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In the Case Shown in (Figure 1), Specify the Distance Where the Resultant Force Acts From Point O.

In this explainer, we will learn how to notic the moment of a platelike system of forces temporary on a body about a guide as a transmitter.

We know that a force, operating room a system of forces, pot have a rotational effect along a trunk, which is described by the moment of the force play, operating room the system of forces, about a point. We recollection that in planar motion, the moment 𝑀 of force ⃑ 𝐹 about a point is defined to be a scalar whose magnitude is apt away | 𝑀 | = β€– β€– ⃑ 𝐹 β€– β€– 𝑑 , βŸ‚ where 𝑑 βŸ‚ is the perpendicular distance 'tween the point and the assembly line of action for force ⃑ 𝐹 . We can then determine the sign of the moment by considering whether the move effect is clockwise or counterclockwise. By convention, we define the moment with the counterclockwise effect to be positive, which means the moment with the clockwise motility burden is defined to be negative.

While this definition works well for planar motion, it is insufficient when we view the motion with a 3-magnitude space because the notion of clockwise operating room left-handed notation does not hold here. Hence, we would comparable to extend the definition of the moment to 3D motion from the scalar moment circumscribed for planar motion. Systematic to preserve the whim of the orientation of a rotation, we define a moment to be a vector as follows.

Definition: Minute of a Force

The moment of a force ⃑ 𝐹 acting along a body, taken over about point 𝑂 , is given by οƒŸ 𝑀 = ⃑ π‘Ÿ Γ— ⃑ 𝐹 , where π‘Ÿ is the position vector of 𝐴 , the point of application of force ⃑ 𝐹 .

Therein definition, we run into that the organise organization has been chosen so much that its origin coincides with the point about which we take the moment. If we wanted to compute the moment of force out ⃑ 𝐹 about point 𝑃 that is not the origin, then we would simply replace ⃑ π‘Ÿ with οƒŸ 𝑃 𝐴 : οƒŸ 𝑀 = οƒŸ 𝑃 𝐴 Γ— ⃑ 𝐹 . 

The letter 𝑃 has been added as a subscript to οƒŸ 𝑀 to indicate that the here and now is taken about point 𝑃 .

In our get-go example, we will apply this formula to cypher the vector moment of a force on a plane about a stop.

Instance 1: Finding the Moment of a Pull along Transmitter about a Point

If the force ⃑ 𝐹 = βˆ’ 5 ⃑ 𝑖 + π‘š ⃑ 𝑗 is acting at the channelis 𝐴 ( 7 , 3 ) , determine the moment of ⃑ 𝐹 about the point 𝐡 ( 7 , βˆ’ 2 ) .

Answer

In this example, we need to find the bit of a planar force approximately a compass point. Recall that the transmitter moment of force ⃑ 𝐹 playing at point 𝐴 about peak 𝐡 is inclined away οƒŸ 𝑀 = οƒ  𝐡 𝐴 Γ— ⃑ 𝐹 .

Let USA begin by determination the vector οƒ  𝐡 𝐴 : οƒ  𝐡 𝐴 = ( 7 , 3 , 0 ) βˆ’ ( 7 , βˆ’ 2 , 0 ) = ( 0 , 5 , 0 ) .

We can write out ⃑ 𝐹 as ⃑ 𝐹 = βˆ’ 5 ⃑ 𝑖 + π‘š ⃑ 𝑗 + 0 ⃑ π‘˜ = ( βˆ’ 5 , π‘š , 0 ) .

Taking the vector product, οƒ  𝐡 𝐴 Γ— ⃑ 𝐹 = | | | | ⃑ 𝑖 ⃑ 𝑗 ⃑ π‘˜ 0 5 0 βˆ’ 5 π‘š 0 | | | | = ( 5 Γ— 0 βˆ’ 0 Γ— π‘š ) ⃑ 𝑖 βˆ’ ( 0 Γ— 0 βˆ’ 0 Γ— ( βˆ’ 5 ) ) ⃑ 𝑗 + ( 0 Γ— π‘š βˆ’ 5 Γ— ( βˆ’ 5 ) ) ⃑ π‘˜ = 2 5 ⃑ π‘˜ .

We note that the unbeknownst ceaseless π‘š in the force out ⃑ 𝐹 cancelled out when we computed the cross product. Hence, the moment of ⃑ 𝐹 about point 𝐡 is 2 5 ⃑ π‘˜ .

