คำอธิบายStructure of Stars (artist’s impression).jpg
Artist's impression of the structure of a solar-like star and a red giant. The two images are not to scale - the scale is given in the lower right corner. It is common to divide the Sun's (and solar-like stars') interior into three distinct zones: The uppermost is the Convective Zone. It extends downwards from the bottom of the photosphere to a depth of about 15% of the radius of the Sun. Here the energy is mainly transported upwards by (convection) streams of gas. The Radiative Zone is below the convection zone and extends downwards to the core. Here energy is transported outwards by radiation and not by convection. From the top of this zone to the bottom, the density increases 100 times. The core occupies the central region and its diameter is about 15% of that of the entire star. Here the energy is produced by fusion processes through which hydrogen nuclei are fused together to produce helium nuclei. In the Sun, the temperature is around 14 million degrees. In red giants, the convection zone is much larger, encompassing more than 35 times more mass than in the Sun.
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{{Information |Description=Artist's impression of the structure of a solar-like star and a red giant. The two images are not to scale - the scale is given in the lower right corner. It is common to divide the Sun's (and solar-like stars') interior into...
Artist's impression of the structure of a solar-like star and a red giant. The two images are not to scale - the scale is given in the lower right corner. It is common to divide the Sun's (and solar-like stars') interior into three distinct zones: The uppermost is the Convective Zone. It extends downwards from the bottom of the photosphere to a depth of about 15% of the radius of the Sun. Here the energy is mainly transported upwards by (convection) streams of gas. The Radiative Zone is below the convection zone and extends downwards to the core. Here energy is transported outwards by radiation and not by convection. From the top of this zone to the bottom, the density increases 100 times. The core occupies the central region and its diameter is about 15% of that of the entire star. Here the energy is produced by fusion processes through which hydrogen nuclei are fused together to produce helium nuclei. In the Sun, the temperature is around 14 million degrees. In red giants, the convection zone is much larger, encompassing more than 35 times more mass than in the Sun.
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divide the Sun s and solar like stars interior into three distinct zones The uppermost is the Convective Zone It extends downwards from the bottom of the photosphere to a depth of about 15 of the radius of the Sun Here the energy is mainly transported upwards by convection streams of gas The Radiative Zone is below the convection zone and extends downwards to the core Here energy is transported outwards by radiation and not by convection From the top of this zone to the bottom the density increases 100 times The core occupies the central region and its diameter is about 15 of that of the entire star Here the energy is produced by fusion processes through which hydrogen nuclei are fused together to produce helium nuclei In the Sun the temperature is around 14 million degrees In red giants the convection zone is much larger encompassing more than 35 times more mass than in the Sun wnthi 6 krkdakhm ph s 2550aehlngthima http www eso org public images eso0729a phusrangsrrkh ESO karxnuyatichsiththi This media was created by the European Southern Observatory ESO Their website states Unless specifically noted the images videos and music distributed on the public ESO website along with the texts of press releases announcements pictures of the week blog posts and captions are licensed under a Creative Commons Attribution 4 0 International License and may on a non exclusive basis be reproduced without fee provided the credit is clear and visible To the uploader You must provide a link URL to the original file and the authorship information if available iflnixyuphayitsyyaxnuyatkhriexthifkhxmmxns run aesdngthima 4 0 nanachatikhunsamarth thicaaebngpn thicathasaena aeckcay aelasngngandngklawtxip thicaeriyberiyngihm thicaddaeplngngandngklaw phayitenguxnikhtxipni aesdngthima khuntxngihekiyrtiecakhxngnganxyangehmaasm odyephimlingkipyngsyyaxnuyat aelarabuhakmikarepliynaeplng khunxacthaechnniidinrupaebbidkidtamkhwr