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南極座λ，又名CP-83 722，HD 206240、SAO 258914、HR 8280，是南極座的一颗恒星，视星等为5.29，位于銀經309.02，銀緯-32.13，其B1900.0坐标为赤經21h 35m 36.4s，赤緯-83° -32.13′ 44″。
, λ Octantis, Latinized as Lambda Octantis, … λ Octantis, Latinized as Lambda Octantis, is a binary star system in the southern circumpolar constellation of Octans. It is visible to the naked eye as a dim point of light with a combined apparent visual magnitude of 5.27. The distance to this system is approximately 398–409 light years, based on parallax, but it is moving closer with a radial velocity of −10 km/s. The primary, designated component A, is an aging, yellow-hued star with a stellar classification of class G8-K0III and a visual magnitude of 5.64. Having exhausted the supply of hydrogen at its core, it has expanded and cooled off the main sequence, becoming a giant. At present it is about 200 million years old and has 13 times the girth of the Sun. This star is radiating 102 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 5,048 K. The magnitude 7.25 secondary companion, component B, is an Am star with a class of kA3hA7VmA8. This notation indicates it has the calcium K line of an A3 class star, the hydrogen lines of a cooler A7 main sequence star, and the metal lines of an A8 star. As of 2008, it lies at an angular separation of 3.233″ from the primary.lar separation of 3.233″ from the primary.
, HD206241 — хімічно пекулярна зоря спектрального класу A3, що має видиму зоряну величину в смузі V приблизно 7,3.Вона розташована на відстані близько 435,5 світлових років від Сонця.
, Lambda Octantis (λ Octantis, förkortat Lam … Lambda Octantis (λ Octantis, förkortat Lambda Oct, λ Oct) som är stjärnans Bayerbeteckning, är en dubbelstjärna belägen i den inre delen av stjärnbilden Oktanten. Den har en skenbar magnitud på 5,27 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. ca 410 ljusår (ca 125 parsek) från solen.
, Lambda Octantis (62 Octantis) é uma estrel … Lambda Octantis (62 Octantis) é uma estrela na direção da constelação de Octans. Possui uma ascensão reta de 21h 50m 54.25s e uma declinação de −82° 43′ 07.8″. Sua magnitude aparente é igual a 5.27. Considerando sua distância de 435 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.36. Pertence à classe espectral G8/K0III+.... Pertence à classe espectral G8/K0III+...
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Lambda Octantis (λ Octantis, förkortat Lam … Lambda Octantis (λ Octantis, förkortat Lambda Oct, λ Oct) som är stjärnans Bayerbeteckning, är en dubbelstjärna belägen i den inre delen av stjärnbilden Oktanten. Den har en skenbar magnitud på 5,27 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. ca 410 ljusår (ca 125 parsek) från solen.
, λ Octantis, Latinized as Lambda Octantis, … λ Octantis, Latinized as Lambda Octantis, is a binary star system in the southern circumpolar constellation of Octans. It is visible to the naked eye as a dim point of light with a combined apparent visual magnitude of 5.27. The distance to this system is approximately 398–409 light years, based on parallax, but it is moving closer with a radial velocity of −10 km/s.closer with a radial velocity of −10 km/s.
, 南極座λ，又名CP-83 722，HD 206240、SAO 258914、HR 8280，是南極座的一颗恒星，视星等为5.29，位于銀經309.02，銀緯-32.13，其B1900.0坐标为赤經21h 35m 36.4s，赤緯-83° -32.13′ 44″。
, Lambda Octantis (62 Octantis) é uma estrel … Lambda Octantis (62 Octantis) é uma estrela na direção da constelação de Octans. Possui uma ascensão reta de 21h 50m 54.25s e uma declinação de −82° 43′ 07.8″. Sua magnitude aparente é igual a 5.27. Considerando sua distância de 435 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.36. Pertence à classe espectral G8/K0III+.... Pertence à classe espectral G8/K0III+...
, HD206241 — хімічно пекулярна зоря спектрального класу A3, що має видиму зоряну величину в смузі V приблизно 7,3.Вона розташована на відстані близько 435,5 світлових років від Сонця.
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, Lambda Octantis
, HD206241
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