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ι Chamaeleontis, Latinized as Iota Chamaeleontis, is a single star in the southern circumpolar constellation of Chamaeleon. It is visible to the naked eye as a dim, yellow-white hued point of light, having an apparent magnitude of about 5.3. Based upon parallax measurements, this star is around 188 light years away from the Sun, but it is drifting closer with a radial velocity of −4 km/s.

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  • Iota Chamaeleontis (en)
  • Iota Chamaeleontis (pt)
  • Йота Хамелеона (ru)
  • Jota Chamaeleontis (sv)
  • 小斗六 (zh)
rdfs:comment
  • Iota Chamaeleontis (13 Chamaeleontis) é uma estrela na direção da constelação de Chamaeleon. Possui uma ascensão reta de 09h 24m 09.73s e uma declinação de −80° 47′ 13.9″. Sua magnitude aparente é igual a 5.34. Considerando sua distância de 184 anos-luz em relação à Terra, sua magnitude absoluta é igual a 1.58. Pertence à classe espectral F3/F5IV. (pt)
  • Jota Chamaeleontis (ι Chamaeleontis, förkortat Jota Cha, ι Cha) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den mellersta delen av stjärnbilden Kameleonten. Den har en skenbar magnitud på 5,36 och är knappt synlig för blotta ögat och endast där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 17,2 mas, beräknas den befinna sig på ett avstånd på ca 190 ljusår (ca 58 parsek) från solen. (sv)
  • 蝘蜓座ι,又名CP-80 350,HD 82554、SAO 258530、HR 3795,是蝘蜓座的一颗恒星,视星等为5.36,位于銀經295.18,銀緯-21.22,其B1900.0坐标为赤經9h 27m 29.2s,赤緯-80° -21.22′ 18″。 (zh)
  • ι Chamaeleontis, Latinized as Iota Chamaeleontis, is a single star in the southern circumpolar constellation of Chamaeleon. It is visible to the naked eye as a dim, yellow-white hued point of light, having an apparent magnitude of about 5.3. Based upon parallax measurements, this star is around 188 light years away from the Sun, but it is drifting closer with a radial velocity of −4 km/s. (en)
  • Йота Хамелеона (лат. ι Chamaeleontis) — одиночная звезда в южном приполярном созвездии Хамелеона. Видна невооружённым глазом как тусклая точка бело-жёлтого цвета с видимой звёздной величиной около 5,3. На основе измерения годичного звёздного параллакса получена оценка расстояния до звезды, равная 188 световым годам, при этом звезда приближается к Солнцу с лучевой скоростью −4 км/с. (ru)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Chamaeleon_IAU.svg
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absmag v
  • +1.52 (en)
appmag v
class
  • F3/5 III/V (en)
constell
epoch
metal fe
  • −0.04 (en)
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