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  3. 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 ...

  4. One-way mirror - Wikipedia

    en.wikipedia.org/wiki/One-way_mirror

    One-way mirrors for upper-level observation deck viewing down into a classroom (University of Wisconsin-Eau Claire) A one-way mirror, also called two-way mirror [1] (or one-way glass, half-silvered mirror, and semi-transparent mirror), is a reciprocal mirror that appears reflective from one side and transparent from the other. The perception of ...

  5. Little Dot Hetherington at the Old Bedford - Wikipedia

    en.wikipedia.org/wiki/Little_Dot_Hetherington_at...

    Min-Tsuei Ni described Little Dot Hetherington at the Old Bedford as one of Sickert's first two paintings (along with The Music Hall, or The Right Part of the Backstage in the Mirror on the Left, Eng. S. Wings in the O. P. P. Mirror, c.1889, canvas, oil, 76.2 x 63.5 cm, and framed 90.5 x 77.5 x 7.3 cm, the work is unsigned and undated by the ...

  6. Curved mirror - Wikipedia

    en.wikipedia.org/wiki/Curved_mirror

    Convex mirror lets motorists see around a corner. Detail of the convex mirror in the Arnolfini Portrait. The passenger-side mirror on a car is typically a convex mirror. In some countries, these are labeled with the safety warning "Objects in mirror are closer than they appear", to warn the driver of the convex mirror's distorting effects on distance perception.

  7. Cassegrain reflector - Wikipedia

    en.wikipedia.org/wiki/Cassegrain_reflector

    Light path in a Cassegrain reflecting telescope. The Cassegrain reflector is a combination of a primary concave mirror and a secondary convex mirror, often used in optical telescopes and radio antennas, the main characteristic being that the optical path folds back onto itself, relative to the optical system's primary mirror entrance aperture.

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