Gas and condensed matter
Starter S-161 Define A.Saturated solution B.Miscible C.Supersaturated solution.
Title: Lesson 2 Collision Theory and Maxwell-Boltzmann Distribution Learning Objectives: – Understand the four main influences on the rate of a reaction.
Do Now
Ch 4 Temperature & Heat
NATS 1311 - From the Cosmos to Earth Law of Conservation of Energy Energy can be neither created nor destroyed. It merely changes it form or is exchanged.
1 Ch 4 Temperature & Heat 4.1Temperature Depends on Particle (atom) Movement.
HEAT. What is Temperature? Temperature is the average kinetic energy of the particles of an object. As temperature increases, kinetic energy of the particles.
WATER Its magical powers and why it is so important in biology.
Kinetic Molecular Theory Teacher: H. Michael Hayes.
Chemical rxns involve changes in energy – Breaking bonds requires energy – Forming bonds releases energy The study of the changes in energy in chem.
