Enanas naranjas | Stellar Catalog

	Mass	Distance
44 Boötis C	K4V	-	42.2 ly
HD 27274 CD−53° 889, GJ 167, Gliese 167, HIC 19884, HIP 19884, SAO 233456	K4.5Vk:	0.74 M☉	42.5 ly
HD 211970 LTT 8985, CD-55 9073, Gliese 1267, GJ 1267, HIC 110443, HIP 110443, 2MASS J22221621-5433383, NLTT 53616, TIC 231704229, TYC 8822-210-1, WISEA J222215.97-543335.6	K7Vk: C	0.61 M☉	42.8 ly
HD 170657 NSV 10944, Gliese 716, GJ 716, HD 170657, HIC 90790, HIP 90790, SAO 161557, WDS J18313-1855A, LTT 7358	K2V	0.79 M☉	43 ly
HD 29697 V834 Tau, V834 Tauri, BD+20° 802, GJ 174, Gliese 174, HD 29697, HIC 21818, HIP 21818, SAO 76708	K4V	0.75 M☉	43.1 ly
HD 128165 HIC 71181, HIP 71181, SAO 29196, Gliese 556, GJ 556, GL 556, TYC-3860-1045-1, BD+53 1719	K3V	0.78 M☉	43.2 ly
HD 214749 LTT 9143, GJ 868.0, Gliese 868.0, PLX 5486, UBV 19400, CD-30 19255, HD 214749, PLX 5486.00, UBV M 26543, CPC 17 12286, HIC 111960, PPM 274115, UGP 576, CPD-30 6663, HIP 111960, SAO 191319, WISEA J224043.67-294028.1, GCRV 73405, IRAS 22379-2955, SKY# 43116, Gaia DR1 6608490497012980224, GEN# +1.00214749, 2MASS J22404335-2940278, TIC 47295522, Gaia DR2 6608490501308343168, GJ 868, Gliese 868, NLTT 54520, TYC 6969-1175-1	K4.5Vk	-	43.3 ly
HD 120476 B	K6V	-	44 ly
BD+62 780	K7V	-	44 ly
HD 120476 Gl 528, Gliese 528, HIC 67422, HIP 67422, LHS 6259, LTT 14035, NLTT 35353, BD+27 2296,	K4V	-	44 ly
HD 10436 BD+63° 229, Gliese 69, GJ 69, HD 10436, HIP 8070, SAO 11943, LHS 1291	K5Vbe	0.62 M☉	44.1 ly
HD 145417 GJ 615, Gliese 615, LHS 413, HIC 79537, HIP 79537, LFT 1255, LTT 6464, NLTT 42227, 2MASS J16134869-5734118, TIC 207556694, TYC 8719-359-1, WISEA J161347.46-573428.1	K3VFe-1.7	-	44.3 ly
HD 22496 CD−48° 1011, GJ 146, Gliese 146, HIC 16711, HIP 16711, LTT 1698, SAO 85397, 2MASS J03350093-4825089	K5/M0V	0.68 M☉	44.4 ly
HD 98712 BD-19 3242, HIC 55454, HIP 55454, PM J11214-2027, TYC 6090-1868-1, WISE J112126.79-202714.3, SZ Crateris, SZ Crt, GJ 425, GJ 425A, Gliese 425, SAO 179801	K7V	-	44.8 ly
HD 154577 CD-60 6576, GCTP, Gliese 656, GJ 656, HD 154577, HIC 83990, HIP 83990, LHS 3268, LTT 6833, SAO 253819	K2.5Vk:	0.68 M☉	44.8 ly
V439 Andromedae BD+28°4704, GC 95, GSC 01735-02532, GSC 01735-00927, GJ 5, Gliese 5, HD 166, HIP 544, HR 8, SAO 73743, NSV 33	K0Ve	0.89 M☉	44.9 ly
BD+39 2376 NS 1045+3830, Gliese 400, GJ 400, HIP 52600, BD+39 2376, CCDM J10454+3831AB	K7/M0V	-	45.2 ly
HD 281621 LHS 1634, HIC 19337, HIP 19337, GL 162, Gliese 162, TYC-2362-37-1	K7V	-	45.4 ly
HD 23356 HIP 17420, BD -19 733, N1 354, LTT1759, NS 0343-1906	K2V	-	45.5 ly
HD 5133 BD−31° 325, Gaia DR2 5031808453624044800, Gliese 42, GJ 42, HD 5133, HIC 4148, HIP 4148, SAO 192793, LTT 498, 2MASS J00530108-3021249	K2.5Vk:	-	45.5 ly