In the previous example, we computed the vector import of a planar pull in approximately a orient using the chemical formula οƒŸ 𝑀 = ⃑ π‘Ÿ Γ— ⃑ 𝐹 .

We tail see that the sequent transmitter of the cross product simply contained a ⃑ π‘˜ component, and the ⃑ 𝑖 and ⃑ 𝑗 components nonexistent. This is not surprising if we consider the nonrepresentational property of a sweep merchandise. Recall that a vector resulting from the cross product of two vectors must cost perpendicular to the deuce vectors. Since οƒŸ 𝑀 is defined to be the cross product of vectors ⃑ π‘Ÿ and ⃑ 𝐹 , it must be perpendicular to both vectors. We know that ⃑ π‘Ÿ and ⃑ 𝐹 both lie on the π‘₯ 𝑦 -flat, so οƒŸ 𝑀 should exist perpendicular to the π‘₯ 𝑦 -plane. A vector that is perpendicular to the π‘₯ 𝑦 -plane should be parallel to the unit vector ⃑ π‘˜ in the 3-dimensional organise system. This means ⃑ π‘Ÿ Γ— ⃑ 𝐹 = 𝑐 ⃑ π‘˜ for some scalar 𝑐 . Since this is e'er the case, we can simplify the calculation of this cross product by victimization the 2D vector product.

Definition: 2D Vector product

Given two 2D vectors ( π‘Ž , 𝑏 ) and ( 𝑐 , 𝑑 ) , the 2D cross merchandise is defined by ( π‘Ž , 𝑏 ) Γ— ( 𝑐 , 𝑑 ) = ( π‘Ž 𝑑 βˆ’ 𝑏 𝑐 ) ⃑ π‘˜ .

As we can construe with, the 2D vector product is quicker to compute. We will use this formula to compute the grumpy product betwixt 2D vectors for the residue of this explainer.

Next, let us talk about the magnitude of the moment, which is capable the order of magnitude of the vector product: β€– β€– οƒŸ 𝑀 β€– β€– = β€– β€– ⃑ π‘Ÿ Γ— ⃑ 𝐹 β€– β€– .

Recall that the crisscross cartesian product between two vectors gives the area of the parallelogram whose cardinal adjacent sides are horn-shaped by the two vectors. Let us detect this using the following diagram.

In the diagram above, the area of the highlighted region represents the order of magnitude of the thwartwise product ⃑ π‘Ÿ Γ— ⃑ 𝐹 and hence the magnitude of the minute οƒŸ 𝑀 . We stern as wel find the area of this parallelogram geometrically away victimisation the geometric formula l e n g t h o f t h e b a s e p e r p e n d i c u l a r h e i g h t Γ— .

In the diagram, the base of this parallelogram is formed past vector ⃑ 𝐹 , and the height is the plumb line distance from the origin to the personal line of credit of action of ⃑ 𝐹 , which is denoted 𝑑 βŸ‚ .

This leads to the tailing formula for the magnitude of the vector instant for a 2D forcefulness about a signal.

Property: Magnitudes of the Transmitter Instant of a Pull up

The magnitude of the vector moment of a planar force ⃑ 𝐹 about a point is given by β€– β€– οƒŸ 𝑀 β€– β€– = β€– β€– ⃑ 𝐹 β€– β€– 𝑑 , βŸ‚ where 𝑑 βŸ‚ is the plumb line distance between the full point and the line of action of force ⃑ 𝐹 .

We can see that the magnitude of the vector consequence given above is equal to the magnitude of the scalar moment. Hence, the order of magnitude of the vector import is consistent with that of the scalar moment for planar motion.

When we rearrange this equation, we obtain a useful formula for computing the perpendicular distance between a point and a furrow of action of a force.

Rul: Perpendicular Aloofness 'tween a Point and a Personal credit line of Action

Let οƒŸ 𝑀 glucinium the vector second of a force, or a system of forces, happening a plane about a point. Then, the perpendicular distance between the point and the line of action of the force is presented aside 𝑑 = β€– β€– οƒŸ 𝑀 β€– β€– β€– β€– ⃑ 𝐹 β€– β€– . βŸ‚

In the next example, we will reckon the moment of a planar force about a point and then exercise this formula to find the perpendicular outdistance between the point and the line of action mechanism of the thrust.

