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Lista de Enanas naranjas

        
    
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Estrellas 21-40
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Nombre de la estrella Mass Distance

Gliese 667
142 G. Scorpii, CD−34°11626, HD 156384, HIP 84709, HR 6426, LHS 442/442/443, SAO 208670, GJ 667
K3V 0.73 M☉ 23.6 ly

Gliese 667 B
K5V 0.69 M☉ 23.6 ly

96 G. Piscium
Gliese 33, HD 4628, LHS 121, Wolf 25, HR 222, BD+04 123, HIP 3765, HR 222, Lal 1299, LHS 121, LTT 10285, SAO 109471
K1.5Ve 0.76 M☉ 24.3 ly

Fomalhaut B
TW Piscis Austrini, TW PsA, Gl 879, HR 8721, CD -32°17321, HD 216803, LTT 9283, GCTP 5562.00, SAO 214197, CP(D)-32 6550, HIP 113283
K5Vp 0.73 M☉ 24.8 ly

107 Piscium
BD+19° 279, CCDM J01425+2016A, GC 2080, Gliese 68, HD 10476, HIP 7981, HR 493, IDS 01371+1947 A, LFT 153, LHS 1287, LTT 10596, NLTT 5685, PPM 91014, SAO 74883, WDS 01425+2016A
K1V 0.89 M☉ 24.9 ly

Gliese 673
Wolf 718, LHS 447, BD +02°3312, HD 157881, LTT 15175, GCTP 3955.00, SAO 122374, Vys 794, HIP 85295
K7 V 0.65 M☉ 25.2 ly

Chi Draconis B
K0 V 0.75 M☉ 26.3 ly

p Eridani
6 Eri, Gliese 66, GJ 66, CD−56°328, GCTP 352.00, SAO 232490, WDS 01398-5612, DUN 5, HIP 7751, HIC 7751, HR 486, HD 10360, LTT 903, * p Eri A
K2 V 0.88 M☉ 26.7 ly

p Eridani B
HR 487, HD 10361, LTT 902, p Eri B
K2 V 0.86 M☉ 26.7 ly

Gliese 884
HD 217357, LHS 3885, HIP 113576, HIC 113576, LAL 44964, LFT 1754, LTT 9308, NLTT 55523, MCC 339, 2MASS J23001607-2231276, CD-23 17699
K7 V 0.63 M☉ 26.9 ly

Gliese 185
BD−21° 1051, HD 32450, HIP 23455, SAO 170003, LTT 2151, MCC 112
K7 V 0.59 M☉ 27.3 ly

Gliese 250
88 G. Monocerotis, BD -05°1844, GCTP 1606.00, HD 50281, HIP 32984, LFT 494, LHS 1875, LTT 2662, SAO 133805
K3.5 V 0.8 M☉ 28.5 ly

5 G. Capricorni
HD 192310, CD-27° 14659, GCTP 4804.00, Gliese 785, HIP 99825, LHS 488, LTT 8009, NSV 12933, SAO 189065, HR 7722
K2 V 0.78 M☉ 28.7 ly

284 G. Eridani
Gliese 183, BD -05°1123, HD 32147, LHS 200, LTT 2142, GCTP 1129.00, SAO 131688, LPM 200, HIP 23311
K3 V 0.84 M☉ 28.8 ly

AK Leporis
BD−22 1210, Gliese 216 B, HD 38392, HR 1982, LTT 2363, SAO 170757, V* AK Lep
K2 V 0.82 M☉ 29 ly

Argelanders Star
BD+38 2285, FK5 1307, GCTP 2745.00, GJ 451, HIP 57939, HR 4550, HD 103095, LHS 44, LTT 13276, SAO 62738, 1830 Groombridge, Gliese 451
K1 V 0.66 M☉ 29.9 ly

289 G. Hydrae
CD−32°8179, Gliese 432, GJ 432, HD 100623, HIP 56452, HR 4458, SAO 202583, LHS 308, LTT 4280, 20 Crt
K0 V 0.87 M☉ 31.2 ly

Gliese 638
HD 151288, BD +33°2777, LTT 14967, NLTT 43504, SAO 65525, NSV 7951, HIC 82003, HIP 82003, G 181-6, 2MASS J16450635+3330330
K7.5 Ve 0 M☉ 32.1 ly

12 Ophiuchi
12 Oph, BD-01 3220, FK5 1433, GCTP 3773.00, Gliese 631, HD 149661, HIP 81300, HR 6171, LHS 3224, LTT 6632, V2133 Oph, SAO 141269
K1 V 0.91 M☉ 32.3 ly

Gliese 75
V987 Cassiopeiae, BD+63°238, HD 10780, HIP 8362, HR 511, LHS 1297, LTT 10619, SAO 11983
K0 V 0.83 M☉ 32.7 ly
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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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