Epsilon Phoenicis

Star in the constellation Phoenix From Wikipedia, the free encyclopedia

Epsilon Phoenicis is a star in the southern constellation of Phoenix. It is visible to the naked eye with an apparent visual magnitude of 3.87.[2] The distance to this star is approximately 144 light years based on parallax measurements, but it is drifting closer with a heliocentric radial velocity of −9.2 km/s.[5]

Quick facts Constellation, Right ascension ...
ε Phoenicis
Location of ε Phoenicis (circled)
Observation data
Epoch J2000      Equinox ICRS
Constellation Phoenix
Right ascension 00h 09m 24.640s[1]
Declination −45° 44 50.73[1]
Apparent magnitude (V) 3.87[2]
Characteristics
Evolutionary stage Red clump[3]
Spectral type K0III[4]
U−B color index +0.84[2]
B−V color index +1.02[2]
Astrometry
Radial velocity (Rv)−9.20[5] km/s
Proper motion (μ) RA: +120.393 mas/yr[1]
Dec.: −179.597 mas/yr[1]
Parallax (π)22.6081±0.1481 mas[1]
Distance144.3 ± 0.9 ly
(44.2 ± 0.3 pc)
Absolute magnitude (MV)0.65[6]
Details[7]
Mass1.93±0.23 M
Radius10.03±0.22 R
Luminosity50.4±1.5 L
Surface gravity (log g)2.560±0.103 cgs
Temperature4,862±42[8] K
Metallicity [Fe/H]+0.00±0.08[8] dex
Rotational velocity (v sin i)< 1.5[9] km/s
Other designations
FK5 3, GC 158, HD 496, HIP 765, HR 25, SAO 214983[10]
Database references
SIMBADdata
Close

This is an evolved giant star with a stellar classification of K0III,[4] a star that has used up its core hydrogen and has expanded. It is a red clump star, indicating that it has passed the red-giant branch, undergone a helium flash and is currently on the core helium-fusing horizontal branch.[3] Epsilon Phoenicis is about two times more massive than the Sun, and expanded to ten times its radius. It radiates 50 the luminosity of the Sun from its photosphere[7] at an effective temperature of 4,862 K. Based on the elemental abundance of iron in the stellar atmosphere, the metallicity of Epsilon Phoenicis is similar to that of the Sun.[8]

References

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