Example 2: Finding the Moment Transmitter of a Force Acting at a Point and the Perpendicular between the Moment and the Line of Action of the Ram

Precondition that pull in ⃑ 𝐹 = 4 ⃑ 𝑖 βˆ’ 3 ⃑ 𝑗 acts through the point 𝐴 ( 3 , 6 ) , determine the here and now οƒŸ 𝑀 about the origin 𝑂 of the force ⃑ 𝐹 . Also, calculate the steep length 𝐿 between 𝑂 and the line of natural action of the force.

Result

In this representative, we need to first find the moment οƒŸ 𝑀 about 𝑂 of the force ⃑ 𝐹 and then calculate the perpendicular space betwixt 𝑂 and the line of action of ⃑ 𝐹 . Let United States of America begin by determination the bit. Call back that the vector moment of force ⃑ 𝐹 temporary at point 𝐴 about the origin 𝑂 is minded past οƒŸ 𝑀 = οƒ  𝑂 𝐴 Γ— ⃑ 𝐹 .

We are given the coordinates of 𝐴 , which substance that οƒ  𝑂 𝐴 is the position vector given by οƒ  𝑂 𝐴 = ( 3 , 6 ) .

We can write ⃑ 𝐹 in component form as ⃑ 𝐹 = 4 ⃑ 𝑖 βˆ’ 3 ⃑ 𝑗 = ( 4 , βˆ’ 3 ) .

In real time, we are ready to figure out the cross product οƒ  𝑂 𝐴 Γ— ⃑ 𝐹 . Think that the cross product of 2D vectors is defined by ( π‘Ž , 𝑏 ) Γ— ( 𝑐 , 𝑑 ) = ( π‘Ž 𝑑 βˆ’ 𝑏 𝑐 ) ⃑ π‘˜ .

Applying this formula, we obtain οƒ  𝑂 𝐴 Γ— ⃑ 𝐹 = ( 3 , 6 ) Γ— ( 4 , βˆ’ 3 ) = ( 3 Γ— ( βˆ’ 3 ) βˆ’ 6 Γ— 4 ) ⃑ π‘˜ = βˆ’ 3 3 ⃑ π‘˜ .

Hence, the moment of ⃑ 𝐹 about the origin is βˆ’ 3 3 ⃑ π‘˜ .

Next, let us find the perpendicular distance between the root and the line of action for ⃑ 𝐹 . Recall that the order of magnitude of the vector moment of a planar hale ⃑ 𝐹 about a point is given by β€– β€– οƒŸ 𝑀 β€– β€– = β€– β€– ⃑ 𝐹 β€– β€– 𝐿 , where 𝐿 is the perpendicular distance between the guide and the agate line of action for force ⃑ 𝐹 . We give notice rearrange this equation to write 𝐿 = β€– β€– οƒŸ 𝑀 β€– β€– β€– β€– ⃑ 𝐹 β€– β€– .

Since we know οƒŸ 𝑀 = βˆ’ 3 3 ⃑ π‘˜ , we can obtain β€– β€– οƒŸ 𝑀 β€– β€– = 3 3 . Countenance us find β€– β€– ⃑ 𝐹 β€– β€– : β€– β€– ⃑ 𝐹 β€– β€– =  4 + ( βˆ’ 3 ) = √ 2 5 = 5 .  

Subbing these values into the formula for 𝐿 , we obtain 𝐿 = 3 3 5 = 6 . 6 .

Hence, οƒŸ 𝑀 = βˆ’ 3 3 ⃑ π‘˜ , 𝐿 = 6 . 6 . l e n g t h u n i t s

We give birth far-famed that the here and now of a force active a point results in a vector that is parallel to the unit vector ⃑ π‘˜ . Put differently, on that point is some scalar 𝑐 such that οƒŸ 𝑀 = 𝑐 ⃑ π‘˜ .

Additionally, we discovered that the order of magnitude of the moment is equal to the magnitude of the scalar moment | 𝑀 | . This means that either 𝑐 = 𝑀 or 𝑐 = βˆ’ 𝑀 . To ascertain which one is true, we want to examine whether or not the sign of 𝑐 matches the sign of the musical notation moment 𝑀 .

