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Solids, Liquids, & Gases I. States of Matter (p.214-220)  Kinetic Molecular Theory  Four States of Matter  Thermal Expansion MATTER.

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Presentation on theme: "Solids, Liquids, & Gases I. States of Matter (p.214-220)  Kinetic Molecular Theory  Four States of Matter  Thermal Expansion MATTER."— Presentation transcript:

1 Solids, Liquids, & Gases I. States of Matter (p.214-220)  Kinetic Molecular Theory  Four States of Matter  Thermal Expansion MATTER

2 Matter is….  Anything that has mass and volume  Everything on the periodic table  All solids, liquids, and gases

3 A. Kinetic Molecular Theory  KMT  Tiny, constantly moving particles make up all matter.  The kinetic energy (motion) of these particles increases as temperature increases.

4 B. Four States of Matter  Solids  low KE - particles vibrate but can’t move around  definite shape & volume  crystalline - repeating geometric pattern  Ex. Snowflake, salt, ice  amorphous - no pattern  Also called NONCRYSTALLINE solids  ex. glass, wax, plastics

5 B. Four States of Matter  Liquids  higher KE - particles can move around but are still close together  indefinite shape  definite volume

6  Will flow and this can be described by VISCOSITY  Viscosity is the resistance to flow  Thicker liquids are more viscous than thinner liquids

7 B. Four States of Matter  Gases  high KE - particles can separate and move throughout container  indefinite shape & volume  Exert PRESSURE on the sides of their container as the particles hit the sides

8 B. Four States of Matter  Plasma  very high KE - particles collide with enough energy to break into charged particles (+/-)  gas-like,  indefinite shape & volume  Most abundant type of matter in the universe stars, fluorescent light bulbs, TV tubes

9 Bose Einstein Condensates  extremely low temperature fluids  have properties that are not completely understood such as their ability to spontaneously flow out of their containers  Only exist at temperatures close to absolute zero ( 0 K or - 273 ◦C )

10 C. Thermal Expansion  Most matter expands when heated & contracts when cooled.   Temp causes  KE. Particles collide with more force & spread out.  EX: thermostats (bimetallic strip)

11 II. Changes in State (p.224-227)  Phase Changes  Heating Curves MATTER

12 A. Phase Changes  All phase changes are physical changes  Melting  solid to liquid  Freezing  liquid to solid melting point = freezing point

13 A. Phase Changes  Vaporization (boiling)  liquid to gas at the boiling point  Evaporation  liquid to gas below the boiling point  Condensation  gas to liquid

14 A. Phase Changes  Sublimation  solid to gas  EX: dry ice, freeze drying, iodine

15 A. Phase Changes

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17 B. Heating Curves  Kinetic Energy  motion of particles  related to temperature  Potential Energy  space between particles  related to phase changes

18 B. Heating Curves Solid - KE  Melting - PE  Liquid - KE  Boiling - PE  Gas - KE 

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21 B. Heating Curves  Heat of Fusion  energy required to change from solid to liquid  some attractive forces are broken

22 B. Heating Curves  Heat of Vaporization  energy required to change from liquid to gas  all attractive forces are broken  EX: steam burns, sweating, and… the drinking bird HEATING CURVE

23 Properties of Matter  Matter can be identified by its PROPERTIES (characteristics).  Some properties are shared by lots of matter; some are unique and can be used to identify different types of matter. These special or unique properties are called CHARACTERISTIC PROPERTIES.

24 PHYSICAL PROPERTIES  PHYSICAL PROPERTIES are properties you can observe without changing the identity of the substance.  Examples: color, shape, size, mass, weight, state, boiling and freezing points, magnetism, tensile strength (stretch), viscosity, malleability (pounded into sheets), density

25  Physical Properties can be SPECIFIC or GENERAL  Specific: can be used to IDENTIFY an object, UNIQUE or “special”  General: not enough DETAIL to identify an object

26 PHYSICAL CHANGE  A PHYSICAL CHANGE is a change that does not affect an object’s identity  Examples: breaking into pieces, changing shape, freezing, melting, boiling  USUALLY can be reversed

27  When substances change STATES, their identity does not change.  As of 1995, 5 states of matter had been identified

28 CHEMICAL PROPERTIES  CHEMICAL PROPERTIES are properties that indicate whether an object can undergo a chemical change.  Examples: flammable, corrosive, explosive, light sensitive, heat sensitive ** Chemical properties cannot be tested without changing the substance chemically!!!**

29 CHEMICAL CHANGES  CHEMICAL CHANGES, also called reactions, involve the changing of one substance into another.  Examples: rusting, burning, digesting, cooking, photosynthesis  Chemical changes usually cannot be REVERSED.

30  However, when a chemical reaction takes place the MASS NEVER changes! The mass of the products always EQUALS the mass of the reactants.  This is a scientific law called the: LAW OF CONSERVATION OF MASS or MATTER


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