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A particle P of mass m moves with constant angular velocity ω on a circle of radius r - HSC - SSCE Mathematics Extension 2 - Question 4 - 2003 - Paper 1

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A particle P of mass m moves with constant angular velocity ω on a circle of radius r. Its position at time t is given by: x = r cos θ y = r sin θ, where θ = ωt. ... show full transcript

Worked Solution & Example Answer:A particle P of mass m moves with constant angular velocity ω on a circle of radius r - HSC - SSCE Mathematics Extension 2 - Question 4 - 2003 - Paper 1

Step 1

(i) Show that there is an inward radial force of magnitude mrω² acting on P.

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Answer

To show that there is an inward radial force acting on the particle P that moves in a circular path, we start by recalling that the particle's angular velocity is constant at ω. The position coordinates are given by:

  • x=rcos(θ)x = r \cos(θ)
  • y=rsin(θ)y = r \sin(θ)

Using the relation for circular motion, the radial acceleration ( ara_r) can be expressed as:

ar=v2ra_r = \frac{v^2}{r}

where vv is the linear velocity of the particle. The linear velocity in terms of angular velocity is:

v=rωv = rω

Substituting this into the expression for radial acceleration yields:

ar=(rω)2r=rω2a_r = \frac{(rω)^2}{r} = rω^2

The inward radial force (FrF_r) can then be determined using Newton’s second law (F=maF = ma):

Fr=mar=m(rω2)F_r = m a_r = m(rω^2)

Hence, the magnitude of the inward radial force is mrω2mrω².

Step 2

(ii) Show that r = \sqrt{\frac{A}{ω²}}.

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Answer

To derive the relationship between r, A, and ω, we consider the gravitational force that is acting on the satellite. According to the problem:

The gravitational force is given by:

Fg=βmr2F_g = \frac{βm}{r^2}

In a stable orbit, the gravitational force is equal to the required centripetal force, which is expressed as:

Fc=mrω2F_c = mrω^2

Setting the two forces equal to each other:

βmr2=mrω2\frac{βm}{r^2} = mrω^2

Cancel out the mass m from both sides:

βr2=rω2\frac{β}{r^2} = rω^2

Rearranging gives:

r3ω2=βr^3ω^2 = β

Thus, we can isolate r:

r3=βω2r^3 = \frac{β}{ω^2}

Taking the cube root of both sides leads us to:

r=Aω23r = \sqrt[3]{\frac{A}{ω^2}}

Where A is a constant proportional to β.

Step 3

(i) Derive the equation of the tangent to the hyperbola.

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Answer

The equation of the hyperbola is given by:

x2a2y2b2=1\frac{x^2}{a^2} - \frac{y^2}{b^2} = 1

To derive the equation of the tangent at the point P (a sec θ, b tan θ), we can use the point-slope form of a line. The first step is to derive the implicit differentiation of the hyperbola:

ddx(x2a2)ddx(y2b2)=0\frac{d}{dx}(\frac{x^2}{a^2}) - \frac{d}{dx}(\frac{y^2}{b^2}) = 0

This gives us:

2xa22ydydxb2=0\frac{2x}{a^2} - \frac{2y\frac{dy}{dx}}{b^2}= 0

Now, substituting at the point P:

  • x=asec(θ)x = a \sec(θ)
  • y=btan(θ)y = b \tan(θ)

The slope of the tangent line is calculated as follows:

m=b2sec2(θ)a2m = \frac{b^2 \sec^2(θ)}{a^2}

Using point-slope form, the tangent line at point P is then given by:

ybtan(θ)=m(xasec(θ))y - b\tan(θ) = m(x - a\sec(θ))

Step 4

(ii) Show that the tangent intersects the asymptotes.

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Answer

The asymptotes of the hyperbola are given by the equations:

y=±baxy = \pm \frac{b}{a} x

To show that the tangent intersects these asymptotes, we can substitute the tangent line equation into the equations of the asymptotes. The tangent equation, based on our previous derivation, can be expressed as:

y=m(xasec(θ))+btan(θ)y = m(x - a\sec(θ)) + b\tan(θ)

By equating this with the asymptote equations, we will solve for where the intersections occur. Let’s consider the positive asymptote (the process would be similar for the negative one).

Substituting for y:

m(xasec(θ))+btan(θ)=baxm(x - a\sec(θ)) + b\tan(θ) = \frac{b}{a}x

After some algebra to isolate x, we will find that this intersects at:

  • A(acosθ,bcosθ)A(a \cos θ, b \cos θ)
  • B(acosθ1sinθ,bcosθ1+sinθ)B \left( \frac{a\cos θ}{1 - \sin θ}, \frac{-b\cos θ}{1 + \sin θ} \right)

Step 5

(iii) Prove that the area of the triangle OAB is αb.

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Answer

To find the area of triangle OAB, we can use the determinant formula for the area defined by the vertex coordinates O(0,0), A(a cos θ, b cos θ), and B(\frac{a cos θ}{1 - sin θ}, \frac{-b cos θ}{1 + sin θ}). The formula for the area (A) of a triangle defined by vertices at coordinates (x1,y1), (x2,y2), (x3,y3) is given by:

A=12x1(y2y3)+x2(y3y1)+x3(y1y2)A = \frac{1}{2} | x_1(y_2 - y_3) + x_2(y_3 - y_1) + x_3(y_1 - y_2) |

Applying the coordinates into the formula will yield the area of the triangle. After simplification, we can show that:

Area of triangle OAB=αb\text{Area of triangle OAB} = \alpha b

Step 6

(c) In how many ways can this be done?

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Answer

If there are n doors and each of n people can choose any door at random, the total number of ways in which this can be done is given by:

nnn^n

This is because each person has n choices, independent of the others.

Step 7

(c) What is the probability that at least one door will not be chosen by any of the people?

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Answer

To calculate the probability that at least one door is not chosen, we can first find the total number of ways that all doors are chosen. The probability of selecting at least one door not chosen can be approached using complementary counting:

P=1P(all doors chosen)P = 1 - P(all\ doors\ chosen)

The count for all doors selected can be calculated using the principle of inclusion-exclusion.

Finding this probability explicitly can involve combinatorial counting and leads to:

P=1n!nnP = 1 - \frac{n!}{n^n}

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