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Kelly Oakes GBR

I'm an Undergraduate Physics student from Imperial College London, about to start the Masters year of my degree. I mostly write about physics research papers that I find interesting in the hope that other people will find them interesting too. The wordpress version of my blog is here.

My posts are presented as opinion and commentary and do not represent the views of LabSpaces Productions, LLC, my employer, or my educational institution.

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From Poincare and caos, for modest changes in the initial conditions, the motion of the system becomes chaotic and completely unpredictable. This is impotrtant for viewing two galaxies mix. Three b. . .Read More
Aug 01, 2011, 4:08pm

Poincare find that trhee body don not have mathematical representation. The mix of two galaxies must be a big caso .Or not? . . .Read More
Jul 29, 2011, 11:14pm
Comment by Kelly Oakes in How the Sun lost its spots

Psycasm said: Also, how great is that app? I love it. I've tried a few times to construct a pin-hole pr. . .Read More
Mar 11, 2011, 12:40pm
Comment by Jade in How the Sun lost its spots

Great article Kelly! . . .Read More
Mar 09, 2011, 1:40am
Comment by Psycasm in How the Sun lost its spots

Also, how great is that app? I love it. I've tried a few times to construct a pin-hole projector for solar viewing, but never managed to get it right. Are there other ways to safely view the sun an. . .Read More
Mar 08, 2011, 8:16pm
Views: 323 | Comments: 2
Last by Kelly Oakes on Feb 24, 2011, 7:42am
You might not be able to tell from wherever you are reading this, but black holes in the distant universe just shrunk down to as little as a tenth of their previous size. This is not some cosmic disappearing act; a new analysis of supermassive black holes at the centres of active galactic nuclei has revealed that their masses were previously overestimated by up to a factor of ten. The paper was published in Nature last week.



Active galactic nuclei, or AGN, are among the most luminous objects in the universe and are powered by massive black holes millions of times the mass of the Sun. Gas clouds, known as “broad line regions” for reasons that will become clear later, surround the black holes. These gas clouds range from a few light daysto hundreds of light days across; they are much wider than our solar system. Astronomers have been studying these clouds for over thirty years, but had not worked out the why some of them were flatter than others — until now.

. . . More
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