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M33 X-7

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The main component of this graphic is an artist's representation of M33 X-7, a binary system in the nearby galaxy M33. In this system, a star about 70 times more massive than the Sun (large blue object) is revolving around a black hole. This black hole is almost 16 times the Sun's mass, a record for black holes created from the collapse of a giant star. Other black holes at the centers of galaxies are much more massive, but this object is the record-setter for a so-called "stellar mass" black hole.

In the illustration, an orange disk surrounds the black hole. This depicts material, fed by a wind from the blue companion star, which has been swept into orbit around the black hole. Rather than flowing unimpeded and uniformly into space, wind from the star is pulled towards the black hole by its powerful gravity. The wind that does make it past the black hole is disrupted, causing turbulence and ripples beyond the disk. The companion star itself is also distorted by the gravity from the black hole. The star is stretched slightly in the direction of the black hole, causing it to become less dense in this region and to appear darker.

The inset shows a composite of data from NASA's Chandra X-ray Observatory (blue) and the Hubble Space Telescope. The bright objects in the inset image are young, massive stars around M33 X-7, and the bright, blue Chandra source is M33 X-7 itself. X-rays from Chandra reveals how long the black hole is eclipsed by the companion star, which indicates the size of the companion. Observations by the Gemini telescope on Mauna Kea, Hawaii track the orbital motion of the companion around the black hole, giving information about the mass of the two members of the binary. Other observed properties of the binary were also used to help constrain the mass estimates of both the black hole and its companion.
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Mənbə http://www.nasa.gov/mission_pages/chandra/multimedia/photos07-112.html
Müəllif Illustration: NASA/CXC/M.Weiss; X-ray: NASA/CXC/CfA/P.Plucinsky et al.; Optical: NASA/STScI/SDSU/J.Orosz et al.


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indiki20:42, 21 oktyabr 2007516 × 516 (65 KB)Vaikunda Raja{{PD-NASA}} This image is from [http://www.nasa.gov/mission_pages/chandra/multimedia/photos07-112.html here] Category:Nasa

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    fayl, fayl, faylın, tarixçəsi, istifadə, edilən, səhifələr, faylın, qlobal, istifadəsi, metaməlumatlardaha, yüksək, versiyası, yoxdur, 8206, piksel, fayl, həcmi, mime, növü, image, jpeg, fayl, vikimedia, commons, dadırvə, digər, layihələrdə, istifadə, edilə, b. Fayl Faylin tarixcesi Istifade edilen sehifeler Faylin qlobal istifadesi MetamelumatlarDaha yuksek versiyasi yoxdur M33 X 7 jpg 8206 516 516 piksel fayl hecmi 65 KB MIME novu image jpeg Bu fayl Vikimedia Commons dadirve diger layihelerde istifade edile biler Faylin tesvir sehifesine get IzahM33 X 7 jpg The main component of this graphic is an artist s representation of M33 X 7 a binary system in the nearby galaxy M33 In this system a star about 70 times more massive than the Sun large blue object is revolving around a black hole This black hole is almost 16 times the Sun s mass a record for black holes created from the collapse of a giant star Other black holes at the centers of galaxies are much more massive but this object is the record setter for a so called stellar mass black hole In the illustration an orange disk surrounds the black hole This depicts material fed by a wind from the blue companion star which has been swept into orbit around the black hole Rather than flowing unimpeded and uniformly into space wind from the star is pulled towards the black hole by its powerful gravity The wind that does make it past the black hole is disrupted causing turbulence and ripples beyond the disk The companion star itself is also distorted by the gravity from the black hole The star is stretched slightly in the direction of the black hole causing it to become less dense in this region and to appear darker The inset shows a composite of data from NASA s Chandra X ray Observatory blue and the Hubble Space Telescope The bright objects in the inset image are young massive stars around M33 X 7 and the bright blue Chandra source is M33 X 7 itself X rays from Chandra reveals how long the black hole is eclipsed by the companion star which indicates the size of the companion Observations by the Gemini telescope on Mauna Kea Hawaii track the orbital motion of the companion around the black hole giving information about the mass of the two members of the binary Other observed properties of the binary were also used to help constrain the mass estimates of both the black hole and its companion Tarix 17 oktyabr 2007Menbe http www nasa gov mission pages chandra multimedia photos07 112 htmlMuellif Illustration NASA CXC M Weiss X ray NASA CXC CfA P Plucinsky et al Optical NASA STScI SDSU J Orosz et al Public domain Public domain false falseThis file is in the public domain in the United States because it was solely created by NASA NASA copyright policy states that NASA material is not protected by copyright unless noted See Template PD USGov NASA copyright policy page or JPL Image Use Policy Warnings Use of NASA logos insignia and emblems is restricted per U S law 14 CFR 1221 The NASA website hosts a large number of images from the Soviet Russian space agency and other non American space agencies These are not necessarily in the public domain Materials based on Hubble Space Telescope data may be copyrighted if they are not explicitly produced by the STScI 1 See also PD Hubble and Cc Hubble The SOHO ESA amp NASA joint project implies that all materials created by its probe are copyrighted and require permission for commercial non educational use 2 Images featured on the Astronomy Picture of the Day APOD web site may be copyrighted 3 The National Space Science Data Center NSSDC site has been known to host copyrighted content Its photo gallery FAQ states that all of the images in the photo gallery are in the public domain Unless otherwise noted CaptionsazerbaycancaAdd a one line explanation of what this file representsItems portrayed in this filetesvir ediryaranma tarixi17 oktyabr 2007 Faylin tarixcesi Faylin evvelki versiyasini gormek ucun gun tarix bolmesindeki tarixlere klikleyin Tarix VaxtKicik sekilOlculerIstifadeciSerh indiki20 42 21 oktyabr 2007516 516 65 KB Vaikunda Raja PD NASA This image is from http www nasa gov mission pages chandra multimedia photos07 112 html here Category Nasa Istifade edilen sehifeler Bu sekile olan kecidler Qara delik Faylin qlobal istifadesi Bu fayl asagidaki vikilerde istifade olunur en wikipedia org layihesinde istifadesi M33 X 7 fr wikipedia org layihesinde istifadesi M33 X 7 it wikipedia org layihesinde istifadesi Buco nero stellare M33 X 7 it wikinews org layihesinde istifadesi Astronomia scoperto il piu massiccio buco nero stellare mai osservato nl wikipedia org layihesinde istifadesi M33 X 7 pl wikipedia org layihesinde istifadesi M33 X 7 ru wikipedia org layihesinde istifadesi M33 X 7 tr wikipedia org layihesinde istifadesi Kara delik www wikidata org layihesinde istifadesi Q2697812 zh wikipedia org layihesinde istifadesi M33 X 7Metamelumatlar Bu faylda fotoaparat ve ya skanerle elave olunmus melumatlar var Eger fayl sonradan redakte olunubsa bezi parametrler bu sekilde gosterilenlerden ferqli ola biler error0 Menbe https az wikipedia org wiki Fayl M33 X 7 jpg, wikipedia, oxu, kitab, kitabxana, axtar, tap, hersey,

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