By shining light through samples, we can learn about the molecular structure of the sample and (sometimes) deduce its structure. IR UV RA DI O By the end of this course you…

1. C 6: T C hhe hemistry of Life6.1 - Atoms and TheirInteractions 2. Section 6.1Inside This Section...What is an Element?What are Atoms?2 Types of Chemical BondsChemical…

Slide 1Outcomes State that NMR spectroscopy involves interaction of materials with low-energy radio-frequency radiation. State the need for deuterated solvents. Describe…

Slide 1 The Deaths of Sunlike Stars Slide 2 Low Mass Dwarfs Low mass red dwarf stars cannot achieve any advanced fusion because they cannot get hot enough (Temp < 100…

Slide 1 (Recalling the Death of a High-Mass Star…) Slide 2 Slide 3 Slide 4 Neutron stars, although they have 1–3 solar masses, are so dense that they are very small.…

Slide 1 Nuclear Magnetic Resonance Spectroscopy An Introduction Slide 2 Over the past fifty years nuclear magnetic resonance spectroscopy, commonly referred to as NMR, has…

Slide 1 Lecture 3 NMR Spectroscopy: Spin-spin Splitting in 1 H NMR Integration Coupling Constants 13 C NMR Sample Preparation for NMR Analysis Due: Lecture Problem 1 Slide…

Slide 1 1 Structure of matter Lec. (7) Slide 2 www.scifun.ed.ac.uk/card/flakes.html Graphite – Van der Waals Bonds 2 Slide 3 www.webelements.com Graphite 3 Slide 4 Soft…

Outcomes State that NMR spectroscopy involves interaction of materials with low-energy radio-frequency radiation. State the need for deuterated solvents. Describe the use…

How do High Mass Stars Die? Class Announcements Homework is due today. Email to me the title of your choice of class project TODAY. Friday there is a class midterm test and…