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Lista de Enanas naranjas

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Estrellas 481-500
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Nombre de la estrella Mass Distance

BD-17 3337
Gliese 421 B, GJ 421 B
K5V - 74.7 ly

BD-17 3336
Gliese 421 A, GJ 421 A
K7V - 74.8 ly

BD+25 84
K5V - 74.8 ly

BD+76 404
K6V - 74.8 ly

HD 17382
GJ 113, Gliese 113, G 36-33, TYC 1789-1155-1, WISEA J024809.38+270405.8, BC Ari, HIP 13081
K2 - 74.9 ly

HD 233719
K6V - 74.9 ly

HD 149192
K4Vk: - 74.9 ly

BD+63 965
K7V - 74.9 ly

HD 53927
K2.5V - 75 ly

HD 14001
K4V - 75 ly

HD 14001 B
K4V - 75 ly

HD 224660
- 75.1 ly

HD 124106
K1V - 75.2 ly

HD 105065
K5V - 75.2 ly

HD 203850
K2.5V - 75.2 ly

HD 97782
- 75.3 ly

BD+81 297
K7V - 75.3 ly

HD 16348
K3.5Vk: - 75.3 ly

HD 20165
K1V - 75.4 ly

HD 101177 B
K2V - 75.6 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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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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