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Lista de Enanas naranjas

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Estrellas 101-120
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Nombre de la estrella Mass Distance

HD 120467
HIC 67487, HIP 67487, SAO 181997, LHS 363, Gliese 529, GJ 529
K6Va 0.73 M☉ 45.9 ly

HD 61606
Gliese 282, Gl 282, HD 61606, HIC 37349, HIP 37349, WDS J07400-0336, 2MASS J07395932-0335506, SAO 134954
K3V - 45.9 ly

HD 61606 B
BD−03° 2002, SAO 134958
K7V - 45.9 ly

HD 110315
HIC 61901, HIP 61901, SAO 100205, Gliese 481, GJ 481, SAO 100205
K4.5V 0.73 M☉ 46 ly

HD 188088
CD−24° 15668, Gliese 770, GJ 770, HIC 97944, HIP 97944, HR 7578, SAO 188692
K3VaCN1 - 46.1 ly

HD 150689
CD-38 11173, HIC 81935, HIP 81935, 2MASS J16441502-3856371, TIC 77929282, TYC 7867-1845-1, 1RXS J164414.8-385645
K3V - 46.4 ly

HD 234078
HIP 67691, SAO 28910, LHS 363, Gliese 532, GJ 532
K7V - 46.5 ly

HD 173818
Gliese 726, GL 726, GJ 726, HIP 92200, TYC-5118-441-1, BD 03 4380, SAO 142621
K5V 0.62 M☉ 46.5 ly

26 Draconis B
K3V 0.83 M☉ 47.1 ly

HD 97584
GJ 420, Gliese 420, G 254-18, BD+74 456, GC 15449, HIP 54952, LTT 13028, NLTT 26722, SAO 7320, TYC 4398-328-1, WISE J111510.98+732832.1
K4V C - 47.2 ly

BD-08 2582
K7V - 47.3 ly

HD 110833
K3 - 47.3 ly

BD+30 2512
Gl 546, Gliese 546, 2MASS J14215724+2937468, SAO 83309, HIP 70218, TYC 2014-591-1, GC 19374, AG+29 1406
K6V - 47.4 ly

111 Tauri B
K4V - 47.4 ly

Gliese 898
HD 221503, HIP 116215, SAO 165756, BD-17° 6769, SAO165756, YPC 5695.00, Vys 864A, GJ 898
K6V - 47.5 ly

HD 120036
HIP 67308, GJ 1177, Gliese 1177, TYC-7270-974-2
K6V - 47.5 ly

HD 120036 B
GJ 1177B
K7V - 47.6 ly

Gliese 269
HD 57095, HIP 35296, LHS 1911, GJ 269
K1 V 0.83 M☉ 47.6 ly

Gliese 269 B
K3V 0.69 M☉ 47.6 ly

OU Geminorum Aa
TYC 1336-16-1, TIC 430173956, WISEA J062610.15+184523.3, OU Gem, BD+18 1214, GJ 233, Gliese 233, HD 45088, HIC 30630, HIP 30630, SAO 95677
K2Ve 0.85 M☉ 47.7 ly
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Enana naranja noticias

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
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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Revised properties of orange dwarf HD 219134 provide new insights into planetary evolution
icon12. 10. 2026
iconEstrellas | Exoplanetas | Enana naranj
Image: Revised properties of orange dwarf HD 219134 provide new insights into planetary evolution
New measurements for the orange dwarf HD 219134 refine its age to 8.92 billion years. Asteroseismic analysis settles past debates on its radius and reveals how the star's radiation history influenced the atmospheres of its companion planets....
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Masses and atmospheric evolution of planets in the young K2-233 system
icon9. 10. 2026
iconEstrellas | Exoplanetas | Enana naranja | Supertierras | Atmósferas planetari
Image: Masses and atmospheric evolution of planets in the young K2-233 system
New study characterizes the three-planet system K2-233. The 400 million year old orange dwarf hosts inner iron-rich planets and an outer planet, K2-233 d, that is actively losing its atmosphere. Over time, K2-233 d will likely become a sub-Neptune or super-Earth....
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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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