ISSN: 2996-6701
Authors: Khlamov S*
This review article explores the diverse forms and appearances of images of Solar System objects (SSOs) captured in frames by the charge-coupled device (CCD). It examines the factors influencing these shapes, including the object's intrinsic characteristics, observing conditions, and instrumental effects. Emphasis is placed on the role of optical systems, atmospheric conditions, and image processing techniques in shaping the observed profiles and recognition patterns. The article also categorizes common image typical shapes, such as circle (point-like) sources, blurred objects, extended (long) objects, objects with intersections with another objects (overlapped), blended objects, and irregular shapes, linking them to specific celestial bodies like minor planets, comets, and asteroids. The findings aim to enhance the understanding of imaging methodologies and support accurate interpretation of observational data.
Keywords: Typical Shape of Image; Aberrations; Atmospheric Turbulence; Blurring; Astrometry; Photometry; Solar System Objects
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