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From the NASA press release:

Remnants from a star that exploded thousands of years ago created a celestial abstract portrait, as captured in this NASA Hubble Space Telescope image of the Pencil Nebula.
Officially known as NGC 2736, the Pencil Nebula is part of the huge Vela supernova remnant, located in the southern constellation Vela. Discovered by Sir John Herschel in the 1840s, the nebula's linear appearance triggered its popular name. The nebula's shape suggests that it is part of the supernova shock wave that recently encountered a region of dense gas. It is this interaction that causes the nebula to glow, appearing like a rippled sheet.
In this snapshot, astronomers are looking along the edge of the undulating sheet of gas. This view shows large, wispy filamentary structures, smaller bright knots of gas, and patches of diffuse gas. The Hubble Heritage Team used the Advanced Camera for Surveys in October 2002 to observe the nebula. The region of the Pencil Nebula captured in this image is about three fourths of a light-year across. The Vela supernova remnant is 114 light-years (35 parsecs) across. The remnant is about 815 light-years (250 parsecs) away from our solar system.
The nebula's luminous appearance comes from dense gas regions that have been struck by the supernova shock wave. As the shock wave travels through space [from right to left in the image], it rams into interstellar material. Initially the gas is heated to millions of degrees, but then subsequently cools down, emitting the optical light visible in the image.
The colors of the various regions in the nebula yield clues about this cooling process. Some regions are still so hot that the emission is dominated by ionized oxygen atoms, which glow blue in the picture. Other regions have cooled more and are seen emitting red in the image (cooler hydrogen atoms). In this situation, color shows the temperature of the gas. The nebula is visible in this image because it is glowing.
The supernova explosion left a spinning pulsar at the core of the Vela region. Based on the rate at which the pulsar is slowing down, astronomers estimate that the explosion may have occurred about 11,000 years ago. Although no historical records of the blast exist, the Vela supernova would have been 250 times brighter than Venus and would have been easily visible to southern observers in broad daylight. The age of the blast, if correct, would imply that the initial explosion pushed material from the star at nearly 22 million miles per hour. As the Vela supernova remnant expands, the speed of its moving filaments, such as the Pencil Nebula, decreases. The Pencil Nebula, for example, is moving at roughly 400,000 miles per hour.
Tarix June 5 2003
Mənbə http://hubblesite.org/newscenter/archive/releases/2003/16/image/a (direct link)
Müəllif NASA and The Hubble Heritage Team (STScI/AURA)
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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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indiki23:38, 18 sentyabr 20063.289 × 3.252 (10,13 MB)WilliamKF{{Information| |Description=From the NASA press release: :Remnants from a star that exploded thousands of years ago created a celestial abstract portrait, as captured in this NASA Hubble Space Telescope image of the Pencil Nebula. :Officially known as N

