GSC 02652-01324

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[[Immagine:445px-Lyra_constellation_map.png|thumb|right|200px|Costellazione della Lira.]]
'''[[Guide Star Catalog|GSC]] 02652-01324''' is an [[orange dwarf]] [[main sequence]] [[star]] approximately 512 [[light-year]]s away in the [[constellation]] of [[Lyra]] (the [[Lyre]]) [1].
'''[[Guide Star Catalog|GSC]] 02652-01324''' is an [[orange dwarf]] [[main sequence]] [[star]] approximately 512 [[light-year]]s away in the [[constellation]] of [[Lyra]] (the [[Lyre]]) [1].
== Planetary system ==
== Planetary system ==
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In 2004 the [[extrasolar planet]] [[TrES-1b]] was found to be orbiting this star by the [[Trans-Atlantic Exoplanet Survey]] using the [[Methods_of_detecting_extrasolar_planets#Transit_method|transit method]]. The planet was detected crossing its parent star using a small 4-inch diameter [[telescope]]. The discovery was confirmed by the [[Keck Observatory]] using the [[Methods_of_detecting_extrasolar_planets#Radial_velocity|radial velocity]] method, allowing its mass to be determined.<ref name="disc">{{cite journal |  author=Alonso ''et al.'' | title=TrES-1: The Transiting Planet of a Bright K0V Star | journal=The [[Astrophysical Journal]] Letters | year=2004 | volume=613 | issue=2 | pages=L153–L156 | doi=10.1086/425256}}</ref>
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In 2004 the [[extrasolar planet]] [[TrES-1]] was found to be orbiting this star by the [[Trans-Atlantic Exoplanet Survey]] using the [[Methods_of_detecting_extrasolar_planets#Transit_method|transit method]]. The planet was detected crossing its parent star using a small 4-inch diameter [[telescope]]. The discovery was confirmed by the [[Keck Observatory]] using the [[Methods_of_detecting_extrasolar_planets#Radial_velocity|radial velocity]] method, allowing its mass to be determined [2].
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{{PlanetboxOrbit begin}}
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{{PlanetboxOrbit
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| exoplanet = [[TrES-1b]]
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| mass = 0.61 &plusmn; 0.06 
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| period = 3.030065 &plusmn; 0.000008
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| semimajor = 0.0393 &plusmn; 0.0007
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| eccentricity = 0.135 &plusmn; 0.096 
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}}
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{{PlanetboxOrbit end}}
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== See also ==
== See also ==
Riga 21: Riga 13:
== References ==
== References ==
1^ [http://simbad.u-strasbg.fr/simbad/sim-id?Ident=GSC02652-01324 SIMBAD query result: NAME TrES-1 Parent Star  -- Star], Centre de Données astronomiques de Strasbourg, access 2009-04-22
1^ [http://simbad.u-strasbg.fr/simbad/sim-id?Ident=GSC02652-01324 SIMBAD query result: NAME TrES-1 Parent Star  -- Star], Centre de Données astronomiques de Strasbourg, access 2009-04-22
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2^ Alonso ''et al.'', TrES-1: The Transiting Planet of a Bright K0V Star, The [[Astrophysical Journal]] Letters, 2004, vol.613, issue 2, pag. L153–L156, 10.1086/425256
== External links ==
== External links ==
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* {{cite web |url=http://www.extrasolar.net/startour.asp?StarCatId=normal&StarId=221 |title=GSC 02652-01324 |accessdate=2008-06-21 |work=Extrasolar Visions}}
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* [http://www.extrasolar.net/startour.asp?StarCatId=normal&StarId=221 GSC 02652-01324], access 2008-06-21, Extrasolar Visions
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* {{cite web
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* [http://media4.obspm.fr/exoplanets/base/etoile.php?nom=TrES-1 TrES-1], Exoplanets, access 2009-04-28
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| url=http://media4.obspm.fr/exoplanets/base/etoile.php?nom=TrES-1
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| title=TrES-1
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| work=Exoplanets  
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| accessdate=2009-04-28}}<br /><br />
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[[Categoria:Stelle]]
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[[categoria:Stelle]]

Versione attuale delle 18:42, 17 dic 2009

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Costellazione della Lira.

GSC 02652-01324 is an orange dwarf main sequence star approximately 512 light-years away in the constellation of Lyra (the Lyre) [1].

Indice

Planetary system

In 2004 the extrasolar planet TrES-1 was found to be orbiting this star by the Trans-Atlantic Exoplanet Survey using the transit method. The planet was detected crossing its parent star using a small 4-inch diameter telescope. The discovery was confirmed by the Keck Observatory using the radial velocity method, allowing its mass to be determined [2].

See also

References

1^ SIMBAD query result: NAME TrES-1 Parent Star -- Star, Centre de Données astronomiques de Strasbourg, access 2009-04-22

2^ Alonso et al., TrES-1: The Transiting Planet of a Bright K0V Star, The Astrophysical Journal Letters, 2004, vol.613, issue 2, pag. L153–L156, 10.1086/425256

External links

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