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English: This is a mosaic image, one of the largest ever taken by NASA's Hubble Space Telescope, of the Crab Nebula, a six-light-year-wide expanding remnant of a star's supernova explosion. Japanese and Chinese astronomers recorded this violent event in 1054 CE.
The orange filaments are the tattered remains of the star and consist mostly of hydrogen. The rapidly spinning neutron star embedded in the center of the nebula is the dynamo powering the nebula's eerie interior bluish glow. The blue light comes from electrons whirling at nearly the speed of light around magnetic field lines from the neutron star. The neutron star, like a lighthouse, ejects twin beams of radiation that appear to pulse 30 times a second due to the neutron star's rotation. A neutron star is the crushed ultra-dense core of the exploded star.
The Crab Nebula derived its name from its appearance in a drawing made by Irish astronomer Lord Rosse in 1844, using a 36-inch telescope. When viewed by Hubble, as well as by large ground-based telescopes such as the European Southern Observatory's Very Large Telescope, the Crab Nebula takes on a more detailed appearance that yields clues into the spectacular demise of a star, 6,500 light-years away.
The newly composed image was assembled from 24 individual Wide Field and Planetary Camera 2 exposures taken in October 1999, January 2000, and December 2000. The colors in the image indicate the different elements that were expelled during the explosion. Blue in the filaments in the outer part of the nebula represents neutral oxygen, green is singly-ionized sulfur, and red indicates doubly-ionized oxygen.
Français : Cette image, une des plus grandes de la Nébuleuse du Crabe jamais prises par le télescope spatial Hubble de la NASA, est en réalité une mosaïque de plusieurs clichés. La nébuleuse s'étend sur une distance de six années-lumière et est composée des restes de l'explosion d'une supernova. Les astronomes chinois et japonais ont observé cette violente explosion il y a environ un millénaire, en 1054.
Les filaments oranges sont les restes en lambeaux de l'étoile et se composent principalement d'hydrogène. L'étoile à neutrons qui tourne rapidement sur elle-même, intégrée dans le centre de la nébuleuse, est la dynamo alimentant l'intérieur de la nébuleuse de l'étrange lueur bleuâtre. La lumière bleue provient des électrons tourbillonnant presque à la vitesse de la lumière autour de lignes du champ magnétique de l'étoile à neutrons. L'étoile à neutrons, comme un phare, émet des faisceaux de rayonnements jumeaux qui semblent battre 30 fois par seconde en raison de la rotation de l'étoile à neutrons. Une étoile à neutrons est le noyau écrasé ultra-dense de l'étoile qui a explosé.
L'image est formée de l'assemblage de 24 prises individuelles de la Wide Field and Planetary Camera 2 datant d'octobre 1999, janvier 2000 et décembre 2000. Les couleurs de l'image indiquent les différents éléments qui ont été expulsé lors de l'explosion. Le bleu dans les filaments de la partie extérieure de la nébuleuse représente l'oxygène neutre, le vert est le souffre ionisé I, et le rouge indique l'oxygène ionisé II.
العربية: هذه الصورة المركبة, هي واحدة من أكبر الصور على الإطلاق التي التقطها تلسكوب هبل لسديم السرطان, وهو بقايا مستعر أعظم تمتد على مساحة قطرها 6 سنوات ضوئية. قام الفلكيون القدماء العرب والصينيون بتسجيل هذا الحدث قبل 1,000 عام في سنة 1054م, كما فعل ذلك البحارة الأمريكيون (بالرغم من أنه ليس من المؤكد تماماً أن ما سجلوه هو هذا).
الخيوط البرتقالية الظاهرة في الصورة هي أشلاء وشظايا متبقّية من النجم الذي انفجر (وكوّن السديم) وهي تتركب بشكل رئيسي من الهيدروجين. النجم النيوتروني سريع "الدوران المحوري" المتواري في وسط السديم يَعمل كمولد طاقة يُسبب البريق المُزرقّ الغريب المُشع من وسط السديم. وهذا الضوء الأزرق قادم من إلكترونات تدور بما يُقارب سرعة الضوء حول الحقل المغناطيسي للنجم النيوتروني. النجم النيوتروني, مثل المنارة, يُطلق شعاعين من الضوء في اتجاهين مختلفين يَجعلناه يبدو كأنه ينبض 30 مرة في الثانية نتيجة لدورانه المحوري السريع (النجوم النيوترونية تُتم بضعة دورات حول نفسها في الثانية على الأقل). والنجم النيوتروني هو نواة مسحوقة شديدة الكثافة لنجم انفجر.
