cbse class 10 science revision notes chapter – 10

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Material downloaded from myCBSEguide.com . 1 / 19 CBSE Class 10 Science Revision Notes CHAPTER – 10 LIGHT REFLECTION & REFRACTION Light is a form of energy, which gives us the power of vision. In this chapter we will study the phenomena of reflection and refraction using the property of light i.e. straight line propagation (Light wave travel from one point to another, along a straight line). Ray of light : It is a line in the direction of movement of light. Beam of light : It is bucnh of rays of light. Parallel beam : All the rays are parallel. Reflection of Light When the light is allowed to fall on highly polished surface, such as mirror, most of the light gets reflected. Laws of Reflection 1. The angle of incidence is always equal to angle of reflection. 2. The incident ray, reflected ray and the normal to the reflecting surface at the point of incidence lie in the same plane. Image formed by Plane Mirror (Plane reflecting surface)

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Page 1: CBSE Class 10 Science Revision Notes CHAPTER – 10

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CBSEClass10Science

RevisionNotes

CHAPTER–10

LIGHTREFLECTION&REFRACTION

Lightisaformofenergy,whichgivesusthepowerofvision.

Inthischapterwewillstudythephenomenaofreflectionandrefractionusingtheproperty

oflighti.e.straightlinepropagation(Lightwavetravelfromonepointtoanother,alonga

straightline).

Rayoflight:Itisalineinthedirectionofmovementoflight.

Beamoflight:Itisbucnhofraysoflight.

Parallelbeam:Alltheraysareparallel.

ReflectionofLight

Whenthelightisallowedtofallonhighlypolishedsurface,suchasmirror,mostofthelight

getsreflected.

LawsofReflection

1.Theangleofincidenceisalwaysequaltoangleofreflection.

2.Theincidentray,reflectedrayandthenormaltothereflectingsurfaceatthepointof

incidencelieinthesameplane.

ImageformedbyPlaneMirror(Planereflectingsurface)

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1.Virtual(imaginary)&Erect:Theimagethatdonotformonscreen.

Realimagescanberecordedonthescreen.

2.Laterallyinverted(Theleftsideofobjectappearonrightsideofimage)

3.Thesizeofimageisequaltothatofobject.

4.Theimageformedisasfarbehindthemirrorastheobjectisinfrontofit.

ReflectionoflightbysphericalMirrors

Mirrors,whosereflectingsurfacearecurvedinwardoroutwardsphericallyarecalled

sphericalmirror.

Forexample-Spoon Thecurvedsurfaceofshinningspooncanbeconsideredascurved

mirror.

Ifitiscurvedinward Actasconcavemirror

Ifitiscurvedoutward Actasaconvexmirror.

FewBasictermsrelatedtoSpherialMirror

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1. Principalaxis:Linejoiningthepoleandcentreofcurvatureofthesphericalmirror.

2. Pole:Thegeometricalcentralpointofthereflectingsphericalsurface.(aperture),

denotedby(P).

3. Aperture:Thewidthofreflectingsphericalsurface.

4. Centreofcurvature:Thecentreofthehollowglasssphereofwhichthespherical

mirrorisapartiscalledascentreofcurvature.

5. Radiusofcurvature:Thedistancebetweenthepoleandthecentreofcurvature.i.e.

PC=RorTheradiusofthehollowsphereofwhichthemirrorisapart.

6. Focuspoint:Thepointontheprincipalaxis,whereallparallelraysmeetafterreflection

iscalledasPrincipalFocusorFocus.Itisdenotedbyletter‘F’.

7. Focallength:Thedistancebetweenthepoleandfocuspointi.e.PF=f

8. RelationshipbetweenfocallengthandRadiusofcurvature.

ImageFormationbySphericalMirror

Beforewelearntheformationofimageorraydiagram,letusgothroughfewtips

(a)Remember,arayoflightwhichisparalleltoprincipleaxisalwayspassthroughfocus

(meetatfocus)orvice-versa.

(b)Arayoflightwhichpassesthroughcentreofcurvature(itisalsoknownasnormalatthe

pointofincidenceonsphericalmirror)willretracetheirpathafterreflection.

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(c)Arayoflightfallingonpolegetreflectedatthesameangleontheothersideofprincipal

axis.

Note:Arayoflightpassesthroughcentreofcurvatureofreflectingsphericalsurfacealways

actasnormalatthepointofincidence.Ifweknowthenormalwecandrawangleof

incidenceandangleofreflection

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Note1:Theimagewillonlyformwhentwoormoreraysmeetsatapoint.Imageformation

byaconcavemirrorfordifferentpositionoftheobject.

