Epsilon Pavonis
{{Short description|Star in the constellation Pavo}}
{{Starbox begin
| name = ε Pavonis
}}
{{Starbox image
|image=
{{Location mark
|image=Pavo constellation map.svg|alt=|float=center|width=280
|label=|position=right
|mark=Red circle.svg|mark_width=10|mark_link=Epsilon Pavonis
|x=434|y=504
}}
|caption=Location of ε Pavonis (circled)
}}
{{Starbox observe
| epoch = J2000
| constell = Pavo
| dec = {{DEC|-72|54|37.8198}}
}}
{{Starbox character
}}
{{Starbox astrometry
| parallax = 31.04
| p_error = 0.17
}}
{{Starbox detail
| radius = 1.74{{citation | display-authors=1
| last1=Gerbaldi | first1=M. | last2=Faraggiana | first2=R.
| last3=Burnage | first3=R. | last4=Delmas | first4=F.
| last5=Gómez | first5=A. E. | last6=Grenier | first6=S.
| title=Search for reference A0 dwarf stars: Masses and luminosities revisited with HIPPARCOS parallaxes
| journal=Astronomy and Astrophysics Supplement | postscript=.
| volume=137 | issue=2 | pages=273–292 |date=June 1999
| doi=10.1051/aas:1999248 | bibcode=1999A&AS..137..273G | doi-access=free }}
}}
{{Starbox catalog
| names = {{odlist | B=ε Pav | CPD=−73° 2086 | FK5=748 | HD=188228 | HIP=98495 | HR=7590 | SAO=257757 | GC=27631 }}
}}
{{Starbox reference
| Simbad = Epsilon+Pavonis
}}
{{Starbox end}}
Epsilon Pavonis, Latinized from ε Pavonis, is a single,{{cite journal | title=A catalogue of multiplicity among bright stellar systems | last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869 | date=2008 | doi=10.1111/j.1365-2966.2008.13596.x | doi-access=free | bibcode=2008MNRAS.389..869E | arxiv=0806.2878 | s2cid=14878976 }} white-hued star in the constellation Pavo. It can be viewed with the naked eye, having an apparent visual magnitude of 3.97. The annual parallax shift of 31.04 mas provides a distance estimate of 105 light years from the Sun. This star is a member of the proposed Argus Association, a young moving group of more than 60 stars associated with the IC 2391 cluster.{{cite journal | title=The Tucana/Horologium, Columba, AB Doradus, and Argus Associations: New Members and Dusty Debris Disks | display-authors=1 | last1=Zuckerman | first1=B. | last2=Rhee | first2=Joseph H. | last3=Song | first3=Inseok | last4=Bessell | first4=M. S. | journal=The Astrophysical Journal | volume=732 | issue=2 | id=61 | pages=19 | date=May 2011 | doi=10.1088/0004-637X/732/2/61 | bibcode=2011ApJ...732...61Z | arxiv=1104.0284 | s2cid=62797470 }} Epsilon Pavonis is moving closer to the Sun with a radial velocity of −6.7 km/s.
With a stellar classification of A0 Va, Epsilon Pavonis is an ordinary A-type main-sequence star that is generating energy through hydrogen fusion at its core. It is just 27 million years old with a projected rotational velocity of 85 km/s. The star has 2.2 times the mass of the Sun and 1.74 the Sun's radius. It is radiating 32 times the Sun's luminosity from its photosphere at an effective temperature of 10,440 K.
References
{{reflist}}
{{Stars of Pavo}}
{{DEFAULTSORT:Epsilon Pavonis}}
Category:A-type main-sequence stars