The properties of the cross product take into account US to conclude premiere that οƒŸ 𝑀 is a vector perpendicular to the plane defined by ⃑ π‘Ÿ and ⃑ 𝐹 . The instruction of οƒŸ 𝑀 is given by the powerful-hand pattern. This rule is sometimes explained aside referring to the rotary motion of a screw: the direction of the vector ⃑ 𝐴 Γ— ⃑ 𝐡 corresponds to the direction of the front (up or down) of a bottle hat Oregon a junkie that peerless would turn in the same sense of rotation As when going from ⃑ 𝐴 to ⃑ 𝐡 , American Samoa illustrated in the following diagram.

Remember that we experience οƒŸ 𝑀 = ⃑ π‘Ÿ Γ— ⃑ 𝐹 = 𝑐 ⃑ π‘˜ .

If 𝑐 > 0 , the import vector would be coming out of the plane (up), which corresponds to sinistral rotary motion reported to the image above. If 𝑐 < 0 , the moment vector would go into the plane (down), which indicates clockwise rotary motion. Recall that for a scalar moment 𝑀 , the counterclockwise orientation corresponds to the formal sign, while the clockwise rotary motion leads to the negative signalize. This tells us that the subscribe of the magnitude relation moment 𝑀 agrees with the sign of the scalar 𝑐 . Hence, we have shown that 𝑐 = 𝑀 .

Property: 2D Transmitter Moment of a Force

Let 𝑀 and οƒŸ 𝑀 be the quantitative relation and transmitter moments of a force, or a system of forces, happening a plane about a point. Then, οƒŸ 𝑀 = 𝑀 ⃑ π‘˜ .

This place securely establishes wherefore this vector moment is a reasonable extension of the scalar moment for a coplanar force. Moreover, the vector moment can be generalized to represent a moment of a universal 3D force about a point since it is obtained using the cross intersection.

We john deduce several useful observations from this place. Firstly, we know that the quantitative relation moment does not depend on the localisation of the point the force is acting connected, A long as the point lies on the synoptical line of action of the force. This is because the magnitude relation moment is obtained by simply using the magnitude of the force β€– β€– ⃑ 𝐹 β€– β€– and the perpendicular distance 𝑑 βŸ‚ . This means that the vector here and now is also independent of the location of the point at which the push is acting. We can read this better when we equate the magnitude of the consequence when we move this point along the line of military action.

We hind end see that the areas of both parallelograms are equate since the duration of the base β€– β€– ⃑ 𝐹 β€– β€– and the height 𝑑 βŸ‚ are the very for both parallelograms. This tells US that the magnitude of the moment for these cardinal systems is the same. Furthermore, we crapper see that both system would cause the dextrorotation about the origin, meaning that the sign of the moment would be the same for both systems. Thence, the transmitter moment is the same for these two systems. This leads to the following useful property.

Property: Vector Moment of a Force

The vector moment οƒŸ 𝑀 of a force near a point is independent of the point at which the wedge Acts, as durable as the point lies in the same line of action.

In the next example, we will find the transmitter moment of a flat force virtually a point when the first point 𝐴 is not given.

Example 3: Finding the Moment of a Force Vector Acting at a Point

End 𝐴 of 𝐴 𝐡 is at ( βˆ’ 6 , 7 ) and 𝐴 𝐡 has midpoint 𝐷 ( βˆ’ 7 , 1 ) . If the line of action of the force ⃑ 𝐹 = βˆ’ 2 ⃑ 𝑖 βˆ’ 6 ⃑ 𝑗 bisects 𝐴 𝐡 , determine the moment of ⃑ 𝐹 about point 𝐡 .

Answer

In this example, we need to find the moment of a planar force about a point. Recall that the vector here and now of thrust ⃑ 𝐹 acting at point 𝑃 about point 𝑂 is given by οƒŸ 𝑀 = οƒŸ 𝑂 𝑃 Γ— ⃑ 𝐹 .

Piece we are non given the point at which the pull is acting, we are given that the line of action of force ⃑ 𝐹 bisects 𝐴 𝐡 . This substance that the tune of natural action passes through the midpoint 𝐷 of 𝐴 𝐡 . Retrieve that the vector moment οƒŸ 𝑀 of a pull up nigh a point is independent of the initial point, A protracted as the spot lies in the unchanged phone line of action. Hence, we can compute the moment by considering the first point to beryllium at 𝐷 ( βˆ’ 7 , 1 ) . This means that the instant of ⃑ 𝐹 about 𝐡 is donated by οƒŸ 𝑀 = οƒ  𝐡 𝐷 Γ— ⃑ 𝐹 .

