text-only page produced automatically by LIFT Text Transcoder Skip all navigation and go to page contentSkip top navigation and go to directorate navigationSkip top navigation and go to page navigation
National Science Foundation
 
News
design element
News
News From the Field
For the News Media
Special Reports
Research Overviews
NSF-Wide Investments
Speeches & Lectures
NSF Current Newsletter
Multimedia Gallery
News Archive
News by Research Area
Arctic & Antarctic
Astronomy & Space
Biology
Chemistry & Materials
Computing
Earth & Environment
Education
Engineering
Mathematics
Nanoscience
People & Society
Physics
 


Press Release 08-067
Catching a Glimpse of a Black Hole's Fury

New telescope evidence suggests twisted magnetic fields in supermassive black holes cause particle and energy jets to surge out in corkscrews

Artist's conception of the region near a supermassive black hole.

Artist's conception of the region near a supermassive black hole.
Credit and Larger Version

April 23, 2008

Using the National Science Foundation's (NSF) Very Long Baseline Array (VLBA) and a host of international telescope partners, a team of researchers has made the clearest observation yet of innermost region of a black hole.

From the observations, astronomers found strong evidence that the enormous jets of particles emitted by supermassive black holes are corkscrewed in a way predicted by theory. The researchers believe the coiling is a result of twisted magnetic fields acting on the particle streams.

The researchers reported their findings in the April 24 issue of Nature.

Led by Alan Marscher of Boston University, the international team of researchers studied the galaxy BL Lacertae located 950 million light years from Earth. By observing an outburst from the galaxy from late 2005 to 2006, the team observed bursts of photons oriented in a way predicted by theories about the twisted magnetic fields of black holes.

The VLBA is part of NSF's National Radio Astronomy Observatory (NRAO). A more detailed release--including graphics and a broadcast-quality animation--is available from NRAO at: http://www.nrao.edu/pr/2008/bllac

Additional images, explanations, data sets and even a related song are available at a Web site posted by Marscher: http://www.bu.edu/blazars/BLLac.html

-NSF-

Media Contacts
Joshua A. Chamot, NSF (703) 292-7730 jchamot@nsf.gov
Dave Finley, NRAO (575) 835-7302 dfinley@nrao.edu

Program Contacts
Vernon L. Pankonin, NSF (703) 292-4902 vpankoni@nsf.gov

Principal Investigators
Alan Marscher, Boston University (617) 353-5029 marscher@bu.edu

The National Science Foundation (NSF) is an independent federal agency that supports fundamental research and education across all fields of science and engineering. In fiscal year (FY) 2009, its budget is $9.5 billion, which includes $3.0 billion provided through the American Recovery and Reinvestment Act. NSF funds reach all 50 states through grants to over 1,900 universities and institutions. Each year, NSF receives about 44,400 competitive requests for funding, and makes over 11,500 new funding awards. NSF also awards over $400 million in professional and service contracts yearly.

 Get News Updates by Email 

Useful NSF Web Sites:
NSF Home Page: http://www.nsf.gov
NSF News: http://www.nsf.gov/news/
For the News Media: http://www.nsf.gov/news/newsroom.jsp
Science and Engineering Statistics: http://www.nsf.gov/statistics/
Awards Searches: http://www.nsf.gov/awardsearch/

 

border=0/


Print this page
Back to Top of page
  Web Policies and Important Links | Privacy | FOIA | Help | Contact NSF | Contact Webmaster | SiteMap  
National Science Foundation
The National Science Foundation, 4201 Wilson Boulevard, Arlington, Virginia 22230, USA
Tel:  (703) 292-5111, FIRS: (800) 877-8339 | TDD: (800) 281-8749
Last Updated:
April 24, 2008
Text Only


Last Updated: April 24, 2008