DOC PREVIEW
UGA CHEM 1211 - Emission and Absorption Spectrums
Type Lecture Note
Pages 2

This preview shows page 1 out of 2 pages.

Save
View full document
View full document
Premium Document
Do you want full access? Go Premium and unlock all 2 pages.
Access to all documents
Download any document
Ad free experience
Premium Document
Do you want full access? Go Premium and unlock all 2 pages.
Access to all documents
Download any document
Ad free experience

Unformatted text preview:

CHEM 1211 Lecture 15Outline of Last Lecture I. Hess’s law continuedII. Chapter 6: Atoms Electronic StructureIII. Color in Neon Lights, Fireworks, etc…A. Properties of Light (photon)IV. Constant Frequency & Variable WavelengthA. Photoelectric EffectB. Light & EnergyOutline of Current Lecture I. Electromagnetic RadiationA. Emission SpectrumB. Absorption SpectrumC. Bohr Model of AtomII. Predicting Emission Lines of HydrogenA. Rydberg EquationIII. Electronic TransitionsA. Wave nature of electronsCurrent Lecture: I. Electromagnetic RadiationA. Emission Spectrum: formed by electric current passing through a gas in a vacuumtube (at a very low pressure) which causes gas to emit lightEx: PrismLight  Prism  Detector- If we add lots of energy to a sample of elemental gas, we get an emission spectrum (elemental specific)1. In the hydrogen emission spectrum a band is observed at 4860A. What is the frequency and energy of this emission line?C = ƛv V = C / ƛ4860A 1 x 10 -10 m = 4.860 x 10-7m 1AV (visible: green light): 3.00 x 10 8 m/s = 6.17 x 1014 s-1 nHz4.860 x 10-7mE= hvE= (6.626 x 10-34 J*s)(6.17 x 108 m/s) = 4.088 x 10-19 J / photon4.088 x 10 -19 J 6.02 x 10 23= 2.46 x 105 J / mol photon photon Mol photonE = 246 KJ / mol photonB. Absorption Spectrum: shine a bean of white light through gas- Indicates wavelengths of light that have been ABSORBEDC. Bohr Model of Atom: only works for hydrogen, explains atomic spectra- Energy of quantized state: - RhC / n2- N: integral numbers only ( 1 to infinity )- Radius of orbitals: n2 (0.0529nm)II. Predicting Emission Lines of HydrogenA. Rydberg Equation1 = RH 1 - 1ƛ n12 n22- RH : 1.097 x 107 m-1- RH: 1.097 x 10-2 nm-1- n refers to one of the infinite possible energy state of the electron in hydrogen- requirement: n1 < n2III. Electronic Transitions1. Move an electron from a lower energy level to a higher energy level, E= -RhC 1 - 1 n12 n222. Start a rotational mode of motion3. Begin a vibrations mode of motion4. Gain kinetic energy (translational motion) ex: waterA. Wave nature of electrons2πr = nƛDE Broglie said the wavelength of an object = h / mv2πr = nh / mv- Angular momentum = mvr – nh /


View Full Document

UGA CHEM 1211 - Emission and Absorption Spectrums

Type: Lecture Note
Pages: 2
Download Emission and Absorption Spectrums
Our administrator received your request to download this document. We will send you the file to your email shortly.
Loading Unlocking...
Login

Join to view Emission and Absorption Spectrums and access 3M+ class-specific study document.

or
We will never post anything without your permission.
Don't have an account?
Sign Up

Join to view Emission and Absorption Spectrums 2 2 and access 3M+ class-specific study document.

or

By creating an account you agree to our Privacy Policy and Terms Of Use

Already a member?