#set document(title: "9.3 Conservation of Linear Momentum", author: "OpenStax / XYZ Homework") #set page(width: 8.5in, height: auto, margin: 1in) #import "@preview/cetz:0.5.2" #set text(font: ("STIX Two Text", "Libertinus Serif", "New Computer Modern"), size: 10.5pt, lang: "en") #show math.equation: set text(font: ("STIX Two Math", "New Computer Modern Math")) #set par(justify: true, leading: 0.62em, spacing: 0.9em) #set enum(spacing: 1.1em) // room between list items so tall inline fractions don't collide #set list(spacing: 1.1em) #set table(stroke: 0.5pt + rgb("#c7ccd3")) #let BLUE = rgb("#183B6F") // brand navy — section bars + example/solution labels (white on navy 11.09:1) #let ORANGE = rgb("#A94509") // brand primary-700 — AA-safe deep orange for TEXT (5.93:1 on white; raw brand #F37021 is 2.94:1 and must never carry text) #let RED = rgb("#DC2626") // brand error-600 #let GREEN = rgb("#059669") // brand success-600 (decoration only; small green text uses green-text #007942) #show heading.where(level: 1): it => block(width: 100%, above: 0pt, below: 16pt, fill: gradient.linear(BLUE, rgb("#2C5AA0")), inset: (x: 14pt, y: 12pt), radius: 3pt, text(fill: white, weight: "bold", size: 19pt, it.body)) #show heading.where(level: 2): it => block(width: 100%, above: 18pt, below: 10pt, fill: BLUE, inset: (x: 10pt, y: 6pt), radius: 2pt, text(fill: white, weight: "bold", size: 12pt, it.body)) #show heading.where(level: 3): it => text(fill: ORANGE, weight: "bold", size: 12.5pt, it.body) #show heading.where(level: 4): it => text(fill: BLUE, weight: "bold", size: 10.5pt, it.body) #let examplebox(label, title, body) = block(width: 100%, breakable: true, fill: rgb("#EFF1F5"), stroke: 0.5pt + rgb("#CFDDF0"), radius: 4pt, inset: 10pt, above: 12pt, below: 12pt)[ #block(below: 6pt)[#box(fill: BLUE, inset: (x: 6pt, y: 2pt), radius: 2pt, text(fill: white, weight: "bold", size: 8.5pt, label)) #h(0.4em) #strong[#title]] #body] // rail = decorative left rule (raw brand token); labelcolor = AA-safe label text shade #let notebox(label, rail, labelcolor, tint, body) = block(width: 100%, breakable: true, fill: tint, stroke: (left: 3pt + rail), inset: (left: 10pt, rest: 8pt), radius: (right: 4pt), above: 11pt, below: 11pt)[ #text(fill: labelcolor, weight: "bold", size: 7.5pt, tracking: 0.5pt)[#upper(label)] #linebreak() #body] #let solutionbox(body) = block(above: 4pt, below: 8pt)[ #text(fill: BLUE, weight: "bold", size: 8.5pt)[Solution] #linebreak() #body] #let figph(msg) = block(width: 100%, height: 60pt, fill: rgb("#f6f7f9"), stroke: (paint: rgb("#c7ccd3"), dash: "dashed"), radius: 4pt, inset: 10pt)[ #align(center + horizon, text(fill: rgb("#889"), style: "italic", size: 9pt, msg))] // Standardize inlined figure sizes: measure the natural CeTZ canvas, then scale to a // consistent envelope (aspect-aware; see build_typst.py FIG_* constants). Unlike the // print preamble, dimensions are FLOORED: in an editor a user can trim a figure to a // degenerate 1-D shape (a bare line), and w/h or tw/w would then divide by zero. #let _STD_W = 3.5 #let _WIDE_W = 5.6 #let _MAX_H = 3.4 #let _ASPECT_WIDE = 2.2 #let _UPSCALE_MAX = 1.15 #let stdfig(body) = context { let m = measure(body) let w = calc.max(m.width / 1in, 0.01) let h = calc.max(m.height / 1in, 0.01) let tw = if w / h > _ASPECT_WIDE { _WIDE_W } else { _STD_W } let s = calc.min(tw / w, _MAX_H / h, _UPSCALE_MAX) align(center, box(scale(x: s * 100%, y: s * 100%, reflow: true, body))) } #show figure: set block(breakable: false) #set figure(gap: 8pt) #show figure.caption: set text(size: 8.5pt, fill: rgb("#555")) == 9.3#h(0.6em)Conservation of Linear Momentum Recall Newton’s third law: When two objects of masses #math.equation(block: false, alt: "m sub 1")[$m_(1)$] and #math.equation(block: false, alt: "m sub 2")[$m_(2)$] interact (meaning that they apply forces on each other), the force that object 2 applies to object 1 is equal in magnitude and opposite in direction to the force that object 1 applies on object 2. Let: - #math.equation(block: false, alt: "F → sub 21 equals")[$arrow(F)_(21) =$] the force on #math.equation(block: false, alt: "m sub 1")[$m_(1)$] from #math.equation(block: false, alt: "m sub 2")[$m_(2)$] - #math.equation(block: false, alt: "F → sub 12 equals")[$arrow(F)_(12) =$] the force on #math.equation(block: false, alt: "m sub 2")[$m_(2)$] from #math.equation(block: false, alt: "m sub 1")[$m_(1)$] Then, in symbols, Newton’s third law says #math.equation(block: true, alt: "F → sub 21, equals, − F → sub 12; m sub 1 a → sub 1, equals, − m sub 2 a → sub 2 .")[$arrow(F)_(21) & = & "−" arrow(F)_(12) \ m_(1) arrow(a)_(1) & = & "−" m_(2) arrow(a)_(2) .$] (Recall that these two forces do not cancel because they are applied to different objects. #math.equation(block: false, alt: "F sub 21")[$F_(21)$] causes #math.equation(block: false, alt: "m sub 1")[$m_(1)$] to accelerate, and #math.equation(block: false, alt: "F sub 12")[$F_(12)$] causes #math.equation(block: false, alt: "m sub 2")[$m_(2)$] to accelerate.) Although the magnitudes of the forces on the objects are the same, the accelerations are not, simply because the masses (in general) are different. Therefore, the changes in velocity of each object are different: #math.equation(block: true, alt: "the fraction d v → sub 1 over d t not equal to the fraction d v → sub 2 over d t .")[$frac(d arrow(v)_(1), d t) ≠ frac(d arrow(v)_(2), d t) .$] However, the products of the mass and the change of velocity #emph[are] equal (in magnitude): #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ #math.equation(block: true, alt: "m sub 1 the fraction d v → sub 1 over d t equals − m sub 2 the fraction d v → sub 2 over d t .")[$m_(1) frac(d arrow(v)_(1), d t) = "−" m_(2) frac(d arrow(v)_(2), d t) .