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İzahFrom microwaves to megamasers.jpg
English: Phenomena across the Universe emit radiation spanning the entire electromagnetic spectrum — from high-energy gamma rays, which stream out from the most energetic events in the cosmos, to lower-energy microwaves and radio waves.
Microwaves, the very same radiation that can heat up your dinner, are produced by a multitude of astrophysical sources, including strong emitters known as masers (microwave lasers), even stronger emitters with the somewhat villainous name of megamasers, and the centres of some galaxies. Especially intense and luminous galactic centres are known as active galactic nuclei. They are in turn thought to be driven by the presence of supermassive black holes, which drag surrounding material inwards and spit out bright jets and radiation as they do so.
The two galaxies shown here, imaged by the NASA/ESA Hubble Space Telescope, are named MCG+01-38-004 (the upper, red-tinted one) and MCG+01-38-005 (the lower, blue-tinted one). MCG+01-38-005 is a special kind of megamaser; the galaxy’s active galactic nucleus pumps out huge amounts of energy, which stimulates clouds of surrounding water. Water’s constituent atoms of hydrogen and oxygen are able to absorb some of this energy and re-emit it at specific wavelengths, one of which falls within the microwave regime. MCG+01-38-005 is thus known as a water megamaser!
Astronomers can use such objects to probe the fundamental properties of the Universe. The microwave emissions from MCG+01-38-005 were used to calculate a refined value for the Hubble constant, a measure of how fast the Universe is expanding. This constant is named after the astronomer whose observations were responsible for the discovery of the expanding Universe and after whom the Hubble Space Telescope was named, Edwin Hubble.
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&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 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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From microwaves to megamasers
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Phenomena across the Universe emit radiation spanning the entire electromagnetic spectrum — from high-energy gamma rays, which stream out from the most energetic events in the cosmos, to lower-energy microwaves and radio waves. Microwaves, the very same radiation that can heat up your dinner, are produced by a multitude of astrophysical sources, including strong emitters known as masers (microwave lasers), even stronger emitters with the somewhat villainous name of megamasers, and the centres of some galaxies. Especially intense and luminous galactic centres are known as active galactic nuclei. They are in turn thought to be driven by the presence of supermassive black holes, which drag surrounding material inwards and spit out bright jets and radiation as they do so. The two galaxies shown here, imaged by the NASA/ESA Hubble Space Telescope, are named MCG+01-38-004 (the upper, red-tinted one) and MCG+01-38-005 (the lower, blue-tinted one). MCG+01-38-005 is a special kind of megamaser; the galaxy’s active galactic nucleus pumps out huge amounts of energy, which stimulates clouds of surrounding water. Water’s constituent atoms of hydrogen and oxygen are able to absorb some of this energy and re-emit it at specific wavelengths, one of which falls within the microwave regime. MCG+01-38-005 is thus known as a water megamaser! Astronomers can use such objects to probe the fundamental properties of the Universe. The microwave emissions from MCG+01-38-005 were used to calculate a refined value for the Hubble constant, a measure of how fast the Universe is expanding. This constant is named after the astronomer whose observations were responsible for the discovery of the expanding Universe and after whom the Hubble Space Telescope was named, Edwin Hubble.
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fayl, from, microwaves, megamasers, 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, həc. Fayl Faylin tarixcesi Fayl kecidleri Faylin qlobal istifadesi MetamelumatlarSinaq gosterisi olcusu 800 469 piksel Diger olculer 320 187 piksel 640 375 piksel 1 024 600 piksel 1 280 750 piksel 2 560 1 500 piksel 3 766 2 206 piksel Faylin orijinali 8206 3 766 2 206 piksel fayl hecmi 1 62 MB MIME novu image jpeg Bu fayl Vikimedia Commons dadirve diger layihelerde istifade edile biler Faylin tesvir sehifesine get Xulase IzahFrom microwaves to megamasers jpg English Phenomena across the Universe emit radiation spanning the entire electromagnetic spectrum from high energy gamma rays which stream out from the most energetic events in the cosmos to lower energy microwaves and radio waves Microwaves the very same radiation that can heat up your dinner are produced by a multitude of astrophysical sources including strong emitters known as masers microwave lasers even stronger emitters with the somewhat villainous name of megamasers and the centres of some galaxies Especially intense and luminous galactic centres are known as active galactic nuclei They are in turn thought to be driven by the presence of supermassive black holes which drag surrounding material inwards and spit out bright jets and radiation as they do so The two galaxies shown here imaged by the NASA ESA Hubble Space Telescope are named MCG 01 38 004 the upper red tinted