Glossary term: Day

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Description: Sometimes, we use "day" in the sense of "daytime": The time when the Sun provides us with natural light, followed by the night when the Sun has set and it is dark. This kind of day is shorter in the winter, and longer in the summertime. In the far North or the far South, there is a time of year where the Sun does not set at all – directly at the poles, the Sun is up for six months without setting! "Day" is also the name of the 24-hour unit of time we use in the calendar. Astronomically speaking, the time from one local noon to the next – that is, from the day's highest position of the Sun above the horizon from one day to the next – is called an apparent solar day. The length of local days varies depending on the time of year, owing to the facts that (a) Earth's orbit is elliptical (with Earth moving faster when it is closer to the Sun), and that (b) the apparent trajectory of the Sun in the sky is at different angles relative to Earth's equator (and no, it is not that easy to understand why that influences the Sun's apparent speed in the sky). For practical purposes, timekeeping instead uses the average length of apparent solar days, which are called mean solar days. The associated time at 24 hours per day is called mean solar time.

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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".