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İzahNGC 6753 - HST Potw1738a.tif
English: More than meets the eye
Despite the advances made in past decades, the process of galaxy formation remains an open question in astronomy. Various theories have been suggested, but since galaxies come in all shapes and sizes — including elliptical, spiral, and irregular — no single theory has so far been able to satisfactorily explain the origins of all the galaxies we see throughout the Universe.
To determine which formation model is correct (if any), astronomers hunt for the telltale signs of various physical processes. One example of this is galactic coronas, which are huge, invisible regions of hot gas that surround a galaxy’s visible bulk, forming a spheroidal shape. They are so hot that they can be detected by their X-ray emission, far beyond the optical radius of the galaxy. Because they are so wispy, these coronas are extremely difficult to detect. In 2013, astronomers highlighted NGC 6753, imaged here by the NASA/ESA Hubble Space Telescope, as one of only two known spiral galaxies that were both massive enough and close enough to permit detailed observations of their coronas. Of course, NGC 6753 is only close in astronomical terms — the galaxy is nearly 150 million light-years from Earth.
NGC 6753 is a whirl of colour in this image — the bursts of blue throughout the spiral arms are regions filled with young stars glowing brightly in ultraviolet light, while redder areas are filled with older stars emitting in the cooler near-infrared.
Credit:
ESA/Hubble & NASA Acknowledgement: Judy Schmidt
Coordinates Position (RA): 19 11 23.69 Position (Dec): -57° 2' 52.29" Field of view: 1.84 x 1.83 arcminutes Orientation: North is 18.8° right of vertical
Colours & filters Band Wavelength Telescope Optical U 300 nm Hubble Space Telescope WFPC2 Optical U 300 nm Hubble Space Telescope WFPC2 Optical I 814 nm Hubble Space Telescope WFPC2 Optical I 814 nm Hubble Space Telescope WFPC2
ESA/Hubble images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the hubblesite.org website, or for ESA/Hubble images on the esahubble.org site before 2009, use the {{PD-Hubble}} tag.
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The full image or footage credit must be presented in a clear and readable manner to all users, with the wording unaltered (for example: "ESA/Hubble"). Web texts should be credited to ESA/Hubble (except when used by media). The credit should not be hidden or disassociated from the image footage. Links should be active if the credit is online. See the usage rights Q&A section on the ESA copyright page for guidance.
ESA/Hubble materials may not be used to state or imply the endorsement by ESA/Hubble or any ESA/Hubble employee of a commercial product or service.
ESA/Hubble requests a copy of the product sent to them to be indexed in their archive.
If an image shows an identifiable person, using that image for commercial purposes may infringe that person's right of privacy, and separate permission should be obtained from the individual.
If images or visuals are changed significantly from the original work (apart from resizing, cropping), we suggest that the changes are mentioned after the credit line. For example "Original image by ESA/Hubble (M. Kornmesser), warping and recolouring by NN".
Notes:
Note that this general permission does not extend to the use of ESA/Hubble's logo, which shall remain protected and may not be used or reproduced without prior and individual written consent of ESA/Hubble.
Also note that music, scientific papers and code on the www.esahubble.org site are not released under this license and can not be used for non-ESA/Hubble products.
By reproducing ESA/Hubble material, in part or in full, the user acknowledges the terms on which such use is permitted.
This file is licensed under the Creative Commons Attribution 4.0 International license.
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=={{int:filedesc}}== {{Information |description={{en|1='''More than meets the eye Despite the advances made in past decades, the process of galaxy formation remains an open question in astronomy. Various theories have been suggested, but since galaxie...
