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Glossary term: Sun Path (Day Arc)

Description: The Sun's path or day arc traces the apparent motion of the Sun in the sky, as seen by an observer at a fixed position on Earth. Each day, the path traces out an arc, starting with sunrise in the eastern part of the sky and ending with sunset in the western part. At the winter solstice, the arc is shortest and lowest in the sky. From then on, the length of that arc, and with it the length of the day, increases, and each successive arc is higher in the sky than the day before, reaching maximum height, and maximum day length, at the summer solstice. This process then repeats in the opposite order, again reaching the shortest, lowest arc at winter solstice. The set of solar arcs can be captured in a long-term exposure image called a solargraph.

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Term and definition status: This term and its definition is still awaiting approval

The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".