. . . . "4.82"^^ . . . "90.1264"^^ . . "+0.875"@en . . "InternetArchiveBot"@en . "HR 6806 is een oranje dwerg met een spectraalklasse van K2.V. De ster bevindt zich 36,19 lichtjaar van de zon."@nl . . . . "HR 6806"@es . "HR 6806"@ko . . "HR 6806 je hv\u011Bzda spektr\u00E1ln\u00EDho typu K2, vzd\u00E1len\u00E1 od Zem\u011B 36,0 ly. Jedn\u00E1 se o oran\u017Eov\u00E9ho trpasl\u00EDka, kter\u00FD se nach\u00E1z\u00ED v souhv\u011Bzd\u00ED Herkula. Radi\u00E1ln\u00ED rychlost hv\u011Bzdy \u010Din\u00ED p\u0159ibli\u017En\u011B 19,5 km/s."@cs . . . . "yes"@en . . . . "J2000"@en . "+0.585"@en . . "HD 166620\uFF0C\u53C8\u540DBD+38 3095\uFF0CSAO 66700\u3001HR 6806\uFF0C\u662F\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A6.4\uFF0C\u4F4D\u4E8E\u9280\u7D9365.34\uFF0C\u9280\u7DEF24.21\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D9318h 6m 18.7s\uFF0C\u8D64\u7DEF+38\u00B0 24.21\u2032 5\u2033\u3002"@zh . "3628800.0"^^ . . "HR 6806"@en . . . . "HD 166620 ( eller HR 6806) \u00E4r en ensam stj\u00E4rna i det mellersta omr\u00E5det av stj\u00E4rnbilden Herkules. Den har en skenbar magnitud av ca 6,40 och \u00E4r mycket svagt synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallax enligt Gaia Data Release 2 p\u00E5 ca 90,1 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 36 ljus\u00E5r (ca 11 parsek) fr\u00E5n solen. Den r\u00F6r sig n\u00E4rmare solen med en heliocentrisk radialhastighet p\u00E5 ca -19 km/s."@sv . . . . . . . . . . . . "4"^^ . "HD 166620\uFF0C\u53C8\u540DBD+38 3095\uFF0CSAO 66700\u3001HR 6806\uFF0C\u662F\u4E00\u9897\u6052\u661F\uFF0C\u89C6\u661F\u7B49\u4E3A6.4\uFF0C\u4F4D\u4E8E\u9280\u7D9365.34\uFF0C\u9280\u7DEF24.21\uFF0C\u5176B1900.0\u5750\u6807\u4E3A\u8D64\u7D9318h 6m 18.7s\uFF0C\u8D64\u7DEF+38\u00B0 24.21\u2032 5\u2033\u3002"@zh . . . . "HR 6806 (HD 166620 / HIP 88972 / GJ 706)\u200B es una estrella de magnitud aparente +6,37. Se localiza en la constelaci\u00F3n de H\u00E9rcules 3\u00BA al noroeste de \u03B8 Herculis.Se encuentra a 36,2 a\u00F1os luz del Sistema Solar, siendo , a poco m\u00E1s de un a\u00F1o luz, la estrella m\u00E1s pr\u00F3xima a HR 6806.\u200B HR 6806 es una enana naranja de tipo espectral K2V con una temperatura efectiva de 5019 K.Su luminosidad corresponde al 35% de la que tiene el Sol y tiene un di\u00E1metro igual al 79% del di\u00E1metro solar.En cuanto a su metalicidad \u2014abundancia relativa de elementos m\u00E1s pesados que el helio\u2014, parece ser menor que la solar; diversos estudios se\u00F1alan una abundancia relativa de hierro equivalente al 66% de la existente en el Sol,\u200B tendencia tambi\u00E9n observada en elementos como n\u00EDquel, silicio y sodio.\u200B La masa de HR 6806 es de aproximadamente 2/3 de la masa solar.Su edad, teniendo en cuenta par\u00E1metros cromosf\u00E9ricos, es de 4750 - 5000 millones de a\u00F1os,\u200B\u200B no muy distinta de la estimada por girocronolog\u00EDa \u2014basada en su per\u00EDodo de rotaci\u00F3n de 42,4 d\u00EDas\u2014, que es de 5300 millones de a\u00F1os.\u200B"@es . . . . "HR 6806 is a solitary, orange, main sequence, and Sun-like (K2 V) star located thirty-six light-years away, in the constellation Hercules. The star is smaller than the Sun, with around 79% of the solar mass and radius, and 35% of the solar luminosity. It appears to be rotating slowly with an estimated period of 42 days. In 1988, it was noticed that the star had an inactive chromosphere, with a surface magnetic field strength of only 1,500 G. From 1990 activity in the chromosphere increased, inline with a 16 year stellar cycle previously observed. But, sometime after 1994 (exact date unknown because of a data collection gap between 1995 and 2004) chromospheric activity greatly reduced, and has stayed flat for more than 16 years. As of 2022, the star appears to have entered the equivalent of"@en . . . . . . . . . "HR 6806 is een oranje dwerg met een spectraalklasse van K2.V. De ster bevindt zich 36,19 lichtjaar van de zon."