"5616000.0"^^ . "10.894"^^ . . "0.8149999999999999"^^ . . "\u2212644.464"@en . . "Gliese 180 (GJ 180), \u00E8 una stella nana rossa nella costellazione dell'Eridano, situata a 39,5 anni luce dal sistema solare. \u00C8 nota per avere due pianeti, Gliese 180 b e Gliese 180 c, in orbita attorno a s\u00E9."@it . "M2V or M3V"@en . . . "GJ 180 llamada igualmente Gliese 180, es una estrella de tipo M, conocida para tener dos planetas GJ 180 b y GJ 180 c. Se ubica a 38 a\u00F1os-luz de la Tierra. Seg\u00FAn laboratorio de habitabilidad planetaria (PHL) a Puerto Rico, dos mundos en el sistema pueden estar clasificados como de los planetas potencialmente habitables. Sin embargo, el Dr Mikko Tuomi, de la Universidad brit\u00E1nica de Hertfordshire, cuyo equipo ha identificado los planetas, es en desacuerdo, declarando : \"El PHL a\u00F1ade un tipo de un \"HZ prolongada\", que francamente, no s\u00E9 c\u00F3mo est\u00E1 calculado, pero que a\u00F1ade ciertas zonas de habitabilidad potencial para los bordes interiores y exteriores de la HZ que nos lo hemos definido. Comprend\u00EDan el compa\u00F1ero interno del sistema GJ 180 (planeta b) que consideramos demasiado caliente para estar potencialmente habitable.\""@es . . "0.553"^^ . . . "0.09"^^ . . "\u0413\u043B\u0438\u0437\u0435 180"@ru . . "Gliese 180"@de . "day"@en . "10.48"^^ . "Gliese 180 (GJ 180), \u00E8 una stella nana rossa nella costellazione dell'Eridano, situata a 39,5 anni luce dal sistema solare. \u00C8 nota per avere due pianeti, Gliese 180 b e Gliese 180 c, in orbita attorno a s\u00E9."@it . "J2000"@en . "GJ180"@en . . . . "1.155"^^ . "Gliese 180 \u2013 gwiazda w gwiazdozbiorze Erydanu. Znajduje si\u0119 w odleg\u0142o\u015Bci oko\u0142o 39 lat \u015Bwietlnych od S\u0142o\u0144ca. Ma uk\u0142ad planetarny."@pl . . "GJ 180"@en . . . "GJ 180 appel\u00E9e \u00E9galement Gliese 180, est un syst\u00E8me plan\u00E9taire comprenant une \u00E9toile naine rouge de type M et comprenant deux plan\u00E8tes de type super-Terre GJ 180 b et GJ 180 c. Ces deux plan\u00E8tes ont \u00E9t\u00E9 d\u00E9couvertes en 2014 par la m\u00E9thode des vitesses radiales. Le syst\u00E8me se situe \u00E0 338,1 ann\u00E9es-lumi\u00E8re dans la constellation de l'Eridan. Selon laboratoire d'habitabilit\u00E9 plan\u00E9taire (PHL) \u00E0 Puerto Rico, deux mondes dans le syst\u00E8me peuvent \u00EAtre class\u00E9s comme des plan\u00E8tes potentiellement habitables. Toutefois, le Dr Mikko Tuomi, de l'Universit\u00E9 britannique de Hertfordshire, dont l'\u00E9quipe a identifi\u00E9 les plan\u00E8tes, est en d\u00E9saccord, d\u00E9clarant : \"Le PHL ajoute une sorte d'un \"HZ prolong\u00E9e\", qui franchement, je ne sais pas comment il est calcul\u00E9, mais qui ajoute certaines zones d'habitabilit\u00E9 potentielle pour les bords int\u00E9rieurs et ext\u00E9rieurs de la HZ que nous l'avons d\u00E9finie. Ils comprenaient le compagnon interne du syst\u00E8me GJ 180 (plan\u00E8te b) que nous consid\u00E9rons trop chaud pour \u00EAtre potentiellement habitable.