Xi1 Canis Majoris
{{short description|Star in the constellation Canis Major}}
{{For|other star systems with this Bayer designation|Xi Canis Majoris}}
{{DISPLAYTITLE:Xi1 Canis Majoris}}
{{Starbox begin
| name = ξ1 Canis Majoris
}}
{{Starbox image
| image=
{{Location mark
|image=Canis Major constellation map.svg|alt=|float=center|width=260
|label=|position=right
|mark=Red circle.svg|mark_width=10|mark_link=ξ1 Canis Majoris
|x=482|y=624
}}
|caption=Location of ξ1 Canis Majoris (circled)
}}
{{Starbox observe
| epoch = J2000.0
| constell = Canis Major
| dec = {{DEC|−23|25|06.3181}}
}}
{{Starbox character
| variable = β Cep
}}
{{Starbox astrometry
| parallax = 2.36
| p_error = 0.20
}}
{{Starbox detail
| luminosity = {{val|30,900|8,900|6,900|fmt=commas}}
| temperature = {{val|27,000|1,000|fmt=commas}}
}}
{{Starbox catalog
| names={{odlist | B=ξ1 CMa | F=4 Canis Majoris | CD=−23°3991 | FK5= | HD=46328 | HIP=31125 | HR=2387 | SAO=171895 | ADS=5176 | CCDM=06319-2325 | GC=8496 }}
}}
{{Starbox reference
|Simbad=ksi01+CMa
}}
{{Starbox end}}
Xi1 Canis Majoris, Latinized from ξ1 Canis Majoris, is a Beta Cephei variable star in the constellation Canis Major. It is approximately 1,400 light years from Earth.
ξ1 Canis Majoris is a blue-white B-type star. It has generally been assigned a luminosity class of III (giant) or IV (subgiant), for example B1III or B0.5IV. Comparison of its properties with model evolutionary tracks suggest that it is a main sequence star about three quarters of the way through its main sequence lifetime.
File:Xi1CMaLightCurve.png for Xi1 Canis Majoris, plotted from TESS data]]
The apparent magnitude varies from +4.33 to +4.36 with a period of 5.03 hours. Its pulsations cause its radius to vary by 1.0% to 1.5%. At the same time its effective temperature by about {{val|500|ul=K}} above and below its mean temperature.
ξ1 Canis Majoris has the longest known rotation period of any B class star, taking around 30 years to complete one revolution on its axis. This is thought to be due to magnetic braking; ξ1 Canis Majoris has the strongest magnetic field of any β Cephei star and would be expected to spin down completely in around four million years. It also has the strongest and hardest X-ray emission of any β Cephei star.
ξ1 Canis Majoris forms a naked eye pairing with ξ2 Canis Majoris a little less than a degree away. The Washington Double Star Catalog lists two 14th magnitude companions about {{val|27|ul="}} away. In addition, an unseen close companion is suspected due to some faint emission lines in the spectrum that are best explained by a Be star invisible against the brighter primary.
References
{{reflist|refs=
| title=MAST: Barbara A. Mikulski Archive for Space Telescopes
| url=https://mast.stsci.edu/portal/Mashup/Clients/Mast/Portal.html
| publisher=Space Telescope Science Institute |access-date=20 August 2022}}
| title=Validation of the new Hipparcos reduction
| last1=van Leeuwen | first1=F.
| journal=Astronomy and Astrophysics
| volume=474 | issue=2 | pages=653–664 | date=2007
| arxiv=0708.1752 | bibcode=2007A&A...474..653V
| doi=10.1051/0004-6361:20078357 | s2cid=18759600 }}
| title=XHIP: An extended hipparcos compilation
| last1=Anderson | first1=E. | last2=Francis | first2=Ch.
| journal=Astronomy Letters
| volume=38 | issue=5 | pages=331 | year=2012
| bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015
| arxiv=1108.4971 | s2cid=119257644 }}
| last=Evans | first=D. S. | date=June 20–24, 1966
| editor1-last=Batten | editor1-first=Alan Henry
| editor2-last=Heard | editor2-first=John Frederick
| contribution=The Revision of the General Catalogue of Radial Velocities
| title=Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30
| journal=Determination of Radial Velocities and Their Applications | volume=30 | pages=57 | bibcode=1967IAUS...30...57E }}
{{cite journal | display-authors=1
| last1=Johnson | first1=H. L. | last2=Iriarte | first2=B.
| last3=Mitchell | first3=R. I. | last4=Wisniewskj | first4=W. Z.
| title=UBVRIJKL photometry of the bright stars
| journal=Communications of the Lunar and Planetary Laboratory
| volume=4 | issue=99 | pages=99 | year=1966
| bibcode=1966CoLPL...4...99J }}
}}
{{Stars of Canis Major}}
{{DEFAULTSORT:Xi1 Canis Majoris}}
Category:Beta Cephei variables