![]() ![]() Sun glitter was discovered on Titan's smallest sea, Punga Mare, in 2014 as a set of brightened pixels at infrared wavelengths across Punga Mare's bright sea surface. Titan hosts lakes and seas of liquid methane at its north polar region. Sun glitter is observed on other planetary bodies with surface liquids, namely Titan. When the sun is really low above the horizon, the glitter breaks because of the waves, which could sometimes obstruct the sun and cast a shadow on the glitter. The lower the sun appears, the longer and more reddish the glitter is. The color and the length of the glitter depend on the altitude of the Sun. The exact pattern seen depends on the viewer's precise location. As a result, a viewer in the right position will see many small images of the sun, formed by portions of waves that are oriented correctly to reflect the sun's light to the viewer's eyes. A rippled but locally smooth surface such as water with waves will reflect the sun at different angles at each point on the surface of the waves. Light reflects from smooth surfaces by specular reflection. Even a ripple from a thrown rock will create a momentary glitter. ![]() ![]() The waves may be caused by natural movement of the water, or by the movement of birds or animals in the water. Sun glitter is a bright, sparkling light formed when sunlight reflects from water waves. Sparkling light formed when sunlight reflects from water waves Sun glitter Sun glitter caused by a duck Sun glitter (blue arrows) in Punga Mare (central black outline) ![]()
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