Whither Does the Sun Rove?

TL;DR

This paper provides simple visualization tools to understand how the Sun's rising and setting points deviate from the east and west throughout the year at different latitudes, aiding teaching in physics and astronomy.

Contribution

It introduces intuitive, math-free tools for visualizing the Sun's horizon positions, enhancing educational approaches in astronomy.

Findings

Tools effectively visualize solar position deviations.

Aid in teaching introductory physics and astronomy.

Applicable across different latitudes and times of year.

Abstract

If one asked some friends where on the horizon they should expect to see the sunrise, half of the answers would be "in the east". Of course, something analogous would happen with the sunset and the west. However, sunrise and sunset virtually never occur at these cardinal points. In fact, those answers correctly describe observations only during the equinoxes, when either autumn or spring begin. Once we recall this, the next natural question to ask ourselves is: how far from the east (or from the west) the rising (or setting) Sun is located for a given latitude of the observer and for a given day of the year. In this paper we supply some simple tools to easily visualize the angular (southward or northward) departure of the rising and setting Sun on the horizon from the east-west direction in a pictorial way, without the need of mathematics. These tools have proven a valuable resource in teaching introductory physics and astronomy courses.