aettxngimichinlksnathiaenawaphuihxnuyatsnbsnunkhunhruxkarichngankhxngkhunhttps creativecommons org licenses by 4 0 CC BY 4 0 Creative Commons Attribution 4 0 true truekhabrryayodyyxithyephimkhabrryaythrrthdediywephuxkhyaykhwamwaiflnimixairixethmthiaesdngxyuiniflniprakxbdwysthanalikhsiththimilikhsiththisyyaxnuyatCreative Commons Attribution 4 0 International xngkvswnthisrang wnkxtng6 krkdakhm 2007 prawtiifl khlikwnthi ewlaephuxduiflthipraktinkhnann wnthi ewlarupyxkhnadphuichkhwamehn pccubn23 35 28 phvsphakhm 25565 176 3 910 4 91 emkaibt Stas1995 Information Description Artist 039 s impression of the structure of a solar like star and a red giant The two images are not to scale the scale is given in the lower right corner It is common to divide the Sun 039 s and solar like stars 039 interior into hnathimiphaphni hnatxipni oyngmathiphaphni dawyks karichiflswnklang wikixuntxipniichiflni karichbn ar wikipedia org نجم عملاق منطقة الحمل الحراري karichbn ast wikipedia org Estrella xigante karichbn bg wikipedia org Gigant zvezda karichbn bn wikipedia org দ ত য ত র karichbn de wikipedia org Riesenstern karichbn en wikipedia org Convection Giant star Convection zone Red giant karichbn es wikipedia org Zona convectiva karichbn eu wikipedia org Eguzkia karichbn fa wikipedia org ستاره غول karichbn fr wikipedia org Geante rouge karichbn fr wikinews org De puissants champs magnetiques caches au coeur des etoiles karichbn he wikipedia org ענק כוכב karichbn hi wikipedia org द नव त र ल ल द नव त र karichbn hr wikipedia org Sunce Konvekcija karichbn hu wikipedia org oriascsillag karichbn hy wikipedia org Հսկա աստղ karichbn id wikipedia org Bintang raksasa Portal Bintang Portal Bintang Artikel pilihan 1 karichbn ja wikipedia org 巨星 karichbn kk wikipedia org Konvekciya ajmagy karichbn ko wikipedia org 거성 karichbn lv wikipedia org Sarkanais milzis karichbn mk wikipedia org Struevit sloј Џinovska ѕvezda karichbn mn wikipedia org Wikipedia Sүүlijn үeijn medee 2014 karichbn ne wikipedia org र त द नव त र karichbn nl wikipedia org Reuzenster karichbn pa wikipedia org ਲ ਲ ਦ ਨਵ ਤ ਰ ਦ ਨਵ ਤ ਰ karichbn pl wikipedia org Czerwony olbrzym Olbrzym gwiazda Historia pierwiastkow chemicznych Strefa konwektywna Dyskusja wikiprojektu Czy wiesz ekspozycje 2014 11 27 karichbn ro wikipedia org Epsilon Tauri karichbn rue wikipedia org Zvizda karichbn ru wikipedia org Zvezda gigant Portal Astronomiya Izobrazhenie nedeli Arhiv 2009 goda karichbn sk wikipedia org Hviezda karichbn sr wikipedia org Divovska zvezda karichbn uk wikipedia org Gigant zorya karichbn vi wikipedia org Vung đối lưu karichbn www wikidata org Q5875 dukarichthwolkephimetimkhxngiflnikhxmulekiywkbphaph phaphnimikhxmulephimetim sungswnihymacakklxngdicitxlhruxsaeknenxrthisamarthekbkhxmuldngklawiwrwmkbphaphid thaphaphnithukprbprungaekikhhruxepliynaeplngcakedim khxmulbangxyangcayngkhngimepliynaeplngehmuxnphaphthithukprbprungaekikhnnchuxphaphArtist s impression of the structure of a solar like star and a red giant The two images are not to scale the scale is given in the lower right corner It is common to divide the Sun s and solar like stars interior into three distinct zones The uppermost is the Convective Zone It extends downwards from the bottom of the photosphere to a depth of about 15 of the radius of the Sun Here the energy is mainly transported upwards by convection streams of gas The Radiative Zone is below the convection zone and extends downwards to the core Here energy is transported outwards by radiation and not by convection From the top of this zone to the bottom the density increases 100 times The core occupies the central region and its diameter is about 15 of that of the entire star Here the energy is produced by fusion processes through which hydrogen nuclei are fused together to produce helium nuclei In the Sun the temperature is around 14 million degrees In red giants the convection zone is much larger encompassing more than 35 times more mass than in the Sun ewlathibnthukphaph00 00 6 krkdakhm 2550tnchbbEuropean Southern Observatoryekhrdit phucdetriymESOchuxeruxngsnStructure of Stars artist s impression khasakhyStarskhxmulsahrbtidtxhttp www eso org Karl Schwarzschild Strasse 2Garching bei Munchen D 85748 GermanykhxtklnginkarichnganCreative Commons Attribution 3 0 Unported license ekhathungcak https th wikipedia org wiki ifl Structure of Stars artist s impression jpg, wikipedia, วิกิ หนังสือ, หนังสือ, ห้องสมุด,
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