@nl . "4900"^^ . "HR 6806 (HD 166620 / HIP 88972 / GJ 706)\u200B es una estrella de magnitud aparente +6,37. Se localiza en la constelaci\u00F3n de H\u00E9rcules 3\u00BA al noroeste de \u03B8 Herculis.Se encuentra a 36,2 a\u00F1os luz del Sistema Solar, siendo , a poco m\u00E1s de un a\u00F1o luz, la estrella m\u00E1s pr\u00F3xima a HR 6806.\u200B La masa de HR 6806 es de aproximadamente 2/3 de la masa solar.Su edad, teniendo en cuenta par\u00E1metros cromosf\u00E9ricos, es de 4750 - 5000 millones de a\u00F1os,\u200B\u200B no muy distinta de la estimada por girocronolog\u00EDa \u2014basada en su per\u00EDodo de rotaci\u00F3n de 42,4 d\u00EDas\u2014, que es de 5300 millones de a\u00F1os.\u200B"@es . "K2 V"@en . "0.35"^^ . . . . . . . . . "\u2212468.214"@en . . . . . . . . "HR 6806"@cs . . . "January 2018"@en . "HR 6806\uC740 \uBD84\uAD11\uD615 K2V\uC758 \uC8FC\uACC4\uC5F4\uC131\uC73C\uB85C \uB2E8\uB3C5\uC131\uC774\uC790 \uC624\uB80C\uC9C0\uC0C9 \uC65C\uC131\uC774\uBA70, \uC9C0\uAD6C\uC5D0\uC11C \uD5C8\uD058\uB9AC\uC2A4\uC790\uB9AC \uBC29\uD5A5\uC73C\uB85C 36\uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4."@ko . . "HD 166620 ( eller HR 6806) \u00E4r en ensam stj\u00E4rna i det mellersta omr\u00E5det av stj\u00E4rnbilden Herkules. Den har en skenbar magnitud av ca 6,40 och \u00E4r mycket svagt synlig f\u00F6r blotta \u00F6gat d\u00E4r ljusf\u00F6roreningar ej f\u00F6rekommer. Baserat p\u00E5 parallax enligt Gaia Data Release 2 p\u00E5 ca 90,1 mas, ber\u00E4knas den befinna sig p\u00E5 ett avst\u00E5nd p\u00E5 ca 36 ljus\u00E5r (ca 11 parsek) fr\u00E5n solen. Den r\u00F6r sig n\u00E4rmare solen med en heliocentrisk radialhastighet p\u00E5 ca -19 km/s."@sv . . . "HR 6806 je hv\u011Bzda spektr\u00E1ln\u00EDho typu K2, vzd\u00E1len\u00E1 od Zem\u011B 36,0 ly. Jedn\u00E1 se o oran\u017Eov\u00E9ho trpasl\u00EDka, kter\u00FD se nach\u00E1z\u00ED v souhv\u011Bzd\u00ED Herkula. Radi\u00E1ln\u00ED rychlost hv\u011Bzdy \u010Din\u00ED p\u0159ibli\u017En\u011B 19,5 km/s."@cs . . . "HR 6806"@nl . "0.02"^^ . . "HR 6806"@en . "15059534"^^ . "6.4"^^ . "4.53"^^ . "HR 6806 is a solitary, orange, main sequence, and Sun-like (K2 V) star located thirty-six light-years away, in the constellation Hercules. The star is smaller than the Sun, with around 79% of the solar mass and radius, and 35% of the solar luminosity. It appears to be rotating slowly with an estimated period of 42 days. In 1988, it was noticed that the star had an inactive chromosphere, with a surface magnetic field strength of only 1,500 G. From 1990 activity in the chromosphere increased, inline with a 16 year stellar cycle previously observed. But, sometime after 1994 (exact date unknown because of a data collection gap between 1995 and 2004) chromospheric activity greatly reduced, and has stayed flat for more than 16 years. As of 2022, the star appears to have entered the equivalent of a Maunder minimum. The star is around six billion years of age. There was suspected to be a nearby very cool, and very dim, T9 to Y brown dwarf companion, WISE J180901.07+383805.4, at an angular separation of 769\u2033, which would have corresponded to a projected separation of 8460 AU at the distance of HR 6806. However, with further observation it was found to be bluer than at first thought and more typical of a slightly brighter T7 dwarf, which would place it at a much greater distance of 91 ly (28 pc)\u2014ruling out a physical association. This is confirmed by the differing proper motion of the star and this object."@en . . . "\u2212316.520"@en . . "9103"^^ . "\u22120.61"@en . "6.17"^^ . "HR 6806\uC740 \uBD84\uAD11\uD615 K2V\uC758 \uC8FC\uACC4\uC5F4\uC131\uC73C\uB85C \uB2E8\uB3C5\uC131\uC774\uC790 \uC624\uB80C\uC9C0\uC0C9 \uC65C\uC131\uC774\uBA70, \uC9C0\uAD6C\uC5D0\uC11C \uD5C8\uD058\uB9AC\uC2A4\uC790\uB9AC \uBC29\uD5A5\uC73C\uB85C 36\uAD11\uB144 \uB5A8\uC5B4\uC838 \uC788\uB2E4."@ko . . "ARICNS: 01473"@en . . . "5.8"^^ . . . . . "HD 166620"@zh . "1086360299"^^ . . . . "HD 166620"@sv .