Enanas naranjas | Stellar Catalog

	Mass	Distance
Delta Capricorni B	K/G	0.73 M☉	38 ly
HD 99279 B GJ 428 B, Gliese 428 B, TYC 8959-1969-1, TIC 315311765, 2MASS J11243947-6138542	K7	0.62 M☉	38.1 ly
Zeta Doradus B GJ 1075, Gliese 1075, HIC 23708, HIP 23708		0.53 M☉	38.1 ly
Gliese 572 B BD+45 2247B	K7V	-	38.2 ly
Gliese 414 HD 97101, GJ 414 A, LHS 2367, DO 14370, G 119-60, G 120-23, G 147-28, HIC 54646, HIP 54646, LFT 767, LTT 13009, NLTT 26534, 2MASS J11110509+3026459, TIC 9001920, TYC 2520-2524-1, WDS J11111+3027A, WISEA J111105.67+302643.6	K7V	0.65 M☉	38.7 ly
HD 99279 DENIS J112440.3-613851, GJ 428, Gliese 428, 2MASS J11244030-6138512, TIC 315311759, TYC 8959-1969-2, WISEA J112439.38-613851.3	K5-V	0.79 M☉	39.5 ly
HD 72673 11 G. Pyxidis, CD−31° 6229, GJ 309, Gliese 309, HD 72673, HIP 41926, HIC 41926, HR 3384, SAO 199352, LHS 249, LTT 3168	K1V	0.75 M☉	39.7 ly
V538 Aurigae V538 Aur, NSV 16618, BD+53° 934, GJ 211, Gliese 211, HD 37394, HIC 26779, HIP 26779, HR 1925, WDS J05413+5329A	K1	0.87 M☉	40 ly
85 Pegasi B ADS 17175 B, GJ 914 B, BD +26°4734 B, BU 733 B		0.55 M☉	40.2 ly
HD 196877	K7V	-	40.3 ly
HD 175224 B	K7Ve	-	40.3 ly
HD 175224 HIC 93069, HIP 93069, IRAS 18532-5603, TIC 379470817, WDS J18575-5600AB, WISEA J185730.57-555934.2	K5Ve	-	40.3 ly
HD 21531	K5V	-	40.7 ly
HD 190007 V1654 Aql, V1654 Aquilae, BD+02° 4076, GJ 775, Gliese 775, HD 190007, HIC 98698, HIP 98698, SAO 125379, GC 27782, 2MASS J20024703+0319344, SAO 125379, TIC 345217789, TYC 498-2720-1, USNO-B1.0 0933-00588224, WISE J200246.98+031935.5	K5V B	0.68 M☉	41.5 ly
HD 101581 LHS 2441, CD-43 7228, GJ 435, Gliese 435, HIC 56998, HIP 56998, LFT 835, LTT 4333, 2MASS J11410247-4424184, NLTT 28235, TIC 397362481, TYC 7753-1657-1, WISEA J114101.82-442416.0	K4.5Vk:	0.74 M☉	41.7 ly
HD 82106 TYC 234-468-1, HIC 46580, HIP 46580, Gliese 349, GJ 349	K3V	0.79 M☉	41.7 ly
HD 158633 BD+67°1014, Gliese 675, GJ 675, HD 158633, HIC 85235, HIP 85235, HR 6518, SAO 17474, LHS 287, LTT 15185	K0V	0.73 M☉	41.7 ly
36 Ursae Majoris B * 36 UMb	K7Ve	-	42.1 ly
Gliese 204 GJ 204, HD 36003, BD-03 1110, 2MASS J0528-0329, 2MASS J05282613-0329576, SAO 132145, HIC 25623, HIP 25623, TYC 4757-1577-1, GC 6757, LFT 412, LHS 1763	K5V	0.75 M☉	42.2 ly
HD 40307 CD−60 1303, CPD−60 508, GC 7474, Gliese 2046, GJ 2046, HIC 27887, HIP 27887, PPM 355061, SAO 249388, 2MASS J05540421-6001245, TIC 374859347, TYC 8892-1247-1	K2.5V C	0.75 M☉	42.2 ly

Nombre de la estrella

Mass

Distance

Delta Capricorni B

K/G

0.73 M☉

38 ly

HD 99279 B

GJ 428 B, Gliese 428 B, TYC 8959-1969-1, TIC 315311765, 2MASS J11243947-6138542

0.62 M☉

38.1 ly

Zeta Doradus B

GJ 1075, Gliese 1075, HIC 23708, HIP 23708

0.53 M☉

38.1 ly

Gliese 572 B

BD+45 2247B

K7V

38.2 ly

Gliese 414

HD 97101, GJ 414 A, LHS 2367, DO 14370, G 119-60, G 120-23, G 147-28, HIC 54646, HIP 54646, LFT 767, LTT 13009, NLTT 26534, 2MASS J11110509+3026459, TIC 9001920, TYC 2520-2524-1, WDS J11111+3027A, WISEA J111105.67+302643.6

