HD 60532 (original) (raw)
HD 60532 is a white (F-type) main sequence star located approximately 84 light-years away in the constellation of Puppis, taking its primary name from its Henry Draper Catalogue designation. It is calculated to be 1.44 times more massive than the Sun. The star is only 59% as old as the Sun (2.7 Gyr) and has metallicity of only 38% that of the Sun. In 2008, two extrasolar planets were discovered in orbit around it.
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dbo:abstract | HD 60532 (HR 2906 / GJ 279 / HIP 36795) es una estrella en la constelación de Puppis. Con magnitud aparente +4,46, es visible a simple vista.Desde 2008 se conoce la existencia de dos planetas extrasolares en órbita alrededor de esta estrella. Aunque en la base de datos SIMBAD HD 60532 aparece catalogada como estrella de tipo-F de la secuencia principal de tipo F6V, se piensa que puede estar evolucionando a subgigante (F6IV-V).Con una temperatura superficial de 6095 K, es 8,6 veces más luminosa que el Sol.Tiene una masa de 1,44 masas solares y rota con una velocidad igual o mayor a 8 km/s.A fecha de 2009, sólo se conoce la existencia de otra estrella más masiva que el Sol que albergue más de un planeta (HD 169830). HD 60532 posee un contenido relativo de hierro notablemente menor que el solar ([Fe/H] = -0,42), lo que no es habitual en planetas con sistemas planetarios.Las abundancias relativas de otros elementos como oxígeno, sodio, magnesio, silicio y titanio siguen la misma tendencia.Su edad se estima en 2700 millones de años y dista 84 años luz del Sistema Solar. (es) HD 60532 is a white (F-type) main sequence star located approximately 84 light-years away in the constellation of Puppis, taking its primary name from its Henry Draper Catalogue designation. It is calculated to be 1.44 times more massive than the Sun. The star is only 59% as old as the Sun (2.7 Gyr) and has metallicity of only 38% that of the Sun. In 2008, two extrasolar planets were discovered in orbit around it. (en) HD 60532 è una stella bianco-gialla nella sequenza principale di magnitudine 4,46 situata nella costellazione della Poppa. Dista 84 anni luce dal sistema solare. (it) HD 60532 – gwiazda w gwiazdozbiorze Rufy, należąca do typu widmowego F. Znajduje się około 83 lata świetlne od Ziemi. Wokół gwiazdy krążą dwie znane planety. (pl) HD 60532 — звезда, которая находится в созвездии Кормы на расстоянии около 84 световых лет от нас. Вокруг звезды обращаются, как минимум, две планеты. (ru) HD 60532 är en ensam stjärna belägen i den mellersta delen av stjärnbilden Akterskeppet. Den har en skenbar magnitud av ca 4,45 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 38,1 mas, beräknas den befinna sig på ett avstånd på ca 86 ljusår (ca 26 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 60 km/s. (sv) HD 60532,又名BD-21 2007,SAO 174009、HR 2906,是一颗位於船尾座的恒星,视星等为4.45,位于銀經237.5,銀緯-1.19,其B1900.0坐标为赤經7h 29m 46.3s,赤緯-22° -1.19′ 48″。該恆星距離地球約84光年,屬於黃-白矮星。它的質量是太陽的1.44倍,年齡約27億年,金屬量只有太陽的38%。2008年在該恆星旁發現兩顆系外行星。 (zh) |
dbo:wikiPageExternalLink | http://media4.obspm.fr/exoplanets/base/etoile.php%3Fnom=HD+60532 https://web.archive.org/web/20091124165050/http:/media4.obspm.fr/exoplanets/base/etoile.php%3Fnom=HD+60532 |
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dbp:absmagV | 2.400000 (xsd:double) |
dbp:ageGyr | 2.700000 (xsd:double) (en) |
dbp:appmagV | 4.450000 (xsd:double) |
dbp:aricns | 578 (xsd:integer) |
dbp:bV | +0.51 (en) |
dbp:class | F6 IV-V (en) |
dbp:constell | dbr:Puppis |
dbp:epe | HD+60532 (en) |
dbp:epoch | J2000.0 (en) |
dbp:exoplanet | dbr:HD_60532_b dbr:HD_60532_c |
dbp:gravity | 4.090000 (xsd:double) |
dbp:luminosity | 8.596000 (xsd:double) |
dbp:mass | 1.440000 (xsd:double) |
dbp:metalFe | –0.42 (en) |
dbp:nsted | HD+60532 (en) |
dbp:pError | 0.108700 (xsd:double) |
dbp:parallax | 38.137900 (xsd:double) |
dbp:propMoDec | 46.840000 (xsd:double) |
dbp:propMoRa | –39.87 (en) |
dbp:radialV | 60.200000 (xsd:double) |
dbp:radius | 2.520000 (xsd:double) |
dbp:rotationalVelocity | 8 (xsd:integer) |
dbp:simbad | HD+60532 (en) |
dbp:temperature | 6095 (xsd:integer) |
dbp:uB | +0.07 (en) |
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rdfs:comment | HD 60532 is a white (F-type) main sequence star located approximately 84 light-years away in the constellation of Puppis, taking its primary name from its Henry Draper Catalogue designation. It is calculated to be 1.44 times more massive than the Sun. The star is only 59% as old as the Sun (2.7 Gyr) and has metallicity of only 38% that of the Sun. In 2008, two extrasolar planets were discovered in orbit around it. (en) HD 60532 è una stella bianco-gialla nella sequenza principale di magnitudine 4,46 situata nella costellazione della Poppa. Dista 84 anni luce dal sistema solare. (it) HD 60532 – gwiazda w gwiazdozbiorze Rufy, należąca do typu widmowego F. Znajduje się około 83 lata świetlne od Ziemi. Wokół gwiazdy krążą dwie znane planety. (pl) HD 60532 — звезда, которая находится в созвездии Кормы на расстоянии около 84 световых лет от нас. Вокруг звезды обращаются, как минимум, две планеты. (ru) HD 60532 är en ensam stjärna belägen i den mellersta delen av stjärnbilden Akterskeppet. Den har en skenbar magnitud av ca 4,45 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 38,1 mas, beräknas den befinna sig på ett avstånd på ca 86 ljusår (ca 26 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet på ca 60 km/s. (sv) HD 60532,又名BD-21 2007,SAO 174009、HR 2906,是一颗位於船尾座的恒星,视星等为4.45,位于銀經237.5,銀緯-1.19,其B1900.0坐标为赤經7h 29m 46.3s,赤緯-22° -1.19′ 48″。該恆星距離地球約84光年,屬於黃-白矮星。它的質量是太陽的1.44倍,年齡約27億年,金屬量只有太陽的38%。2008年在該恆星旁發現兩顆系外行星。 (zh) HD 60532 (HR 2906 / GJ 279 / HIP 36795) es una estrella en la constelación de Puppis. Con magnitud aparente +4,46, es visible a simple vista.Desde 2008 se conoce la existencia de dos planetas extrasolares en órbita alrededor de esta estrella. (es) |
rdfs:label | HD 60532 (es) HD 60532 (en) HD 60532 (it) HD 60532 (pl) HD 60532 (ru) HD 60532 (sv) HD 60532 (zh) |
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foaf:name | HD60532 (en) |
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