Chapter 6: Uniform Circular Motion and Gravitation

Rotation Angle and Angular Velocity

  • Rotation Angle (Δθ\Delta \theta): The angle of rotation defined by the ratio of arc length (Δs\Delta s) to the radius of curvature (rr):   Δθ=Δsr\Delta \theta = \frac{\Delta s}{r}

Angular Velocity: ω=ΔθΔt\omega=\frac{\Delta\theta}{\Delta t}

  • Tangential Velocity (vv): The linear speed tangent to the circular path relates to angular velocity (ω\omega) and radius (rr) by:   v=rωv = r\omega


ω=2πT\omega=\frac{2\pi}{T} , (2π2\pi radians)

v=2πrTv=\frac{2\pi r}{T}

TT = period = time for one revolution to pass





Centripetal Acceleration and Centripetal Force

  • Centripetal Acceleration (aca_c): Radial acceleration pointing directly toward the center of curvature caused by a change in velocity direction:   ac=v2r=rω2a_{c}=\frac{v^2}{r}=r\omega^2

  • Uniform Circular Motion = an object moves in a circle at a constant speed




  • Centripetal Force (FcF_c ): Any net force perpendicular to velocity that directs an object toward the center of curvature:   Fc=mac=mv2rF_{c}=ma_{c}=m\frac{v^2}{r}

T=FcT=F_{c}

Unbanked turn with friction: v=μsgrv=\sqrt{\mu_{s}gr}

Steps to derive

1) Frictional force FfF_{f} = μs⋅N\mu_{s}\cdot N and Centripetal Force Fc=mv2rF_{c}=m\frac{v^2}{r} are set equal in order to maintain circular motion

2) Use N = w = mg →\rightarrow μs⋅mg=mv2r\mu_{s}\cdot mg=m\frac{v^2}{r}

3) Cancel m from both sides, simplify →v2=μs⋅gr\rightarrow v^2=\mu_{s}\cdot gr, so v=μsgrv=\sqrt{\mu_{s}gr}


Banked turn with no friction v=tan⁡θgrv=\sqrt{\tan\theta gr}

Steps to derive

1) set Fnet(y) = 0, so NyN_{y} - w = 0

2) Using trig angle (adjacent), NyN_{y} = Ncosθ\theta →\rightarrow Ncosθ\theta - w = 0

3) Ncosθ\theta = w →\rightarrow Ncosθ\theta = mg →\rightarrow N=mgcosθN=\frac{mg}{cos\theta}


4) set Fnet(x) = maca_{c}, since Fnet only force nin x direction is normal force →\rightarrow NxN_{x} = maca_{c}

5) Use aca_{c} = v2r\frac{v^2}{r} →\rightarrow Nx=mv2rN_{x}=m\frac{v^2}{r}

6) Using trig angle (opposite), NxN_{x} = Nsinθ\theta →\rightarrow Nsinθ\theta = mv2rm\frac{v^2}{r}

7) plug in N=mgcosθN=\frac{mg}{cos\theta} and simplify to gtan⁡θ=v2rg\tan\theta=\frac{v^2}{r} , so v=tan⁡θgrv=\sqrt{\tan\theta gr}

  • Unbanked (Level) Curves: Static friction (ff) between the tires and the roadway supplies the necessary centripetal force:   f=Fc≤μsN=μsmgf = F_c \le \mu_s N = \mu_s m g

  • Banked Curves: The normal force (NN) is tilted at an angle (θ\theta) relative to the vertical to provide centripetal force without relying on friction:

  • X direction:Nsin⁡(θ)=Fc=Fnet(x)N\sin(\theta)=F_{c}=F_{\text{net}}\left(x\right)  

  • Y direction: Ncos⁡(θ)=w=mgN \cos(\theta) = w = m g

Banked curve free-body diagram showing normal force components providing centripetal force




Newton’s Universal Law of Gravitation

  • Universal Gravitation Law: Every mass attracts every other mass along a line intersecting their centers of mass (CM\text{CM} ):  

 F=Gm1m2r2F=G\frac{m_1m_2}{r^2}

  • G = gravitational constant, 6.674⋅10−11N⋅m2kg⁡26.674\cdot10^{-11}N\cdot\frac{m^2}{\operatorname{kg}^2}

  • m1,m2 = two masses

  • r = radius

  • R is distance between their centers of mass


  • Surface Gravity: For objects near Earth's surface, the distance separating their centers of mass is approximated by Earth's radius (rer_e).

  • Earth-Moon System: Earth and the Moon revolve around their common center of mass once per month, producing detectable orbital "wiggles" in Earth's elliptical path around the Sun.

  • Tidal Dynamics: The gravitational differential exerted across Earth creates two high and two low ocean tides per day as Earth rotates under the tidal bulge


For the planet that feels the acceleration:

g=G(Mopposite)Ropposite2g=\frac{G\left(M_{opposite}\right)}{R_{opposite}^{_{}2}}

relative gravity = 4πG3pR\frac{4\pi G}{3}pR