6 Lacertae
{{Short description|Star in the constellation Lacerta}}
{{Starbox begin
| name = 6 Lacertae
}}
{{Starbox observe
| epoch = J2000
| constell = Lacerta
| dec = {{DEC|+43|07|24.1565}}
}}
{{Starbox character
| type =
| u-b =
| variable =
}}
{{Starbox astrometry
| parallax = 1.7577
| p_error = 0.2697
}}
{{Starbox orbit
| period_unitless = 880 days
| eccentricity = 0.30
| periastron = {{Val|2416300|ul=JD|fmt=commas}}
| periarg = 190
| k1 = 9
}}
{{Starbox detail
| source =
| luminosity_bolometric = 34,590
}}
{{Starbox catalog
| names = {{odlist | F=6 Lac | BD=+42°4420 | FK5=3800 | HD=213420 | HIP=111104 | HR=8579 | SAO=52079 }}
}}
{{Starbox reference
| Simbad = 6+Lac
}}
{{Starbox end}}
6 Lacertae is a binary star system in the northern constellation of Lacerta, located around 1,900 light years from the Sun. It is visible to the naked eye as a dim, blue-white hued star with a combined apparent visual magnitude of 4.52. The system is moving closer to the Earth with a heliocentric radial velocity of −9 km/s, and is a suspected member of the Lac OB1 association.
This system forms a single-lined spectroscopic binary with an orbital period of 880 days and an eccentricity of 0.3. The visible component has a stellar classification of B2 IV, matching a B-type subgiant star. It is about 16 million years old with a relatively high projected rotational velocity of 70 km/s. The star has 12.5 times the mass of the Sun and about 7 times the Sun's radius. It is radiating a net 34,590 times the Sun's luminosity from its photosphere at an effective temperature of 21,150 K.
References
{{reflist|refs=
{{cite simbad | title=6 Lac | access-date=2019-01-28 }}
{{cite DR2|1999776222304976384}}
| last=Lesh | first=Janet Rountree
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| journal=Astrophysical Journal Supplement
| volume=17 | page=371 | date=December 1968
| doi=10.1086/190179 | bibcode=1968ApJS...17..371L | doi-access=free }}
| title=XHIP: An extended hipparcos compilation
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| bibcode=2012AstL...38..331A | arxiv=1108.4971
| doi=10.1134/S1063773712050015 | s2cid=119257644 | postscript=. }}
| title=Lacerta OB1 Revisited
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| volume=121 | issue=884 | pages=1045–1053 | date=October 2009
| doi=10.1086/606037 | bibcode=2009PASP..121.1045K | s2cid=120329065 | doi-access=free }}
{{citation | display-authors=1
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| arxiv=astro-ph/0012289 | s2cid=425754 | postscript=.}}
| title=Carbon, Nitrogen, and Oxygen Abundances in Early B-Type Stars
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| journal=Astrophysical Journal | postscript=.
| volume=387 | page=673 | date=March 1992
| doi=10.1086/171116 | bibcode=1992ApJ...387..673G | doi-access=free }}
| display-authors=1 | last1=Strom | first1=Stephen E.
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| title=B Star Rotational Velocities in h and χ Persei: A Probe of Initial Conditions during the Star Formation Epoch?
| journal=The Astronomical Journal
| volume=129 | issue=2 | pages=809–828 | date=2005
| bibcode=2005AJ....129..809S | doi=10.1086/426748
| arxiv=astro-ph/0410337 | s2cid=15059129 | postscript=. }}
| title=The Radial Velocities of 129 Stars in the Years 1906 to 1917
| last1=Beardsley | first1=Wallace R.
| journal=Publications of the Allegheny Observatory of the University of Pittsburgh
| volume=7 | pages=91–263 | year=1969
| bibcode=1969PAllO...8...91B | postscript=. }}
| display-authors=1 | last1=Tetzlaff | first1=N.
| last2=Neuhäuser | first2=R. | last3=Hohle | first3=M. M.
| title=A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun
| journal=Monthly Notices of the Royal Astronomical Society
| volume=410 | issue=1 | pages=190–200 | date=January 2011
| doi=10.1111/j.1365-2966.2010.17434.x | doi-access=free | postscript=.
| bibcode=2011MNRAS.410..190T | arxiv=1007.4883 | s2cid=118629873 }}
| last1=Hohle | first1=M. M. | last2=Neuhäuser | first2=R.
| last3=Schutz | first3=B. F. | display-authors=1
| title=Masses and luminosities of O- and B-type stars and red supergiants
| journal=Astronomische Nachrichten
| volume=331 | issue=4 | page=349 | date=April 2010
| doi=10.1002/asna.200911355 | arxiv=1003.2335
| bibcode=2010AN....331..349H | s2cid=111387483 | postscript=. }}
}}
{{Stars of Lacerta}}
{{DEFAULTSORT:6 Lacertae}}
Category:Spectroscopic binaries