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Liste des Naines blanches
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Etoile 21-40
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Nom de l étoile Mass Distance

L 88-59
GJ 3112, Gliese 3112, EC 01416-6733, GCRV 26186, LFT 158, LHS 145, LTT 934, 2MASS J01430103-6718293, NLTT 5777, TIC 24705587, WD 0141-675, WD0141-675
 DAZ8.1 0.58 M☉ 31.7 ly

Gliese 339.1
EGGR 250, EGGR 250, G 195-19, LHS 262, NLTT 21302, SDSS J091555.98+532522.8, TIC 251080865, WD 0912+536, 2MASS J09155623+5325249, WISEA J091554.79+532512.0
 DCP7 - 33.5 ly

CPD-69 177
WD 0310-688
 DA3.0 0.66 M☉ 33.9 ly

LP 852-7
WD 1202-232, 2MASS J12052666-2333125, NLTT 29555, TIC 398243520
 DA5.7 - 34 ly

Gliese 754.1
LAWD 74, GJ 754.1 A, LDS 678A, EGGR 131, LTT 7658, UBV 16351, Zkh 291, GJ 9653, 2MASS J19203492-0739597, HIC 95071, HIP 95071, L 923-21, LP 692-16, NLTT 47693, TIC 3567346, TYC 5709-698-1, WD 1917-07
 DBQA5 - 34.3 ly

SCR J0821-6703
WD 0821-669, 2MASS J08212670-6703201, SCR J0821-6703, TIC 307363368, WD 0820-668, WISEA J082125.99-670313.0
 DA10.0 - 34.8 ly

Gliese 86 B
GJ 86 B, HD 13445B, WDS J02104-5049B, WD 0208-510
 DQ6 0.49 M☉ 35.2 ly

Gliese 3182
GJ 3182, EGGR 473, G 174-14, LHS 1446, 2MASS J02483643+5423225, NLTT 8988, TIC 470881332, WD 0245+54, WISEA J024835.91+542318.5
 DAZ9 - 35.4 ly

EGGR 381
GJ 1004, Gliese 1004, G 217-37, LHS 1038, NLTT 574, 2MASS J00121479+5025213, TIC 201892746, WISEA J001214.23+502514.7, WD 0009+501
 DA7.6 - 35.5 ly

DN Draconis
V* DN Dra, GJ 1206, Gliese 1206, G 226-29, HIC 82257, HIP 82257, LP 101-148, 2MASS J16482562+5903228, NLTT 43637, TIC 199666369, TYC 3885-860-1, WD 1647+591, WISE J164825.81+590319.6
 DA4.0 - 35.7 ly

EGGR 148
GJ 836.5, Gliese 836.5, G 145-63, G 126-27, LFT 1655, LHS 3703, L 1363-3, LP 458-64, LTT 16348, NLTT 51906, 2MASS J21424099+2059582, SDSS J214240.92+205954.9, TIC 354568302, WD 2140+207, WISEA J214240.83+205951.2
 DQ6 - 36 ly

UPM J0812-3529
WD 0810-353, TIC 145863747, 2MASS J08122707-3529433
 DAH 0.63 M☉ 36.4 ly

EGGR 248
GJ 1086, Gliese 1086, G 106-4, G 99-37, LTT 17876, NLTT 15714, 2MASS J05511947-0010213, SDSS J055119.47-001021.4, TIC 176670072, WD 0548-001
 DQ8P - 36.6 ly

LAWD 79
GJ 772, Gliese 772, G 92-40, LFT 1503, LHS 3501, L 997-21, LP 634-1, LTT 7879, NLTT 48454, 2MASS J19562925-0102317, SDSS J195629.08-010236.0, TIC 251903434, WD 1953-011
 DA6.4 - 37.7 ly

EGGR 438
 DC9 - 38.7 ly

EGGR 375
GJ 1234, Gliese 1234, G 208-17, G 125-3, NLTT 47677, WISEA J191858.64+384318.8, SDSS J191858.65+384319.9, MASS J19185863+3843214, WD 1917+386
 DC7 C - 38.7 ly