$] ] It’s a good idea, at this point, to make sure you’re clear on the physical meaning of the derivatives in . Because of the interaction, each object ends up getting its velocity changed, by an amount #emph[dv]. Furthermore, the interaction occurs over a time interval #emph[dt], which means that the change of velocities also occurs over #emph[dt]. This time interval is the same for each object. Let‘s assume, for the moment, that the masses of the objects do not change during the interaction. (We’ll relax this restriction later.) In that case, we can pull the masses inside the derivatives: #math.equation(block: true, alt: "the fraction d over d t open parenthesis m sub 1 v → sub 1 close parenthesis equals minus the fraction d over d t open parenthesis m sub 2 v → sub 2 close parenthesis")[$frac(d, d t) ( m_(1) arrow(v)_(1) ) = − frac(d, d t) ( m_(2) arrow(v)_(2) )$] and thus #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ #math.equation(block: true, alt: "the fraction d p → sub 1 over d t equals minus the fraction d p → sub 2 over d t .")[$frac(d arrow(p)_(1), d t) = − frac(d arrow(p)_(2), d t) .$] ] This says that #emph[the rate at which momentum changes is the same for both objects.] The masses are different, and the changes of velocity are different, but the rate of change of the product of #emph[m] and #strong[#math.equation(block: false, alt: "v →")[$arrow(v)$]] are the same. Physically, this means that during the interaction of the two objects (#math.equation(block: false, alt: "m sub 1 and m sub 2")[$m_(1) #h(0.2em) "and" #h(0.2em) m_(2)$]), both objects have their momentum changed; but those changes are identical in magnitude, though opposite in sign. For example, the momentum of object 1 might increase, which means that the momentum of object 2 decreases by exactly the same amount. In light of this, let’s re-write in a more suggestive form: #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ #math.equation(block: true, alt: "the fraction d p → sub 1 over d t plus the fraction d p → sub 2 over d t equals 0 .")[$frac(d arrow(p)_(1), d t) + frac(d arrow(p)_(2), d t) = 0 .$] ] This says that during the interaction, although object 1’s momentum changes, and object 2’s momentum also changes, these two changes cancel each other out, so that the total change of momentum of the two objects together is zero. Since the total combined momentum of the two objects together never changes, then we could write #math.equation(block: true, alt: "the fraction d over d t open parenthesis p → sub 1 plus p → sub 2 close parenthesis equals 0")[$frac(d, d t) ( arrow(p)_(1) + arrow(p)_(2) ) = 0$] from which it follows that #math.equation(block: true, alt: "p → sub 1 plus p → sub 2 equals constant .")[$arrow(p)_(1) + arrow(p)_(2) = "constant" .$] As shown in , the total momentum of the system before and after the collision remains the same. #figure(figph[Before collision yellow ball1 is moving down and to the right, aiming at the center of blue ball 2. Blue ball 2 is moving to the left and slightly down, and more slowly than ball 1. We are told that p total vector equals p 1 vector plus p 2 vector and we are shown the sum as a vector diagram: p 1 and p 2 are placed with the tail of p 2 at the head of p 1. A vector is drawn from the tail of p 1 to the head of p 2. After the collision, the yellow ball is moving slowly to the right and p 2 is moving more rapidly down and to the left. We are told that p prime total vector equals p prime 1 vector plus p prime 2 vector and we are shown the sum as a vector diagram: p prime 1 and p prime 2 are placed with the tail of p prime 2 at the head of p prime 1. A vector is drawn from the tail of p prime 1 to the head of p prime 2 and is the same length and in the same direction as the sum vector before collision.], alt: "Before collision yellow ball1 is moving down and to the right, aiming at the center of blue ball 2. Blue ball 2 is moving to the left and slightly down, and more slowly than ball 1. We are told that p total vector equals p 1 vector plus p 2 vector and we are shown the sum as a vector diagram: p 1 and p 2 are placed with the tail of p 2 at the head of p 1. A vector is drawn from the tail of p 1 to the head of p 2. After the collision, the yellow ball is moving slowly to the right and p 2 is moving more rapidly down and to the left. We are told that p prime total vector equals p prime 1 vector plus p prime 2 vector and we are shown the sum as a vector diagram: p prime 1 and p prime 2 are placed with the tail of p prime 2 at the head of p prime 1. A vector is drawn from the tail of p prime 1 to the head of p prime 2 and is the same length and in the same direction as the sum vector before collision.", caption: [Before the collision, the two billiard balls travel with momenta #math.equation(block: false, alt: "p → sub 1")[$arrow(p)_(1)$] and #math.equation(block: false, alt: "p → sub 2")[$arrow(p)_(2)$]. The total momentum of the system is the sum of these, as shown by the red vector labeled #math.equation(block: false, alt: "p → sub total")[$arrow(p)_("total")$] on the left. After the collision, the two billiard balls travel with different momenta #math.equation(block: false, alt: "p → prime sub 1")[$arrow(p)^(′)_(1)$] and #math.equation(block: false, alt: "p → prime sub 2")[$arrow(p)^(′)_(2)$]. The total momentum, however, has not changed, as shown by the red vector arrow #math.equation(block: false, alt: "p → prime sub total")[$arrow(p)^(′)_("total")$] on the right.]) Generalizing this result to #emph[N] objects, we obtain #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ #math.equation(block: true, alt: "p → sub 1 plus p → sub 2 plus p → sub 3 plus ⋯ plus p → sub N, equals, constant; ∑ j equals 1 N p → sub j, equals, constant.")[$arrow(p)_(1) + arrow(p)_(2) + arrow(p)_(3) + ⋯ + arrow(p)_(N) & = & "constant" \ display(limits(∑)^(N)_(j = 1) arrow(p)_(j)) & = & "constant."$] ] is the definition of the total (or net) momentum of a system of #emph[N] interacting objects, along with the statement that the total momentum of a system of objects is constant in time—or better, is conserved. #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ #emph[Conservation Laws] If the value of a physical quantity is constant in time, we say that the quantity is conserved. ] === Requirements for Momentum Conservation There is a complication, however. A system must meet two requirements for its momentum to be conserved: + #emph[The mass of the system must remain constant during the interaction.] #linebreak() As the objects interact (apply forces on each other), they may #emph[transfer] mass from one to another; but any mass one object gains is balanced by the loss of that mass from another. The total mass of the system of objects, therefore, remains unchanged as time passes: #math.equation(block: true, alt: "[ the fraction d m over d t ] sub system equals 0 .")