#set document(title: "4.2 Acceleration Vector", 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")) == 4.2#h(0.6em)Acceleration Vector === Instantaneous Acceleration In addition to obtaining the displacement and velocity vectors of an object in motion, we often want to know its #strong[acceleration vector] at any point in time along its trajectory. This acceleration vector is the instantaneous acceleration and it can be obtained from the derivative with respect to time of the velocity function, as we have seen in a previous chapter. The only difference in two or three dimensions is that these are now vector quantities. Taking the derivative with respect to time #math.equation(block: false, alt: "v → open parenthesis t close parenthesis ,")[$arrow(v) ( t ) ,$] we find #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ #math.equation(block: true, alt: "a → open parenthesis t close parenthesis equals lim ∆ t → 0 the fraction v → open parenthesis t plus Δ t close parenthesis minus v → open parenthesis t close parenthesis over Δ t equals the fraction d v → open parenthesis t close parenthesis over d t .")[$arrow(a) ( t ) = limits("lim")_(∆ t → 0) frac(arrow(v) ( t + "Δ" t ) − arrow(v) ( t ), "Δ" t) = frac(d arrow(v) ( t ), d t) .$] ] The acceleration in terms of components is #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ #math.equation(block: true, alt: "a → open parenthesis t close parenthesis equals ​ the fraction d v sub x open parenthesis t close parenthesis over d t i ^ plus the fraction d v sub y open parenthesis t close parenthesis over d t j ^ plus the fraction d v sub z open parenthesis t close parenthesis over d t k ^ .")[$arrow(a) ( t ) = "​" frac(d v_(x) ( t ), d t) hat(i) + frac(d v_(y) ( t ), d t) hat(j) + frac(d v_(z) ( t ), d t) hat(k) .$] #math.equation(block: true, alt: "equals a sub x open parenthesis t close parenthesis i ^ plus a sub y open parenthesis t close parenthesis j ^ plus a sub z open parenthesis t close parenthesis k ^")[$= a_(x) ( t ) hat(i) + a_(y) ( t ) hat(j) + a_(z) ( t ) hat(k)$] ] Also, since the velocity is the derivative of the position function, we can write the acceleration in terms of the second derivative of the position function: #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ #math.equation(block: true, alt: "a → open parenthesis t close parenthesis equals the fraction d squared x open parenthesis t close parenthesis over d t squared i ^ plus the fraction d squared y open parenthesis t close parenthesis over d t squared j ^ plus the fraction d squared z open parenthesis t close parenthesis over d t squared k ^ .")[$arrow(a) ( t ) = frac(d^(2) x ( t ), d t^(2)) hat(i) + frac(d^(2) y ( t ), d t^(2)) hat(j) + frac(d^(2) z ( t ), d t^(2)) hat(k) .$] ] #examplebox("Example 1")[Finding an Acceleration Vector][ A particle has a velocity of #math.equation(block: false, alt: "v → open parenthesis t close parenthesis equals 5.0 t i ^ plus t squared j ^ minus 2.0 t cubed k ^ m/s .")[$arrow(v) ( t ) = 5.0 t hat(i) + t^(2) hat(j) − 2.0 t^(3) hat(k) "m/s" .$] (a) What is the acceleration function? (b) What is the acceleration vector at #emph[t] = 2.0 s? Find its magnitude and direction. Solution (a) We take the first derivative with respect to time of the velocity function to find the acceleration. The derivative is taken component by component: #math.equation(block: true, alt: "a → open parenthesis t close parenthesis equals 5.0 i ^ plus 2.0 t j ^ minus 6.0 t squared k ^ m/ s squared .")[$arrow(a) ( t ) = 5.0 hat(i) + 2.0 t hat(j) − 6.0 t^(2) hat(k) "m/" "s"^(2) .$] (b) Evaluating #math.equation(block: false, alt: "a → open parenthesis 2.0 s close parenthesis equals 5.0 i ^ plus 4.0 j ^ minus 24.0 k ^ m/ s squared")[$arrow(a) ( 2.0 #h(0.2em) "s" ) = 5.0 hat(i) + 4.0 hat(j) − 24.0 hat(k) "m/" "s"^(2)$] gives us the direction in unit vector notation. The magnitude of the acceleration is #math.equation(block: false, alt: "| a → open parenthesis 2.0 s close parenthesis | equals the square root of 5.0 squared plus 4.0 squared plus open parenthesis −24.0 close parenthesis squared equals 24.8 m/ s squared .")