NASA's Hubble Space Telescope has captured the sharpest view yet of the most famous of all planetary nebulae: the Ring Nebula (M57). In this October 1998 image, the telescope has looked down a barrel of gas cast off by a dying star thousands of years ago. This photo reveals elongated dark clumps of material embedded in the gas at the edge of the nebula; the dying central star floating in a blue haze of hot gas. The nebula is about a light-year in diameter and is located some 2000 light-years from Earth in the direction of the constellation Lyra.
The colors are approximately true colors. The color image was assembled from three black-and-white photos taken through different color filters with the Hubble telescope's Wide Field Planetary Camera 2. Blue isolates emission from very hot helium, which is located primarily close to the hot central star. Green represents ionized oxygen, which is located farther from the star. Red shows ionized nitrogen, which is radiated from the coolest gas, located farthest from the star. The gradations of color illustrate how the gas glows because it is bathed in ultraviolet radiation from the remnant central star, whose surface temperature is a white-hot 120,000 degrees Celsius (216,000 degrees Fahrenheit).
العربية: السديم الحلقي، سديم كوكبي مشابه لما ستصبح عليه الشمس.
This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use. The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or . For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.
This image or video was catalogued by Space Telescope Science Institute of the United States National Aeronautics and Space Administration (NASA) under Photo ID: GPN-2000-000964 and Alternate ID: PR99-01.
This tag does not indicate the copyright status of the attached work. A normal copyright tag is still required.See Commons:Licensing.
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NASA image of M57, the Ring Nebula, taken from English Wikipedia. Image Credit: NASA and The Hubble Heritage Team (STScI/AURA) [http://www.stsci.edu/institute/Copyright] ==Source== * http://heritage.stsci.edu/1999/01/index.html
ไฟล, ring, nebula, ไฟล, ประว, ไฟล, หน, าท, ภาพน, การใช, ไฟล, วนกลาง, อม, ลเก, ยวก, บภาพขนาดของต, วอย, างน, กเซล, ความละเอ, ยดอ, กเซล, กเซล, กเซล, กเซล, ภาพท, ความละเอ, ยดส, งกว, 8206, กเซล, ขนาดไฟล, โลไบต, ชน, ดไมม, image, jpeg, ปภาพหร, อไฟล, เส, ยงน, นฉบ, บอย. ifl prawtiifl hnathimiphaphni karichiflswnklang khxmulekiywkbphaphkhnadkhxngtwxyangni 587 600 phikesl khwamlaexiydxun 235 240 phikesl 470 480 phikesl 752 768 phikesl 1 215 1 241 phikesl duphaphthimikhwamlaexiydsungkwa 8206 1 215 1 241 phikesl khnadifl 631 kiolibt chnidimm image jpeg rupphaphhruxiflesiyngni tnchbbxyuthi khxmmxns raylaexiyddanlang epnkhxkhwamthiaesdngphlcak ifltnchbbinkhxmmxns khxmmxnsepnewbistinokhrngkarsahrbekbrwbrwmsuxesri thi khunsamarthchwyid khwamyx khaxthibayM57 The Ring Nebula JPG NASA s Hubble Space Telescope has captured the sharpest view yet of the most famous of all planetary nebulae the Ring Nebula M57 In this October 1998 image the telescope has looked down a barrel of gas cast off by a dying star thousands of years ago This photo reveals elongated dark clumps of material embedded in the gas at the edge of the nebula the dying central star floating in a blue haze of hot gas The nebula is about a light year in diameter and is located some 2000 light years from Earth in the direction of the constellation Lyra The colors are approximately true colors The color image was assembled from three black and white photos taken through different color filters with the Hubble telescope s Wide Field Planetary Camera 2 Blue isolates emission from very hot helium which is located