly

BD+11 2874
 K5V - 68.8 ly

HD 90343
 K0 - 68.8 ly

HD 183783
 K4+V - 68.9 ly

HD 66020
 K5V - 69 ly

HD 72760
 K0V - 69 ly

BD+10 4534
 K7.5Ve - 69.2 ly

HD 16270
GJ 1048, Gliese 1048
 K3.5Vk: - 69.3 ly

HD 155674
BD+54 1861
 K6V - 69.3 ly

HD 155674 B
BD+54 1862
 K6V - 69.3 ly

13 Ceti B
 K3.5 V 0.9 M☉ 69.3 ly

HD 95174 B
 K5 - 69.4 ly

HD 93380
 K5Vk: - 69.4 ly

HD 95174
 K4V - 69.4 ly

HD 175742
 K0V - 69.6 ly

V* V2578 Oph
 K2V - 69.6 ly

BD+19 451
 K5 - 69.8 ly
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Enana naranja noticias

Sub-Neptune planet candidate observed orbiting the orange dwarf star TIC 402710280
iconToday
iconEstrellas | Exoplanetas | Enana naranj
Image: Sub-Neptune planet candidate observed orbiting the orange dwarf star TIC 402710280
A potential sub-Neptune planet candidate has been identified orbiting the orange dwarf star TIC 402710280. This star, located about 218 light-years away, was monitored using the Transiting Exoplanet Survey Satellite. A sub-Neptune is a type of planet that is larger than Earth but smaller than Neptune, representing one of the most common types of worlds found in our galaxy. This specific candidate completes a full trip around its host star in approximately 36.34 days. The planet was identified...
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Oscillation patterns in Gliese 570 A and Gliese 783 A reveal new stellar physics
icon18. 10. 2026
iconEstrellas | Enana naranj
Image: Oscillation patterns in Gliese 570 A and Gliese 783 A reveal new stellar physics
New measurements of orange dwarfs Gliese 570 A and Gliese 783 A reveal stellar oscillation patterns that challenge current convection models. The observed vibration strengths are steeper than theory predicts, pointing to gaps in our understanding of stellar physics....
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Massive brown dwarf HD 203771 b confirmed in eccentric orbit around orange dwarf
icon14. 10. 2026
iconEstrellas | Exoplanetas | Enana naranja | Enanas marrone
Image: Massive brown dwarf HD 203771 b confirmed in eccentric orbit around orange dwarf
Massive brown dwarf HD 203771 b confirmed in an eccentric orbit around an orange dwarf star. New mass measurements place the companion at approximately 70 times the mass of Jupiter, revealing insights into how brown dwarfs migrate inward over time....
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study iconResearch in Enanas naranjas

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Explore los últimos estudios científicos sobre estrellas y exoplanetas en nuestra galaxia. Descubra las últimas investigaciones sobre astrofísica y astronomía estelar.
La investigación actual

 WISE 0855-0714
7.3 ly
 study icon Water Cloud and Chemical Modulations in the Coldest Brown Dwarf
17. 10. 2026

HD 203771
184 ly
 study icon An Intermediate-orbit Brown Dwarf Confirmed with Astrometry+Radial Velocity Joint Analysis, and the Eccentricity Distribution of Brown Dwarfs Across Different Locations
14. 10. 2026

HD 89744
126 ly
 +2 study icon Gaseous SiO and Silicate Clouds in Three Benchmark Early-L Dwarfs
9. 10. 2026

DENIS J1253-5709
54.4 ly
 study icon Astrometric planet search around southern ultracool dwarfs: V. Discovery of the exoplanet candidate PALTA-1 b
9. 10. 2026

2MASS 0036+1821
28.5 ly
 study icon A Jupiter-like radio aurora in the L3.5 dwarf LSPM J0036+1821
9. 10. 2026
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Publicaciones más antiguas

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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Posición de la estrellaLuminosidadTemperatura de la estrellaMasa estelarTamaño de la estrellaEdad de las estrellas

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