For amateur astronomers the distant planet Uranus is a considerable observing challenge. With its angular size of about 3.6 arcseconds it is not easy to detect details in its atmosphere, and imaging of its faint satellites requires relatively long exposure times. Nevertheless, with the development of new digital cameras with increased sensitivity the planet and its satellites have become interesting objects of study. In this report covering the period 2006-2016, progress in imaging Uranus by the author is demonstrated. In particular this shows that the detection of features in the atmosphere of Uranus has become a promising field for future investigation.
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