Total Members Voted: 5
0 Members and 162 Guests are viewing this topic.
"Rotational radius" is a fictitious concept that no engineer uses.
Please, please, use your definition of torque to address the simple question: what force is required on the parking brake pads to prevent the car from rolling down a hill? I guess around a million cars will have been made since I asked that question, so umpteen engineers who you assert do not understand torque, seem to have worked it out satisfactorily, and all you have done is introduce irrelevancies.Please don't accuse me of defining or using the term "rotational radius" - it's entirely yours.
I've already gave the equations.
What's the torque produced by each forces?
"What radius do you use instead?" The distance from where the force is applied to the fulcrum point.
QuoteI've already gave the equations.And nowhere did they involve angular displacement.QuoteWhat's the torque produced by each forces?Zero, as there is no fulcrum point. But if you reverse or remove one of the forces it is obvious that the rod will rotate. The interesting question is where the center of rotation would be!
In this video Paul Andersen explains rotating object have angular momentum. The angular momentum of a point object is the product of the distant from the center of rotation and the linear momentum. The angular momentum of an extended object is a product of the rotational inertia and the angular velocity. The change in angular momentum is equal to the product of the net torque and the change in time.
Kepler's laws of planetary motion are deeply connected to the conservation of angular momentum, a fundamental principle in physics stating that the angular momentum of a system remains constant unless acted upon by an external torque. Here's how each of Kepler's three laws relates to this concept:First Law (Law of Ellipses): Planets move in elliptical orbits with the Sun at one focus. This law describes the shape of the orbit but doesn't directly address angular momentum. However, the elliptical path ensures that the planet's distance from the Sun varies, which ties into the second law. The absence of external torques (assuming a two-body system with no significant external forces) means angular momentum is conserved throughout the orbit, allowing the planet to follow a stable elliptical path.Second Law (Law of Equal Areas): A line segment joining a planet to the Sun sweeps out equal areas in equal intervals of time. This is a direct consequence of angular momentum conservation. Angular momentum for a planet is given by L=mr^2ω, where ( m ) is the planet's mass, ( r ) is the distance from the Sun, and ω is the angular velocity. Since no external torques act on the planet-Sun system, ( L ) is constant. When the planet is closer to the Sun (smaller ( r )), it moves faster (higher ω) to keep r^2ω constant, sweeping out the same area per unit time as when it is farther away and moving slower. The area swept per unit time is proportional to r^2ω, which remains constant due to conserved angular momentum.Third Law (Law of Periods): The square of a planet?s orbital period is proportional to the cube of the semi-major axis of its orbit (T^2 ∝ a^3). This law relates to angular momentum indirectly through the dynamics of the orbit. For a circular orbit (a simplified case), angular momentum is L=mrv, and velocity v=√(GM/r) (from gravitational force balancing centripetal force). Substituting, L=m√GMr. For elliptical orbits, the semi-major axis ( a ) plays a similar role. The conservation of angular momentum ensures the orbit remains stable, and the third law emerges from the balance of gravitational forces and orbital dynamics, with angular momentum constraining the relationship between period and distance.In essence, conservation of angular momentum underpins Kepler?s second law explicitly and supports the first and third laws by ensuring the stability and predictability of planetary orbits in the absence of external torques. The gravitational force between the planet and Sun is radial (along the line connecting them), producing no torque, so angular momentum remains constant, shaping the elliptical orbits and their timing as described by Kepler.
More obfuscation, as usual.
In view of Hamdani's consistent refusal to use his new definition of torque to solve a simple question of statics, and his apparent inability to identify a fulcrum in his own drawings, I can only conclude that his redefinition serves no purpose other than to confuse him.That being said, if a really clever engineer such as Hamdani can't understand the fault in his own proposal, it has no place in the education of the young.So I won't contribute any further.
If your definition of rotational radius doesn't equal to ∂d/∂θ, you're defining it wrong.
Quote from: alancalverd on 11/04/2025 11:00:43QuoteI've already gave the equations.And nowhere did they involve angular displacement.QuoteWhat's the torque produced by each forces?Zero, as there is no fulcrum point. But if you reverse or remove one of the forces it is obvious that the rod will rotate. The interesting question is where the center of rotation would be! What's important is ∂d/∂θ.If the right force is moved slightly closer to the center of the rod, what the torque will be?If the right force is slightly reduced, what the torque will be?Is there any change in the number of fulcrum?
.... so everyone else who read this thread can learn...
Rotational radius equals derivative of rotational displacement with respect to rotational angle.