HD 100825
{{Short description|Star in the constellation Centaurus}}
{{about|C2 Centauri|c2 Centauri|HD 129685|other stars with this Bayer designation|C Centauri}}
{{Starbox begin
| name = C2 Centauri
}}
{{Starbox observe
| epoch = J2000.0
| constell = Centaurus
| dec = {{DEC|−47|38|29.9009}}
}}
{{Starbox character
| type =
| class = F0V or A7m
| u-b =
| variable =
}}
{{Starbox astrometry
| parallax = 17.3990
| p_error = 0.1049
}}
{{Starbox detail
| source =
| temperature = {{Val|7737|263|fmt=commas}}
| metal_fe =
| rotational_velocity =
}}
{{Starbox catalog
| names = {{odlist | B=C2 Cen | CD=−46°7205 | FK5=435 | HD=100825 | HIP=56573 | HR=4466 | SAO=222895 | GC=15901 }}
}}
{{Starbox reference
| Simbad = HD+100825
}}
{{Starbox end}}
HD 100825 is a single star in the southern constellation of Centaurus. It has the Bayer designation C2 Centauri, while HD 100825 is the identifier from the Henry Draper catalogue. The star has a yellow-white hue and is dimly visible to the naked eye with an apparent visual magnitude of +5.26. It is located at a distance of 187 light years from the Sun based on parallax, with an absolute magnitude of +1.31. The radial velocity is poorly constrained, but the star appears to be drifting further away from the Sun at the rate of around 5 km/s. It is a member of the Sirius supercluster of co-moving stars.
This is an Am star or metallic-line star with a stellar classification of F0V, indicating it is a F-type main-sequence star that is generating energy by core hydrogen fusion. It is an estimated 467 million years old and has 1.62 times the mass of the Sun. The star is radiating 21 times the luminosity of the Sun from its photosphere at an effective temperature of 7,737 K.
References
{{Reflist|colwidth=30em|refs=
{{cite DR2|5372082838294397952}}
{{cite simbad | title=HD 100825 | access-date=2020-03-01}}
| last1=David | first1=Trevor J. | last2=Hillenbrand | first2=Lynne A.
| title=The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets
| journal=The Astrophysical Journal
| volume=804 | issue=2 | pages=146 | year=2015
| bibcode=2015ApJ...804..146D | doi=10.1088/0004-637X/804/2/146
| arxiv=1501.03154 | s2cid=33401607 | postscript=. }}
| title=XHIP: An extended hipparcos compilation
| last1=Anderson | first1=E. | last2=Francis | first2=Ch.
| journal=Astronomy Letters | arxiv=1108.4971
| volume=38 | issue=5 | pages=331 | year=2012
| bibcode=2012AstL...38..331A | postscript=.
| doi=10.1134/S1063773712050015 | s2cid=119257644 }}
| last1=Houk | first1=Nancy
| title=Michigan catalogue of two-dimensional spectral types for the HD stars
| volume=2 | year=1978 | publication-place=Ann Arbor
| publisher=Dept. of Astronomy, University of Michigan
| bibcode=1978mcts.book.....H | postscript=. }}
| 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
| bibcode=2008MNRAS.389..869E | arxiv=0806.2878
| doi=10.1111/j.1365-2966.2008.13596.x | doi-access=free | s2cid=14878976 | postscript=. }}
| last=Eggen | first=Olin J.
| title=The Sirius supercluster in the FK5
| journal=Astronomical Journal | postscript=.
| date=1992 | volume=104 | issue=4 | pages=1493–1504
| bibcode=1992AJ....104.1493E | doi=10.1086/116334 }}
| last=Malaroda | first=S.
| title=Study of the F-type stars. I. MK spectral types
| journal=Astronomical Journal | postscript=.
| volume=80 | pages=637–641 |date=August 1975
| doi=10.1086/111786 | bibcode=1975AJ.....80..637M | doi-access=free }}
}}
{{Stars of Centaurus}}
{{DEFAULTSORT:C2 Centauri}}