Astronomy/Planet formation

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QUESTION: When Earth formed from the accretion disk, I would imagine that the material from which it was formed was pretty well mixed, pretty homogeneous.  So my question is, if Earth was formed from a well mixed medium of all the elements and compounds we find here, why do we find chunks of one element, like veins of gold?  How did the gold clump up like that as the material of the planet coalesced?  

Thanks,
Cole

ANSWER: Hi Cole,

This is a great question, one that researchers are working on today.   I do not have a definitive answer as we are not sure of it, but I'll try to shed some light on the question.

Firstly, the molecular cloud of gas that collapsed down due to gravity to form an accretion disk was probably not that well mixed.  That is because it would be consisted of different supernova explosions and other sources that would have created different densities of material/gas (elements).  

Next, in the accretion disk that the gas cloud was pulled into by gravity, there would be slight variations in temperature.  We know this is true as this is partially explains how we get different types of planets in areas (small rocky planets on the inside, large gas planets on the outside).  We believe that in addition to large scale temperature variations, there would be small scale temperature variations.  Since temperature and pressure are proportional, by changing the temperature in an area, you can change the pressure.  This would mean that you can change in small areas, how well you can compress materials (i.e. make denser, more abundant pockets of an element).  

Lastly, the volcanic and geothermal process over the 4 billions years of the Earth would have affected this too.  These processes would have melted, changed, and moved some of the various elements, creating denser areas in one place, and less denser areas (of an element) in another.

I hope this helps with your question.

Peace,
Brad

---------- FOLLOW-UP ----------

QUESTION: I don`t understand how small pockets of temperature differential (and the coinciding ability to compress elements etc to varying degrees) would bring together clumps of one material.  Any idea?

Thanks,
Cole

Answer
The key is actually nuclear physics.  In order to get higher order elements (i.e. elements with more protons and neutrons than hydrogen), you need something called neutron capture.  Since most of the gas in the early Solar System would have been hydrogen, you can fuse hydrogen together to get helium, and continue this process.  

The second way (and more productive way) is if you have a lot of free particles (protons, neutrons, electrons) and spare energy.  This would be the case with most planetary/solar systems, as they would have been from supernova explosions, which would have created a lot of energy but also split apart all of the atoms that existed in that previous star (therefore creating free protons, neutrons, etc.).  With the extra energy, via nuclear fusion, you can start to pull these particles into elements.  However, since the energy would not have been fully, evenly distributed (as is always the case with supernova explosions), different amounts of higher order (heavier nuclei) elements would be formed in areas where there was more energy

All of this energy would be thermal energy, which would alter the pressure to create these things.  The direct implication is from the free energy, which is manifested as thermal energy (temperature) and then therefore pressure.  

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Brad Tucker

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I'm happy to answer any general questions about Astronomy, Astrophysics, and Cosmology. I'm also happy to take general, specific, and detailed questions related to supernovae, Baryonic Acoustic Oscillations, the Cosmic Microwave Background, dark matter, dark energy, and the Big Bang Theory. I'm also happy to chat about Astronomy/Astrophysics education and careers, and philosophy and science.

Experience

I am a professional research astronomer/astrophysicist/cosmologist. My research focuses on studying supernovae and using them to measure the properties of the Universe, such as how fast it is growing and what it is made of. I also frequently give talks to school groups and the public, and am a regular guest on various radio stations.

Organizations
Current Research Fellow at Mt. Stromlo Observatory, the Australian National University, and in the Department of Astronomy, University of California, Berkeley.

Publications
Lots of journals, including the Astrophysical Journal, the Astronomical Journal, and Nature. I am currently in the middle of writing my first popular book.

Education/Credentials
B.A. Philosophy, University of Notre Dame, Notre Dame, IN USA B.A. Theology, University of Notre Dame, Notre Dame, IN USA B.Sc. Physics, University of Notre Dame, Notre Dame, IN USA Ph.D. Astrophysics, Mt. Stromlo Observatory, the Australian National University, Canberra, ACT, Australia

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