Lista de Enanas blancas

Más sobre Enanas blancas

	Mass	Distance
HD 283750 B	DC8	-	56.8 ly
LP 464-57	DC	-	56.9 ly
EC 20173-3036 WD 2017-306		-	56.9 ly
ZZ Piscium V* ZZ Psc, EGGR 159, GJ 895.2, Gliese 895.2, LHS 5405, LTT 16907, NLTT 56992, WD 2326+049, G 29-38	DAV4.1	0.7 M☉	57.2 ly
EGGR 261	DA3.4	-	57.4 ly
LP 37-186	DC9	-	57.5 ly
SCR J0753-2524	DA10	-	58.1 ly
EGGR 155	DA4.7	-	58.2 ly
EGGR 494 Gaia EDR3 4388138816124225792	DZ7	-	58.2 ly
UCAC4 325-215293		-	58.6 ly
B Carinae B		0.42 M☉	58.9 ly
WT 1759	DZ7	-	59 ly
EGGR 484 WD 0644+025	DA7.0	0.95 M☉	59 ly
EGGR 427	DC9	-	59.2 ly
UCAC4 482-095741 Gaia EDR3 4293873732939569920	DA	-	59.2 ly
PHL 1716	DA	-	59.2 ly
WD J2214-390 [OHD2001] WD J2214-390	DA8	-	59.2 ly
EGGR 426	DC9	-	59.4 ly
LP 606-32	DC	-	59.5 ly
PY Vulpeculae V* PY Vul, EGGR 277, LSPM J1937+2743, USNO-B1.0 1177-00513805, WD 1935+276, USNO 352, WD 1935+27, NLTT 48026, GJ 1241, Gliese 1241, PG 1935+276, G 185-32	DA4.0	0.64 M☉	59.6 ly

Enanas blancas noticias

Evaporating planet explains gaseous disk formation around white dwarf WD J0914+1914

9. 8. 2026

Estrellas | Exoplanetas | Enanas b

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

1. 8. 2026

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

5. 7. 2026

Estrellas | Exoplanetas | Atmósferas planetarias | Enanas b

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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Research in Enanas blancas

Explore los últimos estudios científicos sobre estrellas y exoplanetas en nuestra galaxia. Descubra las últimas investigaciones sobre astrofísica y astronomía estelar.

La investigación actual

	WD J0914+1914 1393 ly			Planetary atmospheric escape and disk formation around WDJ0914+1914 9. 8. 2026
	TOI-5628 360 ly			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			Aerosols and hydrocarbons in the atmosphere of a white dwarf planet 5. 7. 2026
	RS Ophiuchi 7381 ly			Near-infrared spectroscopy of RS Ophiuchi in 2021: the calm, the storm, and the abatement 8. 3. 2026
	Omicron Ceti 299 ly			Is Mira B a low mass white dwarf? 1. 3. 2026

Publicaciones más antiguas

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.

StellarGuide: Estrellas

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.

More about Estrellas

Random terms

Posición de la estrella Luminosidad Temperatura de la estrella Masa estelar Tamaño de la estrella Edad de las estrellas