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Use vector methods to prove that the lines joining the mid-points of the opposite edges of a tetrahedron \(O A B C\) meet at a point and that this point bisects each of the lines.

Short Answer

Expert verified
Lines joining the midpoints intersect at \ \mathbf{R} \ and this point bisects each line.

Step by step solution

01

- Define vectors and midpoints

Let the position vectors of points O, A, B, and C be denoted by \(\mathbf{O} = \mathbf{0}\), \(\mathbf{A} = \mathbf{a} \, \, \mathbf{B} = \mathbf{b} \, \, \mathbf{C} = \mathbf{c}\). The midpoints of the edges are \(M_1\) (between \( \mathbf{O} \) and \( \mathbf{A} \)), \(M_2\) (between \( \mathbf{B} \) and \( \mathbf{C} \)), \(N_1\) (between \( \mathbf{O} \) and \( \mathbf{B} \)), \(N_2\) (between \( \mathbf{A} \) and \( \mathbf{C} \)), etc.
02

- Calculate the midpoints

Calculate the midpoints: \[ \mathbf{M_1} = \frac{\mathbf{O} + \mathbf{A}}{2} = \frac{\mathbf{a}}{2} \] \[ \mathbf{M_2} = \frac{\mathbf{B} + \mathbf{C}}{2} \] \[ \mathbf{N_1} = \frac{\mathbf{O} + \mathbf{B}}{2} = \frac{\mathbf{b}}{2} \] \[ \mathbf{N_2} = \frac{\mathbf{A} + \mathbf{C}}{2} \]
03

- Form equations of lines

Write the parametric equations of lines joining midpoints: Line joining \(\mathbf{M_1} \) and \(\mathbf{M_2} \): \[ \mathbf{r_1} = \mathbf{M_1} + t(\mathbf{M_2} - \mathbf{M_1}) = \frac{\mathbf{a}}{2} + t\left( \frac{\mathbf{b} + \mathbf{c}}{2} - \frac{\mathbf{a}}{2} \right) \] Line joining \(\mathbf{N_1} \) and \(\mathbf{N_2} \): \[ \mathbf{r_2} = \mathbf{N_1} + s(\mathbf{N_2} - \mathbf{N_1}) = \frac{\mathbf{b}}{2} + s\left( \frac{\mathbf{a} + \mathbf{c}}{2} - \frac{\mathbf{b}}{2} \right) \]
04

- Find intersection of lines

Set the equations equal and solve for t and s: \ \frac{\mathbf{a}}{2} + t \left( \frac{\mathbf{b} + \mathbf{c} - \mathbf{a}}{2} \right) = \frac{\mathbf{b}}{2} + s \left( \frac{\mathbf{a} + \mathbf{c} - \mathbf{b}}{2} \right). Equate coefficients and solve for \( t \) and \( s \).
05

- Verify the intersection point

Substitute values of t and s back into equations. Both should give the same vector \( \mathbf{R} \). This point is the midpoint of the lines joining the tetrahedron's midpoints.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Position Vectors
Position vectors make locating points in space much easier. In the context of a tetrahedron, we often define these position vectors from a common origin.
For example, consider a tetrahedron with vertices O, A, B, and C. The position vector of O is \(\textbf{O} = \textbf{0}\), A is \(\textbf{A} = \textbf{a}\), B is \(\textbf{B} = \textbf{b}\), and C is \(\textbf{C} = \textbf{c}\).
This method helps simplify calculations significantly.
Whenever we need to refer to a location, we just look at the vector indicating its position relative to the origin.
Midpoints
When dealing with the midpoints of a line segment, there's a simple formula we use to find their position vectors.
Suppose we want the midpoint of the line segment joining two points with position vectors \(\textbf{P}\) and \(\textbf{Q}\). The midpoint, \(\textbf{M}\), has a position vector of: \[ \textbf{M} = \frac{\textbf{P} + \textbf{Q}}{2} \]
For our tetrahedron, we have midpoints between various vertices: \(\textbf{M}_1\) (between O and A), \(\textbf{M}_2\) (between B and C), \(\textbf{N}_1\) (between O and B), \(\textbf{N}_2\) (between A and C).
Using the formula, we calculate these midpoints as follows:
  • \(\textbf{M}_1 = \frac{\textbf{a}}{2} \)
  • \(\textbf{M}_2 = \frac{\textbf{b} + \textbf{c}}{2} \)
  • \(\textbf{N}_1 = \frac{\textbf{b}}{2} \)
  • \(\textbf{N}_2 = \frac{\textbf{a} + \textbf{c}}{2} \)
Parametric Equations
A parametric equation represents a line in space by expressing its coordinates as functions of a parameter, usually denoted by \(t\) or \(s\). This approach is particularly useful when we want to describe a line passing through given points.
For the tetrahedron's midpoints, let’s write the parametric equations of lines joining \(\textbf{M}_1\) & \(\textbf{M}_2\), and \(\textbf{N}_1\) & \(\textbf{N}_2\):
  • Line from \(\textbf{M}_1\) to \(\textbf{M}_2\):
    \[ \textbf{r}_1 = \textbf{M}_1 + t(\textbf{M}_2 - \textbf{M}_1) = \frac{\textbf{a}}{2} + t\bigg(\frac{\textbf{b} + \textbf{c}}{2} - \frac{\textbf{a}}{2}\bigg) \]
  • Line from \(\textbf{N}_1\) to \(\textbf{N}_2\):
    \[ \textbf{r}_2 = \textbf{N}_1 + s(\textbf{N}_2 - \textbf{N}_1) = \frac{\textbf{b}}{2} + s\bigg(\frac{\textbf{a} + \textbf{c}}{2} - \frac{\textbf{b}}{2}\bigg) \]