[$attach([ frac(d m, d t) ], b: "system") = 0 .$] + #emph[The net external force on the system must be zero.] #linebreak() As the objects collide, or explode, and move around, they exert forces on each other. However, all of these forces are internal to the system, and thus each of these internal forces is balanced by another internal force that is equal in magnitude and opposite in sign. As a result, the change in momentum caused by each internal force is cancelled by another momentum change that is equal in magnitude and opposite in direction. Therefore, internal forces cannot change the total momentum of a system because the changes sum to zero. However, if there is some external force that acts on all of the objects (gravity, for example, or friction), then this force changes the momentum of the system as a whole; that is to say, the momentum of the system is changed by the external force. Thus, for the momentum of the system to be conserved, we must have #math.equation(block: true, alt: "F → sub e x t equals 0 → .")[$arrow(F)_(e x t) = arrow(0) .$] A system of objects that meets these two requirements is said to be a #strong[closed system] (also called an isolated system). Thus, the more compact way to express this is shown below. #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ #emph[Law of Conservation of Momentum] The total momentum of a closed system is conserved: #math.equation(block: true, alt: "∑ j equals 1 N p → sub j equals constant.")[$display(limits(∑)^(N)_(j = 1) arrow(p)_(j)) = "constant."$] ] This statement is called the #strong[Law of Conservation of Momentum]. Along with the conservation of energy, it is one of the foundations upon which all of physics stands. All our experimental evidence supports this statement: from the motions of galactic clusters to the quarks that make up the proton and the neutron, and at every scale in between. #emph[In a closed system, the total momentum never changes.] Note that there absolutely #emph[can] be external forces acting on the system; but for the system’s momentum to remain constant, these external forces have to cancel, so that the #emph[net] external force is zero. Billiard balls on a table all have a weight force acting on them, but the weights are balanced (canceled) by the normal forces, so there is no #emph[net] force. === The Meaning of ‘System’ A #strong[system] (mechanical) is the collection of objects in whose motion (kinematics and dynamics) you are interested. If you are analyzing the bounce of a ball on the ground, you are probably only interested in the motion of the ball, and not of Earth; thus, the ball is your system. If you are analyzing a car crash, the two cars together compose your system . #figure(figph[Illustration of collision of two cars with masses m 1 and m 2. The system of interest is the two cars before and after the collision. Before the collision, car m 2 is in front and moving forward with velocity v 2, and car m 1 is behind it, moving forward with velocity v 1. Net vector F = 0 and vectors p 1 plus p 2 equal p tot. After the collision, car m 2 is in front and moving forward with velocity v 2 prime which is larger than v 2 before the collision, and car m 1 is behind it, moving forward with velocity v 1 prime that is less than v 1 before the collision. Vectors p 1 prime plus p 2 prime equal p tot prime.], alt: "Illustration of collision of two cars with masses m 1 and m 2. The system of interest is the two cars before and after the collision. Before the collision, car m 2 is in front and moving forward with velocity v 2, and car m 1 is behind it, moving forward with velocity v 1. Net vector F = 0 and vectors p 1 plus p 2 equal p tot. After the collision, car m 2 is in front and moving forward with velocity v 2 prime which is larger than v 2 before the collision, and car m 1 is behind it, moving forward with velocity v 1 prime that is less than v 1 before the collision. Vectors p 1 prime plus p 2 prime equal p tot prime.", caption: [The two cars together form the system that is to be analyzed. It is important to remember that the contents (the mass) of the system do not change before, during, or after the objects in the system interact.]) #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ #emph[Conservation of Momentum] Using conservation of momentum requires four basic steps. The first step is crucial: + Identify a closed system (total mass is constant, no net external force acts on the system). + Write down an expression representing the total momentum of the system before the “event” (explosion or collision). + Write down an expression representing the total momentum of the system after the “event.” + Set these two expressions equal to each other, and solve this equation for the desired quantity. ] #examplebox("Example 1")[Colliding Carts][ Two carts in a physics lab roll on a level track, with negligible friction. These carts have small magnets at their ends, so that when they collide, they stick together . The first cart has a mass of 675 grams and is rolling at 0.75 m/s to the right; the second has a mass of 500 grams and is rolling at 1.33 m/s, also to the right. After the collision, what is the velocity of the two joined carts? #figure(figph[An illustration of two lab carts on a track, stuck together.], alt: "An illustration of two lab carts on a track, stuck together.", caption: [Two lab carts collide and stick together after the collision.]) Strategy We have a collision. We’re given masses and initial velocities; we’re asked for the final velocity. This all suggests using conservation of momentum as a method of solution. However, we can only use it if we have a closed system. So we need to be sure that the system we choose has no net external force on it, and that its mass is not changed by the collision. Defining the system to be the two carts meets the requirements for a closed system: The combined mass of the two carts certainly doesn’t change, and while the carts definitely exert forces on each other, those forces are internal to the system, so they do not change the momentum of the system as a whole. In the vertical direction, the weights of the carts are canceled by the normal forces on the carts from the track. Solution Conservation of momentum is #math.equation(block: true, alt: "p → sub f equals p → sub i .")