Let us begin away finding vector οƒ  𝐡 𝐷 . Since 𝐷 is the centre of 𝐴 , we know that β€– β€– οƒ  𝐴 𝐷 β€– β€– = β€– β€– οƒ  𝐡 𝐷 β€– β€– .

Also, these vectors have the opposite direction, which means οƒ  𝐡 𝐷 = βˆ’ οƒ  𝐴 𝐷 .

We can find οƒ  𝐴 𝐷 by using the coordinates of points 𝐴 and 𝐷 : οƒ  𝐴 𝐷 = ( βˆ’ 7 , 1 ) βˆ’ ( βˆ’ 6 , 7 ) = ( βˆ’ 1 , βˆ’ 6 ) .

Hence, οƒ  𝐡 𝐷 = βˆ’ ( βˆ’ 1 , βˆ’ 6 ) = ( 1 , 6 ) .

Now, we are ready to cypher the cross product οƒ  𝐡 𝐷 Γ— ⃑ 𝐹 . Recall that the cross product of 2D vectors is defined by ( π‘Ž , 𝑏 ) Γ— ( 𝑐 , 𝑑 ) = ( π‘Ž 𝑑 βˆ’ 𝑏 𝑐 ) ⃑ π‘˜ .

Applying this formula, we hold οƒ  𝐡 𝐷 Γ— ⃑ 𝐹 = ( 1 , 6 ) Γ— ( βˆ’ 2 , βˆ’ 6 ) = ( 1 Γ— ( βˆ’ 6 ) βˆ’ 6 Γ— ( βˆ’ 2 ) ) ⃑ π‘˜ = 6 ⃑ π‘˜ .

Hence, the moment of ⃑ 𝐹 about point 𝐡 is 6 ⃑ π‘˜ .

In the next lesson, we will find oneself the second of a organisation of planar forces acting at a single point about another point away first finding the consequent of the forces.

Illustration 4: Calculating the Moment of Cardinal Forces Acting on a Single Place about a Given Guide and the Distance between the Points

Given that ⃑ 𝐹 = βˆ’ 2 ⃑ 𝑖 + 2 ⃑ 𝑗  , ⃑ 𝐹 = βˆ’ 3 ⃑ 𝑖 βˆ’ ⃑ 𝑗  , and ⃑ 𝐹 = ⃑ 𝑖 βˆ’ 4 ⃑ 𝑗  are playing at the full stop 𝐴 ( 2 , 3 ) , determine the moment ⃑ π‘š of the resultant of the forces about the point 𝐡 ( βˆ’ 2 , βˆ’ 1 ) , and calculate the length of the perpendicular line 𝐿 connexion the point 𝐡 to the subsequent's line of action.

Response

Therein instance, we are given a system of planar forces impermanent at the Sami bespeak. Let U.S.A begin by finding the resultant of the forces. Recall that the resultant of a system of forces acting at the cookie-cutter tip is the aggregate of all force vectors in the system. Hence, the resultant ⃑ 𝐹 is given by ⃑ 𝐹 = ⃑ 𝐹 + ⃑ 𝐹 + ⃑ 𝐹 = ο€Ί βˆ’ 2 ⃑ 𝑖 + 2 ⃑ 𝑗  + ο€Ί βˆ’ 3 ⃑ 𝑖 βˆ’ ⃑ 𝑗  + ο€Ί ⃑ 𝑖 βˆ’ 4 ⃑ 𝑗  = ο€Ί βˆ’ 2 ⃑ 𝑖 βˆ’ 3 ⃑ 𝑖 + ⃑ 𝑖  + ο€Ί 2 ⃑ 𝑗 βˆ’ ⃑ 𝑗 βˆ’ 4 ⃑ 𝑗  = βˆ’ 4 ⃑ 𝑖 βˆ’ 3 ⃑ 𝑗 .   

This tells us that the resultant of the forces is ⃑ 𝐹 = βˆ’ 4 ⃑ 𝑖 βˆ’ 3 ⃑ 𝑗 . Following, let us find the moment ⃑ π‘š of the resultant well-nig point 𝐡 ( βˆ’ 2 , βˆ’ 1 ) . Recall that the vector moment of force ⃑ 𝐹 playing at point 𝐴 about show 𝐡 is minded past οƒŸ 𝑀 = οƒ  𝐡 𝐴 Γ— ⃑ 𝐹 .

