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Lista de Enanas naranjas

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Estrellas 241-260
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Nombre de la estrella Mass Distance

Rho Geminorum C
ρ Gem C, HIP 36357, BD+32° 1561, Gliese 273.1, V376 Gem
K2.5V 0.77 M☉ 59.1 ly

HD 117936
K3V - 59.2 ly

83 Leonis B
HD 99492, BD+03° 2502
K3 D 0.83 M☉ 59.2 ly

HD 31560
K3.5Vk: - 59.5 ly

BD+13 3578
LHS 3373, G 183-34, G 140-49, GJ 708.2, GJ 9620, Gliese 9620, HIC 89517, HIP 89517, LFT 1403, L 1208-59, LTT 15405, 2MASS J18160224+1354480, MCC 179, NLTT 46192, TIC 406883293, TYC 1022-646-1, WISEA J181602.32+135442.9
K7V - 59.6 ly

BD-13 3333
K7V - 59.6 ly

HD 154088
CD−28° 12769, Gliese 652, GJ 652, HIC 83541, HIP 83541, SAO 184990, LTT 6818, NLTT 44097, GC 23012, JP11 5106, 2MASS J17042783-2834572, TIC 20856917, TYC 6823-1187-1, WISEA J170427.91-283500.3
K0IV-V C 0.97 M☉ 59.6 ly

LQ Hydrae
V* LQ Hya
K1Vp - 59.6 ly

HD 87883
BD+34°2089, HIC 49699, HIP 49699, SAO 61890, PPM 75021, 2MASS J10084315+3414322, TIC 407591082, TYC 2506-894-1
K0V E 0.82 M☉ 59.7 ly

212 G. Puppis B
K3V - 59.8 ly

HD 97503
K5V - 59.8 ly

HD 158233
K5V - 60 ly

HD 73667
K2V - 60.1 ly

Epsilon Reticuli
* eps Ret, GEN# +1.00027442, IRAS 04156-5925, TIC 198079199, ** JSP 56A, GJ 167.3, Gliese 167.3, JP11 882, TYC 8508-2041-1, AKARI-IRC-V1 J0416290-591809, Gliese 9153, GJ 9153, 2MASS J04162902-5918078, UBV 4189, CCDM J04165-5918A, GSC 08508-02041, PLX 958, UBV M 10085, CPC 20 1085, HD 27442A, PLX 958.00, uvby98 100027442, CPD-59 324, HD 27442, PPM 333351, WDS J04165-5918A, CSI-59 324 41, HIC 19921, SAO 233463, WEB 3804, FAUST 538, HIP 19921, SKY# 6536, [BBW2000] FD 58, GC 5194, HR 1355, SPOCS 209, Gaia DR2 4678664766394767616, GCRV 2468, IDS 04148-5932 A, TD1 3044
K2III C 1.5 M☉ 60.1 ly

HD 77175 B
K5 - 60.2 ly

HD 65486
K4-V(k) - 60.2 ly

HD 77175
K5V - 60.2 ly

HD 192961
LTT 8046, DENIS J201936.8-462540, GJ 787, Gliese 787, HIC 100223, HIP 100223, 2MASS J20193694-4625410, NLTT 49035, TIC 129480666, TYC 8405-1805-1, CD-46 13498, Sm 51
K5.5V - 60.3 ly

HD 25329
LHS 21, GJ 158, Gliese 158, HIC 18915, HIP 18915, LFT 326, LSPM J0403+3516, LTT 11321, NLTT 12401, 2MASS J04031512+3516226, TIC 467677978, TYC 2366-3215-1, WISEA J040316.43+351609.9, Gaia DR2 219057458247921536
K1VbFe-2 - 60.4 ly

HD 40887 C
HD 40887C
K5V - 60.4 ly
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Enana naranja noticias

Oscillation patterns in Gliese 570 A and Gliese 783 A reveal new stellar physics
icon18. 10. 2026
iconEstrellas | Enana naranj
Image: Oscillation patterns in Gliese 570 A and Gliese 783 A reveal new stellar physics
Stars like the Sun generate oscillations, or rhythmic vibrations on their surface, caused by the turbulent motion of boiling gas in their outer layers. While these vibrations are easy to measure in Sun-like stars, they are much harder to detect in orange dwarfs because the signals are very faint. To overcome this, high-precision tools can now measure tiny shifts in a star's light caused by these movements, a technique known as Doppler asteroseismology. This approach allows for a direct look at t...
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Massive brown dwarf HD 203771 b confirmed in eccentric orbit around orange dwarf
icon14. 10. 2026
iconEstrellas | Exoplanetas | Enana naranja | Enanas marrone
Image: Massive brown dwarf HD 203771 b confirmed in eccentric orbit around orange dwarf
Massive brown dwarf HD 203771 b confirmed in an eccentric orbit around an orange dwarf star. New mass measurements place the companion at approximately 70 times the mass of Jupiter, revealing insights into how brown dwarfs migrate inward over time....
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Revised properties of orange dwarf HD 219134 provide new insights into planetary evolution
icon12. 10. 2026
iconEstrellas | 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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study iconResearch in Enanas naranjas

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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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