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  2. Secondary mirror - Wikipedia

    en.wikipedia.org/wiki/Secondary_mirror

    The secondary mirror assembly of the Keck Telescope and its relationship to the primary mirror. A secondary mirror (or secondary) is the second deflecting or focusing mirror element in a reflecting telescope. Light gathered by the primary mirror is directed towards a focal point typically past the location of the secondary.

  3. Mirror mount - Wikipedia

    en.wikipedia.org/wiki/Mirror_mount

    The most common type of mirror mount is the kinematic mount. [3] This type of mount is designed according to the principles of kinematic determinacy. Typically, the movable frame that holds the mirror pivots on a ball bearing which is set into a hole in the fixed frame. Ideally, this hole should be trihedral (pyramid-shaped).

  4. Catadioptric system - Wikipedia

    en.wikipedia.org/wiki/Catadioptric_system

    The Schmidt camera is a wide-field photographic telescope, with the corrector plate at the center of curvature of the primary mirror, producing an image at a focus inside the tube assembly at the prime focus where a curved film plate or detector is mounted. The relatively thin and lightweight corrector allows Schmidt cameras to be constructed ...

  5. 62 Gifts for Teens That Are Actually Cool, According to Real ...

    www.aol.com/lifestyle/72-gifts-teens-actually...

    The flexible wires make it easy to place them around picture frames, mirrors or other decor for a pretty effect (that won’t ruin your walls). This particular set offers a plethora of fun color ...

  6. Reflecting telescope - Wikipedia

    en.wikipedia.org/wiki/Reflecting_telescope

    A convex secondary mirror is placed just to the side of the light entering the telescope, and positioned afocally so as to send parallel light on to the tertiary. The concave tertiary mirror is positioned exactly twice as far to the side of the entering beam as was the convex secondary, and its own radius of curvature distant from the secondary.

  7. Hale Telescope - Wikipedia

    en.wikipedia.org/wiki/Hale_Telescope

    The mirror was coated (and still is re-coated every 18–24 months) with a reflective aluminum surface using the same aluminum vacuum-deposition process invented in 1930 by Caltech physicist and astronomer John Strong. [21] The Hale's 200 in (510 cm) mirror was near the technological limit of a primary mirror made of a single rigid piece of glass.

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