[$arrow(p)_(f) = arrow(p)_(i) .$] Define the direction of their initial velocity vectors to be the +#emph[x]-direction. The initial momentum is then #math.equation(block: true, alt: "p → sub i equals m sub 1 v sub 1 i ^ plus m sub 2 v sub 2 i ^ .")[$arrow(p)_(i) = m_(1) v_(1) hat(i) + m_(2) v_(2) hat(i) .$] The final momentum of the now-linked carts is #math.equation(block: true, alt: "p → sub f equals open parenthesis m sub 1 plus m sub 2 close parenthesis v → sub f .")[$arrow(p)_(f) = ( m_(1) + m_(2) ) arrow(v)_(f) .$] Equating: #math.equation(block: true, alt: "open parenthesis m sub 1 plus m sub 2 close parenthesis v → sub f, equals, m sub 1 v sub 1 i ^ plus m sub 2 v sub 2 i ^; v → sub f, equals, open parenthesis the fraction m sub 1 v sub 1 plus m sub 2 v sub 2 over m sub 1 plus m sub 2 close parenthesis i ^ .")[$( m_(1) + m_(2) ) arrow(v)_(f) & = & m_(1) v_(1) hat(i) + m_(2) v_(2) hat(i) \ arrow(v)_(f) & = & ( frac(m_(1) v_(1) + m_(2) v_(2), m_(1) + m_(2)) ) hat(i) .$] Substituting the given numbers: #math.equation(block: true, alt: "v → sub f, equals [ the fraction open parenthesis 0.675 kg close parenthesis open parenthesis 0.75 m/s close parenthesis plus open parenthesis 0.5 kg close parenthesis open parenthesis 1.33 m/s close parenthesis over 1.175 kg ] i ^; equals open parenthesis 0.997 m/s close parenthesis i ^ .")[$arrow(v)_(f) & = [ frac(( 0.675 #h(0.2em) "kg" ) ( 0.75 #h(0.2em) "m/s" ) + ( 0.5 #h(0.2em) "kg" ) ( 1.33 #h(0.2em) "m/s" ), 1.175 #h(0.2em) "kg") ] hat(i) \ & = ( 0.997 #h(0.2em) "m/s" ) hat(i) .$] Significance The principles that apply here to two laboratory carts apply identically to all objects of whatever type or size. Even for photons, the concepts of momentum and conservation of momentum are still crucially important even at that scale. (Since they are massless, the momentum of a photon is defined very differently from the momentum of ordinary objects. You will learn about this when you study quantum physics.) ] #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ Suppose the second, smaller cart had been initially moving to the left. What would the sign of the final velocity have been in this case? #solutionbox[ If the smaller cart were rolling at 1.33 m/s to the left, then conservation of momentum gives #linebreak() #math.equation(block: false, alt: "open parenthesis m sub 1 plus m sub 2 close parenthesis v → sub f, equals, m sub 1 v sub 1 i ^ minus m sub 2 v sub 2 i ^; v → sub f, equals, open parenthesis the fraction m sub 1 v sub 1 minus m sub 2 v sub 2 over m sub 1 plus m sub 2 close parenthesis i ^; equals, [ the fraction open parenthesis 0.675 kg close parenthesis open parenthesis 0.75 m/s close parenthesis minus open parenthesis 0.500 kg close parenthesis open parenthesis 1.33 m/s close parenthesis over 1.175 kg ] i ^; equals, − open parenthesis 0.135 m/s close parenthesis i ^")[$( m_(1) + m_(2) ) arrow(v)_(f) & = & m_(1) v_(1) hat(i) − m_(2) v_(2) hat(i) \ arrow(v)_(f) & = & ( frac(m_(1) v_(1) − m_(2) v_(2), m_(1) + m_(2)) ) hat(i) \ & = & [ frac(( 0.675 #h(0.2em) "kg" ) ( 0.75 #h(0.2em) "m/s" ) − ( 0.500 #h(0.2em) "kg" ) ( 1.33 #h(0.2em) "m/s" ), 1.175 #h(0.2em) "kg") ] hat(i) \ & = & "−" ( 0.135 #h(0.2em) "m/s" ) hat(i)$] #linebreak() Thus, the final velocity is 0.135 m/s to the left. ] ] #examplebox("Example 2")[A Bouncing Superball][ A superball of mass 0.25 kg is dropped from rest from a height of #math.equation(block: false, alt: "h equals 1.50 m")[$h = 1.50 #h(0.2em) "m"$] above the floor. It bounces with no loss of energy and returns to its initial height . + What is the superball’s change of momentum during its bounce on the floor? + What was Earth’s change of momentum due to the ball colliding with the floor? + What was Earth’s change of velocity as a result of this collision? (This example shows that you have to be careful about defining your system.) #figure(figph[A ball is shown at four different times. At t sub 0 the ball is at a distance h above the floor and has p sub 0 equals 0. At t sub 1 the ball is near the floor. A downward arrow at the ball is labeled minus p sub 1. At t sub 2 the ball is near the floor. An upward arrow at the ball is labeled plus p sub 2. The p sub 1 and p sub 2 arrows are the same length. At t sub 3 the ball at height h again and p sub 3 equals zero.], alt: "A ball is shown at four different times. At t sub 0 the ball is at a distance h above the floor and has p sub 0 equals 0. At t sub 1 the ball is near the floor. A downward arrow at the ball is labeled minus p sub 1. At t sub 2 the ball is near the floor. An upward arrow at the ball is labeled plus p sub 2. The p sub 1 and p sub 2 arrows are the same length. At t sub 3 the ball at height h again and p sub 3 equals zero.", caption: [A superball is dropped to the floor (#math.equation(block: false, alt: "t sub 0")[$t_(0)$]), hits the floor (#math.equation(block: false, alt: "t sub 1")[$t_(1)$]), bounces (#math.equation(block: false, alt: "t sub 2")[$t_(2)$]), and returns to its initial height (#math.equation(block: false, alt: "t sub 3")[$t_(3)$]).]) Strategy Since we are asked only about the ball’s change of momentum, we define our system to be the ball. But this is clearly not a closed system; gravity applies a downward force on the ball while it is falling, and the normal force from the floor applies a force during the bounce. Thus, we cannot use conservation of momentum as a