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21 Jan 2014 , 13:59
Our Milky Way galaxy may have formed from the inside-out, according to a ground-breaking study which provides new insight into galactic evolution.
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. 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.
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. Immediately after the Big Bang, the universe consisted almost entirely of hydrogen and helium, with levels of “contaminant metals” growing over time.
Consequently, older stars have fewer elements in their make-up – so have lower metallicity, researchers said. 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.
Two enormous, gamma-ray-emitting structures are bubbling out of the center of our galaxy. And astronomers have no idea what caused them. These bubbles, which stretch an astonishing 25,000 light years above and below the galactic plane, are invisible to the naked eye. But astronomers working with data from the Fermi space telescope, which detects gamma rays, were able to see the structures.
SLAYER69
[atsimg]http://files.abovetopsecret.com/images/member/b6b8c5bacb91.jpg[/atsimg]Vast, mysterious structure discovered at the heart of our galaxy
Two enormous, gamma-ray-emitting structures are bubbling out of the center of our galaxy. And astronomers have no idea what caused them. These bubbles, which stretch an astonishing 25,000 light years above and below the galactic plane, are invisible to the naked eye. But astronomers working with data from the Fermi space telescope, which detects gamma rays, were able to see the structures.
Thoughts?
...The team have shown that older, ‘metal-poor’ stars inside the Solar Circle – are far more likely to have high levels of magnesium.
Milky Way galaxy may have formed inside-out
The measurement of a quantum state poses a unique challenge for experimentalists. Recently, the technique of ‘direct measurement’ was proposed for characterizing a quantum state in situ through sequential weak and strong measurements.
"Since 1982 it has been known that quasars tend to group together in clumps or 'structures' of surprisingly large sizes, forming large quasar groups or LQGs," the society said.
This newly discovered large quasar group has a dimension of 500 megaparsecs, each megaparsec measuring 3.3 million light-years.