[$| arrow(a) ( 2.0 #h(0.2em) "s" ) | = sqrt(5.0^(2) + 4.0^(2) + attach(( −24.0 ), t: 2)) = 24.8 #h(0.2em) "m/" "s"^(2) .$] Significance In this example we find that acceleration has a time dependence and is changing throughout the motion. Let’s consider a different velocity function for the particle. ] #examplebox("Example 2")[Finding a Particle Acceleration][ A particle has a position function #math.equation(block: false, alt: "r → open parenthesis t close parenthesis equals open parenthesis 10 t minus t squared close parenthesis i ^ plus 5 t j ^ plus 5 t ​ k ^ m .")[$arrow(r) ( t ) = ( 10 t − t^(2) ) hat(i) + 5 t hat(j) + 5 t "​" hat(k) "m" .$] (a) What is the velocity? (b) What is the acceleration? (c) Describe the motion from #emph[t] = 0 s. Strategy We can gain some insight into the problem by looking at the position function. It is linear in #emph[y] and #emph[z], so we know the acceleration in these directions is zero when we take the second derivative. Also, note that the position in the #emph[x] direction is zero for #emph[t] = 0 s and #emph[t] = 10 s. Solution (a) Taking the derivative with respect to time of the position function, we find #math.equation(block: true, alt: "v → open parenthesis t close parenthesis equals open parenthesis 10 minus 2 t close parenthesis i ^ plus 5 j ^ plus 5 k ^ m/s .")[$arrow(v) ( t ) = ( 10 − 2 t ) hat(i) + 5 hat(j) + 5 hat(k) #h(0.2em) "m/s" .$] The velocity function is linear in time in the #emph[x] direction and is constant in the #emph[y] and #emph[z] directions. (b) Taking the derivative of the velocity function, we find #math.equation(block: true, alt: "a → open parenthesis t close parenthesis equals −2 i ^ m/s squared .")[$arrow(a) ( t ) = −2 hat(i) #h(0.2em) "m/s"^(2) .$] The acceleration vector is a constant in the negative #emph[x]-direction. (c) The trajectory of the particle can be seen in . Let’s look in the #emph[y] and #emph[z] directions first. The particle’s position increases steadily as a function of time with a constant velocity in these directions. In the #emph[x] direction, however, the particle follows a path in positive #emph[x] until #emph[t] = 5 s, when it reverses direction. We know this from looking at the velocity function, which becomes zero at this time and negative thereafter. We also know this because the acceleration is negative and constant—meaning, the particle is accelerating in the opposite direction. The particle’s position reaches 25 m, where it then reverses direction and begins to accelerate in the negative #emph[x] direction. The position reaches zero at #emph[t] = 10 s. #figure(figph[An x y z coordinate system is shown. All the axes show distance in meters and run from -50 to 50 meters. A series of 10 red stars are shown, with the sixth star is labeled as t = 6 s and the tenth as t = 10 s. The red series of stars starts at the origin and curves upward (both y and z increasing with time). Vertical dashed lines connect the red dots to a series of blue dots in the x y plane. The blue dots are all in the first quadrant (positive x and y). The dots are regularly spaced along the y coordinate, while the x coordinate starts at 0, increases, reaches a maximum of x = 25 m at t = 5, and then decreases back to x = 0 at t 10 s.], alt: "An x y z coordinate system is shown. All the axes show distance in meters and run from -50 to 50 meters. A series of 10 red stars are shown, with the sixth star is labeled as t = 6 s and the tenth as t = 10 s. The red series of stars starts at the origin and curves upward (both y and z increasing with time). Vertical dashed lines connect the red dots to a series of blue dots in the x y plane. The blue dots