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  • NGC 2736
  • Contact (1997 US film)
  • John Herschel
  • Wikiquote:Quote of the day/November 2010
  • Wikiquote:Quote of the day/November 9, 2010
  • Love
  • Wikiquote:Quote of the day/March 2020
  • Wikiquote:Quote of the day/March 7, 2020
  • Anexo:Objetos del catálogo NGC (2000-2999)
  • Межзвёздная среда
  • Portál:Astronómia/Obrázky týždňa (2008)
  • Portál:Astronómia/Obrázok týždňa/38 2008
  • Portal:Astronomi/Veckans bild/Vecka 51
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    fayl, pencil, 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, image,. Fayl Faylin tarixcesi Fayl kecidleri Faylin qlobal istifadesi MetamelumatlarSinaq gosterisi olcusu 606 599 piksel Diger olculer 243 240 piksel 485 480 piksel 777 768 piksel 1 036 1 024 piksel 2 071 2 048 piksel 3 289 3 252 piksel Faylin orijinali 8206 3 289 3 252 piksel fayl hecmi 10 13 MB MIME novu image jpeg Bu fayl Vikimedia Commons dadirve diger layihelerde istifade edile biler Faylin tesvir sehifesine get IzahPencil hst big jpg From the NASA press release Remnants from a star that exploded thousands of years ago created a celestial abstract portrait as captured in this NASA Hubble Space Telescope image of the Pencil Nebula Officially known as NGC 2736 the Pencil Nebula is part of the huge Vela supernova remnant located in the southern constellation Vela Discovered by Sir John Herschel in the 1840s the nebula s linear appearance triggered its popular name The nebula s shape suggests that it is part of the supernova shock wave that recently encountered a region of dense gas It is this interaction that causes the nebula to glow appearing like a rippled sheet In this snapshot astronomers are looking along the edge of the undulating sheet of gas This view shows large wispy filamentary structures smaller bright knots of gas and patches of diffuse gas The Hubble Heritage Team used the Advanced Camera for Surveys in October 2002 to observe the nebula The region of the Pencil Nebula captured in this image is about three fourths of a light year across The Vela supernova remnant is 114 light years 35 parsecs across The remnant is about 815 light years 250 parsecs away from our solar system The nebula s luminous appearance comes from dense gas regions that have been struck by the supernova shock wave As the shock wave travels through space from right to left in the image it rams into interstellar material Initially the gas is heated to millions of degrees but then subsequently cools down emitting the optical light visible in the image The colors of the various regions in the nebula yield clues about this cooling process Some regions are still so hot that the emission is dominated by ionized oxygen atoms which glow blue in the picture Other regions have cooled more and are seen emitting red in the image cooler hydrogen atoms In this situation color shows the temperature of the gas The nebula is visible in this image because it is glowing The supernova explosion left a spinning pulsar at the core of the Vela region Based on the rate at which the pulsar is slowing down astronomers estimate that the explosion may have occurred about 11 000 years ago Although no historical records of the blast exist the Vela supernova would have been 250 times brighter than Venus and would have been easily visible to southern observers in broad daylight The age of the blast if correct would imply that the initial explosion pushed material from the star at nearly 22 million miles per hour As the Vela supernova remnant expands the speed of its moving filaments such as the Pencil Nebula decreases The Pencil Nebula for example is moving at roughly 400 000 miles per hour Tarix June 5 2003 Menbe http hubblesite org newscenter archive releases 2003 16 image a direct link Muellif NASA and The Hubble Heritage Team STScI AURA Icaze Faylin tekrar istifadesi 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 Faylin tarixcesi Faylin evvelki versiyasini gormek ucun gun tarix bolmesindeki tarixlere klikleyin Tarix VaxtKicik sekilOlculerIstifadeciSerh indiki23 38 18 sentyabr 20063 289 3 252 10 13 MB WilliamKF Information Description From the NASA press release Remnants from a star that exploded thousands of years ago created a celestial abstract portrait as captured in this NASA Hubble Space Telescope image of the Pencil Nebula Officially known as N Fayl kecidleri Bu sekile olan kecidler NGC 2736 Faylin qlobal istifadesi Bu fayl asagidaki vikilerde istifade olunur ar wikipedia org layihesinde istifadesi سديم القلم ast wikipedia org layihesinde istifadesi Llista d oxetos del catalogu NGC 2000 2999 be wikipedia org layihesinde istifadesi NGC 2736 cs wikipedia org layihesinde istifadesi John Herschel NGC 2736 de wikipedia org layihesinde istifadesi Bleistiftnebel en wikipedia org layihesinde istifadesi NGC 2736 en wikiquote org layihesinde istifadesi Carl Sagan Contact 1997 US film John Herschel Wikiquote Quote of the day November 2010 Wikiquote Quote of the day November 9 2010 Love Wikiquote Quote of the day March 2020 Wikiquote Quote of the day March 7 2020 eo wikipedia org layihesinde istifadesi NGC 2736 es wikipedia org layihesinde istifadesi Portal Exploracion espacial IDD 7 01 2008 Anexo Objetos del catalogo NGC 2000 2999 fr wikipedia org layihesinde istifadesi Nebuleuse du Crayon hr wikipedia org layihesinde istifadesi NGC 2736 hu wikipedia org layihesinde istifadesi Csillagkozi anyag it wikipedia org layihesinde istifadesi NGC 2736 kk wikipedia org layihesinde istifadesi NGC 2736 ko wikipedia org layihesinde istifadesi 연필 성운 lb wikipedia org layihesinde istifadesi NGC 2736 mk wikipedia org layihesinde istifadesi Moliv maglina pl wikipedia org layihesinde istifadesi NGC 2736 pt wikipedia org layihesinde istifadesi NGC 2736 ro wikipedia org layihesinde istifadesi Pulsar ru wikipedia org layihesinde istifadesi NGC 2736 Mezhzvyozdnaya sreda sk wikipedia org layihesinde istifadesi NGC 2736 Portal Astronomia Obrazky tyzdna 2008 Portal Astronomia Obrazok tyzdna 38 2008 sr wikipedia org layihesinde istifadesi NGC 2736 sv wikipedia org layihesinde istifadesi Portal Astronomi Veckans bild V 43 Portal Astronomi Veckans bild Vecka 51 tr wikipedia org layihesinde istifadesi NGC 2736 tr wikiquote org layihesinde istifadesi Carl Sagan uk wikipedia org layihesinde istifadesi NGC 2736 uz wikipedia org layihesinde istifadesi NGC 2736 vi wikipedia org layihesinde istifadesi NGC 2736 zh wikipedia org layihesinde istifadesi NGC 2736Metamelumatlar Bu faylda fotoaparat ve ya skanerle elave olunmus melumatlar var Eger fayl sonradan redakte olunubsa bezi parametrler bu sekilde gosterilenlerden ferqli ola biler Sekil basligiIDL TIFF fileOrientasiyaNormalUfuqi xett100 dpiSaquli xett100 dpiProqram teminatiAdobe Photoshop 7 0Faylin deyismesi tarixi ve vaxti11 09 20 may 2003Reng sahesiFotosekilde reng secimi edilmemisdir Menbe https az wikipedia org wiki Fayl Pencil hst big jpg, wikipedia, oxu, kitab, kitabxana, axtar, tap, hersey,

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