strategy. Instead, we simply determine the ball’s momentum just before it collides with the floor and just after, and calculate the difference. We have the ball’s mass, so we need its velocities. Solution + Since this is a one-dimensional problem, we use the scalar form of the equations. Let: #linebreak() - #math.equation(block: false, alt: "p sub 0 equals")[$p_(0) =$] the magnitude of the ball’s momentum at time #math.equation(block: false, alt: "t sub 0")[$t_(0)$], the moment it was released; since it was dropped from rest, this is zero. - #math.equation(block: false, alt: "p sub 1 equals")[$p_(1) =$] the magnitude of the ball’s momentum at time #math.equation(block: false, alt: "t sub 1")[$t_(1)$], the instant just before it hits the floor. - #math.equation(block: false, alt: "p sub 2 equals")[$p_(2) =$] the magnitude of the ball’s momentum at time #math.equation(block: false, alt: "t sub 2")[$t_(2)$], just after it loses contact with the floor after the bounce. #linebreak() The ball’s change of momentum is #math.equation(block: true, alt: "Δ p →, equals p → sub 2 minus p → sub 1; equals p sub 2 j ^ minus open parenthesis − p sub 1 j ^ close parenthesis; equals open parenthesis p sub 2 plus p sub 1 close parenthesis j ^ .")[$"Δ" arrow(p) & = arrow(p)_(2) − arrow(p)_(1) \ & = p_(2) hat(j) − ( "−" p_(1) hat(j) ) \ & = ( p_(2) + p_(1) ) hat(j) .$] Its velocity just before it hits the floor can be determined from either conservation of energy or kinematics. We use kinematics here; you should re-solve it using conservation of energy and confirm you get the same result. #linebreak() We want the velocity just before it hits the ground (at time #math.equation(block: false, alt: "t sub 1")[$t_(1)$]). We know its initial velocity #math.equation(block: false, alt: "v sub 0 equals 0")[$v_(0) = 0$] (at time #math.equation(block: false, alt: "t sub 0")[$t_(0)$]), the height it falls, and its acceleration; we don’t know the fall time. We could calculate that, but instead we use #math.equation(block: true, alt: "v → sub 1 equals − j ^ the square root of 2 g y equals −5.4 m/s j ^ .")[$arrow(v)_(1) = "−" hat(j) sqrt(2 g y) = −5.4 #h(0.2em) "m/s" hat(j) .$] Thus the ball has a momentum of #math.equation(block: true, alt: "p → sub 1, equals − open parenthesis 0.25 kg close parenthesis open parenthesis −5.4 m/s j ^ close parenthesis; equals − open parenthesis 1.4 kg times m/s close parenthesis j ^ .")[$arrow(p)_(1) & = "−" ( 0.25 #h(0.2em) "kg" ) ( −5.4 #h(0.2em) "m/s" hat(j) ) \ & = "−" ( 1.4 #h(0.2em) "kg" · "m/s" ) hat(j) .$] We don’t have an easy way to calculate the momentum after the bounce. Instead, we reason from the symmetry of the situation. #linebreak() Before the bounce, the ball starts with zero velocity and falls 1.50 m under the influence of gravity, achieving some amount of momentum just before it hits the ground. On the return trip (after the bounce), it starts with some amount of momentum, rises the same 1.50 m it fell, and ends with zero velocity. Thus, the motion after the bounce was the mirror image of the motion before the bounce. From this symmetry, it must be true that the ball’s momentum after the bounce must be equal and opposite to its momentum before the bounce. (This is a subtle but crucial argument; make sure you understand it before you go on.) #linebreak() Therefore, #math.equation(block: true, alt: "p → sub 2 equals − p → sub 1 equals plus open parenthesis 1.4 kg times m/s close parenthesis j ^ .")[$arrow(p)_(2) = "−" arrow(p)_(1) = + ( 1.4 #h(0.2em) "kg" · "m/s" ) hat(j) .$] Thus, the ball’s change of momentum during the bounce is #linebreak() #math.equation(block: true, alt: "Δ p →, equals p → sub 2 minus p → sub 1; equals open parenthesis 1.4 kg times m/s close parenthesis j ^ minus open parenthesis −1.4 kg times m/s close parenthesis j ^; equals plus open parenthesis 2.8 kg times m/s close parenthesis j ^ .")[$"Δ" arrow(p) & = arrow(p)_(2) − arrow(p)_(1) \ & = ( 1.4 #h(0.2em) "kg" · "m/s" ) hat(j) − ( −1.4 #h(0.2em) "kg" · "m/s" ) hat(j) \ & = + ( 2.8 #h(0.2em) "kg" · "m/s" ) hat(j) .$] + What was Earth’s change of momentum due to the ball colliding with the floor? #linebreak() Your instinctive response may well have been either “zero; the Earth is just too massive for that tiny ball to have affected it” or possibly, “more than zero, but utterly negligible.” But no—if we re-define our system to be the Superball + Earth, then this system is closed (neglecting the gravitational pulls of the Sun, the Moon, and the other planets in the solar system), and therefore the total change of momentum of this new system must be zero. Therefore, Earth’s change of momentum is exactly the same magnitude: #math.equation(block: true, alt: "Δ p → sub Earth equals −2.8 kg times m/s j ^ .")[$"Δ" arrow(p)_("Earth") = −2.8 #h(0.2em) "kg" · "m/s" hat(j) .$] + What was Earth’s change of velocity as a result of this collision? #linebreak() This is where your instinctive feeling is probably correct: #math.equation(block: true, alt: "Δ v → sub Earth, equals the fraction Δ p → sub Earth over M sub Earth; equals minus the fraction 2.8 kg times m/s over 5 . 97 times 10 to the power 24 kg j ^; equals − open parenthesis 4.7 times 10 to the power −25 m/s close parenthesis j ^ .")[$"Δ" arrow(v)_("Earth") & = frac("Δ" arrow(p)_("Earth"), M_("Earth")) \ & = − frac(2.8 #h(0.2em) "kg" · "m/s", 5 . 97 #h(0.2em) × #h(0.2em) 10^(24) #h(0.2em) "kg") hat(j) \ & = "−" ( 4.7 #h(0.2em) × #h(0.2em) 10^(−25) #h(0.2em) "m/s" ) hat(j) .