are all in the first quadrant (positive x and y). The dots are regularly spaced along the y coordinate, while the x coordinate starts at 0, increases, reaches a maximum of x = 25 m at t = 5, and then decreases back to x = 0 at t 10 s.", caption: [The particle starts at point (#emph[x], #emph[y], #emph[z]) = (0, 0, 0) with position vector #math.equation(block: false, alt: "r → equals 0")[$arrow(r) = 0$] as shown with red stars. The projection of the trajectory onto the #emph[xy-]plane is shown with blue dots. The values of #emph[y] and #emph[z] increase linearly as a function of time, whereas #emph[x] has a turning point at #emph[t] = 5 s and 25 m, when it reverses direction. At this point, the #emph[x] component of the velocity becomes negative. At #emph[t] = 10 s, the particle is back to 0 m in the #emph[x] direction.]) Significance By graphing the trajectory of the particle, we can better understand its motion, given by the numerical results of the kinematic equations. ] #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ Suppose the acceleration function has the form #math.equation(block: false, alt: "a → open parenthesis t close parenthesis equals a i ^ plus b j ^ plus c k ^ m/ s squared ,")[$arrow(a) ( t ) = a hat(i) + b hat(j) + c hat(k) "m/" "s"^(2) ,$] where #emph[a, b,] and #emph[c] are constants. What can be said about the functional form of the velocity function? #solutionbox[ The acceleration vector is constant and doesn’t change with time. If #emph[a, b], and #emph[c] are not zero, then the velocity function must be linear in time. We have #math.equation(block: false, alt: "v → open parenthesis t close parenthesis equals ∫ a → d t equals ∫ open parenthesis a i ^ plus b j ^ plus c k ^ close parenthesis d t equals open parenthesis a i ^ plus b j ^ plus c k ^ close parenthesis t m/s ,")[$arrow(v) ( t ) = display(∫ arrow(a) d t =) display(∫ ( a hat(i) + b hat(j) + c hat(k) ) d t =) ( a hat(i) + b hat(j) + c hat(k) ) t #h(0.2em) "m/s" ,$] since taking the derivative of the velocity function produces #math.equation(block: false, alt: "a → open parenthesis t close parenthesis .")[$arrow(a) ( t ) .$] If any of the components of the acceleration are zero, then that component of the velocity would be a constant. ] ] === Constant Acceleration Multidimensional motion with constant acceleration can be treated the same way as shown in the previous chapter for one-dimensional motion. Earlier we showed that three-dimensional motion is equivalent to three one-dimensional motions, each along an axis perpendicular to the others. To develop the relevant equations in each direction, let’s consider the two-dimensional problem of a particle moving in the #emph[xy] plane with constant acceleration, ignoring the #emph[z]-component for the moment. The acceleration vector is #math.equation(block: true, alt: "a → equals a sub x i ^ plus a sub y j ^ .")[$arrow(a) = a_(x) hat(i) + a_(y) hat(j) .$] Each component of the motion has a separate set of equations similar to – of the previous chapter on one-dimensional motion. We show only the equations for position and velocity in the #emph[x]- and #emph[y]-directions. A similar set of kinematic equations could be written for motion in the #emph[z]-direction: #math.equation(block: true, alt: "x open parenthesis t close parenthesis equals x sub 0 plus open parenthesis v sub x close parenthesis sub avg t")[$x ( t ) = x_(0) + attach(( v_(x) ), b: "avg") t$] #math.equation(block: true, alt: "a → sub ave equals the fraction v → open parenthesis t sub 2 close parenthesis minus v → open parenthesis t sub 1 close parenthesis over t sub 2 minus t sub 1")[$arrow(a)_("ave") = frac(arrow(v) ( t_(2) ) − arrow(v) ( t_(1) ), t_(2) − t_(1))$] #math.equation(block: true, alt: "v sub x open parenthesis t close parenthesis equals v sub 0 x plus a sub x t")[$v_(x) ( t ) = v_(0 x) + a_(x) t$] #math.equation(block: true, alt: "x open parenthesis t close parenthesis equals x sub 0 plus v sub 0 x t plus the fraction 1 over 2 a sub x t squared")[$x ( t ) = x_(0) + v_(0 x) t + frac(1, 2) a_(x) t^(2)$] #math.equation(block: true, alt: "v x 2 open parenthesis t close parenthesis equals v 0 x 2 plus 2 a sub x open parenthesis x minus x sub 0 close parenthesis")[$v_(x)^(2) ( t ) = v_(0 x)^(2) + 2 a_(x) ( x − x_(0) )$] #math.equation(block: true, alt: "y open parenthesis t close parenthesis equals y sub 0 plus open parenthesis v sub y close parenthesis sub avg t")[$y ( t ) = y_(0) + attach(( v_(y) ), b: "avg") t$] #math.equation(block: true, alt: "v sub y open parenthesis t close parenthesis equals v sub 0 y plus a sub y t")[$v_(y) ( t ) = v_(0 y) + a_(y) t$] #math.equation(block: true, alt: "y open parenthesis t close parenthesis equals y sub 0 plus v sub 0 y t plus the fraction 1 over 2 a sub y t squared")[$y ( t ) = y_(0) + v_(0 y) t + frac(1, 2) a_(y) t^(2)$] #math.equation(block: true, alt: "v y 2 open parenthesis t close parenthesis equals v 0 y 2 plus 2 a sub y open parenthesis y minus y sub 0 close parenthesis .")[$v_(y)^(2) ( t ) = v_(0 y)^(2) + 2 a_(y) ( y − y_(0) ) .$] Here the subscript 0 denotes the initial position or velocity. to can be substituted into and without the #emph[z]-component to obtain the position vector and velocity vector as a function of time in two dimensions: #math.equation(block: true, alt: "r → open parenthesis t close parenthesis equals x open parenthesis t close parenthesis i ^ plus y open parenthesis t close parenthesis j ^ and v → open parenthesis t close parenthesis equals v sub x open parenthesis t close parenthesis i ^ plus v sub y open parenthesis t close parenthesis j ^ .")[$arrow(r) ( t ) = x ( t ) hat(i) + y ( t ) hat(j) #h(0.2em) "and" #h(0.2em) arrow(v) ( t ) = v_(x) ( t ) hat(i) + v_(y) ( t ) hat(j) .$] The following example illustrates a practical use of the kinematic equations in two dimensions. #examplebox("Example 3")[A Skier][ shows a skier moving with an acceleration of #math.equation(block: false, alt: "2.1 m/ s squared")[$2.1 #h(0.2em) "m/" "s"^(2)$] down a slope of #math.equation(block: false, alt: "15 °")[$15 "°"$] at #emph[t] = 0. With the origin of the coordinate system at the front of the lodge, her initial position and velocity are #math.equation(block: true, alt: "r → open parenthesis 0 close parenthesis equals open parenthesis 75.0 i ^ minus 20.0 j ^ close parenthesis m")[$arrow(r) ( 0 ) = ( 75.0 hat(i) − 20.0 hat(j) ) #h(0.2em) "m"$] and #math.equation(block: true, alt: "v → open parenthesis 0 close parenthesis equals open parenthesis 4.1 i ^ minus 1.1 j ^ close parenthesis m/s .")[$arrow(v) ( 0 ) = ( 4.1 hat(i) − 1.1 hat(j) ) #h(0.2em) "m/s" .$] (a) What are the #emph[x-] and #emph[y]-components of the skier’s position and velocity as functions of time? (b) What are her position and velocity at #emph[t] = 10.0 s? #figure(figph[An illustration of a skier in an x y coordinate system is shown. The skier is moving along a line that is 15 degrees below the horizontal x direction and has an acceleration of a = 2.1 meters per second squared also directed in his direction of motion. The acceleration is represented as a purple arrow.], alt: "An illustration of a skier in an x y coordinate system is shown. The skier is moving along a line that is 15 degrees below the horizontal x direction and has an acceleration of a = 2.1 meters per second squared also directed in his direction of motion. The acceleration is represented as a purple arrow.", caption: [A skier has an acceleration of #math.equation(block: false, alt: "2.1 m/s squared")[$2.1 #h(0.2em) "m/s"^(2)$] down a slope of #math.equation(block: false, alt: "15 ° .")[$15 "°" .