Demonstrating cosmological and Doppler redshift in the classroom

Oriel Marshall, R. Tojeiro, A. Weijmans
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Abstract

Cosmology is often a difficult subject to teach as it can involve many confusing and sometimes abstract concepts. One particular topic with many existing misconceptions and difficulties surrounding it is redshift, specifically the difference between Doppler shift (due to the peculiar velocities of galaxies) and cosmological redshift (due to the expansion of the side). Redshift of galaxies, despite being an extremely useful and interesting scientific tool, can often become a tedious subject to teach as it is largely theoretical and usually does not include demonstrations or interaction in the classroom. It can be challenging to understand, and therefore also challenging to explain, the differences between Doppler and cosmological redshift, often leading to this distinction being overlooked entirely. The set of demonstrations developed during this astrophysics masters project, along with the accompanying presentation, worksheet, and teacher notes, aim to explain both Doppler and cosmological redshift clearly and in an engaging and memorable way. The demonstrations use remote control vehicles to represent peaks of a travelling wave of light. When demonstrating Doppler shift, the vehicles are released from a plastic board that is being pulled away, representing a receding source of light. When demonstrating cosmological redshift, the vehicles are driven along a wide stretchy exercise band, representing a section of the expanding Universe through which this wave of light is travelling. This teaching resource will introduce interactive learning, proven to be very effective when teaching astronomy, and provides a useful and fun physical analogy to demonstrate an often-misunderstood subject.
在教室里演示宇宙和多普勒红移
宇宙学通常是一个很难教的学科,因为它可能涉及许多令人困惑的,有时是抽象的概念。关于红移,有许多现存的误解和困难,特别是多普勒频移(由于星系的特殊速度)和宇宙学红移(由于侧面的膨胀)之间的区别。星系的红移,尽管是一个非常有用和有趣的科学工具,但往往会成为一个乏味的主题,因为它很大程度上是理论性的,通常不包括课堂上的演示或互动。理解和解释多普勒红移和宇宙红移之间的差异是具有挑战性的,往往导致这种区别被完全忽视。在这个天体物理学硕士项目中开发的一套演示,以及随附的演示,工作表和教师笔记,旨在以一种引人入胜和令人难忘的方式清楚地解释多普勒和宇宙红移。演示使用遥控车辆来表示光的行波的峰值。在演示多普勒频移时,车辆从一块被拉开的塑料板上释放出来,代表一个后退的光源。在演示宇宙红移时,载具沿着一条宽的伸展运动带行驶,这条运动带代表了这波光波所经过的膨胀宇宙的一部分。这个教学资源将介绍互动学习,在天文学教学中被证明是非常有效的,并提供一个有用和有趣的物理类比来演示一个经常被误解的学科。
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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