jun 132012
 
Spotting Ultrafine Loops in the Sun's Corona

  A key to understanding the dynamics of the sun and what causes the great solar explosions there relies on deciphering how material, heat and energy swirl across the sun’s surface and rise into the upper atmosphere, or corona. Tracking the constantly moving material requires state-of-the-art telescopes with the highest resolution possible.  An image of [continue reading]

jun 012012
 
Light 'Echo' Around Supermassive Black Hole

  Astronomers studying the galaxy NGC 4151 with ESA’s XMM-Newton space observatory have detected X-rays emitted and then reflected by ionised iron atoms very close to the supermassive black hole hosted at the galaxy’s core. By measuring the time delays occurring in these ‘reverberation’ events, they were able to map the vicinity of this black [continue reading]