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Caldwell 109

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English: The final item in the Caldwell catalog, Caldwell 109 resembles a phantom snowball. The glowing shroud of gas was shed by its central star in a final act before dying. Like all stars, the one in the middle of this nebula spent its life participating in a precarious balance act, with the outward pressure generated by nuclear fusion countered by the inward pull of gravity. During most of the star’s lifetime the two held an uneasy truce, making the star a giant, controlled nuclear bomb.

When the star began to exhaust its hydrogen fuel, however, there wasn’t enough pressure to fight off gravity. The core began to contract, becoming denser and hotter, triggering the fusion of helium into carbon. The heat produced caused the star’s outer layers of gas to expand, transforming the star into a red giant. After spending about a billion years as a red giant, the star began a 10,000-year process to shed its outer layers of gas, ultimately uncovering the remaining core of the star — a white dwarf. High-energy radiation from the white dwarf makes the cast-off gaseous layers glow, creating a ghostly specter in the night sky. In tens of thousands of years, Caldwell 109 will fade into darkness as the white dwarf cools like an ember until it finally burns out completely.

Planetary nebulas like Caldwell 109 are especially interesting to scientists because they represent a future stage of our own Sun, which is destined to meet a similar fate in about 6 billion years. This Hubble image was taken in visible and infrared light using the Wide Field and Planetary Camera 2 as part of a survey of planetary nebulas. The observations revealed many surprisingly intricate, glowing patterns spun into space by aging stars: pinwheels, lawn-sprinkler–style jets, elegant goblet shapes and even some that look like a rocket engine’s exhaust.

Caldwell 109 was discovered by John Herschel in 1835 and subsequently cataloged as NGC 3195. It lies 5,500 light-years away toward the Chamaeleon constellation. It is visible year-round from the Southern Hemisphere but is highest in the autumn. With a magnitude of 11.6 it can be a challenging target to spot for small telescopes. Through a moderate-sized telescope, Caldwell 109 will look like a swollen star.

For more information about Hubble’s observations of Caldwell 109, see:

www.spacetelescope.org/images/opo9738c12/

hubblesite.org/contents/news-releases/1997/news-1997-38.html

Credit: NASA, ESA and Howard Bond (STScI); Processing: Gladys Kober (NASA/Catholic University of America)

For Hubble's Caldwell catalog site and information on how to find these objects in the night sky, visit:

www.nasa.gov/content/goddard/hubble-s-caldwell-catalog
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This image was originally posted to Flickr by NASA Hubble at https://flickr.com/photos/144614754@N02/49214703236 (). It was reviewed on 23 fevral 2020 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc-by-2.0.

