Problem 64
Question
The orbits of stars, planets, comets, asteroids, and satellites all have the shape of one of the conic sections. Astronomers use a measure called eccentricity to describe the shape and elongation of an orbital path. For the circle and ellipse, eccentricity e is calculated with the formula \(e=\frac{c}{d},\) where \(c^{2}=\left|a^{2}-b^{2}\right|\) and \(d\) is the larger value of a or b. For a hyperbola, eccentricity e is calculated with the formula \(e=\frac{c}{d},\) where \(c^{2}=a^{2}+b^{2}\) and the value of \(d\) is equal to a if the hyperbola has \(x\) -intercepts or equal to b if the hyperbola has \(y\) -intercepts. A. \(\frac{x^{2}}{36}-\frac{y^{2}}{13}=1\) B. \(\frac{x^{2}}{4}+\frac{y^{2}}{4}=1\) C. \(\frac{x^{2}}{25}+\frac{y^{2}}{16}=1\) D. \(\frac{y^{2}}{25}-\frac{x^{2}}{39}=1\) G. \(\frac{x^{2}}{16}-\frac{y^{2}}{65}=1\) E. \(\frac{x^{2}}{17}+\frac{y^{2}}{81}=1\) F. \(\frac{x^{2}}{36}+\frac{y^{2}}{36}=1\) H. \(\frac{x^{2}}{144}+\frac{y^{2}}{140}=1\) For each of the equations \(A-H,\) find the value of \(d\).
Step-by-Step Solution
VerifiedKey Concepts
Eccentricity
- A circle has an eccentricity of 0, indicating it is perfectly round.
- An ellipse has an eccentricity greater than 0 and less than 1, showing varying degrees of flattening.
- A parabola has an eccentricity exactly equal to 1, reflecting its unique open curve.
- A hyperbola has an eccentricity greater than 1, indicating an open form with two branches.
Ellipses
If \(a = b\), the ellipse is actually a circle. However, when \(a eq b\), the ellipse is stretched in the direction of the larger axis. The largest of \(a\) or \(b\) is identified as the semi-major axis. This plays a major role in calculating eccentricity and understanding the stretch of the ellipse. Each ellipse has two axes – the longer major axis and the shorter minor axis – which determine its overall shape.
Ellipses are crucial in various fields, including astronomy, as they describe the orbits of planets and satellites.
Hyperbolas
For hyperbolas, \(a\) is always associated with the first term in the equation. The line through the centers of both branches is called the transverse axis. The eccentricity of hyperbolas (\(e > 1\)) reflects their two-branched nature and open form. In hyperbolas, instead of a continuous curve like ellipses, you get two diverging paths, making them unique among conic sections.
Understanding hyperbolas aids in areas ranging from navigation systems to the design of certain telescopes.
Standard Form of Conics
- For circles, the standard form is \(x^2 + y^2 = r^2\), where \(r\) is the radius.
- Ellipses are given by \(\frac{x^2}{a^2} + \frac{y^2}{b^2} = 1\), where \(a\) and \(b\) determine the axes lengths.
- Hyperbolas have the form \(\frac{x^2}{a^2} - \frac{y^2}{b^2} = 1\) or \(\frac{y^2}{a^2} - \frac{x^2}{b^2} = 1\), which describes their diverging paths.
Circle
Circles have an eccentricity of \(0\), reflecting their perfect symmetry and uniformity. They serve as a fundamental shape in geometry and are ubiquitous in the natural and manufactured world. By understanding a circle’s properties and characteristics, one can better appreciate the more complex properties of other conic sections such as ellipses and hyperbolas.
Circles are extensively used in design and engineering because their geometry is fundamental and inherently stable.