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Advanced Mathematics 2

The Ellipse

takriban dakika 17 kusoma

Mada za sehemu hiiCoordinate Geomrtry 2Mada 6

The ellipse is a conic section defined as the locus of a point that moves such that the ratio of its distance from a fixed point (focus) to its distance from a fixed line (directrix) is constant. It can also be defined as the locus of points such that the sum of the distances from any point to the two foci is constant. This constant is equal to 2a2a, where aa is the semi-major axis. The eccentricity of an ellipse is less than 1.

The standard equation of an ellipse

Figure below represents an ellipse with foci F1F_1 and F2F_2, moving point PP, and directrix x=dx = d.

Ellipse with foci F1 and F2, moving point P, and directrix x = d

From the definition, PF1/PQ=ePF_1 / PQ = e. Also, PF1+PF2=2aPF_1 + PF_2 = 2a.

Derivation from PF1+PF2=2aPF_1 + PF_2 = 2a:

PF1=(xc)2+y2PF_1 = \sqrt{(x - c)^2 + y^2}

PF2=(x+c)2+y2PF_2 = \sqrt{(x + c)^2 + y^2}

Substituting into PF1+PF2=2aPF_1 + PF_2 = 2a:

(xc)2+y2+(x+c)2+y2=2a\sqrt{(x - c)^2 + y^2} + \sqrt{(x + c)^2 + y^2} = 2a

Rearranging:

(xc)2+y2=2a(x+c)2+y2\sqrt{(x - c)^2 + y^2} = 2a - \sqrt{(x + c)^2 + y^2}

Squaring both sides:

(xc)2+y2=4a24a(x+c)2+y2+(x+c)2+y2(x - c)^2 + y^2 = 4a^2 - 4a\sqrt{(x + c)^2 + y^2} + (x + c)^2 + y^2

x22xc+c2+y2=4a24a(x+c)2+y2+x2+2xc+c2+y2x^2 - 2xc + c^2 + y^2 = 4a^2 - 4a\sqrt{(x + c)^2 + y^2} + x^2 + 2xc + c^2 + y^2

4xc4a2=4a(x+c)2+y2-4xc - 4a^2 = -4a\sqrt{(x + c)^2 + y^2}

xc+a2=a(x+c)2+y2xc + a^2 = a\sqrt{(x + c)^2 + y^2}

Squaring both sides again:

x2c2+2a2xc+a4=a2(x2+2xc+c2+y2)x^2c^2 + 2a^2xc + a^4 = a^2(x^2 + 2xc + c^2 + y^2)

x2c2+2a2xc+a4=a2x2+2a2xc+a2c2+a2y2x^2c^2 + 2a^2xc + a^4 = a^2x^2 + 2a^2xc + a^2c^2 + a^2y^2

a4a2c2=a2x2x2c2+a2y2a^4 - a^2c^2 = a^2x^2 - x^2c^2 + a^2y^2

a2(a2c2)=x2(a2c2)+a2y2a^2(a^2 - c^2) = x^2(a^2 - c^2) + a^2y^2

Let b2=a2c2b^2 = a^2 - c^2:

a2b2=x2b2+a2y2a^2b^2 = x^2b^2 + a^2y^2

Dividing by a2b2a^2b^2:

x2a2+y2b2=1\frac{x^2}{a^2} + \frac{y^2}{b^2} = 1

From the right-angled triangle formed by OF1OF_1, OBOB, and BF1BF_1, using Pythagoras' theorem:

OF12+OB2=BF12OF_1^2 + OB^2 = BF_1^2

c2+b2=a2c^2 + b^2 = a^2

b2=a2c2b^2 = a^2 - c^2

From the definition using directrix and focus: FV1=eV1RFV_1 = eV_1R, where FV1=acFV_1 = a - c and V1R=daV_1R = d - a so ac=e(da)a - c = e(d - a). Similarly, FV2=a+cFV_2 = a + c and V2R=d+aV_2R = d + a so a+c=e(d+a)a + c = e(d + a).

Solving these gives d=a/ed = a/e and c=aec = ae.

The foci are (±ae,0)(\pm ae, 0) and the directrices are x=±aex = \pm \frac{a}{e}.

If a>ba > b, then b2=a2(1e2)b^2 = a^2(1 - e^2) or c2=a2e2=a2b2c^2 = a^2e^2 = a^2 - b^2 with foci (±ae,0)(\pm ae, 0), directrices x=±aex = \pm \frac{a}{e}, and vertices (±a,0)(\pm a, 0). The lengths of the major and minor axes are 2a2a and 2b2b, respectively.

