69 Orionis
{{Short description|Star in the constellation Orion}}
{{about|f1 Orionis|other stars with this Bayer designation|f Orionis}}
{{Starbox begin}}
{{Starbox image
| image =
{{Location mark
|image=Orion constellation map.svg|alt=|float=center|width=280
|label=|position=right
|mark=Red circle.svg|mark_width=10|mark_link=69 Orionis
|x=335|y=72
}}
| caption = Location of 69 Orionis (circled)
}}
{{Starbox observe
| epoch = J2000
| constell = Orion
}}
{{Starbox character
| type = main sequence
| variable =
}}
{{Starbox astrometry
| parallax = 6.17
| p_error = 0.25
}}
{{Starbox detail
| mass = {{Val|6.4|0.2}}
| temperature = 17,090
| luminosity = {{Val|1442|248|212|fmt=commas}}
| rotational_velocity = {{Val|285|23}}
| gravity = {{Val|4.05|0.17}}
}}
{{Starbox catalog
| names = {{odlist | B=f1 Ori | F=69 Ori | BD=+16°1035 | FK5= | HD=42545 | HIP=29434 | HR=2198 | SAO=95365 | GC=7891 }}
}}
{{Starbox reference
| Simbad = 69+Ori
}}
{{Starbox end}}
69 Orionis is a single star in the equatorial constellation of Orion, positioned a couple of degrees to the north of Xi Orionis. It has the Bayer designation f1 Orionis; 69 Orionis is the Flamsteed designation. The star is visible to the naked eye as faint, blue-white hued point of light with an apparent visual magnitude of 4.92. It is located approximately 530 light-years from the Sun based on parallax, and is drifting further away with a radial velocity of +22 km/s. In 2015, H. Bouy and J. Alves suggested that it is a member of the newly discovered Taurion OB association.
This object is a B-type main-sequence star with a stellar classification of B5Vn, where the 'n' suffix indicates "nebulous" (broad) lines due to rapid rotation. It has a projected rotational velocity of 285 km/s, compared to a critical velocity of {{Val|476|37|ul=km/s}}; the polar axis is inclined by {{Val|64|16|u=°}}. This is a known Be star that began behaving as a normal star in November, 1982. It has 6.4 times the mass of the Sun and is radiating around 1,442 times the Sun's luminosity from its photosphere at an effective temperature of {{val|17090|ul=K|fmt=commas}}.
References
{{reflist|refs=
{{cite simbad | title=69 Ori | access-date=2018-08-06 }}
| title=A catalogue of multiplicity among bright stellar systems
| last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A.
| journal=Monthly Notices of the Royal Astronomical Society
| volume=389 | issue=2 | pages=869 | date=2008
| bibcode=2008MNRAS.389..869E | arxiv=0806.2878
| doi=10.1111/j.1365-2966.2008.13596.x | doi-access=free | s2cid=14878976 }}
| 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 }}
| last1=Ducati | first1=J. R.
| title=VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system
| journal=CDS/ADC Collection of Electronic Catalogues
| volume=2237 | year=2002 | bibcode=2002yCat.2237....0D }}
| last1=Evans | first1=D. S.
| title=The Revision of the General Catalogue of Radial Velocities
| journal=Determination of Radial Velocities and Their Applications
| volume=30 | pages=57 | year=1967
| bibcode=1967IAUS...30...57E }}
| title=XHIP: An extended hipparcos compilation
| journal=Astronomy Letters | arxiv=1108.4971
| volume=38 | issue=5 | pages=331 | year=2012
| last1=Anderson | first1=E. | last2=Francis | first2=Ch.
| bibcode=2012AstL...38..331A | doi=10.1134/S1063773712050015
| s2cid=119257644 }} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=V/137D/XHIP&HIP=29434 Vizier catalog entry]
| last1=Zorec | first1=J. | last2=Frémat | first2=Y.
| last3=Domiciano De Souza | first3=A. | last4=Royer | first4=F.
| last5=Cidale | first5=L. | last6=Hubert | first6=A.-M.
| last7=Semaan | first7=T. | last8=Martayan | first8=C.
| last9=Cochetti | first9=Y. R. | last10=Arias | first10=M. L.
| last11=Aidelman | first11=Y. | last12=Stee | first12=P.
| title=Critical study of the distribution of rotational velocities of Be stars
| display-authors=1 | journal=Astronomy & Astrophysics
| volume=595 | pages=A132 | year=2016
| bibcode=2016A&A...595A.132Z | doi=10.1051/0004-6361/201628760 | doi-access=free | hdl=11336/37946 | hdl-access=free }}
| last1=Gontcharov | first1=G. A.
| title=Dependence of kinematics on the age of stars in the solar neighborhood
| journal=Astronomy Letters
| volume=38 | issue=12 | pages=771–782 | year=2012
| bibcode=2012AstL...38..771G | arxiv=1606.08814
| doi=10.1134/S1063773712120031
| s2cid=118345778
}} [http://vizier.u-strasbg.fr/viz-bin/VizieR-4?-source=J/PAZh/38/860/thin&HIP=29434 Vizier catalog entry]
| title=Cosmography of OB stars in the solar neighbourhood
| last1=Bouy | first1=H. | last2=Alves | first2=J.
| journal=Astronomy & Astrophysics
| volume=584 | id=A26 | pages=13 | date=December 2015
| doi=10.1051/0004-6361/201527058
| bibcode=2015A&A...584A..26B | doi-access=free }}
| last=Lesh | first=Janet Rountree
| title=The Kinematics of the Gould Belt: an Expanding Group?
| journal=Astrophysical Journal Supplement
| volume=17 | page=371 | date=December 1968
| doi=10.1086/190179 | bibcode=1968ApJS...17..371L | doi-access=free }}
| title=Spectrophotometric Study of Four Bright Be Stars
| last1=Goraya | first1=P. S. | last2=Tur | first2=N. S.
| journal=Astrophysics and Space Science
| volume=236 | issue=2 | pages=175–183 | date=February 1996
| doi=10.1007/BF00645142 | bibcode=1996Ap&SS.236..175G | s2cid=123576634 }}
| display-authors=1 | last1=Pasinetti Fracassini | first1=L. E.
| last2=Pastori | first2=L. | last3=Covino | first3=S. | last4=Pozzi | first4=A.
| title=Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)
| edition=Third | journal=Astronomy and Astrophysics
| volume=367 | issue=2 | pages=521–524 | date=February 2001
| bibcode=2001A&A...367..521P | arxiv=astro-ph/0012289
| doi=10.1051/0004-6361:20000451 | s2cid=425754 }}
| title=Spectroscopic and photometric observations of the Be star 69 Orionis
| last1=Bossi | first1=M. | last2=Guerrero | first2=G.
| last3=Mantegazza | first3=L. | last4=Rusconi | first4=L.
| last5=Scardia | first5=M. | last6=Sedmak | first6=G.
| journal=Astronomy and Astrophysics Supplement Series
| volume=46 | pages=173–177 | date=November 1981
| display-authors=1 | bibcode=1981A&AS...46..173B }}
}}
{{Stars of Orion}}
{{DEFAULTSORT:69 Orionis}}
Category:B-type main-sequence stars