TheraydiagramsgiveninNCERTBooksarealsogoodtobefollowed.

ImageFormationbyConcaveMirror

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ImageformationbyConvexMirror

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UsesofConcaveMirror

1Usedintorches,searchlightandheadlightofvehicle.

2.Usedtoseelargeimageoffaceasshavingmirror

3.Usedbydentisttoseelargeimagesoftheteeth

4.Largeconcavemirrorusedtofocussunlight(heat)insolarfurnaces.

UsesofConvexMirror

Usedasrear-viewmirrorinvehiclesbecauseitgiveserectimage.Italsohelpsthedriverto

viewlargearea.

SignConventionforReflectionbySphericalMirror

1. Theobjectisalwaysplacedtotheleftsideofmirror.

2. Alldistanceshouldbemeasuredfrompole(P);paralleltoprincipalaxis.

3. Take'P'asorigin.Distancesmeasured

Rightoftheorigin(+x-Axis)aretakenpositive

Leftoftheorigin(–x-Axis)aretakennegative

Perpendiculartoandaboveprincipalaxis(+y-Axis)aretakenpositive

Perpendiculartoandbelowprincipalaxis(–y-Axis)aretakennegative

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MirrorFormula

f distancebetweenFandPole

v distanceofimagefromPole

u distanceofobjectfromPole

R distancebetweencentreofcurvatureandpole.

Where

Magnification

Itisexpressedastheratiooftheheightoftheimagetoheightoftheobject.

From1and2equation

When imageheightfromprincipleaxis.

Objectheightfromprincipleaxis

FewtipstoremembersignconventionforSphericalmirror

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f u v

CONCAVE -ve(real) -ve(real)-ve(real)

+ve(virtual)

CONVEX +ve +ve +ve

h–isalways+ve

h´–is+veforvirtual,–veforReal.

RefractionofLight

RefractionofLight:HappensinTransparentmediumwhenalighttravelsfromone

mediumtoanother,refractiontakesplace.

ArayoflightbendsasitmovesfromonemediumtoanotherRefractionisduetochangein

thespeedoflightasitentersfromonetransparentmediumtoanother.

Speedoflightdecreasesasthebeamoflighttravelfromrarermediumtothedensermedium.

SomeCommonlyobservedphenomenonduetoRefraction

Youreyes.

Rainbows.

Lightbendinginaglassofwater.

Glasses.

Cameralenses.

Objectdislocationinwater.

Binoculars..

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RefractionthroughaRectangularGlassSlab

WhenaincidentrayoflightAOpassesfromararermedium(air)toadensermedium(glass)

atpoint.OoninterfaceKL,itwillbendstowardsthenormal.AtptO1,oninterfaceNMthe

lightrayenteredfromdensermedium(glass)torarermedium(air)herethelightraywill

bendawayfromnormalOO1isarefractedrayO Bisanemergentray.Iftheincidentrayis

extendedtoC,wewillobservethatemergentrayO1BIparalleltoincidentray.Theraywill

slightlydisplacedlaterallyafterrefraction.

Note:Whenarayoflightisincidentnormallytotheinterfaceoftwomediaitwillgo

straight,withoutanydeviation.

LawsofRefractionofLight

Theincidentray,therefractedrayandthenormaltotheinterfaceoftwotransparentmedia

atthepointofincidence,alllieinthesameplane.

Theratioofsineofangleofincidencetothesineofangleofrefractionisaconstant

i.e.

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Forgivencolourandpairofmedia,thislawisalsoknownasSnell’sLaw

Constantnistherefractiveindexforagivenpairofmedium.Itistherefractiveindexofthe

secondmediumwithrepecttofirstmedium.

RefractiveIndex

Therefractiveindexofglasswithrespecttoairisgivenbyratioofspeedoflightinairtothe

speedoflightinglass.

c Speedoflightinvacuum= speedoflightinairismarginallyless,

comparedtothatinvacuum.

Refractiveindexofairwithrespecttoglassisgivenby

Refractiveindexofwater

Refractiveindexofwater

SphericalLens

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Atransparentmaterialboundbytwosurfaces,ofwhichoneorbothsurfacesarespherical,

formsalens.

ConvexlensConcavelens

1.Bulgingoutwards1.Bulginginwards.

2.Converginglens.2.Diverginglens.