$] This change of Earth’s velocity #emph[is] utterly negligible. Significance It is important to realize that the answer to part (c) is not a velocity; it is a change of velocity, which is a very different thing. Nevertheless, to give you a feel for just how small that change of velocity is, suppose you were moving with a velocity of #math.equation(block: false, alt: "4.7 times 10 to the power −25 m/s")[$4.7 #h(0.2em) × #h(0.2em) 10^(−25) #h(0.2em) "m/s"$]. At this speed, it would take you about 7 million years to travel a distance equal to the diameter of a hydrogen atom. ] #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ Would the ball’s change of momentum have been larger, smaller, or the same, if it had collided with the floor and stopped (without bouncing)? #solutionbox[ If the ball does not bounce, its final momentum #math.equation(block: false, alt: "p → sub 2")[$arrow(p)_(2)$] is zero, so #linebreak() #math.equation(block: false, alt: "Δ p →, equals p → sub 2 minus p → sub 1; equals open parenthesis 0 close parenthesis j ^ minus open parenthesis −1.4 kg times m/s close parenthesis j ^; equals plus open parenthesis 1.4 kg times m/s close parenthesis j ^")[$"Δ" arrow(p) & = arrow(p)_(2) − arrow(p)_(1) \ & = ( 0 ) hat(j) − ( −1.4 #h(0.2em) "kg" · "m/s" ) hat(j) \ & = + ( 1.4 #h(0.2em) "kg" · "m/s" ) hat(j)$] ] ] #examplebox("Example 3")[Ice Hockey 1][ Two hockey pucks of identical mass are on a flat, horizontal ice hockey rink. The red puck is motionless; the blue puck is moving at 2.5 m/s to the left . It collides with the motionless red puck. The pucks have a mass of 15 g. After the collision, the red puck is moving at 2.5 m/s, to the left. What is the final velocity of the blue puck? #figure(figph[Two hockey pucks are shown. The top diagram shows the puck on the left with 0 meters per second and the puck on the right moving to the left with 2.5 meters per second. The bottom diagram shows the puck on the left moving to the left at 2.5 meters per second and the puck on the right moving with unknown v.], alt: "Two hockey pucks are shown. The top diagram shows the puck on the left with 0 meters per second and the puck on the right moving to the left with 2.5 meters per second. The bottom diagram shows the puck on the left moving to the left at 2.5 meters per second and the puck on the right moving with unknown v.", caption: [Two identical hockey pucks colliding. The top diagram shows the pucks the instant before the collision, and the bottom diagram show the pucks the instant after the collision. The net external force is zero.]) Strategy We’re told that we have two colliding objects, we’re told the masses and initial velocities, and one final velocity; we’re asked for both final velocities. Conservation of momentum seems like a good strategy. Define the system to be the two pucks; there’s no friction, so we have a closed system. Before you look at the solution, what do you think the answer will be? The blue puck final velocity will be: - zero - 2.5 m/s to the left - 2.5 m/s to the right - 1.25 m/s to the left - 1.25 m/s to the right - something else Solution Define the +#emph[x]-direction to point to the right. Conservation of momentum then reads #math.equation(block: true, alt: "p → sub f, equals, p → sub i; m v sub r sub f i ^ plus m v sub b sub f i ^, equals, m v sub r sub i i ^ minus m v sub b sub i i ^ .")[$arrow(p)_(f) & = & arrow(p)_(i) \ m v_("r"_("f")) hat(i) + m v_("b"_("f")) hat(i) & = & m v_("r"_("i")) hat(i) − m v_("b"_("i")) hat(i) .$] Before the collision, the momentum of the system is entirely and only in the blue puck. Thus, #math.equation(block: true, alt: "m v sub r sub f i ^ plus m v sub b sub f i ^, equals, − m v sub b sub i i ^; v sub r sub f i ^ plus v sub b sub f i ^, equals, − v sub b sub i i ^ .")[$m v_("r"_("f")) hat(i) + m v_("b"_("f")) hat(i) & = & "−" m v_("b"_("i")) hat(i) \ v_("r"_("f")) hat(i) + v_("b"_("f")) hat(i) & = & "−" v_("b"_("i")) hat(i) .$] (Remember that the masses of the pucks are equal.) Substituting numbers: #math.equation(block: true, alt: "minus open parenthesis 2.5 m/s close parenthesis i ^ plus v → sub b sub f, equals, − open parenthesis 2.5 m/s close parenthesis i ^; v → sub b sub f, equals, 0 .")[$− ( 2.5 #h(0.2em) "m/s" ) hat(i) + arrow(v)_("b"_("f")) & = & "−" ( 2.5 #h(0.2em) "m/s" ) hat(i) \ arrow(v)_("b"_("f")) & = & 0 .$] Significance Evidently, the two pucks simply exchanged momentum. The blue puck transferred all of its momentum to the red puck. In fact, this is what happens in similar collision where #math.equation(block: false, alt: "m sub 1 equals m sub 2 .")[$m_(1) = m_(2) .$] ] #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ Even if there were some friction on the ice, it is still possible to use conservation of momentum to solve this problem, but you would need to impose an additional condition on the problem. What is that additional condition? #solutionbox[ Consider the impulse momentum theory, which is #math.equation(block: false, alt: "J → equals Δ p →")[$arrow(J) = "Δ" arrow(p)$]. If #math.equation(block: false, alt: "J → equals 0")[$arrow(J) = 0$], we have the situation described in the example. If a force acts on the system, then #math.equation(block: false, alt: "J → equals F → sub ave Δ t")[$arrow(J) = arrow(F)_("ave") "Δ" t$]. Thus, instead of #math.equation(block: false, alt: "p → sub f equals p → sub i")[$arrow(p)_(f) = arrow(p)_(i)$], we have #linebreak() #math.equation(block: false, alt: "F → sub ave Δ t equals Δ p → equals p → sub f minus p → sub i")[$arrow(F)_("ave") "Δ" t = "Δ" arrow(p) = arrow(p)_("f") − arrow(p)_("i")$] #linebreak() where #math.equation(block: false, alt: "F → sub ave")[$arrow(F)_("ave")$] is the force due to friction. ] ] #examplebox("Example 4")[Landing of #emph[Philae]][ On November 12, 2014, the European Space Agency successfully landed a probe named #strong[#emph[Philae]] on Comet 67P/Churyumov/Gerasimenko . During the landing, however, the probe actually landed three times, because it bounced twice. Let’s calculate how much the comet’s speed changed as a result of the first bounce. #figure(figph[An artist’s rendering of Philae landing on a comet.], alt: "An artist’s rendering of Philae landing on a comet.", caption: [An artist’s rendering of #emph[Philae] landing on a comet.]) Let’s define upward to be the +#emph[y]-direction, perpendicular to the surface of the comet, and #math.equation(block: false, alt: "y equals 0")[$y = 0$] to be at the surface of the comet. Here’s what we know: - The mass of Comet 67P: #math.equation(block: false, alt: "M sub c equals 1.0 times 10 to the power 13 kg")[$M_(c) = 1.0 #h(0.2em) × #h(0.2em) 10^(13) #h(0.2em) "kg"$] - The acceleration due