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A circle has its centre at M(-2; 1) and passes through S(1; -2). Determine the coordinates of M and the radius of the circle. Determine the equation of the tangent RS.

Mathematics

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  1. Determine the coordinates of M and the radius of the circle (for 7.1)

    The equation of the circle with centre M is given as (x+2)2+(y−1)2=r2(x+2)^2 + (y-1)^2 = r^2.
    Comparing this to the standard form of a circle equation (x−a)2+(y−b)2=r2(x-a)^2 + (y-b)^2 = r^2, the coordinates of the centre M are (−2;1)(-2; 1).
    The point S(1;−2)(1; -2) lies on the circle. Substitute these coordinates into the equation to find r2r^2:

    (1+2)2+(−2−1)2=r2(1+2)^2 + (-2-1)^2 = r^2 (3)2+(−3)2=r2(3)^2 + (-3)^2 = r^2 9+9=r29 + 9 = r^2 r2=18r^2 = 18

    The radius r=18=9×2=32r = \sqrt{18} = \sqrt{9 \times 2} = 3\sqrt{2}.
    The coordinates of M are (−2;1)\boxed{(-2; 1)} and the radius is 32\boxed{3\sqrt{2}}.

  2. Determine the equation of the tangent RS (for 7.2)

    The tangent RS touches the circle at point S(1;−2)(1; -2). The radius MS is perpendicular to the tangent at S.
    First, calculate the gradient of the radius MS, mMSm_{MS}, using M(−2;1)(-2; 1) and S(1;−2)(1; -2):

    mMS=yS−yMxS−xM=−2−11−(−2)=−31+2=−33=−1m_{MS} = \frac{y_S - y_M}{x_S - x_M} = \frac{-2 - 1}{1 - (-2)} = \frac{-3}{1 + 2} = \frac{-3}{3} = -1

    Since the tangent RS is perpendicular to the radius MS, the gradient of the tangent, mRSm_{RS}, is the negative reciprocal of mMSm_{MS}:

    mRS=−1mMS=−1−1=1m_{RS} = -\frac{1}{m_{MS}} = -\frac{1}{-1} = 1

    Now, use the point-slope form of a linear equation, y−y1=m(x−x1)y - y_1 = m(x - x_1), with point S(1;−2)(1; -2) and mRS=1m_{RS} = 1:

    y−(−2)=1(x−1)y - (-2) = 1(x - 1) y+2=x−1y + 2 = x - 1 y=x−1−2y = x - 1 - 2

    The equation of the tangent RS is y=x−3\boxed{y = x - 3}.

  3. Determine the coordinates of point P (for 7.3)

    The circles with centres P and M touch externally at point S. This means S lies on the line segment MP.
    We are given the ratio MS : MP = 1 : 3.
    This implies that the distance from M to S is one-third of the distance from M to P.
    Let M be (−2;1)(-2; 1) and S be (1;−2)(1; -2). Let P be (a;b)(a; b).
    We can use the section formula or vector approach. Using the vector approach:
    The vector MS⃗\vec{MS} represents the displacement from M to S:

    MS⃗=(xS−xM,yS−yM)=(1−(−2),−2−1)=(3,−3)\vec{MS} = (x_S - x_M, y_S - y_M) = (1 - (-2), -2 - 1) = (3, -3)

    Since MS : MP = 1 : 3, the vector MP⃗\vec{MP} is 3 times the vector MS⃗\vec{MS}:

    MP⃗=3×MS⃗=3(3,−3)=(9,−9)\vec{MP} = 3 \times \vec{MS} = 3(3, -3) = (9, -9)

    The vector MP⃗\vec{MP} also represents the displacement from M to P:

    MP⃗=(xP−xM,yP−yM)=(a−(−2),b−1)=(a+2,b−1)\vec{MP} = (x_P - x_M, y_P - y_M) = (a - (-2), b - 1) = (a+2, b-1)

    Equating the components of MP⃗\vec{MP}:

    a+2=9  ⟹  a=7a+2 = 9 \implies a = 7 b−1=−9  ⟹  b=−8b-1 = -9 \implies b = -8

    The coordinates of point P are (7;−8)\boxed{(7; -8)}.

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