Exploitation the coordinates of 𝐴 and 𝐡 , we toilet find οƒ  𝐡 𝐴 = ( 2 , 3 ) βˆ’ ( βˆ’ 2 , βˆ’ 1 ) = ( 4 , 4 ) .

Today, we are ready to calculate the cross product οƒ  𝐡 𝐴 Γ— ⃑ 𝐹 . Return that the vector product of 2D vectors is defined by ( π‘Ž , 𝑏 ) Γ— ( 𝑐 , 𝑑 ) = ( π‘Ž 𝑑 βˆ’ 𝑏 𝑐 ) ⃑ π‘˜ .

This leads to οƒ  𝐡 𝐴 Γ— ⃑ 𝐹 = ( 4 , 4 ) Γ— ( βˆ’ 4 , βˆ’ 3 ) = ( 4 Γ— ( βˆ’ 3 ) βˆ’ 4 Γ— ( βˆ’ 4 ) ) ⃑ π‘˜ = 4 ⃑ π‘˜ .

Thence, the moment of the termination of forces about point 𝐡 is 4 ⃑ π‘˜ .

Next, let United States find the distance of the perpendicular line 𝐿 connexion power point 𝐡 to the subsequent's furrow of action. This length 𝐿 is also titled the perpendicular distance between point 𝐡 and the resultant's line of action. To figure this length, we think back that the magnitude of the transmitter moment of a flattened force ⃑ 𝐹 about a detail is given by β€– β€– οƒŸ 𝑀 β€– β€– = β€– β€– ⃑ 𝐹 β€– β€– 𝐿 , where 𝐿 is the orthogonal outstrip 'tween the point in time and the line of action mechanism for ⃑ 𝐹 . We can rearrange this equation to write 𝐿 = β€– β€– οƒŸ 𝑀 β€– β€– β€– β€– ⃑ 𝐹 β€– β€– .

Since we know οƒŸ 𝑀 = 4 ⃑ π‘˜ , we can obtain β€– β€– οƒŸ 𝑀 β€– β€– = 4 . Lashkar-e-Tayyiba the States find β€– β€– ⃑ 𝐹 β€– β€– : β€– β€– ⃑ 𝐹 β€– β€– =  ( βˆ’ 4 ) + ( βˆ’ 3 ) = √ 2 5 = 5 .  

Substituting these values into the pattern for 𝐿 , we obtain 𝐿 = 4 5 = 0 . 8 .

Hence, οƒŸ 𝑀 = 4 ⃑ π‘˜ , 𝐿 = 0 . 8 . l e n g t h u n i t s

In the previous example, we found the moment of a system of planar forces acting at the same point about another point. We can note that the process of finding the moment for the system of forces is the comparable as that for one force, if the forces are acting at the same point.

Let us now consider the job of finding the second of a system of planar forces where the forces are not acting at the same point.

Definition: The Moment of a System of Planar Forces

Consider the system of forces ⃑ 𝐹  , ⃑ 𝐹  , … , and ⃑ 𝐹  acting at 𝐴  , 𝐴  , … , and 𝐴  respectively. To find the moment of this arrangement of forces about point 𝑂 , we need to find the moments οƒŸ 𝑀  , οƒŸ 𝑀  , … , and οƒŸ 𝑀  of forces ⃑ 𝐹  , ⃑ 𝐹  , … , and ⃑ 𝐹  about point 𝑂 . And then, the bit of the arrangement οƒŸ 𝑀 about point 𝑂 is given by οƒŸ 𝑀 = οƒŸ 𝑀 + οƒŸ 𝑀 + β‹― + οƒŸ 𝑀 .   

This definition tells US that the moment of a system of forces is equal to the sum of individual moments of each hale in the system approximately the same item.

In our final example, we will find the unknown constants in forces in a system impermanent at diametrical points when we are given the import of the system of forces about two different points.

Model 5: Finding Unknown Components of Cardinal Forces given the Sum of Their Moments virtually Two Points

⃑ 𝐹 = π‘š ⃑ 𝑖 + ⃑ 𝑗  and ⃑ 𝐹 = 𝑛 ⃑ 𝑖 βˆ’ 5 ⃑ 𝑗  , where ⃑ 𝐹  and ⃑ 𝐹  are two forces acting at the points 𝐴 ( 3 , 1 ) and 𝐡 ( βˆ’ 1 , βˆ’ 1 ) respectively. The sum of moments about the point of origin equals zero. The sum of the moments approximately the full point 𝐢 ( 1 , 2 ) also equals zero. Determine the values of π‘š and 𝑛 .

