Jupiter’s atmosphere is generally organized in dark belts and bright zones the presence, latitudinal limits, color and intensities of which are changeable [1]. The study of these changes may reveal…
The Hellenic Astronomical conference is the biennial meeting of the Greek professional astronomers’ society. During the 11th version of this conference (held in Athens, Sep. 8-12, 2013), we contributed with…
This work is a collective presentation of the type of contributions within the professional-amateur framework for the study of gaseous giants. In particular: The need for Professional-Amateur collaborations in studies…
Results (15/04/2015): Announcement (13/12/2015): The structure and variability of the upper atmospheres of the giant planets may be investigated by occultation techniques [1]. Ground-based photometric monitoring of stellar occultations measure…
Polar caps: Both caps look bright, the south cap is brighter, and the north cap more extended than the south cap. SSTB: The white Ovals look bright. The…
During the European Planetary Science Congress 2013 (Sep 8-13, 2013, London, UK) we presented the following work: Digital daylight observations of the planets with small telescopes Emmanuel (Manos) I. Kardasis…
