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'''Gliese 686''' (GJ 686 / HIP 86287 / LHS 452)<ref name="SIMBAD1"/> is a ] in the constellation of ], with an ] +9.577.<ref name=Affer/> Although it is close to the ] – at 26.6 ]s – it is not the closest known star in its constellation, since ] is 20.9 light years away.<ref name="closeststars">{{cite web|url=http://www.closeststars.com/|website=closeststars.com|title=Closest stars|access-date=2019-03-31}}</ref> The closest system to this star is the bright ], at 4.5 light years. They are followed by ] and ], at 7.2 and 7.6 light years respectively.<ref name="ISDB">{{cite web|url=http://www.stellar-database.com/Scripts/find_neighbors.exe?ID=122400&ly=15|website=stellar-database.com|title=Stars within 15 light-years of Bonner Durchmusterung +18°3421 (The Internet Stellar Database)|access-date=2019-03-31}}</ref> |
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'''Gliese 686''' (GJ 686 / HIP 86287 / LHS 452)<ref name="SIMBAD1"/> is a ] in the constellation of ], with an ] +9.577.<ref name=Affer/> Although it is close to the ] – at 26.6 ]s – it is not the closest known star in its constellation, since ] is 20.9 light years away.<ref name="closeststars">{{cite web|url=http://www.closeststars.com/|website=closeststars.com|title=Closest stars|access-date=2019-03-31|archive-date=2023-04-11|archive-url=https://web.archive.org/web/20230411091505/http://www.closeststars.com/|url-status=live}}</ref> The closest system to this star is the bright ], at 4.5 light years. They are followed by ] and ], at 7.2 and 7.6 light years respectively.<ref name="ISDB">{{cite web|url=http://www.stellar-database.com/Scripts/find_neighbors.exe?ID=122400&ly=15|website=stellar-database.com|title=Stars within 15 light-years of Bonner Durchmusterung +18°3421 (The Internet Stellar Database)|access-date=2019-03-31}}</ref> |
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Gliese 686 is one of the many ] in the Solar System neighborhood with a ] of M1V,<ref name=Affer/><ref name="SIMBAD1" /> and has an ] of about 3600 ].<ref name=Affer/> Its ] in the ] is equal to 0.82% of that of the ],<ref name="ISDB2">{{cite web|url=http://www.stellar-database.com/Scripts/search_star.exe?Catalog=HIC&CatNo=86287|website=stellar-database.com|title=Bonner Durchmusterung +18°3421 (The Internet Stellar Database)|access-date=2019-03-31}}</ref> while its total luminosity is equivalent to 2.7% that of the Sun,<ref name="Morales"/> since a significant amount of the radiation emitted by these stars is ]. Considering only this last parameter, Gliese 686 is considerably brighter than other known red dwarfs; thus, it is 6.5 times more luminous than ] and 15 times more than ], the closest star to the Solar System. |
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Gliese 686 is one of the many ] in the Solar System neighborhood with a ] of M1V,<ref name=Affer/><ref name="SIMBAD1" /> and has an ] of about 3600 ].<ref name=Affer/> Its ] in the ] is equal to 0.82% of that of the ],<ref name="ISDB2">{{cite web|url=http://www.stellar-database.com/Scripts/search_star.exe?Catalog=HIC&CatNo=86287|website=stellar-database.com|title=Bonner Durchmusterung +18°3421 (The Internet Stellar Database)|access-date=2019-03-31|archive-date=2023-04-11|archive-url=https://web.archive.org/web/20230411091504/http://www.stellar-database.com/Scripts/search_star.exe?Catalog=HIC&CatNo=86287|url-status=live}}</ref> while its total luminosity is equivalent to 2.7% that of the Sun,<ref name="Morales"/> since a significant amount of the radiation emitted by these stars is ]. Considering only this last parameter, Gliese 686 is considerably brighter than other known red dwarfs; thus, it is 6.5 times more luminous than ] and 15 times more than ], the closest star to the Solar System. |
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Gliese 686 has a radius approximately equal to half the ]. Its projected ] is 2.5 km / s, its ] being equal to or less than 10.3 days.<ref name="Houdebine" /> It has a metallic content lower than that of the Sun; various studies estimate its index ] between -0.25 and -0.44.<ref name="Houdebine"/><ref name="Jenkins"/> It has an approximate mass between 45% and 49% of the solar mass<ref name="Bonfils"/> and is a star with characteristics comparable to that of ]. |
