our networks
tlcanimal planetthe science channelmilitary channelthe health channel
site search
shop now
 
 

Omega Centauri Hides Middle-Weight Black Hole

Irene Klotz, Discovery News
    print
 

The most logical explanation, they say, is a medium-sized black hole that is about 40,000 times bigger than our sun. Only one other black hole of this size has been found, said astronomer Karl Gebhardr with the University of Texas at Austin.

"This result shows that there is a continuous range of masses for black holes, from supermassive, to intermediate-mass, to small stellar-mass types, said astronomer Eva Noyola with the Max-Planck Institute in Germany.

Scientists theorize that intermediate-mass black holes may be seeds for supermassive black holes, which exist in the centers of many galaxies, including the Milky Way. "We may be on the verge of uncovering one possible mechanism for the formation of supermassive black holes," Noyola said.

Scientists next plan to use the European Southern Observatory's Very Large Telescope in Chile for followup observations.


Related Links :

Irene Klotz's blog: Free Space

NASA's 50th Anniversary

Hubble Space Telescope

The Gemini Observatory

 
advertisement

Download Space News!

 
newsletter
 

Sponsored Links

 
SITE SEARCH
SUBSCRIBE TO OUR NEWSLETTERS
CREDITS Copyright 2002-2008 by Volker Wendel and Bernd Flach-Wilken |
DISCOVERY SITES Discovery Channel / TLC / Animal Planet / Discovery Health / Science Channel / Planet Green / Discovery Kids / Military Channel /
Investigation Discovery / HD Theater / Turbo / FitTV / HowStuffWorks / TreeHugger / Petfinder / PetVideo / Discovery Education
VIDEO Discovery Channel Video Player
SHOP Toys / Games / Telescopes / DVD Sets / Planet Earth DVD Sets / Gift Ideas
CUSTOMER SERVICE Contact Us / Free Newsletters / RSS / Sitemap / TV FAQs
CORPORATE Discovery Communications, LLC / Advertising / Careers @ Discovery / Privacy Policy / Visitor Agreement
ATTENTION! We recently updated our privacy policy. The changes are effective as of Tuesday, October 30, 2007. To see the new policy, click here. Questions? See the policy for the contact information.