Interactive cosmology visualization using the Hubble UltraDeep Field data in the classroom

Liam Nolan, M. Mechtley, R. Windhorst, K. Knierman, T. Ashcraft, S. Cohen, S. Tompkins, L. Will
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Abstract

We have developed a Java-based teaching tool, "Appreciating Hubble at Hyper-speed" ("AHaH"), intended for use by students and instructors in beginning astronomy and cosmology courses, which we have made available online. This tool lets the user hypothetically traverse the Hubble Ultra Deep Field (HUDF) in three dimensions at over 500x10^12 times the speed of light, from redshifts z=0 today to z=6, about 1 Gyr after the Big Bang. Users may also view the Universe in various cosmology configurations and two different geometry modes - standard geometry that includes expansion of the Universe, and a static pseudo-Euclidean geometry for comparison. In this paper we detail the mathematical formulae underlying the functions of this Java application, and provide justification for the use of these particular formulae. These include the manner in which the angular sizes of objects are calculated in various cosmologies, as well as how the application's coordinate system is defined in relativistically expanding cosmologies. We also briefly discuss the methods used to select and prepare the images in the application, the data used to measure the redshifts of the galaxies, and the qualitative implications of the visualization - that is, what exactly users see when they "move" the virtual telescope through the simulation. Finally, we conduct a study of the effectiveness in this teaching tool in the classroom, the results of which show the efficacy of the tool, with over 90% approval by students, and provide justification for its further use in a classroom setting.
在课堂上使用哈勃超深场数据的交互式宇宙学可视化
我们开发了一个基于java的教学工具,“超高速欣赏哈勃”(“AHaH”),旨在供学生和教师在天文学和宇宙学的入门课程中使用,我们已经在网上提供。这个工具可以让用户以超过光速500x10^12倍的速度在三维空间中穿越哈勃超深场(HUDF),从今天的红移z=0到z=6,大约是大爆炸后的1gyr。用户还可以在不同的宇宙学配置和两种不同的几何模式下观察宇宙——包括宇宙膨胀的标准几何,以及用于比较的静态伪欧几里得几何。在本文中,我们详细介绍了这个Java应用程序的功能背后的数学公式,并为使用这些特定公式提供了理由。这包括在各种宇宙学中计算物体角尺寸的方式,以及如何在相对论扩展的宇宙学中定义应用程序的坐标系。我们还简要讨论了在应用程序中选择和准备图像的方法,用于测量星系红移的数据,以及可视化的定性含义-即用户在模拟中“移动”虚拟望远镜时确切看到的内容。最后,我们对该教学工具在课堂上的有效性进行了研究,结果显示该工具的有效性,超过90%的学生认可,并为其在课堂环境中的进一步使用提供了理由。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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