Hertzsprung–Russell diagram. A plot of luminosity (absolute magnitude) against the colour of the stars ranging from the high-temperature blue-white stars on the left side of the diagram to the low temperature red stars on the right side. "This diagram below is a plot of 22000 stars from the Hipparcos Catalogue together with 1000 low-luminosity stars (red and white dwarfs) from the Gliese Catalogue of Nearby Stars. The ordinary hydrogen-burning dwarf stars like the Sun are found in a band running from top-left to bottom-right called the Main Sequence. Giant stars form their own clump on the upper-right side of the diagram. Above them lie the much rarer bright giants and supergiants. At the lower-left is the band of white dwarfs – these are the dead cores of old stars which have no internal energy source and over billions of years slowly cool down towards the bottom-right of the diagram." Converted to png and compressed with pngcrush.
{{Information |Description=Hertzsprung-Russell diagram. A plot of luminosity (absolute magnitude) against the colour of the stars ranging from the high-temperature blue-white stars on the left side of the diagram to the low temperature red stars on the ri
ไฟล, hrdiagram, ไฟล, ประว, ไฟล, หน, าท, ภาพน, การใช, ไฟล, วนกลางขนาดของต, วอย, างน, กเซล, ความละเอ, ยดอ, กเซล, กเซล, กเซล, ภาพท, ความละเอ, ยดส, งกว, 8206, กเซล, ขนาดไฟล, โลไบต, ชน, ดไมม, image, ปภาพหร, อไฟล, เส, ยงน, นฉบ, บอย, คอมมอนส, รายละเอ, ยดด, านล, าง, เ. ifl prawtiifl hnathimiphaphni karichiflswnklangkhnadkhxngtwxyangni 526 599 phikesl khwamlaexiydxun 211 240 phikesl 421 480 phikesl 720 820 phikesl duphaphthimikhwamlaexiydsungkwa 8206 720 820 phikesl khnadifl 19 kiolibt chnidimm image png rupphaphhruxiflesiyngni tnchbbxyuthi khxmmxns raylaexiyddanlang epnkhxkhwamthiaesdngphlcak ifltnchbbinkhxmmxns khxmmxnsepnewbistinokhrngkarsahrbekbrwbrwmsuxesri thi khunsamarthchwyid khaxthibayHRDiagram png Hertzsprung Russell diagram A plot of luminosity absolute magnitude against the colour of the stars ranging from the high temperature blue white stars on the left side of the diagram to the low temperature red stars on the right side This diagram below is a plot of 22000 stars from the Hipparcos Catalogue together with 1000 low luminosity stars red and white dwarfs from the Gliese Catalogue of Nearby Stars The ordinary hydrogen burning dwarf stars like the Sun are found in a band running from top left to bottom right called the Main Sequence Giant stars form their own clump on the upper right side of the diagram Above them lie the much rarer bright giants and supergiants At the lower left is the band of white dwarfs these are the dead cores of old stars which have no internal energy source and over billions of years slowly cool down towards the bottom right of the diagram Converted to png and compressed with pngcrush aehlngthima The Hertzsprung Russell Diagramphusrangsrrkh Richard Powellkarxnuyat karichiflniihm iflnixyuphayitsyyaxnuyat khriexthifkhxmmxns aebbaesdngthima xnuyataebbediywkn 2 5 thwipkhunsamarth thicaaebngpn thicathasaena aeckcay aelasngngandngklawtxip thicaeriyberiyngihm thicaddaeplngngandngklaw phayitenguxnikhtxipni aesdngthima khuntxngihekiyrtiecakhxngnganxyangehmaasm odyephimlingkipyngsyyaxnuyat aelarabuhakmikarepliynaeplng khunxacthaechnniidinrupaebbidkidtamkhwr aettxngimichinlksnathiaenawaphuihxnuyatsnbsnunkhunhruxkarichngankhxngkhun xnuyataebbediywkn hakkhunddaeplng epliynrup hruxtxetimnganni khuntxngichsyyaxnuyataebbediywknhruxaebbthiehmuxnkbsyyaxnuyatthiichkbnganniethannhttps creativecommons org licenses by sa 2 5 CC BY SA 2 5 Creative Commons Attribution Share Alike 2 5 true true See Copyright ewxrchnxun aekikh Hertzsprung Russell diagramAfrikaans Afrikaans alt catala cestina English English alt espanol francais galego italiano magyar oʻzbekcha polski slovencina suomi alt svenska belaruskaya kazaksha russkij հայերեն 日本語 中文 繁體 עברית עברית العربيةSun Sirius sparsecatala Deutsch PNG Deutsch English PNG English espanol galego Letzebuergesch TurkceWell known stars in the Milky WayAfrikaans Hertzsprung Russel StarData png English English alt Kiswahili Deutsch blgarski phaphaephnphaphni khwrcathuksrangihmepnkrafiksewketxr sungmikhxdixikhlayprakar duephimetimthikhxmmxns suxtxngkarekbkwadsahrbsarsnethsephimetim hakphaphnimiinrupaebbkrafiksewketxrxyuaelw krunaxpohldaelaaethnthiaemaebbnidwy vector version available i chuxphaphihm i aenanaepnxyangyingihtngchuxiflewketxrihmnninrupaebb HRDiagram svg aelwisaemaebb Vector version available hrux Vva sungimtxngichpharamietxr chuxphaphihmkhabrryayodyyxithyephimkhabrryaythrrthdediywephuxkhyaykhwamwaiflnimixairxngkvsHertzsprung Russell diagramixethmthiaesdngxyuiniflniprakxbdwyidxaaekrmkhxngaehrthschprung rsesllsthanalikhsiththimilikhsiththisyyaxnuyatCreative Commons Attribution ShareAlike 2 5 Generic xngkvs prawtiifl khlikwnthi ewlaephuxduiflthipraktinkhnann wnthi ewlarupyxkhnadphuichkhwamehn pccubn01 32 19 phvsphakhm 2554720 820 19 kiolibt SaiboReverted to version as of 03 42 3 March 2007 Commons Avoid overwriting existing files 05 17 26 minakhm 2554720 820 59 kiolibt Tomruenblack labels 01 25 26 minakhm 2554720 820 34 kiolibt Tomrueninvert colors white background 10 42 3 minakhm 2550720 820 19 kiolibt Falcorian Information Description Hertzsprung Russell diagram A plot of luminosity absolute magnitude against the colour of the stars ranging from the high temperature blue white stars on the left side of the diagram to the low temperature red stars on the ri hnathimiphaphni hnatxipni oyngmathiphaphni aethbladbhlk aephnphaphkhxngaehrthschprung rsesll karichiflswnklang wikixuntxipniichiflni karichbn af wikipedia org Hoofreeks karichbn af wiktionary org hoofreeks Hertzsprung Russell diagram karichbn ar wikipedia org نجم عملاق تكون النجوم النسق الأساسي رسم هرتزشبرونغ راسل متغير بيتا سيفي karichbn bg wikipedia org Diagrama na Hercshprung Rsel Glavna posledovatelnost karichbn bn wikipedia org হ র ডসব র র স ল চ ত র প রধ ন ধ র নক ষত র র শ র ণ karichbn bs wikipedia org Glavni niz karichbn cy wikipedia org Prif ddilyniant karichbn de wikipedia org Hauptreihe Zehnerpotenz Hertzsprung Lucke karichbn de wikibooks org 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