\""@fr . . . . . "Gliese 180"@en . . "5"^^ . "\u30B0\u30EA\u30FC\u30BC180 (\u82F1\u8A9E: Gliese 180\uFF09\u306F\u3001\u30B0\u30EA\u30FC\u30BC180b \u3068 \u30B0\u30EA\u30FC\u30BC180c\u306E2\u3064\u306E\u592A\u967D\u7CFB\u5916\u60D1\u661F\u3092\u6301\u3064\u8D64\u8272\u77EE\u661F\u3067\u3042\u308B\u3002\u5730\u7403\u304B\u3089\u306F\u7D0439\u5149\u5E74\u96E2\u308C\u3066\u3044\u308B\u3002"@ja . . . "\u0413\u043B\u0438\u0437\u0435 180 (\u0442\u0430\u043A\u0436\u0435 GJ 180) \u2014 \u043E\u0434\u0438\u043D\u043E\u0447\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u042D\u0440\u0438\u0434\u0430\u043D\u0430. \u041D\u0430\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 38 \u0441\u0432. \u043B\u0435\u0442 \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0413\u043B\u0438\u0437\u0435 180 \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u043A\u0440\u0430\u0441\u043D\u044B\u043C \u043A\u0430\u0440\u043B\u0438\u043A\u043E\u043C \u0441\u043F\u0435\u043A\u0442\u0440\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u043B\u0430\u0441\u0441\u0430 M2V. \u041C\u0430\u0441\u0441\u0430 \u0437\u0432\u0435\u0437\u0434\u044B \u2014 0,39 \u043C\u0430\u0441\u0441\u044B \u0421\u043E\u043B\u043D\u0446\u0430, \u0440\u0430\u0434\u0438\u0443\u0441 \u2014 0,42 \u0440\u0430\u0434\u0438\u0443\u0441\u0430 \u0421\u043E\u043B\u043D\u0446\u0430, \u0442\u0435\u043C\u043F\u0435\u0440\u0430\u0442\u0443\u0440\u0430 \u043F\u043E\u0432\u0435\u0440\u0445\u043D\u043E\u0441\u0442\u0438 \u2014 3562 K."@ru . . "1.205"^^ . . . . "0.02014"^^ . "43730488"^^ . . "\u30B0\u30EA\u30FC\u30BC180"@ja . . . . . "Gliese 180"@en . . . "24.329"^^ . "0.14"^^ . . . . "\u30B0\u30EA\u30FC\u30BC180 (\u82F1\u8A9E: Gliese 180\uFF09\u306F\u3001\u30B0\u30EA\u30FC\u30BC180b \u3068 \u30B0\u30EA\u30FC\u30BC180c\u306E2\u3064\u306E\u592A\u967D\u7CFB\u5916\u60D1\u661F\u3092\u6301\u3064\u8D64\u8272\u77EE\u661F\u3067\u3042\u308B\u3002\u5730\u7403\u304B\u3089\u306F\u7D0439\u5149\u5E74\u96E2\u308C\u3066\u3044\u308B\u3002"@ja . . . "1118116117"^^ . . . . . "0.11"^^ . "Gliese 180 (auch GJ 180) ist ein Roter Zwerg im Sternbild Eridanus, der rund 39 Lichtjahre von der Sonne entfernt ist. Der Stern besitzt mutma\u00DFlich ein Planetensystem mit zwei bekannten Exoplaneten. Wie alle Roten Zwerge ist Gliese 180 deutlich masse\u00E4rmer und leuchtschw\u00E4cher als die Sonne. Seine Masse betr\u00E4gt 43 % der Sonnenmasse, seine Leuchtkraft 1,3 % der Sonnenleuchtkraft."@de . . . . "\u0413\u043B\u0438\u0437\u0435 180 (\u0442\u0430\u043A\u0436\u0435 GJ 180) \u2014 \u043E\u0434\u0438\u043D\u043E\u0447\u043D\u0430\u044F \u0437\u0432\u0435\u0437\u0434\u0430 \u0432 \u0441\u043E\u0437\u0432\u0435\u0437\u0434\u0438\u0438 \u042D\u0440\u0438\u0434\u0430\u043D\u0430. \u041D\u0430\u0445\u043E\u0434\u0438\u0442\u0441\u044F \u043D\u0430 \u0440\u0430\u0441\u0441\u0442\u043E\u044F\u043D\u0438\u0438 38 \u0441\u0432. \u043B\u0435\u0442 \u043E\u0442 \u0421\u043E\u043B\u043D\u0446\u0430. \u0413\u043B\u0438\u0437\u0435 180 \u044F\u0432\u043B\u044F\u0435\u0442\u0441\u044F \u043A\u0440\u0430\u0441\u043D\u044B\u043C \u043A\u0430\u0440\u043B\u0438\u043A\u043E\u043C \u0441\u043F\u0435\u043A\u0442\u0440\u0430\u043B\u044C\u043D\u043E\u0433\u043E \u043A\u043B\u0430\u0441\u0441\u0430 M2V. \u041C\u0430\u0441\u0441\u0430 \u0437\u0432\u0435\u0437\u0434\u044B \u2014 0,39 \u043C\u0430\u0441\u0441\u044B \u0421\u043E\u043B\u043D\u0446\u0430, \u0440\u0430\u0434\u0438\u0443\u0441 \u2014 0,42 \u0440\u0430\u0434\u0438\u0443\u0441\u0430 \u0421\u043E\u043B\u043D\u0446\u0430, \u0442\u0435\u043C\u043F\u0435\u0440\u0430\u0442\u0443\u0440\u0430 \u043F\u043E\u0432\u0435\u0440\u0445\u043D\u043E\u0441\u0442\u0438 \u2014 3562 K."