A) A straight line trajectory B) A circular path around the origin with radius α C) A velocity vector magnitude D) A parabolic path
A) [α, 0] B) [α, α] C) [0, α] D) [0, 0]
A) They are always parallel. B) They are always orthogonal. C) They change at the same rate as the acceleration. D) They point toward the origin.
A) Zero because it is a unit vector. B) uρ multiplied by the rate of change of θ. C) uθ multiplied by the rate of change of θ. D) uρ multiplied by the rate of change of ρ.
A) Only the radial velocity. B) The angular momentum of the particle. C) Centripetal force and Euler force terms. D) The total distance travelled.
A) The radial velocity. B) The total acceleration. C) The Euler force. D) Related to the centripetal component.
A) Polar coordinates lack a time component. B) Local coordinates are always zero. C) Polar coordinates cannot be used for general motion. D) It is not straightforward to separate centripetal and Euler terms in general polar coordinates.
A) It loses its unit length. B) It points in the direction of the origin. C) It remains fixed in space. D) It rotates by dθ to remain orthogonal to uρ.
A) Positive uρ multiplied by the rate of change of θ. B) Negative uρ multiplied by the rate of change of θ. C) Positive uθ multiplied by the rate of change of θ. D) Zero.
A) The centripetal acceleration. B) The total velocity. C) The tangential acceleration. D) The Euler force.
A) r(t) × Ω dt B) dθ / dt C) Ω × r(t) dt D) Ω × (Ω × r(t))
A) The Pythagorean theorem B) Lagrange's formula C) Newton's second law D) The chain rule
A) r / ω B) ω / r² C) rω² D) Ω × r
A) Center-avoiding B) Linear motion C) Center-seeking D) Constant speed
A) Christiaan Huygens B) Johannes Kepler C) Isaac Newton D) Albert Einstein
A) Centrifugal force B) Dark energy C) Electromagnetism D) Gravity
A) Galileo Galilei B) James Clerk Maxwell C) Christiaan Huygens D) Isaac Newton
A) Newtonian constant B) Lorentz factor C) Gravity constant D) Centripetal factor
A) The ball remains perfectly still. B) The ball gains extra mass. C) The ball moves toward the center. D) The ball slides off the road.
A) Sharper turns require a steeper banking angle. B) Sharper turns require no banking. C) The turn radius does not affect the banking angle. D) Sharper turns require a shallower banking angle.
A) θ B) v C) ω D) a
A) Frenet-Serret coordinates B) Absolute coordinates C) nt-coordinates D) Cartesian coordinates
A) Arc length B) Radius of curvature C) Centripetal acceleration D) Time
A) ρ(s) = 1 - κ(s) B) ρ(s) = κ(s) C) ρ(s) = κ(s)2 D) ρ(s) = 1 / κ(s)
A) (d2s / dt2)ut B) -(v / ρ)un C) -(v2 / ρ)un D) (dv / dt)ut
A) v(s) / ρ(s) B) dθ / ds C) v(s) * ρ(s) D) ρ(s) / v(s)
A) s B) θ C) Zero D) ρ |