Hubbry Logo
Section formulaSection formulaMain
Open search
Section formula
Community hub
Section formula
logo
7 pages, 0 posts
0 subscribers
Be the first to start a discussion here.
Be the first to start a discussion here.
Section formula
Section formula
from Wikipedia

In coordinate geometry, the Section formula is a formula used to find the ratio in which a line segment is divided by a point internally or externally.[1] It is used to find out the centroid, incenter and excenters of a triangle. In physics, it is used to find the center of mass of systems, equilibrium points, etc.[2][3][4][5]

Internal divisions

[edit]
Internal division with section formula

If point P (lying on AB) divides the line segment AB joining the points and in the ratio m:n, then

[6]

The ratio m:n can also be written as , or , where . So, the coordinates of point dividing the line segment joining the points and are:

[4][5]

Similarly, the ratio can also be written as , and the coordinates of P are .[1]

Proof

[edit]

Triangles .

External divisions

[edit]
External division with section formula

If a point P (lying on the extension of AB) divides AB in the ratio m:n then

[6]

Proof

[edit]

Triangles (Let C and D be two points where A & P and B & P intersect respectively). Therefore ∠ACP = ∠BDP


Midpoint formula

[edit]

The midpoint of a line segment divides it internally in the ratio . Applying the Section formula for internal division:[4][5]

Derivation

[edit]

Centroid

[edit]
Centroid of a triangle

The centroid of a triangle is the intersection of the medians and divides each median in the ratio . Let the vertices of the triangle be , and . So, a median from point A will intersect BC at . Using the section formula, the centroid becomes:

In three dimensions

[edit]

Let A and B be two points with Cartesian coordinates (x1, y1, z1) and (x2, y2, z2) and P be a point on the line through A and B. If . Then the section formula gives the coordinates of P as

[1]

If, instead, P is a point on the line such that , its coordinates are .[1]

In vectors

[edit]

The position vector of a point P dividing the line segment joining the points A and B whose position vectors are and

  1. in the ratio internally, is given by [7][1]
  2. in the ratio externally, is given by [7]

See also

[edit]

References

[edit]
[edit]
Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
The section formula in coordinate geometry is a fundamental mathematical tool used to calculate the coordinates of a point that divides the joining two given points, either internally or externally, in a specified m:nm:n. This formula bridges algebraic expressions with geometric positions on a plane, enabling precise determination of point locations along a line. For internal division, where the point lies between the two endpoints A(x1,y1)A(x_1, y_1) and B(x2,y2)B(x_2, y_2), the coordinates of the dividing point PP are given by
P(mx2+nx1m+n,my2+ny1m+n).P\left( \frac{m x_2 + n x_1}{m + n}, \frac{m y_2 + n y_1}{m + n} \right). In contrast, for external division, where the point lies outside the segment, the coordinates are
P(mx2nx1mn,my2ny1mn),P\left( \frac{m x_2 - n x_1}{m - n}, \frac{m y_2 - n y_1}{m - n} \right), assuming mnm \neq n. A special case is the formula, derived when m:n=1:1m:n = 1:1, yielding P(x1+x22,y1+y22)P\left( \frac{x_1 + x_2}{2}, \frac{y_1 + y_2}{2} \right).
The section formula finds extensive applications in , such as computing centroids of triangles, verifying of points, and solving problems in vector geometry and for between coordinates. It also aids in determining the ratio in which a given point divides a , enhancing problem-solving in fields like physics for position vectors and for spatial calculations.

Two-dimensional geometry

Internal division

In coordinate geometry, internal division occurs when a point lies between the two endpoints of a and divides it in a specified m:nm:n, where mm and nn are indicating the proportional segments from the division point to each endpoint. This concept allows for the precise location of points along a based on weighted proportions, forming a foundational tool in for solving problems involving positions and intersections. The coordinates of the point PP that divides the joining points A(x1,y1)A(x_1, y_1) and B(x2,y2)B(x_2, y_2) internally in the m:nm:n are given by the section formula: P(nx1+mx2m+n,ny1+my2m+n).P\left( \frac{n x_1 + m x_2}{m + n}, \frac{n y_1 + m y_2}{m + n} \right). Here, the weights nn and mm reflect the relative distances, ensuring the point is positioned such that the segment from AA to PP is to the segment from PP to BB as m:nm:n. This formula arises directly from the principles of coordinate systems in the plane. To derive the formula, consider the parametric representation along the . The position of PP can be expressed as a weighted , where the coordinate is shifted from AA by a mm+n\frac{m}{m+n} of the total displacement to BB. For the x-coordinate: x=x1+mm+n(x2x1)=x1+mx2mx1m+n=(m+n)x1+mx2mx1m+n=nx1+mx2m+n.x = x_1 + \frac{m}{m + n} (x_2 - x_1) = x_1 + \frac{m x_2 - m x_1}{m + n} = \frac{(m + n) x_1 + m x_2 - m x_1}{m + n} = \frac{n x_1 + m x_2}{m + n}. The y-coordinate follows analogously: y=y1+mm+n(y2y1)=ny1+my2m+n.y = y_1 + \frac{m}{m + n} (y_2 - y_1) = \frac{n y_1 + m y_2}{m + n}. This derivation relies on the proportionality of distances in a straight line, confirming the through the uniform scaling of coordinates. A geometric proof using similar triangles reinforces this: construct horizontal lines from AA and PP to align with the y-level of BB, and vertical lines to form triangles whose similarity (by AA criterion, sharing angles and proportional sides) yields the same m:nm:n in both x- and y-directions, leading to the . For example, if A(1,2)A(1, 2) and B(3,4)B(3, 4) are divided internally in the 1:11:1, the coordinates of PP are (11+131+1,12+141+1)=(2,3)\left( \frac{1 \cdot 1 + 1 \cdot 3}{1 + 1}, \frac{1 \cdot 2 + 1 \cdot 4}{1 + 1} \right) = (2, 3), illustrating a balanced position. The origins of the section formula trace back to the development of by in his 1637 work , where coordinate methods enabled algebraic representation of geometric divisions; it gained prominence in 19th-century textbooks as a standard tool for plane geometry problems.