$] The origin of the coordinate system is at the ski lodge.]) Strategy Since we are evaluating the components of the motion equations in the #emph[x] and #emph[y] directions, we need to find the components of the acceleration and put them into the kinematic equations. The components of the acceleration are found by referring to the coordinate system in . Then, by inserting the components of the initial position and velocity into the motion equations, we can solve for her position and velocity at a later time #emph[t]. Solution (a) The origin of the coordinate system is at the top of the hill with #emph[y-]axis vertically upward and the #emph[x-]axis horizontal. By looking at the trajectory of the skier, the #emph[x-]component of the acceleration is positive and the #emph[y-]component is negative. Since the angle is #math.equation(block: false, alt: "15 °")[$15 "°"$] down the slope, we find #math.equation(block: true, alt: "a sub x equals open parenthesis 2.1 m/ s squared close parenthesis cos open parenthesis 15 ° close parenthesis equals 2.0 m/ s squared")[$a_(x) = ( 2.1 #h(0.2em) "m/" "s"^(2) ) #h(0.2em) "cos" ( 15 "°" ) = 2.0 #h(0.2em) "m/" "s"^(2)$] #math.equation(block: true, alt: "a sub y equals open parenthesis −2.1 m/ s squared close parenthesis sin 15 ° equals −0.54 m/ s squared .")[$a_(y) = ( −2.1 #h(0.2em) "m/" "s"^(2) ) #h(0.2em) "sin" #h(0.2em) 15 "°" = −0.54 #h(0.2em) "m/" "s"^(2) .$] Inserting the initial position and velocity into and for #emph[x], we have #math.equation(block: true, alt: "x open parenthesis t close parenthesis equals 75.0 m plus open parenthesis 4.1 m/s close parenthesis t plus the fraction 1 over 2 open parenthesis 2.0 m/ s squared close parenthesis t squared")[$x ( t ) = 75.0 #h(0.2em) "m" + ( 4.1 #h(0.2em) "m/s" ) t + frac(1, 2) ( 2.0 #h(0.2em) "m/" "s"^(2) ) t^(2)$] #math.equation(block: true, alt: "v sub x open parenthesis t close parenthesis equals 4.1 m/s plus open parenthesis 2.0 m/ s squared close parenthesis t .")[$v_(x) ( t ) = 4.1 #h(0.2em) "m/s" + ( 2.0 #h(0.2em) "m/" "s"^(2) ) t .$] For #emph[y], we have #math.equation(block: true, alt: "y open parenthesis t close parenthesis equals −20.0 m plus open parenthesis −1.1 m/s close parenthesis t plus the fraction 1 over 2 open parenthesis −0.54 m/ s squared close parenthesis t squared")[$y ( t ) = −20.0 #h(0.2em) "m" + ( −1.1 #h(0.2em) "m/s" ) t + frac(1, 2) ( −0.54 #h(0.2em) "m/" "s"^(2) ) t^(2)$] #math.equation(block: true, alt: "v sub y open parenthesis t close parenthesis equals −1.1 m/s plus open parenthesis −0.54 m/ s squared close parenthesis t .")[$v_(y) ( t ) = −1.1 #h(0.2em) "m/s" + ( −0.54 #h(0.2em) "m/" "s"^(2) ) t .$] (b) Now that we have the equations of motion for #emph[x] and #emph[y] as functions of time, we can evaluate them at #emph[t] = 10.0 s: #math.equation(block: true, alt: "x open parenthesis 10.0 s close parenthesis equals 75.0 m plus open parenthesis 4.1 m/ s squared close parenthesis open parenthesis 10.0 s close parenthesis plus the fraction 1 over 2 open parenthesis 2.0 m/ s squared close parenthesis open parenthesis 10.0 s close parenthesis squared equals 216.0 m")[$x ( 10.0 #h(0.2em) "s" ) = 75.0 #h(0.2em) "m" + ( 4.1 #h(0.2em) "m/" "s"^(2) ) ( 10.0 #h(0.2em) "s" ) + frac(1, 2) ( 2.0 #h(0.2em) "m/" "s"^(2) ) attach(( 10.0 #h(0.2em) "s" ), t: 2) = 216.0 #h(0.2em) "m"$] #math.equation(block: true, alt: "v sub x open parenthesis 10.0 s close parenthesis equals 4.1 m/s plus open parenthesis 2.0 m/ s squared close parenthesis open parenthesis 10.0 s close parenthesis equals 24.1 m /s")[$v_(x) ( 10.0 #h(0.2em) "s" ) = 4.1 #h(0.2em) "m/s" + ( 2.0 #h(0.2em) "m/" "s"^(2) ) ( 10.0 #h(0.2em) "s" ) = 24.1 "m" "/s"$] #math.equation(block: true, alt: "y open parenthesis 10.0 s close parenthesis equals −20.0 m plus open parenthesis −1.1 m/s close parenthesis open parenthesis 10.0 s close parenthesis plus the fraction 1 over 2 open parenthesis −0.54 m/ s squared close parenthesis open parenthesis 10.0 s close parenthesis squared equals −58.0 m")[$y ( 10.0 #h(0.2em) "s" ) = −20.0 #h(0.2em) "m" + ( −1.1 #h(0.2em) "m/s" ) ( 10.0 #h(0.2em) "s" ) + frac(1, 2) ( −0.54 #h(0.2em) "m/" "s"^(2) ) attach(( 10.0 #h(0.2em) "s" ), t: 2) = −58.0 #h(0.2em) "m"$] #math.equation(block: true, alt: "v sub y open parenthesis 10.0 s close parenthesis equals −1.1 m/s plus open parenthesis −0.54 m/ s squared close parenthesis open parenthesis 10.0 s close parenthesis equals −6.5 m/s .")