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Most stars, planets, and moons spin around their own axis. This means that every moment in time, telescopes are looking at a specific space object at an angle that is different from that of previous moments. For instance, the sun rotates once about its own axis about every 30 days (the sun's equator spins faster than its polar regions, but that does not concern us here). If you take pictures of the sun continuously for 30 days as it rotates, then you have a photo collection of what the sun looks like from all vantage points. SOHO does just that. Note that the sun is a turbulent ball of bubbling plasma, so its surface features are slowly evolving. But thanks to its rotation, we are able to see what a particular sunspot looks like from the top, from the side, and from all sorts of other angles.
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The strict definition of rotation is "the circular movement of an object about a point in space." This is used in geometry as well as astronomy and physics. To help visualize it, imagine a point on a piece of paper
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