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ALPO Observations of the Remote Planets in 2012-2013. Richard W. Schmude, Jr. Gordon State College. Overview. Introduction Images Photometry Conclusions. Introduction. Seasonal brightness changes Uranus Neptune Images Visible Near-infrared. Images. Usually a large telescope
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ALPO Observations of the Remote Planets in 2012-2013 Richard W. Schmude, Jr. Gordon State College
Overview • Introduction • Images • Photometry • Conclusions
Introduction • Seasonal brightness changes • Uranus • Neptune • Images • Visible • Near-infrared
Images • Usually a large telescope • 1.0 m Pic du Midi Observatory (France) • 1.29 m Skinakas Observatory (Greece) • Filters: • B, V, R • Near-infrared
Uranus: August 8, 2012F. Colas, J. L. Dauvergne, M. Delcroix, T. Legault & C. ViladrichPic du Midi 1.0 m telescope
Uranus: September 17, 2012A. Obukhov, Moscow Russia (C11 telescope)
Uranus Belt Latitudes • Equatorial Belt • 2° S to 13° N (3° uncertainty) • North Temperate Belt • 45 3° N to 59° N (3° uncertainty)
Neptune: August 27, 2012G. Maravelias and M. Kardasis Skinakas Observatory 1.29 m
Photometry • Measurement of Brightness • Accurate brightness measurements since 1950 • B, V, R and I filters
Photometry: Uranus V(1,a) = -7.117 ± 0.007 B – V = 0.47 R – V = 0.307 I – R = 1.18 *Uranus is a little fainter than in the previous apparition
Photometry: Neptune V(1,a) = -7.005 ± 0.009 B – V = 0.384
Photometry: Oberon • September 24, 2012 unfiltered image: • Titania was 0.25 mag. brighter than Oberon
Conclusions • Several astronomers have imaged albedo features on Uranus using telescopes as small as a C11. • Uranus is a little fainter than in the previous apparition
Acknowledgements P. Abbott, K. Bailey, J. Boudreau, F. Colas, J. L. Dauvergne, M. Delcroix, F. Emond, J. Fox, M, Kardasis, T. Legault, S. Maksymowicz, G. Maravelias, M. Mattei, F. Melillo, C. Pellier, J. P. Prost, T. Boyle, C. Viladrich P. Abel, P. Bayle, G. Bianchi, D. Gray, T. Ikemura, F. Isac, A. Kazemoto, A. Lasala, P. Maxson, A. Medugno, S. Mogami, A. Obukhov, D. Peach, J. J. Poupeau, E. Punzo, S. Quaresima, H. Sasse, J. Sussenbach, G. Tarsoudis and A. Yamazaki