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Radioactive Decay

Radioactive Decay. Alpha Radiation – Emission of a helium nucleus Alternatively we write . Radioactive Decay. Beta Radiation – nuclear emission of an electron or β particle. Radioactive Decay. Gamma Radiation – emission of photons by excited or metastable nuclei.

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Radioactive Decay

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  1. Radioactive Decay • Alpha Radiation – Emission of a helium nucleus • Alternatively we write

  2. Radioactive Decay • Beta Radiation – nuclear emission of an electron or β particle

  3. Radioactive Decay • Gamma Radiation – emission of photons by excited or metastable nuclei

  4. Looking at the decay more carefully, We see that it undergoes a complex chain of reactions before reaching the stable isotope. This decay chain emits 8 α particles and 6 β particles. If the half lives of the intermediate daughters are orders of magnitude less than the Parent, then the rate of decay of the daughter is equal to the rate of decay of the parent. http://www.atral.com/U2381.html

  5. Geochronometers • Choice of radioactive dating method depends on several factors • Age of the sample • T1/2 should be same order of magnitude as rock age so that there are an adequate number of parent and daughter products to accurately determine ratio

  6. Geochronometers • Other important factors • Amount of parent and daughter elements present in the sample • Potassium is an abundant element so K – Ar dating can be used on most rocks • Was the system closed? • Was daughter or parent lost or gained by some other mechanism, e.g. • Radiogenic lead may be deposited with Uranium • Argon can escape until the rock is below the closure temperature

  7. Rubidium-strontium system • We cannot assume that all strontium in rocks is due to rubidium decay so we modify the above equation

  8. Rubidium-strontium system • Four naturally occurring isotopes of strontium • 84Sr: 0.6%, 86Sr: 10%, 87Sr: 7%, 88Sr: 83% • 86Sr is not a product of radioactive decay so the amount present now should be equal to the amount present when the rock formed (t0)

  9. Rubidium-strontium system • Normalize our equation by 86Sr to get • This is a straight line with slope (eλt-1) and the intercept gives 87Sr/ 86Sr at the time the rock formed. • Assumes that the initial Sr ratio was the same for all the minerals in rock or for all the rocks in a single location • The straight line is called an isochron

  10. Rubidium-strontium system • Disadvantages • Rubidium and strontium are mobile • Rubidium does not occur in limestone or ultramafic rocks

  11. Rubidium-strontium system • The [87Sr/ 86Sr]0 is an indicator of the rock origin • Rocks derived directly from the mantle will have an initial ratio of less than .704 • Rocks derived from remelting of crustal rocks will have a initial ratio substantially greater than 0.704

  12. Rubidium-strontium system • Since t1/2 is much larger than the age of the earth, we can make the approximation for any rock • Then plotting 87Sr/ 86Sr vs t defines the growth curve

  13. Uranium-lead system • Three naturally occurring isotopes of uranium • 238U: 99.3%, 235U: 0.7%, 234U: 0.006% • 238U and 235U are used for dating

  14. Concordia Diagrams • If a system has been closed to uranium and lead and a correction is made for initial lead then the isotope ratios will plot on the concordia – an ideal plot of 206Pb/238U vs207Pb/235U • If lead or uranium are lost or gained then the ratios will lie along a straight line that intersects the concordia at the time the rock crystallized (t) and when it was disturbed (t’). This line is called the discordia.

  15. U-Pb and Pb-Pbisochrons

  16. U-Pb and Pb-Pbisochrons • U-Pbisochrons often fail because of extensive uranium loss • Pb-Pbisochron is a straight line

  17. Th-Pb • The Th-Pb system can be more successful than U-Pbisochrons because thorium and lead tend to be less mobile than uranium

  18. Argon-Argon • The argon-argon method depends on bombarding a sample with fast neutrons in a nuclear reactor converting some of the 39K into 39Ar • Modern technique utilizes a laser to heat individual mineral grains or targeted spots within grains to release the argon after being irradiated. • 39Ar is unstable with half life of 269 yr

  19. Argon-Argon • The amount of 39Ar produce is given by

  20. Ar-Ar • Now using the equation we derived previously for 40K decay to 40Ar we arrive at the following relations

  21. Ar-Ar • If we irradiate a standard sample (sample of known age, ts) at the same time then we can determine J • And we can now find the age of our sample using

  22. Fission Track Dating • 238U undergoes spontaneous fission releasing two or three neutrons and a large amount of energy • λs =8.46x10-17 yr-1 • λ =1.55x10-10 yr-1 • Passage of charged particle results in a damage zone along its path or fission track • Energy below a certain threshold leaves no track so the types of reactions recorded are limited http://www.detectingdesign.com/radiometricdating.html

  23. Fission Track Dating • 238U can then be considered as undergoing a dual decay mechanism similar to the K-Ar-Ca system

  24. Fission Track Dating • Induced fission of 235U can be used to simplify dating problem • Requires bombarding sample with neutrons in a nuclear reactor

  25. Fission Track Dating • Then taking the ratios we have

  26. Fission Track Dating • A major advantage of fission track dating is that the stability of the tracks is temperature dependent. • Healing of damaged zones is called annealing • Rate of annealing depends on the mineral and temperature • The temperature history of rock can then be determined by measuring dates of various minerals within the rock

  27. http://www.mnsu.edu/emuseum/archaeology/dating/dat_fission.htmlhttp://www.mnsu.edu/emuseum/archaeology/dating/dat_fission.html Spontaneous fission tracks Induced fission tracks

  28. Samarium-neodymium • T1/2 for 147Sm-143Nd is 106 Gy so this system is good for dating very old rocks • Meteorites and some basalts • Abundance < 10 ppm • 147Sm/ 144Nd are ~0.1-0.2 in present rock samples • Advantage of this system is that geochemical processes do not preferentially separate Sm-Nd

  29. Samarium-neodymium • [143Nd/ 144Nd]0 gives and indication of the rocks origin similar to the Rb-Sr system • Concentration of 143Nd has increased through time because of 147Sm decay • Model time dependence of 143Nd/ 144Nd by assuming the that the ratio in the earth is the same as chondritic meteorites

  30. CHUR model • CHondritic Uniform Reservoir

  31. Age of the Earth • Oldest rocks are found on the cratons – ancient continental cores • Acasta gneisses in Canada – 3962 Ma (U-Pb) • Isuasupracrustal rocks in Greenland – 3772 Ma (Sm-Nd) and 3769 (U-Pb) • So by 4000 Ma continents existed

  32. Age of the Earth • Meteorites are thought to have common origin with the planets • Chondrites are most common (90%) and contain chondrules (small glassy spheres of silicate) indicating heating followed by rapid cooling • Achondrites are crystalline silicates with no chondrules and low metal concentrations • Iron

  33. Lead Evolution of the Earth • Holmes-Houtermans model • Assumes that earth quickly differentiated in to mantle and core then U-Pb ratio changed only as a result of radioactive decay • Further assumes that lead minerals completely separated from U and Th when formed

  34. Lead Evolution of the Earth • Holmes-Houtermans model • Can be used with meteorites because they are closed system with t=0 • Yields ages of between 4530 and 4570 Ma

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