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36 Большой Медведицы — двойная звезда в се … 36 Большой Медведицы — двойная звезда в северном созвездии Большой Медведицы. Компонент А имеет видимую звёздную величину 4.82m, и, согласно шкале Бортля, видна невооружённым глазом как минимум на пригородном/городском небе (англ. Suburban/urban transition). Из измерений параллакса, полученных во время миссии Hipparcos, известно, что система удалена примерно на 41,7 св. лет (12,78 пк). Звезда наблюдается севернее 35° ю. ш., то есть севернее Буэнос-Айреса (35° ю. ш.), Кейптауна (34° ю. ш.) и Канберры (35° ю. ш.). Т.о. звезда наблюдается практически на всей территории обитаемой Земли, за исключением Антарктиды. Лучшее время наблюдения — февраль.рктиды. Лучшее время наблюдения — февраль.
, 36 Ursae Majoris, som är stjärnans Flamste … 36 Ursae Majoris, som är stjärnans Flamsteed-beteckning, är en dubbelstjärna belägen i den mellersta delen av stjärnbilden Stora björnen. Den har en skenbar magnitud på ca 4,82 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 78,3 mas, beräknas den befinna sig på ett avstånd på ca 42 ljusår (ca 13 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet av ca 8,5 km/s.iocentrisk radialhastighet av ca 8,5 km/s.
, 36 Ursae Majoris is a double star in the n … 36 Ursae Majoris is a double star in the northern constellation of Ursa Major. With an apparent visual magnitude of 4.8, it can be seen with the naked eye in suitable dark skies. Based upon parallax measurements, this binary lies at a distance of 42 light-years (13 parsecs) from Earth. The brighter star of the two is a solar analog—meaning it has physical properties that make it similar to the Sun. It has 10% more mass and a radius 17% larger than the Sun, with an estimated age of four billion years. The spectrum of this star matches a stellar classification of F8 V, which indicates this is a main sequence star that is generating energy at its core through the nuclear fusion of hydrogen. The energy is being radiated into space from its outer envelope at an effective temperature of 6,066 K. This gives the star the characteristic yellow-white hue of an F-type star. The fainter of the two stars has an apparent magnitude 8.86 and shares a common proper motion witIts spectral type of K7Ve indicates it is a red dwarf. Its has a mass 60% of the Sun's, a temperature of 4,132 K and a bolometric luminosity only 1% of the Sun's. 36 Ursae Majoris has a second companion with a magnitude of 11.44 located at an angular separation of 240.6″ along a position angle of 292°, as of 2004. It does not share the proper motion of the other two stars and is a more massive and luminous star but much further away.e and luminous star but much further away.
, 36 Ursae Majoris is een tweevoudige ster met een spectraalklasse van F8.V en M.V. De ster bevindt zich 42,22 lichtjaar van de zon.
, 36 Ursae Majoris è una stella di classe spettrale F8-V, distante 41,7 anni luce dal Sistema solare.
, 큰곰자리 36은 분광형 F8V의 주계열성이다. 이 별은 태양 질량의 1.2배에 반지름도 1.2배 더 크다. 나이는 20억 살 정도로 생각된다. 이 항성은 반성 NLTT 24505를 거느리고 있는데 분광형은 K7V에 1,500 천문단위 떨어져 있다. 광학적 이중성 큰곰자리 36 C는 주성에서 49,000 천문단위 떨어져 있고 분광형은 K2V이지만, 중력으로 묶여 있지는 않은 것으로 보인다.
, 36 Ursae Majoris (36 UMa) es una estrella … 36 Ursae Majoris (36 UMa) es una estrella en la constelación de la Osa Mayor de magnitud aparente +4,83. Se encuentra a 41,9 años luz del Sistema Solar. 36 Ursae Majoris es una estrella blanco-amarilla de tipo espectral F8V, una estrella semejante al Sol pero más caliente, con una temperatura efectiva de 6110 K.De un tamaño similar al Sol, se estima que su masa es un 12% mayor que la masa solar. Con una edad aproximada entre 2700 y 3390 millones de años, es unos 1500 millones de años más joven que el Sol.Tiene una metalicidad menor que la solar; distintos estudios sitúan este valor entre el 66 y el 83% del encontrado en el Sol. 36 Ursae Majoris forma un sistema binario amplio con Gliese 394 (HD 237903), enana naranja de tipo K7V y 4070 K de temperatura. De parecidas características a Groombridge 1618, es una estrella tenue con un 6% de la luminosidad solar y una masa de 0,69 masas solares. Visualmente a 123 segundos de arco de 36 Ursae Majoris, la separación real entre ambas estrellas es de al menos 2043 UA.e ambas estrellas es de al menos 2043 UA.
