Reflecting telescopes use a curved primary mirror to gather and focus light. The light is then directed to a secondary mirror, which reflects it to the eyepiece or a detector. This design allows for larger apertures and better image quality compared to refracting telescopes.
By mastering these topics, you will develop a solid understanding of reflecting telescopes and their significance in the field of astronomy and optics.
Identify and analyze forces responsible for changes in rotational motion and develop an understanding of the effect of rotational inertia on the motion of a rotating object (e.g., merry-go-round, spinning toy, spinning figure skater, stellar collapse [supernova], rapidly spinning pulsar).