HD 93083 b is an extrasolar planet orbiting the star HD 93083 in Antlia constellation. It is probably much less massive than Jupiter, although only the minimum mass is known. The planet's mean distance from the star is about half that of Earth, and the orbit is slightly eccentric. This planet is another discovery by the HARPS search team. Stability analysis reveals that the orbits of Earth-sized planets located in HD 93083 b's Trojan points would be stable for long periods of time.

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dbo:abstract
  • HD 93083 b ist ein Exoplanet, der den Hauptreihenstern HD 93083 alle 143,58 Tage umkreist. Auf Grund seiner hohen Masse wird angenommen, dass es sich um einen Gasplaneten handelt. (de)
  • HD 93083 b es un planeta extrasolar que orbita a la estrella HD 93083 en la constelación de Antlia. Es probablemente menos massivo que Júpiter (tiene 0,37 de su masa), sin embargo solamente su masa mínima es conocida. La distancia media del planeta a HD 93083 es de 0,477 UA, aproximadamente la mitad de la distancia de la Tierra al Sol. Su órbita es un poco excéntrica (0,14). El período orbital de HD 93083 b es aproximadamente de 143,58 días (0,3931 años). (es)
  • HD 93083 b – planeta pozasłoneczna typu gazowy olbrzym okrążająca gwiazdę HD 93083. Została odkryta w 2005 roku. (pl)
  • HD 93083 b é um planeta extrassolar que orbita a estrela HD 93083 na constelação de Antlia. É provavelmente menos massivo do que Júpiter (tem 0,37 de sua massa), porém somente sua massa mínima é conhecida. A distância média do planeta de HD 93083 é de 0,477 UA, aproximadamente a metade da distância da Terra ao Sol. Sua órbita é um pouco excêntrica (0,14). O período orbital de HD 93083 b é de cerca de 143,58 dias (0,3931 anos). (pt)
  • HD 93083 b是一個環繞唧筒座恆星HD 93083的太陽系外行星。雖然目前仍不知道它的質量下限,但可能遠低於木星。這顆行星和母恆星的平均距離大約是日地距離的一半,且軌道離心率稍高。該行星由智利拉西拉天文台的高精度徑向速度行星搜索器發現。 對該行星動力學穩定性分析顯示該行星軌道的L4或L5拉格朗日點可以讓體積相當於地球的行星常時間穩定存在。 (zh)
  • HD 93083 b - экзопланета - газовый гигант, вращающийся вокруг красного карлика HD 93083 в созвездии Насоса. Открыт методом доплеровской спектроскопии поисковой группой HARPS в 2005 году. (ru)
  • HD 93083 b is an extrasolar planet orbiting the star HD 93083 in Antlia constellation. It is probably much less massive than Jupiter, although only the minimum mass is known. The planet's mean distance from the star is about half that of Earth, and the orbit is slightly eccentric. This planet is another discovery by the HARPS search team. Stability analysis reveals that the orbits of Earth-sized planets located in HD 93083 b's Trojan points would be stable for long periods of time. (en)
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  • 333.500000 (xsd:double)
dbp:class
  • K2IV-V
dbp:constell
dbp:discoverers
  • Lovis et al.
dbp:discoveryDate
  • 2005-02-14 (xsd:date)
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  • Published
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  • >0.37
dbp:massEarth
  • >118
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  • 0.410000 (xsd:double)
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  • 143.580000 (xsd:double)
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  • 0.393100 (xsd:double)
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  • b
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  • 2453181.700000 (xsd:double)
dct:subject
http://purl.org/linguistics/gold/hypernym
rdf:type
rdfs:comment
  • HD 93083 b ist ein Exoplanet, der den Hauptreihenstern HD 93083 alle 143,58 Tage umkreist. Auf Grund seiner hohen Masse wird angenommen, dass es sich um einen Gasplaneten handelt. (de)
  • HD 93083 b es un planeta extrasolar que orbita a la estrella HD 93083 en la constelación de Antlia. Es probablemente menos massivo que Júpiter (tiene 0,37 de su masa), sin embargo solamente su masa mínima es conocida. La distancia media del planeta a HD 93083 es de 0,477 UA, aproximadamente la mitad de la distancia de la Tierra al Sol. Su órbita es un poco excéntrica (0,14). El período orbital de HD 93083 b es aproximadamente de 143,58 días (0,3931 años). (es)
  • HD 93083 b – planeta pozasłoneczna typu gazowy olbrzym okrążająca gwiazdę HD 93083. Została odkryta w 2005 roku. (pl)
  • HD 93083 b é um planeta extrassolar que orbita a estrela HD 93083 na constelação de Antlia. É provavelmente menos massivo do que Júpiter (tem 0,37 de sua massa), porém somente sua massa mínima é conhecida. A distância média do planeta de HD 93083 é de 0,477 UA, aproximadamente a metade da distância da Terra ao Sol. Sua órbita é um pouco excêntrica (0,14). O período orbital de HD 93083 b é de cerca de 143,58 dias (0,3931 anos). (pt)
  • HD 93083 b是一個環繞唧筒座恆星HD 93083的太陽系外行星。雖然目前仍不知道它的質量下限,但可能遠低於木星。這顆行星和母恆星的平均距離大約是日地距離的一半,且軌道離心率稍高。該行星由智利拉西拉天文台的高精度徑向速度行星搜索器發現。 對該行星動力學穩定性分析顯示該行星軌道的L4或L5拉格朗日點可以讓體積相當於地球的行星常時間穩定存在。 (zh)
  • HD 93083 b - экзопланета - газовый гигант, вращающийся вокруг красного карлика HD 93083 в созвездии Насоса. Открыт методом доплеровской спектроскопии поисковой группой HARPS в 2005 году. (ru)
  • HD 93083 b is an extrasolar planet orbiting the star HD 93083 in Antlia constellation. It is probably much less massive than Jupiter, although only the minimum mass is known. The planet's mean distance from the star is about half that of Earth, and the orbit is slightly eccentric. This planet is another discovery by the HARPS search team. Stability analysis reveals that the orbits of Earth-sized planets located in HD 93083 b's Trojan points would be stable for long periods of time. (en)
rdfs:label
  • HD 93083 b (de)
  • HD 93083 b (es)
  • HD 93083 b (fr)
  • HD 93083 b (pl)
  • HD 93083 b (en)
  • HD 93083 b (pt)
  • HD 93083 b (ru)
  • HD 93083 b (zh)
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