Step 1: Understanding the purpose of a secondary mirror. - A reflecting telescope primarily uses a concave primary mirror to collect and focus light. - A secondary mirror is placed at an intermediate point to redirect the focused light to an eyepiece.
Step 2: Function of the secondary mirror. - The primary mirror focuses light inside the telescope tube, making it difficult to place an eyepiece directly. - The secondary mirror redirects the light outside the tube, allowing for convenient viewing. - This design is seen in the Cassegrain and Newtonian telescopes.
Step 3: Evaluating other Option. - (A) Reducing mechanical support problems → Incorrect. The secondary mirror is not primarily used for structural support. - (B) Removing spherical aberration → Incorrect. Spherical aberration is corrected by parabolic mirrors, not by the secondary mirror. - (C) Making chromatic aberration zero → Incorrect. Chromatic aberration is caused by lenses, but reflecting telescopes use mirrors, which naturally eliminate this issue.
Final Answer: \[ \boxed{{Move the eyepiece outside the telescopic tube}} \]
A disc is rolling without slipping on a surface. The radius of the disc is \( R \). At \( t = 0 \), the topmost point on the disc is \( A \) as shown in the figure. When the disc completes half of its rotation, the displacement of point \( A \) from its initial position is: