. 24/7 Space News .
Simulations Reveal Surprising News About Black Holes

Computer simulations of how black holes swallow matter show surprising violence and turbulence.

Baltimore MD (SPX) Mar 08, 2005
For more than 30 years, astrophysicists have believed that black holes can swallow nearby matter and release a tremendous amount of energy as a result. Until recently, however, the mechanisms that bring matter close to black holes have been poorly understood, leaving researchers puzzled about many of the details of the process.

Now, however, computer simulations of black holes developed by researchers, including two at The Johns Hopkins University, are answering some of those questions and challenging many commonly held assumptions about the nature of this enigmatic phenomenon.

"Only recently have members of the research team - John Hawley and Jean-Pierre De Villiers, both of the University of Virginia - created a computer program powerful enough to track all the elements of accretion onto black holes, from turbulence and magnetic fields to relativistic gravity," said Julian Krolik, a professor in the Henry A. Rowland Department of Physics and Astronomy at Johns Hopkins and co-leader of the research team.

"These programs are opening a new window on the complicated story of how matter falls into black holes, revealing for the first time how tangled magnetic fields and Einsteinian gravity combine to squeeze out a last burst of energy from matter doomed to infinite imprisonment in a black hole."

Close to the black hole's outer edge, where the Newtonian description of gravity breaks down, ordinary orbits are no longer possible. At that point - or so it has been imagined for the past three decades - matter plunges quickly, smoothly and quietly into the black hole.

In the end, according to the prevailing picture, the black hole - except for exerting its gravitational pull - is a passive recipient of mass donations.

The team's first realistic calculations of matter falling into black holes have strongly contradicted many of these expectations. They show, for instance, that life in the vicinity of a black hole is anything but calm and quiet.

Instead, the relativistic effects that force matter to plunge inward magnify random motions within the fluid to create violent disturbances in density, velocity and magnetic field strength, driving waves of matter and magnetic field to and fro. This violence can have observable consequences, according to research team co-leader Hawley.

"Just like any fluid that has been stirred into turbulence, matter immediately outside the edge of the black hole is heated. This extra heat makes additional light that astronomers on Earth can see," Hawley said.

"One of the hallmarks of black holes is that their light output varies. Although this has been known for more than 30 years, it has not been possible to study the origins of these variations until now.

The violent variations in heating - now seen to be a natural byproduct of magnetic forces near the black hole - offer a natural explanation for black holes' ever-changing brightness."

One of the most striking properties of a black hole is its ability to expel jets at close to the speed of light. While it has long been expected that magnetic fields are crucial to this process, the latest simulations show for the first time how a field can be expelled from the accreting gas to create such a jet.

Perhaps the most surprising result of the team's new computer simulations is that the magnetic fields brought near a rotating black hole also couple the hole's spin to matter orbiting farther out, in the same way that a car's transmission connects its rotating motor to the axle.

Says Krolik, "If a black hole is born spinning extremely rapidly, its 'drive train' can be so powerful that its capture of additional mass causes its rotation to slow down. Accretion of mass would then act as a 'governor,' enforcing a cosmic speed limit on black hole spins."

According to Krolik, that "governor" may have strong implications for many of the most striking properties of black holes. It is widely thought, for example, that the strength of a black hole's jet is related to its spin, so a "spin speed limit" might determine a characteristic strength for the jets, Krolik said.

Related Links
Johns Hopkins University
SpaceDaily
Search SpaceDaily
Subscribe To SpaceDaily Express



Memory Foam Mattress Review
Newsletters :: SpaceDaily :: SpaceWar :: TerraDaily :: Energy Daily
XML Feeds :: Space News :: Earth News :: War News :: Solar Energy News


Astronomers Measure Mass Of Smallest Black Hole In A Galactic Nucleus
Washington DC (SPX) Feb 21, 2005
A group led by astronomers from Ohio State University and the Technion-Israel Institute of Technology have measured the mass of a unique black hole, and determined that it is the smallest found so far.







  • Astronomers Measure Slowest Motion Across The Sky
  • ILC Dover Exploring Intelligent Materials For Inflatable Structures
  • Super-Sharp Radio "Vision" Measures Galaxy's Motion In Space
  • First Habitat Design Workshop: Call For Applicants

  • Spirit Perched At Larry's Lookout
  • Is Mars' Ring Around The Collar An Ancient Receding Glacier?
  • Mars Rovers Break Driving Records, Examine Salty Soil
  • Spirit Taking In Tennessee Valley

  • US Air Force Lifts Ban On Boeing In Satellite Launches
  • Brazilian Military Team Attends Russian Space Launch
  • Japan Returns To Space
  • Japan's First Rocket Launch Since 2003 Scheduled For Saturday

  • Rosetta's View Of Earth
  • Satellites Guide World's Top Yachts Through Southern Ocean 'Iceberg Alley'
  • GeoVantage Brings High-Resolution Digital Orthophotography To NorthWest
  • CloudSat Concludes Environmental Testing

  • NASA Awards Contract For Kepler Mission Photometer
  • Pluto At 75: A Uniquely American Anniversary
  • Discovery of Pluto Reaches 75th Anniversary
  • Pluto-Charon Origin May Mirror That Of Earth And Its Moon

  • Temperature Inside Collapsing Bubble Four Times That Of Sun
  • In The Stars: Starmaking's Helping Hand
  • Newly Seen Force May Help Gravity In Star Formation
  • Brightest Explosion Ever Observed Overwhelms Telescopes

  • Moonbeams Shine On Einstein, Galileo And Newton
  • India "A Step ahead" Of China In Satellite Technology: Space Chief
  • Confidence Restored, Japan Aims For Station On The Moon In 2025
  • Space Watch: An Oasis On The Moon?

  • Beijing Cabs To Have GPS Protection Against Hijacks
  • ILS Atlas V Gets Go-Ahead For GPS Mission In 2007
  • Two Stay In The Game To Win Galileo As EU Dithers Over Decision
  • Geo-Location Tracking Key To Singapore's Expanded Homeland Security Program

  • The content herein, unless otherwise known to be public domain, are Copyright 1995-2006 - SpaceDaily.AFP and UPI Wire Stories are copyright Agence France-Presse and United Press International. ESA PortalReports are copyright European Space Agency. All NASA sourced material is public domain. Additionalcopyrights may apply in whole or part to other bona fide parties. Advertising does not imply endorsement,agreement or approval of any opinions, statements or information provided by SpaceDaily on any Web page published or hosted by SpaceDaily. Privacy Statement