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Caldwell 109

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NGC 3195

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17 dekabr 1997

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fayl, caldwell, fayl, faylın, tarixçəsi, fayl, keçidləri, faylın, qlobal, istifadəsi, metaməlumatlardaha, yüksək, versiyası, yoxdur, caldwell, 8206, piksel, fayl, həcmi, mime, növü, image, jpeg, fayl, vikimedia, commons, dadırvə, digər, layihələrdə, istifadə, . Fayl Faylin tarixcesi Fayl kecidleri Faylin qlobal istifadesi MetamelumatlarDaha yuksek versiyasi yoxdur Caldwell 109 jpg 8206 464 471 piksel fayl hecmi 209 KB MIME novu image jpeg Bu fayl Vikimedia Commons dadirve diger layihelerde istifade edile biler Faylin tesvir sehifesine get Xulase IzahCaldwell 109 jpg English The final item in the Caldwell catalog Caldwell 109 resembles a phantom snowball The glowing shroud of gas was shed by its central star in a final act before dying Like all stars the one in the middle of this nebula spent its life participating in a precarious balance act with the outward pressure generated by nuclear fusion countered by the inward pull of gravity During most of the star s lifetime the two held an uneasy truce making the star a giant controlled nuclear bomb When the star began to exhaust its hydrogen fuel however there wasn t enough pressure to fight off gravity The core began to contract becoming denser and hotter triggering the fusion of helium into carbon The heat produced caused the star s outer layers of gas to expand transforming the star into a red giant After spending about a billion years as a red giant the star began a 10 000 year process to shed its outer layers of gas ultimately uncovering the remaining core of the star a white dwarf High energy radiation from the white dwarf makes the cast off gaseous layers glow creating a ghostly specter in the night sky In tens of thousands of years Caldwell 109 will fade into darkness as the white dwarf cools like an ember until it finally burns out completely Planetary nebulas like Caldwell 109 are especially interesting to scientists because they represent a future stage of our own Sun which is destined to meet a similar fate in about 6 billion years This Hubble image was taken in visible and infrared light using the Wide Field and Planetary Camera 2 as part of a survey of planetary nebulas The observations revealed many surprisingly intricate glowing patterns spun into space by aging stars pinwheels lawn sprinkler style jets elegant goblet shapes and even some that look like a rocket engine s exhaust Caldwell 109 was discovered by John Herschel in 1835 and subsequently cataloged as NGC 3195 It lies 5 500 light years away toward the Chamaeleon constellation It is visible year round from the Southern Hemisphere but is highest in the autumn With a magnitude of 11 6 it can be a challenging target to spot for small telescopes Through a moderate sized telescope Caldwell 109 will look like a swollen star For more information about Hubble s observations of Caldwell 109 see www spacetelescope org images opo9738c12 hubblesite org contents news releases 1997 news 1997 38 htmlCredit NASA ESA and Howard Bond STScI Processing Gladys Kober NASA Catholic University of America For Hubble s Caldwell catalog site and information on how to find these objects in the night sky visit www nasa gov content goddard hubble s caldwell catalog Tarix 17 dekabr 1997 06 00 00 Menbe https www flickr com photos 144614754 N02 49214703236 Muellif NASA Hubble Lisenziya Bu fayl Creative Commons Attribution 2 0 Generic lisenziyasi altinda yayimlanir Azadsiniz paylasmaq eseri kocurmek paylamaq ve oturmek ucun remiks etmek eseri adaptasiya etmek Asagidaki sertlere riayet etmekle istinad Muvafiq kredit vermelisiniz lisenziyaya bir kecid vermelisiniz ve deyisikliklerin olub olmadigini bildirmelisiniz Bunu her hansi bir aglabatan sekilde ede bilersiniz ancaq lisenziyalasdiricinin sizi ve ya istifadenizi tesdiqlemesini teklif eden bir sekilde deyil https creativecommons org licenses by 2 0 CC BY 2 0 Creative Commons Attribution 2 0 true true This image was originally posted to Flickr by NASA Hubble at https flickr com photos 144614754 N02 49214703236 nbsp archive It was reviewed on 23 fevral 2020 by FlickreviewR 2 and was confirmed to be licensed under the terms of the cc by 2 0 23 fevral 2020CaptionsazerbaycancaAdd a one line explanation of what this file representsingilisCaldwell 109Items portrayed in this filetesvir edirNGC 3195Planetar dumanliqBuqelemunyaradiciSome value without a Vikiverilenler itemmuellifin qisa adi NASA Hubblecopyright status nbsp ingiliscopyrighted nbsp ingilislisenziyaCreative Commons Attribution 2 0 Generic nbsp ingilisyaranma tarixi17 dekabr 1997source of file nbsp ingilisfile available on the internet nbsp ingilisistifadeci Flickrdescribed at URL nbsp ingilis https www flickr com photos 144614754 N02 49214703236MIME type nbsp ingilisimage jpeg Faylin tarixcesi Faylin evvelki versiyasini gormek ucun gun tarix bolmesindeki tarixlere klikleyin Tarix VaxtKicik sekilOlculerIstifadeciSerh indiki20 02 23 fevral 2020464 471 209 KB KillarneeUser created page with UploadWizard Fayl kecidleri Bu sekile olan kecidler NGC 3195 Faylin qlobal istifadesi Bu fayl asagidaki vikilerde istifade olunur ce wikipedia org layihesinde istifadesi NGC 3195 diq wikipedia org layihesinde istifadesi NGC 3195 pl wikipedia org layihesinde istifadesi NGC 3195 ru wikipedia org layihesinde istifadesi NGC 3195 tt wikipedia org layihesinde istifadesi NGC 3195 www wikidata org layihesinde istifadesi Q241301Metamelumatlar Bu faylda fotoaparat ve ya skanerle elave olunmus melumatlar var Eger fayl sonradan redakte olunubsa bezi parametrler bu sekilde gosterilenlerden ferqli ola biler Sekil basligiThis image is a part of the Hubble Gallery of Planetary Nebulae Orijinal tarix ve vaxt06 00 17 dekabr 1997Qisa basliqNGC 3195Temin ediciHoward Bond ST ScI and NASA ESMenbeESA HubbleNasirESA HubbleIstifade qaydasiCreative Commons Attribution 4 0 International LicenseJPEG sekil serhiThis image is a part of the Hubble Gallery of Planetary Nebulae OrientasiyaNormalUfuqi xett72 dpiSaquli xett72 dpiProqram teminatiAdobe Photoshop CC 2018 Macintosh Faylin deyismesi tarixi ve vaxti10 17 15 noyabr 2019Y ve C komponetlerine gore yerlesme sirasiMerkezlesdirilmisExif versiyasi2 31Tarix ve vaxt reqemlesdirilir17 49 9 dekabr 2003Meaning of each componentY Cb Cr movcud deyilSupported Flashpix version1Reng sahesisRGBIIM versiya4Acar sozlerIRAS 10099 8036 NGC 3195Bits per component8 8 8SixilmamisSixilmisHundurluk471 pxGenislik464 pxReng modeliRGBReng komponentlerinin sayi3Elaqe melumatihttp www spacetelescope org Karl Schwarzschild Strasse 2Garching bei Munchen D 85748 GermanyMedianin tipiObservationDate metadata was last modified05 17 15 noyabr 2019Unique ID of original documentadobe docid photoshop a591f0f7 2a67 11d8 8281 a580eb5b60aaStatusun muelliflik huququMuelliflik huququ gosterilmeyib Menbe https az wikipedia org wiki Fayl Caldwell 109 jpg, wikipedia, oxu, kitab, kitabxana, axtar, tap, hersey,

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