[$v_(y) ( 10.0 #h(0.2em) "s" ) = −1.1 #h(0.2em) "m/s" + ( −0.54 #h(0.2em) "m/" "s"^(2) ) ( 10.0 #h(0.2em) "s" ) = −6.5 #h(0.2em) "m/s" .$] The position and velocity at #emph[t] = 10.0 s are, finally, #math.equation(block: true, alt: "r → open parenthesis 10.0 s close parenthesis equals open parenthesis 216.0 i ^ minus 58.0 j ^ close parenthesis m")[$arrow(r) ( 10.0 #h(0.2em) "s" ) = ( 216.0 hat(i) − 58.0 hat(j) ) #h(0.2em) "m"$] #math.equation(block: true, alt: "v → open parenthesis 10.0 s close parenthesis equals open parenthesis 24.1 i ^ minus 6.5 j ^ close parenthesis m/s .")[$arrow(v) ( 10.0 #h(0.2em) "s" ) = ( 24.1 hat(i) − 6.5 hat(j) ) "m/s" .$] The magnitude of the velocity of the skier at 10.0 s is 25 m/s, which is 60 mi/h. Significance It is useful to know that, given the initial conditions of position, velocity, and acceleration of an object, we can find the position, velocity, and acceleration at any later time. ] With through we have completed the set of expressions for the position, velocity, and acceleration of an object moving in two or three dimensions. If the trajectories of the objects look something like the “Red Arrows” in the opening picture for the chapter, then the expressions for the position, velocity, and acceleration can be quite complicated. In the sections to follow we examine two special cases of motion in two and three dimensions by looking at projectile motion and circular motion. #notebox("Note", rgb("#8a94a6"), rgb("#556666"), rgb("#f7f8fa"))[ At this #link("https://openstax.org/l/21phetmotladyb")[University of Colorado Boulder website], you can explore the position velocity and acceleration of a ladybug with an interactive simulation that allows you to change these parameters. ] === Summary - In two and three dimensions, the acceleration vector can have an arbitrary direction and does not necessarily point along a given component of the velocity. - The instantaneous acceleration is produced by a change in velocity taken over a very short (infinitesimal) time period. Instantaneous acceleration is a vector in two or three dimensions. It is found by taking the derivative of the velocity function with respect to time. - In three dimensions, acceleration #math.equation(block: false, alt: "a → open parenthesis t close parenthesis")[$arrow(a) ( t )$] can be written as a vector sum of the one-dimensional accelerations #math.equation(block: false, alt: "a sub x open parenthesis t close parenthesis , a sub y open parenthesis t close parenthesis , and a sub z open parenthesis t close parenthesis")[$a_(x) ( t ) , a_(y) ( t ) , "and" #h(0.2em) a_(z) ( t )$] along the #emph[x-], #emph[y]-, and #emph[z-]axes. - The kinematic equations for constant acceleration can be written as the vector sum of the constant acceleration equations in the #emph[x], #emph[y], and #emph[z] directions. === Conceptual Questions If the position function of a particle is a linear function of time, what can be said about its acceleration? If an object has a constant #emph[x]-component of the velocity and suddenly experiences an acceleration in the #emph[y] direction, does the #emph[x-]component of its velocity change? #solutionbox[ No, motions in perpendicular directions are independent. ] If an object has a constant #emph[x-]component of velocity and suddenly experiences an acceleration at an angle of #math.equation(block: false, alt: "70 °")[$70 "°"$] in the #emph[x] direction, does the #emph[x-]component of velocity change? === Problems The position of a particle is #math.equation(block: false, alt: "r → open parenthesis t close parenthesis equals open parenthesis 3.0 t squared i ^ plus 5.0 j ^ minus 6.0 t k ^ close parenthesis m .")