Epsilon Phoenicis
{{Short description|Star in the constellation Phoenix}}
{{Starbox begin
| name = ε Phoenicis
}}
{{Starbox image
| image =
{{Location mark
| image=Phoenix constellation map.svg | alt= | float=center | width=280
| label=|position=right
| mark=Red circle.svg | mark_width=10 | mark_link=Epsilon Phoenicis
| x = 622 | y = 270
}}
| caption = Location of ε Phoenicis (circled)
}}
{{Starbox observe
| epoch = J2000
| constell = Phoenix
}}
{{Starbox character
}}
{{Starbox astrometry
| prop_mo_ra = +120.393
| prop_mo_dec = −179.597
| parallax = 22.6081
| p_error = 0.1481
}}
{{Starbox detail
| mass = {{val|1.93|0.23}}
| radius = {{val|10.03|0.22}}
| luminosity = {{val|50.4|1.5}}
| gravity = {{val|2.560|0.103}}
| age_gyr =
}}
{{Starbox catalog
| names = {{odlist | FK5=3 | GC=158 | HIP=765 | HR=25 | HD=496 | SAO=214983 }}
}}
{{Starbox reference
| Simbad = Epsilon+Phoenicis
}}
{{Starbox end}}
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. 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.
This is an evolved giant star with a stellar classification of K0III, 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. 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 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.
References
{{reflist|refs=
{{cite simbad | title=eps Phe | access-date=2024-11-07 }}
{{Cite Gaia EDR3|4990516294443333504}}
| title=Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys
| display-authors=1 | last1=Soubiran | first1=C.
| last2=Brouillet | first2=N. | last3=Casamiquela | first3=L.
| journal=Astronomy and Astrophysics
| volume=663 | pages=A4 | date=July 1, 2022
| doi=10.1051/0004-6361/202142409 |issn=0004-6361
| bibcode=2022A&A...663A...4S | arxiv=2112.07545 }}
| title=A new Large Magellanic Cloud K-band distance from precision measurements of nearby red clump stars
| display-authors=1 | last1=Laney | first1=C. D.
| last2=Joner | first2=M. D. | last3=Pietrzyński | first3=G.
| journal=Monthly Notices of the Royal Astronomical Society
| volume=419 | issue=2 | pages=1637 | year=2012
| bibcode=2012MNRAS.419.1637L
| doi=10.1111/j.1365-2966.2011.19826.x | doi-access=free
| arxiv=1109.4800 | s2cid=117788450 }}
| last1=Houk | first1=N.
| title=Michigan catalogue of two-dimensional spectral types for the HD stars
| volume=2 | date=1978
| publisher=Dept. of Astronomy, University of Michigan
| bibcode=1978mcts.book.....H
}}
{{Cite journal |last1=Ottoni |first1=G. |last2=Udry |first2=S. |last3=Ségransan |first3=D. |last4=Buldgen |first4=G. |last5=Lovis |first5=C. |last6=Eggenberger |first6=P. |last7=Pezzotti |first7=C. |last8=Adibekyan |first8=V. |last9=Marmier |first9=M. |last10=Mayor |first10=M. |last11=Santos |first11=N. C. |last12=Sousa |first12=S. G. |last13=Lagarde |first13=N. |last14=Charbonnel |first14=C. |date=2022-01-01 |title=CORALIE radial-velocity search for companions around evolved stars (CASCADES). I. Sample definition and first results: Three new planets orbiting giant stars |bibcode=2022A&A...657A..87O |journal=Astronomy and Astrophysics |volume=657 |pages=A87 |doi=10.1051/0004-6361/202040078 |issn=0004-6361|arxiv=2201.01528}} [https://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/657/A87&HD=496 Epsilon Phoenicis' database entry] at VizieR.
}}
{{Stars of Phoenix}}
Category:Horizontal-branch stars
Category:Phoenix (constellation)
Category:Durchmusterung objects
{{giant-star-stub}}