16 Persei
{{Short description|Star in the constellation Perseus}}
{{Starbox begin
| name = 16 Persei
}}
{{Starbox image
|image=
{{Location mark
|image=Perseus constellation map.svg|alt=|float=center|width=280
|label=|position=right
|mark=Red circle.svg|mark_width=10|mark_link=16 Persei
|x=744|y=724
}}
|caption=Location of 16 Persei (circled)
}}
{{Starbox observe
| epoch = J2000
| constell = Perseus
}}
{{Starbox character
| variable=δ Sct(?){{cite web|title=NSV 956 |url=https://www.aavso.org/vsx/index.php?view=detail.top&oid=39580 |work=The International Variable Star Index |publisher=AAVSO – American Association of Variable Star Observers |access-date=17 February 2019 }}{{cite journal | display-authors=1 | last1=Samus | first1=N. N. | last2=Kazarovets | first2=E. V. | last3=Durlevich | first3=O. V. | last4=Kireeva | first4=N. N. | last5=Pastukhova | first5=E. N. | title=General Catalogue of Variable Stars | version=5.1 | journal=Astronomy Reports | year=2017 | volume=61 | issue=1 | pages=80–88 | doi=10.1134/S1063772917010085 | bibcode=2017ARep...61...80S | s2cid=125853869 }}
}}
{{Starbox astrometry
| radial_v = +14.00{{cite journal | last=Wilson | first=R. E. | year=1953 | title=General Catalogue of Stellar Radial Velocities | journal=Carnegie Institute Washington D.C. Publication | publisher=Carnegie Institution for Science | bibcode=1953GCRV..C......0W | lccn=54001336 }}
| parallax = 27.01
| p_error = 0.19
}}
{{Starbox detail
}}
{{Starbox catalog
| names = {{odlist | F=16 Per | BD=+37°646 | FK5=2194 | HD=17584 | HIP=13254 | HR=840 | SAO=55928 | CCDM=J02506+3818A | GC=3401 | LTT=10924 | NSV=956 | WDS+J02506+3819A }}{{cite simbad | title=16 Per | access-date=2019-04-01 }}
}}
{{Starbox reference
| Simbad = 16+Persei
}}
{{Starbox end}}
16 Persei is a single,{{cite journal | 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 | arxiv=0806.2878 | s2cid=14878976 }} suspected variable star in the northern constellation of Perseus, located approximately 121 light years away based on parallax. It is visible to the naked eye as a yellow-white hued star with an apparent visual magnitude of 4.22. This object is moving further from the Earth with a heliocentric radial velocity of +14 km/s. It displays a relatively high proper motion, traversing the celestial sphere at the rate of {{Val|0.224|ul=arcsecond}} per year.{{citation | last1=Lépine | first1=Sébastien | last2=Shara | first2=Michael M. | title=A Catalog of Northern Stars with Annual Proper Motions Larger than 0.15" (LSPM-NORTH Catalog) | journal=The Astronomical Journal | volume=129 | issue=3 | pages=1483–1522 | date=March 2005 | doi=10.1086/427854 | bibcode=2005AJ....129.1483L | arxiv=astro-ph/0412070 | s2cid=2603568 | postscript=. }}
File:16PerLightCurve.png for 16 Persei, plotted from TESS data]]
Based upon a stellar classification of F2 III, this matches an aging giant star that has exhausted the hydrogen at its core and is evolving away from the main sequence. It is a possible pulsating Delta Scuti variable, although there is some uncertainty about this classification. However, Kunzli and North (1998) found no variation.{{cite journal | title=Are metallic A-F giants evolved AM stars? Rotation and rate of binaries among giant F stars | last1=Kunzli | first1=M. | last2=North | first2=P. | journal=Astronomy and Astrophysics Supplement | volume=127 | pages=277–294 | date=January 1998 | issue=2 | doi=10.1051/aas:1998350 | bibcode=1998A&AS..127..277K | arxiv=astro-ph/9710226 | s2cid=7535170 }} The star is 1.44 billion years old with 1.8 times the mass of the Sun and 3.2 times the Sun's radius. It shows a high rotation rate with a projected rotational velocity of 149 km/s, which is causing an equatorial bulge that is an estimated 24% larger than the polar radius.{{citation | last1=van Belle, Gerard T. | title=Interferometric observations of rapidly rotating stars | journal=The Astronomy and Astrophysics Review | volume=20 | issue=1 | page=51 |date=March 2012 | doi=10.1007/s00159-012-0051-2 | bibcode=2012A&ARv..20...51V | postscript=. |arxiv = 1204.2572 | s2cid=119273474 }} 16 Persei is radiating 23 times the Sun's luminosity from its photosphere at an effective temperature of 7,004 K.
It has two reported visual companions: B, with a magnitude of 12.8 and separation of 76.7", and C, with magnitude 10.43 and separation 234".{{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=02506%2B3819 Vizier catalog entry]
References
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{{Stars of Perseus}}
{{DEFAULTSORT:16 Persei}}
Category:Delta Scuti variables