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HD 183263 b is an extrasolar planet orbiting the star HD 183263. This planet has a minimum mass of 3.6 times more than Jupiter and takes 625 days to orbit the star. The planet was discovered on January 25, 2005 using multiple Doppler measurements of five nearby FGK main-sequence stars and subgiants obtained during the past 4–6 years at the Keck Observatory in Mauna Kea, Hawaii. These stars, namely, HD 183263, HD 117207, HD 188015, HD 45350, and HD 99492, all exhibit coherent variations in their Doppler shifts consistent with a planet in Keplerian motion, and the results were published in a paper by Geoffrey Marcy et al. Photometric observations were acquired for four of the five host stars with an automatic telescope at Fairborn Observatory. The lack of brightness variations in phase with

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  • HD 183263 b (ar)
  • HD 183263 b (de)
  • HD 183263 b (en)
  • HD 183263 b (es)
  • HD 183263 b (fr)
  • HD 183263 b (in)
  • HD 183263 b (ko)
  • HD 183263 b (ru)
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  • HD 183263 b (بالإنجليزية: HD 183263 b)‏ الذي يرمز له بالرمز HD 183263b، هو كوكب خارج المجموعة الشمسية، في كوكبة العقاب، يتبع ‏. (ar)
  • HD 183263 b ist ein Exoplanet, der den gelben Unterriesen HD 183263 alle 635,4 Tage umkreist. Er wurde von Geoffrey Marcy et al. im Jahr 2004 mit Hilfe der Radialgeschwindigkeitsmethode entdeckt. (de)
  • HD 183263 b adalah sebuah planet luar surya yang terletak sekitar 177,04 tahun cahaya dari Bumi. Planet ini ditemukan pada tahun 2004 dengan menggunakan metode kecepatan radial. HD 183263 b memiliki massa sebesar 3,95 massa Jupiter. (in)
  • HD 183263 b est une exoplanète orbitant autour de l'étoile HD 183263 ; elle a été découverte en 2004. (fr)
  • HD 183263 b는 지구에서 보았을 때 어머니 항성 으로부터 각거리 28.8 밀리초각만큼 떨어져 있는 외계 행성이다. 항성과 지구 사이 거리를 고려하면 이 간격은 실제로 1.52 천문단위에 해당한다(이는 화성 궤도 반지름과 비슷하다). 최소 질량은 목성의 3.69배, 1회 공전 주기는 1.7364년이다. 2005년 1월 25일 미국 하와이주 켁 천문대 망원경을 이용, 도플러 효과를 응용하여 발견했다. 켁 천문대에서는 수 년 전부터 5개의 지구 근처 주계열성과 준거성들을 연구해 왔다. 구체적으로 연구 대상이 된 항성들은 HD 183263, , , , 이다. 이들 다섯 별들은 케플러 운동 관점에서 행성을 거느리고 있다고 믿기에 충분한, 의미 있는 시선 속도 변화량을 보여준다. 이 연구 결과는 제프리 마시 연구진이 집필했다. 5개 별들 중 4개 별들에 대해 페어본 천문대 자동 망원경을 이용, 측광학적 관측을 실시했다. (ko)
  • HD 183263 b — экзопланета, находящаяся в созвездии Орла на расстоянии около 180 световых лет (55 парсек) от Солнца. Одна из двух планет, открытых у жёлтого субгиганта HD 183263, имеющего массу 1,17 масс Солнца и диаметр 1,21 диаметра Солнца. Открыта в 2005 году методом Доплеровской спектроскопии. HD 183263 b это газовый гигант (прохладный юпитер) с массой 3,73 массы Юпитера. Обращается на расстоянии около 2 а. е. от материнской звезды, совершая полный оборот за 624 дня. Большая полуось орбиты (a) — 1.51±0,087 а. е. Эксцентриситет орбиты (e) — 0,357±0,09. (ru)
  • HD 183263 b is an extrasolar planet orbiting the star HD 183263. This planet has a minimum mass of 3.6 times more than Jupiter and takes 625 days to orbit the star. The planet was discovered on January 25, 2005 using multiple Doppler measurements of five nearby FGK main-sequence stars and subgiants obtained during the past 4–6 years at the Keck Observatory in Mauna Kea, Hawaii. These stars, namely, HD 183263, HD 117207, HD 188015, HD 45350, and HD 99492, all exhibit coherent variations in their Doppler shifts consistent with a planet in Keplerian motion, and the results were published in a paper by Geoffrey Marcy et al. Photometric observations were acquired for four of the five host stars with an automatic telescope at Fairborn Observatory. The lack of brightness variations in phase with (en)
  • HD 183263 b es un planeta extrasolar que órbita la estrella . Este planeta tiene una masa mínima de 3,69 veces más que Júpiter y tarda 1,7364 años para órbitar su estrella. El planeta fue descubierto el 25 de enero de 2005 utilizando varias mediciones Doppler de cinco estrellas cercanas FGK de secuencia principal y subgigantes obtenidos durante los últimos 4-6 años en el Observatorio Keck en Mauna Kea, Hawái. Estas estrellas, a saber, HD 183263, , HD 188015, , y HD 99492, todas exhiben variaciones de exposición coherente con sus desplazamientos Doppler consistentes con un planeta en movimiento Keplerianos y los resultados fueron publicados en un artículo de Geoffrey Marcy et al. Observaciones fotométricas fueron adquiridas para cuatro de las cinco estrellas de huésped con un telescopio aut (es)
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  • HD 183263 b (en)
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  • HD 183263 b (en)
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