<p>Our Milky Way galaxy may have formed from the inside-out, according to a ground-breaking study which provides new insight into galactic evolution.<br /><br /></p>.<p>Data from the Gaia-ESO project has provided evidence backing theoretically predicted divisions in the chemical composition of the stars that make up the Milky Way's disc - vast collection of giant gas clouds and billions of stars that give our galaxy its 'flying saucer' shape.<br /><br />The research suggests that stars in the inner regions of the galactic disc were the first to form, supporting ideas that our galaxy grew from the inside-out.<br /><br />An international team of astronomers took detailed observations of stars with a wide range of ages and locations in the galactic disc to accurately determine their 'metallicity': the amount of chemical elements in a star other than hydrogen and helium, the two elements most stars are made from.<br /><br />Immediately after the Big Bang, the universe consisted almost entirely of hydrogen and helium, with levels of "contaminant metals" growing over time.<br /><br />Consequently, older stars have fewer elements in their make-up - so have lower metallicity, researchers said.<br /><br />The team have shown that older, 'metal-poor' stars inside the Solar Circle - the orbit of our Sun around the centre of the Milky Way - are far more likely to have high levels of magnesium.<br /><br />The higher level of the element inside the Solar Circle suggests this area contained more stars that "lived fast and die young" in the past, researchers said.<br /><br />The stars that lie in the outer regions of the galactic disc are predominantly younger, both 'metal-rich' and 'metal-poor', and have surprisingly low magnesium levels compared to their metallicity.<br /><br />This discovery signifies important differences in stellar evolution across the Milky Way disc, with very efficient and short star formation timescales occurring inside the Solar Circle; whereas, outside the Sun's orbit, star formation took much longer.<br /><br />"We have been able to shed new light on the timescale of chemical enrichment across the Milky Way disc, showing that outer regions of the disc take a much longer time to form," said Maria Bergemann from Cambridge University's Institute of Astronomy, who led the study.<br /><br />The study appears in the journal Astronomy and Astrophysics. </p>
<p>Our Milky Way galaxy may have formed from the inside-out, according to a ground-breaking study which provides new insight into galactic evolution.<br /><br /></p>.<p>Data from the Gaia-ESO project has provided evidence backing theoretically predicted divisions in the chemical composition of the stars that make up the Milky Way's disc - vast collection of giant gas clouds and billions of stars that give our galaxy its 'flying saucer' shape.<br /><br />The research suggests that stars in the inner regions of the galactic disc were the first to form, supporting ideas that our galaxy grew from the inside-out.<br /><br />An international team of astronomers took detailed observations of stars with a wide range of ages and locations in the galactic disc to accurately determine their 'metallicity': the amount of chemical elements in a star other than hydrogen and helium, the two elements most stars are made from.<br /><br />Immediately after the Big Bang, the universe consisted almost entirely of hydrogen and helium, with levels of "contaminant metals" growing over time.<br /><br />Consequently, older stars have fewer elements in their make-up - so have lower metallicity, researchers said.<br /><br />The team have shown that older, 'metal-poor' stars inside the Solar Circle - the orbit of our Sun around the centre of the Milky Way - are far more likely to have high levels of magnesium.<br /><br />The higher level of the element inside the Solar Circle suggests this area contained more stars that "lived fast and die young" in the past, researchers said.<br /><br />The stars that lie in the outer regions of the galactic disc are predominantly younger, both 'metal-rich' and 'metal-poor', and have surprisingly low magnesium levels compared to their metallicity.<br /><br />This discovery signifies important differences in stellar evolution across the Milky Way disc, with very efficient and short star formation timescales occurring inside the Solar Circle; whereas, outside the Sun's orbit, star formation took much longer.<br /><br />"We have been able to shed new light on the timescale of chemical enrichment across the Milky Way disc, showing that outer regions of the disc take a much longer time to form," said Maria Bergemann from Cambridge University's Institute of Astronomy, who led the study.<br /><br />The study appears in the journal Astronomy and Astrophysics. </p>