Spectroscopy methods errors:
http://www.ldolphin.org/univ-age.htmlThorium/Neodymium Ratio and Age of Universe
Mitchell Waldrop, a reporter for Science, interviewed Harvey Butcher who had discovered an interesting way to determine the age of the universe using essentially the same principles from radiometric dating. He measured the ratios of thorium (Th) and neodymium (Nd) in the sun and 20 nearby stars spectroscopically. Analyzing stars' spectral lines to determine the abundance of parent/daughter ratio is fairly simple. The stars have done the hard work of preparing the sample by vaporizing these isotopes and mixing them in their atmospheres. Each element has its own characteristic absorption lines: three for thorium and one for neodymium. Neodymium is a stable daughter product of thorium. Butcher says:
"What I expected to find was a change in the ratio of thorium to neodymium between the oldest and youngest stars."
"Virtually all the original thorium is still there, even in the oldest of the sampled stars," writes Waldrop.
Butcher expected that the ratio would be as much as two or three times smaller in the older stars, the white dwarfs, because the thorium would have had more time to decay. What he actually did find, however, was almost no variation in the thorium/neodymium ratio. Butcher suggested that, based upon the results of his measurements, the galaxy must be about five billion years younger than previously thought, possibly as young as 8 billion years. If "virtually all the original thorium is still there," the stars can't have aged much.
I looked at the data published in his 1987 report in Nature and compared the estimated age for each of the stars tested, including our sun, with the actual spectral data. The Th/Nd ratios of the sun and the other stars were essentially the same, although the age of some stars was supposed to be 600 million years and others 15-19 billion years.
After Butcher made this information available, Waldrop reports that Schramm was strongly skeptical of it, saying "it was a very uncertain kind of measurement and the results were grossly over-interpreted."
Schramm's assessment of Butcher's results pivoted on whether Butcher's instruments could read the faint spectral lines representing the concentrations of thorium and neodymium. Nuclear fusion reactions in supernova and other violent events produce thorium.
To decide how much thorium and neodymium should be present in stars, one has to make assumptions about when and how much thorium was made during the life of the galaxy. Butcher had to keep his assumptions of thorium production consistent with the abundance of thorium in meteorites and moon rocks because they, too, coalesced from the supernovae products along with the sun and the rest of the solar system. He says that once a star is born, its outer atmosphere provides an unchanging sample of the general composition of the Galaxy at that time, modified only by the free decay of radioactive species.
X-rays from the Sun are not generated thermally, electromagnetic particles are being accelerated through the Sun's own ether field to create x-rays. The cause of the solar x-rays is electrical, not thermal.
Koronium
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