Guida alle costellazioni - Regioni celesti scelte/Gruppi di galassie nel Pavone
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Fayl Faylin tarixcesi Fayl kecidleri Faylin qlobal istifadesi MetamelumatlarBu TIF faylin JPG formatindaki bu gorunusunun olcusu 601 600 piksel Diger olculer 240 240 piksel 481 480 piksel 769 768 piksel 1 103 1 101 piksel Faylin orijinali 8206 1 103 1 101 piksel fayl hecmi 2 86 MB MIME novu image tiff Bu fayl Vikimedia Commons dadirve diger layihelerde istifade edile biler Faylin tesvir sehifesine get Xulase IzahNGC 6753 HST Potw1738a tif English More than meets the eye Despite the advances made in past decades the process of galaxy formation remains an open question in astronomy Various theories have been suggested but since galaxies come in all shapes and sizes including elliptical spiral and irregular no single theory has so far been able to satisfactorily explain the origins of all the galaxies we see throughout the Universe To determine which formation model is correct if any astronomers hunt for the telltale signs of various physical processes One example of this is galactic coronas which are huge invisible regions of hot gas that surround a galaxy s visible bulk forming a spheroidal shape They are so hot that they can be detected by their X ray emission far beyond the optical radius of the galaxy Because they are so wispy these coronas are extremely difficult to detect In 2013 astronomers highlighted NGC 6753 imaged here by the NASA ESA Hubble Space Telescope as one of only two known spiral galaxies that were both massive enough and close enough to permit detailed observations of their coronas Of course NGC 6753 is only close in astronomical terms the galaxy is nearly 150 million light years from Earth NGC 6753 is a whirl of colour in this image the bursts of blue throughout the spiral arms are regions filled with young stars glowing brightly in ultraviolet light while redder areas are filled with older stars emitting in the cooler near infrared Credit ESA Hubble amp NASA Acknowledgement Judy Schmidt Coordinates Position RA 19 11 23 69 Position Dec 57 2 52 29 Field of view 1 84 x 1 83 arcminutes Orientation North is 18 8 right of vertical Colours amp filters Band Wavelength Telescope Optical U 300 nm Hubble Space Telescope WFPC2 Optical U 300 nm Hubble Space Telescope WFPC2 Optical I 814 nm Hubble Space Telescope WFPC2 Optical I 814 nm Hubble Space Telescope WFPC2 Tarix 18 sentyabr 2017 06 00 00 Menbe https www spacetelescope org images potw1738a Muellif ESA Hubble amp NASA Acknowledgement Judy Schmidt Lisenziya ESA Hubble images videos and web texts are released by the ESA under the Creative Commons Attribution 4 0 International license and may on a non exclusive basis be reproduced without fee provided they are clearly and visibly credited Detailed conditions are below see the ESA copyright statement for full information For images created by NASA or on the hubblesite org website or for ESA Hubble images on the esahubble org site before 2009 use the PD Hubble tag Conditions The full image or footage credit must be presented in a clear and readable manner to all users with the wording unaltered for example ESA Hubble Web texts should be credited to ESA Hubble except when used by media The credit should not be hidden or disassociated from the image footage Links should be active if the credit is online See the usage rights Q amp A section on the ESA copyright page for guidance ESA Hubble materials may not be used to state or imply the endorsement by ESA Hubble or any ESA Hubble employee of a commercial product or service ESA Hubble requests a copy of the product sent to them to be indexed in their archive If an image shows an identifiable person using that image for commercial purposes may infringe that person s right of privacy and separate permission should be obtained from the individual If images or visuals are changed significantly from the original work apart from resizing cropping we suggest that the changes are mentioned after the credit line For example Original image by ESA Hubble M Kornmesser warping and recolouring by NN Notes Note that this general permission does not extend to the use of ESA Hubble s logo which shall remain protected and may not be used or reproduced without prior and individual written consent of ESA Hubble Also note that music scientific papers and code on the www esahubble org site are not released under this license and can not be used for non ESA Hubble products By reproducing ESA Hubble material in part or in full the user acknowledges the terms on which such use is permitted This file is licensed under the Creative Commons Attribution 4 0 International license Istinad ESA HubbleAzadsiniz 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 4 0 CC BY 4 0 Creative Commons Attribution 4 0 true trueCaptionsazerbaycancaAdd a one line explanation of what this file representsItems portrayed in this filetesvir edircopyright status nbsp ingiliscopyrighted nbsp ingilislisenziyaCreative Commons Attribution 4 0 International nbsp ingilisyaranma tarixi18 sentyabr 2017 Faylin tarixcesi Faylin evvelki versiyasini gormek ucun gun tarix bolmesindeki tarixlere klikleyin Tarix VaxtKicik sekilOlculerIstifadeciSerh indiki09 02 18 sentyabr 20171 103 1 101 2 86 MB Fabian RRRR int filedesc Information description en 1 039 039 039 More than meets the eye Despite the advances made in past decades the process of galaxy formation remains an open question in astronomy Various theories have been suggested but since galaxie Fayl kecidleri Bu sekile olan kecidler NGC 6753 Faylin qlobal istifadesi Bu fayl asagidaki vikilerde istifade olunur de wikipedia org layihesinde istifadesi NGC 6753 hr wikipedia org layihesinde istifadesi NGC 6753 it wikibooks org layihesinde istifadesi Guida alle costellazioni Regioni celesti scelte Gruppi di galassie nel Pavone kk wikipedia org layihesinde istifadesi NGC 6753 pt wikipedia org layihesinde istifadesi NGC 6753 sr wikipedia org layihesinde istifadesi NGC 6753 tr wikipedia org layihesinde istifadesi NGC 6753 uz wikipedia org layihesinde istifadesi NGC 6753Metamelumatlar Bu faylda fotoaparat ve ya skanerle elave olunmus melumatlar var Eger fayl sonradan redakte olunubsa bezi parametrler bu sekilde gosterilenlerden ferqli ola biler Genislik1 103 pxHundurluk1 101 pxBits per component8 8 8SixilmamisLZWReng modeliRGBOrientasiyaNormalReng komponentlerinin sayi3Her blokdaki setirlerin sayi79Ufuqi xett72 dpiSaquli xett72 dpiData arrangementchunky formatProqram teminatiAdobe Photoshop CC 2015 Windows Faylin deyismesi tarixi ve vaxti14 02 9 iyun 2017Reng sahesiFotosekilde reng secimi edilmemisdir Menbe https az wikipedia org wiki Fayl NGC 6753 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