English: Artist's rendition of a black hole with an orbiting companion star that overflows its Roche lobe. Mass from the companion star is drawn towards the black hole, forming an accretion disk. GRO J1655-40 is the second so-called 'microquasar' discovered in our Galaxy. Microquasars are black holes of about the same mass as a star. They behave as scaled-down versions of much more massive black holes that are at the cores of extremely active galaxies, called quasars. Astronomers have known about the existence of stellar-mass black holes since the early 1970s. Their masses can range from 3.5 to approximately 15 times the mass of our Sun. Using Hubble data, astronomers were able to describe the black-hole system. The companion star had apparently survived the original supernova explosion that created the black hole. It is an aging star that completes an orbit around the black hole every 2.6 days. It is being slowly devoured by the black hole. Blowtorch-like jets (shown in blue) are streaming away from the black-hole system at 90 percent of the speed of light.
ESA, NASA, and Felix Mirabel (French Atomic Energy Commission and Institute for Astronomy and Space Physics/Conicet of Argentina)
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ไฟล, accretion, disk, ไฟล, ประว, ไฟล, หน, าท, ภาพน, การใช, ไฟล, วนกลางขนาดของต, วอย, างน, กเซล, ความละเอ, ยดอ, กเซล, กเซล, กเซล, กเซล, กเซล, กเซล, ภาพท, ความละเอ, ยดส, งกว, 8206, กเซล, ขนาดไฟล, โลไบต, ชน, ดไมม, image, jpeg, ปภาพหร, อไฟล, เส, ยงน, นฉบ, บอย, คอม. ifl prawtiifl hnathimiphaphni karichiflswnklangkhnadkhxngtwxyangni 750 600 phikesl khwamlaexiydxun 300 240 phikesl 600 480 phikesl 960 768 phikesl 1 280 1 024 phikesl 2 560 2 048 phikesl 3 000 2 400 phikesl duphaphthimikhwamlaexiydsungkwa 8206 3 000 2 400 phikesl khnadifl 679 kiolibt chnidimm image jpeg rupphaphhruxiflesiyngni tnchbbxyuthi khxmmxns raylaexiyddanlang epnkhxkhwamthiaesdngphlcak ifltnchbbinkhxmmxns khxmmxnsepnewbistinokhrngkarsahrbekbrwbrwmsuxesri thi khunsamarthchwyid khwamyx khaxthibayAccretion disk jpg English Artist s rendition of a black hole with an orbiting companion star that overflows its Roche lobe Mass from the companion star is drawn towards the black hole forming an accretion disk GRO J1655 40 is the second so called microquasar discovered in our Galaxy Microquasars are black holes of about the same mass as a star They behave as scaled down versions of much more massive black holes that are at the cores of extremely active galaxies called quasars Astronomers have known about the existence of stellar mass black holes since the early 1970s Their masses can range from 3 5 to approximately 15 times the mass of our Sun Using Hubble data astronomers were able to describe the black hole system The companion star had apparently survived the original supernova explosion that created the black hole It is an aging star that completes an orbit around the black hole every 2 6 days It is being slowly devoured by the black hole Blowtorch like jets shown in blue are streaming away from the black hole system at 90 percent of the speed of light wnthi 18 phvscikayn ph s 2545 released aehlngthima https hubblesite org contents media images 2002 30 1273 Image html phusrangsrrkh ESA NASA and Felix Mirabel French Atomic Energy Commission and Institute for Astronomy and Space Physics Conicet of Argentina karxnuyatichsiththi 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 iflnixyuphayitsyyaxnuyatkhriexthifkhxmmxns run aesdngthima 4 0 nanachatikaraesdngthima ESA Hubblekhunsamarth thicaaebngpn thicathasaena aeckcay aelasngngandngklawtxip thicaeriyberiyngihm thicaddaeplngngandngklaw phayitenguxnikhtxipni aesdngthima khuntxngihekiyrtiecakhxngnganxyangehmaasm odyephimlingkipyngsyyaxnuyat aelarabuhakmikarepliynaeplng khunxacthaechnniidinrupaebbidkidtamkhwr aettxngimichinlksnathiaenawaphuihxnuyatsnbsnunkhunhruxkarichngankhxngkhunhttps creativecommons org licenses by 4 0 CC BY 4 0 Creative Commons Attribution 4 0 true true This file which was originally posted to Hubble Site was reviewed on 17 May 2020 by reviewer Green Giant who confirmed that it was available there under the stated license on that date khabrryayodyyxithyephimkhabrryaythrrthdediywephuxkhyaykhwamwaiflnimixairxngkvsArtist s View of Black Hole and Companion Star GRO J1655 40ixethmthiaesdngxyuiniflniprakxbdwysthanalikhsiththimilikhsiththisyyaxnuyatCreative Commons Attribution 4 0 International nbsp xngkvswnthisrang wnkxtng18 phvscikayn 2002 prawtiifl khlikwnthi ewlaephuxduiflthipraktinkhnann wnthi ewlarupyxkhnadphuichkhwamehn pccubn22 17 26 emsayn 25623 000 2 400 679 kiolibt FriedrichKiefererBetter quality 06 12 16 minakhm 25483 000 2 400 112 kiolibt Bebenko commonswikicopy paste from english wiki hnathimiphaphni hnatxipni oyngmathiphaphni canphxkphunmwl rabbdawkhurngsiexks hlumda karichiflswnklang wikixuntxipniichiflni karichbn af wikipedia org Swartkolk X straaldubbelster Akkresieskyf karichbn ar wikipedia org ثقب أسود قرص مزود بوابة علم الفلك صورة الأسبوع أرشيف تنامي GRO J1655 40 ثنائي أشعة إكس karichbn ar wikibooks org علم الفلك ثقوب سوداء karichbn ast wikipedia org Acrecimientu Stephen Hawking Teoria de la relativida Cosmos A Spacetime Odyssey Furacu negru estelar Discu d acrecimientu Binaria de Rayos X 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ekhathungcak https th wikipedia org wiki ifl Accretion disk jpg, wikipedia, วิกิ หนังสือ, หนังสือ, ห้องสมุด,
