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In this section, we explore the properties of ellipses, including their standard equation, which describes their geometric shape, and foundational concepts such as foci, major and minor axes, and eccentricity, providing crucial insights into their behavior and applications in coordinate geometry.
An ellipse is a fundamental concept in conic sections and plays a significant role in analytic geometry. It is defined as the collection of points where the sum of the distances from two fixed points, known as foci, remains constant. The visual representation of an ellipse is oval in shape, pointing toward the foci positions.
The standard equation for an ellipse centered at the origin, with the major axis aligned along the x-axis, is given by:
\[\frac{x^2}{a^2} + \frac{y^2}{b^2} = 1\]
Where:
- a: semi-major axis (half the length of the longest diameter of the ellipse)
- b: semi-minor axis (half the length of the shortest diameter of the ellipse)
When the ellipse is vertical, the equation changes slightly to:
\[\frac{y^2}{a^2} + \frac{x^2}{b^2} = 1\]
Key properties that characterize an ellipse include:
1. Foci: The two fixed points are located inside the ellipse, and the distance from any point on the ellipse to the foci is constant.
2. Major and Minor Axes: The longest diameter is the major axis, while the shortest one is the minor axis.
3. Eccentricity: A measure of how
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An ellipse is the set of points where the sum of the distances from two fixed points called foci is constant.
An ellipse consists of all the points in a plane such that the total distance from two specific points, known as the foci, remains the same, regardless of which point on the ellipse you choose. This property is key in understanding how ellipses are formed and their geometry. Imagine stretching a string between two points; if you keep the string taut while tracing around, the shape created is an ellipse.
Think of a family trip: if you have two family members standing at fixed locations (the foci), and everyone else must hold a rope that keeps them at a fixed distance from both family members, the path traced out by the rope will be an ellipse. This is similar to how gravitational forces from two celestial bodies can create elliptical orbits.
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For an ellipse centered at the origin with major axis along the x-axis, the equation is:
\[ \frac{x^2}{a^2} + \frac{y^2}{b^2} = 1 \]
An ellipse can be mathematically represented with a standard equation depending on its orientation. This particular formula shows how the lengths of the axes (the horizontal and vertical) relate to the ellipse's shape. The terms 'a' and 'b' represent half the lengths of the major and minor axes, respectively. If a > b, the ellipse is wider horizontally; if b > a, it's taller vertically.
Imagine a basketball and a football. The basketball, which is round, is like an ellipse where the major and minor axes are almost equal, whereas the football is elongated, resembling an ellipse with a long major axis. The equation helps to quantify these relationships in mathematical terms.
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Includes definitions of foci, major and minor axes, and eccentricity.
Ellipses have several important properties. The foci are fixed points inside the ellipse that define its shape. The major axis is the longest diameter that passes through both foci, while the minor axis is perpendicular to the major axis at the center of the ellipse. Eccentricity measures the 'flattening' of the ellipse; it is a number between 0 (for a circle) and 1 (for a line). A lower eccentricity means a shape closer to a circle.
Picture a racetrack where cars have to move in an oval. The two endpoints of the track (foci) dictate their path. The longest straight part of the track represents the major axis, while the shorter parts make up the minor axis. The eccentricity can be visualized by how stretched or curved the track is: a perfectly circular track (like a roundabout) has an eccentricity of 0, while a long straight 'track' (like a straight line) has an eccentricity approaching 1.