chitr:Crab Nebula.jpg

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varnan[sampaadan]

jaankaari
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 nearly 1,000 years ago in 1054, as did, almost certainly, Native Americans.

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.
Françaais : Cette image, une des plus grandes de la Néabuleuse du Crabe jamais prises par le téalescope spatial Hubble de la NASA, est en réaaalité une mosaïaaque de plusieurs clichéaas. La néaabuleuse s'éaatend sur une distance de six annéaaes-lumièaare et est composéaae des restes de l'explosion d'une supernova. Les astronomes chinois et japonais ont observé cette violente explosion il y a environ un milléaanaire, en 1054, comme l'ont certainement éaagalement fait les indiens d'Améarique.

Les filaments oranges sont les restes en lambeaux de l'éatoile et se composent principalement d'hydrogèaane. L'éatoile à neutrons qui tourne rapidement sur elle-mêame, intéaagréaae dans le centre de la néaabuleuse, est la dynamo alimentant l'intéaarieur de la néaabuleuse de l'éatrange lueur bleuâaatre. La lumièaare bleue provient des éalectrons tourbillonnant presque à la vitesse de la lumièaare autour de lignes du champ magnéaatique de l'éatoile à neutrons. L'éatoile à neutrons, comme un phare, éamet des faisceaux de rayonnements jumeaux qui semblent battre 30 fois par seconde en raison de la rotation de l'éatoile à neutrons. Une éatoile à neutrons est le noyau éaacrasé ultra-dense de l'éatoile qui a explosé.

L'image est forméaae de l'assemblage de 24 prises individuelles de la Wide Field and Planetary Camera 2 datant d'octobre 1999, janvier 2000 et déaacembre 2000. Les couleurs de l'image indiquent les difféaarents éaléaments qui ont éaté expulsé lors de l'explosion. Le bleu dans les filaments de la partie extéaarieure de la néaabuleuse repréasente l'oxygèaane neutre, le vert est le souffre ionisé I, et le rouge indique l'oxygèaane ionisé II.
اaaلaaعaaرaaبaaيaaة: هaaذaaه اaaلaaصaaوaaرaaة اaaلaaمaaرaaكaaبaaة, هaaي وaaاaaحaaدaaة مaaن أaaكaaبaaر اaaلaaصaaوaaر عaaلaaى اaaلaaإaaطaaلaaاaaق اaaلaaتaaي اaaلaaتaaقaaطaaهaaا تaaلaaسaaكaaوaaب هaaبaaل لسaaدaaيaaم اaaلaaسaaرaaطaaاaaن, وaaهaaو بaaقaaاaaيaaا مaaسaaتaaعaaر أaaعaaظaaم تaaمaaتaaد عaaلaaى مaaسaaاaaحaaة قaaطaaرaaهaaا 6 سaaنaaوaaاaaت ضaaوaaئaaيaaة. قaaاaaم اaaلaaفaaلaaكaaيaaوaaن اaaلaaقaaدaaمaaاaaء اaaلaaعaaرaaب وaaاaaلaaصaaيaaنaaيaaوaaن بaaتaaسaaجaaيaaل هaaذaaا اaaلaaحaaدaaث قaaبaaل 1,000 عaaاaaم فaaي سaaنaaة 1054م, كaaمaaا فaaعaaل ذaaلaaك اaaلaaبaaحaaاaaرaaة اaaلaaأaaمaaرaaيaaكaaيaaوaaن (بaaاaaلaaرaaغaaم مaaن أaaنaaه لaaيaaس مaaن اaaلaaمaaؤaaكaaد تaaمaaاaaمaaاaaً أaaن مaaا سaaجaaلaaوaaه هaaو هaaذaaا).

