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Recent Observations of Plutos System Probing Pluto's Atmosphere, - - PowerPoint PPT Presentation
Recent Observations of Plutos System Probing Pluto's Atmosphere, - - PowerPoint PPT Presentation
Recent Observations of Plutos System Probing Pluto's Atmosphere, Charon's Size and Orbital Elements Bruno Sicardy Observatoire de Paris - LESIA & Universit Pierre et Marie Curie ESOP XXXI meeting Pescara 24-27 August 2012
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radius, shape & limb features at kilometric accuracy density, if mass known from satellite motion ---> internal
structure
albedo ---> composition, state of surface if double occultation primary/secondary: accuracy ~ 10 km,
e.g. Pluton/Charon ---> better orbital elements airless Trans-Neptunian Objects (TNO's)
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density & temperature profiles down to nbar levels variations with time detection of activity ( e.g. gravity waves) zonal winds measurements through central flash haze properties through chromatic dependence
TNO's with atmosphere
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Geometry of the double occultation 22 June 2008
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circumstances of the double occultation of 04 June 2011: Charon
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circumstances of the double occultation of 04 June 2011: Pluto
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La Silla/Chile 60cm San Pedro de Atacama/Chile 50cm Pico dos Dias/Brazil 160cm Santa Martina/Santiago/Chile 40cm
the double Pluto/Charon event 4 June 2011, S. America
Charon/airless Pluto/atmosphere
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R= 602.0 km (vs. 603.6 km in 2005)
the double occultation of 04 June 2011: Charon
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Sicardy et al. 2011 JPL #017 Tholen et al. 2008 HST-based Buie et al 2012 HST-based
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PrePredicted ~ one week before
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Observed
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Pluto stellar occultation, 18 july 2012 ESO Very Large Telescope, NACO, H band before the event, without AO after the event, with AO Charon star Pluto’s motion Charon Pluto star Pluto
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gravity waves
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