PPT-Light: Thermal Spectra

Emission and Absorption Spectra Recap Canvas homework due FRIDAY Lab this week the Hertzsprung Russell diagram unfortunately getting here a little ahead of class Project due 11 22 see information from Canvas home page . Astronomy: The Science of Seeing. Goals. What is light?. What are the types of light?. Where does the light we see come from?. Understanding the light of heat.. On a sunny day why is it hot in my car?. Objectives. . . 1. Determine the. . emission spectrum of Hydrogen and other elements.. 2. Calculate the expected wavelengths of H using the Rydberg equation.. 3. Determine the composition of unknown solutions using flame tests.. www.highpoint.edu. /~. afuller. /PHY-1050. Pre. -Lecture Quiz:. MasteringAstronomy. Ch15 . pre-lecture quiz due . February 17. MasteringAstronomy. . Ch16 . pre-lecture quiz due . March 10. Homework: . Recap. No HW this . week. Project due 11/22. Light . /electromagnetic energy. Wavelength, frequency, energy. Electromagnetic spectrum: X rays, ultraviolet, visible, infrared, microwave, radio waves. s. [3]. Heat transfer processes. convection. conduction. radiation . . Physics of the atmosphere. the ozone layer. Greenhouse effect. climate change. Lecture 17. 1. .  . radiation. heat can be transferred by the emission of electromagnetic waves – thermal “light waves”, . 10/24/14. Electron . Config. , Orbital diagrams, Valence, Unpaired electrons, etc.. Drill. What are the three principle that govern electrons?. What are the shapes of the orbitals?. HW: pg. 8 Star Spectra. [3]. Heat transfer processes. convection. conduction. . . radiation . . Physics of the atmosphere. the ozone layer. Greenhouse effect. climate change. 1. Thermodynamics- review. Thermodynamics. of RHIC Paradigms. April 14–17, 2010. The Department of Physics . The University of Texas at Austin. RHIC paradigms: Early . Thermalization. and Collectivity -. are they achieved in RHIC’s new state of matter ?. Extending this to Hydrogen. Results from solving the . Shrodinger. equation for the hydrogen atom. Z is the atomic number. m. e. is the mass of an electron. e is the charge of an electron or proton. Astronomy: The Science of Seeing. Goals. What is light?. What are the types of light?. Where does the light we see come from?. Understanding the light of heat.. On a sunny day why is it hot in my car?. 10/27/14. Spectral Analysis. Drill. How do you calculate valence?. How many valence electrons do these elements have?. O. Xe. Fe. Ba. HW: pg. 9 Valence electrons. Objectives. IWBAT. Calculate valence for any element.. Emitting to the Truth. Start a new thread/topic. Learning Target: What does color tell us about the underlying structure of matter?. Update TOC. Emitting to the Truth. Read the Introduction p. 158 & 159. PI: Asegun Henry, Ph.D.. Co-PI: Kyriaki Kalaitzidou, Ph.D.. Graduate Students: Wei Lv, Sanzida Sultana. Intel Update Meeting: . 7. /11/2014. Objective and Approach. Objective . –. Higher TC chassis. All reactions were monitored by thin-layer chromatography carried out on 02 mm E Merck silica gel plates 60F-254 Column chromatography was performed on silica gel Wakogel C-300 H NMR spectra were reco