External division

External division refers to the case where a point divides the line segment joining two points in a given ratio but lies outside the segment, extending the line beyond one of the endpoints. In coordinate geometry, this occurs when the division ratio m:n results in the point P being positioned such that the directed segments satisfy AP:PB = m:n, but with P not between A and B. For points A(x₁, y₁) and B(x₂, y₂), the coordinates of the point P dividing AB externally in the ratio m:n are given by: P(nx1mx2nm,ny1my2nm)P\left( \frac{n x_1 - m x_2}{n - m}, \frac{n y_1 - m y_2}{n - m} \right) This formula can equivalently be written as (mx2nx1mn,my2ny1mn)\left( \frac{m x_2 - n x_1}{m - n}, \frac{m y_2 - n y_1}{m - n} \right), reflecting the sign convention for directed distances. The derivation of this formula relies on the geometry of similar triangles and the concept of directed segments. Consider points A(x₁, y₁) and B(x₂, y₂) on the plane, with P(x, y) dividing AB externally in ratio m:n. Drop perpendiculars from A, B, and P to the x-axis, meeting at points C, D, and M respectively, forming right triangles AMC and BND. Since P is external, the triangles ∆AMC and ∆BND are similar because their corresponding angles are equal (both right-angled, and sharing the angle with the line AB). The ratio of similarity is m:n, so the ratios of corresponding sides are equal: AMBN=mn\frac{AM}{BN} = \frac{m}{n}. Substituting the lengths, AM = |x - x₁| and BN = |x₂ - x|, but accounting for direction in external division (where P is beyond B, say), yields xx1x2x=mn\frac{x - x_1}{x_2 - x} = -\frac{m}{n} due to the opposite orientation. Solving xx1x2x=mn\frac{x - x_1}{x_2 - x} = -\frac{m}{n}: cross-multiplying gives n(xx1)=m(x2x)n(x - x_1) = -m (x_2 - x). Expanding, nxnx1=mx2+mxn x - n x_1 = -m x_2 + m x, then nxmx=nx1mx2n x - m x = n x_1 - m x_2, so x(nm)=nx1mx2x (n - m) = n x_1 - m x_2, hence x=nx1mx2nmx = \frac{n x_1 - m x_2}{n - m}. A similar process for the y-coordinates, using vertical distances, yields y=ny1my2nmy = \frac{n y_1 - m y_2}{n - m}. This proof emphasizes the opposite direction in external division compared to the internal case, where the ratio is positive without the sign flip. For example, consider points A(1, 2) and B(3, 4) divided externally in the 2:1 (m=2, n=1). The coordinates of P are (112312,122412)=(161,281)=(5,6)\left( \frac{1 \cdot 1 - 2 \cdot 3}{1 - 2}, \frac{1 \cdot 2 - 2 \cdot 4}{1 - 2} \right) = \left( \frac{1 - 6}{-1}, \frac{2 - 8}{-1} \right) = (5, 6). This point lies outside the segment AB, extended beyond B. The formula requires m ≠ n to avoid , which would occur if the ratio led to an indeterminate position; otherwise, the point would coincide with one endpoint or be undefined. This external counterpart to internal division finds applications in concepts like harmonic divisions, where points divide segments in specific negative ratios.

Midpoint formula

The midpoint of a line segment in two-dimensional coordinate geometry is defined as the point that divides the segment in the ratio 1:1, meaning it lies exactly halfway between the endpoints. This formula arises as a special case of the internal division section formula when the ratio m:n=1:1m:n = 1:1. For endpoints A(x1,y1)A(x_1, y_1) and B(x2,y2)B(x_2, y_2), the coordinates of the midpoint MM are given by M=(x1+x22,y1+y22).M = \left( \frac{x_1 + x_2}{2}, \frac{y_1 + y_2}{2} \right). This expression simplifies the general section formula by averaging the coordinates directly, reflecting equal partitioning. A proof of the midpoint formula can be derived using vector averaging in coordinate geometry. Consider the position vectors of points AA and BB as A=(x1,y1)\vec{A} = (x_1, y_1)
Add your contribution
Related Hubs
User Avatar
No comments yet.