In this video, I demonstrate how to use the Law of Cosines to find an unknown long side of a scalene triangle, given an angle and adjacent 2 shorter sides.
The triangle has been constructed from 2 shorter sides of lengths 2.0m and 3.0m, subtended by an angle of 135°. We are required to find the length of the longest side - and we can do that by using the Cosine Rule (aka Law of Cosines) which states...
c^2 = a^2 + b^2 - 2ab\cos \theta
where c is the longest side and θ is the angle between the 2 shorter sides a and b.
The equation of an ellipse that is offset from (0,0) is very similar to the standard form, except that the centre coordinates (p,q) are subtracted from the variables x and y respectively. That is...
Here, a and b still are the lengths of the semi-major and semi-minor axes respectively.
For an ellipse with a given semi-major and semi-minor axis, the shape and every other feature remains the same as one located at (0,0), except all features have been offset by the centre point coordinates (p, q). That is...
The centre is located at: (p,q) rather than (0,0)
The foci are located at: (±ae+p , q) rather than (±ae , 0)
The horizontal vertices are located at: (±a+p , q) rather than (±a , 0)
The vertical vertices are located at: (±p, b+q) rather than (0 , ±b)
The directrices have the equations: x = ±(a/e)+p rather than x = ±a/e
In this video, we also sketch the ellipse formed by the equation:
9x^2 + 36x + 16y^2 + 96y = -36
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In this lesson, we find the equation of an ellipse given it has vertices or x-intercepts of (8,0) and (-8,0) and focal points (5,0) and (-5,0).
The standard form of the ellipse is:
\frac{x^2}{a^2} + \frac{y^2}{b^2} = 1
And the x-intercepts are given by:
(\pm a,0)
which means that a = 8.
For the term b2, it can be expressed as...
b^2 = a^2 - (ae)^2
where a is the length of the semi-major axis, e is the eccentricity, ae is the distance from the centre of the ellipse to a focal point. So in this case, we have...
ae = 5
Thus
b^2 = 8^2 - 5^2 = 64 - 25 = 39
So the equation of the ellipse is...
\frac{x^2}{64} + \frac{y^2}{39} = 1
or...
39x^2 + 64y^2 = 2496
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4x2 + 9y2 = 36 is the equation of an ellipse centred at the origin (0,0). Before we can sketch the ellipse, we need to find the vertices (i.e. the x and y intercepts) by transforming the equation to the standard form, which is:
\frac{x^2}{a^2} + \frac{y^2}{b^2} = 1
where...
a is the semi-major axis b is the semi-minor axis
So, dividing the equation by 36, we get:
\frac{x^2}{9} + \frac{y^2}{4} = 1
Or...
\frac{x^2}{3^2} + \frac{y^2}{2^2} = 1
Thus a = 3 and b = 2, and hence the vertices are:
A = (3,0) A' = (-3,0) B = (0,2) B' = (0,-2)
To fully define the ellipse, we should also find the focal points and the directrices. Thus we to find the eccentricity. We can do this through the relationship:
The integral ∫dx/√(a2 + x2) may be approached in 2 ways:
1. Trigonometric substitution, or
2. Hyperbolic substitution
The goal of both methods is to simplify the denominator expression: √(a2 + x2).
With trigonometric substitution, we can let x = atanθ, and thus dx = asec2θdθ, and √(a2 + x2) simplifies to √[a2(1 + tan2θ)] = asecθ. And the integral becomes ∫secθdθ.
With hyperbolic substitution, we can let x = asinhu, and thus dx = acoshudu, and √(a2 + x2) simplifies to √[a2(1 + sinh2u)] = acoshu, so the integral becomes ∫du.
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With the standard form of the ellipse being x2/a2 + y2/b2 = 1 and given the eccentricity, e, we can define and determine all of the features of the ellipse.
For instance, the:
x-intercepts are located at coordinates (a,0) and (-a,0)
y-intercepts are located at coordinates (0,b) and (0,-b)
Integrals of powers of trigonometric functions get increasingly difficult and tedious as the power increases. The idea is to reduce the power to the first order, and this can be done with power reduction formulas such as the half-angle formula. But as the power increases, the number of iterations of the half-angle formula also increases accordingly.
But there is a neat alternative for power reduction in complex numbers. Consider De Moivre's Theorem. It is probably the most efficient method of power reduction. For instance, in polar form...
z = cos(x) + isin(x)
If we raise z to the nth power, then by De Moivre's Theorem...
zn = [cos(x) + isin(x)]n = cos(nx) + isin(nx)
So we've reduced the power from n to 1 in just one step! Similarly...