K7V

0.65 M☉

38.7 ly

HD 99279

DENIS J112440.3-613851, GJ 428, Gliese 428, 2MASS J11244030-6138512, TIC 315311759, TYC 8959-1969-2, WISEA J112439.38-613851.3

K5-V

0.79 M☉

39.5 ly

HD 72673

11 G. Pyxidis, CD−31° 6229, GJ 309, Gliese 309, HD 72673, HIP 41926, HIC 41926, HR 3384, SAO 199352, LHS 249, LTT 3168

K1V

0.75 M☉

39.7 ly

V538 Aurigae

V538 Aur, NSV 16618, BD+53° 934, GJ 211, Gliese 211, HD 37394, HIC 26779, HIP 26779, HR 1925, WDS J05413+5329A

0.87 M☉

40 ly

85 Pegasi B

ADS 17175 B, GJ 914 B, BD +26°4734 B, BU 733 B

0.55 M☉

40.2 ly

HD 196877

K7V

40.3 ly

HD 175224 B

K7Ve

40.3 ly

HD 175224

HIC 93069, HIP 93069, IRAS 18532-5603, TIC 379470817, WDS J18575-5600AB, WISEA J185730.57-555934.2

K5Ve

40.3 ly

HD 21531

K5V

40.7 ly

HD 190007

V1654 Aql, V1654 Aquilae, BD+02° 4076, GJ 775, Gliese 775, HD 190007, HIC 98698, HIP 98698, SAO 125379, GC 27782, 2MASS J20024703+0319344, SAO 125379, TIC 345217789, TYC 498-2720-1, USNO-B1.0 0933-00588224, WISE J200246.98+031935.5

K5V B

0.68 M☉

41.5 ly

HD 101581

LHS 2441, CD-43 7228, GJ 435, Gliese 435, HIC 56998, HIP 56998, LFT 835, LTT 4333, 2MASS J11410247-4424184, NLTT 28235, TIC 397362481, TYC 7753-1657-1, WISEA J114101.82-442416.0

K4.5Vk:

0.74 M☉

41.7 ly

HD 82106

TYC 234-468-1, HIC 46580, HIP 46580, Gliese 349, GJ 349

K3V

0.79 M☉

41.7 ly

HD 158633

BD+67°1014, Gliese 675, GJ 675, HD 158633, HIC 85235, HIP 85235, HR 6518, SAO 17474, LHS 287, LTT 15185

K0V

0.73 M☉

41.7 ly

36 Ursae Majoris B

* 36 UMb

K7Ve

42.1 ly

Gliese 204

GJ 204, HD 36003, BD-03 1110, 2MASS J0528-0329, 2MASS J05282613-0329576, SAO 132145, HIC 25623, HIP 25623, TYC 4757-1577-1, GC 6757, LFT 412, LHS 1763

K5V

0.75 M☉

42.2 ly

HD 40307

CD−60 1303, CPD−60 508, GC 7474, Gliese 2046, GJ 2046, HIC 27887, HIP 27887, PPM 355061, SAO 249388, 2MASS J05540421-6001245, TIC 374859347, TYC 8892-1247-1

K2.5V C

0.75 M☉

42.2 ly

Enana naranja noticias

Massive brown dwarf HD 203771 b confirmed in eccentric orbit around orange dwarf

14. 10. 2026

Estrellas | 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

12. 10. 2026

Estrellas | 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

9. 10. 2026

Estrellas | 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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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.

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

	WASP 94 687 ly			A New Method for Constraining 3D Exoplanet Atmospheres: Application to WASP-94A b's Panchromatic Spectrum today
	KELT-2 439 ly			Emission spectroscopy of KELT-2A b with Gemini-North/IGRINS-2: hints of a stellar C/O ratio and sub-stellar metallicity yesterday
	TOI-2257 189 ly			The Limits of Tidal Circularization and Atmospheric Escape for Mini-Neptunes and Super-Earths: The Case of TOI-2257 b yesterday
	KELT-18 1032 ly			High-resolution transmission spectroscopy of KELT-18b Metastable helium detection at 1083 nm 14. 10. 2026
	WASP 17 1315 ly			A Spatial Map of the Atmospheric Limb of a Hot Jupiter 14. 10. 2026

Lista de Enanas naranjas

Enana naranja noticias

Research in Enanas naranjas

Frequently Asked Questions about nearby stars

What is the nearest star?

What are the nearest stars to Earth?

What is the solar neighborhood?

How do astronomers measure distances to stars?

Are there any exoplanets orbiting the nearest stars?

Why are the nearest stars important for astronomy and physics?

StellarGuide: Estrellas