Nombre de la estrella

Mass

Distance

44 Boötis C

K4V

42.2 ly

HD 27274

CD−53° 889, GJ 167, Gliese 167, HIC 19884, HIP 19884, SAO 233456

K4.5Vk:

0.74 M☉

42.5 ly

HD 211970

LTT 8985, CD-55 9073, Gliese 1267, GJ 1267, HIC 110443, HIP 110443, 2MASS J22221621-5433383, NLTT 53616, TIC 231704229, TYC 8822-210-1, WISEA J222215.97-543335.6

K7Vk: C

0.61 M☉

42.8 ly

HD 170657

NSV 10944, Gliese 716, GJ 716, HD 170657, HIC 90790, HIP 90790, SAO 161557, WDS J18313-1855A, LTT 7358

K2V

0.79 M☉

43 ly

HD 29697

V834 Tau, V834 Tauri, BD+20° 802, GJ 174, Gliese 174, HD 29697, HIC 21818, HIP 21818, SAO 76708

K4V

0.75 M☉

43.1 ly

HD 128165

HIC 71181, HIP 71181, SAO 29196, Gliese 556, GJ 556, GL 556, TYC-3860-1045-1, BD+53 1719

K3V

0.78 M☉

43.2 ly

HD 214749

LTT 9143, GJ 868.0, Gliese 868.0, PLX 5486, UBV 19400, CD-30 19255, HD 214749, PLX 5486.00, UBV M 26543, CPC 17 12286, HIC 111960, PPM 274115, UGP 576, CPD-30 6663, HIP 111960, SAO 191319, WISEA J224043.67-294028.1, GCRV 73405, IRAS 22379-2955, SKY# 43116, Gaia DR1 6608490497012980224, GEN# +1.00214749, 2MASS J22404335-2940278, TIC 47295522, Gaia DR2 6608490501308343168, GJ 868, Gliese 868, NLTT 54520, TYC 6969-1175-1

K4.5Vk

43.3 ly

HD 120476 B

K6V

44 ly

BD+62 780

K7V

44 ly

HD 120476

Gl 528, Gliese 528, HIC 67422, HIP 67422, LHS 6259, LTT 14035, NLTT 35353, BD+27 2296,

K4V

44 ly

HD 10436

BD+63° 229, Gliese 69, GJ 69, HD 10436, HIP 8070, SAO 11943, LHS 1291

K5Vbe

0.62 M☉

44.1 ly

HD 145417

GJ 615, Gliese 615, LHS 413, HIC 79537, HIP 79537, LFT 1255, LTT 6464, NLTT 42227, 2MASS J16134869-5734118, TIC 207556694, TYC 8719-359-1, WISEA J161347.46-573428.1

K3VFe-1.7

44.3 ly

HD 22496

CD−48° 1011, GJ 146, Gliese 146, HIC 16711, HIP 16711, LTT 1698, SAO 85397, 2MASS J03350093-4825089

K5/M0V

0.68 M☉

44.4 ly

HD 98712

BD-19 3242, HIC 55454, HIP 55454, PM J11214-2027, TYC 6090-1868-1, WISE J112126.79-202714.3, SZ Crateris, SZ Crt, GJ 425, GJ 425A, Gliese 425, SAO 179801

K7V

44.8 ly

HD 154577

CD-60 6576, GCTP, Gliese 656, GJ 656, HD 154577, HIC 83990, HIP 83990, LHS 3268, LTT 6833, SAO 253819

K2.5Vk:

0.68 M☉

44.8 ly

V439 Andromedae

BD+28°4704, GC 95, GSC 01735-02532, GSC 01735-00927, GJ 5, Gliese 5, HD 166, HIP 544, HR 8, SAO 73743, NSV 33

K0Ve

0.89 M☉

44.9 ly

BD+39 2376

NS 1045+3830, Gliese 400, GJ 400, HIP 52600, BD+39 2376, CCDM J10454+3831AB

K7/M0V

45.2 ly

HD 281621

LHS 1634, HIC 19337, HIP 19337, GL 162, Gliese 162, TYC-2362-37-1

K7V

45.4 ly

HD 23356

HIP 17420, BD -19 733, N1 354, LTT1759, NS 0343-1906

K2V

45.5 ly

HD 5133

BD−31° 325, Gaia DR2 5031808453624044800, Gliese 42, GJ 42, HD 5133, HIC 4148, HIP 4148, SAO 192793, LTT 498, 2MASS J00530108-3021249

K2.5Vk:

45.5 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 yesterday
	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 15. 10. 2026
	TOI-2257 189 ly			The Limits of Tidal Circularization and Atmospheric Escape for Mini-Neptunes and Super-Earths: The Case of TOI-2257 b 15. 10. 2026
	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