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Full Story - Guardian
A team of scientists at the Australian National University has discovered the oldest known star in the universe.
The discovery of the heavenly body, which formed about 13.6bn years ago, has allowed astronomers to study the chemistry of the first stars.
Lead researcher Dr Stefan Keller of the ANU’s Research School of Astronomy and Astrophysics called the find a “one in a 60m chance”.
Havick007
The star designated SMSS J031300.36-670839.3 lay within the Milky Way Galaxy at a distance of 6,000 light years from Earth and would have died long ago after a spectacular super-nova...
Kratos40
reply to post by Havick007
Something does not make sense here. This star cannot be this ancient if it is within our own galaxy. We are a middle aged galaxy compared to this star.
Kratos
Kratos40
reply to post by Havick007
Something does not make sense here. This star cannot be this ancient if it is within our own galaxy. We are a middle aged galaxy compared to this star.
Kratos
The most recent estimates using both improved theories of stellar structure and more accurate distance data from the Hubble Space Telescope give a more reasonable estimate of 14.5 billion years (with an uncertainty of plus or minus 800 million years). This makes HD 140283 the oldest known star with a well-determined age. It has been called the “Methuselah Star”, and although it looks quite normal at first, looking closely we see what a strange star it is. Its diameter is almost half as a large again as our own Sun, but its surface temperature is roughly the same as the Sun’s. This combination of size and temperature means HD 140283 is almost four times as bright as our Sun. None of these statistics are unusual, but the star’s composition has been known to be anomalous since the 1950s. Compared to other relatively nearby stars HD 140283 is “metal-poor”, in astronomical jargon this means it is lacking in elements heavier than hydrogen and helium. This may not seem particularly odd but is a vital clue in determining the star’s age.
'Oldest star' found from iron fingerprint (Update)
Full Article - Phys.org
The team has identified a distant star several thousand light-years away—named SMSS J031300.36-670839.3—that contains a level of iron whose upper limit is so low that it suggests that the star is a second-generation star, having arisen from the gas cloud enriched by one of the very first stars in the universe. But because there is so little iron in the star, the researchers say the star's progenitor must not have been very energetic, as it may have failed to expel all the heavy elements made in its own core.
The findings, which are published this week in the journal Nature, provide a glimpse of what the activity in the very early universe may have looked like, and point to much more diverse properties among the very first population of stars.
To find the earliest generations of stars, scientists look for vanishingly small abundances of the first heavy elements created, such as iron. Stars with very low chemical abundances, they believe, may have formed in the earliest epoch of the universe, more than 13 billion years ago, when few elements had yet formed.
The Large Magellanic Cloud
(LMC - Wide field)
(The nebula around 30 Doradus (NGC 2070) in the LMC)
he Large Magellanic Cloud (LMC) is the nearest galaxy to the Milky Way but less than one tenth as massive; even so it contains the equivalent of over ten billion solar masses of material in the form of stars, gas and dust. The LMC is at a distance of 170,000 light years and is visible to the unaided eye from southern latitudes, with an apperance rather like a detached piece of the Milky Way, in the otherwise barren constellation of Dorado.
Havick007
reply to post by Kratos40
It didn't make much sense to me when I first read either.
When writing the OP, I also made the assumption that if the star was that old (13 billion yrs) that it would have since died out. Unless it actually has died in the past 6000 years, that part doesn't make sense to me. How could a star burn for so long?
The less massive the star, the longer this evolutionary process takes; for example, it has been calculated that a red dwarf with a mass of 0.16 solar masses (approximately the mass of the nearby Barnard's star) would stay on the main sequence during 2.5 trillion years that would be followed by five billion years as blue dwarf, in which the star would have 1/3 of the Sun's luminosity and a surface temperature of 8,500 Kelvin.[8]