Notes 1 Intro to Physical Science

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    SCIENCE

    a large b ody of knowledge b ased on facts andtruth known by actual experience an d

    observation.

    It is a lso d ened as search for t he a cceptedand accumulated knowledge which has beensystematically coordinated and formulatedto serve as t he basis f or t he discovery ofgeneral truth.

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    TECHNOLOGY

    refers t o the practical application of theprinciple o f physics.

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    BRANCHES OFPHYSICAL SCIENCE

    Physics - deals with matter and energyand their interactions i n the eld ofmechanics, acoustics, optics, heat,electricity, magnetism, and radiation. Thestudy of natural forces and energy.

    Chemistry - deals w ith composition,structure a nd properties of substancesand the changes they u ndergo.

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    Astronomy - deals w ith heavenly bodiesand their l ocations, sizes, compositions,motions, and other aspects.

    Geology - deals w ith the h istory of earthand its l ife, as reco rded in rocks. Petrologyis on e ex ample of this s cience w hich deals

    with rocks.

    Meteorology - deals w ith the st udy ofweather and climate.

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    IMPORTANCE OF PHYSICAL SCIENCE

    Research on the importance of physicalscience i n everyday living.

    To be written in one whole sheet ofyellow paper.

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    MATTEREverything that has mass and volume.

    STATES OF MATTER

    SolidLiquid

    Gas

    Plasma

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    STATES OF MATTER

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    Have a definite shapeHave a definite volume

    Molecules are held close together andthere is very little movement betweenthem .

    Kinetic Molecular Theory

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    Have an indefinite shapeHave a definite volumeKinetic Molecular Theory

    Atoms and molecules have more spacebetween them than a solid does, but lessthan a gas (ie. It is more fluid .!

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    Have an indefinite shapeHave an indefinite volume

    Kinetic Molecular Theory

    Molecules are moving inrandom patterns with varyingamounts of distance between

    the particles.

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    At "##$%, water

    becomes watervapor, a gas.Molecules canmove randomlyover largedistances.

    &elow #$%, watersolidifies to becomeice. In the solidstate, watermolecules are heldtogether in a rigidstructure.

    &etween #$% and"## $%, water is ali'uid. In the li'uidstate, watermolecules are closetogether, but canmove about freely.

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    %hanging states re'uires energy in either theform of heat. %hanging states may also bedue to the change in pressure in a system.

    Heat of formation, H f . Heat of vapori ation, H v

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    )lasma is by far the most commonform of matter. )lasma in the starsand in the tenuous space betweenthem ma*es up over ++ of thevisible universe and perhaps most ofthat which is not visible.

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    -n earth we live upon an island of ordinarymatter. /he different states of matter generallyfound on earth are solid, li'uid, and gas. 0ehave learned to wor*, play, and rest using these

    familiar states of matter.

    Sir William Crookes , an 1nglish physicist,

    identified a fourth state of matter, now calledplasma, in "23+.

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    )lasma temperatures and densities range fromrelatively cool and tenuous (li*e aurora! to very hotand dense (li*e the central core of a star!. -rdinarysolids, li'uids, and gases are both electricallyneutral and too cool or dense to be in a plasmastate.

    /he word "PLASMA" was first applied to ioni ed

    gas by Dr. Irving Langmuir an American chemistand physicist, in "+4+ .

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    Atom comes from the Greek wordatomos not sliceable.

    - the smallest particle of matter.

    The a tomic concept is very old and datingback to ancient Greek philosophers about

    2,500 years a go.

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    Democritus developed the AtomicTheory of Matter in the 4 th B.C.

    - he coined the t erm atom .

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    John Dalton an English chemist whoreintroduced the a tomic concept of matterin the e arly 1800s

    The summary of his theory:1. Indivisible m inute p articles ca lled atoms

    make up all matter.

    2. All the a toms of an element are exa ctlyalike in shape an d mass.

    3. The a toms of different elements differfrom one a nother in their masses.

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    J.J Thompson discovered electron negatively charged particle.

    Robert A. Millikan measured thecharge a nd mass of the el ectron.

    charge on an electron 1.60x10 raise t onegative 19 coulombmass of an electron 9.11x 10 raise t onegative 3 1 kgs.

