Presentation is loading. Please wait.

Presentation is loading. Please wait.

Chemistry 141 Friday, December 1, 2017 Lecture 35

Similar presentations


Presentation on theme: "Chemistry 141 Friday, December 1, 2017 Lecture 35"— Presentation transcript:

1 Chemistry 141 Friday, December 1, 2017 Lecture 35
Chemistry 11 - Lecture 11 9/30/2009 Chemistry 141 Friday, December 1, 2017 Lecture 35 Kinetic Molecular Theory of Gases

2 Energy levels for 2p MOs σ*2p π*2p 2p 2p π2p σ2p σ*2s 2s 2s σ2s XA X2
XB

3 s-p Orbital Interactions

4 Energy levels for 2p MOs σ*2p σ*2p π*2p π*2p 2p 2p 2p π2p σ2p σ2p π2p
XA X2 XB XA X2 XB

5 MO Diagrams for 2nd Period Diatomics

6 Heteronuclear diatomics: NO
σ*2p Example: NO (5 + 6 = 11 valence e–) Electron configuration: (σ2s)2(σ*2s)2(σ2p)2(π2p)4(π*2p)1 Where is the unpaired electron? MO scheme suggests more density on N This is in agreement with the Lewis structure: π*2p 2p π2p 2p σ2p σ*2s 2s 2s σ2s N NO O N O : .

7 Molecular Orbital Theory
Two models of bonding Hybridization Simple Hybridization of valence shell s,p, and d orbitals on one atom to form new atomic orbitals with the correct geometry Atomic orbitals on adjacent pairs of atoms overlap to form bonds Electrons are shared by only 2 atoms Molecular Orbital Theory Simple only for diatomic molecules Atomic orbitals on all atoms combine to form molecular orbitals Electrons fill molecular orbitals; bonds form when there are more e- in bonding than antibonding orbitals Electrons delocalized over molecule Doesn’t handle resonance excited states O2 paramagnetism Does handle resonance excited states O2 paramagnetism

8 Recall that for gases Pressure is proportional to temperature
Pressure is inversely proportional to volume Can we explain these observations in terms of motions of individual gas molecules?

9 Principles of Kinetic Molecular Theory
A gas is many small particles in constant, linear motion. The majority of the volume of a gaseous substance is empty space. Particles collide with each other and with the walls of the container. Intermolecular forces are negligible, other than collisions. Total kinetic energy remains constant, though individual particles may gain or lose energy via collisions.

10 Distribution of speeds

11 Speed vs. molecular mass

12 Effusion & Diffusion Effusion is the escape of gas molecules through a tiny hole into an evacuated space. Diffusion is the spread of one substance throughout a space or a second substance.

13 Principles of Kinetic Molecular Theory
A gas is many small particles in constant, linear motion. The majority of the volume of a gaseous substance is empty space. Particles collide with each other and with the walls of the container. Intermolecular forces are negligible, other than collisions. Total kinetic energy remains constant, though individual particles may gain or lose energy via collisions.

14 Real Gases


Download ppt "Chemistry 141 Friday, December 1, 2017 Lecture 35"

Similar presentations


Ads by Google