Buchi neri primordiali per forgiare elementi pesanti


Si dice comunemente che siamo polvere di stelle, le fornaci nucleari in cui molto tempo fa sono stati prodotti elementi fondamentali per la vita attraverso un processo chiamato nucleosintesi. Ma l’origine degli elementi più pesanti, come oro, platino e uranio non è ancora del tutto chiara. Continua a leggere

Una Rara, Antica Supernova Superluminosa


La morte di una stella massiccia, avvenuta in una galassia ben dieci miliardi di anni fa, ha creato una rara supernova superluminosa, che gli astronomi ritengono una delle più distanti mai scoperte. Continua a leggere

Nuova luce sulle prime stelle dell’Universo

The  NASA/ESA Hubble Space Telescope has produced this beautiful image of  the globular cluster Messier 56 (also known as M 56 or NGC 6779), which  is located about 33 000 light years away from the Earth in the  constellation of Lyra (The Lyre). The cluster is composed of a large  number of stars, tightly bound to each other by gravity. However,  this was not known when Charles Messier first observed it in January  1779.  He described Messier 56 as “a nebula without stars”, like most  globular clusters that he discovered — his telescope was not powerful  enough to individually resolve any of the stars visible here, making it  look like a fuzzy ball through his telescope’s eyepiece. We clearly see  from Hubble’s image how the development of technology over the years has  helped our understanding of astronomical objects. Astronomers  typically infer important properties of globular clusters by looking at  the light of their constituent stars. But they have to be very careful  when they observe objects like Messier 56, which is located close to the  Galactic plane. This region is crowded by “field-stars”, in other  words, stars in the Milky Way that happen to lie in the same direction  but do not belong to the cluster. These objects can contaminate the  light, and hence undermine the conclusions reached by astronomers.   A  tool often used by scientists for studying stellar clusters is the  colour-magnitude (or Hertzsprung-Russell) diagram. This chart compares  the brightness and colour of stars – which in turn, tells scientists  what the surface temperature of a star is. By  comparing high quality observations taken with the Hubble Space  Telescope with results from the standard theory of stellar evolution,  astronomers can characterise the properties of a cluster. In the case of  Messier 56, this includes its age, which at 13 billion years is  approximately three times the age of the Sun. Furthermore, they have  also been able to study the chemical


Un team di astronomi dell’Università di Notre Dame ha individuato quella che potrebbe essere la seconda generazione di stelle, rivelando nuovi indizi sulla natura dei primi astri nati nell’Universo. Continua a leggere

Una stella simile al Sole ospita un denso gioviano caldo


Gli astronomi hanno rilevato un esopianeta gioviano caldo in transito davanti ad una stella simile al Sole localizzata a circa 1800 anni luce dalla Terra. Il pianeta appena scoperto, chiamato EPIC 220504338b, è stato individuato grazie alla missione K2 del telescopio Kepler. Continua a leggere