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    Ernest Rutherford he concluded thatan atom must have a tiny, massive andpositively charged nucleus surrounded by

    electron.- electrons moving around the n ucleusare a t the d istance 1 00,000 times theradius of the n ucleus.- discovered the positive chargedparticle called proton.

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    James Chadwick identied theneutral particle i n the n ucleus c alledneutron in 1932 .

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    It turns ou t that protons, neutrons, anda zoo of other exot ic p articles a re n owthought to b e c omposed of six particles

    called quarks .

    These p articles have b een given the

    names up, down, strange, charm,bottom, and top.

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    The up, charm, and top quarks each carrya charge eq ual to t hat of the proton.

    whereas the down, strange, and bottomquarks each carry a charge eq ual to t heelectron.

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    PHYSICS

    Physics - deals with matter and energyand their interactions in the eld ofmechanics, acoustics, optics, heat,

    electricity, magnetism, and radiation. Thestudy of natural forces and energy.

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    BRANCHES OF PHYSICS

    1. Classical PhysicsMechanics deals w ith the st udy ofmotion of macroscopic bodies.

    Kinematics is the b ranch of mechanicsthat deals w ith the description ofmotion. It studies m otion without regardto t he f orces p resent.Dynamics is the b ranch of mechanicsthat deals w ith the b ehavior of objectsunder t he action of external forces.

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    Thermodynamics deals w ith the s tudy ofheat transfer and the changes t hat result fromit. It also studies h eat and its re lationshipwith other forms of energy.

    Electromagnetism deals with the s tudy of

    the rel ationship between electricity andmagnetism and describes al l kinds o felectromagnetic phenomena, from atomic toglobal scales.

    Optics deals with the st udy of the p hysicalproperties of light and its n ature a nd behavior.

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    2. Modern Physics Atomic Physics studies t he p roperties o f

    matter at the at omic scale an d examines thestructure, behavior, and properties of atoms.

    Biophysics applies t he t ools a nd techniques

    of physics i n studying living organisms.

    Chemical Physics involves t he u se o f theprinciples a nd theories of physics in studyingchemical processes

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    Cryogenics studies t he b ehavior of materials a tvery low temperatures.

    Fluid mechanics studies t he n ature, behavior,and movements of gases and liquids.

    Geophysics deals w ith the s tudy of Earthusing the p rinciples o f physics.

    Health physics involves the protection of

    people a gainst health hazards esp eciallyradiation.

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    Mathematical Physics emphasizes themathematics used as a m edium forunderstanding physics.

    Nuclear P hysics deals with the s tudy ofthe st ructure, properties, and reactions of

    atomic nucleus, and their applications.

    Plasma Physics deals with the b ehaviorand properties of fully ionized plasma.

    Planetary Physics studies t he origin,structure, and evolution of planets a ndplanetary systems.

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    Quantum Physics studies the qu antumtheory, which deals w ith interactionsbetween matter and electromagneticradiation.

    Relativity describes o bjects n early at the

    speed of light.

    Solid state Physics examines thestructures a nd properties of materials i nsolid state u sing quantum physics.

    Space Physics is t he study of planetaryand interplanetary m agnetized plasmas.

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    APPLICATION OF PHYSICS

    Research on the d ifferent application ofphysics in the m odern society.

    To be written in one whole sheet ofyellow paper.

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    SCIENTIFIC METHOD

    Refers to t he s ystematic method used ininvestigations or a logical way approach to t hesolution of problems

    1. Problem - know what specicproblem is.2. Observation - gathered data orinformation3. Hypothesis -educated guess4. Test Hypothesis - experimentation5. Theory/Conclusion

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    MEASUREMENT

    The p rocess that brings p recision to adescription by specifying how much and ofwhat of a property in particular s ituation.

    A number expresses the va and the n ame of the u nit tells you what thereferent is a s w ell as i mplies t he procedure f orobtaining the number.

    When standards ar e es tablished the r eferentunit is c alled standard unit.

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    2 MAJOR SYSTEMS OFMEASUREMENT

    English System - adopted in England (FPS)foot-pound-second

    Metric System - originally in France ( 1791) SI or known as System

    Internationale

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    ENGLISH SYSTEM

    Some of the ad opted units of this system wereoriginally b ased on the p art of the h uman body.

