Going live to the beating heart

“Please hold absolutely still”: This instruction is crucial for patients being examined by magnetic resonance imaging (MRI). It is the only way to obtain clear images for diagnosis. Up to now, it was therefore almost impossible to image moving …

All genes in 1 go

The majority of rare diseases are hereditary. But despite significant progress in genome research, in most cases their exact cause remains unclear. The discovery of the underlying genetic defect is, however, a prerequisite for their definitive…

Atmospheric Mercury Has Declined — But Why?

The amount of gaseous mercury in the atmosphere has dropped sharply from its peak in the 1980s and has remained relatively constant since the mid 1990s. This welcome decline may result from control measures undertaken in western Europe and North America, but scientists who have just concluded a study of atmospheric mercury say they cannot reconcile the amounts actually found with current understanding of natural and manmade sources of the element.

Gene analysis finds ‘fingerprint’ of defects in heart development

Using a multiple-gene analysis technique, German researchers have gained new insights into specific genetic alterations that lead to congenital heart defects, according to a report in today’s rapid access issue of Circulation: Journal of the American Heart Association. The technique, called microarray analysis, allowed investigators to identify specific patterns of gene expression in the entire human genome associated with common types of congenital heart defects. They sought to demonstrate the feasibility of using gene array analysis to study congenital heart defects. But their findings could represent an early step toward developing effective strategies to improve the quality of life in children and adults with heart defects.

Speeding star indicates mondo black hole in middle of Milky Way

Researchers say they’ve successfully tracked a star racing around a dark mass at the center of our Milky Way galaxy, offering strong support for the theory that a black hole is at the center of our little corner of space. Astronomers at the Max Planck Institute for Astrophysics tracked the orbit of the closest known star to the black hole candidate Sagittarius A*, a dark mass 3,000,000 times the mass of the sun. Following the star for 10 years, they found that it does indeed orbit Sagittarius A*. Approaching the black hole’s maw, the star reaches its highest velocity, whizzing past it at 5,000 kilometers per second.