, 大熊座36，又名BD+56 1459，HD 90839、SAO 27670、HR 4112，是大熊座的一颗恒星，视星等为4.84，位于銀經154.29，銀緯51.7，其B1900.0坐标为赤經10h 24m 13.8s，赤緯+56° 51.7′ 36″。
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| rdfs:comment |
36 Ursae Majoris (36 UMa) es una estrella … 36 Ursae Majoris (36 UMa) es una estrella en la constelación de la Osa Mayor de magnitud aparente +4,83. Se encuentra a 41,9 años luz del Sistema Solar. 36 Ursae Majoris es una estrella blanco-amarilla de tipo espectral F8V, una estrella semejante al Sol pero más caliente, con una temperatura efectiva de 6110 K.De un tamaño similar al Sol, se estima que su masa es un 12% mayor que la masa solar. Con una edad aproximada entre 2700 y 3390 millones de años, es unos 1500 millones de años más joven que el Sol.Tiene una metalicidad menor que la solar; distintos estudios sitúan este valor entre el 66 y el 83% del encontrado en el Sol.el 66 y el 83% del encontrado en el Sol.
, 큰곰자리 36은 분광형 F8V의 주계열성이다. 이 별은 태양 질량의 1.2배에 반지름도 1.2배 더 크다. 나이는 20억 살 정도로 생각된다. 이 항성은 반성 NLTT 24505를 거느리고 있는데 분광형은 K7V에 1,500 천문단위 떨어져 있다. 광학적 이중성 큰곰자리 36 C는 주성에서 49,000 천문단위 떨어져 있고 분광형은 K2V이지만, 중력으로 묶여 있지는 않은 것으로 보인다.
, 大熊座36，又名BD+56 1459，HD 90839、SAO 27670、HR 4112，是大熊座的一颗恒星，视星等为4.84，位于銀經154.29，銀緯51.7，其B1900.0坐标为赤經10h 24m 13.8s，赤緯+56° 51.7′ 36″。
, 36 Ursae Majoris is een tweevoudige ster met een spectraalklasse van F8.V en M.V. De ster bevindt zich 42,22 lichtjaar van de zon.
, 36 Ursae Majoris, som är stjärnans Flamste … 36 Ursae Majoris, som är stjärnans Flamsteed-beteckning, är en dubbelstjärna belägen i den mellersta delen av stjärnbilden Stora björnen. Den har en skenbar magnitud på ca 4,82 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 78,3 mas, beräknas den befinna sig på ett avstånd på ca 42 ljusår (ca 13 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet av ca 8,5 km/s.iocentrisk radialhastighet av ca 8,5 km/s.
, 36 Ursae Majoris è una stella di classe spettrale F8-V, distante 41,7 anni luce dal Sistema solare.
, 36 Большой Медведицы — двойная звезда в се … 36 Большой Медведицы — двойная звезда в северном созвездии Большой Медведицы. Компонент А имеет видимую звёздную величину 4.82m, и, согласно шкале Бортля, видна невооружённым глазом как минимум на пригородном/городском небе (англ. Suburban/urban transition). Из измерений параллакса, полученных во время миссии Hipparcos, известно, что система удалена примерно на 41,7 св. лет (12,78 пк).алена примерно на 41,7 св. лет (12,78 пк).
, 36 Ursae Majoris is a double star in the n … 36 Ursae Majoris is a double star in the northern constellation of Ursa Major. With an apparent visual magnitude of 4.8, it can be seen with the naked eye in suitable dark skies. Based upon parallax measurements, this binary lies at a distance of 42 light-years (13 parsecs) from Earth. The fainter of the two stars has an apparent magnitude 8.86 and shares a common proper motion witIts spectral type of K7Ve indicates it is a red dwarf. Its has a mass 60% of the Sun's, a temperature of 4,132 K and a bolometric luminosity only 1% of the Sun's.olometric luminosity only 1% of the Sun's.
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36 Ursae Majoris
, 큰곰자리 36
, 天璇增一
, 36 Большой Медведицы
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