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cheechnchong
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MY Question was answered! thanks to those who posted...i got the right answer from the book!
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Hootenanny said:HINT: To create the artificial gravitational force what must the centripetal acceleration of the space station be? How fast must the station be rotating to achieve this centripetal acceleration?
Why do you need to know anything about the centripetal acceleration? The artificial gravity would not have to be the same as Earth's gravity.Hootenanny said:HINT: To create the artificial gravitational force what must the centripetal acceleration of the space station be? How fast must the station be rotating to achieve this centripetal acceleration?
Indeed, I was wrong. This should be treated as a conservation of angular momentum problem. Good Catch Dan, apologies to chee.OlderDan said:Why do you need to know anything about the centripetal acceleration? The artificial gravity would not have to be the same as Earth's gravity.
Hootenanny said:Indeed, I was wrong. This should be treated as a conservation of angular momentum problem. Good Catch Dan, apologies to chee.
Office_Shredder said:You know what I is initally. You should be able to figure out what I is if everyone is in the center. You should also be able to figure out what I is if everyone is on the outer shell.
You know Iw is constant (angular momentum is constant), so put I when everyone is in the middle over I when everyone is on the outside, you get w when everyone is on the outside over w when everyone is inside
Hootenanny said:Indeed, I was wrong. This should be treated as a conservation of angular momentum problem. Good Catch Dan, apologies to chee.
Rotational kinematics is the branch of physics that deals with the motion of objects that are rotating around an axis. It involves studying the position, velocity, and acceleration of these objects as they rotate.
While linear kinematics deals with the motion of objects in a straight line, rotational kinematics deals with the motion of objects in a circular or curved path. This means that rotational kinematics involves studying angular displacement, angular velocity, and angular acceleration, rather than linear displacement, linear velocity, and linear acceleration.
The equation for rotational kinematics is θ = ωt + ½αt², where θ is angular displacement, ω is angular velocity, α is angular acceleration, and t is time. This equation is similar to the equation for linear kinematics, but it uses angular instead of linear quantities.
Rotational kinematics can be seen in many everyday activities, such as swinging on a playground swing, spinning a top, or throwing a frisbee. It is also essential in understanding the motion of celestial bodies, such as planets and stars, and in designing and analyzing machines like gears and turbines.
Rotational motion can affect an object's kinetic energy by changing its rotational kinetic energy. As an object rotates faster, its rotational kinetic energy increases, and as it slows down, its rotational kinetic energy decreases. This means that rotational motion can have a significant impact on the overall kinetic energy of an object.