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Zeta Chamaeleontis, Latinized from ζ Chamaeleontis, is a star located in the constellation Chamaeleon. Located around 570 light-years distant, it shines with a luminosity approximately 522 times that of the Sun and has a surface temperature of 15,655 K. South African Astronomer A.W.J. Cousins noted it to vary between magnitudes 5.06 and 5.17 in 1960. It was classified as a Beta Cephei variable in the Hipparcos and Tycho Catalogues (ESA 1997), with a period of 1.07 days, before being reclassified as a slowly pulsating B star in the 2011 version. It is also an eclipsing binary star, with a period of 2.7 days.

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rdf:type
rdfs:label
  • Zeta Chamaeleontis (pt)
  • Дзета Хамелеона (ru)
  • Zeta Chamaeleontis (en)
  • Zeta Chamaeleontis (sv)
  • 小斗五 (zh)
rdfs:comment
  • Zeta Chamaeleontis (ζ Chamaeleontis, förkortat Zeta Cha, ζ Cha), som är stjärnans Bayer-beteckning, är en ensam stjärna i den mellersta delen av stjärnbilden Kameleonten. Den har en skenbar magnitud på +5,06 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätningar i Hipparcos-uppdraget på 5,7 mas beräknas den befinna sig på ca 570 ljusårs (175 parsek) avstånd från solen. (sv)
  • Zeta Chamaeleontis (14 Chamaeleontis) é uma estrela na direção da constelação de Chamaeleon. Possui uma ascensão reta de 09h 33m 53.51s e uma declinação de −80° 56′ 28.7″. Sua magnitude aparente é igual a 5.07. Considerando sua distância de 539 anos-luz em relação à Terra, sua magnitude absoluta é igual a −1.02. Pertence à classe espectral B5V. É uma estrela variável. (pt)
  • 蝘蜓座ζ,又名CP-80 365,HD 83979、SAO 258538、HR 3860,是蝘蜓座的一颗恒星,视星等为5.11,位于銀經295.57,銀緯-21.04,其B1900.0坐标为赤經9h 36m 50.1s,赤緯-80° -21.04′ 31″。 (zh)
  • Zeta Chamaeleontis, Latinized from ζ Chamaeleontis, is a star located in the constellation Chamaeleon. Located around 570 light-years distant, it shines with a luminosity approximately 522 times that of the Sun and has a surface temperature of 15,655 K. South African Astronomer A.W.J. Cousins noted it to vary between magnitudes 5.06 and 5.17 in 1960. It was classified as a Beta Cephei variable in the Hipparcos and Tycho Catalogues (ESA 1997), with a period of 1.07 days, before being reclassified as a slowly pulsating B star in the 2011 version. It is also an eclipsing binary star, with a period of 2.7 days. (en)
  • Дзета Хамелеона (лат. Zeta Chamaeleontis) — звезда в созвездии Хамелеона на расстоянии около 570 световых лет от Солнца. Звезда приближается к Солнцу с лучевой скоростью около 42 км/с. Дзета Хамелеона обладает светимостью около 522 светимостей Солнца при температуре поверхности около 13544 K. Южноафриканский астроном А. В. Дж. Казинс в 1960 году заметил, что у звезды меняется видимая звёздная величина от 5,06 до 5,17. Дзету Хамелеона относят к переменным звёздам типа Беты Цефея, такой тип переменности указан в каталогах Hipparcos и Tycho (ESA 1997), период переменности составляет 1,07 суток, но в версии каталогов от 2011 года звезду отнесли к медленно пульсирующим переменным спектрального класса B. (ru)
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  • ζ Chamaeleontis (en)
foaf:depiction
  • http://commons.wikimedia.org/wiki/Special:FilePath/ZetaChaLightCurve.png
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absmag v
  • −1.15 (en)
age myr
appmag v
class
  • B5V (en)
constell
epoch
  • J2000 (en)
gravity
luminosity
mass
metal fe
  • −0.31 (en)
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