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Why do we care if the mass is still falling or has hit the table or ground before the disc finishes rotating?
It is important to release the disc with the pinhole as close as possible to the photogate because:
Consider a small sphere with a radius of R=1 cm and mass of m=50 g, attached to one end of a nearly massless rod of length r=3 m.
If someone rotates the rod and sphere using the free end of the rod (the end without the sphere attached) as the axis of rotation, what is the moment of inertia of the combined rod and sphere?
Enter your answer exactly as it appears on your calculator, in SI units, but do not type the units.
What is the angular velocity of the hour hand of a clock (which completes 1 revolution in 12 hours) in radians per second.
Give your answer to 3 significant figures and do NOT type the units. That is, to enter 0.00098212 rad/s, you would type 0.000982
True or False:
Torque plays the same role in rotational dynamics as force does in linear dynamics.
True or False:
The centre of mass of an object describes how the object resists changes to its rotational motion.
Why is the transfer orbit more efficient than a direct flight to the Mun?
Assuming you have managed to complete your crossing and timed things well, you are likely to encounter the Mun and make a hyperbolic pass of the Mun rather than actually orbit it. What should you do now to enter orbit?
How do we actually depart our original orbit around Kerbin and start on the Transfer orbit?
If we start our transfer orbit and depart for the Mun at the point indicated along the space craft orbit, where should the Mun be at this same time? I.e., What angle on the scale corresponds to the Mun's location when we depart?