هذه الصورة المركبة رُكّبت من 24 صورة بعضها التطقت في تشرين الأول (أكتوبر) 1999, وكانون الثاني (يناير) 2000, وكانون الأول (ديسمبر) 2000. الألوان في الصورة تدل على عناصر مختلفة قذفت أثناء الانفجار. اللون الأزرق في الشعيرات في الجزء الخارجي من السديم هو لأكسجين طبيعي, والأخضر لكبريت متأين فردياً, والأحمر لأكسجين متأين.
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HubbleSite: gallery, release.
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NASA, ESA, J. Hester and A. Loll (Arizona State University)
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Material credited to STScI on this site was created, authored, and/or prepared for NASA under Contract NAS5-26555. Unless otherwise specifically stated, no claim to copyright is being asserted by STScI and it may be freely used as in the public domain in accordance with NASA's contract. However, it is requested that in any subsequent use of this work NASA and STScI be given appropriate acknowledgement. STScI further requests voluntary reporting of all use, derivative creation, and other alteration of this work. Such reporting should be sent to copyright@stsci.edu.
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.
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This is a featured picture on Wikimedia Commons (Featured pictures) and is considered one of the finest images.
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This is a featured picture on the ərəb language Wikipedia (صور مختارة) and is considered one of the finest images. This is a featured picture on the alman language Wikipedia (Exzellente Bilder) and is considered one of the finest images. This is a featured picture on the ingilis language Wikipedia (Featured pictures) and is considered one of the finest images. This is a featured picture on the ispan language Wikipedia (Recursos destacados) and is considered one of the finest images. This is a featured picture on the fars language Wikipedia (نگارههای برگزیده) and is considered one of the finest images. This is a featured picture on the tamil language Wikipedia (இன்றைய சிறப்புப் படம்) and is considered one of the finest images. This is a featured picture on the türk language Wikipedia (Seçkin resimler) and is considered one of the finest images. This is a featured picture on the vyetnam language Wikipedia (Hình ảnh chọn lọc) and is considered one of the finest images. This is a featured picture on the çin language Wikipedia (特色图片) and is considered one of the finest images.
If you have an image of similar quality that can be published under a suitable copyright license, be sure to upload it, tag it, and nominate it.
Annotations
InfoField
This image is annotated: View the annotations at Commons
1996
1926
52
64
3864
3864
Crab Pulsar
Captions
Add a one-line explanation of what this file represents
Crab Nebula
Krebsnebel im Sternbild Stier
ערפילית הסרטן
Krabí mlhovina
صورة سديم السرطان
A Rák-köd a Hubble Űrtávcső felvételén.
კირჩხიბის ნისლეული
Items portrayed in this file
təsvir edir
NGC 1952
Crab Pulsar ingilis
Commons quality assessment ingilis
Wikimedia Commons featured picture ingilis
yaranma tarixi
1 dekabr 2005
MIME type ingilis
image/jpeg
Faylın tarixçəsi
Faylın əvvəlki versiyasını görmək üçün gün/tarix bölməsindəki tarixlərə klikləyin.
