News
“Planetary Nebulae” receive more meaningful physical presence
Despite their name, planetary nebulae have nothing to do with planets. They were described as such by early astronomers whose telescopes showed them as glowing disc-like objects, but we now know that they represent the final stage of activity of stars like our Sun. A way of estimating more accurate distances to planetary nebulae dispersed across our Galaxy has just been announced.
Hubble survey reveals early galaxies were more efficient at making stars
A study just published by University of Texas at Austin assistant professor Steven Finkelstein and colleagues reveals that galaxies were more efficient at making stars when the universe was younger. The announcement explains the team’s discovery that there are a lot more bright, highly star-forming galaxies in the early universe than scientists previously thought.
Stanford astronomers observe the birth of an alien planet
Stanford University researchers announce evidence of an exoplanet being born that could move us one step closer to understanding the process of planet formation around other stars. The alien planet, called LkCa 15 b, orbits a star 450 light-years away and appears to be on its way to growing into a world similar to Jupiter.
Dark matter dominates in nearby dwarf galaxy
Dark matter is called “dark” for a good reason. Although they outnumber particles of regular matter by more than a factor of 10, particles of dark matter are elusive. Now, by measuring the mass of a nearby dwarf galaxy called Triangulum II, astronomers believe they may have found the highest concentration of dark matter in any known galaxy.
The birth of monsters: VISTA pinpoints earliest giant galaxies
ESO’s VISTA survey telescope has spied a horde of previously hidden massive galaxies that existed when the universe was in its infancy. By discovering and studying more of these galaxies than ever before, astronomers have, for the first time, found out exactly when such monster galaxies first appeared.
Visualising the Sun’s neighbourhood in 3-D
Astronomers have used modern techniques to create a 3-D visualisation of all of the O- and B-type stars within 500 parsecs (1,630 light-years) of the Sun using data from ESA’s Hipparcos satellite. This new visualisation uncovers evidence for new structures in the distribution of these nearby hot stars, and new and surprising theories of how those stars formed.