1P1 Mechanics Flashcards

1
Q

What are the unit vectors for cartesian, polar and intrinsic coordinates?

A

Cartesian: e_i, e_j
Polar: e_r, e_theta
Intrinsic: e_t, e_s

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2
Q

Differentiate unit vectors in polar coordinates.

A

e_rdot = e_theta x thetadot
e_thetadot = - e_r x thetadot

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3
Q

What is Euler’s method of numerical integration?

A

vn = v_n-1 + a_n-1 x t
xn = x_n-1 + v_n-1 x t

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4
Q

What is the Euler-Cromer/Semi-implicit method of integration?

A

v_n = v_n-1 + a_n-1 x t
x_n = x_n-1 + v_n x t

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5
Q

How do the Euler and semi-implicit method of integration differ in terms of energy?

A

Euler method tends to overestimate energy, growth in energy.
Whereas, the semi-implicit tends to underestimate energy.

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6
Q

Integral form of the change in kinetic energy:

A

Tb-Ta = integral(F.dr)[a->b] = integral(F.v dt) [a->b]

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7
Q

When is energy conservation true for the particles total energy?

A

When only conservative forces act on the particle

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8
Q

What is the gain in total energy of a particle equal to?

A

The work done by non-conservative forces acting on it.

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9
Q

How do you determine equilibrium positions from potential energy?

A

With conservative forces, the minima and maxima of the potential energy curves are equilibrium position.

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10
Q

How is the rate of change of linear momentum determined?

A

The total external force applied

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11
Q

How is the total change of momentum determined?

A

The total external impulse applied

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12
Q

What is the vector form of the moment of a force?

A

q = r x F

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13
Q

What is the moment of force about an axis?

A

Q = (r x F).n

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14
Q

Vector form of angular momentum?

A

h = r x p = r x (mv)

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15
Q

How is angular momentum and moment of force related

A

q = dh/dt

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16
Q

When is angular momentum conserved around an axis?

A

When all forces applied are parallel to the axis, or pass through the axis

17
Q

When is a force conservative?

A

When the work done in moving a particle from A -> B is independent of the path taken and is fully reversible.

18
Q

How do you derive the eq of motion of a satellite?

A

Using energy conservation
T+V = E where V is GPE, and T is kinetic energy v^2 = 0.5 m (rdot^2 + (r thetadot)^2)
And then differentiate since E is constant so goes to 0.

Using Newtons second law (slighlty easier)

Define specific angular moment h = ho/m = r^2 thetadot

19
Q

How to find a solution of the equation of motion of a satelite?

A

Define u = 1/r and substitute in.

20
Q

Velocity of point b on a rigid body in terms of velocity and position of point a.

A

vb =va + omega x r_b/a

21
Q

What is always true for two points on a rigid body.

A

v_b/a .e= 0 where a is in the direction r_b/a

21
Q

Equation for instantaeneous centres.

A

v = omega x instantaeneous radius

22
Q

Integral equation for centre of mass.

A

1/M integral(rdm) where r is a position vector

23
Q

Newton’s second law for rigid bodies.

A

F = M rddot_g

24
Q

Integral form of polar mass moment of inertia.

A

integral(r^2 dm)

25
Q

Perpendicular axis theorem and when is it valid.

A

For lamina it is true such that Izz = Ixx +Iyy

26
Q

Mass Moment of inertia about a certain axis.

A

Ixx = integral(y^2 + z^2 dm)

27
Q

Parallel axis theorem

A

Io = Ig + rg^2 * M.
The moment of inertia about an axis passing through O is equal to the mass moment of inertia about a parallel axis passing through the centre of gravity plus the correction term. Only works with the centre of mass.

28
Q

Relationship between total moment of the forces and angular acceleration.

A

For a planar body: q = Ig * omegadot

29
Q
A