Image: A New View of the Helix Nebula Source: http://hubblesite.org/gallery/album/entire_collection/pr2004032d/ Copyright Notice: Material credited to STScI on this site was created, authored, and/or prepared for NASA under Contract NAS5-26555. Unless
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300 dpi
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Adobe Photoshop CS2 Windows
Faylın dəyişməsi tarixi və vaxtı
11:37, 28 noyabr 2005
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Tarix və vaxt rəqəmləşdirilir
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Date metadata was last modified
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Aprel 02, 2023
fayl, crab, nebula, fayl, faylın, tarixçəsi, fayl, keçidləri, faylın, qlobal, istifadəsi, metaməlumatlarsınaq, göstərişi, ölçüsü, piksel, digər, ölçülər, piksel, piksel, piksel, piksel, piksel, piksel, faylın, orijinalı, 8206, piksel, fayl, həcmi, mime, növü, . Fayl Faylin tarixcesi Fayl kecidleri Faylin qlobal istifadesi MetamelumatlarSinaq gosterisi olcusu 600 600 piksel Diger olculer 240 240 piksel 480 480 piksel 768 768 piksel 1 024 1 024 piksel 2 048 2 048 piksel 3 864 3 864 piksel Faylin orijinali 8206 3 864 3 864 piksel fayl hecmi 13 84 MB MIME novu image jpeg Bu fayl Vikimedia Commons dadirve diger layihelerde istifade edile biler Faylin tesvir sehifesine get Xulase IzahCrab Nebula jpg English This is a mosaic image one of the largest ever taken by NASA s Hubble Space Telescope of the Crab Nebula a six light year wide expanding remnant of a star s supernova explosion Japanese and Chinese astronomers recorded this violent event in 1054 CE The orange filaments are the tattered remains of the star and consist mostly of hydrogen The rapidly spinning neutron star embedded in the center of the nebula is the dynamo powering the nebula s eerie interior bluish glow The blue light comes from electrons whirling at nearly the speed of light around magnetic field lines from the neutron star The neutron star like a lighthouse ejects twin beams of radiation that appear to pulse 30 times a second due to the neutron star s rotation A neutron star is the crushed ultra dense core of the exploded star The Crab Nebula derived its name from its appearance in a drawing made by Irish astronomer Lord Rosse in 1844 using a 36 inch telescope When viewed by Hubble as well as by large ground based telescopes such as the European Southern Observatory s Very Large Telescope the Crab Nebula takes on a more detailed appearance that yields clues into the spectacular demise of a star 6 500 light years away The newly composed image was assembled from 24 individual Wide Field and Planetary Camera 2 exposures taken in October 1999 January 2000 and December 2000 The colors in the image indicate the different elements that were expelled during the explosion Blue in the filaments in the outer part of the nebula represents neutral oxygen green is singly ionized sulfur and red indicates doubly ionized oxygen Francais nbsp Cette image une des plus grandes de la Nebuleuse du Crabe jamais prises par le telescope spatial Hubble de la NASA est en realite une mosaique de plusieurs cliches La nebuleuse s etend sur une distance de six annees lumiere et est composee des restes de l explosion d une supernova Les astronomes chinois et japonais ont observe cette violente explosion il y a environ un millenaire en 1054 Les filaments oranges sont les restes en lambeaux de l etoile et se composent principalement d hydrogene L etoile a neutrons qui tourne rapidement sur elle meme integree dans le centre de la nebuleuse est la dynamo alimentant l interieur de la nebuleuse de l etrange lueur bleuatre La lumiere bleue provient des electrons tourbillonnant presque a la vitesse de la lumiere autour de lignes du champ magnetique de l etoile a neutrons L etoile a neutrons comme un phare emet des faisceaux de rayonnements jumeaux qui semblent battre 30 fois par seconde en