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Subject: (Free Body Diagrams; F = ma) Usedfor: Tofindtheaccelerationofoneofmoreobjectswhentheyfeeloneor moreforces. Priorknowledge: Math:trigonometry,vectors The FBD recipe! OftenaFreeBodyDiagramisusefulornecessarytosolveaproblemthatinvolvesforces.Follow thesesteps,andyou’llsolveanyproblemwithlittledifficulty. 1. DrawoneFreeBodyDiagramforeachobject(seebelowforwhatisagoodFBD). 2. Breaktheforcesupintocomponents. 3. Foreachobjectandeachdirection,writedownΣ F=(sumofforces)= ma . 4. Solvethissetofequations.Ifthereare Nunknownsthenyouneed Nequations.Oftenyou

needtoincludeadditionalequationslike fk = k FN tosolvetheproblemcompletely. How to draw the perfect FBD Thebetteryourdrawing,theeasieritistosolveaproblem.Trytostick totherulesbelow.Asanexample,considerablockthatslidesdownan incline,butslowsdownbecauseof. • Keepitsimple;oftenyoucanrepresentanobjectwitha simpleboxorcircle.Don’trepresentitasapoint(because theforcesoftenstartatacertainpointoftheobject,which couldproducea) • Don’tmakethediagramtoosmall.You’lloftenaddalotof stufftoit. • Drawtheforces,makethemtouchtheobject.Seetable belowforalistofpossibleforces.Don’tbreakthemupincomponentsyet;itoftenmakes yourdiagrammessy. • Itoftenhelpstodrawasmallcoordinatesystem(with xand y)nearthediagram.Eachobject canhaveitsowncoordinatesystem. • Itoftenhelpstoincludeanyanglesthataregiven. • Drawanarrowwithvor ainyourdiagram,ifyouknowtheirdirection.Don’tletittouchthe object!Onlyforcesshouldtouchtheobject. • Ifyouhaveseveralobjects,usethesamesymbolforquantitieswiththesamemagnitude!For example,iftwoobjectsareconnectedwitharope,youshouldusethesame FTforthetension thateachobjectfeels.Similarly,iftheobjectshavedifferentmasses,youneedtouse m1gfor oneobjectand m2gfortheother(andnot mg forbothofthem,becausethe m’saredifferent).

byErikLascaris([email protected])–version25Sep09 1

List of forces and how to find them:

Equation Name Direction Notes 2 Fg = mg ; Downwards g=9.8m/s ontheEarth (towardscenterof theEarth). FN Normal Perpendicular(i.e. Equaltowhateverforceisneededto normal)tothe preventtheobjectfromfalling surface. throughthefloor. UsetheFBDrecipetofind FN. FT Tension Indirectionofthe Iseithergivenalready,orneedstobe ropeorstring(away foundviatheFBDrecipe. fromtheobject). Fs = kx Springforce Oppositetothe xisindicateshowmuchthespringis (Hooke’slaw) directionof x compressedorstretched,and x=0if it’snotstretchedorcompressedat all.kiscalledthespringconstant . Kineticfriction Oppositetothe µ isthecoefficientofkineticfriction fk = k FN k directionofthe and FNthenormalforce. velocity Staticfriction Paralleltothe Equaltowhateverforceisneededto fs surface,butthe preventobjectfrommoving. exactdirection However,themaxvalueof fs is: dependsonwhatis f = F neededtoprevent s,max s N objectfrommoving. with µsthecoefficientofstatic friction and FNthenormalforce. m m Gravitational Fromcenterofone Usethisequationinsteadof Fg = mg F = G 1 2 G r 2 force masstowardsthe whenther isapproximatelythe centeroftheother radiusoftheEarthorlarger(i.e.for planetsandsuch). Buoyancyforce Upwards FB = ρ f Vs g ρfisthedensityofthefluid,and Vs thepartofthevolumeoftheobject thatissubmerged. Whenanobjectofmass mis

floating, FB = ρ f Vs g = mg . Circular motion: Whenanobjectmovesinacircleofradius r andwithspeed v,thenthenetforceΣFthisobjectis experiencingshouldbe: mv2 F = ∑ r Thisiscalledthecentripetalforce.

byErikLascaris([email protected])–version25Sep09 2 Extended example: Given the situation as shown in the figure. Determine the acceleration with which the blocks move. Assume there is no friction. Theproblemasksfortheacceleration,andtherefore“Forces”isthebestwaytoapproachthis problem(becauseifwefindthenetforce,we’vefoundtheacceleration–viaΣF= ma .). 1. DrawoneFreeBodyDiagramforeachobject. Wecanignorethepulley(it’snotmentionedthatwe shouldtakeitintoaccount,andweknownothing aboutit,sowecanignoreit). Notethatthetension FTisthesameforbothobjects, soweusethesamesymbol(anddifferentsymbolsfor the m1gand m2g).Also vand aarethesame forbothobjects,andtheirdirectionsareasindicated. 2. Breaktheforcesupintocomponents. Becauseofthewaywe’vechosenourcoordinatesysteminstep1, weonlyneedtobreakupthegravitationalforceof m2into components. 3. Foreachobjectandeachdirection,writedownΣ F=(sumofforces)= ma . Wehavetwoobjects,but m1onlyhasforcesinonedirection.Weshouldthereforewritedown three equations:

∑ Fx = m2 g sinθ − FT = m2a Mass m1: ∑ Fy = FT − m1g = m1a Mass m2: ∑ Fy = FN − mg cosθ = 0 4. Solvethissetofequations.Ifthereare Nunknownsthenyouneed Nequations. Wehave3equationsand3unknowns( FT, FN,and a),sothisissolvable.Oftenthisisthehardest part,becauseitrequiresalotofmathandpractice.

• First“solve”for FTusingtheequationfor m1as: FT = m1a + m1g

• Next,plugthisintotheupperequationfor m2: m2 g sinθ − (m1a + m1g) = m2a • Wenowhaveanequationwithonlyoneunknown,whichiseasiertosolve:

m2 g sinθ − m1g m2 g sinθ − m1g = m1a + m2a = (m1 + m2 )a ⇒ a = m1 + m2

byErikLascaris([email protected])–version25Sep09 3