Variazioni di luminosità del pianeta Urano

Details Variazioni di luminosità del pianeta Urano Variazioni di luminosità del pianeta Urano

Apr 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005asuai...2...24b&link_type=abstract

Astronomia. La rivista dell'Unione Astrofili Italiani (ISSN 0392-2308), N. 2, p. 24 - 25 (marzo-aprile 2005)

Astronomy and Astrophysics

Astronomy

1

Uranus:Bightness Variations

Scientific paper

This report describes R-CCD differential photometric studies of Uranus from 21 July 2004 through 18 September 2004. Results do not confirm the report by A. J. Hollis (2000) describing variations of magnitude of 0.3-0.5 over a 2 month period, and support the existence of brightness variations of some hundredths of a magnitude, in small (hours) and long (month) time scales. Uranus' appearance continues to change as it approaches its 2007 equinox, and even amateurs should dedicate particular attention to photometric evaluation of the planet. The same is true for Pluto, as it approaches its perihelion.

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