Space telescopes reveal secrets of turbulent black hole
This image of the distant active galaxy Markarian 509 was taken in April 2007 with the Hubble Space Telescope's Wide Field Camera 2. Credit: NASA, ESA, G. Kriss (STScI), and J. de Plaa (SRON Netherlands Institute for Space Research); Acknowledgment: B. Peterson (Ohio State University)
(PhysOrg.com) -- A fleet of spacecraft including NASA's Hubble Space Telescope has uncovered unprecedented details in the surroundings of a supermassive black hole. Observations reveal huge bullets of gas being driven away from the gravitational monster and a corona of very hot gas hovering above the disk of matter that is falling into the black hole.
A team led by Jelle Kaastra of SRON Netherlands Institute for Space Research made use of data from ESA's XMM-Newton and INTEGRAL spacecraft (which study X-rays and gamma rays, respectively), the Hubble Space Telescope (for ultraviolet observations with the COS instrument), and NASA's Chandra (X-ray) Observatory and Swift (gamma-ray) satellites.
The black hole that the team chose to study lies at the heart of the galaxy Markarian 509 (Mrk 509), nearly 500 million light-years away. This black hole is colossal, containing 300 million times the mass of the Sun, and is growing more massive every day as it continues to feed on surrounding matter, which glows brightly as it forms a rotating disk around the black hole. Mrk 509 was chosen because it is known to vary in brightness, which indicates that the flow of matter is turbulent.
The above image of Mrk 509 was taken in April 2007 with Hubble's Wide Field Planetary Camera 2. But using a large number of telescopes that are sensitive to different wavelengths of light gave astronomers unprecedented coverage running from the infrared, through the visible, ultraviolet, X-rays, and into the gamma-ray band.
In this artist's illustration, turbulent winds of gas swirl around a black hole. Some of the gas is spiraling inward toward the black hole, but another part is blown away. Artwork Credit: NASA, and M. Weiss (Chandra X -ray Center)
The study is presented in a series of seven papers in the journal Astronomy and Astrophysics, with more expected to be published in coming months.More information: A full account of the research can be read on the SRON website at http://www.sron.nl
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JPL/NASA
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Sep 29, 2011
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Yes, observations violate models of:
a.) "Black Holes" that are not really black, and
b.) "Dead" nuclear embers of stars are violently energetic!
Why? The most powerful form of nuclear energy [1-3] was overlooked in nuclear rest mass data.
1. "Attraction and repulsion of nucleons: Sources of stellar energy," JFE 19, 93-98 (2001)
www.omatumr.com/a...tnuc.pdf
2. "Neutron repulsion confirmed as energy source", JFE 20, 197-201 (2002)
www.springerlink....6685079/
3."Neutron Repulsion", The APEIRON Journal, in press (2011)
http://arxiv.org/...2.1499v1
With kind regards,
Oliver K. Manuel
http://myprofile....anuelo09
Sep 30, 2011
Rank: 4 / 5 (4)
Sep 30, 2011
Rank: 5 / 5 (2)
a.) "Black Holes" that are not really black, and
b.) "Dead" nuclear embers of stars are violently energetic!"
Well, yes, those 803 published peer reviewed papers on Markarian 501, I presume, are in error: http://ned.ipac.c...of=table
I look forward to your published objections to their conclusions regarding Mrk 501 on a point-by-point basis sometime in the future. I guess you're not ready, able or willing to publish at this time. ;-)
Oct 01, 2011
Rank: 5 / 5 (2)
Oct 01, 2011
Rank: 5 / 5 (1)
These observations of Mrk 501 reveal the presence of a very hot UV-emitting corona surrounding the inner regions of this active galaxy which extends beyond 15ly from the center. UV light from the disk energizes and forms outflows of extremely hot, x-ray emitting regions within the 15ly corona surrounding the disk.
It was observations by XMM-Newton that discovered five of these x-ray emitting outflows in the hot corona of Mrk 501. Further work with the COS instrument on the HST revealed cooler UV-emitting gas spiraling inward near the edge of the 15ly-wide corona surrounding the AGN.
These observations may indicate that past merger activity might be responsible for the AGN activity we currently see in this galaxy. The press release has links to several papers that detail this current work on this nearby active galaxy: http://www.sron.n...emid=754
Oct 01, 2011
Rank: 5 / 5 (1)