Answer:
B.) Primary mirror--->secondary mirror--->eyepiece--->eye
Explanation:
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The correct path of light through a reflecting telescope will be Primary mirror--->secondary mirror--->eyepiece--->eye.
A reflecting telescope (also called a reflector) is a telescope that uses a single or a combination of curved mirrors that reflect light and form an image
it is a design that allows for very large diameter objectives. Almost all of the major telescopes used in astronomy research are reflectors.
Reflecting telescopes come in many design variations and may employ extra optical elements to improve image quality or place the image in a mechanically advantageous position.
A curved primary mirror is the reflector telescope's basic optical element that creates an image at the focal plane. The distance from the mirror to the focal plane is called the focal length.
Film or a digital sensor may be located here to record the image, or a secondary mirror may be added to modify the optical characteristics and/or redirect the light to film, digital sensors, or an eyepiece for visual observation.
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