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Conics (Under Construction)
Conics (Conic Sections, in full) are defined as the intersection of a plane and a cone (and, at a simple level, we just consider the four shapes obtained when the plane does not pass thru the vertex of the cone).
Alternatively : - If S is a fixed point and l is a fixed line which does not pass thru S, a conic is the locus of points such that the ratio of the distance from S to the distance from l is a constant. The fixed point is the focus, and the fixed line is the directrix. The constant ratio is called the eccentricity.
Summary of Basic Properties
Circle Ellipse Parabola Hyperbola Standard Cartesian Equation : x2 + y2 = r2 ![]()
y2 = 4ax ![]()
Eccentricity (e): 0 0 < e <1 1 1 < e Relation between a,b and e b = a b2 = a2(1-e2) b2 = a2(e2-1) Parametric Representation ![]()
x = at2
y = 2at
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or
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Definition : It is the locus of all points which meet the condition... distance to the origin is constant sum of distances to each focus is constant distance to focus = distance to directrix difference between distances to each foci is constant It might tidy the logic up to consider a circle to be a special case of an ellipse. Then there are two 'main' classes
and a 'critical' class - the parabola with e = 1.
- an ellipse, with e < 1
- a hyperbola, with e > 1
The General Equation of a Conic
The General Equation for a Conic isAx2 + Bxy + Cy2 + Dx + Ey + F = 0
The actual type of conic can be found from the sign of B2 - 4AC
If B2 - 4AC is... then the curve is a... < 0 ellipse, circle, point or no curve. = 0 parabola, 2 parallel lines, 1 line or no curve. > 0 hyperbola or 2 intersecting lines. note : the above notation brings a close analogy with the formulas of quadratic equations. Sometimes, however, the formula is stated slightly differently
Ax2 + 2Bxy + Cy2 + Dx + Ey + F = 0
Here the type of conic must be found from the sign of B2 - AC
If B2 - AC is... then the curve is a... < 0 ellipse, circle, point or no curve. = 0 parabola, 2 parallel lines, 1 line or no curve. > 0 hyperbola or 2 intersecting lines.
Polar Form
For an origin at a focus, the general polar form (apart from a circle) is
where L is the semi latus rectum. ![]()
Ellipse
The cartesian equation of an ellipse is
where a and b would give the lengths of the semi-major and semi-minor axes. ![]()
In its general form, with the origin at the center of coordinates
- the foci are at
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- the directrix are at
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- the major axis of of length 2a
- the minor axis is of length 2b
- the semi latus rectum is of length
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From the general polar form, the equation for an ellipse is
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For any point P on the perimeter, the sum
PF1 + PF2
will be constant, no matter which point is chosen as P.
Hence, an ellipse can also be defined as the locus of a point which moves in a plane so that the sum of its distances from two fixed points is constant.
According to Kepler's First law, the orbit of a planet is an ellipse.
The Earth is shaped like an ellipsoid.
Any signal from one of the foci will pass thru the other focus. ![]()
Hyperbola
The cartesian equation of an hyperbola is
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In its general form, with the origin at the center of coordinates
- the foci are at (+/- ae, 0)
- the directrix are at x = +/- a/e
- the transverse axis of of length 2a
- the conjugate axis is of length 2b
- the semi latus rectum is of length 2b2/a
Note the similarity in notation with ellipses; although now the eccentricity is greater than one
Also by analogy with an ellipse
For any point P on a hyperbola, the sum
PF1 - PF2
will be constant, no matter which point is chosen as P.
Hence, a hyperbola can also be defined as the locus of a point which moves in a plane so that the difference of its distances from two fixed points is constant.
Asymptotes of Hyperbola
Rejigging the hyperbola formula to
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As x becomes larger, y tends to
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these are the equations of the asymptotes.
Rectangular Hyperbola
A hyperbola is rectangular if its asymptotes are perpendicular.From
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this requires
b = a
Substituting this into the cartesian formula for a hyperbola produces
x2 - y2 = 1
which has an eccentricity equal to the square root of 2
Rotating a rectangular so as to makes its asymptotes into the coordinates axes, changes the formula to
xy = c2
where c2 = (a2/2)
Moire Patterns