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HD 209458 b will not evaporate entirely, although it may have lost up to about 7% of its mass over its estimated lifetime of 5 billion years. De planeet werd op 5 oktober 2005 ontdekt nadat Franse astronomen de overgang van de planeet observeerden. Hallo, Inloggen. HD 209458 b is a gas giant exoplanet that orbits a F-type star. HD 209458 b (sometimes though unofficially named Osiris) is an extrasolar planet that orbits the Solar analog star HD 209458 in the constellation Pegasus, some 150 light-years from Earth's solar system. HD 209458 b is an extrasolar planet that orbits the Sun-like star HD 209458 in the constellation Pegasus, some 150 light-years from Earth's solar system, with evidence of water vapor.[1]. HD 209458 b is an extrasolar planet (unofficially referred to as Osiris) that orbits the Solar analog star HD 209458 in the constellation Pegasus, some 150 light-years from Earth's solar system, with evidence of water vapor. HD 209458b is a hot Jovian planet orbiting the HD 209458 at 156 light years from Earth, it orbits very close to the star, only 7 million kilometers, which is very little and takes only 3.5 days to complete an orbit at a temperature of 1000 degrees, and with a large volume, twice the mass of Jupiter and slightly larger.. HD 209458 b is 159 light years away from Earth. HD 209458 b is an extrasolar planet (unofficially referred to as Osiris) that orbits the Solar analog star HD 209458 in the constellation Pegasus, some 150 light-years from Earth's solar system, with evidence of water vapor. Het laatste nieuws met duiding van redacteuren, achtergronden, columns, opinie, wetenschap, en recensies van kunst & cultuur door de Volkskrant. Hd 209458 B: Miller, Frederic P.: Amazon.nl Selecteer uw cookievoorkeuren We gebruiken cookies en vergelijkbare tools om uw winkelervaring te verbeteren, onze services aan te bieden, te begrijpen hoe klanten onze services gebruiken zodat we verbeteringen … It orbits HD 209458 in the constellation Pegasus.It is approximately 159 light years from the Solar System.A year on HD 209458 b is 3.5 Earth days. HD 209458 b (sometimes unofficially called Osiris) is an exoplanet that orbits the solar analog HD 209458 in the constellation Pegasus, some 150 light-years from the Solar System. HD 209458 b, Osiris genaamd is op 5 november 1999 ontdekt en is de eerste planeet buiten het zonnestelsel die door de mens is waargenomen volgens de transit-methode.De planeet is naar de Egyptische god Osiris genoemd en draait om de ster HD 209458.Osiris ligt meer dan 150 lichtjaren verwijderd van de aarde. Spectroscopic studies first revealed the presence of a planet around HD 209458 on November 5, 1999. The planet is now under even more public scrutiny with … HD 189733 b is the second planet after HD 209458 b for which atmospheric evaporation has been detected. HD 209458 b; Alternative planet names: TYC 1688-1821-1 b, Gaia DR2 1779546757669063552 b, HIP 108859 b: Description: By studying the carbon monoxide gas in the upper atmosphere with great accuracy, astronomers found evidence for a wind, blowing at a speed of 5000 to 10000 km per hour. Den HD 209458 b ass en Exoplanéit, deen 150 Liichtjoer vun eiser Äerd ewech läit. Ga naar primaire content.nl. El radi de l'òrbita del planeta és de 7 milions de quilòmetres, unes 0,047 unitats astronòmiques, o una vuitena part del radi de l'òrbita de Mercuri. Op 27 november 2001 is door de beelden van de Hubble ruimtetelescoop … The radius of the planet's orbit is 7 million kilometres, about 0.047 astronomical units, … HD 209458 b merupakan sebuah planet ekstrasurya yang mengorbit bintang HD 209458 dalam rasi Pegasus, kira-kira 150 tahun cahaya dari Tata Surya.HD 209458 merupakan bintang bermagnitudo 8, dan dapat dilihat dari Bumi menggunakan teropong.. Radius orbit planet ini ialah 7 juta kilometer, atau 0,047 unit astronomi, atau satu perdelapan radius orbit Merkurius. HD 209458 b, also given the nickname Osiris, is an exoplanet that orbits the solar analog HD 209458 in the constellation Pegasus, some 159 light-years from the Solar System. News: Detection of oxygen and carbon in the hydrodynamically escaping atmosphere of the extrasolar planet HD209458b (2 February 2004) 2 February 2004: The first detection of oxygen and carbon in the atmosphere of … The radius of the planet's orbit is 7 million kilometres, about 0.047 astronomical units, or one eighth the radius of Mercury's orbit. Probeer. In July 2014, NASA announced the finding of a very dry atmosphere on the stars like the Sun at 209458 b and two other exoplanets was done. Tools. HD 189733 b is een exoplaneet die om de ster HD 189733 draait. Kënschtleresch Duerstellung vum Osiris viru sengem Stär HD 209458 mat engem Schwäif deen aus Material besteet dat aus senger Atmosphär austrëtt HD 209458 b is an extrasolar planet that orbits the Sun-like star HD 209458 in the constellation Pegasus. The planet represents a number of milestones in additional extraplanetary disciplines. [2] The radius of the planet's orbit is 7 million kilometres, about 0.047 astronomical units, or one eighth the radius of Mercury's orbit. The high size and volume of HD 209458 b indicates that it is a gas giant. Vu sengen Entdecker gouf hien nom alegyptesche Fruchtbarkeets- an Doudesgott inoffiziell och Osiris genannt. HD 209458 b is an extrasolar planet (unofficially referred to as Osiris) that orbits the Solar analog star HD 209458 in the constellation Pegasus, some 150 light-years from Earth's solar system, with evidence of water vapor. 1999 hunn zwéin Teams onofhängeg vuneneen d'Existenz vun engem Begleeder mat der Bezeechnung HD 209458 b entdeckt. HD 209458 b, ook bekend onder sy bynaam, Osiris, is ’n eksoplaneet wat sowat 150 ligjare van hier om die ster HD 209458, soortgelyk aan die Son, wentel in die sterrebeeld Vlieënde Perd.Die radius van die planeet se wentelbaan is 7 miljoen kilometer, sowat 0,047 AE of ’n agtste van Mercurius se wentelbaan. The radius of the planet's orbit is 7 million kilometres, about 0.047 astronomical units, or one eighth the radius of Mercury HD 209458 b (sometimes unofficially called Osiris) is an exoplanet that orbits the solar analog HD 209458 in the constellation Pegasus, some 150 light-years from the Solar System. Explore the Archive Interactive Table Search and File Upload Version Française de ce document. lació de Pegàs, a 150 anys llum de la Terra.S'hi van detectar proves de possibles presència d'aigua. The radius of the planet's orbit is 7 million kilometres, about 0.047 astronomical units, or one eighth the radius of Mercury's orbit. 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