ESS C109/C209: Isotope Geochemistry

Lecture 1 Notes

Introduction to Isotope Geochemistry

April 2, 2007

 

Introduction

               Syllabus

               PaulingÕs Rules reading, supplemental geology reading

 

Isotope Geochemistry

1. Geochemistry:

Study of the origins and chemistry of natural materials.

               Composition

               Phase changes

               Reactions

               Temperature.

               Age or duration.

               Cosmochemistry (subdiscipline):

                              Study of the origin and composition of the solar system.

                                             Nucleosynthesis.

                                             Age of meteorites.

                                             Condensation of planets.

                                             Differentiation of planets.

               Biogeochemistry (subdiscipline)

                              Interactions between life, oceans, atmosphere, and geology.

                                             Origins of life.

                                             Climate change.

              

2. Isotopes:

                              Atoms belonging to the same element, but with different masses.

                                             Element::atomic number::# of protons.

                                             Isotopes: different # of neutrons.

                                             Mass ~(# of protons + # of neutrons).

                              Chemistry: Isotopes generally have very similar chemical behavior.

                                             1st five weeks of class Ð assume no chemical separation.

                                             Weeks 6-10 Ð all about chemical separation.

                              Nuclear Chemistry: Isotopes have distinct nuclear structures

                                             Radioactivity

                                             Isomers

                                             Stability to nuclear reactions