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Analysis of new photometry and spectroscopy of the binary Mira-type variable star X Ophiuchi between 2016 May and 2016 Dec indicates that the V magnitude of the constant star is 9.0 and its spectral type K1III. The spectral type of the Mira changed from M6III at maximum to M7III as it faded and passed through minimum. The Mira’s V magnitude varied between 6.47 at maximum and 9.83 at minimum, a range of 3.36 mags.

This paper looks at NLC frequency and distribution of observations during the first two years of solar cycle 24’s decline from maximum.

In this paper we review telescopic observational data of Mercury from 2007 November to 2016 October inclusive, and describe the results of the 2016 solar transit. A gradual improvement in imaging technique has enabled observers to record albedo features upon Mercury’s surface as well as many bright patches corresponding to the ejecta regions of bright craters. An albedo chart and a Messenger map are presented for comparison. At the solar transit, observers obtained images in white light as well as in the wavelengths of H-alpha and Calcium K, timed the various contacts, and re-observed certain optical effects, comparing the results with those obtained at previous events.

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.