HD 27274

Star in the constellation Dorado From Wikipedia, the free encyclopedia

HD 27274, also known as Gliese 167, is a solitary,[11] orange hued star located in the southern constellation Dorado. It has an apparent magnitude of 7.63,[3] making it readily visible in binoculars, but not to the naked eye. Based on parallax measurements from the Gaia spacecraft, the star is known to be located 42.5 light-years (13.02 parsecs) away from the Solar System[2] However, it is drifting closer with a heliocentric radial velocity of −23 km/s. At its current distance, HD 27274 is dimmed down by 0.05 magnitudes due to interstellar dust.[12]

Right ascension04h 15m 56.90154s[2]
Declination−53° 18 35.3067[2]
Quick facts Constellation, Right ascension ...
HD 27274
Observation data
Epoch J2000.0      Equinox ICRS
Constellation Dorado[1]
Right ascension 04h 15m 56.90154s[2]
Declination −53° 18 35.3067[2]
Apparent magnitude (V) 7.63[3]
Characteristics
Evolutionary stage main sequence[2]
Spectral type K4.5 Vk:[4]
U−B color index +1.08[3]
B−V color index +1.12[3]
Astrometry
Radial velocity (Rv)−23.4±0.3[5] km/s
Proper motion (μ) RA: +784.529 mas/yr[2]
Dec.: +396.695 mas/yr[2]
Parallax (π)76.6638±0.0146 mas[2]
Distance42.544 ± 0.008 ly
(13.044 ± 0.002 pc)
Absolute magnitude (MV)+7.06[1]
Details
Mass0.73±0.09[6] M
Radius0.70±0.05[6] R
Luminosity19.6±0.5%[2] L
Surface gravity (log g)4.64[7] cgs
Temperature4,602±80[7] K
Metallicity [Fe/H]+0.16±0.01[7] dex
Rotational velocity (v sin i)1[8] km/s
Age4.5[9] Gyr
Other designations
CD−53° 889, CPD−53° 672, GC 5176, GJ 167, HD 27274, HIP 19884, SAO 233456[10]
Database references
SIMBADdata
ARICNSdata
Close

HD 27274 has a stellar classification of K4.5 Vk:,[4] indicating that it is a K-type main-sequence star with interstellar absorption features. However, there is uncertainty behind the classification. At present it has 73% the mass of the Sun and 70% of its radius.[6] It has an effective temperature of 4,602 K,[7] but its small size yields a luminosity only 19.6% that of the Sun.[2] HD 27274 is metal enriched, having an iron abundance 44.6% above solar levels.[7] The star spins with a projected rotational velocity of 1 km/s,[8] and is estimated to be 4.5 billion years old.[9] This is similar to the Sun's current age (4.6 Gyr).

References

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