Sunday, April 28, 2024

4446 - OLDEST GALAXY - how to tell the ages? ?

 

-    4446  - OLDEST  GALAXY -  how to tell the ages? ?  -    Scientists find one of the oldest stars in the universe in a galaxy right next to ours.   An ancient star discovered in the Large Magellanic Cloud has revealed the chemical fingerprint of the early universe. It hints that conditions were not the same everywhere when the first stars forged the elements for life.

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-------------------------  4446    -    OLDEST  GALAXY -  how to tell the ages? ?

-    Scientists have identified one of the oldest known stars outside the Milky Way. The discovered has uncovered a relic from the early days of the universe in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way,  and it's revealing the conditions from a time before the sun even existed.

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-   The first stars born after the Big Bang lived and died billions of years ago, so there are none left to tell the story of the early universe. But traces of these stellar ancestors were preserved in the second generation of stars that formed and still survive today.

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-   The outer layers of these ancient stars preserve the chemical composition of their natal gas cloud, and reveal the composition of the first generation of stars that seeded  those clouds with new chemicals.  The composition of these stars offers a window into the early production of elements when the stars formed billions of years ago.

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-    The earliest stars blazed to life billions of years ago, soon after the Big Bang. They were behemoths made from the only elements that existed in abundance at the time: about three-fourths hydrogen and one-fourth helium. Those giants quickly burned through their nuclear fuel, shedding their outer layers and then exploding as supernovas and polluting their stellar neighborhood with new, heavier elements forged within their cores.

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-   This stellar ash entered the mix when a second generation of stars was born from the gas clouds enriched by the first. This cycle continued, building ever-heavier elements and even seeding the cosmos with the building blocks for life. This is the source of the oxygen we breathe, the calcium in our bones, and the iron in our blood cells.

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-    By measuring the amounts of these elements in a star, astronomers can estimate its age. The less "ash" that has accumulated, the older the star must be, while younger stars have built up a lot of elements from many earlier generations.

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-    None of the first-generation stars has ever been observed, but astronomers have spotted some ancient stars of the second generation in our galaxy. These fossils are very rare. Fewer than 1 in 100,000 stars in our galaxy is from that second generation.

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-    From these relics, astronomers have learned a lot about the early conditions in our galaxy. Now, they want to understand if the Milky Way is typical or if those conditions were different in other galaxies.

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-   To answer this question, astronomers turned their sights to one of our nearest galactic neighbors, the “LMC”. Visible to the naked eye from the Southern Hemisphere, the LMC is smaller than the Milky Way and  destined to merge with it in about 2.4 billion years.

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-   The team searched for old stars in the LMC in data gathered by the European Space Agency's Gaia space telescope. They followed up using the 6.5-meter Magellan telescope in Chile and identified 10 stars with about 100 times less iron than other LMC stars contain, meaning they were very ancient.

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-   One stood out. Known as “LMC-119”, it had less of this cosmic pollution than any known star outside our galaxy. This suggested it formed from gas enriched by just one supernova and was a sure sign that LMC-119 is a second-generation star and very ancient.  It is very likely at least 13 billion years old.  For comparison, the universe itself is estimated to be 13.8 billion years old.

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-    Today, the LMC is about 160,000 light-years away, but the authors estimated that it was about 6 million light-years distant when its earliest stars formed.  This isolates the early LMC from ejecta from the first stars that formed in the early Milky Way. This means that the LMC's ancient stars can tell astronomers about infant conditions in another galaxy.

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-     LMC-119 has much less carbon than ancient stars in our galaxy do. This hints at a previously unknown difference in how heavier elements built up in these two galaxies and suggests the environment in our young galaxy was likely different from that of the LMC.

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-   A new program to photograph one-quarter of the southern sky is using the Blanco 4 meter telescope in Chile and equipment designed to identify the most ancient fossil stars in the Milky Way and our galactic neighbor. By uncovering these relics, astronomers hope to paint a better picture of how stars have enriched the cosmos with the elements that make up all that we see around us.

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April 27, 2023          OLDEST  GALAXY -  how to tell the ages? ?         4446

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