to the comet’s gravity: #math.equation(block: false, alt: "a → equals − open parenthesis 5.0 times 10 to the power −3 m/s squared close parenthesis j ^")[$arrow(a) = "−" ( 5.0 #h(0.2em) × #h(0.2em) 10^(−3) #h(0.2em) "m/s"^(2) ) hat(j)$] - #emph[Philae’s] mass: #math.equation(block: false, alt: "M sub p equals 96 kg")[$M_(p) = 96 #h(0.2em) "kg"$] - Initial touchdown speed: #math.equation(block: false, alt: "v → sub 1 equals − open parenthesis 1.0 m/s close parenthesis j ^")[$arrow(v)_(1) = "−" ( 1.0 #h(0.2em) "m/s" ) hat(j)$] - Initial upward speed due to first bounce: #math.equation(block: false, alt: "v → sub 2 equals open parenthesis 0.38 m/s close parenthesis j ^")[$arrow(v)_(2) = ( 0.38 #h(0.2em) "m/s" ) hat(j)$] - Landing impact time: #math.equation(block: false, alt: "Δ t equals 1.3 s")[$"Δ" t = 1.3 #h(0.2em) "s"$] Strategy We’re asked for how much the comet’s speed changed, but we don’t know much about the comet, beyond its mass and the acceleration its gravity causes. However, we #emph[are] told that the #emph[Philae] lander collides with (lands on) the comet, and bounces off of it. A collision suggests momentum as a strategy for solving this problem. If we define a system that consists of both #emph[Philae] and Comet 67/P, then there is no net external force on this system, and thus the momentum of this system is conserved. (We’ll neglect the gravitational force of the sun.) Thus, if we calculate the change of momentum of the lander, we automatically have the change of momentum of the comet. Also, the comet’s change of velocity is directly related to its change of momentum as a result of the lander “colliding” with it. Solution Let #math.equation(block: false, alt: "p → sub 1")[$arrow(p)_(1)$] be #emph[Philae’s] momentum at the moment just before touchdown, and #math.equation(block: false, alt: "p → sub 2")[$arrow(p)_(2)$] be its momentum just after the first bounce. Then its momentum just before landing was #math.equation(block: true, alt: "p → sub 1 equals M sub p v → sub 1 equals open parenthesis 96 kg close parenthesis open parenthesis − 1.0 m/s j ^ close parenthesis equals − open parenthesis 96 kg times m/s close parenthesis j ^")[$arrow(p)_(1) = M_(p) arrow(v)_(1) = ( 96 #h(0.2em) "kg" ) ( "−" 1.0 #h(0.2em) "m/s" hat(j) ) = "−" ( 96 #h(0.2em) "kg" · "m/s" ) hat(j)$] and just after was #math.equation(block: true, alt: "p → sub 2 equals M sub p v → sub 2 equals open parenthesis 96 kg close parenthesis open parenthesis plus 0.38 m/s j ^ close parenthesis equals open parenthesis 36.5 kg times m/s close parenthesis j ^ .")[$arrow(p)_(2) = M_(p) arrow(v)_(2) = ( 96 #h(0.2em) "kg" ) ( + 0.38 #h(0.2em) "m/s" hat(j) ) = ( 36.5 #h(0.2em) "kg" · "m/s" ) hat(j) .$] Therefore, the lander’s change of momentum during the first bounce is #math.equation(block: true, alt: "Δ p → equals p → sub 2 minus p → sub 1; equals open parenthesis 36.5 kg times m/s close parenthesis j ^ minus open parenthesis −96.0 kg times m/s j ^ close parenthesis equals open parenthesis 133 kg times m/s close parenthesis j ^")[$"Δ" arrow(p) = arrow(p)_(2) − arrow(p)_(1) \ & = ( 36.5 #h(0.2em) "kg" · "m/s" ) hat(j) − ( −96.0 #h(0.2em) "kg" · "m/s" hat(j) ) = ( 133 #h(0.2em) "kg" · "m/s" ) hat(j)$] Notice how important it is to include the negative sign of the initial momentum. Now for the comet. Since momentum of the system must be conserved, the #emph[comet’s] momentum changed by exactly the negative of this: #math.equation(block: true, alt: "Δ p → sub c equals − Δ p → equals − open parenthesis 133 kg times m/s close parenthesis j ^ .")[$"Δ" arrow(p)_(c) = "−" "Δ" arrow(p) = "−" ( 133 #h(0.2em) "kg" · "m/s" ) hat(j) .$] Therefore, its change of velocity is #math.equation(block: true, alt: "Δ v → sub c equals the fraction Δ p → sub c over M sub c equals the fraction − open parenthesis 133 kg times m/s close parenthesis j ^ over 1.0 times 10 to the power 13 kg equals − open parenthesis 1.33 times 10 to the power −11 m/s close parenthesis j ^ .")[$"Δ" arrow(v)_(c) = frac("Δ" arrow(p)_(c), M_(c)) = frac("−" ( 133 #h(0.2em) "kg" · "m/s" ) hat(j), 1.0 #h(0.2em) × #h(0.2em) 10^(13) #h(0.2em) "kg") = "−" ( 1.33 #h(0.2em) × #h(0.2em) 10^(−11) #h(0.2em) "m/s" ) hat(j) .$] Significance This is a very small change in velocity, about a thousandth of a billionth of a meter per second. Crucially, however, it is #emph[not] zero. ] #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ The changes of momentum for #emph[Philae] and for Comet 67/P were equal (in magnitude). Were the impulses experienced by #emph[Philae] and the comet equal? How about the forces? How about the changes of kinetic energies? #solutionbox[ The impulse is the change in momentum multiplied by the time required for the change to occur. By conservation of momentum, the changes in momentum of the probe and the comment are of the same magnitude, but in opposite directions, and the interaction time for each is also the same. Therefore, the impulse each receives is of the same magnitude, but in opposite directions. Because they act in opposite directions, the impulses are not the same. As for the impulse, the force on each body acts in opposite directions, so the forces on each are not equal. However, the change in kinetic energy differs for each, because the collision is not elastic. ] ] === Summary - The law of conservation of momentum says that the momentum of a closed system is constant in time (conserved). - A closed (or isolated) system is defined to be one for which the mass remains constant, and the net external force is zero. - The total momentum of a system is conserved #emph[only] when the system is closed. === Conceptual Questions Under what circumstances is momentum conserved? #solutionbox[ Momentum is conserved when the mass of the system of interest remains constant during the interaction in question and when no #emph[net] external force acts on the system during the interaction. ] Can momentum be conserved for a system if there are external forces acting on the system? If so, under what conditions? If not, why not? Explain in terms of momentum and Newton’s laws