Module 13: 2D and 3D Equilibrium Equations

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來自 Georgia Institute of Technology 的課程

工程力学导论

1204 個評分

Georgia Institute of Technology

工程力学导论

1204 個評分

This course is an introduction to learning and applying the principles required to solve engineering mechanics problems. Concepts will be applied in this course from previous courses you have taken in basic math and physics. The course addresses the modeling and analysis of static equilibrium problems with an emphasis on real world engineering applications and problem solving. The copyright of all content and materials in this course are owned by either the Georgia Tech Research Corporation or Dr. Wayne Whiteman. By participating in the course or using the content or materials, whether in whole or in part, you agree that you may download and use any content and/or material in this course for your own personal, non-commercial use only in a manner consistent with a student of any academic course. Any other use of the content and materials, including use by other academic universities or entities, is prohibited without express written permission of the Georgia Tech Research Corporation. Interested parties may contact Dr. Wayne Whiteman directly for information regarding the procedure to obtain a non-exclusive license.

從本節課中

Equilibrium and Equivalence of Force Systems

In this section, students will learn the equilibrium equations in two (2D) and three (3D) dimensions. Students will solve equivalent system problems. System force results will be defined and calculated.

Module 13: 2D and 3D Equilibrium Equations4:34

Module 14: Conditions for Equivalent Equations9:21

Module 15: Solve an Equivalent Systems Problem10:34

Module 16: Single Force Resultants-Coplanar System5:08

Module 17: Single Force Resultants-Parallel Force Systems7:10

Module 18: Distributed Force Systems9:22

與講師見面

Dr. Wayne Whiteman, PE
Senior Academic Professional
Woodruff School of Mechanical Engineering

Hi, and welcome to module thirteen of an Introduction to Engineering Mechanics.

Today, we're going to express the 2D and 3D static equilibrium equations. We're

going to recognize and apply the principle of transmissibility and we're going to

explain the relationships between sums of moments. So let's start off by looking at

the static equilibrium equations. In vector form for static equilibrium, we

have to have a balance of forces and we have to have a balance of moments about a

point p, where p is any point that we choose, and so, let's look at this first

of all in, in Dd. So we have to have a balance of forces in two orthogonal

directions in the plane, so I've got an x direction here and a y direction. So I, I

don't have any acceleration in the x direction, I don't have any acceleration

in the y direction, and so, that's a balance of forces that keeps it in static

equilibrium there. And I also don't have any angular acceleration about any point

and this point can be on or off the body. And so, it could be a point p down here,

at the origin or up here, but there is no angular acceleration either, and so,

that's for 2D in, in a plane. we have three independent equations in that case.

When we go to 3D we have six independent equations, because now, we not only have

to have a balance of forces in the x and y direction, but we also have to have a

balance of forces in a z direction. And, instead of a moment around the, the normal

to the plane of the moment, moment about the z-axis in this case, we also have to

have a balance of moments about the, the x-axis and about the y-axis for any point,

again, on the body or off the body. And so, those are, are our static equilibrium

equations. Let's next look at the principle of transmissibility. And so,

what the principle of transmissibility says is that for a body like this or if we

consider this a rigid body, if I have a force and I push on the body here, that

force, if it's the same magnitude, and I pull on the other side in the same line of

action, it, it externally, it doesn't matter. Okay?

That force can be transmitted along the line of absolute force and works anywhere.

Now, internally, if the body were to be able to deform, then it would make a

difference, but that's, that's for a future course in mechanics and materials.

In this course, we're only dealing with rigid bodies. let's next look at the

relationship between sums of moments. If a body is in static equilibrium, again, the

sum of the forces vectorially has to be equal to zero and the sum of the moments

about any point p has to be equal to zero. And I said that we could pick point p

maybe down here at the origin or another place, but if, if we have static

equilibrium, then the moments about any point, any arbitrary point a we choose on

or off the body has to also be equal zero. And so, here is an example. I've got a

have a cantilever beam here, and, if I have some of the forces equal to zero, and

sum of the moments about p equals zero, then the sum of the moments about point A,

or about point B as it's shown, or about point C, all have to be equal to zero. So

we may sum moments about any point to enforce static equilibrium and we'll do

that in example problems in future modules, so, what that leads to is, is for

the static equilibrium equations, in 2D. Again, we said, some of the force in x,

and the y, and moments about a point equals zero in fact we may even have two

orthogonal directions, which would be on a slope. So we may have a parallel,

direction the slope and a perpendicular direction to the slope and a, and a moment

again about any point, force and static equilibrium, or since there's three

independent equations, we may have the sum of the forces in just one direction, which

may be along an arbitrary line equal to zero and we could sum moments about two

points, maybe a point here and a point here. again, or we can sum moments about

three points and have three independent equations and, and we'll use all of these

cases in, in, in problems that we solve. But, just realize that the sum of the

forces, the sum of the moments have to be equal to zero vectorially and we can get

three independent equations in 2D. And so I look forward to working with you in

future modules to use these equations to solve some real world problems.

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