Answer

In that model, we need to find the unknown constants π‘š and 𝑛 in the forces ⃑ 𝐹  and ⃑ 𝐹  when we are given that the sum of the moments of the deuce forces about the pedigree and also about the point 𝐢 is zero. We can find the unknown constants past identifying a pair of simultaneous equations involving π‘š and 𝑛 . We bequeath receive the first equation by computing the sum of moments of ⃑ 𝐹  and ⃑ 𝐹  about the origin and setting them equal to zero.

Recall that the vector moment of force ⃑ 𝐹 acting at point 𝑃 about point 𝑄 is conferred by οƒŸ 𝑀 = ⃑ π‘Ÿ Γ— ⃑ 𝐹 , where ⃑ π‘Ÿ is the vector from point 𝑄 to point 𝑃 . Let United States of America forward find the moment of ⃑ 𝐹  about the origin. Since ⃑ 𝐹  Acts of the Apostles at point 𝐴 , we can write ⃑ π‘Ÿ = οƒ  𝑂 𝐴 = ( 3 , 1 ) .

We can spell ⃑ 𝐹  in component form equally ⃑ 𝐹 = π‘š ⃑ 𝑖 + ⃑ 𝑗 = ( π‘š , 1 ) . 

Now, we are ready to compute the track product οƒ  𝑂 𝐴 Γ— ⃑ 𝐹 . Return that the cross product of 2D vectors is formed aside ( π‘Ž , 𝑏 ) Γ— ( 𝑐 , 𝑑 ) = ( π‘Ž 𝑑 βˆ’ 𝑏 𝑐 ) ⃑ π‘˜ .

This leads to ⃑ π‘Ÿ Γ— ⃑ 𝐹 = ( 3 , 1 ) Γ— ( π‘š , 1 ) = ( 3 Γ— 1 βˆ’ 1 Γ— π‘š ) ⃑ π‘˜ = ( 3 βˆ’ π‘š ) ⃑ π‘˜ . 

Next, Army of the Pure U.S. find the moment of ⃑ 𝐹  about the origin. Since ⃑ 𝐹  acts at point 𝐡 , we can write ⃑ π‘Ÿ = οƒŸ 𝑂 𝐡 = ( βˆ’ 1 , βˆ’ 1 ) .

We can buoy write ⃑ 𝐹  in element organise as ⃑ 𝐹 = 𝑛 ⃑ 𝑖 βˆ’ 5 ⃑ 𝑗 = ( 𝑛 , βˆ’ 5 ) . 

Taking the cross product, ⃑ π‘Ÿ Γ— ⃑ 𝐹 = ( βˆ’ 1 , βˆ’ 1 ) Γ— ( 𝑛 , βˆ’ 5 ) = ( βˆ’ 1 Γ— ( βˆ’ 5 ) βˆ’ ( βˆ’ 1 ) Γ— 𝑛 ) ⃑ π‘˜ = ( 5 + 𝑛 ) ⃑ π‘˜ . 

Then, the sum of these two moments about the origin is ( 3 βˆ’ π‘š ) ⃑ π‘˜ + ( 5 + 𝑛 ) ⃑ π‘˜ = ( 8 βˆ’ π‘š + 𝑛 ) ⃑ π‘˜ .

Since we are given that the sum of these moments should equal zero, we get

This gives us indefinite equation involving π‘š and 𝑛 . We john repeat this computation for the time being about point 𝐢 to obtain other equation, but we can also find the second equation by using properties of the moments. Let US find the moment of ⃑ 𝐹  about channelis 𝐢 : ⃑ π‘Ÿ = οƒ  𝐢 𝐴 = ( 3 , 1 ) βˆ’ ( 1 , 2 ) = ( 2 , βˆ’ 1 ) .

Taking the cross product, ⃑ π‘Ÿ Γ— ⃑ 𝐹 = ( 2 , βˆ’ 1 ) Γ— ( π‘š , 1 ) = ( 2 Γ— 1 βˆ’ ( βˆ’ 1 ) Γ— π‘š ) ⃑ π‘˜ = ( 2 + π‘š ) ⃑ π‘˜ . 