ConcaveLens

Alensboundedbytwosphericalsurfaces,curvedinwardsisknownasdoubleconcavelens

(orsimplyconcavelens)

Itisalsoknownasdiverginglensbecauseitdivergesthelight.

FewBasicTermsRelatedtoSphericalLens

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1.Centreofcurvature:Alens,eitheraconvexlensoraconcavelensiscombinationoftwo

sphericalsurfaces.Eachofthesesurfacesformapartofsphere.Thecentreofthesetwo

spheresarecalledcentreofcurvaturerepresentedbyC1andC2.

2.Principalaxis:Imaginarystraightlinepassingthroughthetwocentresofcurvature

3.OpticalCentre:Thecentralpointoflensisitsopticalcentre(O).Arayoflight,when

passesthrough'O'itremainsundeviatedi.e.itgoesstraight.

4.Aperture:Theeffectivediameterofthecircularoutlineofasphericallens.

5.Focusoflens:Beamoflightparalleltoprincipalaxis,afterrefractionfrom

1.Convexlens,convergetothepointonprincipalaxis,denotedbyF,knownasPrincipal

focus

2.Concavelens,appeartodivergefromapointontheprincipalaxisknownasprincipal

focus.

ThedistanceOF2andOF1iscalledasfocallength

TipsforDrawaomgRayDiagram

1. Afterrefraction,arayparalleltoprincipalaxiswillpassthroughF.

2. AraypassesthroughF,afterrefractionwillemergeparalleltoprincipalaxis

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Imageformationbyaconvexlensforvariouspositionofobject

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ImageFormationbyConcaveLens

SignConventionforRefractionbySphericalLens

Similartothatofsphericalmirror,onlythedifferenceisthatallthemeasurementaremade

fromopticalcentre'O'

Lensformula

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Magnification

Itisdefinedastheratiooftheheightofimagetotheheightofobject.

Itisalsorelatedto‘u’&‘v’

Fromequation(1)&(2)

Ifmagnification

m>1,thenimageismagnified

m=1,imageisofsamesize

m<1,imageisdiminished

FewTipstoRememberSignConventionforSphericalLens

f u v

CONCAVE -ve -ve -ve(virtualimagealways)

CONVEX +ve -ve+ve(real)

-ve(virtual)

hisalways+ve

h´–veforRealand+veforVirtual&Errect.

PowerofLens

Thedegreeofconvergenceordivergenceoflightrayachievedbyalensisknownaspowerof

alens.

ItisdefinedasthereciprocalofitsfocallengthRepresentedbyP.

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IfFisgiveninmeter,then

IfFisgivenincm,then

SIunitofpowerofalensis“diopter”denotedby‘D’

IdiopterorID ItisthepoweroflenswhosefocallengthisIm

Powerofconvavelensordiverginglensisalwaysnegative

Ifanyopticalinstrumenthasmanylens,thennetpowerwillbe

Whatyouhavelearnt

Lightseemstotravelinstraightlines.

Mirrorsandlensesformimagesofobjects.Imagescanbeeitherrealorvirtual,

dependingonthepositionoftheobject.

Thereflectingsurfaces,ofalltypes,obeythelawsofreflection.Therefracting

surfacesobeythelawsofrefraction.

NewCartesianSignConventionsarefollowedforsphericalmirrorsandlenses.

Mirrorformula, givestherelationshipbetweentheobject-distance

(u),image-distance(v),andfocallength(f)ofasphericalmirror.

Thefocallengthofasphericalmirrorisequaltohalfitsradiusofcurvature.

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Themagnificationproducedbyasphericalmirroristheratiooftheheightofthe

imagetotheheightoftheobject.

Alightraytravellingobliquelyfromadensermediumtoararermediumbendsaway

fromthenormal.Alightraybendstowardsthenormalwhenittravelsobliquelyfrom

ararertoadensermedium.

Lighttravelsinvacuumwithanenormousspeedof3×108ms-1.Thespeedoflightis

differentindifferentmedia.

Therefractiveindexofatransparentmediumistheratioofthespeedoflightin

vacuumtothatinthemedium.

Incaseofarectangularglassslab,therefractiontakesplaceatbothair-glassinterface

andglass-airinterface.Theemergentrayisparalleltothedirectionofincidentray.

Lensformula, givestherelationshipbetweentheobject-distance(u),

image-distance(v),andthefocallength(f)ofasphericallens.

Powerofalensisthereciprocalofitsfocallength.TheSIunitofpowerofalensis

dioptre.