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Lista de Enanas blancas

        
    
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Estrellas 1-20
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Nombre de la estrella Mass Distance

Sirius B
DA1.9 1 M☉ 8.6 ly

Procyon B
DQZ D 0.6 M☉ 11.5 ly

Van Maanens star
Van Maanen 2, Gliese 35, GJ 35, vMa2, G 001-027, GCTP 160.00, HIP 3829, LFT 76, LHS 7, LTT 10292, WD 0046+051, Wolf 28
DZ7.5 0.68 M☉ 14.1 ly

Gliese 440
LP 145-141, HIC 57367, HIP 57367, BPM 7108, Ci 20 658, EGGR 82, L 145-141, LAWD 37, LHS 43, LPM 396, LTT 4364, NLTT 28447, PLX 2716, PM 11429-6434, WD 1142-645, TYC 8981-4417-1, GSC 08981-04418, 2MASS J11454297-6450297
DQ6 0.56 M☉ 15.1 ly

40 Eridani B
BD-07° 781, G 160-060, HD 26976, LHS 24, LTT 1908, SAO 131065, omi02 Eri B
DA4 0.57 M☉ 16.3 ly

Stein 2051 B
EGGR 180, LHS 27, NLTT 13375, TYC 3744-2062-1, 2MASS J04311201+5858476, WD 0426+58, WD2 0426+585, WD3 0426+588
DC5 0.68 M☉ 18 ly

Gliese 1221
EGGR 372, G 240-72, LP 44-113, WD 1748+708, LHS 455, NLTT 45565
DQ9P 0.81 M☉ 20.3 ly

Gliese 223.2
GJ 223.2, GJ 9193, HL 4, LHS 32, LP 658-2, NLTT 15811, G 099-044, G 99-44, G 106-12, WD 0552–041, EGGR 45
DZ11.8 0.45 M☉ 21 ly

Gliese 3991 B
D12 0.5 M☉ 24.8 ly

Gliese 1087
G 99-47, V1201 Orionis, V1201 Ori, LHS 212, LTT 17891, NLTT 15834, WD 0553+05, EGGR 290
DA8P 0.71 M☉ 26.5 ly

Gliese 293
Luyten 97-12, LHS 34, LFT 555, LTT 2981, WD 0752-676, EGGR 56, 2MASS J07530814-6747314, LAWD 26
DC8.8 0.59 M☉ 26.6 ly

Gliese 915
LHS 1005, Luyten 362-81, WD 2359-434, LFT 1849, LTT 9857, LP 988-88, EGGR 165, 2MASS J00021076-4309560, LAWD 96, GJ 915, EGGR 165, WISEA J000211.31-431002.6, L 362-81
DAP5.8 0.9 M☉ 27.2 ly

Gliese 518
Wolf 489, WD 1334+039, LHS 46, G 062-053, LFT 1023, LTT 13961, NLTT 34618, G 62-53, G 64-4, EGGR 100, 2MASS J13363181+0340458, USNO-B1.0 0936-00229354
DC9 0.55 M☉ 27.2 ly

TYC 3980-1081-1 B
UCAC4 747-070768, Gaia DR2 2202703050401536000
DAH - 27.6 ly

Gliese 318
CD−32° 5613, LHS 253, L 532-81, LTT 3218, WD 0839-327, CD-32 5613, LFT 600, GJ 318, LAWD 28, PLX 2080.1
DA5.5 0.45 M☉ 27.8 ly

Gliese 1276
LP 701-29, LHS 69, WD 2251-070, EGGR 453, 2MASS J22535314-0646536, NLTT 55164, GJ 1276
DZ13 0.54 M☉ 27.8 ly

Gliese 2012
LHS 1126, G 66-57, WD 0038-226, LFT 65, L 651-57, LP 825-669, LTT 375, NLTT 2258
DQ9 0.52 M☉ 29.7 ly

Gliese 283
LAWD 25, L 745-46, LFT 543, LHS 235, LHS 234, LTT 2915, LP 783-3, LP 7783-2
DZQA6 0.62 M☉ 29.8 ly

Gliese 3306
EGGR 41, CSI-08-04354, LFT 367, LHS 194, L 879-14, LP 655-42, LTT 2049, NLTT 13658, 2MASS J04374739-0849089, WD 0435-088
DQ8 - 30.7 ly

289 G. Hydrae B
WD 1132-325, VB 04, GJ 432 B, 20 Crt B
DC8 0 M☉ 31.2 ly
Estrellas 1-20
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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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