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Carson Witt

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% PROJECT 1
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% filename: p2_paralax.tex
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% last modified: 2016-10-13
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\documentclass
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[justified,nohyper]
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{tufte-handout}
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\usepackage{amsmath}
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\usepackage{booktabs}
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\usepackage{graphicx}
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\usepackage{kmath,kerkis} % The order of the packages matters; kmath changes the default text font
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\usepackage[T1]{fontenc}
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\usepackage{enumitem}
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% USEFUL SHORTCUTS FOR MATH
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\newcommand{\ds}{\displaystyle}
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\newcommand{\dt}[1]{\dfrac{d#1}{dt}}
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\newcommand{\lp}{\left(}
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\newcommand{\rp}{\right)}
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\newcommand{\lb}{\left[}
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\newcommand{\rb}{\right]}
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\newcommand{\evalat}{\biggr\rvert}
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\begin{document}
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\begin{fullwidth}
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\mbox{\LARGE PreCalculus BC: Project Two - \today }\hfill
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\end{fullwidth}
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\section*{Introduction}
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In the project, we will be investigating the parallax effect. Parallax is a
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displacement or difference in the apparent position of an object viewed along
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two different lines of sight, and is measured by the angle or semi-angle of
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inclination between those two lines. (src: wikipedia)
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Parallax can be used to approximate the distance to objects that are far away,
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such as stars. Alpha Centauri, which is the nearest star to Earth has a parallax
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of 0.000211 degrees.
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\section*{Places to start}
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Your first task will be to research the concept of parallax. What is it? How
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can it be used to find distances of far away objects? What information is needed
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in the calculation? In the process of this investigation, you will learn that
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most astronomical angle measurements use degrees, minutes of arc, and seconds
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of arc. A portion of your report should be dedicated to explaining how these
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angle measurements are used in astronomy and some historical background into
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why they are used. We will often talk in class about how radians provide a better
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way to measure angles. If that's the case, then why do astronomers continue
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to use degrees? There are many clues as to why this is the case in history. While
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I am not asking you to write a history report, I do think that addressing
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the historical background of the practice of astronomy will provide your report
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with a great deal of depth and meaning.
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Second, you will need to describe the process of finding the distance to Alpha
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Centauri using parallax. Your report will need to present the calculation and
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interpret the results. You can also compare your results to the measurement
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found on the Alpha Centauri wikipedia page which is 4.37 light years or 1.34
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pc.
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Last, your report will need to address how robust this method of finding distances
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is. For example, can parallax be used to find the distance to objects that are
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not far away? Is there some minimum distance that can be used? In other words,
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where does this process breakdown?
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\section*{Your report}
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As always, your report should include an abstract, procedure, and conclusion
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section. This report will be somewhat different in that there is not a specific
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mathematical problem to solve. This report will read more like a research paper
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whose goal is to explain the concept of parallax to the reader. Your report will
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accomplish this by providing some historical background and examples related
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to using parallax. Your report should also investigate advantages and disadvantages
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to this method of measuring distances.
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To help you with the abstract and conclusion, please consider the following.
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The abstract should be a short introduction to the problem of approximating distances
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we cannot directly measure such as the distance to nearby stars. The conclusion
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will contain a summary of the method of parallax and will highlight the advantages
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and disadvantages of the method.
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You have two main areas of focus. The first is developing your ability to explain
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concepts in a clear and meanginful way. The second is to use SageMathCloud to
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draw illustrations.
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During the next few weeks, we will talk about how to draw illustrations
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using SageMathCloud. Your report will need to make use of these illustrations
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to explain how parallax works to measure distances.
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\end{document}
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