21 Persei
{{Short description|Star in the constellation Perseus}}
{{Starbox begin
| name = 21 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=21 Persei
|x=728|y=906
}}
|caption=Location of 21 Persei (circled)
}}
{{Starbox observe
| epoch = J2000
| constell = Perseus
| ra = {{RA|02|57|17.28228}}{{cite DR2|135525184764395776}}
}}
{{Starbox character
| variable = α² CVn{{cite journal | bibcode=2009yCat....102025S |title=VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)|journal=VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S|volume=1|display-authors=etal|last1=Samus|first1=N. N.|last2=Durlevich|first2=O. V.|year=2009}}
}}
{{Starbox astrometry
| parallax = 9.8477
| p_error = 0.2575
}}
{{Starbox detail
}}
{{Starbox catalog
| names = {{odlist | V=LT Per | F=21 Per | BD=+31°509 | FK5=2205 | HD=18296 | HIP=13775 | HR=873 | SAO=56031 | GC=3544 }}{{cite simbad | title=21 Per | access-date=2019-03-29 }}
}}
{{Starbox reference
| Simbad = 21+Persei
}}
{{Starbox end}}
21 Persei is a single,{{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 }} variable star in the northern constellation of Perseus, located about 331 light years away from the Sun. It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 5.10 km/s. The object is moving further from the Earth with a heliocentric radial velocity of +8.5 km/s. It has the variable star designation LT Persei; 21 Persei is the Flamsteed designation.
File:LTPerLightCurve.png for LT Persei, plotted from Hipparcos data{{cite web |title=Hipparcos Tools Interactive Data Access |url=https://www.cosmos.esa.int/web/hipparcos/interactive-data-access |website=Hipparcos |publisher=ESA |access-date=8 December 2021}}]]
This is an Ap star with a stellar classification of A2VspSiEu, where the A2V indicates it is an A-type main-sequence star, 's' means narrow "sharp" absorption, and SiEu shows abundance anomalies of the elements silicon and europium. The star is an Alpha2 Canum Venaticorum variable, meaning that the star has a strong magnetic field chromium, silicon, and strontium spectral lines. 21 Persei's period of variability is approximately 2.88 days.{{cite journal | title=Third supplement to the catalogue of observed periods of Ap stars | last1=Catalano | first1=F. A. | last2=Renson | first2=P. | last3=Leone | first3=F. | journal=Astronomy and Astrophysics Supplement Series | volume=98 | issue=2 | pages=269–273 | bibcode=1993A&AS...98..269C | year=1993 }}
{{clear left}}
References
{{Reflist}}
{{Stars of Perseus}}
{{DEFAULTSORT:21 Persei}}
Category:B-type main-sequence stars
Category:Alpha2 Canum Venaticorum variables