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Gliese 686 has a radius approximately equal to half the ]. Its projected ] is 2.5 km / s, its ] being equal to or less than 10.3 days.<ref name="Houdebine" /> It has a metallic content lower than that of the Sun; various studies estimate its index ] between -0.25 and -0.44.<ref name="Houdebine"/><ref name="Jenkins"/> It has an approximate mass between 45% and 49% of the solar mass<ref name="Bonfils"/> and is a star with characteristics comparable to that of ]. |
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<ref name="Bonfils">{{cite journal |doi=10.1051/0004-6361:20053046 |last1=Bonfils |first1=Xavier |last2=Delfosse |first2=Xavier|last3=Udry |first3=Stéphane |last4=Santos |first4=Nuno C. |last5=Forveille |first5=Thierry |last6=Ségransan |first6=Damien |title=Metallicity of M dwarfs. I. A photometric calibration and the impact on the mass-luminosity relation at the bottom of the main sequence |year=2005 |journal=] |volume=442 |issue=2 |arxiv=astro-ph/0503260 |bibcode=2005A&A...442..635B |s2cid=13900901 |pages=635–642 |url=http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2005A%26A...442..635B&db_key=AST&nosetcookie=1 }}</ref> |
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<ref name="Bonfils">{{cite journal |doi=10.1051/0004-6361:20053046 |last1=Bonfils |first1=Xavier |last2=Delfosse |first2=Xavier|last3=Udry |first3=Stéphane |last4=Santos |first4=Nuno C. |last5=Forveille |first5=Thierry |last6=Ségransan |first6=Damien |title=Metallicity of M dwarfs. I. A photometric calibration and the impact on the mass-luminosity relation at the bottom of the main sequence |year=2005 |journal=] |volume=442 |issue=2 |arxiv=astro-ph/0503260 |bibcode=2005A&A...442..635B |s2cid=13900901 |pages=635–642 |url=http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2005A%26A...442..635B&db_key=AST&nosetcookie=1 }}</ref> |
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<ref name="Morales">{{cite journal|author1=Morales, J. C.|author2=Ribas, I.|author3=Jordi, C.|title=The effect of activity on stellar temperatures and radii|year=2008|journal=]|volume=478|issue=2|id=pp. 507-512|url=http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2008A%26A...478..507M&db_key=AST&nosetcookie=1|arxiv=0711.3523|doi=10.1051/0004-6361:20078324|pages=507–512|bibcode=2008A&A...478..507M|s2cid=16238033}}</ref> |
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<ref name="Morales">{{cite journal|author1=Morales, J. C.|author2=Ribas, I.|author3=Jordi, C.|title=The effect of activity on stellar temperatures and radii|year=2008|journal=]|volume=478|issue=2|id=pp. 507-512|url=http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2008A%26A...478..507M&db_key=AST&nosetcookie=1|arxiv=0711.3523|doi=10.1051/0004-6361:20078324|pages=507–512|bibcode=2008A&A...478..507M|s2cid=16238033|access-date=2019-03-31|archive-date=2018-10-02|archive-url=https://web.archive.org/web/20181002100426/http://cdsads.u-strasbg.fr/cgi-bin/nph-bib_query?2008A%26A...478..507M&db_key=AST&nosetcookie=1|url-status=live}}</ref> |
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<ref name="Jenkins">{{cite journal|author1=Jenkins, J. S.|author2=Ramsey, L. W.|author3=Jones, H. R. A.|author4=Pavlenko, Y.|author5=Gallardo, J.|author6=Barnes, J. R.|author7=Pinfield, D. J.|title=Rotational Velocities for M Dwarfs|year=2009|journal=]|volume=704|issue=2|pages=975–988|doi=10.1088/0004-637X/704/2/975|bibcode=2009ApJ...704..975J|arxiv=0908.4092|s2cid=119203469}}</ref> |
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<ref name="Jenkins">{{cite journal|author1=Jenkins, J. S.|author2=Ramsey, L. W.|author3=Jones, H. R. A.|author4=Pavlenko, Y.|author5=Gallardo, J.|author6=Barnes, J. R.|author7=Pinfield, D. J.|title=Rotational Velocities for M Dwarfs|year=2009|journal=]|volume=704|issue=2|pages=975–988|doi=10.1088/0004-637X/704/2/975|bibcode=2009ApJ...704..975J|arxiv=0908.4092|s2cid=119203469}}</ref> |
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