    Example:

    inch end joint of the t humbfoot length of the f ootyard - distance f rom the t ip of the n ose t o t he n edof ngers on an arm held straight out.

    cubit - distance f rom the en d of an elbow to t henger t ipfathom distance b etween the ngertips of armsheld straight out.

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    METRIC SYSTEM

    It was established by t he F rench Academyof Sciences i n 1791.

    The academy created a m easurementsystem that was based on invariablereferents in nature, not human body parts.

    The S I, is a modernized version of themetric system.

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    THE SEVEN BASE UNITS OF SISYSTEM

    Property Unit SymbolLength Meter mMass Kilogram kgTime Second s

    Electric current Ampere ATemperature Kelvin K

    Amount ofsubstance

    Mole mol

    Luminousintensity

    Candela cd

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    It uses p rexes t o rep resent larger orsmaller amounts by factors of 10.

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    Prex Symbol Meaning Unit

    MultiplierExa E Quintillion

    Peta P Quadrillion

    Tera T Trillion

    Giga G Billion

    Mega M Million

    Kilo k Thousand

    Hecto h HundredDeka da Ten

    Deci d One-tenth

    Centi c One-hundredth

    Milli m One-thousandthMicro One- millionth

    Nano n One- billionth

    Pico p One- trillionth

    Femto f One- quadrillionth

    Atto a One- quintillionth

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    CONVERSION UNITS

    Mass 1 kg= 1000g = 2.2 lbs. ( pounds)1 m etric ton= 1000 kg.

    Length 1cm= 0.394 in.1m=100 cm.=3.28 ft.=39.4 in.1 km= 1000m= 0.621 mi1 in= 2.54 cm.

    1 ft=0.3048 m=30.48 cm1 m i= 5,280 ft.=1,609 m =1.609 km1 yard = 0.9144 m

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    Area 1 cm 2 = 0.1550 in 2

    1 m 2 = 10,000 cm 2 = 10.76 ft 2

    1 ft 2 = 144 in 2 =929 cm 2 = 0.0929 m 2

    Volume 1 cm 3 = 0.000001 m 3

    1 m 3 = 1,000,000 cm 3 = 1,000 L=264 ga l.1 liter = 1,000 cm 3 = 1.056 qt. = 0.264 gal.

    1 ft 3 = 1,728 in 3 = 7.48 gal = 28.3 liters

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    Time 1 hr = 60 min. = 3,600 s1 day = 24 h = 1440 min.1 yr = 365 days

    Speed 1 m/s = 3.60 km/h = 3.28 ft/s= 2.24 mi/h1 ft/s = 0.682 mi/h = 0.305 m/s = 1.10 km/h

    Energy 1 Kcal = 1000 cal.1 J = 0.239 cal = 0.738 ft.lb1 Kcal = 4,184 J = 3.966 Btu

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    Power 1 KW = 1000 Watts1 h p = 745.7 W = 2,544.43 Btu/h= 550 ft-

    lb/s

    Temperature O F = 9/5 O C + 32O C = 5/9 ( O F- 32 )

    K = O C + 273

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    SCIENTIFIC NOTATION

    Also called wer

    Notation.

    A method does exist or small numbers in a m ore condensed form.

    It is u sually expressed as t he p roduct of twonumbers

    (1) Number 1 9 that is called coefficient(2) A power of ten

    eg. 1.97 X 10 raise t o t he 3 0 th power .

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    To multiply scientic notation numbers,the coefficients are m ultiplied as usualand the ex ponents a re a dded algebraically.

    To divide two sci entic notationnumbers, the coefficients are d ivided asusual and the exp onents are s ubtracted.

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    To add or subtract two numbers in scienticnotation:

    Step 1: Adjust the powers of 10 in the 2 n umbers sothat they have the sa me i ndex. (Tip: It is ea sier t oadjust the sm aller i ndex to eq ual the l arger i ndex).

    Step 2 : Add or subtract the n umbers.

    Step 3: Give t he a nswer in scientic notation .

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    EXERCISES ON SCIENTIFICNOTATION

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    EXERCISES ONCONVERSION OF UNITS