Side by side, for the moment of ⃑ 𝐹  about 𝐢 , ⃑ π‘Ÿ = οƒŸ 𝐢 𝐡 = ( βˆ’ 1 , βˆ’ 1 ) βˆ’ ( 1 , 2 ) = ( βˆ’ 2 , βˆ’ 3 ) .

Taking the cross product, ⃑ π‘Ÿ Γ— ⃑ 𝐹 = ( βˆ’ 2 , βˆ’ 3 ) Γ— ( 𝑛 , βˆ’ 5 ) = ( βˆ’ 2 Γ— ( βˆ’ 5 ) βˆ’ ( βˆ’ 3 ) Γ— 𝑛 ) ⃑ π‘˜ = ( 1 0 + 3 𝑛 ) ⃑ π‘˜ . 

Summing these two moments about 𝐢 , ( 2 + π‘š ) ⃑ π‘˜ + ( 1 0 + 3 𝑛 ) ⃑ π‘˜ = ( 1 2 + π‘š + 3 𝑛 ) ⃑ π‘˜ .

Since we are inclined that the sum of these moments should equal nada, we prevail

Now that we have obtained ii equations for π‘š and 𝑛 , let United States of America write equations (1) and (2) present: 8 βˆ’ π‘š + 𝑛 = 0 , 1 2 + π‘š + 3 𝑛 = 0 .

We can nitty-gritt the ii equations to eliminate π‘š . This leads to 2 0 + 4 𝑛 = 0 .

Rearranging this equation then 𝑛 is the subject gives us 𝑛 = βˆ’ 5 . We can substitute this value into equality (1) to write out 8 βˆ’ π‘š βˆ’ 5 = 0 .

Rearranging this equivalence then π‘š is the subject leads to π‘š = 3 . Hence, we have π‘š = 3 , 𝑛 = βˆ’ 5 .

Army of the Righteou us finish by recapping a few critical concepts from this explainer.

Key Points

  • The transmitter moment of force ⃑ 𝐹 impermanent at point 𝐴 about point 𝑂 is given past οƒŸ 𝑀 = ⃑ π‘Ÿ Γ— ⃑ 𝐹 , where ⃑ π‘Ÿ is the vector from manoeuver 𝑂 to spot 𝐴 .
  • The magnitude of the vector moment of a placoid force ⃑ 𝐹 about a signal is given by β€– β€– οƒŸ 𝑀 β€– β€– = β€– β€– ⃑ 𝐹 β€– β€– 𝑑 , βŸ‚ where 𝑑 βŸ‚ is the perpendicular distance between the luff and the line of action of force ⃑ 𝐹 .
  • The vector moment οƒŸ 𝑀 of a force about a point is independent of the initial point, every bit long as the point lies in the same line of execute.
  • Rent out 𝑀 and οƒŸ 𝑀 be the scalar and transmitter moments of a force-out, or a system of forces, on a plane about a breaker point. Then, οƒŸ 𝑀 = 𝑀 ⃑ π‘˜ .
  • The computation of the cross product ⃑ π‘Ÿ Γ— ⃑ 𝐹 to reckon the moment οƒŸ 𝑀 of a planar force about a point can constitute simplified by exploitation the 2D vector product, which is outlined aside ( π‘Ž , 𝑏 ) Γ— ( 𝑐 , 𝑑 ) = ( π‘Ž 𝑑 βˆ’ 𝑏 𝑐 ) ⃑ π‘˜ .
  • Consider the system of forces ⃑ 𝐹  , ⃑ 𝐹  , … , and ⃑ 𝐹  performing at 𝐴  , 𝐴  , … , and 𝐴  respectively. To find the moment of this system of forces nigh point 𝑂 , we need to get the moments οƒŸ 𝑀  , οƒŸ 𝑀  , … , and οƒŸ 𝑀  of forces ⃑ 𝐹  , ⃑ 𝐹  , … , and ⃑ 𝐹  about point 𝑂 . Then, the moment of system οƒŸ 𝑀 most point 𝑂 is given by οƒŸ 𝑀 = οƒŸ 𝑀 + οƒŸ 𝑀 + β‹― + οƒŸ 𝑀 .   

In the Case Shown in (Figure 1), Specify the Distance Where the Resultant Force Acts From Point O.

Source: https://www.nagwa.com/en/explainers/653128293684/

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