\documentstyle[11pt]{article} \textheight 22cm \textwidth 16cm \hoffset= -0.6in \voffset= -0.5in \setlength{\parindent}{0cm} \setlength{\parskip}{15pt plus 2pt minus 2pt} \pagenumbering{roman} \setcounter{page}{-9} \newcommand{\be}{\begin{equation}} \newcommand{\ee}{\end{equation}} \newcommand{\bd}{\begin{displaymath}} \newcommand{\ed}{\end{displaymath}} \begin{document} \begin{center} {\Large ASTR450 Homework \# 3 -- Central Force Motion\\ Due Tuesday, February 25} \end{center} Reading: Start Danby's Chapter 6. 1. Danby: Page 82, Problem 8. Draw a picture of the elliptical orbit and label the semimajor axis, semiminor axis and latus rectum. 2. Danby: Page 84, Problem 10. Under what conditions will the future orbit be a circle? An ellipse? A parabola? A hyperbola? 3. Danby: Page 84, Problem 14. 4. Danby: Page 85, Problem 25. Use the Central Force Integrator to determine numerically what happens to each of the six cases when the force law is changed to $r^{-2.9}$. 5. Danby: Page 86, Problem 31. Sketch the orbit for several different values of a. \enddocument}