@ru . . "0.103"^^ . . "408.571"^^ . . "Gliese 180 (often shortened to GJ 180), is a small red dwarf star in the equatorial constellation of Eridanus. It is invisible to the naked eye with an apparent visual magnitude of 10.9. The star is located at a distance of 39 light years from the Sun based on parallax, and is drifting closer with a radial velocity of \u221214.6 km/s. It has a high proper motion, traversing the sky at the rate of 0.765 arcseconds per year. The stellar classification of GJ 180 is catalogued as M2V or M3V, depending on the study, which indicates this is a dim red dwarf \u2013 an M-type main-sequence star that is generating energy by core hydrogen fusion. Reiners and associates (2012) do not consider it to be an active star. It is about five billion years old and is spinning with a projected rotational velocity of ~3 km/s, giving it a rotation period of about 65 days. The star has 43% of the Sun's mass and 42% of the radius of the Sun. It is radiating just 2.4% of the luminosity of the Sun from its photosphere at an effective temperature of 3,634 K."@en . . "404"^^ . . "0.309"^^ . . "GJ 180 appel\u00E9e \u00E9galement Gliese 180, est un syst\u00E8me plan\u00E9taire comprenant une \u00E9toile naine rouge de type M et comprenant deux plan\u00E8tes de type super-Terre GJ 180 b et GJ 180 c. Ces deux plan\u00E8tes ont \u00E9t\u00E9 d\u00E9couvertes en 2014 par la m\u00E9thode des vitesses radiales. Le syst\u00E8me se situe \u00E0 338,1 ann\u00E9es-lumi\u00E8re dans la constellation de l'Eridan."@fr . . "Gliese 180"@it . "1.549"^^ . . . . . "7.56"^^ . . . "Gliese 180"@es . "17.38"^^ . "0.02611"^^ . . . . . "106.3"^^ . . . . "14542"^^ . . . . . . . "GJ 180 llamada igualmente Gliese 180, es una estrella de tipo M, conocida para tener dos planetas GJ 180 b y GJ 180 c. Se ubica a 38 a\u00F1os-luz de la Tierra. Seg\u00FAn laboratorio de habitabilidad planetaria (PHL) a Puerto Rico, dos mundos en el sistema pueden estar clasificados como de los planetas potencialmente habitables. Sin embargo, el Dr Mikko Tuomi, de la Universidad brit\u00E1nica de Hertfordshire, cuyo equipo ha identificado los planetas, es en desacuerdo, declarando :"@es . "0.0313"^^ . . . . . . . "83.7182"^^ . "Gliese 180 (auch GJ 180) ist ein Roter Zwerg im Sternbild Eridanus, der rund 39 Lichtjahre von der Sonne entfernt ist. Der Stern besitzt mutma\u00DFlich ein Planetensystem mit zwei bekannten Exoplaneten. Wie alle Roten Zwerge ist Gliese 180 deutlich masse\u00E4rmer und leuchtschw\u00E4cher als die Sonne. Seine Masse betr\u00E4gt 43 % der Sonnenmasse, seine Leuchtkraft 1,3 % der Sonnenleuchtkraft."@de . "1.018"^^ . . . . "Gliese 180"@fr . . . . "Gliese 180 \u2013 gwiazda w gwiazdozbiorze Erydanu. Znajduje si\u0119 w odleg\u0142o\u015Bci oko\u0142o 39 lat \u015Bwietlnych od S\u0142o\u0144ca. Ma uk\u0142ad planetarny."@pl . "Gliese 180 (often shortened to GJ 180), is a small red dwarf star in the equatorial constellation of Eridanus. It is invisible to the naked eye with an apparent visual magnitude of 10.9. The star is located at a distance of 39 light years from the Sun based on parallax, and is drifting closer with a radial velocity of \u221214.6 km/s. It has a high proper motion, traversing the sky at the rate of 0.765 arcseconds per year."@en . . "Gliese 180"@sv . . "Gliese 180"@pl . . . "0.129"^^ . . . .