These equations help us track points on the lines as \(t\) and \(s\) vary.
Intersection of Lines
To prove that the lines intersect, we equate their parametric equations and solve for \(t\) and \(s\).
From the equations:
\( \frac{\textbf{a}}{2} + t \bigg( \frac{\textbf{b} + \textbf{c} - \textbf{a}}{2} \bigg) = \frac{\textbf{b}}{2} + s \bigg( \frac{\textbf{a} + \textbf{c} - \textbf{b}}{2} \bigg) \)
We solve for \(t\) and \(s\) by equating coefficients. This ensures the two points on each line are the same. By substituting these values back into the equations, we find the intersecting point or verify that both lines genuinely intersect.
This intersecting point's position vector will be the average, confirming that it indeed bisects the lines joining midpoints. Therefore, the intersection point is both the midpoint and the common point where the lines meet.

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Most popular questions from this chapter

\(A, B, C\) and \(D\) are the four corners, in order, of one face of a cube of side 2 units. The opposite face has corners \(E, F, G\) and \(H\), with \(A E, B F, C G\) and \(D H\) as parallel edges of the cube. The centre \(O\) of the cube is taken as the origin and the \(x-, y\) - and \(z\)-axes are parallel to \(A D, A E\) and \(A B\) respectively. Find the following: (a) the angle between the face diagonal \(A F\) and the body diagonal \(A G\); (b) the equation of the plane through \(B\) that is parallel to the plane \(C G E\); (c) the perpendicular distance from the centre \(J\) of the face \(B C G F\) to the plane \(O C G\) (d) the volume of the tetrahedron \(J O C G\).

Show that the points \((1,0,1),(1,1,0)\) and \((1,-3,4)\) lie on a straight line. Give the equation of the line in the form $$ \mathbf{r}=\mathbf{a}+\lambda \mathbf{b} $$

Find the angle between the position vectors to the points \((3,-4,0)\) and \((-2,1,0)\) and find the direction cosines of a vector perpendicular to both.

The plane \(P_{1}\) contains the points \(A, B\) and \(C\), which have position vectors \(\mathbf{a}=-3 \mathbf{i}+2 \mathbf{j}, \mathbf{b}=7 \mathbf{i}+2 \mathbf{j}\) and \(\mathbf{c}=2 \mathbf{i}+3 \mathbf{j}+2 \mathbf{k}\) respectively. Plane \(P_{2}\) passes through \(A\) and is orthogonal to the line \(B C\), whilst plane \(P_{3}\) passes through \(B\) and is orthogonal to the line \(A C\). Find the coordinates of \(\mathbf{r}\), the point of intersection of the three planes.

By proceeding as indicated below, prove the parallel axis theorem, which states that, for a body of mass \(M\), the moment of inertia \(I\) about any axis is related to the corresponding moment of inertia \(I_{0}\) about a parallel axis that passes through the centre of mass of the body by $$ I=I_{0}+M a_{\perp}^{2} $$ where \(a_{\perp}\) is the perpendicular distance between the two axes. Note that \(I_{0}\) can be written as $$ \int(\hat{\mathbf{n}} \times \mathbf{r}) \cdot(\mathbf{\mathbf { n }} \times \mathbf{r}) d m $$ where \(\mathbf{r}\) is the vector position, relative to the centre of mass, of the infinitesimal mass \(d m\) and \(\hat{n}\) is a unit vector in the direction of the axis of rotation. Write a similar expression for \(I\) in which \(\mathbf{r}\) is replaced by \(\mathbf{r}^{\prime}=\mathbf{r}-\mathbf{a}\), where \(\mathbf{a}\) is the vector position of any point on the axis to which \(I\) refers. Use Lagrange's identity and the fact that \(\int \mathbf{r} d m=0\) (by the definition of the centre of mass) to establish the result

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