EGGR 52 B
 DA - 39.1 ly

EGGR 52
LHS 230, WD0727+482, G 111-8, G 193-51, G 107-70, GJ 275.2, Gliese 275.2, LSPM J0730+4810, NLTT 17953, TIC 328328649, WISEA J073047.07+481013.1
 DA+DA - 39.1 ly

LAWD 34
 DA5n - 40 ly

LAWD 10
 DA+D1 - 41.2 ly
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Naines blanches nouvelles

Evaporating planet explains gaseous disk formation around white dwarf WD J0914+1914
icon9. 8. 2026
iconÉtoiles | Exoplanètes | Naines blanche
Image: Evaporating planet explains gaseous disk formation around white dwarf WD J0914+1914
The white dwarf WD J0914+1914 is surrounded by a ring of gas containing hydrogen, oxygen, and sulfur. This material originates from a nearby Neptune-like or super-puff planet—a planet with a very low density—that is losing its atmosphere due to intense radiation from the star. The escaping gas forms a disk around the star, which is then slowly pulled onto the white dwarf's surface, creating the unique light signals observed by instruments. Advanced simulations were used to model the atmos...
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Wide-orbit stellar companions influence formation of giant planets around Red dwarf stars
icon1. 8. 2026
iconÉtoiles | Exoplanètes | TESS | Naines rouges | Formation des planètes | Naines blanche
Image: Wide-orbit stellar companions influence formation of giant planets around Red dwarf stars
The giant planet TOI-5628Ab orbits a Red dwarf star every 4.34 days. Observations reveal that Red dwarfs with close-in giant planets are 6 times more likely to have a distant stellar companion, suggesting these neighbors influence planetary migration....
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Atmosphere of planet WD 1856 b contains hydrocarbons and aerosols
icon5. 7. 2026
iconÉtoiles | Exoplanètes | Atmosphères planétaires | Naines blanche
Image: Atmosphere of planet WD 1856 b contains hydrocarbons and aerosols
The atmosphere of planet WD 1856 b, orbiting a white dwarf star, contains hydrocarbons and aerosols. Data from the James Webb Space Telescope reveal the planet is significantly warmer than expected, pointing to a past reheating event during its orbital migration....
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study iconResearch in Naines blanches

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Parcourez les dernières études scientifiques sur les étoiles et les exoplanètes de notre galaxie. Découvrez les dernières recherches en astrophysique et en astronomie stellaire.
Les recherches en cours

 WD J0914+1914
1393 ly
 study icon Planetary atmospheric escape and disk formation around WDJ0914+1914
9. 8. 2026

TOI-5628
360 ly
 study icon Stellar Multiplicity of M Dwarfs with Short-period Giant Planets, and the Characterization of TOI-5628Ab
1. 8. 2026

WD 1856+534
80.7 ly
 study icon Aerosols and hydrocarbons in the atmosphere of a white dwarf planet
5. 7. 2026

RS Ophiuchi
7381 ly
 study icon Near-infrared spectroscopy of RS Ophiuchi in 2021: the calm, the storm, and the abatement
8. 3. 2026

Omicron Ceti
299 ly
 study icon Is Mira B a low mass white dwarf?
1. 3. 2026
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Publications plus anciennes

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: Étoiles

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Étoiles
Les étoiles sont d’immenses sphères de gaz chaud qui brillent en produisant de l’énergie grâce à la fusion nucléaire dans leur noyau. La plupart des étoiles sont composées principalement d’hydrogène et d’hélium. Au centre d’une étoile, la pression et la température élevées provoquent la fusion des atomes d’hydrogène en hélium, libérant ainsi une énorme quantité d’énergie sous forme de lumière et de chaleur.
More about Étoiles tag icon
Random terms
Position de la étoileLuminositéTempérature des étoilesMasse stellaireTaille de l´étoileL´âge des étoiles

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