epsilon Scuti
{{Short description|Star in the constellation Scutum}}
{{Starbox begin
| name = ε Scuti
}}
{{Starbox image
|image=
{{Location mark
|image=Scutum constellation map.svg|alt=|float=center|width=280
|label=|position=right
|mark=Red circle.svg|mark_width=10|mark_link=Epsilon Scuti
|x=478|y=390
}}
|caption=Location of ε Scuti (circled)
}}
{{Starbox observe
| epoch = J2000
| constell = Scutum
}}
{{Starbox character
}}
{{Starbox astrometry
| parallax = 5.7100
| p_error = 0.1842
| parallax_footnote = {{cite Gaia DR3|4251743058774556288}}
}}
{{Starbox detail
}}
{{Starbox catalog
| names = {{odlist | B=ε Sct | F=3 Aquilae | BD=−08°4686 | FK5=702 | HD=173009 | HIP=91845 | HR=7032 | SAO=142546 | GC=25610 | ADS=11601 | CCDM=J18435-0817A | GSC=05692-02504 | WDS=J18435-0817A }}
}}
{{Starbox reference
| Simbad = Epsilon+Scuti
}}
{{Starbox end}}
Epsilon Scuti, Latinized from ε Scuti, is a probable astrometric binary
{{citation | last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | title=A catalogue of multiplicity among bright stellar systems | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869–879 |date=September 2008 | doi=10.1111/j.1365-2966.2008.13596.x | doi-access=free | bibcode=2008MNRAS.389..869E | postscript=. |arxiv = 0806.2878 | s2cid=14878976 }} star system in the constellation Scutum. It is faintly visible to the naked eye with an apparent visual magnitude of +4.88. Based upon an annual parallax shift of 5.71 mas as seen from Earth,> it is located approximately 570 light years from the Sun. It is moving closer to the Sun with a radial velocity of −9.8 km/s.
Epsilon Scuti was a latter designation of 3 Aquilae.{{cite journal | last=Wagman | first=M. | title=Flamsteed's Missing Stars | journal=Journal for the History of Astronomy | volume=18 | issue=3 | date=August 1987 | page=212 | bibcode=1987JHA....18..209W | doi=10.1177/002182868701800305 | s2cid=118445625 }}
The visible component is a yellow-hued bright giant with a G-type bright giant It is radiating 403 times the Sun's luminosity from its photosphere at an effective temperature of 4,500 K. Epsilon Scuti has at least three faint visual companions, two 14th magnitude stars, B and D, separated from the primary by 13.6 and 15.4 arcseconds respectively, and the 13th magnitude C, which is 38 arcseconds away.{{cite journal | bibcode=2001AJ....122.3466M | doi=10.1086/323920 | title=The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog | journal=The Astronomical Journal | volume=122 | issue=6 | pages=3466 | year=2001 | last1=Mason | first1=Brian D. | last2=Wycoff | first2=Gary L. | last3=Hartkopf | first3=William I. | last4=Douglass | first4=Geoffrey G. | last5=Worley | first5=Charles E. | doi-access=free }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=B/wds/wds&WDS=18435-0817 Vizier catalog entry]