Helium diffusion

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Helium atom

Helium diffusion is one type of nuclear decay dealing with the emission of Helium nuclei known as an alpha emission. Elements like uranium and thorium produce helium in zircons as a biproduct of their radioactivity. This helium seeps out of (sic) zircons quickly over a wide range of temperatures. If the zircons really are about 1.5 billion years old (the age which conventional dating gives assuming a constant decay rate), almost all of the helium should have dissipated from the zircons long ago. But there is a significant amount of helium still inside the zircons, showing their ages to be 6000 +/- 2000 years. Accelerated decay must have produced a billion years worth of helium in that short amount of time.

1 A Helium Diffusion Model Proposed
2 Helium in Atmosphere
3 References
4 See Also

A Helium Diffusion Model Proposed

As early as the 1970s, Robert Gentry pointed out that rocks appeared to be retaining more Helium than they should using standard models. Russell Humphreys, Steven Austin, Andrew Snelling, and John Baumgardner, the first three professors at the Institute for Creation Research and the last, a scientist at Los Alamos National Laboratory, conceived a model using what was known regarding helium diffusion in zircons. Their report [1] suggested that the amount of helium in the zircon was well over what would be observed in an old universe, citing a 5 order of magnitude error. Following the scientific method, they used their model to predict a collection of diffusion rates at hitherto untested temperatures. Humphreys claims these predictions were validated in a separate experiment reported in his 2004 report [2].

Kevin Henke, an instructor at the University of Kentucky, spent 25000 words challenging these results. [3] Humphreys responded in a 2005 report. [4] It should be noted that Henke's attack was on the 2003 model, not the putatively correct predictions found after the original report.

Helium in Atmosphere

There is also insufficient mass of helium in earth's atmosphere to account for 4.6 billion years of radioactive decay. Helium is a noble gas which doesn't combine with any other element, but there is not enough of it to account for the radioactive decay which should have occurred in an old earth scenario.

Uniformitarians suggest models for which helium can escape due to the solar wind.