raison de la rotation de l etoile a neutrons Une etoile a neutrons est le noyau ecrase ultra dense de l etoile qui a explose L image est formee de l assemblage de 24 prises individuelles de la Wide Field and Planetary Camera 2 datant d octobre 1999 janvier 2000 et decembre 2000 Les couleurs de l image indiquent les differents elements qui ont ete expulse lors de l explosion Le bleu dans les filaments de la partie exterieure de la nebuleuse represente l oxygene neutre le vert est le souffre ionise I et le rouge indique l oxygene ionise II العربية هذه الصورة المركبة هي واحدة من أكبر الصور على الإطلاق التي التقطها تلسكوب هبل لسديم السرطان وهو بقايا مستعر أعظم تمتد على مساحة قطرها 6 سنوات ضوئية قام الفلكيون القدماء العرب والصينيون بتسجيل هذا الحدث قبل 1 000 عام في سنة 1054م كما فعل ذلك البحارة الأمريكيون بالرغم من أنه ليس من المؤكد تماما أن ما سجلوه هو هذا الخيوط البرتقالية الظاهرة في الصورة هي أشلاء وشظايا متبق ية من النجم الذي انفجر وكو ن السديم وهي تتركب بشكل رئيسي من الهيدروجين النجم النيوتروني سريع الدوران المحوري المتواري في وسط السديم ي عمل كمولد طاقة ي سبب البريق الم زرق الغريب الم شع من وسط السديم وهذا الضوء الأزرق قادم من إلكترونات تدور بما ي قارب سرعة الضوء حول الحقل المغناطيسي للنجم النيوتروني النجم النيوتروني مثل المنارة ي طلق شعاعين من الضوء في اتجاهين مختلفين ي جعلناه يبدو كأنه ينبض 30 مرة في الثانية نتيجة لدورانه المحوري السريع النجوم النيوترونية ت تم بضعة دورات حول نفسها في الثانية على الأقل والنجم النيوتروني هو نواة مسحوقة شديدة الكثافة لنجم انفجر هذه الصورة المركبة ر ك بت من 24 صورة بعضها التطقت في تشرين الأول أكتوبر 1999 وكانون الثاني يناير 2000 وكانون الأول ديسمبر 2000 الألوان في الصورة تدل على عناصر مختلفة قذفت أثناء الانفجار اللون الأزرق في الشعيرات في الجزء الخارجي من السديم هو لأكسجين طبيعي والأخضر لكبريت متأين فرديا والأحمر لأكسجين متأين Tarix 1 dekabr 2005 Menbe HubbleSite gallery release Muellif NASA ESA J Hester and A Loll Arizona State University Icaze Faylin tekrar istifadesi Material credited to STScI on this site was created authored and or prepared for NASA under Contract NAS5 26555 Unless otherwise specifically stated no claim to copyright is being asserted by STScI and it may be freely used as in the public domain in accordance with NASA s contract However it is requested that in any subsequent use of this work NASA and STScI be given appropriate acknowledgement STScI further requests voluntary reporting of all use derivative creation and other alteration of this work Such reporting should be sent to copyright stsci edu Diger versiyalar https www flickr com photos gsfc 4398655649 and https www flickr com photos nasahubble 27747556420 Lisenziya 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 Assessment This is a featured picture on Wikimedia Commons Featured pictures and is considered one of the finest images Vikipediya nbsp This is a featured picture on the ereb language Wikipedia صور مختارة and is considered one of the finest images nbsp This is a featured picture on the alman language Wikipedia Exzellente Bilder and is considered one of the finest images nbsp This is a featured picture on the ingilis language Wikipedia Featured pictures and is considered one of the finest images nbsp This is a featured picture on the ispan language Wikipedia Recursos destacados and is considered one of the finest images nbsp This is a featured picture on the fars language Wikipedia نگاره های برگزیده and is considered one of the finest images nbsp This is a featured picture on the tamil language Wikipedia இன ற ய ச றப ப ப படம and is considered one of the finest images nbsp This is a featured picture on the turk language Wikipedia Seckin resimler and is considered one of the finest images nbsp This is a featured picture on the vyetnam language Wikipedia Hinh ảnh chọn lọc and is considered one of the finest images nbsp This is a featured picture on the cin language Wikipedia 特色图片 and is considered one of the finest images If you have an image of similar quality that can be