[$arrow(r) ( t ) = ( 3.0 t^(2) hat(i) + 5.0 hat(j) − 6.0 t hat(k) ) #h(0.2em) "m" .$] (a) Determine its velocity and acceleration as functions of time. (b) What are its velocity and acceleration at time #emph[t] = 0? A particle’s acceleration is #math.equation(block: false, alt: "open parenthesis 4.0 i ^ plus 3.0 j ^ close parenthesis m/ s squared .")[$( 4.0 hat(i) + 3.0 hat(j) ) "m/" "s"^(2) .$] At #emph[t] = 0, its position and velocity are zero. (a) What are the particle’s position and velocity as functions of time? (b) Find the equation of the path of the particle. Draw the #emph[x-] and #emph[y-]axes and sketch the trajectory of the particle. #solutionbox[ a. #math.equation(block: false, alt: "v → open parenthesis t close parenthesis equals open parenthesis 4.0 t i ^ plus 3.0 t j ^ close parenthesis m/s ,")[$arrow(v) ( t ) = ( 4.0 t hat(i) + 3.0 t hat(j) ) "m/s" ,$]#math.equation(block: false, alt: "r → open parenthesis t close parenthesis equals open parenthesis 2.0 t squared i ^ plus the fraction 3 over 2 t squared j ^ close parenthesis m")[$arrow(r) ( t ) = ( 2.0 t^(2) hat(i) + frac(3, 2) t^(2) hat(j) ) #h(0.2em) "m"$], #linebreak() b. #math.equation(block: false, alt: "x open parenthesis t close parenthesis equals 2.0 t squared m, y open parenthesis t close parenthesis equals the fraction 3 over 2 t squared m, t squared equals the fraction x over 2 ⇒ y equals the fraction 3 over 4 x")[$x ( t ) = 2.0 t^(2) "m," #h(0.2em) y ( t ) = frac(3, 2) t^(2) "m," #h(0.2em) t^(2) = frac(x, 2) ⇒ y = frac(3, 4) x$] #linebreak() #figure(figph[A graph of the linear function y equals 3 quarters x. The graph is a straight, positive slope line through the origin.], alt: "A graph of the linear function y equals 3 quarters x. The graph is a straight, positive slope line through the origin.", caption: none) ] A boat leaves the dock at #emph[t] = 0 and heads out into a lake with an acceleration of #math.equation(block: false, alt: "2.0 m/ s squared i ^ .")[$2.0 #h(0.2em) "m/" "s"^(2) hat(i) .$] A strong wind is pushing the boat, giving it an additional velocity of #math.equation(block: false, alt: "2.0 m/s i ^ plus 1.0 m/s j ^ .")[$2.0 #h(0.2em) "m/s" hat(i) + 1.0 #h(0.2em) "m/s" hat(j) .$] (a) What is the velocity of the boat at #emph[t] = 10 s? (b) What is the position of the boat at #emph[t] = 10s? Draw a sketch of the boat’s trajectory and position at #emph[t] = 10 s, showing the #emph[x-] and #emph[y]-axes. The position of a particle for #emph[t] \> 0 is given by #math.equation(block: false, alt: "r → open parenthesis t close parenthesis equals open parenthesis 3.0 t squared i ^ minus 7.0 t cubed j ^ minus 5.0 t to the power −2 k ^ close parenthesis m .")[$arrow(r) ( t ) = ( 3.0 t^(2) hat(i) − 7.0 t^(3) hat(j) − 5.0 t^(−2) hat(k) ) #h(0.2em) "m" .$] (a) What is the velocity as a function of time? (b) What is the acceleration as a function of time? (c) What is the particle’s velocity at #emph[t] = 2.0 s? (d) What is its speed at #emph[t] = 1.0 s and #emph[t] = 3.0 s? (e) What is the average velocity between #emph[t] = 1.0 s and #emph[t] = 2.0 s? #solutionbox[ a. #math.equation(block: false, alt: "v → open parenthesis t close parenthesis equals open parenthesis 6.0 t i ^ minus 21.0 t squared j ^ plus 10.0 t to the power −3 k ^ close parenthesis m/s")[$arrow(v) ( t ) = ( 6.0 t hat(i) − 21.0 t^(2) hat(j) + 10.0 t^(−3) hat(k) ) "m/s"$] #linebreak() b. #math.equation(block: false, alt: "a → open parenthesis t close parenthesis equals open parenthesis 6.0 i ^ minus 42.0 t j ^ minus 30 t to the power −4 k ^ close parenthesis m/ s squared")[$arrow(a) ( t ) = ( 6.0 hat(i) − 42.0 t hat(j) − 30 t^(−4) hat(k) ) "m/" "s"^(2)$] #linebreak() c. #math.equation(block: false, alt: "v → open parenthesis 