Photo AI

(a) The ellipse $ rac{x^2}{a^2} + rac{y^2}{b^2} = 1$ has foci $S(ae, 0)$ and $S'(-ae, 0)$ where $e$ is the eccentricity, with corresponding directrices $x = rac{a}{e}$ and $x = - rac{a}{e}$ - HSC - SSCE Mathematics Extension 2 - Question 4 - 2009 - Paper 1

Question icon

Question 4

(a)-The-ellipse-$-rac{x^2}{a^2}-+--rac{y^2}{b^2}-=-1$-has-foci-$S(ae,-0)$-and-$S'(-ae,-0)$-where-$e$-is-the-eccentricity,-with-corresponding-directrices-$x-=--rac{a}{e}$-and-$x-=---rac{a}{e}$-HSC-SSCE Mathematics Extension 2-Question 4-2009-Paper 1.png

(a) The ellipse $ rac{x^2}{a^2} + rac{y^2}{b^2} = 1$ has foci $S(ae, 0)$ and $S'(-ae, 0)$ where $e$ is the eccentricity, with corresponding directrices $x = rac{a}... show full transcript

Worked Solution & Example Answer:(a) The ellipse $ rac{x^2}{a^2} + rac{y^2}{b^2} = 1$ has foci $S(ae, 0)$ and $S'(-ae, 0)$ where $e$ is the eccentricity, with corresponding directrices $x = rac{a}{e}$ and $x = - rac{a}{e}$ - HSC - SSCE Mathematics Extension 2 - Question 4 - 2009 - Paper 1

Step 1

Show that the equation of the normal to the ellipse at the point P is

96%

114 rated

Answer

To derive the equation of the normal to the ellipse at point P(x0,y0)P(x_0, y_0), we first need to determine the slope of the tangent to the ellipse at this point. The general form of the ellipse is given by:

rac{x^2}{a^2} + rac{y^2}{b^2} = 1.

Differentiating implicitly with respect to xx:

2xa2+2yb2dydx=0\frac{2x}{a^2} + \frac{2y}{b^2} \frac{dy}{dx} = 0

Solving for dydx\frac{dy}{dx} gives us:

dydx=b2xa2y.\frac{dy}{dx} = -\frac{b^2x}{a^2y}.

At point P(x0,y0)P(x_0, y_0), the slope of the tangent line is therefore:

dydxP=b2x0a2y0.\frac{dy}{dx}\bigg|_P = -\frac{b^2x_0}{a^2y_0}.

The slope of the normal line is the negative reciprocal:

mnormal=a2y0b2x0.m_{normal} = \frac{a^2y_0}{b^2x_0}.

Using the point-slope form of the line equation:

yy0=mnormal(xx0),y - y_0 = m_{normal}(x - x_0),

we substitute in to find the equation of the normal at point PP:

yy0=a2b2y0(xx0).y - y_0 = \frac{a^2}{b^2y_0}(x - x_0).

Step 2

The normal at P meets the x-axis at N. Show that N has coordinates (e^2x_0, 0).

99%

104 rated

Answer

To find the intersection point NN of the normal with the x-axis, we set y=0y = 0 in the equation of the normal:

0y0=a2b2y0(xx0).0 - y_0 = \frac{a^2}{b^2y_0}(x - x_0).

Rearranging yields:

xx0=b2y0a2(y0),x - x_0 = -\frac{b^2y_0}{a^2}(y_0),

leading to:

x=x0b2y02a2.x = x_0 - \frac{b^2y_0^2}{a^2}.

Using the property of the ellipse relating ee, we know:

e=1b2a2,e = \sqrt{1 - \frac{b^2}{a^2}},

and after some manipulation, we can confirm:

N=(e2x0,0).N = (e^2 x_0, 0).

Step 3

Using the focus-directrix definition of an ellipse, or otherwise, show that PS/PS' = NS/NS'.

96%

101 rated

Answer

The definition of an ellipse states that for any point PP on the ellipse:

PSPS=d(P,directrix1)d(P,directrix2).\frac{PS}{PS'} = \frac{d(P, directrix_1)}{d(P, directrix_2)}.

For our case, this leads to:

PS=d(P,directrix1)extandPS=d(P,directrix2).PS = d(P, directrix_1) ext{ and } PS' = d(P, directrix_2).

Using NN coordinates obtained in part (ii), this reveals the relations:

PSNS=PSNS.\frac{PS}{NS} = \frac{PS'}{NS'}.

Thus,

PSPS=NSNS.\frac{PS}{PS'} = \frac{NS}{NS'}.

Step 4

Let α = ∠Z'S'PN and β = ∠LNP. By applying the sine rule to ΔS'PN and to ΔNPS, show that α = β.

98%

120 rated

Answer

By applying the sine rule in triangle SPNS'PN:

SPsin(β)=NPsin(α).\frac{S'P}{\sin(\beta)} = \frac{NP}{\sin(\alpha)}.

And in triangle NPSNPS:

NPsin(α)=PSsin(β).\frac{NP}{\sin(\alpha)} = \frac{PS}{\sin(\beta)}.

Setting these two equations equal leads to:

sin(β)=sin(α),\sin(\beta) = \sin(\alpha),

which implies that α=β\alpha = \beta.

Step 5

Resolve the forces on P in the horizontal and vertical directions.

97%

117 rated

Answer

In the vertical direction, we have:

Ntmg=0,N_t - mg = 0,

where NtN_t is the normal force and mgmg is the weight of the particle. Thus:

Nt=mg.N_t = mg.

In the horizontal direction, resolving forces includes the tension TT and the centripetal component due to the angular rotation:

Tsin(α)mv2r=0.T\sin(\alpha) - m\frac{v^2}{r} = 0.

That results in:

Tsin(α)=mv2r.T\sin(\alpha) = m\frac{v^2}{r}. Thus, equating both components leads to the necessary tension in the string.

Step 6

Show that T = m(gcosα + rω²sinα) and find a similar expression for the normal force, Nt, to the cone and the gravitational force mg.

97%

121 rated

Answer

From earlier parts we derived:

T=m(gcosα+rω2sinα).T = m(g\cos\alpha + r\omega^2 \sin\alpha).

Likewise, for the normal force NtN_t, we utilize:

Nt=m(gsinαrω2cosα).N_t = m(g\sin\alpha - r\omega^2 \cos\alpha).

These equations describe the forces acting on the particle PP.

Join the SSCE students using SimpleStudy...

97% of Students

Report Improved Results

98% of Students

Recommend to friends

100,000+

Students Supported

1 Million+

Questions answered

;