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  2. Mirror - Wikipedia

    en.wikipedia.org/wiki/Mirror

    A mirror reflecting the image of a vase A first-surface mirror coated with aluminium and enhanced with dielectric coatings. The angle of the incident light (represented by both the light in the mirror and the shadow behind it) exactly matches the angle of reflection (the reflected light shining on the table). 4.5-metre (15 ft)-tall acoustic mirror near Kilnsea Grange, East Yorkshire, UK, from ...

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    Get AOL Mail for FREE! Manage your email like never before with travel, photo & document views. Personalize your inbox with themes & tabs. You've Got Mail!

  4. Infinity mirror - Wikipedia

    en.wikipedia.org/wiki/Infinity_mirror

    A self-contained infinity mirror used as a wall decoration. In a classic self-contained infinity mirror, a set of light bulbs, LEDs, or other point-source lights are placed around the periphery of a fully reflective mirror, and a second, partially reflective "one-way mirror" is placed a short distance in front of it, in a parallel alignment.

  5. Objects in mirror are closer than they appear - Wikipedia

    en.wikipedia.org/wiki/Objects_in_mirror_are...

    It is present because while these mirrors' convexity gives them a useful field of view, it also makes objects appear smaller. Since smaller-appearing objects seem farther away than they actually are, a driver might make a maneuver such as a lane change assuming an adjacent vehicle is a safe distance behind, when in fact it is quite a bit closer ...

  6. Canon EOS-1V - Wikipedia

    en.wikipedia.org/wiki/Canon_EOS-1V

    The 1V was the last model of Canon professional film cameras before it was discontinued on May 30, 2018. [ 6 ] Canon used the suffix 'V' because the camera introduced the fifth generation of Canon professional SLRs, after the Canon F-1 and New F-1 , the Canon T90 , and earlier EOS 1 models; Canon also stated that the 'V' stands for "vision".

  7. 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.

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