2.0 s close parenthesis equals open parenthesis 12.0 i ^ minus 84.0 j ^ plus 1.25 k ^ close parenthesis m/s")[$arrow(v) ( 2.0 s ) = ( 12.0 hat(i) − 84.0 hat(j) + 1.25 hat(k) ) "m/s"$] #linebreak() d. #math.equation(block: false, alt: "v → open parenthesis 1.0 s close parenthesis equals 6.0 i ^ minus 21.0 j ^ plus 10.0 k ^ m/s , | v → open parenthesis 1.0 s close parenthesis | equals 24.0 m/s")[$arrow(v) ( 1.0 #h(0.2em) "s" ) = 6.0 hat(i) − 21.0 hat(j) + 10.0 hat(k) "m/s" , #h(0.2em) | arrow(v) ( 1.0 #h(0.2em) "s" ) | = 24.0 #h(0.2em) "m/s"$] #linebreak() #math.equation(block: false, alt: "v → open parenthesis 3.0 s close parenthesis equals 18.0 i ^ minus 189.0 j ^ plus 0.37 k ^ m/s ,")[$arrow(v) ( 3.0 #h(0.2em) "s" ) = 18.0 hat(i) − 189.0 hat(j) + 0.37 hat(k) "m/s" ,$], #math.equation(block: false, alt: "| v → open parenthesis 3.0 s close parenthesis | equals 190 m/s")[$| arrow(v) ( 3.0 #h(0.2em) "s" ) | = 190 #h(0.2em) "m/s"$] #linebreak() e. #math.equation(block: false, alt: "r → open parenthesis t close parenthesis equals open parenthesis 3.0 t squared i ^ minus 7.0 t cubed j ^ minus 5.0 t to the power −2 k ^ close parenthesis m")[$arrow(r) ( t ) = ( 3.0 t^(2) hat(i) − 7.0 t^(3) hat(j) − 5.0 t^(−2) hat(k) ) "m"$], #math.equation(block: false, alt: "v → sub avg equals 9.0 i ^ minus 49.0 j ^ plus 3.75 k ^ m/s")[$arrow(v)_("avg") = 9.0 hat(i) − 49.0 hat(j) + 3.75 hat(k) "m/s"$] ] The acceleration of a particle is a constant. At #emph[t] = 0 the velocity of the particle is #math.equation(block: false, alt: "open parenthesis 10 i ^ plus 20 j ^ close parenthesis m/s .")[$( 10 hat(i) + 20 hat(j) ) "m/s" .$] At #emph[t] = 4 s the velocity is #math.equation(block: false, alt: "10 j ^ m/s .")[$10 hat(j) "m/s" .$] (a) What is the particle’s acceleration? (b) How do the position and velocity vary with time? Assume the particle is initially at the origin. A particle has a position function #math.equation(block: false, alt: "r → open parenthesis t close parenthesis equals cos open parenthesis 1.0 t close parenthesis i ^ plus sin open parenthesis 1.0 t close parenthesis j ^ plus t k ^ ,")[$arrow(r) ( t ) = "cos" ( 1.0 t ) hat(i) + "sin" ( 1.0 t ) hat(j) + t hat(k) ,$] where the arguments of the cosine and sine functions are in radians. (a) What is the velocity vector? (b) What is the acceleration vector? #solutionbox[ a. #math.equation(block: false, alt: "v → open parenthesis t close parenthesis equals −sin open parenthesis 1.0 t close parenthesis i ^ plus cos open parenthesis 1.0 t close parenthesis j ^ plus k ^")[$arrow(v) ( t ) = "−sin" ( 1.0 t ) hat(i) + "cos" ( 1.0 t ) hat(j) + hat(k)$], b. #math.equation(block: false, alt: "a → open parenthesis t close parenthesis equals −cos open parenthesis 1.0 t close parenthesis i ^ minus sin open parenthesis 1.0 t close parenthesis j ^")[$arrow(a) ( t ) = "−cos" ( 1.0 t ) hat(i) − "sin" ( 1.0 t ) hat(j)$] ] A Lockheed Martin F-35 II Lighting jet takes off from an aircraft carrier with a runway length of 90 m and a takeoff speed 70 m/s at the end of the runway. Jets are catapulted into airspace from the deck of an aircraft carrier with two sources of propulsion: the jet propulsion and the catapult. At the point of leaving the deck of the aircraft carrier, the F-35’s acceleration decreases to a constant acceleration of #math.equation(block: false, alt: "5.0 m/ s squared")[$5.0 #h(0.2em) "m/" "s"^(2)$] at #math.equation(block: false, alt: "30 °")[$30 "°"$] with respect to the horizontal. (a) What is the initial acceleration of the F-35 on the deck of the aircraft carrier to make it airborne? (b) Write the position and velocity of the F-35 in unit vector notation from the point it leaves the deck of the aircraft carrier. (c) At what altitude is the fighter 5.0 s after it leaves the deck of the aircraft carrier? (d) What is its velocity and speed at this time? (e) How far has it traveled horizontally?