اaaلaaخaaيaaوaaط اaaلaaبaaرaaتaaقaaاaaلaaيaaة اaaلaaظaaاaaهaaرaaة فaaي اaaلaaصaaوaaرaaة هaaي أaaشaaلaaاaaء وaaشaaظaaاaaيaaا مaaتaaبaaقaaّaaيaaة مaaن اaaلaaنaaجaaم اaaلaaذaaي اaaنaaفaaجaaر (وaaكaaوaaّaaن اaaلaaسaaدaaيaaم) وaaهaaي تaaتaaرaaكaaب بaaشaaكaaل رaaئaaيaaسaaي مaaن اaaلaaهaaيaaدaaرaaوaaجaaيaaن. اaaلaaنaaجaaم اaaلaaنaaيaaوaaتaaرaaوaaنaaي سaaرaaيaaع "اaaلaaدaaوaaرaaاaaن اaaلaaمaaحaaوaaرaaي" اaaلaaمaaتaaوaaاaaرaaي فaaي وaaسaaط اaaلaaسaaدaaيaaم يaaَaaعaaمaaل كaaمaaوaaلaaد طaaاaaقaaة يaaُaaسaaبaaب اaaلaaبaaرaaيaaق اaaلaaمaaُaaزaaرaaقaaّ اaaلaaغaaرaaيaaب اaaلaaمaaُaaشaaع مaaن وaaسaaط اaaلaaسaaدaaيaaم. وaaهaaذaaا اaaلaaضaaوaaء اaaلaaأaaزaaرaaق قaaاaaدaaم مaaن إaaلaaكaaتaaرaaوaaنaaاaaت تaaدaaوaaر بaaمaaا يaaُaaقaaاaaرaaب سaaرaaعaaة اaaلaaضaaوaaء حaaوaaل اaaلaaحaaقaaل اaaلaaمaaغaaنaaاaaطaaيaaسaaي لaaلaaنaaجaaم اaaلaaنaaيaaوaaتaaرaaوaaنaaي. اaaلaaنaaجaaم اaaلaaنaaيaaوaaتaaرaaوaaنaaي, مaaثaaل اaaلaaمaaنaaاaaرaaة, يaaُaaطaaلaaق شaaعaaاaaعaaيaaن مaaن اaaلaaضaaوaaء فaaي اaaتaaجaaاaaهaaيaaن مaaخaaتaaلaaفaaيaaن يaaَaaجaaعaaلaaنaaاaaه يaaبaaدaaو كaaأaaنaaه يaaنaaبaaض 30 مaaرaaة فaaي اaaلaaثaaاaaنaaيaaة نaaتaaيaaجaaة لaaدaaوaaرaaاaaنaaه اaaلaaمaaحaaوaaرaaي اaaلaaسaaرaaيaaع (اaaلaaنaaجaaوaaم اaaلaaنaaيaaوaaتaaرaaوaaنaaيaaة تaaُaaتaaم بaaضaaعaaة دaaوaaرaaاaaت حaaوaaل نaaفaaسaaهaaا فaaي اaaلaaثaaاaaنaaيaaة عaaلaaى اaaلaaأaaقaaل). وaaاaaلaaنaaجaaم اaaلaaنaaيaaوaaتaaرaaوaaنaaي هaaو نaaوaaاaaة مaaسaaحaaوaaقaaة شaaدaaيaaدaaة اaaلaaكaaثaaاaaفaaة لaaنaaجaaم اaaنaaفaaجaaر.

هaaذaaه اaaلaaصaaوaaرaaة اaaلaaمaaرaaكaaبaaة رaaُaaكaaّaaبaaت مaaن 24 صaaوaaرaaة بaaعaaضaaهaaا اaaلaaتaaطaaقaaت فaaي تaaشaaرaaيaaن اaaلaaأaaوaaل (أaaكaaتaaوaaبaaر) 1999, وaaكaaاaaنaaوaaن اaaلaaثaaاaaنaaي (يaaنaaاaaيaaر) 2000, وaaكaaاaaنaaوaaن اaaلaaأaaوaaل (دaaيaaسaaمaaبaaر) 2000. اaaلaaأaaلaaوaaاaaن فaaي اaaلaaصaaوaaرaaة تaaدaaل عaaلaaى عaaنaaاaaصaaر مaaخaaتaaلaaفaaة قaaذaaفaaت أaaثaaنaaاaaء اaaلaaاaaنaaفaaجaaاaaر. اaaلaaلaaوaaن اaaلaaأaaزaaرaaق فaaي اaaلaaشaaعaaيaaرaaاaaت فaaي اaaلaaجaaزaaء اaaلaaخaaاaaرaaجaaي مaaن اaaلaaسaaدaaيaaم هaaو لaaأaaكaaسaaجaaيaaن طaaبaaيaaعaaي, وaaاaaلaaأaaخaaضaaر لaaكaaبaaرaaيaaت مaaتaaأaaيaaن فaaرaaدaaيaaاaaً, وaaاaaلaaأaaحaaمaaر لaaأaaكaaسaaجaaيaaن مaaتaaأaaيaaن.
dinaank
srot HubbleSite: gallery, release.
lekhak NASA, ESA, J. Hester and A. Loll (Arizona State University)
anumati
(is faail ki pun: upayog)

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.

laaisensing[sampaadan]

Public domain 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.
Hubble 01.jpg
Annotations This image is annotated: View the annotations at Commons

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vartamaan 14:56, 25 November 2012 14:56, 25 नवम्बर 2012 के संस्करण का अंगूठाकार प्रारूप। 3,864 × 3,864 (13.84 MB) Hawky.diddiz Lossless optimization
10:13, 17 May 2012 10:13, 17 मई 2012 के संस्करण का अंगूठाकार प्रारूप। 3,864 × 3,864 (14.61 MB) Metróanomo Higher quality
09:31, 20 June 2009 09:31, 20 जून 2009 के संस्करण का अंगूठाकार प्रारूप। 3,864 × 3,864 (6.18 MB) Tryphon Higher resolution.
21:26, 9 March 2006 21:26, 9 मार्च 2006 के संस्करण का अंगूठाकार प्रारूप। 2,224 × 2,212 (3.08 MB) Stianbh larger version
00:35, 16 January 2006 00:35, 16 जनवरी 2006 के संस्करण का अंगूठाकार प्रारूप। 400 × 400 (23 KB) DragonFire1024 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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