The calculation of variations in the sea level is relatively simple. It is by far more complicated to then determine the change in the water mass. A team of geodesists and oceanographers... — full story
Will the universe expand outward for all of eternity and end in a vast, dark, cold, sterile, diffuse nothingness? Or will the 'Big Bang' - the gargantuan explosion that formed the universe... — full story
Using devices millionths of a metre in size, physicists at the California Institute of Technology (Caltech) have developed a technique to determine the mass of a single molecule, in... — full story
Intermediate-mass black holeThe detection of an ultraluminous X-ray source is now the strongest observational evidence for the existence of intermediate-mass black holes, as reported in a paper titled 'An intermediate-mass... — full story
Whether it's the summer grass that tickles your feet or the red Bordeaux smacking on your palette, nearly every part of the world around you carries special chemical markers. These... — full story
Astronomers discover youngest and lowest mass dwarfsAstronomers have found three brown dwarfs with estimated masses of less than 10 times that of Jupiter, making them among the youngest and lowest mass sub-stellar objects detected in... — full story
Mass-loss leaves close-in exoplanets exposed to the coreAn international team of scientists has found that giant exoplanets orbiting very close to their stars could lose a quarter of their mass during their lifetime. The team found that... — full story
New results from NASA's Chandra X-ray Observatory have made a major advance in explaining how a special class of black holes may shut off the high-speed jets they produce. These results... — full story
Calculations show Saturn's rings may be more massive, olderSaturn's rings may be more massive than previously thought, and potentially much older, according to calculations that simulate colliding particles in Saturn's rings and their erosion... — full story
Halos of planetary nebulae revealedStars without enough mass to turn into exploding supernovae end their lives blowing away most of their mass in a non-explosive, but intense stellar wind. Only a hot stellar core remains... — full story