Abstract
Everything we see in the Solar System, and most things that we see beyond it, participate in angular motion, that is to say, motion around a central point or axis. The most important angular motions that we need to understand are rotation and revolution. Rotation occurs when an object spins around an internal axis; revolution happens when an object moves around a point external to itself. When we are speaking about the Earth-Moon system, we must remember that the Earth rotates on its axis, while the Moon revolves around the Earth in its own orbit.
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Notes
- 1.
This works out because of a unit of angular measure called a radian. If you measure a distance along a circle equal to the length of its radius, you get one radian. One radian = 57.2 degrees.
- 2.
360 deg/24 hr = 15 deg/hr.
- 3.
Stellarium planetarium software is my favorite – it is open source and available free at Stellarium.org
- 4.
After I wrote this, I had to do the research and work it out. At my local donut shop, round cake donuts are about 7 × 7 × 3 cm. One million donuts work out to a stack of 15 × 15 × 6.4 meters, roughly the size of a four-flat apartment building two stories high!
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Barth, D.E. (2022). Exploring Size, Distance, and Motion. In: Star Mentor: Hands-On Projects and Lessons in Observational Astronomy for Beginners. The Patrick Moore Practical Astronomy Series. Springer, Cham. https://doi.org/10.1007/978-3-030-98771-8_3
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DOI: https://doi.org/10.1007/978-3-030-98771-8_3
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