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Statements

Subject Item
dbr:Epsilon_Cir
dbo:wikiPageWikiLink
dbr:Epsilon_Circini
dbo:wikiPageRedirects
dbr:Epsilon_Circini
Subject Item
dbr:Epsilon_Circini
rdf:type
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rdfs:label
Epsilon Circini Epsilon Circini Эпсилон Циркуля Epsilon Circini
rdfs:comment
Epsilon Circini (ε Circini, ε Cir) é uma estrela na constelação de Circinus. Com uma magnitude aparente de 4,85, é a quarta estrela mais brilhante da constelação, sendo visível a olho nu em boas condições de visualização. Sua distância da Terra, calculada com base em medições de paralaxe, é de aproximadamente 428 anos-luz (131 parsecs). De sua magnitude aparente e distância, calcula-se uma magnitude absoluta visual de -0,7. Epsilon Circini(ε Circini, förkortat, Epsilon Cir, ε Cir), som är stjärnans Bayer-beteckning, är en ensam stjärna med en skenbar magnitud 4,86 i den östra delen av Cirkelpassarens stjärnbild och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 8,0 mas, beräknas den befinna sig på ett avstånd på ca 410 ljusår (ca 125 parsek) från solen. Эпсилон Циркуля (англ. Epsilon Circini, ε Cir), ε Циркуля — одиночная звезда в созвездии Циркуля. Плохо видна невооружённым глазом, видимая звёздная величина составляет 4,86. Расстояние до звезды, определённое по измерению годичного параллакса, равного 8.00 мсд, составляет около 410 световых лет. Epsilon Circini, Latinized from ε Circini, is a solitary star located in the southern constellation of Circinus. It is faintly visible to the naked eye, having an apparent visual magnitude of 4.86. The distance to this star, as determined by a measured annual parallax shift of 7.63 mas, is around 428 light years. It is drifting closer to the Sun with a radial velocity of −4 km/s.
foaf:name
ε Circini
dcterms:subject
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dbo:wikiPageID
36034307
dbo:wikiPageRevisionID
1079518222
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dbt:Reflist dbt:Odlist dbt:Short_description dbt:Stars_of_Circinus dbt:DEC dbt:RA dbt:Starbox_observe dbt:Starbox_detail dbt:Starbox_end dbt:Starbox_character dbt:Starbox_begin dbt:Starbox_catalog dbt:Starbox_astrometry dbt:Starbox_reference dbt:Val
dbp:absmagV
−0.63
dbp:appmagV
4.86
dbp:class
K2.5 III
dbp:constell
dbr:Circinus
dbp:epoch
dbr:J2000.0
dbp:equinox
J2000.0
dbp:pError
0.1503
dbp:parallax
7.6263
dbp:propMoDec
+8.728
dbp:propMoRa
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dbp:uB
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dbo:abstract
Epsilon Circini, Latinized from ε Circini, is a solitary star located in the southern constellation of Circinus. It is faintly visible to the naked eye, having an apparent visual magnitude of 4.86. The distance to this star, as determined by a measured annual parallax shift of 7.63 mas, is around 428 light years. It is drifting closer to the Sun with a radial velocity of −4 km/s. This is an evolved K-type giant star with a stellar classification of K2.5 III. With the supply of hydrogen at its core exhausted, the star has cooled and expanded to 28.5 times the girth of the Sun. It radiates about 290 times the solar luminosity from its photosphere at an effective temperature of 4,457 K. Epsilon Circini (ε Circini, ε Cir) é uma estrela na constelação de Circinus. Com uma magnitude aparente de 4,85, é a quarta estrela mais brilhante da constelação, sendo visível a olho nu em boas condições de visualização. Sua distância da Terra, calculada com base em medições de paralaxe, é de aproximadamente 428 anos-luz (131 parsecs). De sua magnitude aparente e distância, calcula-se uma magnitude absoluta visual de -0,7. Epsilon Circini é uma estrela gigante com um tipo espectral de K2.5 III e temperatura efetiva de 4 600 K, portanto possui coloração alaranjada. Seu diâmetro angular é de 2,02 milissegundos de arco, o que corresponde a um raio de 28,5 vezes o raio solar. Não possui estrelas companheiras conhecidas. Epsilon Circini(ε Circini, förkortat, Epsilon Cir, ε Cir), som är stjärnans Bayer-beteckning, är en ensam stjärna med en skenbar magnitud 4,86 i den östra delen av Cirkelpassarens stjärnbild och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 8,0 mas, beräknas den befinna sig på ett avstånd på ca 410 ljusår (ca 125 parsek) från solen. Эпсилон Циркуля (англ. Epsilon Circini, ε Cir), ε Циркуля — одиночная звезда в созвездии Циркуля. Плохо видна невооружённым глазом, видимая звёздная величина составляет 4,86. Расстояние до звезды, определённое по измерению годичного параллакса, равного 8.00 мсд, составляет около 410 световых лет. Данная звезда представляет собой звезду-гигант спектрального класса K (K2.5 III). Измеренный угловой диаметр звезды составляет 2,02 ± 0,11 мсд. Если учесть оценку расстояния, физические размеры звезды в 27 раз превосходят Солнце по радиусу. Звезда обладает светимостью, в 244 раза превышающей солнечную, эффективная температура поверхности составляет 4576 K.
gold:hypernym
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dbr:Table_of_stars_with_Bayer_designations
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dbr:List_of_stars_in_Circinus
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dbr:Ε_Circini
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