Carson Witt
%%%%%%1%2% PROJECT 13%4% filename: p2_paralax.tex5% last modified: 2016-10-136%7%%%%%%%8%9%10%%%%%%%1112\documentclass13[justified,nohyper]14{tufte-handout}1516\usepackage{amsmath}1718\usepackage{booktabs}19\usepackage{graphicx}20\usepackage{kmath,kerkis} % The order of the packages matters; kmath changes the default text font21\usepackage[T1]{fontenc}2223\usepackage{enumitem}242526% USEFUL SHORTCUTS FOR MATH27\newcommand{\ds}{\displaystyle}2829\newcommand{\dt}[1]{\dfrac{d#1}{dt}}3031\newcommand{\lp}{\left(}32\newcommand{\rp}{\right)}33\newcommand{\lb}{\left[}34\newcommand{\rb}{\right]}3536\newcommand{\evalat}{\biggr\rvert}3738\begin{document}39\begin{fullwidth}40\mbox{\LARGE PreCalculus BC: Project Two - \today }\hfill41\end{fullwidth}42\section*{Introduction}4344In the project, we will be investigating the parallax effect. Parallax is a45displacement or difference in the apparent position of an object viewed along46two different lines of sight, and is measured by the angle or semi-angle of47inclination between those two lines. (src: wikipedia)4849Parallax can be used to approximate the distance to objects that are far away,50such as stars. Alpha Centauri, which is the nearest star to Earth has a parallax51of 0.000211 degrees.5253\section*{Places to start}5455Your first task will be to research the concept of parallax. What is it? How56can it be used to find distances of far away objects? What information is needed57in the calculation? In the process of this investigation, you will learn that58most astronomical angle measurements use degrees, minutes of arc, and seconds59of arc. A portion of your report should be dedicated to explaining how these60angle measurements are used in astronomy and some historical background into61why they are used. We will often talk in class about how radians provide a better62way to measure angles. If that's the case, then why do astronomers continue63to use degrees? There are many clues as to why this is the case in history. While64I am not asking you to write a history report, I do think that addressing65the historical background of the practice of astronomy will provide your report66with a great deal of depth and meaning.6768Second, you will need to describe the process of finding the distance to Alpha69Centauri using parallax. Your report will need to present the calculation and70interpret the results. You can also compare your results to the measurement71found on the Alpha Centauri wikipedia page which is 4.37 light years or 1.3472pc.7374Last, your report will need to address how robust this method of finding distances75is. For example, can parallax be used to find the distance to objects that are76not far away? Is there some minimum distance that can be used? In other words,77where does this process breakdown?7879\section*{Your report}8081As always, your report should include an abstract, procedure, and conclusion82section. This report will be somewhat different in that there is not a specific83mathematical problem to solve. This report will read more like a research paper84whose goal is to explain the concept of parallax to the reader. Your report will85accomplish this by providing some historical background and examples related86to using parallax. Your report should also investigate advantages and disadvantages87to this method of measuring distances.8889To help you with the abstract and conclusion, please consider the following.90The abstract should be a short introduction to the problem of approximating distances91we cannot directly measure such as the distance to nearby stars. The conclusion92will contain a summary of the method of parallax and will highlight the advantages93and disadvantages of the method.9495You have two main areas of focus. The first is developing your ability to explain96concepts in a clear and meanginful way. The second is to use SageMathCloud to97draw illustrations.9899During the next few weeks, we will talk about how to draw illustrations100using SageMathCloud. Your report will need to make use of these illustrations101to explain how parallax works to measure distances.102103\end{document}104105106107