one and MCG 01 38 005 the lower blue tinted one MCG 01 38 005 is a special kind of megamaser the galaxy s active galactic nucleus pumps out huge amounts of energy which stimulates clouds of surrounding water Water s constituent atoms of hydrogen and oxygen are able to absorb some of this energy and re emit it at specific wavelengths one of which falls within the microwave regime MCG 01 38 005 is thus known as a water megamaser Astronomers can use such objects to probe the fundamental properties of the Universe The microwave emissions from MCG 01 38 005 were used to calculate a refined value for the Hubble constant a measure of how fast the Universe is expanding This constant is named after the astronomer whose observations were responsible for the discovery of the expanding Universe and after whom the Hubble Space Telescope was named Edwin Hubble Tarix 28 avqust 2017 06 00 00 Menbe https www spacetelescope org images potw1735a Muellif ESA Hubble amp NASA 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 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 tarixi28 avqust 2017 Faylin tarixcesi Faylin evvelki versiyasini gormek ucun gun tarix bolmesindeki tarixlere klikleyin Tarix VaxtKicik sekilOlculerIstifadeciSerh indiki08 23 28 avqust 20173 766 2 206 1 62 MB JmencisomUser created page with UploadWizard Fayl kecidleri Bu sekile olan kecidler NGC 5765 Faylin qlobal istifadesi Bu fayl asagidaki vikilerde istifade olunur arz wikipedia org layihesinde istifadesi NGC 5765B مجره be wikipedia org layihesinde istifadesi NGC 5765 ce wikipedia org layihesinde istifadesi NGC 5765 de wikipedia org layihesinde istifadesi NGC 5765 diq wikipedia org layihesinde istifadesi NGC 5765 en wikipedia org layihesinde istifadesi Megamaser NGC 5765 en wikiversity org layihesinde istifadesi User Marshallsumter Radiation astronomy1 Microwaves User Marshallsumter Radiation astronomy1 Galaxies User Marshallsumter Radiation astronomy Active galactic nuclei User Marshallsumter Radiation astronomy1 Holes eu wikipedia org layihesinde istifadesi NGC 5765 fr wikipedia org layihesinde istifadesi Discussion Wikipedia Projets pedagogiques Cegep de Chicoutimi Galaxie de Seyfert NGC 5765 id wikipedia org layihesinde istifadesi Megamaser mk wikipedia org layihesinde istifadesi NGC 5765 NGC 5765B nl wikipedia org layihesinde istifadesi NGC 5765 NGC 5765B pl wikipedia org layihesinde istifadesi NGC 5765 pt wikipedia org layihesinde istifadesi NGC 5765 ru wikipedia org layihesinde istifadesi NGC 5765 sk wikipedia org layihesinde istifadesi NGC 5765 tr wikipedia org layihesinde istifadesi NGC 5765 tt wikipedia org layihesinde istifadesi NGC 5765 www wikidata org layihesinde istifadesi Q1122702Metamelumatlar Bu faylda fotoaparat ve ya skanerle elave olunmus melumatlar var Eger fayl sonradan redakte olunubsa bezi parametrler bu sekilde gosterilenlerden ferqli ola biler Temin ediciESA Hubble amp NASAMenbeESA HubbleQisa basliqFrom microwaves to megamasersSekil basligiPhenomena across the Universe emit radiation spanning the entire electromagnetic spectrum from high energy gamma rays which stream out from the most energetic events in the cosmos to lower energy microwaves and radio waves Microwaves the very same radiation that can heat up your dinner are produced by a multitude of astrophysical sources including strong emitters known as masers microwave lasers even stronger emitters with the somewhat villainous name of megamasers and the centres of some galaxies Especially intense and luminous galactic centres are known as active galactic nuclei They are in turn thought to be driven by the presence of supermassive black holes which drag surrounding material inwards and spit out bright jets and radiation as they do so The two galaxies shown here imaged by the NASA ESA Hubble Space Telescope are named MCG 01 38 004 the upper red tinted one and MCG 01 38 005 the lower blue tinted one MCG 01 38 005 is a special kind of megamaser the galaxy s active galactic nucleus pumps out huge amounts of energy which stimulates clouds of surrounding water Water s constituent atoms of hydrogen and oxygen are able to absorb some of this energy and re emit it at specific wavelengths one of which falls within the microwave regime MCG 01 38 005 is thus known as a water megamaser Astronomers can use such objects to probe the fundamental properties of the Universe The microwave emissions from MCG 01 38 005 were used to calculate a refined value for the Hubble constant a measure of how fast the Universe is expanding This constant is named after the astronomer whose observations were responsible for the discovery of the expanding Universe and after whom the Hubble Space Telescope was named Edwin Hubble 160 Istifade qaydasiCreative Commons Attribution 4 0 International LicenseOrijinal tarix ve vaxt06 00 28 avqust 2017Proqram teminatiAdobe Photoshop CC 2015 5 Windows Faylin deyismesi tarixi ve vaxti17 17 7 noyabr 2016Tarix ve vaxt reqemlesdirilir20 35 21 oktyabr 2016Date metadata was last modified18 17 7 noyabr 2016Unique ID of original documentxmp did 3a14ea89 3da6 1e4c 93d0 ed564bfc6986Acar sozlerMCG 01 38 004 MCG 01 38 005Elaqe melumatihttp www spacetelescope org Karl Schwarzschild Strasse 2Garching bei Munchen D 85748 GermanyIIM versiya4 Menbe https az wikipedia org wiki Fayl From microwaves to megamasers jpg, wikipedia, oxu, kitab, kitabxana, axtar, tap, hersey,
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