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