published under a suitable copyright license be sure to upload it tag it and nominate it AnnotationsInfoFieldThis image is annotated View the annotations at Commons1996 1926 52 64 3864 3864 Crab PulsarCaptionsazerbaycancaAdd a one line explanation of what this file representsingilisCrab NebulaalmanKrebsnebel im Sternbild Stierivritערפילית הסרטןcexKrabi mlhovinaerebصورة سديم السرطانmacarA Rak kod a Hubble Urtavcso felvetelen gurcuკირჩხიბის ნისლეულიItems portrayed in this filetesvir edirNGC 1952Crab Pulsar nbsp ingilisCommons quality assessment nbsp ingilisWikimedia Commons featured picture nbsp ingilisyaranma tarixi1 dekabr 2005MIME type nbsp ingilisimage jpeg Faylin tarixcesi Faylin evvelki versiyasini gormek ucun gun tarix bolmesindeki tarixlere klikleyin Tarix VaxtKicik sekilOlculerIstifadeciSerh indiki14 56 25 noyabr 20123 864 3 864 13 84 MB Hawky diddizLossless optimization 10 13 17 may 20123 864 3 864 14 61 MB MetronomoHigher quality 09 31 20 iyun 20093 864 3 864 6 18 MB TryphonHigher resolution 21 26 9 mart 20062 224 2 212 3 08 MB Stianbhlarger version 00 35 16 yanvar 2006400 400 23 KB DragonFire1024Image A New View of the Helix Nebula Source http hubblesite org gallery album entire collection pr2004032d Copyright Notice Material credited to STScI on this site was created authored and or prepared for NASA under Contract NAS5 26555 Unless Fayl kecidleri Bu sekile olan kecidler Astronomiya Goy cismi Messier cisimleri Xerceng dumanligi Vikipediya Movzulu ay Astronomiya ayi Portal Astronomiya Portal Astronomiya Elaqedar portallar Portal Astronomiya Esas resm Portal Elektronika Portal Elektronika Elaqeli portallar Portal Elm Portal Elm Elaqeli portallar Portal Fizika Portal Fizika Elaqeli portallar Portal Gunes sistemi Portal Gunes sistemi Elaqeli Portallar Portal Gunes sistemi Elaqeli VikiLayiheler Portal Kimya Portal Kimya Elaqeli portallar Portal Yupiter Portal Yupiter Elaqeli Portallar Portal Informatika Portal Informatika Elaqeli portallar Faylin qlobal istifadesi Bu fayl asagidaki vikilerde istifade olunur af wikipedia org layihesinde istifadesi 1054 Wikipedia Uitgesoekte herdenkings 22 April Wikipedia Uitgesoekte herdenkings Julie Wikipedia Uitgesoekte herdenkings April Wikipedia Uitgesoekte herdenkings 4 Julie Supernova Ster Wikipedia Beeld van die week 2012 Wikipedia Voorbladbeeld week 2 2012 Newel Kompakte ster Veranderlike ster Lys van Messier voorwerpe Krap newel Portaal Sterrekunde Inleiding Portaal Sterrekunde Hemelliggaam SN 1054 Supernova oorblyfsel Sterevolusie als wikipedia org layihesinde istifadesi Vorlage Houptsyte 4 07 4 Juli am wikipedia org layihesinde istifadesi ሠማያዊ አካላት ar wikipedia org layihesinde istifadesi مجرة نجم سنة تطور النجوم ثلاثي الكربون فجر مستعر أعظم بوابة علم الفلك مقالة مختارة شهاب مطلع مستقيم جمعية منسا الدولية علم الفلك خارج المجري فيلا أقمار اصطناعية الشلياق خرزات بيلي راية الأرض سمت نظرية الحالة الثابتة توهج القمر الصناعي بوابة الفيزياء بوابات ذات علاقة الظهر اقتران علم الفلك علم الهيئة مقراب راديوي طاقة إشعاعية كتلة حقيقية القمر الصناعي لتغطية حقل الجاذبية واختبار المناخ Bu faylin qlobal istifadesine baxin Metamelumatlar Bu faylda fotoaparat ve ya skanerle elave olunmus melumatlar var Eger fayl sonradan redakte olunubsa bezi parametrler bu sekilde gosterilenlerden ferqli ola biler Genislik3 864 pxHundurluk3 864 pxBits per component8 8 8SixilmamisLZWReng modeliRGBOrientasiyaNormalReng komponentlerinin sayi3Ufuqi xett300 dpiSaquli xett300 dpiData arrangementchunky formatProqram teminatiAdobe Photoshop CS2 WindowsFaylin deyismesi tarixi ve vaxti11 37 28 noyabr 2005Reng sahesiFotosekilde reng secimi edilmemisdir Sekilin eni3 864 pxSekilin hundurluyu3 864 pxTarix ve vaxt reqemlesdirilir06 37 28 noyabr 2005Date metadata was last modified06 37 28 noyabr 2005IIM versiya2 Menbe https az wikipedia org wiki Fayl Crab Nebula jpg, wikipedia, oxu, kitab, kitabxana, axtar, tap, hersey,
ne axtarsan burda
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