If b>ab > a, then a2=b2(1e2)a^2 = b^2(1 - e^2) or c2=b2e2=b2a2c^2 = b^2e^2 = b^2 - a^2 with foci (0,±be)(0, \pm be), directrices y=±bey = \pm \frac{b}{e}, and vertices (0,±b)(0, \pm b). The lengths of the major and minor axes are 2b2b and 2a2a, respectively.

Example 1

Given the equation 4x2+9y2=364x^2 + 9y^2 = 36, find:

  1. Lengths of the major and minor axes.
  2. Coordinates of the foci.
  3. Equations of the directrices.
  4. Coordinates of the vertices.

Solution:

Standard form: x29+y24=1\frac{x^2}{9} + \frac{y^2}{4} = 1. Here, a=3a = 3 and b=2b = 2. Since a>ba > b, the major axis is along the x-axis.

  1. Major axis: 2a=62a = 6; Minor axis: 2b=42b = 4
  2. c2=a2b2=94=5c^2 = a^2 - b^2 = 9 - 4 = 5, so c=5c = \sqrt{5}. Foci: (±5,0)(\pm \sqrt{5}, 0)
  3. e=ca=53e = \frac{c}{a} = \frac{\sqrt{5}}{3}. Directrices: x=±ae=±95=±955x = \pm \frac{a}{e} = \pm \frac{9}{\sqrt{5}} = \pm \frac{9\sqrt{5}}{5}
  4. Vertices: (±3,0)(\pm 3, 0)

Example 2

An ellipse is defined by 9x2+4y2=1449x^2 + 4y^2 = 144. Find:

  1. The coordinates of the foci.
  2. The lengths of the major and minor axes.
  3. The equations of the directrices.
  4. The coordinates of the vertices.

Solution:

Standard form: x216+y236=1\frac{x^2}{16} + \frac{y^2}{36} = 1. Here, a=4a = 4 and b=6b = 6. Since b>ab > a, the major axis is along the y-axis.

  1. c2=b2a2=3616=20c^2 = b^2 - a^2 = 36 - 16 = 20, so c=25c = 2\sqrt{5}. Foci: (0,±25)(0, \pm 2\sqrt{5})
  2. Major axis: 2b=122b = 12; Minor axis: 2a=82a = 8
  3. e=cb=256=53e = \frac{c}{b} = \frac{2\sqrt{5}}{6} = \frac{\sqrt{5}}{3}. Directrices: y=±be=±185=±1855y = \pm \frac{b}{e} = \pm \frac{18}{\sqrt{5}} = \pm \frac{18\sqrt{5}}{5}
  4. Vertices: (0,±6)(0, \pm 6)

Example 3

Astronomers have revealed that planets revolve around the sun in an elliptical orbit and that the sun is always at one of the foci of the elliptical orbit. Pluto is said to be the farthest from the sun with an eccentricity of 0.248. Astronomers have also revealed that Pluto's orbit is at a distance about 30 Astronomical Unit (AU) from the sun at its closest point to the sun (perihelion). The length of its major axis is about 79 AU.

  1. Sketch the Pluto's orbit showing the position of the sun. (See Diagram: Sketch of Pluto's orbit)
  2. Find the length of the semi-minor axis of the orbit.
  3. Find the distance of Pluto from the sun at its farthest point (aphelion).

Solution:

a. (See Diagram: Sketch of Pluto's orbit)

b. The length of the major axis is 2a=792a = 79 AU, so a=39.5a = 39.5 AU.

The distance at perihelion is ac=30a - c = 30 AU. Since c=aec = ae, we have aae=30a - ae = 30.

39.539.5(0.248)=3039.5 - 39.5(0.248) = 30

39.59.8=29.730 (This confirms the given data).39.5 - 9.8 = 29.7 \approx 30 \text{ (This confirms the given data).}

Now, we use b2=a2c2b^2 = a^2 - c^2:

c=ae=39.5×0.248=9.7969.8 AUc = ae = 39.5 \times 0.248 = 9.796 \approx 9.8 \text{ AU}

b2=(39.5)2(9.8)2=1560.2596.04=1464.21b^2 = (39.5)^2 - (9.8)^2 = 1560.25 - 96.04 = 1464.21

b=1464.2138.3 AUb = \sqrt{1464.21} \approx 38.3 \text{ AU}

The length of the semi-minor axis is approximately 38.3 AU.

c. The distance at aphelion is a+c=39.5+9.8=49.3a + c = 39.5 + 9.8 = 49.3 AU

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