how a car’s air resistance is due in part to the fact that it pushes air in its direction of motion. #solutionbox[ To accelerate air molecules in the direction of motion of the car, the car must exert a force on these molecules by Newton’s second law #math.equation(block: false, alt: "F → equals d p → / d t")[$arrow(F) = d arrow(p) "/" d t$]. By Newton’s third law, the air molecules exert a force of equal magnitude but in the opposite direction on the car. This force acts in the direction opposite the motion of the car and constitutes the force due to air resistance. ] Can objects in a system have momentum while the momentum of the system is zero? Explain your answer. A sprinter accelerates out of the starting blocks. Can you consider him as a closed system? Explain. #solutionbox[ No, he is not a closed system because a net nonzero external force acts on him in the form of the starting blocks pushing on his feet. ] A rocket in deep space (zero gravity) accelerates by firing hot gas out of its thrusters. Does the rocket constitute a closed system? Explain. === Problems Train cars are coupled together by being bumped into one another. Suppose two loaded train cars are moving toward one another, the first having a mass of #math.equation(block: false, alt: "1.50 times 10 to the power 5 kg")[$1.50 #h(0.2em) × #h(0.2em) 10^(5) #h(0.2em) "kg"$] and a velocity of #math.equation(block: false, alt: "open parenthesis 0.30 m/s close parenthesis i ^")[$( 0.30 #h(0.2em) "m/s" ) hat(i)$], and the second having a mass of #math.equation(block: false, alt: "1.10 times 10 to the power 5 kg")[$1.10 #h(0.2em) × #h(0.2em) 10^(5) #h(0.2em) "kg"$] and a velocity of #math.equation(block: false, alt: "− open parenthesis 0.12 m/s close parenthesis i ^")[$"−" ( 0.12 #h(0.2em) "m/s" ) hat(i)$]. What is their final velocity? #figure(figph[Two train cars are shown moving toward each other. The car on the left is moving with v sub i 1 equals 0.30 meters per second i hat to the right, and the car on the right is moving with v sub i 2 equals -0.12 meters per second i hat to the left.], alt: "Two train cars are shown moving toward each other. The car on the left is moving with v sub i 1 equals 0.30 meters per second i hat to the right, and the car on the right is moving with v sub i 2 equals -0.12 meters per second i hat to the left.", caption: none) #solutionbox[ #math.equation(block: true, alt: "open parenthesis 0.122 m/s close parenthesis i ^")[$( 0.122 #h(0.2em) "m/s" ) hat(i)$] ] Two identical pucks collide elastically on an air hockey table. Puck 1 was originally at rest; puck 2 has an incoming speed of 6.00 m/s and scatters at an angle of #math.equation(block: false, alt: "30 °")[$30 "°"$] with respect to its incoming direction. What is the velocity (magnitude and direction) of puck 1 after the collision? #figure(figph[Two sets of red and blue hockey pucks are shown. The first row has a blue hockey puck with an arrow pointing left toward a red hockey puck. The second row shows a similar blue puck with a shorter arrow pointing left toward a red hockey puck at a 30-degree angle from the horizontal.], alt: "Two sets of red and blue hockey pucks are shown. The first row has a blue hockey puck with an arrow pointing left toward a red hockey puck. The second row shows a similar blue puck with a shorter arrow pointing left toward a red hockey puck at a 30-degree angle from the horizontal.", caption: none) The figure below shows a bullet of mass 200 g traveling horizontally towards the east with speed 400 m/s, which strikes a block of mass 1.5 kg that is initially at rest on a frictionless table. #figure(figph[A drawing of a block on a table, and a bullet headed toward it.], alt: "A drawing of a block on a table, and a bullet headed toward it.", caption: none) After striking the block, the bullet is embedded in the block and the block and the bullet move together as one unit. + What is the magnitude and direction of the velocity of the block/bullet combination immediately after the impact? + What is the magnitude and direction of the impulse by the block on the bullet? + What is the magnitude and direction of the impulse from the bullet on the block? + If it took 3 ms for the bullet to change the speed from 400 m/s to the final speed after impact, what is the average force between the block and the bullet during this time? #solutionbox[ a. 47 m/s in the bullet to block direction; b.#math.equation(block: false, alt: "70.6 N times s")[$70.6 #h(0.2em) "N" · "s"$], toward the bullet; c. #math.equation(block: false, alt: "70.6 N times s")[$70.6 #h(0.2em) "N" · "s"$], toward the block; d. magnitude is #math.equation(block: false, alt: "2.35 times 10 to the power 4 N")[$2.35 #h(0.2em) × #h(0.2em) 10^(4) #h(0.2em) "N"$] ] A 20-kg child is coasting at 3.3 m/s over flat ground in a 4.0-kg wagon. + If the child drops a 1-kg ball out the back of the wagon, what is the final speed of the child and wagon? + If the child drops a 1-kg ball out the back of the wagon so that the ball is at rest relative to the ground, what is the final speed of the child and wagon? A 4.5 kg puffer fish expands to 40% of its mass by taking in water. When the puffer fish is threatened, it releases the water toward the threat to move quickly forward. What is the ratio of the speed of the puffer fish forward to the speed of the expelled water backwards? #solutionbox[ 2:5 ] Explain why a cannon recoils when it fires a shell. Two figure skaters are coasting in the same direction, with the leading skater moving at 5.5 m/s and the trailing skating moving at 6.2 m/s. When the trailing skater catches up with the leading skater, he picks her up without applying any horizontal forces on his skates. If the trailing skater is 50% heavier than the 50-kg leading skater, what is their speed after he picks her up? #solutionbox[ 5.9 m/s ] A 2000-kg railway freight car coasts at 4.4 m/s underneath a grain terminal, which dumps grain directly down into the freight car. If the speed of the loaded freight car must not go below 3.0 m/s, what is the maximum mass of grain that it can accept?