primarily close to the hot central star Green represents ionized oxygen which is located farther from the star Red shows ionized nitrogen which is radiated from the coolest gas located farthest from the star The gradations of color illustrate how the gas glows because it is bathed in ultraviolet radiation from the remnant central star whose surface temperature is a white hot 120 000 degrees Celsius 216 000 degrees Fahrenheit العربية السديم الحلقي سديم كوكبي مشابه لما ستصبح عليه الشمس wnthi tulakhm ph s 2541 aehlngthima http hubblesite org newscenter archive releases 1999 01 image a direct link phusrangsrrkh The Hubble Heritage Team AURA STScI NASA karxnuyat karichiflniihm Public domain Public domain false false This file is in the public domain because it was created by NASA and ESA NASA Hubble material and ESA Hubble material prior to 2009 is copyright free and may be freely used as in the public domain without fee on the condition that only NASA STScI and or ESA is credited as the source of the material This license does not apply if ESA material created after 2008 or source material from other organizations is in use The material was created for NASA by Space Telescope Science Institute under Contract NAS5 26555 or for ESA by the Hubble European Space Agency Information Centre Copyright statement at hubblesite org or 2008 copyright statement at spacetelescope org For material created by the European Space Agency on the spacetelescope org site since 2009 use the ESA Hubble tag This image or video was catalogued by Space Telescope Science Institute of the United States National Aeronautics and Space Administration NASA nbsp under Photo nbsp ID GPN 2000 000964 nbsp and Alternate nbsp ID PR99 01 This tag does not indicate the copyright status of the attached work A normal copyright tag is still required See Commons Licensing Other languages العربية nbsp belaruskaya tarashkevica nbsp blgarski nbsp catala nbsp cestina nbsp dansk nbsp Deutsch nbsp English nbsp espanol nbsp فارسی nbsp francais nbsp galego nbsp magyar nbsp հայերեն nbsp Bahasa Indonesia nbsp italiano nbsp 日本語 nbsp makedonski nbsp മലയ ള nbsp Nederlands nbsp polski nbsp portugues nbsp russkij nbsp sicilianu nbsp slovenscina nbsp Turkce nbsp ukrayinska nbsp 简体中文 nbsp 繁體中文 nbsp khabrryayodyyxithyephimkhabrryaythrrthdediywephuxkhyaykhwamwaiflnimixairxahrbسديم حلقيhngkariA Lyra Gyurus vagy Gyuru planetaris kod a Hubble urtavcso felvetelenixethmthiaesdngxyuiniflniprakxbdwyenbiwlawngaehwnenbiwladawekhraahwnthisrang wnkxtngtulakhm 1998 prawtiifl khlikwnthi ewlaephuxduiflthipraktinkhnann wnthi ewlarupyxkhnadphuichkhwamehn pccubn09 06 21 thnwakhm 25491 215 1 241 631 kiolibt Egghigh quality 21 49 5 phvscikayn 25481 024 768 41 kiolibt Czar usurped NASA image of M57 the Ring Nebula taken from English Wikipedia Image Credit NASA and The Hubble Heritage Team STScI AURA http www stsci edu institute Copyright Source http heritage stsci edu 1999 01 index html hnathimiphaphni hnatxipni oyngmathiphaphni raychuxwtthuthxngfakhxngemsiey enbiwladawekhraah enbiwlawngaehwn karichiflswnklang wikixuntxipniichiflni karichbn af wikipedia org Ring newel Lys van planetere newels karichbn ar wikipedia org ويكيبيديا صناديق المستخدم تعليم مستخدم Riddler مستخدم وسام زقوت مستخدم Usamasaad مستخدم Safirsawtak سديم كوكبي مستخدم أحمد عبد الواحد القونى مستخدم DigitalLife arwiki مستخدم صلاح قيسي فلكي تشكل المجموعة الشمسية وتطورها سديم 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khxmulbangxyangcayngkhngimepliynaeplngehmuxnphaphthithukprbprungaekikhnnkhwamehnifl JPEGFile written by Adobe Photoshop 5 2 ekhathungcak https th wikipedia org wiki ifl M57 The Ring Nebula JPG, wikipedia, วิกิ หนังสือ, หนังสือ, ห้องสมุด,
