There are 16 problems. Please give a short explanation for all multiple choice questions. Show your work for all numerical answers.
G =
N
m
/kg
Earth's mass
kg
Earth's radius
m
Moon's mass
kg
Moon's radius
m
Earth-Moon distance
m
Earth-Sun distance
m
PE = mgh.
1 kg rock: PE = 1 kg * 10 m/s^2 * 6 m = 60 J
2 kg rock: PE = 2 kg * 10 m/s^2 * 3 m = 60 J
If you drop it from higher up, it will be
going faster when it hits.
Yes, I know that they both have the same
kinetic energy when they hit. The question asked about speed, not
energy. KE = 0.5 mv^2. The 2 kg rock has more mass os it must
have less v^2 when it hits.
B hits first. The horizontal speeds
are irrelevant so we can make them zero. In that case, the question
becomes: 'If you throw A higher up than B, which one lands first?'
Clearly, the ball that is thrown higher up stays in the air longer.
The answer is thus B lands first.
W = F d = 100 N * 5 m = 500 Nm =
500 J
The force and distance are in the same
direction.
If I push him twice as far, I will
do twice as much work. Thus I will double his kinetic energy.
This means that his velocity will increase. We know that doubling
the velocity will quadruple KE so the velocity cannot increase that much.
Thus the answer has to be 'between v and 2v'.
Changing the size of the sun does not change
the distance between the center of the sun and the center of the Earth.
Therefore the force will not change.
The earth is so large, that if we move around
on it, we will not change its rotational velocity significantly.
(We looked at this in a home work problem.) Therefore rotational
velocity is fixed.
The earth rotates around its axis. The
axis passes through the north and south poles. Therefore, the farther
you move from the poles, the farther you are from the axis. At the
equator, you are farthest from the axis and your distance to the axis is
equal to the radius of the earth. Therefore, by moving from Norfolk
to the equator, you are increasing the radius of the circle you are moving
in. This means that your linear velocity increases.
The platform is free to rotate. This
means that once it is spinning, there is no motor to keep it spinning at
the same rotational velocity. It also means that there is no external
torque so that angular momentum is conserved.
To get full credit for the problem, you needed
to point out that a) angular momentum is conserved, b) that the moment
of inertia decreases when the children move closer to the axis, and that
therefore c) angular velocity has to increase.
The horizontal velocity is irrelevant.
The only thing that matters is that the rock falls 20 m vertically.
Using d = 1/2 g t^2 we can see that a rock drops 5 m in the first second,
and 20 m in the first 2 seconds. Thus, the answer is 2 s.
Note that falling objects do NOT fall at constant
velocity. You cannot say that because a rock falls 5 m in the first
second that it will continue to fall at 5 m/s. It speeds up.
You need a centripetal force of F = mv^2/r
to stay on the curve. If you double v, then you need 4 times as much
force. You can do this either symbolically:
F(30 mph) = mv^2/r -> F(60 mph) = m (2v)^2 /
r = m4v^2 / r = 4 (mv^2 / r) = 4 * F(30 mph)
or by choosing some totally arbitrary value for
r, plugging in numbers, and seeing what you get.
Gravitational force = GMm/R^2
Tidal force = difference in gravitational force
= gravitational force on the side of the Earth closest to the moon minus
the gravitational force on the side of the Earth farthest from the moon.
If the Earth gets bigger (but the distance from the center of the Earth
to the center of the moon stays unchanged), then the distance from the
moon to the near side of the Earth gets smaller so the force on the near
side of the Earth increases. Similarly, the distance from the moon
to the far side of the Earth gets bigger so the force on the far side of
the Earth decreases. Therefore, the difference between the force
on the far side and force on the near side increases, increasing tidal
forces.
Alternatively, you can use the equation that tidal force = GMmd/R^3 where d is the size of the Earth and R is the Earth-moon distance. Increasing d increases the tidal force.
Alternatively, we know that the tidal force on
the water in a swimming pool is incredibly infinitesimally tiny because
the pool is small. The tidal force on the water on the Earth is bigger
because the Earth is bigger. Therefore, if we increase the size of
the Earth, we increase the tidal force.
The orbital speed of 8 km/s near the surface
of the Earth comes from a) the curvature of the Earth is 5 m in 8
km and b) objects fall 5 m in 1 second. If we go further from the
Earth then g is smaller so objects fall more slowly. This means
that it takes more than 1 second to fall 5 m so the minimum velocity
is less than 8 km/s.
Torque = force times lever arm. When
you reduce the lever arm, you need more force to apply the same torque.
They appear weightless because there is no
normal force on them. Gravity still sucks.
D tips over, A might tip over, B and C are stable. Draw a line vertically downward from the center of mass. If it passes through the base of the object, then it is stable. A vertical line drawn downward from the CoM of D will pass to the left of the base. It will fall over. A vertical line drawn downward from the CoM of A will pass through the leftmost point on the base.