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The Genesis of Elements

An in-depth exploration of isotopes born from radioactive decay and their geological significance, covering radiometric dating, isotopic signatures, and radiogenic heating.

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Definition

Born from Decay

A radiogenic nuclide is a nuclide produced by the process of radioactive decay. It can be either a radioactive nuclide (a radionuclide) or a stable nuclide. These isotopes are fundamental to understanding the Earth's composition and history.

Parent and Daughter

Radiogenic nuclides are often referred to as 'daughter products' that arise from the decay of a 'parent isotope'. The relationship between these parent and daughter isotopes is key to many scientific applications, particularly in dating geological materials.

Applications in Science

Radiometric Dating

Radiogenic nuclides are indispensable tools in geology for radiometric dating. By comparing the quantity of a radioactive parent isotope to its radiogenic daughter product within a geological sample, scientists can estimate the time elapsed since the sample solidified. This technique, known as radiometric dating, allows us to determine the age of rocks and minerals, providing a timeline for Earth's history. Prominent examples include Uranium-Lead dating.

Isotopic Signatures

The quantity of a radiogenic isotope, when compared to a non-radiogenic isotope of the same element, defines its 'isotopic signature'. This signature provides crucial information about the origin and history of geological materials. Techniques in isotope geochemistry leverage these signatures to trace geological processes, understand mantle and crustal evolution, and identify the sources of elements.

Key Examples

Lead Isotopes

Lead (Pb) is a prime example of a partly radiogenic element. While all four of its stable isotopes (204Pb, 206Pb, 207Pb, 208Pb) are primordial, the latter three are also produced radiogenically. Specifically, 206Pb originates from 238U decay, 207Pb from 235U, and 208Pb from 232Th. The excess of these isotopes in rocks containing uranium and thorium allows for precise dating of geological events.

Argon-40

Argon-40 (40Ar) is a significant radiogenic nuclide formed from the decay of Potassium-40 (40K). Almost all the argon found in Earth's atmosphere is radiogenic, distinguishing it from the primordial argon isotope, Argon-36 (36Ar).

Helium Isotopes

Helium (He) isotopes, particularly Helium-4 (4He), are predominantly radiogenic, originating from the decay of heavier elements within the Earth's crust. While some primordial helium was trapped during Earth's formation, the vast majority found in gas wells and the atmosphere is produced through radioactive decay. Helium-3 (3He) is primarily primordial, though small amounts can be produced by nuclear reactions.

Radon

Radon (Rn) is entirely radiogenic. Due to its very short half-life, it cannot exist primordially and is only found as a product of the ongoing radioactive decay of heavier elements, such as uranium, within the Earth's crust.

Extinct Radionuclides

Some radionuclides, like Iodine-129 (129I), have half-lives too short (e.g., 15.7 million years for 129I) to survive from the primordial formation of the solar system. These are known as 'extinct radionuclides'. Although no longer present directly, their decay products (e.g., Xenon-129, 129Xe) can be found in excess in meteorites, providing evidence of their past existence and the timing of early solar system events.

Radiogenic Nuclides in Geology

Key Isotope Systems

The study of radiogenic nuclides is central to isotope geology. Various parent-daughter isotope systems are employed for dating, each with different half-lives suitable for different geological timescales. The table below outlines some of the most significant systems used.

Parent nuclide Daughter nuclide Decay constant (yr−1) Half-life
190Pt 186Os 1.477 ×10−12 483 Gyr
147Sm 143Nd 6.54 ×10−12 106 Gyr
87Rb 87Sr 1.402 ×10−11 49.44 Gyr
187Re 187Os 1.666 ×10−11 41.6 Gyr
176Lu 176Hf 1.867 ×10−11 37.1 Gyr
232Th 208Pb** 4.9475 ×10−11 14.01 Gyr
40K 40Ar 5.81 ×10−11 11.93 Gyr
238U 206Pb** 1.55125 ×10−10 4.468 Gyr
40K 40Ca 4.962 ×10−10 1.397 Gyr
235U 207Pb** 9.8485 ×10−10 0.7038 Gyr
129I 129Xe 4.3 ×10−8 16 Myr
10Be 10B 4.6 ×10−7 1.5 Myr
26Al 26Mg 9.9 ×10−7 0.70 Myr
36Cl 36Ar (98%)
36S (2%)
2.24 ×10−6 310 kyr
234U 230Th 2.826 ×10−6 245.25 kyr
230Th 226Ra 9.1577 ×10−6 75.69 kyr
231Pa 227Ac 2.116 ×10−5 32.76 kyr
14C 14N 1.2097 ×10−4 5730 yr
226Ra 222Rn 4.33 ×10−4 1600 yr

Radiogenic Heating

Earth's Internal Heat Source

The process of radioactive decay, which produces radiogenic nuclides, also releases significant amounts of heat energy. This phenomenon, known as radiogenic heating, is one of the two primary sources contributing to the Earth's internal heat budget, alongside primordial heat from planetary accretion. The decay chains of Uranium-238, Thorium-232, and Potassium-40 are particularly important contributors to this heat within the Earth's mantle and crust.

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References

References

  1.  Note: this not the half-life of 40K, but rather the half-life that would correspond to the decay constant for decay to 40Ar. About 89% of the 40K decays to 40Ca.
A full list of references for this article are available at the Radiogenic nuclide Wikipedia page

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